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1

Meson Production and Baryon Resonances at CLAS  

Science Conference Proceedings (OSTI)

I give a brief overview of the exploration of baryon properties in meson photo- and electroproduction. These processes provide ample information for the study of electromagnetic couplings of baryon resonances and to search for states, yet to be discovered. The CLAS detector, combined with the use of energy-tagged polarized photons and polarized electrons, as well as polarized targets and the measurement of recoil polarization, provide the tools for a comprehensive nucleon resonance program. I briefly present the status of this program, prospects for the next few years, and plans for the Jefferson Lab 12 GeV upgrade.

Volker Burkert

2011-02-01T23:59:59.000Z

2

Meson Production and Baryon Resonances at CLAS  

E-Print Network (OSTI)

I give a brief overview of the exploration of baryon properties in meson photo- and electroproduction. These processes provide ample information for the study of electromagnetic couplings of baryon resonances and to search for states, yet to be discovered. The CLAS detector, combined with the use of energy-tagged polarized photons and polarized electrons, as well as polarized targets and the measurement of recoil polarization, provide the tools for a comprehensive nucleon resonance program. I briefly present the status of this program, prospects for the next few years, and plans for the Jefferson Lab 12 GeV upgrade.

Volker D. Burkert

2010-08-17T23:59:59.000Z

3

Resonating group method study of baryon-meson systems  

NLE Websites -- All DOE Office Websites (Extended Search)

Resonating group method study of baryon-meson systems in a chiral quark model F. Huang Institute of High Energy Physics, Chinese Academy of Sciences Using the resonating group...

4

Multiquark Correlations in Light Mesons and Baryons from holographic QCD  

Science Conference Proceedings (OSTI)

A hadron's multiquark content reflects itself in the quark composition of the interpolator with which it has maximal overlap. The AdS/CFT dictionary translates the anomalous dimension of this interpolator into a mass correction for the corresponding dual mode. Hence such bulk-mass corrections can carry specific information on multiquark correlations. Two prominent examples are studied by implementing this robust and universal holographic mechanism into AdS/QCD gravity duals. In the baryon sector bulk-mass corrections are used to describe systematic good (i.e. maximally attractive) diquark effects. The baryon sizes are predicted to decrease with increasing good-diquark content, and the masses of all 48 observed light-quark baryon states are reproduced with unprecedented accuracy. Our approach further provides the first holographic description of a dominant tetraquark component in the lowest-lying scalar mesons. The tetraquark ground state emerges naturally as the lightest scalar nonet whereas higher excitations become heavier than their quark--antiquark counterparts and are thus likely to dissolve into the multiparticle continuum.

Forkel, Hilmar [Institut fuer Physik, Humboldt-Universitaet zu Berlin, D-12489 Berlin (Germany)

2011-10-21T23:59:59.000Z

5

Measurement of baryon production in B -meson decay  

Science Conference Proceedings (OSTI)

Using the CLEO detector at the Cornell Electron Storage Ring, we observe {ital B}-meson decays to {Lambda}{sub {ital c}}{sup +} and report on improved measurements of inclusive branching fractions and momentum spectra of other baryons. For the inclusive decay {ital {bar B}}{r arrow}{Lambda}{sub {ital c}}{sup +}{ital X} with {Lambda}{sub {ital c}}{sup +}{r arrow}{ital pK}{sup {minus}}{pi}{sup +}, we find that the product branching fraction {ital B}({ital {bar B}}{r arrow}{Lambda}{sub {ital c}}{sup +}{ital X}){ital B}({Lambda}{sub {ital c}}{sup +}{r arrow}{ital pK}{sup {minus}}{pi}{sup +})=(0.273{plus minus}0.051{plus minus} 0.039)%. Our measured inclusive branching fractions to noncharmed baryons are {ital B}({ital B}{r arrow}{ital pX})=(8.0{plus minus}0.5{plus minus}0.3)%, {ital B}({ital B}{r arrow}{Lambda}{ital X})=(3.8{plus minus}0.4{plus minus}0.6)%, and {ital B}({ital B}{r arrow}{Xi}{sup {minus}}{ital X})=(0.27{plus minus}0.05{plus minus}0.04)%. From these rates and studies of baryon-lepton and baryon-antibaryon correlations in {ital B} decays, we have estimated the branching fraction {ital B}({ital {bar B}}{r arrow}{Lambda}{sub {ital c}}{sup +}{ital X}) to be (6.4{plus minus}0.8{plus minus}0.8)%. Combining these results, we calculate {ital B}({Lambda}{sub {ital c}}{sup +}{r arrow}{ital pK}{sup {minus}}{pi}{sup +}) to be (4.3{plus minus}1.0{plus minus}0.8)%.

Crawford, G.; Fulton, R.; Jensen, T.; Johnson, D.R.; Kagan, H.; Kass, R.; Malchow, R.; Morrow, F.; Whitmore, J.; Wilson, P.; Bortoletto, D.; Brown, D.; Dominick, J.; McIlwain, R.L.; Miller, D.H.; Modesitt, M.; Ng, C.R.; Schaffner, S.F.; Shibata, E.I.; Shipsey, I.P.J.; Battle, M.; Kroha, H.; Sparks, K.; Thorndike, E.H.; Wang, C.; Alam, M.S.; Kim, I.J.; Li, W.C.; Lou, X.C.; Nemati, B.; Romero, V.; Sun, C.R.; Wang, P.; Zoeller, M.M.; Goldberg, M.; Haupt, T.; Horwitz, N.; Jain, V.; Kennett, R.; Mestayer, M.D.; Moneti, G.C.; Rozen, Y.; Rubin, P.; Skwarnicki, T.; Stone, S.; Thusalidas, M.; Yao, W.; Zhu, G.; Barnes, A.V.; Bartelt, J.; Csorna, S.E.; Letson, T.; Alexander, J.; Artuso, M.; Bebek, C.; Berkelman, K.; Besson, D.; Browder, T.; Cassel, D.G.; Cheu, E.; Coffman, D.M.; Drell, P.S.; Ehrlich, R.; Galik, R.S.; Garcia-Sciveres, M.; Geiser, B.; Gittelman, B.; Gray, S.W.; Hartill, D.L.; Heltsley, B.K.; Honscheid, K.; Kandaswamy, J.; Katayama, N.; Kreinick, D.L.; Lewis, J.D.; Ludwig, G.S.; Mas

1992-02-01T23:59:59.000Z

6

RESULTS ON CHARMED BARYONS AND MESONS FROM THE SLAC-LBL MARK II DETECTOR AT SPEAR  

E-Print Network (OSTI)

1, 309 (1978). Members of the SLAC-LBL Mark II collaborationBatavia, Illinois, August 2 3 - 2 9 , 1979; SLAC-PUB-2I+I9.BARYONS AND MESONS FROM THE SLAC-LBL MARK II DETECTOR AT

Goldhaber, G.

2010-01-01T23:59:59.000Z

7

Study of B-Meson Decays to Final States with a Single Charm Baryon  

Science Conference Proceedings (OSTI)

A study of B-meson decays to final states with a single charm baryon is presented based on data recorded by the BABAR detector at the Stanford Linear Accelerator Center. Although the B meson is the lightest bottom-flavored meson, it is heavy enough to decay to a baryon made of three quarks and an antibaryon made of three antiquarks. By studying the baryonic weak decays of the B meson, we can investigate baryon production mechanisms in heavy meson decays. In particular, we measure the rates of the decays B{sup -} {yields} {Lambda}{sub c}{sup +}{bar p}{pi}{sup -} and {bar B}{sup 0} {yields} {Lambda}{sub c}{sup +}{bar p}. Comparing these rates, we confirm an observed trend in baryonic B decays that the decay with the lower energy release, B{sup -} {yields} {Lambda}{sub c}{sup +}{bar p}{pi}{sup -}, is favored over {bar B}{sup 0} {yields} {Lambda}{sub c}{sup +}{bar p}. The dynamics of the baryon-antibaryon ({Lambda}{sub c}{sup +}{bar p}) system in the three-body decay also provide insight into baryon-antibaryon production mechanisms. The B{sup -} {yields} {Lambda}{sub c}{sup +}{bar p}{pi}{sup -} system is a laboratory for searches for excited {Sigma}{sub c} baryon states; we observe the resonant decays B{sup -} {yields} {Sigma}{sub c}(2455){sup 0}{bar p} and B{sup -} {yields} {Sigma}{sub c}(2800){sup 0}{bar p}. This is the first observation of the decay B{sup -} {yields} {Sigma}{sub c}(2800){sup 0}{bar p}; however, the mass of the observed {Sigma}{sub c}(2800){sup 0} state is inconsistent with previous measurements. Finally, we examine the angular distribution of the B{sup -} {yields} {Sigma}{sub c}(2455){sup 0}{bar p} decays and measure the spin of the {Sigma}{sub c}(2455){sup 0} baryon to be J = 1/2, as predicted by the quark model.

Majewski, Stephanie A.; /SLAC

2009-06-02T23:59:59.000Z

8

The Thermal Delocalization of the Flux Tubes in Mesons and Baryons  

Science Conference Proceedings (OSTI)

The gluon action density in a static mesonic system is analyzed at finite temperature using lattice QCD techniques in quenched QCD. The obtained results are compared to predictions of bosonic string models for the flux-tube profiles to understand the changes of the flux-tube profiles with temperature. The mesonic flux tube curved-width profile is found to compare well with that of the bosonic string at large distances. In the intermediate distance region, a free bosonic string behaviour is observed for analysis performed on highly UV-filtered gauge configurations. Extending the analysis to the static baryon reveals a delocalization of the baryonic node in the Y-shape gluonic configuration observed at zero temperature. At finite temperature, a filled delta-shaped configuration is observed, even at large distances. We study a baryonic string model at finite temperature.

Bakry, Ahmed S.; Leinweber, Derek B.; Williams, Anthony G. [Special Research Center for the Subatomic Structure of Matter, Departement of Physics, Adelaide, South Australia 5005 (Australia)

2011-05-24T23:59:59.000Z

9

Baryon-Number-Induced Chern-Simons Couplings of Vector and Axial-Vector Mesons in Holographic QCD  

Science Conference Proceedings (OSTI)

We show that holographic models of QCD predict the presence of a Chern-Simons coupling between vector and axial-vector mesons at finite baryon density. In the Anti de Sitter/Conformal Field Theory dictionary, the coefficient of this coupling is proportional to the baryon number density and is fixed uniquely in the five-dimensional holographic dual by anomalies in the flavor currents. For the lightest mesons, the coupling mixes transverse {rho} and a{sub 1} polarization states. At sufficiently large baryon number densities, it produces an instability, which causes the {rho} and a{sub 1} mesons to condense in a state breaking both rotational and translational invariance.

Domokos, Sophia K.; Harvey, Jeffrey A. [Enrico Fermi Institute and Department of Physics, University of Chicago, Chicago, Illinois 60637 (United States)

2007-10-05T23:59:59.000Z

10

History of exotic Meson (4-quark) and Baryon (5-quark) States  

E-Print Network (OSTI)

I briefly review the history of exotic meson (4-quark) and baryon (5-quark) states, which is rooted in the formalism of Regge pole and duality. There are robust model-independent predictions for the exchange of 4-quark (Baryonium) Regge trajectories in several processes, which are strongly supported by experiment. On the other hand the predictions for the spectroscopy of 4-quark resonances are based on specific QCD inspired models, with some experimental support. The corresponding predictions for the recently discovered exotic baryon (Pentaquark) state are briefly discussed.

D. P. Roy

2003-11-17T23:59:59.000Z

11

Ratios of heavy baryons to heavy mesons in relativistic nucleus-nucleus collisions  

E-Print Network (OSTI)

Heavy baryon/meson ratios Lambda(c)/D(0) and Lambda(b)/(B) over bar (0) in relativistic heavy ion collisions are studied in the quark coalescence model. For heavy baryons, we include production from coalescence of heavy quarks with free light quarks as well as with bounded light diquarks that might exist in the strongly coupled quark-gluon plasma produced in these collisions. Including the contribution from decays of heavy hadron resonances and also that due to fragmentation of heavy quarks that are left in the system after coalescence, the resulting Lambda(c)/D(0) and Lambda(b)/(B) over bar (0) ratios in midrapidity (vertical bar y vertical bar heavy baryon/meson ratios is found to be sensitive to the heavy quark mass, with the Lambda(b)/(B) over bar (0) ratio being much flatter than the Lambda(c)/D(0) ratio. The latter peaks at the transverse momentum p(T) similar or equal to 0.8 GeV but the peak shifts to p(T) similar or equal to 2 GeV in the absence of diquarks.

Oh, Yongseok; Ko, Che Ming; Lee, Su Houng; Yasui, Shigehiro.

2009-01-01T23:59:59.000Z

12

New thermal model with distinct freeze-out temperatures for baryons and mesons  

SciTech Connect

A significant amount of experimental data for particle production in high-energy heavy ion collisions (10 - 200 GeV/A at center of mass) has been accumulated during last years. Many different theoretical attempts have tried to describe these data using thermal models in the approximation of global thermal equilibrium considering only one freeze-out temperature. However the thermal models often are not able to describe adequately the whole multiplicities of hadrons. For instance, the abundance of strange particles is overestimate and the pion yields are underestimated. In this work is presented a thermal hadronic model with two different temperatures in order to describe the baryonic and mesonic chemical freeze-out in ultra-relativistic heavy ion collisions. The model is used to fit the particle population ratios of the hadrons produced in the reaction. The proposal is not merely to incorporate one additional degree of freedom in the adjustment procedure of data, but to present and alternative scenario for the freeze out stage in the collisional proces s. This new reformulated version of thermal model was applied to a set of data, offering a rather good improvement in the fitting of the calculated particle ratios to the data. The results suggest that the introduced model makes the thermal approach more robust to handle with a larger number of colliding systems and a more comprehensive set of reaction observables.

De Assis, Leonardo P. G.; Duarte, Sergio B. [Centro Brasileiro de Pesquisas Fisicas Dr. Xavier Sigaud 150, 22290-180 Rio de Janeiro-RJ (Brazil); Chiapparini, Marcelo [Instituto de Fisica, Universidade do Estado do Rio de Janeiro Rua Sao Francisco Xavier 524, 20 550-900 Rio de Janeiro-RJ (Brazil); Hirsch, Luciana R. [Departamento de Fisica, Universidade Tecnologica Federal do Parana Av. Sete de Setembro, 3165, 8 0230-901 Curitiba-PR (Brazil); Delfino, Antonio Jr. [Instituto de Fisica, Universidade Federal Fluminense Av. Gal. Milton Tavares de Souza, 24210-346 Niteroi-RJ (Brazil)

2013-05-06T23:59:59.000Z

13

Observation and study of the baryonic B-meson decays B?D(*)pp? (?)(?)  

E-Print Network (OSTI)

We present results for B-meson decay modes involving a charm meson, protons, and pions using 455×10[superscript 6] BB? pairs recorded by the BaBar detector at the SLAC PEP-II asymmetric-energy e[superscript +]e[superscript ...

Cowan, Ray Franklin

14

Baryons  

NLE Websites -- All DOE Office Websites (Extended Search)

Bariones Bariones Volver Principal ESTOY PERDIDO!!! Los bariones siempre contienen tres quarks y pueden también contener algunos gluones y pares quark-antiquark. Un protón = uud y un neutrón = udd. Cada quark dentro de un barión intercambia rápidamente cargas de color con los otros quarks en ese barión. Sin embargo, el barión (al igual que todos los hadrones) no tiene carga neta de color porque las diferentes cargas de color se cancelan entre sí. Los valores posibles del spin de los bariones son 1/2, 3/2, ..., es decir son fermiones. Por cada barión existe un barión de antimateria (antibarión) constituído por los 3 antiquarks correspondientes. Tabla de Bariones | Mesones Volver Use el botón "Volver" de su navegador o regrese a la Ruta del Modelo Standard.

15

Soft-core meson-baryon interactions. II. $?N$ and $K^+ N$ scattering  

E-Print Network (OSTI)

The $\\pi N$ potential includes the t-channel exchanges of the scalar-mesons $\\sigma$ and f_0, vector-meson $\\rho$, tensor-mesons f_2 and f_2' and the Pomeron as well as the s- and u-channel exchanges of the nucleon N and the resonances $\\Delta$, Roper and S_{11}. These resonances are not generated dynamically. We consider them as, at least partially, genuine three-quark states and we treat them in the same way as the nucleon. The latter two resonances were needed to find the proper behavior of the phase shifts at higher energies in the corresponding partial waves. The soft-core $\\pi N$-model gives an excellent fit to the empirical $\\pi N$ S- and P-wave phase shifts up to T_{lab}=600 MeV. Also the scattering lengths have been reproduced well and the soft-pion theorems for low-energy $\\pi N$ scattering are satisfied. The soft-core model for the $K^+ N$ interaction is an SU_f(3)-extension of the soft-core $\\pi N$-model. The $K^+ N$ potential includes the t-channel exchanges of the scalar-mesons a_0, $\\sigma$ and f_0, vector-mesons $\\rho$, $\\omega$ and $\\phi$, tensor-mesons a_2, f_2 and f_2' and the Pomeron as well as u-channel exchanges of the hyperons $\\Lambda$ and $\\Sigma$. The fit to the empirical $K^+ N$ S-, P- and D-wave phase shifts up to T_{lab}=600 MeV is reasonable and certainly reflects the present state of the art. Since the various $K^+ N$ phase shift analyses are not very consistent, also scattering observables are compared with the soft-core $K^+ N$-model. A good agreement for the total and differential cross sections as well as the polarizations is found.

H. Polinder; Th. A. Rijken

2005-05-31T23:59:59.000Z

16

Mesons  

NLE Websites -- All DOE Office Websites (Extended Search)

Mesones Volver Principal ESTOY PERDIDO Un mesn est compuesto por un quark y un antiquark, ligados por medio de gluones. Un ejemplo es un pin, de carga +1, ( +), que est...

17

Nuclear modification factor of nonphotonic electrons in heavy-ion collisions, and the heavy-flavor baryon-to-meson ratio  

E-Print Network (OSTI)

The nuclear modification factor R(AA) of nonphotonic electrons in Au + Au collisions at root(S)NN = 200 GeV is studied by considering the decays of heavy-flavor hadrons produced in a quark coalescence model. Although an enhanced Lambda(c)/D(0) ratio is predicted by the coalescence model, it is peaked at small transverse momenta (similar to 2 GeV) due to the large difference between heavy and light quark masses. As a result, the enhanced Lambda(c)/D(0) ratio, which is expected to suppress the electron R(AA) as the branching ratio of Lambda(c) decay into electrons is smaller than that of D(0), does not lead to additional suppression of the electron R(AA) at large transverse momenta (>= 5 GeV), where the suppression is mainly due to heavy quark energy loss in produced quark-gluon plasma. Also, the enhanced Lambda(b)/(B) over bar (0) ratio predicted by the coalescence model has even smaller effect on the nonphotonic electron R(AA) as bottom baryons and mesons have similar branching ratios for semileptonic decays into electrons.

Oh, Yongseok; Ko, Che Ming.

2009-01-01T23:59:59.000Z

18

Observation and Study of the Baryonic B-meson Decays B to D(*) p pbar (pi) (pi)  

SciTech Connect

We present results for B-meson decay modes involving a charm meson, protons, and pions using 455 x 10{sup 6} B{bar B} pairs recorded by the BABAR detector at the SLAC PEP-II asymmetric-energy e{sup +}e{sup -} collider. The branching fractions are measured for the following ten decays: {bar B}{sup 0} {yields} D{sup 0}p{bar p}, {bar B}{sup 0} {yields} D*{sup 0}p{bar p}, {bar B}{sup 0} {yields} D{sup +}p{bar p}{pi}{sup -}, {bar B}{sup 0} {yields} D*{sup +}p{bar p}{pi}{sup -}, B{sup -} {yields} D{sup 0}p{bar p}{pi}{sup -}, B{sup -} {yields} D*{sup 0}pp{pi}{sup -}, {bar B}{sup 0} {yields} D{sup 0}p{bar p}{pi}{sup -}{pi}{sup +}, {bar B}{sup 0} {yields} D*{sup 0}p{bar p}{pi}{sup -}{pi}{sup +}, B{sup -} {yields} D{sup +}p{bar p}{pi}{sup -}{pi}{sup -}, and B{sup -} {yields} D*{sup +}p{bar p}{pi}{sup -}{pi}{sup -}. The four B{sup -} and the two five-body B{sup 0} modes are observed for the first time. The four-body modes are enhanced compared to the three- and the five-body modes. In the three-body modes, the M(p{bar p}) and M(D{sup (*)0}p) invariant mass distributions show enhancements near threshold values. In the four-body mode {bar B}{sup 0} {yields} D{sup +}p{bar p}{pi}{sup -}, the M(p{pi}{sup -}) distribution shows a narrow structure of unknown origin near 1.5GeV/c{sup 2}. The distributions for the five-body modes, in contrast to the others, are similar to the expectations from uniform phase-space predictions.

del Amo Sanchez, P.; Lees, J.P.; Poireau, V.; Prencipe, E.; Tisserand, V.; /Annecy, LAPP; Garra Tico, J.; Grauges, E.; /Barcelona U., ECM; Martinelli, M.; Palano, A.; Pappagallo, M.; /Bari U. /INFN, Bari; Eigen, G.; Stugu, B.; Sun, L.; /Bergen U.; Battaglia, M.; Brown, D.N.; Hooberman, B.; Kerth, L.T.; Kolomensky, Yu.G.; Lynch, G.; Osipenkov, I.L.; Tanabe, T.; /LBL, Berkeley /UC, Berkeley /Birmingham U. /Ruhr U., Bochum /British Columbia U. /Brunel U. /Novosibirsk, IYF /UC, Irvine /UC, Riverside /UC, Santa Barbara /UC, Santa Cruz /Caltech /Cincinnati U. /Colorado U. /Colorado State U. /Dortmund U. /Dresden, Tech. U. /Ecole Polytechnique /Edinburgh U. /Ferrara U. /INFN, Ferrara /Frascati /Genoa U. /INFN, Genoa /Indian Inst. Tech., Guwahati /Harvard U. /Heidelberg U. /Humboldt U., Berlin /Imperial Coll., London /Iowa State U. /Iowa State U. /Johns Hopkins U. /Orsay, LAL /LLNL, Livermore /Liverpool U. /Queen Mary, U. of London /Royal Holloway, U. of London /Louisville U. /Mainz U., Inst. Kernphys. /Manchester U., Comp. Sci. Dept. /Maryland U. /Massachusetts U., Amherst /MIT /McGill U. /Milan U. /INFN, Milan /Mississippi U. /Montreal U. /Naples U. /INFN, Naples /NIKHEF, Amsterdam /Notre Dame U. /Ohio State U. /Oregon U. /Padua U. /INFN, Padua /Paris U., VI-VII /Perugia U. /INFN, Perugia /INFN, Pisa /Princeton U. /Rome U. /INFN, Rome /Rostock U. /Rutherford /DAPNIA, Saclay /SLAC /South Carolina U. /Southern Methodist U. /Stanford U., Phys. Dept. /SUNY, Albany /Tel Aviv U. /Tennessee U. /Texas U. /Texas U., Dallas /Turin U. /INFN, Turin /Trieste U. /INFN, Trieste /Valencia U., IFIC /Victoria U. /Warwick U. /Wisconsin U., Madison

2012-02-15T23:59:59.000Z

19

Light Vector Mesons  

E-Print Network (OSTI)

This article reviews the current status of experimental results obtained in the measurement of light vector mesons produced in proton-proton and heavy ion collisions at different energies. The review is focused on two phenomena related to the light vector mesons; the modification of the spectral shape in search of Chiral symmetry restoration and suppression of the meson production in heavy ion collisions. The experimental results show that the spectral shape of light vector mesons are modified compared to the parameters measured in vacuum. The nature and the magnitude of the modification depends on the energy density of the media in which they are produced. The suppression patterns of light vector mesons are different from the measurements of other mesons and baryons. The mechanisms responsible for the suppression of the mesons are not yet understood. Systematic comparison of existing experimental results points to the missing data which may help to resolve the problem.

Alexander Milov

2008-09-23T23:59:59.000Z

20

Baryon Spectroscopy and Resonances  

SciTech Connect

A short review of current efforts to determine the highly excited state spectrum of QCD, and in particular baryons, using lattice QCD techniques is presented. The determination of the highly excited spectrum of QCD is a major theoretical and experimental challenge. The experimental investigation of the excited baryon spectrum has been a long-standing element of the hadronic-physics program, an important component of which is the search for so-called 'missing resonances', baryonic states predicted by the quark model based on three constituent quarks but which have not yet been observed experimentally. Should such states not be found, it may indicate that the baryon spectrum can be modeled with fewer effective degrees of freedom, such as in quark-diquark models. In the past decade, there has been an extensive program to collect data on electromagnetic production of one and two mesons at Jefferson Lab, MIT-Bates, LEGS, MAMI, ELSA, and GRAAL. To analyze these data, and thereby refine our knowledge of the baryon spectrum, a variety of physics analysis models have been developed at Bonn, George Washington University, Jefferson Laboratory and Mainz. To provide a theoretical determination and interpretation of the spectrum, ab initio computations within lattice QCD have been used. Historically, the calculation of the masses of the lowest-lying states, for both baryons and mesons, has been a benchmark calculation of this discretized, finite-volume computational approach, where the aim is well-understood control over the various systematic errors that enter into a calculation; for a recent review. However, there is now increasing effort aimed at calculating the excited states of the theory, with several groups presenting investigations of the low-lying excited baryon spectrum, using a variety of discretizations, numbers of quark flavors, interpolating operators, and fitting methodologies. Some aspects of these calculations remain unresolved and are the subject of intense effort, notably the ordering of the Roper resonance in the low-lying Nucleon spectrum.

Robert Edwards

2011-12-01T23:59:59.000Z

Note: This page contains sample records for the topic "mesons contents baryons" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


21

Relativistic SU(3) chiral baryon-baryon Lagrangian up to order q^2  

E-Print Network (OSTI)

We construct the most general chiral effective Lagrangian for baryon-baryon contact interactions in flavor SU(3) up to order q^2 using a covariant power counting. A subset of these contact terms contributes to the baryon-baryon potential in chiral effective field theory. The Lorentz invariant effective Lagrangian is constructed to fulfill the invariance under charge conjugation, parity transformation, Hermitian conjugation and the local chiral symmetry group SU(3)_L x SU(3)_R. Goldstone bosons and external fields are included as well, thus providing additional four-baryon contact vertices involving e.g. pseudoscalar mesons and/or photons. In order to eliminate the linearly dependent terms, we use the Fierz identities, the equations of motion, and a Cayley-Hamilton relation for SU(3). As an application the baryon-baryon scattering contact potentials in low partial waves are considered.

Stefan Petschauer; Norbert Kaiser

2013-05-15T23:59:59.000Z

22

Searches for the baryon- and lepton-number violating decays B[superscript 0]-->Lambda c+l-, B--->Lambda l-, and B--->Lambda[over-bar] l- l-  

E-Print Network (OSTI)

Searches for B mesons decaying to final states containing a baryon and a lepton are performed, where the baryon is either ?c or ? and the lepton is a muon or an electron. These decays violate both baryon and lepton number ...

Cowan, Ray Franklin

23

Isospin Splittings of Doubly Heavy Baryons  

SciTech Connect

The SELEX Collaboration has reported a very large isospin splitting of doubly charmed baryons. We show that this effect would imply that the doubly charmed baryons are very compact. One intriguing possibility is that such baryons have a linear geometry Q-q-Q where the light quark q oscillates between the two heavy quarks Q, analogous to a linear molecule such as carbon dioxide. However, using conventional arguments, the size of a heavy-light hadron is expected to be around 0.5 fm, much larger than the size needed to explain the observed large isospin splitting. Assuming the distance between two heavy quarks is much smaller than that between the light quark and a heavy one, the doubly heavy baryons are related to the heavy mesons via heavy quark-diquark symmetry. Based on this symmetry, we predict the isospin splittings for doubly heavy baryons including {Xi}{sub cc}, {Xi}{sub bb} and {Xi}{sub bc}. The prediction for the {Xi}{sub cc} is much smaller than the SELEX value. On the other hand, the {Xi}{sub bb} baryons are predicted to have an isospin splitting as large as (6.3 {+-} 1.7) MeV. An experimental study of doubly bottomed baryons is therefore very important to better understand the structure of baryons with heavy quarks.

Brodsky, Stanley J.; /SLAC; Guo, Feng-Kun; /Bonn U., HISKP /Bonn U.; Hanhart, Christoph; /Julich, Forschungszentrum /JCHP, Julich /IAS, Julich; Meissner, Ulf-G.; /Julich, Forschungszentrum /JCHP, Julich /IAS, Julich /Bonn U., HISKP /Bonn U.

2011-08-18T23:59:59.000Z

24

Baryons 2002: Outlook  

E-Print Network (OSTI)

Summary and outlook presented at the 9th International Conference on the Structure of Baryons (BARYONS 2002), Jefferson Lab, March 3-8, 2002

Wolfram Weise

2002-06-05T23:59:59.000Z

25

Dynamical coupled-channels study of meson production reactions from EBACatJLab  

Science Conference Proceedings (OSTI)

We present the current status of a combined and simultaneous analysis of meson production reactions based on a dynamical coupled-channels (DCC) model, which is conducted at Excited Baryon Analysis Center (EBAC) of Jefferson Lab.

Kamano, Hiroyuki [Excited Baryon Analysis Center (EBAC), Thomas Jefferson National Accelerator Facility, Newport News, VA 23606 (United States)

2011-10-24T23:59:59.000Z

26

Hyperon-nucleon interaction and baryonic contact terms in SU(3) chiral effective field theory  

E-Print Network (OSTI)

In this proceeding we summarize results for baryonic contact terms derived within SU(3) chiral effective field theory. The four-baryon contact terms, necessary for the description of the hyperon-nucleon interaction, include SU(3) symmetric and explicit chiral symmetry breaking terms. They also include four-baryon contact terms involving pseudoscalar mesons, which become important for three-body forces. Furthermore we derive the leading order six-baryon contact terms in the non-relativistic limit and study their contribution to the $\\Lambda NN$ three-body contact interaction. These results could play an important role in studies of hypernuclei or hyperons in nuclear matter.

Stefan Petschauer

2013-12-16T23:59:59.000Z

27

Meson Photoproduction Experiments with CLAS  

SciTech Connect

A large part of the experimental program in Hall B of the Jefferson Lab is dedicated to light baryon spectroscopy. Meson photoprodcution experiments are essential part of this program. CEBAF Large Acceptance Spectrometer (CLAS) and availability of circularly and linearly polarized tagged photon beams and frozen spin polarized targets provide unique conditions for this type of experiments. This combination of experimental tools gives a remarkable opportunity to measure double polarization observables for different pseudo-scalar meson photoproduction processes. For the first time, a complete or nearly complete measurement became possible and will facilitate model independent extraction of the reaction amplitude. An overview of the experimental program and its current status together with recent results on double polarization measurements in ?{sup +} photoproduction are presented.

Eugene Pasyuk

2012-12-01T23:59:59.000Z

28

Physics Out Loud - Baryon  

NLE Websites -- All DOE Office Websites (Extended Search)

User Facility Previous Video (User Facility) Physics Out Loud Main Index Next Video (Cerenkov Light) Cerenkov Light Baryon David Lawrence, a physicist, describes the class of...

29

Chiral Analysis of Quenched Baryon Masses  

E-Print Network (OSTI)

We extend to quenched QCD an earlier investigation of the chiral structure of the masses of the nucleon and the delta in lattice simulations of full QCD. Even after including the meson-loop self-energies which give rise to the leading and next-to-leading non-analytic behaviour (and hence the most rapid variation in the region of light quark mass), we find surprisingly little curvature in the quenched case. Replacing these meson-loop self-energies by the corresponding terms in full QCD yields a remarkable level of agreement with the results of the full QCD simulations. This comparison leads to a very good understanding of the origins of the mass splitting between these baryons.

R. D. Young; D. B. Leinweber; A. W. Thomas; S. V. Wright

2002-05-16T23:59:59.000Z

30

MESONS --- 1998 UPDATE  

NLE Websites -- All DOE Office Websites (Extended Search)

MESONS MESONS in the 1998 Review of Particle Physics Please use this CITATION: C. Caso et al. (Particle Data Group), The European Physical Journal C3 (1998) 1 Cut-off date for this update was January 1998. Some of the Particle Listings also have Review articles. PostScript Files PDF Files Combined list of PostScript and PDF Files (with the number of pages) PostScript Files for the Mesons * PostScript Light Unflavored Mesons (pi, eta, rho, ...) * PostScript Strange Mesons (K's) * PostScript Charmed Mesons (D's) * PostScript Charmed, Strange Mesons (D(s)'s) * PostScript Bottom Mesons (B's) * PostScript Bottom, Strange Mesons (B(s)'s) * PostScript Bottom, Charmed Mesons (B(c)'s) * PostScript c cbar Mesons (eta(c), ... J/psi, ... chi(c0)) * PostScript b bbar Mesons (Upsilon, ... chi(b0))

31

Thermodynamic phases and mesonic fluctuations in a chiral nucleon-meson model  

E-Print Network (OSTI)

Studies of the QCD phase diagram must properly include nucleonic degrees of freedom and their thermodynamics in the range of baryon chemical potentials characteristic of nuclear matter. A useful framework for incorporating relevant nuclear physics constraints in this context is a chiral nucleon-meson effective Lagrangian. In the present paper, such a chiral nucleon-meson model is extended with systematic inclusion of mesonic fluctuations using the functional renormalization group approach. The resulting description of the nuclear liquid-gas phase transition shows a remarkable agreement with three-loop calculations based on in-medium chiral effective field theory. No signs of a chiral first-order phase transition and its critical endpoint are found in the region of applicability of the model, at least up to twice the density of normal nuclear matter and at temperatures Tliquid-gas transition are also examined with a detailed study of the chiral susceptibility.

Matthias Drews; Thomas Hell; Bertram Klein; Wolfram Weise

2013-08-26T23:59:59.000Z

32

Applications of AdS/QCD and Light-Front Holography to Baryon Physics  

SciTech Connect

The correspondence between theories in anti-de Sitter space and field theories in physical space-time leads to an analytic, semiclassical model for strongly-coupled QCD which has scale invariance at short distances and color confinement at large distances. These equations, for both mesons and baryons, give a very good representation of the observed hadronic spectrum, including a zero mass pion. Light-front holography allows hadronic amplitudes in the AdS fifth dimension to be mapped to frame-independent light-front wavefunctions of hadrons in physical space-time, thus providing a relativistic description of hadrons at the amplitude level. The meson and baryon wavefunctions derived from light-front holography and AdS/QCD also have remarkable phenomenological features, including predictions for the electromagnetic form factors and decay constants. The approach can be systematically improved using light-front Hamiltonian methods. Some novel features of QCD for baryon physics are also discussed.

Brodsky, Stanley J.; /SLAC; de Teramond, Guy F.; /Costa Rica U.

2011-08-22T23:59:59.000Z

33

The Need for Polarization for Extracting Baryon Resonances and the NSTAR Program at CLAS  

SciTech Connect

We report on the NSTAR program in Hall B of JLab on using polarization observables to extract parameters of baryon resonances. The scientific purpose of the program is to improve the understanding of the underlying quark degrees of freedom, especially in the higher resonance regions, where we expect to uncover many of missing baryon resonances that mainly decay through multi-meson channels. With the high-quality beam of circularly- and linearly-polarized photons onto unpolarized and polarized proton and deteurium targets, and coupled with the nearly complete solid angle coverage of CLAS, we will extract the differential cross sections and associated polarization observables obtained by the photoproduction of vector mesons and kaons at center of mass energies of 1.7 to 2.2 GeV. The paper will primarily present the photon beam aspects of the excited baryon program.

Cole, Philip L. [Idaho State University, Dept. of Physics, Pocatello, Idaho 83209 (United States)

2007-10-26T23:59:59.000Z

34

Meson-baryon sigma terms in QCD Sum Rules  

E-Print Network (OSTI)

We evaluate the pion-nucleon and the pion-Delta sigma terms by employing the method of quantum chromodynamics (QCD) sum rules. The obtained value of the pion-nucleon sigma term is compatible with the larger values already anticipated by the recent calculations. It is also found that the pion-Delta sigma term is as large as the pion-nucleon sigma term.

G. Erkol; M. Oka

2007-05-28T23:59:59.000Z

35

Baryon Mass Extrapolation  

E-Print Network (OSTI)

Consideration of the analytical properties of pion-induced baryon self-energies leads to new functional forms for the extrapolation of light baryon masses. These functional forms reproduce the leading non-analytic behavior of chiral perturbation theory, the correct heavy-quark limit and have the advantage of containing information on the extended structure of hadrons. The forms involve only three unknown parameters which may be optimized by fitting to present lattice data. Recent dynamical fermion results from CP-PACS and UK-QCD are extrapolated using these new functional forms. We also use these functions to probe the limit of the chiral perturbative regime and shed light on the applicability of chiral perturbation theory to the extrapolation of present lattice QCD results.

Derek B. Leinweber; Anthony W. Thomas; Kazuo Tsushima; Stewart V. Wright

1999-09-14T23:59:59.000Z

36

THE BARYON CENSUS IN A MULTIPHASE INTERGALACTIC MEDIUM: 30% OF THE BARYONS MAY STILL BE MISSING  

Science Conference Proceedings (OSTI)

Although galaxies, groups, and clusters contain {approx}10% of the baryons, many more reside in the photoionized and shocked-heated intergalactic medium (IGM) and in the circumgalactic medium (CGM). We update the baryon census in the (H I) Ly{alpha} forest and warm-hot IGM (WHIM) at 10{sup 5-6} K traced by O VI {lambda}1032, 1038 absorption. From Enzo cosmological simulations of heating, cooling, and metal transport, we improve the H I and O VI baryon surveys using spatially averaged corrections for metallicity (Z/Z {sub Sun }) and ionization fractions (f {sub HI}, f {sub OVI}). Statistically, the O VI correction product correlates with column density, (Z/Z {sub Sun })f {sub OVI} Almost-Equal-To (0.015)(N {sub OVI}/10{sup 14} cm{sup -2}){sup 0.70}, with an N {sub OVI}-weighted mean of 0.01, which doubles previous estimates of WHIM baryon content. We also update the Ly{alpha} forest contribution to baryon density out to z = 0.4, correcting for the (1 + z){sup 3} increase in absorber density, the (1 + z){sup 4.4} rise in photoionizing background, and cosmological proper length dl/dz. We find substantial baryon fractions in the photoionized Ly{alpha} forest (28% {+-} 11%) and WHIM traced by O VI and broad-Ly{alpha} absorbers (25% {+-} 8%). The collapsed phase (galaxies, groups, clusters, CGM) contains 18% {+-} 4%, leaving an apparent baryon shortfall of 29% {+-} 13%. Our simulations suggest that {approx}15% reside in hotter WHIM (T {>=} 10{sup 6} K). Additional baryons could be detected in weaker Ly{alpha} and O VI absorbers. Further progress requires higher-precision baryon surveys of weak absorbers, down to minimum column densities N {sub HI} {>=} 10{sup 12.0} cm{sup -2}, N {sub OVI} {>=} 10{sup 12.5} cm{sup -2}, N {sub OVII} {>=} 10{sup 14.5} cm{sup -2}, using high signal-to-noise data from high-resolution UV and X-ray spectrographs.

Shull, J. Michael; Danforth, Charles W.; Smith, Britton D., E-mail: michael.shull@colorado.edu, E-mail: smit1685@msu.edu, E-mail: charles.danforth@colorado.edu [CASA, Department of Astrophysical and Planetary Sciences, University of Colorado, Boulder, CO 80309 (United States)

2012-11-01T23:59:59.000Z

37

Charmed Bottom Baryon Spectroscopy  

Science Conference Proceedings (OSTI)

The arena of doubly and triply heavy baryons remains experimentally unexplored to a large extent. This has led to a great deal of theoretical effort being put forth in the calculation of mass spectra in this sector. Although the detection of such heavy particle states may lie beyond the reach of experiments for some time, it is interesting to compare results between lattice QCD computations and continuum theoretical models. Several recent lattice QCD calculations exist for both doubly and triply charmed as well as doubly and triply bottom baryons. In this work we present preliminary results from the first lattice calculation of the mass spectrum of doubly and triply heavy baryons including both charm and bottom quarks. The wide range of quark masses in these systems require that the various flavors of quarks be treated with different lattice actions. We use domain wall fermions for 2+1 flavors (up down and strange) of sea and valence quarks, a relativistic heavy quark action for the charm quarks, and non-relativistic QCD for the heavier bottom quarks. The calculation of the ground state spectrum is presented and compared to recent models.

Zachary Brown, William Detmold, Stefan Meinel, Konstantinos Orginos

2012-09-01T23:59:59.000Z

38

Meson Summary Table See  

NLE Websites -- All DOE Office Websites (Extended Search)

Meson Summary Table See also the table of suggested qq quark-model assignments in the Quark Model section. * Indicates particles that appear in the preceding Meson Summary Table....

39

Baryonic Decays of Charmonium - a Window on Internal Baryon Structure  

E-Print Network (OSTI)

The baryonic decays of $J/ \\psi$ provide a new way to study the internal structure of baryons. A simple diquark model applied to the calculation of the $\\bar{B}B$ decay cross-sections is compared with the ordinary constituent quark model. Various models also give different predictions for the rates involving the $N^{\\ast}(1440)$ resonance in the final state.

A. Cieply

2004-12-03T23:59:59.000Z

40

Contents  

Science Conference Proceedings (OSTI)

Page 1. Volume 98, Number 6, November-December 1993 Journal of Research of the National Institute of Standards and Technology Contents ...

2003-10-21T23:59:59.000Z

Note: This page contains sample records for the topic "mesons contents baryons" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


41

Contents  

Science Conference Proceedings (OSTI)

Page 1. Volume 96, Number 4, July-August 1991 Journal of Research of the National Institute of Standards and Technology Contents Articles ...

2003-10-08T23:59:59.000Z

42

CONTENTS  

Science Conference Proceedings (OSTI)

Page 1. JOURNAL OF RESEARCH of the National Bureau of Standards Vol. 88, No. 6, November-December 1983 CONTENTS Page ...

2003-07-03T23:59:59.000Z

43

Contents  

Science Conference Proceedings (OSTI)

Page 1. Volume 97, Number 5, September-October 1992 Journal of Research of the National Institute of Standards and Technology Contents ...

2003-10-15T23:59:59.000Z

44

Contents  

Science Conference Proceedings (OSTI)

Page 1. Volume 96, Number 2, March-April 1991 Journal of Research of the National Institute of Standards and Technology Contents Articles ...

2003-10-06T23:59:59.000Z

45

Contents  

Science Conference Proceedings (OSTI)

Page 1. Volume 96, Number 6, November-December 1991 Journal of Research of the National Institute of Standards and Technology Contents ...

2003-10-10T23:59:59.000Z

46

Contents  

Science Conference Proceedings (OSTI)

Page 1. Volume 97, Number 6, November-December 1992 Journal of Research of the National Institute of Standards and Technology Contents ...

2003-10-15T23:59:59.000Z

47

Progress towards understanding baryon resonances  

Science Conference Proceedings (OSTI)

The composite nature of baryons manifests itself in the existence of a rich spectrum of excited states, in particular in the important mass region 1?2 GeV for the light-flavoured baryons. The properties of these resonances can be identified by systematic investigations using electromagnetic and strong probes, primarily with beams of electrons, photons, and pions. After decades of research, the fundamental degrees of freedom underlying the baryon excitation spectrum are still poorly understood. The search for hitherto undiscovered but predicted resonances continues at many laboratories around the world. Recent results from photo- and electroproduction experiments provide intriguing indications for new states and shed light on the structure of some of the known nucleon excitations. The continuing study of available data sets with consideration of new observables and improved analysis tools have also called into question some of the earlier findings in baryon spectroscopy. Other breakthrough measurements have been performed in the heavy-baryon sector, which has seen a fruitful period in recent years, in particular at the B factories and the Tevatron. First results from the large hadron collider indicate rapid progress in the field of bottom baryons. In this review, we discuss the recent experimental progress and give an overview of theoretical approaches.

Crede, Volker [FSU; Roberts, Winston [FSU

2013-07-01T23:59:59.000Z

48

The CLAS Excited Baryon Program at Jlab  

DOE Green Energy (OSTI)

Nucleons are complex systems of confined quarks and exhibit characteristic spectra of excited states. Highly excited nucleon states are sensitive to details of quark confinement which is poorly understood within Quantum Chromodynamics (QCD), the fundamental theory of strong interactions. Thus, measurements of excited states and the corresponding determination of their properties are needed to come to a better understanding of how confinement works in nucleons. However, the excited states of the nucleon cannot simply be inferred from cleanly separated spectral lines. Quite the contrary, a spectral analysis in nucleon resonance physics is challenging because of the fact that the resonances are broadly overlapping states which decay into a multitude of final states involving mesons and baryons. To provide a consistent and complete picture of an individual nucleon resonance, the various possible production and decay channels must be treated in a multichannel framework that permits separating resonance from background contributions. Very often, resonances reveal themselves more clearly through interference with dominant amplitudes. These interference terms can be isolated via polarization observables. The current CLAS effort is to utilize highly-polarized hydrogen and deuterium targets as well as polarized photon beams toward a complete measurement of a large number of reaction channels.

Volker Crede

2007-10-01T23:59:59.000Z

49

CONTENTS  

NLE Websites -- All DOE Office Websites (Extended Search)

CONTENTS CONTENTS Introduction ........................................................................................................3 ON THE HORIZON: Promising Research Efforts Currently Underway A Smarter Charge .........................................................................................4 Unlocking Fire Ice .........................................................................................5 CRISP Crunches Cyber Threats ....................................................................6 Gel Zeroes in on Cancer ...............................................................................7 Liquid Solvent: A Solid Solution for CO 2 .....................................................8 Real-time Grid Stability ................................................................................9

50

Decays of J/psi (3100) to baryon final states  

SciTech Connect

We present results for the decays of psi(3100) into baryon and hyperon final states. The sample studied here consists of 1.3 million produced psi decays. The decays into nonstrange baryons agree well with currently established results, but with better statistics. In addition, significant resonance formation in multibody final states is observed. The decay psi ..-->.. anti pp..gamma.., the first direct photon decay of the psi involving baryons in the final state, is presented and the theoretical implications of the decays are briefly explored. Several new decays of the psi involving strange baryons are explored, including the first observations of three body final states involving hyperons. The I-spin symmetry of the strong decay psi ..-->.. baryons has clearly been observed. The reduced matrix elements for psi ..-->.. B anti B are presented for final states of different SU(3) content. The B/sub 8/ anti B/sub 8/ results are in excellent agreement with the psi being an SU(3) singlet as are the results for psi ..-->.. B/sub 10/ anti B/sub 10/. We present the first evidence for the SU(3) violating decays of the type psi ..-->.. B/sub 8/ anti B/sub 10/ + c.c.. Angular distributions for psi ..-->.. B/sub 8/ anti B/sub 8/ are presented and compared with theoretical predictions. Statistics are limited, but the data tends to prefer other than a 1 + Cos/sup 2/theta distribution.

Eaton, M.W.

1982-05-01T23:59:59.000Z

51

Excited light isoscalar mesons from lattice QCD  

Science Conference Proceedings (OSTI)

I report a recent lattice QCD calculation of an excited spectrum of light isoscalar mesons, something that has up to now proved challenging for lattice QCD. With novel techniques we extract an extensive spectrum with high statistical precision, including spin-four states and, for the first time, light isoscalars with exotic quantum numbers. In addition, the hidden flavour content of these mesons is determined, providing a window on annihilation dynamics in QCD. I comment on future prospects including applications to the study of resonances.

Christopher Thomas

2011-07-01T23:59:59.000Z

52

String Correction for Baryon Orbital Excitations  

E-Print Network (OSTI)

The correction to the string junction three-quark potential in a baryon due to the proper moment of inertia of the QCD string is calculated. The magnitudes of the string corrections in P-wave heavy baryons are estimated.

Driga, O N; Veselov, A I

2010-01-01T23:59:59.000Z

53

Baryonic Dark Matter in Galaxies  

E-Print Network (OSTI)

Cosmological nucleosynthesis calculations imply that many of the baryons in the Universe must be dark. We discuss the likelihood that some of these dark baryons may reside in the discs or halos of galaxies. If they were in the form of compact objects, they would then be natural MACHO candidates, in which case they are likely to be the remnants of a first generation of pregalactic or protogalactic Population III stars. Various candidates have been proposed for such remnants - brown dwarfs, red dwarfs, white dwarfs, neutron stars or black holes - and we review the many types of observations (including microlensing searches) which can be used to constrain or exclude them.

B. J. Carr

2000-08-01T23:59:59.000Z

54

CONTENTS  

E-Print Network (OSTI)

February 2010This document is in the public domain and may be freely copied or reprinted. Disclaimer Mention of any company or product does not constitute endorsement by the National Institute for Occupational Safety and Health (NIOSH). In addition, citations to Web sites external to NIOSH do not constitute NIOSH endorsement of the sponsoring organizations or their programs or products. Furthermore, NIOSH is not responsible for the content of these Web sites. Ordering Information To receive documents or other information about occupational safety and health topics, contact NIOSH at

A. Breslin, Ph.D.

2010-01-01T23:59:59.000Z

55

CONTENTS  

E-Print Network (OSTI)

This report was prepared by Sargent & Lundy, L.L.C., hereinafter referred to as S&L, expressly for Perrin Quarles Associates, Inc., hereinafter referred to as PQA, under EPA Contract No. EP-W-07-064. Neither S&L nor any person acting on its behalf (a) makes any warranty, express or implied, with respect to the use of any information or methods disclosed in this report or (b) assumes any liability with respect to the use of any information or methods disclosed in this report. Although prepared with EPA funding and reviewed by the EPA, this report has not been approved by the EPA for publication as an EPA report. The contents do not necessarily reflect the views or policies of the EPA, nor does mention of trade names or commercial products constitute endorsement or recommendation for use. COAL-FIRED POWER PLANT HEAT RATE REDUCTIONS i

unknown authors

2009-01-01T23:59:59.000Z

56

Symmetry energy effects on the mixed hadron-quark phase at high baryon density  

Science Conference Proceedings (OSTI)

The phase transition of hadronic to quark matter at high baryon and isospin density is analyzed. Relativistic mean-field models are used to describe hadronic matter, and the MIT bag model is adopted for quark matter. The boundaries of the mixed phase and the related critical points for symmetric and asymmetric matter are obtained. Due to the different symmetry term in the two phases, isospin effects appear to be rather significant. With increasing isospin asymmetry the binodal transition line of the (T,{rho}{sub B}) diagram is lowered to a region accessible through heavy-ion collisions in the energy range of the new planned facilities (e.g., the FAIR/NICA projects). Some observable effects are suggested, in particular an isospin distillation mechanism with a more isospin asymmetric quark phase, to be seen in charged meson yield ratios, and an onset of quark number scaling of the meson-baryon elliptic flows. The presented isospin effects on the mixed phase appear to be robust with respect to even large variations of the poorly known symmetry term at high baryon density in the hadron phase. The dependence of the results on a suitable treatment of isospin contributions in effective QCD Lagrangian approaches, at the level of explicit isovector parts and/or quark condensates, is discussed.

Di Toro, M.; Greco, V.; Plumari, S. [Laboratori Nazionali del Sud INFN, I-95123 Catania (Italy); Pysics and Astronomy Department, University of Catania (Italy); Liu, B. [IHEP, Chinese Academy of Sciences, Beijing (China); Theoretical Physics Center for Scientific Facilities, Chinese Academy of Sciences, 100049 Beijing (China); Baran, V. [Pysics Faculty, University of Bucharest and NIPNE-HH (Romania); Colonna, M. [Laboratori Nazionali del Sud INFN, I-95123 Catania (Italy)

2011-01-15T23:59:59.000Z

57

Correlated Leading Baryon-antibaryon Production in e+e- to ccbar to Lambda_c+ antiLambda_c- X  

SciTech Connect

We present a study of 649 {+-} 35 e{sup +}e{sup -} {yields} c{bar c} events produced at {radical}s {approx} 10.6 GeV containing both a {Lambda}{sub c}{sup +} baryon and a {bar {Lambda}}{sub c}{sup -} antibaryon. The number observed is roughly four times that expected if the leading charmed hadron types are uncorrelated, confirming an observation by the CLEO Collaboration. We find a 2-jet topology in these events but very few additional baryons, demonstrating that the primary c and {bar c} are predominantly contained in a correlated baryon-antibaryon system. In addition to the charmed baryons we observe on average 2.6 {+-} 0.2 charged intermediate mesons, predominantly pions, carrying 65% of the remaining energy.

Aubert, B.; Karyotakis, Y.; Lees, J.P.; Poireau, V.; Prencipe, E.; Prudent, X.; Tisserand, V.; /Annecy, LAPP; Garra Tico, J.; Grauges, E.; /Barcelona U., ECM; Martinelli, M.; Palano, A.; Pappagallo, M.; /INFN, Bari /Bari U.; Eigen, G.; Stugu, B.; Sun, L.; /Bergen U.; Battaglia, M.; Brown, D.N.; Hooberman, B.; Kerth, L.T.; Kolomensky, Yu.G.; Lynch, G. /UC, Berkeley /Birmingham U. /Ruhr U., Bochum /British Columbia U. /Brunel U. /Novosibirsk, IYF /UC, Irvine /UCLA /UC, Riverside /UC, San Diego /UC, Santa Barbara /UC, Santa Cruz /Caltech /Cincinnati U. /Colorado U. /Colorado State U. /Dortmund U. /Dresden, Tech. U. /Ecole Polytechnique /Edinburgh U. /INFN, Ferrara /Ferrara U. /INFN, Ferrara /INFN, Ferrara /Ferrara U. /INFN, Ferrara /INFN, Ferrara /Ferrara U. /Frascati /INFN, Genoa /Genoa U. /INFN, Genoa /INFN, Genoa /Genoa U. /INFN, Genoa /INFN, Genoa /Genoa U. /Harvard U. /Heidelberg U. /Humboldt U., Berlin /Imperial Coll., London /Iowa State U. /Iowa State U. /Johns Hopkins U. /Orsay, LAL /LLNL, Livermore /Liverpool U. /Queen Mary, U. of London /Royal Holloway, U. of London /Louisville U. /Mainz U., Inst. Kernphys. /Manchester U. /Maryland U. /Massachusetts U., Amherst /MIT /McGill U. /INFN, Milan /Milan U. /INFN, Milan /INFN, Milan /Milan U. /Mississippi U. /Montreal U. /Mt. Holyoke Coll. /INFN, Naples /Naples U. /INFN, Naples /INFN, Naples /Naples U. /NIKHEF, Amsterdam /Notre Dame U. /Ohio State U. /Oregon U. /INFN, Padua /Padua U. /INFN, Padua /INFN, Padua /Padua U. /Paris U., VI-VII /Pennsylvania U. /INFN, Perugia /Perugia U. /INFN, Pisa /Pisa U. /INFN, Pisa /Pisa, Scuola Normale Superiore /INFN, Pisa /Pisa U. /INFN, Pisa /Princeton U. /INFN, Rome /INFN, Rome /Rome U. /INFN, Rome /INFN, Rome /Rome U. /INFN, Rome /INFN, Rome /Rome U. /INFN, Rome /INFN, Rome /Rome U. /INFN, Rome /Rostock U. /Rutherford /DAPNIA, Saclay /SLAC /South Carolina U. /Stanford U., Phys. Dept. /SUNY, Albany /Tel Aviv U. /Tennessee U. /Texas U. /Texas U., Dallas /INFN, Turin /Turin U. /INFN, Trieste /Trieste U. /Valencia U. /Victoria U. /Warwick U. /Wisconsin U., Madison

2011-08-22T23:59:59.000Z

58

Searches for the baryon- and lepton-number violating decays $B^0\\rightarrow\\Lambda_c^ \\ell^-$, $B^-\\rightarrow\\Lambda\\ell^-$, and $B^-\\rightarrow\\bar{\\Lambda}\\ell^-$  

SciTech Connect

Searches for B mesons decaying to final states containing a baryon and a lepton are performed, where the baryon is either {Lambda}{sub c} or {Lambda} and the lepton is a muon or an electron. These decays violate both baryon and lepton number and would be a signature of physics beyond the standard model. No significant signal is observed in any of the decay modes, and upper limits in the range (3.2 - 520) x 10{sup -8} are set on the branching fractions at the 90% confidence level.

del Amo Sanchez, P.; Lees, J.P.; Poireau, V.; Prencipe, E.; Tisserand, V.; /Annecy, LAPP; Garra Tico, J.; Grauges, E.; /Barcelona U., ECM; Martinelli, M.; /INFN, Bari /Bari U.; Milanes, D.A.; /INFN, Bari; Palano, A.; Pappagallo, M.; /INFN, Bari /Bari U.; Eigen, G.; Stugu, B.; Sun, L.; /Bergen U.; Brown, D.N.; Kerth, L.T.; Kolomensky, Yu.G.; Lynch, G.; Osipenkov, I.L.; /UC, Berkeley; Koch, H.; Schroeder, T.; /Ruhr U., Bochum /British Columbia U. /Brunel U. /Novosibirsk, IYF /UC, Irvine /UC, Riverside /UC, Santa Barbara /UC, Santa Cruz /Caltech /Cincinnati U. /Colorado U. /Colorado State U. /Dortmund U. /Dresden, Tech. U. /Ecole Polytechnique /Edinburgh U. /INFN, Ferrara /Ferrara U. /INFN, Ferrara /INFN, Ferrara /Ferrara U. /INFN, Ferrara /Frascati /INFN, Genoa /Genoa U. /INFN, Genoa /INFN, Genoa /Genoa U. /INFN, Genoa /Indian Inst. Tech., Guwahati /Harvard U. /Harvey Mudd Coll. /Heidelberg U. /Humboldt U., Berlin /Imperial Coll., London /Iowa State U. /Iowa State U. /Johns Hopkins U. /Paris U., VI-VII /LLNL, Livermore /Liverpool U. /Queen Mary, U. of London /Royal Holloway, U. of London /Royal Holloway, U. of London /Louisville U. /Mainz U., Inst. Kernphys. /Manchester U. /Maryland U. /Massachusetts U., Amherst /MIT /McGill U. /Milan U. /Milan U. /Milan U. /Milan U. /Milan U. /Mississippi U. /Montreal U. /INFN, Naples /Naples U. /NIKHEF, Amsterdam /NIKHEF, Amsterdam /Notre Dame U. /Ohio State U. /Oregon U. /INFN, Padua /Padua U. /INFN, Padua /INFN, Padua /Padua U. /Paris U., VI-VII /INFN, Perugia /Perugia U. /INFN, Pisa /Pisa U. /INFN, Pisa /Pisa, Scuola Normale Superiore /INFN, Pisa /Pisa U. /INFN, Pisa /Princeton U. /INFN, Rome /INFN, Rome /Rome U. /INFN, Rome /INFN, Rome /Rome U. /INFN, Rome /INFN, Rome /Rome U. /INFN, Rome /INFN, Rome /Rome U. /Rostock U. /Rutherford /DAPNIA, Saclay /SLAC /South Carolina U. /Southern Methodist U. /Stanford U., Phys. Dept. /SUNY, Albany /Tel Aviv U. /Tennessee U. /Texas Nuclear Corp., Austin /Texas U., Dallas /INFN, Turin /Turin U. /INFN, Trieste /Trieste U. /Valencia U. /Victoria U. /Warwick U. /Wisconsin U., Madison

2011-06-22T23:59:59.000Z

59

Baryons and baryonic matter in the large Nc and heavy quark limits  

E-Print Network (OSTI)

This paper explores properties of baryons and finite density baryonic matter in an artificial world in which N[subscript c], the number of colors, is large and the quarks of all species are degenerate and much larger than ...

Cohen, Thomas D.

60

Techniques in meson spectroscopy  

SciTech Connect

This report contains lectures on the following topics: the quark model and beyond using quantum chromodynamics; analysis of formation reactions; energy dependence of the partial wave amplitudes; where the data for the t-matrix analysis comes from; and coupled channel analysis of isoscalar mesons.

Longacre, R.S.

1991-12-31T23:59:59.000Z

Note: This page contains sample records for the topic "mesons contents baryons" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


61

Magnetized baryonic matter in holographic QCD  

E-Print Network (OSTI)

We investigate the properties of the Sakai-Sugimoto model at finite magnetic field and baryon chemical potentials. We show that in a finite magnetic field, there exists a spatially homogeneous configuration carrying finite baryon number density. At low magnetic field and baryon chemical potential the equation of state of the matter coincides with that obtained from the chiral perturbation theory Lagrangian with an anomalous term. We discuss the behavior of the system at larger magnetic fields.

Ethan G. Thompson; Dam T. Son

2008-06-02T23:59:59.000Z

62

Negative parity baryon decays in the 1/N{sub c} expansion  

Science Conference Proceedings (OSTI)

The partial decay widths of lowest lying negative parity baryons belonging to the 70-plet of SU(6) are analyzed in the framework of the 1/N{sub c} expansion. The channels considered are those with single pseudoscalar meson emission. The analysis is carried out to sub-leading order in 1/N{sub c} and to first order in SU(3) symmetry breaking. Conclusions about the magnitude of SU(3) breaking effects along with predictions for some unknown or poorly determined partial decay widths of known resonances are obtained.

Jayalath, C. [Department of Physics, Hampton University, Hampton, Virginia 23668 (United States); Thomas Jefferson National Accelerator Facility, Newport News, Virginia 23606 (United States); Department of Physics, Peradeniya University, Peradeniya 20400 (Sri Lanka); Goity, J. L. [Department of Physics, Hampton University, Hampton, Virginia 23668 (United States); Thomas Jefferson National Accelerator Facility, Newport News, Virginia 23606 (United States); Gonzalez de Urreta, E. [Department of Theoretical Physics, Comision Nacional de Energia Atomica, 1429 Buenos Aires (Argentina); CONICET, Rivadavia 1917, 1033 Buenos Aires (Argentina); Scoccola, N. N. [Department of Theoretical Physics, Comision Nacional de Energia Atomica, 1429 Buenos Aires (Argentina); CONICET, Rivadavia 1917, 1033 Buenos Aires (Argentina); Universidad Favaloro, Solis 453, 1078 Buenos Aires (Argentina)

2011-10-01T23:59:59.000Z

63

Negative parity baryon decays in the 1/N{sub c} expansion  

Science Conference Proceedings (OSTI)

The partial decay widths of lowest lying negative parity baryons belonging to the 70-plet of SU(6)are analyzed in the framework of the 1/N{sub c} expansion. The channels considered are those with single pseudoscalar meson emission. The analysis is carried out to sub-leading order in 1/Nc and to first order in SU(3) symmetry breaking. Conclusions about the magnitude of SU(3) breaking effects along with predictions for some unknown or poorly determined partial decay widths of known resonances are given.

Chandana Jayalath,Jose Goity,Emiliano Gonzalez de Urreta,Norberto Scoccola

2011-10-01T23:59:59.000Z

64

Gluon field distribution in baryons  

E-Print Network (OSTI)

Methods for revealing the distribution of gluon fields within the three-quark static-baryon potential are presented. In particular, we outline methods for studying the sensitivity of the source on the emerging vacuum response for the three-quark system. At the same time, we explore the possibility of revealing gluon-field distributions in three-quark systems in QCD without the use of gauge-dependent smoothing techniques. Renderings of flux tubes from a preliminary high-statistics study on a 12^3 X 24 lattice are presented.

F. Bissey; F-G. Cao; A. Kitson; B. G. Lasscock; D. B. Leinweber; A. I. Signal; A. G. Williams; J. M. Zanotti

2005-01-05T23:59:59.000Z

65

Light Meson Distribution Amplitudes  

E-Print Network (OSTI)

We calculated the first two moments of the light-cone distribution amplitudes for the pseudoscalar mesons ($\\pi$ and $K$) and the longitudinally polarised vector mesons ($\\rho$, $K^*$ and $\\phi$) as part of the UKQCD and RBC collaborations' $N_f=2+1$ domain-wall fermion phenomenology programme. These quantities were obtained with a good precision and, in particular, the expected effects of $SU(3)$-flavour symmetry breaking were observed. Operators were renormalised non-perturbatively and extrapolations to the physical point were made, guided by leading order chiral perturbation theory. The main results presented are for two volumes, $16^3\\times 32$ and $24^3\\times 64$, with a common lattice spacing. Preliminary results for a lattice with a finer lattice spacing, $32^3\\times64$, are discussed and a first look is taken at the use of twisted boundary conditions to extract distribution amplitudes.

R. Arthur; P. A. Boyle; D. Brömmel; M. A. Donnellan; J. M. Flynn; A. Jüttner; H. Pedroso de Lima; T. D. Rae; C. T. Sachrajda; B. Samways

2010-11-12T23:59:59.000Z

66

Results and Frontiers in Lattice Baryon Spectroscopy  

SciTech Connect

The Lattice Hadron Physics Collaboration (LHPC) baryon spectroscopy effort is reviewed. To date the LHPC has performed exploratory Lattice QCD calculations of the low-lying spectrum of Nucleon and Delta baryons. These calculations demonstrate the effectiveness of our method by obtaining the masses of an unprecedented number of excited states with definite quantum numbers. Future work of the project is outlined.

Bulava, John; Morningstar, Colin [Department of Physics, Carnegie Mellon University, Pittsburgh, PA 15213 (United States); Edwards, Robert; Richards, David [Thomas Jefferson National Accelerator Facility, Newport News, VA 23606 (United States); Fleming, George [Yale University New Haven, CT 06520 (United States); Juge, K. Jimmy [Department of Physics, University of the Pacific, Stockton, CA 95211 (United States); Lichtl, Adam C. [RBRC, Brookhaven National Laboratory, Upton, NY 11973 (United States); Mathur, Nilmani [Tata Institute of Fundamental Research, Mumbai 40005 (India); Wallace, Stephen J. [University of Maryland, College Park, MD 20742 (United States)

2007-10-26T23:59:59.000Z

67

Baryon Fluctuations in High Energy Nuclear Collisions  

E-Print Network (OSTI)

We propose that dramatic changes in the variances and covariance of protons and antiprotons can result if baryons approach chemical equilibrium in nuclear collisions at RHIC. To explore how equilibration alters these fluctuations, we formulate both equilibrium and nonequilibrium hadrochemical descriptions of baryon evolution. Contributions to fluctuations from impact parameter averaging and finite acceptance in nuclear collisions are numerically simulated.

Sean Gavin; Claude Pruneau

1999-07-09T23:59:59.000Z

68

An Alternative View of the Dynamical Origin of the P11 Nucleon Resonances: Results from the Excited Baryon Analysis Center  

Science Conference Proceedings (OSTI)

We present an alternative interpretation for the dynamical origin of the P{sub 11} nucleon resonances, which results from the dynamical coupled-channels analysis at Excited Baryon Analysis Center of Jefferson Lab. The results indicate the crucial role of the multichannel reaction dynamics in determining the N* spectrum. An understanding of the spectrum and structure of the excited nucleon (N*) states is a fundamental challenge in the hadron physics. The N* states, however, couple strongly to the meson-baryon continuum states and appear only as resonance states in the {gamma}N and {pi}N reactions. One can expect from such strong couplings that the (multichannel) reaction dynamics will affect significantly the N* states and cannot be neglected in extracting the N* parameters from the data and giving physical interpretations. It is thus well recognized nowadays that a comprehensive study of all relevant meson production reactions with {pi}N,{eta}N,{pi}{pi}N,KY, {hor_ellipsis} final states is necessary for a reliable extraction of the N* parameters. To address this challenging issue, the Excited Baryon Analysis Center (EBAC) of Jefferson Lab has been conducting the comprehensive analysis of the world data of {gamma}N,{pi}N {yields} {pi}N,{eta}N,{pi}{pi}N,KY, {hor_ellipsis} reactions systematically, covering the wide energy and kinematic regions. The analysis is pursued with a dynamical coupled-channels (DCC) model, the EBAC-DCC model, within which the unitarity among relevant meson-baryon channels, including the three-body {pi}{pi}N channel, is fully taken into account.

Hiroyuki Kamano

2012-04-01T23:59:59.000Z

69

Baryon destruction by asymmetric dark matter  

SciTech Connect

We investigate new and unusual signals that arise in theories where dark matter is asymmetric and carries a net antibaryon number, as may occur when the dark matter abundance is linked to the baryon abundance. Antibaryonic dark matter can cause induced nucleon decay by annihilating visible baryons through inelastic scattering. These processes lead to an effective nucleon lifetime of 10{sup 29}-10{sup 32} yrs in terrestrial nucleon decay experiments, if baryon number transfer between visible and dark sectors arises through new physics at the weak scale. The possibility of induced nucleon decay motivates a novel approach for direct detection of cosmic dark matter in nucleon decay experiments. Monojet searches (and related signatures) at hadron colliders also provide a complementary probe of weak-scale dark-matter-induced baryon number violation. Finally, we discuss the effects of baryon-destroying dark matter on stellar systems and show that it can be consistent with existing observations.

Davoudiasl, Hooman [Department of Physics, Brookhaven National Laboratory, Upton, New York 11973 (United States); Morrissey, David E.; Tulin, Sean [Theory Group, TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3 (Canada); Sigurdson, Kris [Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1 (Canada)

2011-11-01T23:59:59.000Z

70

Charmonium and Light Meson Spectroscopy  

E-Print Network (OSTI)

This talk reviews recent experimental results on selected topics in the spectroscopy of charmonia, charmonium-like states and light mesons.

Kai Zhu

2012-12-10T23:59:59.000Z

71

Quantum interferences in the $?N \\to e^+e^- N$ reaction close to the vector meson production threshold  

E-Print Network (OSTI)

The exclusive photoproduction of $e^+e^-$ pairs from nucleons close to the vector meson production threshold ($1.4electromagnetic and reflect mostly the nucleon magnetic structure. The $\\gamma N\\to e^+e^- N$ amplitudes arising from vector meson production and decay are derived from $\\gamma N\\to \\rho^0 N$ and $\\gamma N \\to \\omega N$ amplitudes supplemented by the Vector Meson Dominance assumption. The vector meson photoproduction amplitudes are calculated using a relativistic and unitary coupled-channel approach to meson-nucleon scattering. They depend sensitively on the coupling of vector fields to baryon resonances. The $\\gamma N \\to e^+e^- N$ differential cross sections display interference patterns. The interference of Bethe-Heitler pair production with vector meson $e^+e^-$ decay is quite small in the domain of validity of our model for all angles of the emitted $e^+e^-$ pair. The interference of $\\rho^0$- and $\\omega$-mesons in the $e^+e^-$ channel can be large. It is constructive for the $\\gamma p \\to e^+e^- p$ reaction and destructive for the $\\gamma n \\to e^+e^- n$ reaction. We discuss the shape and magnitude of the $e^+e^-$ pair spectra produced in the $\\gamma p \\to e^+e^- p$ and $\\gamma n \\to e^+e^- n$ reactions as functions of the pair emission angle and of the total center of mass energy $\\sqrt s$.

Matthias F. M. Lutz; Madeleine Soyeur

2005-03-31T23:59:59.000Z

72

BOSS: THE BARYON OSCILLATION SPECTROSCOPIC SURVEY Probing the Physics of Dark Energy with Baryon Acoustic Oscillations  

E-Print Network (OSTI)

BOSS: THE BARYON OSCILLATION SPECTROSCOPIC SURVEY Probing the Physics of Dark Energy with Baryon demand the existence of a pervasive new component of the Universe ("dark energy") with exotic physical on cosmological scales. Because of the fundamental importance of the dark energy problem, the Dark Energy Task

Knowles, David William

73

SIMULATIONS OF EARLY BARYONIC STRUCTURE FORMATION WITH STREAM VELOCITY. II. THE GAS FRACTION  

SciTech Connect

Understanding the gas content of high-redshift halos is crucial for studying the formation of the first generation of galaxies and reionization. Recently, Tseliakhovich and Hirata showed that the relative 'stream' velocity between the dark matter and baryons at the time of recombination-formally a second-order effect, but an unusually large one-can influence the later structure formation history of the universe. We quantify the effect of the stream velocity on the so-called characteristic mass-the minimum mass of a dark matter halo capable of retaining most of its baryons throughout its formation epoch-using three different high-resolution sets of cosmological simulations (with separate transfer functions for baryons and dark matter) that vary in box size, particle number, and the value of the relative velocity between the dark matter and baryons. In order to understand this effect theoretically, we generalize the linear theory filtering mass to properly account for the difference between the dark matter and baryonic density fluctuation evolution induced by the stream velocity. We show that the new filtering mass provides an accurate estimate for the characteristic mass, while other theoretical ansatzes for the characteristic mass are substantially less precise.

Naoz, Smadar [Institute for Theory and Computation, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)] [Institute for Theory and Computation, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Yoshida, Naoki [Department of Physics, University of Tokyo, Tokyo 113-0033 (Japan)] [Department of Physics, University of Tokyo, Tokyo 113-0033 (Japan); Gnedin, Nickolay Y., E-mail: snaoz@cfa.harvard.edu [Particle Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, IL 60510 (United States)

2013-01-20T23:59:59.000Z

74

Physics Out Loud - Hybrid Meson  

NLE Websites -- All DOE Office Websites (Extended Search)

Hadron Previous Video (Hadron) Physics Out Loud Main Index Next Video (Laser) Laser Hybrid Meson We're well on our way in exploring how the strong force glues the nucleus together....

75

Experimental Investigation of Weak Non-Mesonic Decay of 10Be(Lambda)Hypernuclei at CEBAF  

E-Print Network (OSTI)

Hypernuclei are convenient laboratory to study the baryon-baryon weak interaction and associated effective Hamiltonian. The strangeness changing process, in which a Lambda hyperon converts to a neutron with a release up to 176 MeV, provides a clear signal for a conversion of an s-quark to a d-quark. We propose to perform a non-mesonic weak decay study of 10Be(Lambda)hypernuclei using the (e,eK) reaction. These investigations will fully utilize the unique parameters of the CEBAF CW electron beam and RF system and are enabled by (1) the use of new detector for alpha particles based on the recently developed RF timing technique with picosecond resolution and (2) the small angle and large acceptance kaon spectrometer-HKS in Hall C.

S. Majewski; L. Majling; A. Margaryan; L. Tang

2005-08-05T23:59:59.000Z

76

High Statistics Analysis using Anisotropic Clover Lattices: (II) Three-Baryon Systems  

E-Print Network (OSTI)

We present the results of an exploratory Lattice QCD calculation of three-baryon systems through a high-statistics study of one ensemble of anisotropic clover gauge-field configurations with a pion mass of m_\\pi ~ 390 MeV. Because of the computational cost of the necessary contractions, we focus on correlation functions generated by interpolating-operators with the quantum numbers of the $\\Xi^0\\Xi^0 n$ system, one of the least demanding three baryon systems in terms of the number of contractions. We find that the ground state of this system has an energy of E_{\\Xi^0\\Xi^0n}= 3877.9\\pm 6.9\\pm 9.2\\pm3.3 MeV corresponding to an energy-shift due to interactions of \\delta E_{\\Xi^0\\Xi^0n}=E_{\\Xi^0\\Xi^0n}-2M_{\\Xi^0} -M_n=4.6\\pm 5.0\\pm 7.9\\pm 4.2 MeV. There are a significant number of time-slices in the three-baryon correlation function for which the signal-to-noise ratio is only slowly degrading with time. This is in contrast to the exponential degradation of the signal-to-noise ratio that is observed at larger times, and is due to the suppressed overlap of the source and sink interpolating-operators that are associated with the variance of the three-baryon correlation function onto the lightest eigenstates in the lattice volume (mesonic systems). As one of the motivations for this area of exploration is the calculation of the structure and reactions of light nuclei, we also present initial results for a system with the quantum numbers of the triton (pnn). This present work establishes a path to multi-baryon systems, and shows that Lattice QCD calculations of the properties and interactions of systems containing four and five baryons are now within sight.

Silas R. Beane; William Detmold; Thomas C Luu; Kostas Orginos; Assumpta Parreno; Martin J. Savage; Aaron Torok; Andre Walker-Loud

2009-05-04T23:59:59.000Z

77

MESON LISTINGS UNDER REVISION (FOR ENCODERS)  

NLE Websites -- All DOE Office Websites (Extended Search)

MESON LISTINGS UNDER REVISION MESON LISTINGS UNDER REVISION (FOR ENCODERS) This WWW page is designed so that encoders can get current Listings of encoded particles with the 'NODES' on the right-hand side of the page. Disclaimer These sections are private PDG files. Please do not quote or refer to them. The authors reserve the right to radically alter these non-completed sections from minute to minute. They are certainly not error free. Conservation Laws The List by Particle Code (includes hidden particle codes) The List in Book Order by Name Light Unflavored Mesons Summary Table Other Light Unflavored Mesons Strange Mesons Summary Table Charmed Mesons Summary Table Charmed, Strange Mesons Summary Table (c cbar) Mesons Summary Table (b bbar) Mesons Summary Table Non (q qbar) Candidates

78

BNL | Baryonic Oscillation Spectroscopic Survey (BOSS)  

NLE Websites -- All DOE Office Websites (Extended Search)

Baryonic Oscillation Spectroscopic Survey (BOSS) Baryonic Oscillation Spectroscopic Survey (BOSS) sloan telescope The 2.5-meter Sloan telescope in New Mexico Mapping the Luminous Universe How are galaxies clustered together? What is fueling the accelerating expansion of the universe? Just what is dark energy? These are the big questions that scientists working at the Baryon Oscillation Spectroscopic Survey (BOSS) are asking. Brookhaven National Lab is a member of BOSS, the largest of the four surveys that make up the Sloan Digital Sky Survey III, which maps the sky over the Northern Hemisphere with New Mexico's 2.5-meter Sloan telescope in an attempt to define dark energy and measure its effects. Building on the legacy of the Sloan Digital Sky Survey (SDSS) and SDSS-II, the SDSS-III collaboration is working to map the Milky Way, search

79

Scattering and mesons; P-matrix theory.  

E-Print Network (OSTI)

??We present the P-matrix, an alternative method to parameterize the S-matrix, which is particularly useful for low energy meson-meson scattering. We discuss its basic properties… (more)

Ramazano?lu, Fethï Mübïn

2006-01-01T23:59:59.000Z

80

Evidence for B Semileptonic Decays into the Lambda_c Charm Baryon  

SciTech Connect

We present the first evidence for B semileptonic decays into the charmed baryon {Lambda}{sub c}{sup +} based on 420 fb{sup -1} of data collected at the {Upsilon}(4S) resonance with the BABAR detector at the PEP-II e{sup +}e{sup -} storage rings. Events are tagged by fully reconstructing one of the B mesons in a hadronic decay mode. We measure the relative branching fraction {Beta}({bar B} {yields} {Lambda}{sub c}{sup +} X{ell}{sup -}{bar {nu}}{sub {ell}})/{Beta}({bar B} {yields} {Lambda}{sub c}{sup +}/{bar {Lambda}}{sub c}{sup -}X) = (3.2 {+-} 0.9{sub stat.} {+-} 0.9{sub syst.})%. The significance of the signal including the systematic uncertainty is 4.9 standard deviations.

Aubert, Bernard; Bona, M.; Karyotakis, Y.; Lees, J.P.; Poireau, V.; Prencipe, E.; Prudent, X.; Tisserand, V.; /Annecy, LAPP; Garra Tico, J.; Grauges, E.; /Barcelona U., ECM; Lopez, L.; Palano, Antimo; Pappagallo, M.; /Bari U. /INFN, Bari; Eigen, G.; Stugu, Bjarne; Sun, L.; /Bergen U.; Abrams, G.S.; Battaglia, M.; Brown, D.N.; Cahn, Robert N.; Jacobsen, R.G.; /LBL, Berkeley /Birmingham U. /Ruhr U., Bochum /Bristol U. /British Columbia U. /Brunel U. /Novosibirsk, IYF /UC, Irvine /UCLA /UC, Riverside /UC, San Diego /UC, Santa Barbara /UC, Santa Cruz /Caltech /Cincinnati U. /Colorado U. /Colorado State U. /Dortmund U. /Dresden, Tech. U. /Ecole Polytechnique /Edinburgh U. /Ferrara U. /INFN, Ferrara /Frascati /Genoa U. /INFN, Genoa /Harvard U. /Heidelberg U. /Humboldt U., Berlin /Imperial Coll., London /Iowa U. /Iowa State U. /Johns Hopkins U. /Orsay, LAL /LLNL, Livermore /Liverpool U. /Queen Mary, U. of London /Royal Holloway, U. of London /Louisville U. /Mainz U., Inst. Kernphys. /Manchester U. /Maryland U. /Massachusetts U., Amherst /MIT /McGill U. /Consorzio Milano Ricerche /INFN, Milan /Mississippi U. /Montreal U. /Mt. Holyoke Coll. /Napoli Seconda U. /INFN, Naples /NIKHEF, Amsterdam /Notre Dame U. /Ohio State U. /Oregon U. /Padua U. /INFN, Padua /Paris U., VI-VII /Pennsylvania U. /Perugia U. /INFN, Perugia /INFN, Pisa /Princeton U. /Banca di Roma /Frascati /Rostock U. /Rutherford /DAPNIA, Saclay /South Carolina U. /SLAC /Stanford U., Phys. Dept. /SUNY, Albany /Tennessee U. /Texas U. /Texas U., Dallas /Turin U. /INFN, Turin /Trieste U. /INFN, Trieste /Valencia U., IFIC /Victoria U. /Warwick U. /Wisconsin U., Madison

2008-11-05T23:59:59.000Z

Note: This page contains sample records for the topic "mesons contents baryons" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


81

Baryon spectroscopy with CLAS at Jefferson Lab  

Science Conference Proceedings (OSTI)

A substantial part of the experimental efforts at the experimental Hall-B of Jefferson Laboratory is dedicated to this studies of light baryon spectroscopy. In this report a general overview of the experimental capabilities in the Experimental Hall-B will be presented together with preliminary results of recent double polarization measurements and finally overall status of the program.

Eugene Pasyuk, CLAS Collaboration

2012-04-01T23:59:59.000Z

82

Parton Equilibration Enforcing Baryon Number Conservation  

E-Print Network (OSTI)

Parton equilibration for a thermally equilibrated but chemically non-equilibrated quark gluon plasma is presented. Parton equilibration is studied enforcing baryon numbver conservation. Process like quark flavour interchanging is also considered. The degree of equilibration is studied comparatively for the various reactions / constraints that are being considered.

Abhijit Sen

2007-10-01T23:59:59.000Z

83

Meson spectroscopy with unitary coupled-channels model for heavy-meson decay into three mesons  

Science Conference Proceedings (OSTI)

We develop a model for describing excited mesons decay into three mesons. The properties of the excited mesons can be extracted with this model. The model maintains the three-body unitarity that has been missed in previous data analyses based on the conventional isobar models. We study an importance of the three-body unitarity in extracting hadron properties from data. For this purpose, we use the unitary and isobar models to analyze the same pseudo data of {gamma}p {yields} {pi}{sup +}{pi}{sup +}{pi}{sup -}n, and extract the properties of excited mesons. We find a significant difference between the unitary and isobar models in the extracted properties of excited mesons, such as the mass, width and coupling strength to decay channels. Hadron properties such as quantum numbers (spin, parity, etc.), mass and (partial) width have been long studied as a subject called hadron spectroscopy. The hadron properties provide important information for understanding internal structure of the hadron and dynamics which governs it. The dynamics here is of course QCD in its nonperturbative regime. The hadron properties can be extracted from data through a careful analysis, in many cases, partial wave analysis (PWA). Thus it is essential for hadron spectroscopy to have a reliable theoretical analysis tool.

Satoshi Nakamura

2012-04-01T23:59:59.000Z

84

Quantum Electrodynamics for Vector Mesons  

Science Conference Proceedings (OSTI)

Quantum electrodynamics for {rho} mesons is considered. It is shown that, at the tree level, the value of the gyromagnetic ratio of the {rho}{sup +} is fixed to 2 in a self-consistent effective quantum field theory. Further, the mixing parameter of the photon and the neutral vector meson is equal to the ratio of electromagnetic and strong couplings, leading to the mass difference M{sub {rho}}{sub {sup 0}}-M{sub {rho}}{sub {sup {+-}}}{approx}1 MeV at tree order.

Djukanovic, Dalibor; Schindler, Matthias R.; Scherer, Stefan [Institut fuer Kernphysik, Johannes Gutenberg-Universitaet, 55099 Mainz (Germany); Gegelia, Jambul [Institut fuer Kernphysik, Johannes Gutenberg-Universitaet, 55099 Mainz (Germany); High Energy Physics Institute, Tbilisi State University, Tbilisi (Georgia)

2005-07-01T23:59:59.000Z

85

Study light scalar meson property from heavy meson decays  

SciTech Connect

In the SU(3) symmetry limit, the ratio R {identical_to} (B(D{sup +{yields}}f{sub 0}l{sup +{nu}})+B(D{sup +{yields}{sigma}}l{sup +{nu}})/B(D{sup +{yields}}a{sub 0}{sup 0}l{sup +{nu}})) is equal to 1 if the scalar mesons are q-barq states, while it is 3 if these mesons are tentraquark states. This ratio provides a model-independent way to distinguish the descriptions for light scalar mesons. It also applies to the B{sup -{yields}}Sl{sup -{nu}}-bar, and B{sup 0}-bar{yields}J/{psi}({eta}{sub c})S decays. The SU(3) symmetry breaking effect is found to be under control, which will not spoil our method. The branching fractions of the D{sup +{yields}}Sl{sup +{nu}}, B{sup -{yields}}Sl{sup -{nu}}-bar and B{sup 0}-bar{yields}J/{psi}({eta}{sub c})S decays roughly have the order 10{sup -4}, 10{sup -5} and 10{sup -6}, respectively. The B factory experiments and ongoing BEPC-II experiments are able to measure these channels and accordingly to provide the detailed information of the scalar meson inner structure.

Lu Caidian [Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049 (China); Wang Wei [Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Bari 70126 (Italy)

2010-08-05T23:59:59.000Z

86

Decoherence free Bd and Bs meson systems  

E-Print Network (OSTI)

We study the impact of decoherence on B meson systems with specific emphasis on Bs. For consistency we also study the Bd mesons based on the most recent data. We find that the Bd mesons are 34 sigma away from total decoherence, while the Bs mesons are seen to be upto 31sigma away from total decoherence. Thus, our results prove, with experimental verity, that neutral meson systems are free from decoherence effects. Therefore, this provides a very useful laboratory for testing the foundations of quantum mechanics.

Ashutosh Kumar Alok; Subhashish Banerjee

2013-04-15T23:59:59.000Z

87

B-meson distribution amplitudes  

E-Print Network (OSTI)

B-meson light-cone distribution amplitudes are discussed in these lectures in the framework of HQET. The evolution equation for the leading-twist distribution amplitude is derived in one-loop approximation. QCD sum rules for distribution amplitudes are discussed.

A. G. Grozin

2005-06-23T23:59:59.000Z

88

Distribution Amplitudes of Vector Mesons  

E-Print Network (OSTI)

Results are presented for the lowest moment of the distribution amplitude for the K-star vector meson. Both longitudinal and transverse moments are investigated. We use two flavours of O(a) improved Wilson fermions, together with a non-perturbative renormalisation of the matrix element.

V. M. Braun; D. Brömmel; M. Göckeler; R. Horsley; Y. Nakamura; H. Perlt; D. Pleiter; P. E. L. Rakow; A. Schäfer; G. Schierholz; A. Schiller; W. Schroers; T. Streuer; H. Stüben; J. M. Zanotti

2007-11-14T23:59:59.000Z

89

Distribution Amplitudes of Pseudoscalar Mesons  

E-Print Network (OSTI)

We present results for the first two moments of the distribution amplitudes of pseudoscalar mesons. Using two flavors of non-perturbatively improved clover fermions and non-perturbative renormalization of the matrix elements we perform both chiral and continuum extrapolations and compare with recent results from models and experiments.

V. M. Braun; M. Gockeler; R. Horsley; H. Perlt; D. Pleiter; P. E. L. Rakow; G. Schierholz; A. Schiller; W. Schroers; H. Stueben; J. M. Zanotti

2006-10-09T23:59:59.000Z

90

Compressed Baryonic Matter: from Nuclei to Pulsars  

E-Print Network (OSTI)

Our world is wonderful because of the negligible baryonic part although unknown dark matter and dark energy dominate the Universe. Those nuclei in the daily life are forbidden to fuse by compression due to the Coulomb repulse, nevertheless, it is usually unexpected in extraterrestrial extreme-environments: the gravity in a core of massive evolved star is so strong that all the other forces (including the Coulomb one) could be neglected. Compressed baryonic matter is then produced after supernova, manifesting itself as pulsar-like stars observed. The study of this compressed baryonic matter can not only be meaningful in fundamental physics (e.g., the elementary color interaction at low-energy scale, testing gravity theories, detecting nano-Hertz background gravitational waves), but has also profound implications in engineering applications (including time standard and navigation), and additionally, is focused by Chinese advanced telescopes, either terrestrial or in space. Historically, in 1930s, L. Landau speculated that dense matter at supra-nuclear density in stellar cores could be considered as gigantic nuclei (the prototype of standard model of neutron star), however, we address that the residual compact object of supernova could be of condensed matter of quark clusters. The idea that pulsars are quark-cluster stars was not ruled out during the last decade, and we are expecting to test further by future powerful facilities. (in Chinese)

Renxin Xu

2013-10-12T23:59:59.000Z

91

Light Baryons from 2+1 flavor DWF QCD  

E-Print Network (OSTI)

We present results from the RBC and UKQCD collaboration ensembles of 2+1 flavor DWF QCD for the light baryon spectrum.

C. M. Maynard; RBC; UKQCD collaborations

2010-01-28T23:59:59.000Z

92

Meson Spectroscopy at CLAS and CLAS12  

Science Conference Proceedings (OSTI)

We report on meson spectroscopy using the CLAS at Jefferson Lab. We study photo?production of exotic mesons and strangeonia on the largest data sample ever to be produced at photon energies of about 5 GeV. We also describe an experiment to continue meson spectroscopy at CLAS12 (CLAS energy upgrade) using electroproduction at very low Q 2 (“quasireal photons”) up to photon energies of 10 GeV.

Carlos Salgado; The CLAS Collaboration

2011-01-01T23:59:59.000Z

93

Search for doubly charmed baryons and study of charmed strange baryons at Belle  

E-Print Network (OSTI)

We report results of a study of doubly charmed baryons and charmed strange baryons. The analysis is performed using a 980 fb^-1 data sample collected with the Belle detector at the KEKB asymmetric-energy e^+e^- collider. We search for doubly charmed baryons Xi_cc^+(+) with the Lambda_c^+K^-pi^+(pi^+) and Xi_c^0pi^+(pi^+) final states. No significant signal is observed. We also search for two excited charmed strange baryons, Xi_c(3055)^+ and Xi_c(3123)^+ with the Sigma_c^++(2455)K^- and Sigma_c^++(2520)K^- final states. The Xi_c(3055)^+ signal is observed with a significance of 6.6 standard deviations including systematic uncertainty, while no signature of the Xi_c(3123)^+ is seen. We also study properties of the Xi_c(2645)^+ and measure a width of 2.6 +- 0.2 (stat) +- 0.4 (syst) MeV/c^2, which is the first significant determination.

Y. Kato; T. Iijima; I. Adachi; H. Aihara; D. M. Asner; T. Aushev; A. M. Bakich; A. Bala; Y. Ban; V. Bhardwaj; B. Bhuyan; A. Bobrov; G. Bonvicini; A. Bozek; M. Bra?ko; T. E. Browder; D. ?ervenkov; V. Chekelian; A. Chen; B. G. Cheon; K. Chilikin; R. Chistov; K. Cho; V. Chobanova; Y. Choi; D. Cinabro; J. Dalseno; M. Danilov; Z. Doležal; Z. Drásal; A. Drutskoy; D. Dutta; K. Dutta; S. Eidelman; H. Farhat; J. E. Fast; T. Ferber; V. Gaur; N. Gabyshev; S. Ganguly; A. Garmash; R. Gillard; Y. M. Goh; B. Golob; J. Haba; K. Hayasaka; H. Hayashii; X. H. He; Y. Horii; Y. Hoshi; W. -S. Hou; Y. B. Hsiung; K. Inami; A. Ishikawa; Y. Iwasaki; T. Iwashita; I. Jaegle; T. Julius; J. H. Kang; E. Kato; T. Kawasaki; C. Kiesling; D. Y. Kim; H. J. Kim; J. B. Kim; J. H. Kim; M. J. Kim; Y. J. Kim; J. Klucar; B. R. Ko; P. Kodyš; S. Korpar; P. Krokovny; T. Kuhr; A. Kuzmin; Y. -J. Kwon; S. -H. Lee; J. Li; Y. Li; L. Li Gioi; J. Libby; Y. Liu; D. Liventsev; D. Matvienko; K. Miyabayashi; H. Miyata; R. Mizuk; A. Moll; N. Muramatsu; R. Mussa; Y. Nagasaka; E. Nakano; M. Nakao; M. Nayak; E. Nedelkovska; C. Ng; M. Niiyama; N. K. Nisar; S. Nishida; O. Nitoh; S. Ogawa; S. Okuno; P. Pakhlov; G. Pakhlova; C. W. Park; H. Park; H. K. Park; T. K. Pedlar; T. Peng; R. Pestotnik; M. Petri?; L. E. Piilonen; M. Ritter; M. Röhrken; A. Rostomyan; H. Sahoo; T. Saito; Y. Sakai; S. Sandilya; L. Santelj; T. Sanuki; V. Savinov; O. Schneider; G. Schnell; C. Schwanda; D. Semmler; K. Senyo; O. Seon; M. Shapkin; C. P. Shen; T. -A. Shibata; J. -G. Shiu; B. Shwartz; A. Sibidanov; Y. -S. Sohn; A. Sokolov; E. Solovieva; S. Stani?; M. Stari?; M. Steder; M. Sumihama; T. Sumiyoshi; U. Tamponi; K. Tanida; G. Tatishvili; Y. Teramoto; M. Uchida; S. Uehara; T. Uglov; Y. Unno; S. Uno; C. Van Hulse; P. Vanhoefer; G. Varner; A. Vinokurova; V. Vorobyev; M. N. Wagner; C. H. Wang; M. -Z. Wang; P. Wang; M. Watanabe; Y. Watanabe; K. M. Williams; E. Won; Y. Yamashita; S. Yashchenko; Z. P. Zhang; V. Zhilich; V. Zhulanov; A. Zupanc

2013-12-04T23:59:59.000Z

94

Baryons and Low-Density Baryonic Matter in 1+1 Dimensional Large N_c QCD with Heavy Quarks  

E-Print Network (OSTI)

This paper studies baryons and baryonic matter in the combined large N_c and heavy quark mass limits of QCD in 1+1 dimension. In this non-relativistic limit, baryons are composed of N_c quarks that interact, at leading order in N_c, through a color Coulomb potential. Using variational techniques, very accurate calculations of single baryon masses and interaction energies of low-density baryon crystal are performed. These results are used to cross-check a general numerical approach applicable for arbitrary quark masses and baryon densities recently proposed by Bringoltz, which is based on a lattice in a finite box with periodic boundary conditions. The Bringoltz method differs from a previous approach of Salcedo, et al. in its treatment of a finite box effect - namely gauge configurations that wind around the box. One might expect these effects to be small for large enough boxes, in which the baryon density approaches zero to high accuracy at the edges. However, the effects of these windings appear to be quite large even in such boxes. The large mass infinite volume calculations performed here are consistent with the results of numerical calculations using the Bringoltz method. The calculation of the baryon crystal interaction energy requires the assumption that at low-densities the ground state is composed of individual baryons, each in a color-singlet state and orthogonal to each other. This assumption is plausible but ad hoc in that one can construct configurations in which the entire state is color-singlet but cannot be broken into individual color-singlet baryons. The interaction energy of low-density baryon crystals calculated with the assumption is consistent with numerical results based on Bringoltz's approach suggesting that the assumption is justified. This further supports a similar assumption that was made in 3+1 dimensions, where no alternative means of calculation exist.

Prabal Adhikari; Thomas D. Cohen; Arec Jamgochian; Nilay Kumar

2012-12-10T23:59:59.000Z

95

GlueX: Photoproduction of Hybrid Mesons  

SciTech Connect

The goal of the GlueX experiment is to provide critical data to help understand the soft gluonic field responsible for binding quarks in hadrons. Hybrid mesons, and in particular exotic hybrid mesons, provide the ideal laboratory for testing QCD in the confinement regime since these mesons explicitly manifest the gluonic degrees of freedom. Photoproduction is expected to be particularly effective in producing exotic hybrids but there is little data on the photoproduction of light mesons. GlueX will use the new 12-GeV electron beam to produce a 9-GeV beam of linearly polarized photons using the technique of coherent bremsstrahlung. A solenoid-based hermetic detector is under construction, which will be used to collect data on meson production and decays. These data will also be used to study the spectrum of conventional mesons, including the poorly understood excited vector mesons. This talk will describe the latest theoretical developments to help understand how the data of hybrid mesons can provide insights into the fundamental theory of strong interactions.

Elton Smith

2012-12-01T23:59:59.000Z

96

Quantum Operator Design for Lattice Baryon Spectroscopy  

Science Conference Proceedings (OSTI)

A previously-proposed method of constructing spatially-extended gauge-invariant three-quark operators for use in Monte Carlo lattice QCD calculations is tested, and a methodology for using these operators to extract the energies of a large number of baryon states is developed. This work is part of a long-term project undertaken by the Lattice Hadron Physics Collaboration to carry out a first-principles calculation of the low-lying spectrum of QCD. The operators are assemblages of smeared and gauge-covariantly-displaced quark fields having a definite flavor structure. The importance of using smeared fields is dramatically demonstrated. It is found that quark field smearing greatly reduces the couplings to the unwanted high-lying short-wavelength modes, while gauge field smearing drastically reduces the statistical noise in the extended operators.

Adam Lichtl

2007-09-06T23:59:59.000Z

97

QCD phase diagram at imaginary baryon and isospin chemical potentials  

E-Print Network (OSTI)

We explore the phase diagram of two-flavor QCD at imaginary values of baryon and isospin chemical potentials analyzing the thermodynamic potential of QCD analytically and that of the Polyakov-loop extended Nambu-Jona-Lasinio (PNJL) model numerically. QCD has no pion condensation at imaginary baryon and isospin chemical potentials, and therefore has discrete symmetries that are not present at real baryon and isospin chemical potentials. The PNJL model possesses all the discrete symmetries. The PNJL model can reproduce qualitatively lattice QCD data presented very lately.

Sakai, Yuji; Yahiro, Masanobu

2009-01-01T23:59:59.000Z

98

Fock exchange in meson theories of nuclei  

Science Conference Proceedings (OSTI)

The Fock exchange term in meson field theories of nuclear systems is shown to arise from a two-loop ground-state self-energy diagram. Evaluation of this diagram gives the relativistic or semirelativistic analog of the Fock exchange energy; it differs from the nucleon-nucleon Fock energy in including retardation effects. In finite meson-field theories of nuclear systems, the variational nature of the meson-field analog of the Hartree-Fock energy functional can be further elucidated. 4 refs.

Bolsterli, M.

1986-01-01T23:59:59.000Z

99

The phase diagram of nuclear and quark matter at high baryon density  

E-Print Network (OSTI)

We review theoretical approaches to explore the phase diagram of nuclear and quark matter at high baryon density. We first look over the basic properties of quantum chromodynamics (QCD) and address how to describe various states of QCD matter. In our discussions on nuclear matter we cover the relativistic mean-field model, the chiral perturbation theory, and the approximation based on the large-Nc limit where Nc is the number of colors. We then explain the liquid-gas phase transition and the inhomogeneous meson condensation in nuclear matter with emphasis put on the relevance to quark matter. We commence the next part focused on quark matter with the bootstrap model and the Hagedorn temperature. Then we turn to properties associated with chiral symmetry and exposit theoretical descriptions of the chiral phase transition. There emerge some quark-matter counterparts of phenomena seen in nuclear matter such as the liquid-gas phase transition and the inhomogeneous structure of the chiral condensate. The third regime that is being recognized recently is what is called quarkyonic matter, which has both aspects of nuclear and quark matter. We closely elucidate the basic idea of quarkyonic matter in the large-Nc limit and its physics implications. Finally, we discuss some experimental indications for the QCD phase diagram and close the review with outlooks.

Kenji Fukushima; Chihiro Sasaki

2013-01-27T23:59:59.000Z

100

Death of Stellar Baryonic Dark Matter Candidates  

E-Print Network (OSTI)

The nature of the dark matter in the Universe is one of the outstanding questions in astrophysics. In this talk, I address possible stellar baryonic contributions to the 50-90% of our Galaxy that is made of unknown dark matter. First I show that faint stars and brown dwarfs constitute only a few percent of the mass of the Galaxy. Next, I show that stellar remnants, including white dwarfs and neutron stars, are also insufficient in abundance to explain all the dark matter of the Galaxy. High energy gamma-rays observed in HEGRA data place the most robust constraints, $\\Omega_{WD} < 3 \\times 10^{-3} h^{-1}$, where $h$ is the Hubble constant in units of 100 km s$^{-1}$ Mpc$^{-1}$. Overproduction of chemical abundances (carbon, nitrogen, and helium) provide the most stringent constraints, $\\Omega_{WD} < 2 \\times 10^{-4} h^{-1}$. Comparison with recent updates of microlensing data are also made. According to the gamma-ray limit, all Massive Compact Halo Objects seen by the experiments (Machos) can be white dwarfs if one takes the extreme numbers; however, from chemical overproduction limits, NOT all Machos can be white dwarfs. Comments on recent observations of the infrared background and of white dwarfs are also made. In conclusion, a nonbaryonic component in the Halo seems to be required.

Katherine Freese; Brian Fields; David Graff

2000-07-28T23:59:59.000Z

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101

Light Vector Mesons in the Nuclear Medium  

E-Print Network (OSTI)

The light vector mesons ($\\rho$, $\\omega$, and $\\phi$) were produced in deuterium, carbon, titanium, and iron targets in a search for possible in-medium modifications to the properties of the $\\rho$ meson at normal nuclear densities and zero temperature. The vector mesons were detected with the CEBAF Large Acceptance Spectrometer (CLAS) via their decays to $e^{+}e^{-}$. The rare leptonic decay was chosen to reduce final-state interactions. A combinatorial background was subtracted from the invariant mass spectra using a well-established event-mixing technique. The $\\rho$ meson mass spectrum was extracted after the $\\omega$ and $\\phi$ signals were removed in a nearly model-independent way. Comparisons were made between the $\\rho$ mass spectra from the heavy targets ($A > 2$) with the mass spectrum extracted from the deuterium target. With respect to the $\\rho$-meson mass, we obtain a small shift compatible with zero. Also, we measure widths consistent with standard nuclear many-body effects such as collisional broadening and Fermi motion.

M. H. Wood; R. Nasseripour; D. P. Weygand; C. Djalali; C. Tur; U. Mosel; P. Muehlich; CLAS Collaboration

2008-03-04T23:59:59.000Z

102

Strange and charm meson masses from twisted mass lattice QCD  

E-Print Network (OSTI)

We present first results of a 2+1+1 flavor twisted mass lattice QCD computation of strange and charm meson masses. We focus on D and D_s mesons with spin J = 0,1 and parity P = -,+.

Martin Kalinowski; Marc Wagner

2012-12-03T23:59:59.000Z

103

Photoproduction of scalar mesons at medium energies  

SciTech Connect

In this work we will focus on photoproduction of mesons states a{sub 0}(980), f{sub 0}(1500) and f{sub 0}(1710). The f{sub 0}(1500) and f{sub 0}(1710) mesons will be considered in distinct mixing possibilities and assuming that a{sub 0}(980) is member of the ground-state nonet. The theoretical formalism is the Regge approach with reggeized {rho} and {omega} exchange. The differential and integrated total cross section are computed for the cases of the mesons a{sub 0}(980), f{sub 0}(1500) and f{sub 0}(1710) focusing the GlueX energy regime with photon energy E = 9 GeV.

Da Silva, M. L. [Instituto de Fisica e Matematica, Universidade Federal de Pelotas, Caixa Postal 354, CEP 96010-090, Pelotas, RS (Brazil); Machado, M. V. [High Energy Physics Phenomenology Group, GFPAE IF-UFRGS, Caixa Postal 15051, CEP 91501-970, Porto Alegre, RS (Brazil)

2013-03-25T23:59:59.000Z

104

Lattice test of 1/N[subscript c] baryon mass relations  

E-Print Network (OSTI)

1/N[subscript c] baryon mass relations are compared with lattice simulations of baryon masses using different values of the light-quark masses, and hence different values of SU(3) flavor-symmetry breaking. The lattice ...

Jenkins, Elizabeth E.

105

Meson Spectrum in Strong Magnetic Fields  

E-Print Network (OSTI)

We study the relativistic quark-antiquark system embedded in magnetic field. The Hamiltonian containing confinement, one gluon exchange and spin-spin interaction is derived. We analytically follow the evolution of the lowest meson states as a functions of MF strength. Calculating the one gluon exchange interaction energy and spin-spin contribution we have observed, that these corrections remain finite at large magnetic fields, preventing the vanishing of the total rho-meson mass at some B_crit, as previously thought. We display the rho masses as functions of magnetic field in comparison with recent lattice data.

M. A. Andreichikov; B. O. Kerbikov; V. D. Orlovsky; Yu. A. Simonov

2013-04-09T23:59:59.000Z

106

Observation of a new charmed strange meson  

Science Conference Proceedings (OSTI)

Using the CLEO II detector, we have obtained evidence for a new meson decaying to [ital D][sup 0][ital K][sup +]. Its mass is 2573.2[sub [minus]1.6][sup +1.7][plus minus]0.8[plus minus]0.5 MeV/[ital c][sup 2] and its width is 16[sub [minus]4][sup +5][plus minus]3 MeV/[ital c][sup 2]. Although we do not establish its spin and parity, the new meson is consistent with predictions for an [ital L]=1, [ital S]=1, [ital J][sup [ital P

Kubota, Y.; Lattery, M.; Nelson, J.K.; Patton, S.; Perticone, D.; Poling, R.; Savinov, V.; Schrenk, S.; Wang, R.; Alam, M.S.; Kim, I.J.; Nemati, B.; O'Neill, J.J.; Severini, H.; Sun, C.R.; Zoeller, M.M.; Crawford, G.; Daubenmier, C.M.; Fulton, R.; Fujino, D.; Gan, K.K.; Honscheid, K.; Kagan, H.; Kass, R.; Lee, J.; Malchow, R.; Morrow, F.; Skovpen, Y.; Sung, M.; White, C.; Butler, F.; Fu, X.; Kalbfleisch, G.; Ross, W.R.; Skubic, P.; Snow, J.; Wang, P.L.; Wood, M.; Brown, D.N.; Fast, J.; McIlwain, R.L.; Miao, T.; Miller, D.H.; Modesitt, M.; Payne, D.; Shibata, E.I.; Shipsey, I.P.J.; Wang, P.N.; Battle, M.; Ernst, J.; Kwon, Y.; Roberts, S.; Thorndike, E.H.; Wang, C.H.; Dominick, J.; Lambrecht, M.; Sanghera, S.; Shelkov, V.; Skwarnicki, T.; Stroynowski, R.; Volobouev, I.; Wei, G.; Zadorozhny, P.; Artuso, M.; Goldberg, M.; He, D.; Horwitz, N.; Kennett, R.; Mountain, R.; Moneti, G.C.; Muheim, F.; Mukhin, Y.; Playfer, S.; Rozen, Y.; Stone, S.; Thulasidas, M.; Vasseur, G.; Zhu, G.; Bartelt, J.; (CLEO Collaboration)

1994-03-28T23:59:59.000Z

107

Combining Quark and Link Smearing to Improve Extended Baryon Operators  

SciTech Connect

The effects of Gaussian quark-field smearing and analytic stout-link smearing on the correlations of gauge-invariant extended baryon operators are studied. Gaussian quark-field smearing substantially reduces contributions from the short wavelength modes of the theory, while stout-link smearing significantly reduces the noise from the stochastic evaluations. The use of gauge-link smearing is shown to be crucial for baryon operators constructed of covariantly-displaced quark fields. Preferred smearing parameters are determined for a lattice spacing a_s ~ 0.1 fm.

Adam Lichtl; Subhasish Basak; Robert Edwards; George T. Fleming; Urs M. Heller; Colin Morningstar; David Richards; Ikuro Sato; Stephen Wallace

2005-09-29T23:59:59.000Z

108

Type-II seesaw mass models and baryon asymmetry  

E-Print Network (OSTI)

We compute and also compare the contributions of canonical and noncanonical mass terms towards baryon asymmetry by considering type-II seesaw mass models of neutrinos: Degenerare(3 varieties), Normal hierarchical and Inverted hierarchical(2 varieties). We have shown that for particular choices of parameter '$\\gamma$'(the so-called discriminator) for different neutrino mass models, the baryon asymmetry is largely dominated by canonical term. Within such type-II seesaw scenario, we find normal hierarchical mass model as the most favourable choice of nature.

Amal Kr. Sarma; H. Zeen Devi; N. Nimai Singh

2006-12-12T23:59:59.000Z

109

Photoproduction of Baryons Decaying into N pi and N eta  

E-Print Network (OSTI)

A combined analysis of photoproduction data on \\gamma p to \\pi N, eta N was performed including the data on K Lambda and K Sigma. The data are interpreted in an isobar model with s--channel baryon resonances and pi, rho,(omega), K, and K^* exchange in the t--channel. Three baryon resonances have a substantial coupling to eta N, the well known N(1535)S_{11}, N(1720)P_{13}, and N(2070)D_{15}. The inclusion of data with open strangeness reveals the presence of further new resonances, N(1840)P_{11}, N(1875)D_{13} and N(2170)D_{13}.

A. V. Anisovich; A. Sarantsev; O. Bartholomy; E. Klempt; V. A. Nikonov; U. Thoma

2005-06-06T23:59:59.000Z

110

Light Baryon Spectroscopy using the CLAS Spectrometer at Jefferson Laboratory  

Science Conference Proceedings (OSTI)

Baryons are complex systems of confined quarks and gluons and exhibit the characteristic spectra of excited states. The systematics of the baryon excitation spectrum is important to our understanding of the effective degrees of freedom underlying nucleon matter. High-energy electrons and photons are a remarkably clean probe of hadronic matter, providing a microscope for examining the nucleon and the strong nuclear force. Current experimental efforts with the CLAS spectrometer at Jefferson Laboratory utilize highly-polarized frozen-spin targets in combination with polarized photon beams. The status of the recent double-polarization experiments and some preliminary results are discussed in this contribution.

Volker Crede

2011-12-01T23:59:59.000Z

111

Chiral Corrections to Baryon Masses Calculated within Lattice QCD  

E-Print Network (OSTI)

Consideration of the analytic properties of pion-induced baryon self energies leads to new functional forms for the extrapolation of light baryon masses. These functional forms reproduce the leading non-analytic behavior of chiral perturbation theory, the correct non-analytic behavior at the $N \\pi$ threshold and the appropriate heavy-quark limit. They involve only three unknown parameters, which may be obtained by fitting lattice QCD data. Recent dynamical fermion results from CP-PACS and UKQCD are extrapolated using these new functional forms. We also use these functions to probe the limit of applicability of chiral perturbation theory.

Anthony W. Thomas; Derek B. Leinweber; Kazuo Tsushima; Stewart V. Wright

1999-09-17T23:59:59.000Z

112

Issues in Light Meson Spectroscopy: The Case for Meson Spectroscopy at Cebaf  

E-Print Network (OSTI)

I review some outstanding issues in meson spectroscopy. The most important qualitative issue is whether hadrons with explicit gluonic degrees of freedom exist. To answer this question requires a much better understanding of conventional $q\\bar{q}$ mesons. I therefore begin by examining the status of conventional meson spectroscopy and how the situation can be improved. The expected properties of gluonic excitations are discussed with particular emphasis on hybrids to give guidance to experimental searches. Multiquark systems are commented upon as they are likely to be important in the mass region under study and will have to be understood better. In the final section I discuss the opportunities that CEBAF can offer for the study of meson spectroscopy.

Stephen Godfrey

1994-06-10T23:59:59.000Z

113

{sigma} meson exchange effect on non-mesonic hypernuclear weak decay observables  

Science Conference Proceedings (OSTI)

We analyze the influence of {sigma} meson exchange on the main non-mesonic hypernuclear weak decay observables: Total rate {gamma}{sub NM}, neutron-to-proton branching ratio {gamma}{sub n/p}, and proton asymmetry parameter a{sub {lambda}}. The {sigma} meson exchange is added to the standard strangeness-changing weak {lambda}N{yields}NN transition potential, which includes the exchange of the complete pseudoscalar and vector mesons octet ({pi},{eta},K,{rho},{omega},K{sup *}). Using a shell model formalism, the {sigma} meson weak coupling constants are adjusted to reproduce the recent {gamma}{sub NM} and {gamma}{sub n/p} experimental data for {sub {lambda}}{sup 5}He. Numerical results for the remaining observables of {sub {lambda}}{sup 5}He and all the observables of {sub {lambda}}{sup 12}C decays are presented. They clearly show that the addition of the {sigma} meson improves the agreement with the data. However, its effect it is not enough to reproduce well the a{sub {lambda}} values, which means that other improvements of the model must be explored to explain the puzzle posed by the experiments.

Barbero, C.; Mariano, A. [Departamento de Fisica, Facultad de Ciencias Exactas, Universidad Nacional de La Plata, C.C. 67, 1900 La Plata (Argentina)

2006-02-15T23:59:59.000Z

114

Particle Data Group - 2011 Summary Tables  

NLE Websites -- All DOE Office Websites (Extended Search)

Gauge and Higgs Bosons (gamma, g, W, Z, ...) Leptons (e, mu, tau, ... neutrinos ...) Quarks (u, d, s, c, b, t, b', t', Free) Mesons contents Baryons contents Searches (Monopoles,...

115

Particle Data Group - 2010 Summary Tables  

NLE Websites -- All DOE Office Websites (Extended Search)

Gauge and Higgs Bosons (gamma, g, W, Z, ...) Leptons (e, mu, tau, ... neutrinos ...) Quarks (u, d, s, c, b, t, b', t', Free) Mesons errata contents Baryons errata contents...

116

Particle Data Group - 2009 Summary Tables  

NLE Websites -- All DOE Office Websites (Extended Search)

Gauge and Higgs Bosons (gamma, g, W, Z, ...) Leptons (e, mu, tau, ... neutrinos ...) Quarks (u, d, s, c, b, t, b', t', Free) Mesons contents Baryons contents Searches (Monopoles,...

117

Particle Data Group - 2008 Summary Tables  

NLE Websites -- All DOE Office Websites (Extended Search)

Gauge and Higgs Bosons (gamma, g, W, Z, ...) Leptons (e, mu, tau, ... neutrinos ...) Quarks (u, d, s, c, b, t, b', t', Free) Mesons contents Baryons contents Searches (Monopoles,...

118

BPS Skyrme model and baryons at large N{sub c}  

Science Conference Proceedings (OSTI)

Within the class of field theories with the field content of the Skyrme model, one submodel can be found which consists of the square of the baryon current and a potential term only. For this submodel, a Bogomol'nyi-Prasad-Sommerfield bound exists, and the static soliton solutions saturate this bound. Further, already on the classical level, this Bogomol'nyi-Prasad-Sommerfield Skyrme model reproduces some features of the liquid drop model of nuclei. Here, we investigate the model in more detail and, besides, we perform the rigid rotor quantization of the simplest Skyrmion (the nucleon). In addition, we discuss indications that the viability of the model as a low-energy effective field theory for QCD is further improved in the limit of a large number of colors N{sub c}.

Adam, C.; Sanchez-Guillen, J. [Departamento de Fisica de Particulas, Universidad de Santiago, and Instituto Galego de Fisica de Altas Enerxias (IGFAE) E-15782 Santiago de Compostela (Spain); Wereszczynski, A. [Institute of Physics, Jagiellonian University, Reymonta 4, Krakow (Poland)

2010-10-15T23:59:59.000Z

119

{phi}-Meson Photoproduction with Linearly Polarized Photons at Threshold Energies  

SciTech Connect

The observables provided by linearly-polarized photons are of interest in delineating the contributions of the various hadronic processes giving rise to vector meson photoproduction. In particular, we describe how {phi}-meson production affords an incisive tool for exploring the nature of the parity exchange at threshold energies, the strangeness content of proton, as well as extracting signatures for the violation of Okubo-Zweig-Iizuka observation (OZI rule). Our goal is to study the {gamma}-vectorp{yields}{phi}p reaction, with {phi}{yields}K{sup +}K{sup -}, in the photon energy range of 1.7 to 2.1 GeV by using the Coherent Linear Bremsstrahlung Facility in Hall B of Jefferson Laboratory, Newport News, VA. The data were collected during the g8b run in the summer of 2005.

Salamanca, Julian; Cole, Philip L. [Idaho State University, Dept. of Physics, Pocatello, Idaho 83209 (United States)

2007-10-26T23:59:59.000Z

120

Nuclear modification factors of phi mesons in d+Au, Cu+Cu and Au+Au collisions at sqrt(S_NN)=200 GeV  

E-Print Network (OSTI)

The PHENIX experiment at the Relativistic Heavy Ion Collider (RHIC) has performed systematic measurements of phi meson production in the K+K- decay channel at midrapidity in p+p, d+Au, Cu+Cu and Au+Au collisions at sqrt(S_NN)=200 GeV. Results are presented on the phi invariant yield and the nuclear modification factor R_AA for Au+Au and Cu+Cu, and R_dA for d+Au collisions, studied as a function of transverse momentum (1phi exhibits a suppression relative to expectations from binary scaled p+p results. The amount of suppression is smaller than that of the neutral pion and the eta meson in the intermediate p_T range (2--5 GeV/c); whereas at higher p_T the phi, pi^0, and eta show similar suppression. The baryon (protons and anti-protons) excess observed in central Au+Au collisions at intermediate p_T is not observed for the phi meson despite the similar mass of the proton and the phi. This suggests that the excess is lin...

Adare, A; Aidala, C; Ajitanand, N N; Akiba, Y; Al-Bataineh, H; Alexander, J; Al-Jamel, A; Angerami, A; Aoki, K; Aphecetche, L; Aramaki, Y; Armendariz, R; Aronson, S H; Asai, J; Atomssa, E T; Averbeck, R; Awes, T C; Azmoun, B; Babintsev, V; Bai, M; Baksay, G; Baksay, L; Baldisseri, A; Barish, K N; Barnes, P D; Bassalleck, B; Basye, A T; Bathe, S; Batsouli, S; Baublis, V; Bauer, F; Baumann, C; Bazilevsky, A; Belikov, S; Belmont, R; Bennett, R; Berdnikov, A; Berdnikov, Y; Bhom, J H; Bickley, A A; Bjorndal, M T; Blau, D S; Boissevain, J G; Bok, J S; Borel, H; Borggren, N; Boyle, K; Brooks, M L; Brown, D S; Bucher, D; Buesching, H; Bumazhnov, V; Bunce, G; Burward-Hoy, J M; Butsyk, S; Campbell, S; Caringi, A; Cassano, N; Chai, J -S; Chang, B S; Charvet, J -L; Chen, C -H; Chernichenko, S; Chiba, J; Chi, C Y; Chiu, M; Choi, I J; Choi, J B; Choudhury, R K; Christiansen, P; Chujo, T; Chung, P; Churyn, A; Chvala, O; Cianciolo, V; Citron, Z; Cleven, C R; Cobigo, Y; Cole, B A; Comets, M P; del Valle, Z Conesa; Connors, M; Constantin, P; Csanad, M; Csorgo, T; Dahms, T; Dairaku, S; Danchev, I; Das, K; Datta, A; David, G; Dayananda, M K; Deaton, M B; Dehmelt, K; Delagrange, H; Denisov, A; d'Enterria, D; Deshpande, A; Desmond, E J; Dharmawardane, K V; Dietzsch, O; Dion, A; Donadelli, M; Orazio, L D; Drachenberg, J L; Drapier, O; Drees, A; Drees, K A; Dubey, A K; Durham, J M; Durum, A; Dutta, D; Dzhordzhadze, V; Edwards, S; Efremenko, Y V; Egdemir, J; Ellinghaus, F; Emam, W S; Engelmore, T; Enokizono, A; En'yo, H; Espagnon, B; Esumi, S; Eyser, K O; Fadem, B; Fields, D E; Finger, M; Finger, M; Fleuret, F; Fokin, S L; Forestier, B; Fraenkel, Z; Frantz, J E; Franz, A; Frawley, A D; Fujiwara, K; Fukao, Y; Fung, S -Y; Fusayasu, T; Gadrat, S; Garishvili, I; Gastineau, F; Germain, M; Glenn, A; Gong, H; Gonin, M; Gosset, J; Goto, Y; de Cassagnac, R Granier; Grau, N; Greene, S V; Grim, G; Perdekamp, M Grosse; Gunji, T; Gustafsson, H -A; Hachiya, T; Henni, A Hadj; Haegemann, C; Haggerty, J S; Hagiwara, M N; Hahn, K I; Hamagaki, H; Hamblen, J; Hanks, J; Han, R; Harada, H; Hartouni, E P; Haruna, K; Harvey, M; Haslum, E; Hasuko, K; Hayano, R; Heffner, M; Hemmick, T K; Hester, T; Heuser, J M; He, X; Hiejima, H; Hill, J C; Hobbs, R; Hohlmann, M; Holmes, M; Holzmann, W; Homma, K; Hong, B; Horaguchi, T; Hornback, D; Huang, S; Hur, M G; Ichihara, T; Ichimiya, R; Iinuma, H; Ikeda, Y; Imai, K; Inaba, M; Inoue, Y; Isenhower, D; Isenhower, L; Ishihara, M; Isobe, T; Issah, M; Isupov, A; Ivanischev, D; Iwanaga, Y; Jacak, B V; Jia, J; Jiang, X; Jin, J; Jinnouchi, O; Johnson, B M; Jones, T; Joo, K S; Jouan, D; Jumper, D S; Kajihara, F; Kametani, S; Kamihara, N; Kamin, J; Kaneta, M; Kang, J H; Kanou, H; Kapustinsky, J; Karatsu, K; Kasai, M; Kawagishi, T; Kawall, D; Kawashima, M; Kazantsev, A V; Kelly, S; Kempel, T; Khanzadeev, A; Kijima, K M; Kikuchi, J; Kim, A; Kim, B I; Kim, D H; Kim, D J; Kim, E J; Kim, E; Kim, Y -J; Kim, Y -S; Kinney, E; Kiss, A; Kistenev, E; Kiyomichi, A; Klay, J; Klein-Boesing, C; Kochenda, L; Kochetkov, V; Komkov, B; Konno, M; Koster, J; Kotchetkov, D; Kotov, D; Kozlov, A; Kral, A; Kravitz, A; Kroon, P J; Kubart, J; Kunde, G J; Kurihara, N; Kurita, K; Kurosawa, M; Kweon, M J; Kwon, Y; Kyle, G S; Lacey, R; Lai, Y S; Lajoie, J G; Lebedev, A; Le Bornec, Y; Leckey, S; Lee, D M; Lee, J; Lee, K B; Lee, K S; Lee, M K; Lee, T; Leitch, M J; Leite, M A L; Lenzi, B; Lichtenwalner, P; Liebing, P; Lim, H; Levy, L A Linden; Liska, T; Litvinenko, A; Liu, H; Liu, M X; Li, X; Li, X H; Love, B; Lynch, D; Maguire, C F; Makdisi, Y I; Malakhov, A; Malik, M D; Manko, V I; Mannel, E; Mao, Y; Masek, L; Masui, H; Matathias, F; McCain, M C; McCumber, M; McGaughey, P L; Means, N; Meredith, B; Miake, Y; Mibe, T; Mignerey, A C; Mikes, P; Miki, K; Miller, T E; Milov, A; Mioduszewski, S; Mishra, G C; Mishra, M; Mitchell, J T; Mitrovski, M; Mohanty, A K; Moon, H J; Morino, Y; Morreale, A; Morrison, D P; Moss, J M; Moukhanova, T V; Mukhopadhyay, D; Murakami, T; Murata, J; Nagamiya, S; Nagata, Y; Nagle, J L; Naglis, M; Nagy, M I; Nakagawa, I; Nakamiya, Y; Nakamura, K R; Nakamura, T; Nakano, K; Nam, S; Newby, J; Nguyen, M; Nihashi, M; Norman, B E; Nouicer, R; Nyanin, A S; Nystrand, J; Oakley, C; O'Brien, E; Oda, S X; Ogilvie, C A; Ohnishi, H; Ojha, I D; Okada, K; Oka, M; Omiwade, O O; Onuki, Y; Oskarsson, A; Otterlund, I; Ouchida, M; Ozawa, K; Pak, R; Pal, D; Palounek, A P T; Pantuev, V; Papavassiliou, V; Park, I H; Park, J; Park, S K; Park, W J; Pate, S F; Pei, H; Peng, J -C; Pereira, H; Peresedov, V; Peressounko, D Yu; Petti, R; Pinkenburg, C; Pisani, R P; Proissl, M; Purschke, M L; Purwar, A K; Qu, H; Rak, J; Rakotozafindrabe, A; Ravinovich, I; Read, K F; Rembeczki, S; Reuter, M; Reygers, K; Riabov, V; Riabov, Y; Richardson, E; Roach, D; Roche, G; Rolnick, S D; Romana, A; Rosati, M; Rosen, C A; Rosendahl, S S E; Rosnet, P; Rukoyatkin, P; Ruzicka, P; Rykov, V L

2010-01-01T23:59:59.000Z

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121

Rare B Meson Decays at the Tevatron  

SciTech Connect

Rare B meson decays are an excellent probe for beyond the Standard Model physics. Two very sensitive processes are the b {yields} s{mu}{sup +}{mu}{sup -} and B{sub s,d}{sup 0} {yields} {mu}{sup +}{mu}{sup -} decays. We report recent results at a center of mass energy of {radical}s = 1.96 TeV from CDF II using 7 fb{sup -1} at the Fermilab Tevatron Collider.

Hopkins, Walter

2012-01-01T23:59:59.000Z

122

Interaction of eta mesons with nuclei  

E-Print Network (OSTI)

Back in the mid eighties, a new branch of investigation which was related to the interaction of eta mesons with nuclei came into existence. It started with the theoretical prediction of possible exotic states of eta mesons and nuclei bound by the strong interaction and later developed into an extensive experimental program to search for such unstable states as well as understand the underlying interaction via eta meson producing reactions. The vast literature of experimental as well as theoretical works which studied various aspects of eta producing reactions such as the $\\pi ^+$ $n$ $\\to \\eta p$, $p d \\to ^3$He $\\eta$, $p \\,^6$Li $\\to ^7$Be $\\eta$ and $\\gamma ^3$He $\\to \\eta$ X, to name a few, had but one objective in mind: to understand the eta - nucleon ($\\eta N$) and hence the $\\eta$-nucleus interaction which could explain the production data and confirm the existence of some $\\eta$-mesic nuclei. In spite of these efforts, there remain uncertainties in the knowledge of the $\\eta N$ and hence the $\\eta$-nucleus interaction. The present review is hence an attempt to bind together the findings in these works and draw some global and specific conclusions which can be useful for future explorations.

N. G. Kelkar; K. P. Khemchandani; N. J. Upadhyay; B. K. Jain

2013-06-12T23:59:59.000Z

123

Observation of the doubly strange b-Baryon Omega(b)-  

SciTech Connect

This thesis reports the first experimental evidence of the doubly strange b-baryon {Omega}{sub b}{sup -} (ssb) following the decay channel {Omega}{sub b}{sup -} {yields} J/{psi}(1S) {mu}{sup +}{mu}{sup -} {Omega}{sup -} {Lambda} K{sup -} p {pi}{sup -} in p{bar p} collisions at {radical}s = 1.96 Tev. Using approximately 1.3 fb{sup -1} of data collected with the D0 detector at the Fermilab Tevatron Collider, they observe 17.8 {+-} 4.9(stat) {+-} 0.8(syst) {Omega}{sub b}{sup -} signal events at 6.165 {+-} 0.010(stat) {+-} 0.013(syst) GeV/c{sup 2} with a corresponding significance of 5.4 {sigma}, meaning that the probability of the signal coming from a fluctuation in the background is 6.7 x 10{sup -8}. The theoretical model we have to describe what we believe are the building blocks of nature and the interactions between them, is known as Standard Model. The Standard Model is the combination of Electroweak Theory and Quantum Chromodynamics into a single core in the attempt to include all interactions of subatomic particles except those due to gravity in a simple framework. This model has proved highly accurate in predicting certain interactions, but it does not explain all aspects of subatomic particles. For example, it cannot say how many particles there should be or what their masses are. The search goes on for a more complete theory, and in particular an unified field theory describing the strong, weak, and electromagnetic forces. Twelve elementary particles are known in the Standard Model: the Fermions. They have spin -1/2 and obey the Pauli Exclusion Principle. Fermions are divided into six Quarks: up u, down d, charm c, strange s, top t and, bottom b; and six Leptons: electron e, muon {mu}, tau {tau}, electron neutrino {nu}{sub e}, muon neutrino {nu}{sub {mu}} and, tau neutrino {nu}{sub {tau}}. Quarks interact via the strong force because they carry color charge, electromagnetically because of their electric charge and via the weak nuclear interaction because of the weak isospin. Quarks form color-neutral composite particles known as Hadrons which are divided in Mesons, containing a quark and an antiquark and Baryons, made up three quarks. Leptons have no color charge and can not interact via the strong force. Only three of them have electric charge, hence interact electromagnetically. The motion of non-electrically charged leptons, the neutrinos, is influenced only by the weak nuclear interaction. Every fermion have an associated antiparticle. For quarks, the antiparticle carry opposite electric charge, color charge and baryon number. For leptons, the antiparticle carry opposite electric charge and lepton number. Fermions are suitably grouped together considering their properties and three generations of them are defined. A higher generation fermion have greater mass than those in lower generations. Charged members of the first generation do not decay and form the ultimate building blocks for all the baryonic matter we know about. Charged members of higher generations have very short half lives and are found normally in high-energy environments. Non-electrically charged fermions do not decay and rarely interact with baryonic matter. The way particles interact and influence each other in the Standard Model is result from matter particles exchanging other particles, known as Force Mediating Particles. They are believed to be the reason of the existence of the forces and interactions between particles observed in the laboratory and the universe. Force mediating particles have spin 1, i.e., they are Bosons, and do not follow the Pauli Exclusion Principle. The types of force mediating particles are: the photon {gamma}, three gauge bosons W{sup {+-}} and Z and, eight gluons g. Photons have no mass, the theory of Quantum Electrodynamics describe them very well and are responsible for mediation of the electromagnetic force between electrically charged particles. Gauge bosons are massive, being Z heavier than W{sup {+-}}. They are responsible for the mediation of the weak interactions between particles of different flavors but

Hernandez Orduna, de Jesus, Jose; /CINVESTAV, IPN

2011-02-01T23:59:59.000Z

124

Recent developments in the search for baryonic dark matter  

E-Print Network (OSTI)

Cosmological nucleosynthesis calculations imply that many of the baryons in the Universe must be dark. We discuss the likelihood that some of these dark baryons may reside in galaxies as Massive Compact Halo Objects (MACHOs), the remnants of a first generation of pregalactic or protogalactic stars. Various candidates have been proposed for such remnants and we review the many types of observations which can be used to detect or exclude them. Claims to have found positive evidence for some of the candidates have generally turned out to be spurious or questionable, so the status of the MACHO scenario remains controversial. However, it would be premature to reject MACHOs altogether and further observations are likely to resolve the issue soon.

B. J. Carr

2001-02-22T23:59:59.000Z

125

Study of Chemical Equilibration of a Baryon Rich QGP  

E-Print Network (OSTI)

Parton equilibration studies for thermally equilibrated but chemically non-equilibrated quark-gluon-plasma (QGP), likely to be formed at the relativistic colliders at BNL and CERN is presented.Parton equilibration is studied enforcing baryon number conservation. Process like quark-flavor interchanging is also taken into consideration.The degree of equilibration is studied comparatively for the various reactions/ constraints that are being considered.

Abhijit Sen

2008-02-26T23:59:59.000Z

126

Bosonic and Baryonic String Theory in Quantum Chromodynamics  

Science Conference Proceedings (OSTI)

Bosonic string formation in gauge theories is reviewed with particular attention to the confining flux in lattice QCD and its effective string theory description. Recent results on the Casimir energy of the ground state and the string excitation spectrum are analyzed in the Dirichlet string limit of large separation between static sources. The closed string-soliton (torelon) with electric flux winding around a compact dimension is discussed and a new bound state tower spectrum at baryon string junctions is presented.

Kuti, Julius [Department of Physics, University of California, San Diego, La Jolla, California 92093 (United States)

2007-02-27T23:59:59.000Z

127

A BARYONIC SOLUTION TO THE MISSING SATELLITES PROBLEM  

SciTech Connect

It has been demonstrated that the inclusion of baryonic physics can alter the dark matter densities in the centers of low-mass galaxies, making the central dark matter slope more shallow than predicted in pure cold dark matter simulations. This flattening of the dark matter profile can occur in the most luminous subhalos around Milky Way mass galaxies. Zolotov et al. have suggested a correction to be applied to the central masses of dark matter-only satellites in order to mimic the affect of (1) the flattening of the dark matter cusp due to supernova feedback in luminous satellites and (2) enhanced tidal stripping due to the presence of a baryonic disk. In this paper, we apply this correction to the z = 0 subhalo masses from the high resolution, dark matter-only Via Lactea II (VL2) simulation, and find that the number of massive subhalos is dramatically reduced. After adopting a stellar mass to halo mass relationship for the VL2 halos, and identifying subhalos that are (1) likely to be destroyed by stripping and (2) likely to have star formation suppressed by photo-heating, we find that the number of massive, luminous satellites around a Milky Way mass galaxy is in agreement with the number of observed satellites around the Milky Way or M31. We conclude that baryonic processes have the potential to solve the missing satellites problem.

Brooks, Alyson M. [Department of Astronomy, University of Wisconsin-Madison, 475 N. Charter Street, Madison, WI 53706 (United States)] [Department of Astronomy, University of Wisconsin-Madison, 475 N. Charter Street, Madison, WI 53706 (United States); Kuhlen, Michael [Theoretical Astrophysics Center, University of California, Berkeley, CA 94720 (United States)] [Theoretical Astrophysics Center, University of California, Berkeley, CA 94720 (United States); Zolotov, Adi [Racah Institute of Physics, The Hebrew University, Jerusalem 91904 (Israel)] [Racah Institute of Physics, The Hebrew University, Jerusalem 91904 (Israel); Hooper, Dan, E-mail: abrooks@astro.wisc.edu, E-mail: mqk@astro.berkeley.edu, E-mail: zolotov@phys.huji.ac.il, E-mail: dhooper@fnal.gov [Theoretical Astrophysics, Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL 60510 (United States)] [Theoretical Astrophysics, Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL 60510 (United States)

2013-03-01T23:59:59.000Z

128

Dissipative hydrodynamic evolution of hot quark matter at finite baryon density  

E-Print Network (OSTI)

High-energy heavy ion collider experiments at RHIC and LHC have revealed that relativistic hydrodynamic models describe the hot and dense quark matter quantitatively. In this study, I develop a novel dissipative hydrodynamic model at finite baryon density to investigate the net baryon rapidity distribution. The results show that the distribution is widened in hydrodynamic evolution, which implies that the transparency of the collisions is effectively enhanced. This suggests that the kinetic energy loss for medium production at the initial stage could be larger. Furthermore, the net baryon distribution is found sensitive to baryon diffusion, implying that dissipative hydrodynamic modeling would be important for understanding the hot medium.

Monnai, Akihiko

2013-01-01T23:59:59.000Z

129

Static-light meson masses from twisted mass lattice QCD  

E-Print Network (OSTI)

We compute the static-light meson spectrum using two-flavor Wilson twisted mass lattice QCD. We have considered five different values for the light quark mass corresponding to 300 MeV < m_PS < 600 MeV. We have extrapolated our results, to make predictions regarding the spectrum of B and B_s mesons.

ETM Collaboration; Karl Jansen; Chris Michael; Andrea Shindler; Marc Wagner

2008-08-15T23:59:59.000Z

130

MESON CORRELATION FUNCTIONS AT HIGH TEMPERATURES.  

Science Conference Proceedings (OSTI)

We present preliminary results for the correlation- and spectral functions of different meson channels on the lattice. The main focus lies on gaining control over cut-off as well as on the finite-volume effects. Extrapolations of screening masses above the deconfining temperature are guided by the result of the free (T = {infinity}) case on the lattice and in the continuum. We study the quenched non-perturbatively improved Wilson-clover fermion as well as the hypercube fermion action which might show less cut-off effects.

WISSEL, S.; DATTA, S.; KARSCH, F.; LAERMANN, E.; SHCHEREDIN, S.

2005-07-25T23:59:59.000Z

131

Light Meson Spectroscopy with the Kloe Experiment  

E-Print Network (OSTI)

We describe the status of the analyses in progress on light meson spectroscopy in the KLOE experiment. We present the analyses of phi decays into f0(980)gamma and a0(980)gamma, the Dalitz plot analysis of the eta to pie+ pie- pie0 decay, the branching ratio measurement of eta to pie0 gamma gamma, the upper limits on Br(eta to 3 gamma) and Br(eta to pie^+ pie^-), the measurement of the ratio Br(phi to eta' gamma)/Br(phi to eta gamma) and phi leptonic width measurements.

The KLOE collaboration; B. Di Micco

2004-10-25T23:59:59.000Z

132

Dark matter growth and baryon bias in an accelerating universe  

E-Print Network (OSTI)

We investigate the exact analytic solutions for the growths of the dark matter and the baryon in sub-horizon scale. The growth of the dark matter $\\delta_{\\DM}$ is related to that of the halos. Thus, the exact solution for the growth of the dark matter is important to obtain the proper properties of dark matter halos. However, the dark energy model dependence of $\\delta_{\\DM}$ is confused with the $\\delta_{\\DM}$ dependence on $\\Omega_{m}^{0}$. Thus, the careful investigation is necessary for the $\\delta_{\\DM}$ dependence on dark energy models. We also obtain the exact solution of the growth of the baryon $\\delta_{\\B}$ which can be used to obtain the baryon bias factor $b(a)$. This might be able to be observed in intracluster gas or in Lyman-$\\alpha$ clouds. However, $b(a)$ is quite model independent. Recently, we obtained the exact analytic solution for the growing mode solution of the matter linear density perturbation $\\delta$ on sub-horizon scale for general dark energy model \\cite{SK}. This solution is not same as the well known approximate analytic solution \\cite{Waga}. The exact analytic solution shows the same evolution behavior of the growth factor obtained numerically. However, the exact solution is simple and useful for the extension to other models including modified gravity theories. Furthermore, it guides to the fact that the growth index parameter depends on both models $\\omega_{\\de}$ and $\\Omega_{m}^{0}$ and thus we need to be careful for applying the fitting formulae to the general models \\cite{WS}. The exact analytic solutions for the growth factor will provide the more accurate tools for the weak lensing, the number density of clusters, their mass and etc.

Seokcheon Lee

2009-06-17T23:59:59.000Z

133

Group theoretical construction of extended baryon operators in lattice QCD  

SciTech Connect

The design and implementation of large sets of spatially-extended, gauge-invariant operators for use in determining the spectrum of baryons in lattice QCD computations are described. Group theoretical projections onto the irreducible representations of the symmetry group of a cubic spatial lattice are used in all isospin channels. The operators are constructed to maximize overlaps with the low-lying states of interest, while minimizing the number of sources needed in computing the required quark propagators. Issues related to the identification of the spin quantum numbers of the states in the continuum limit are addressed.

Subhasish Basak; Robert Edwards; George Fleming; Urs Heller; Colin Morningstar; David Richards; Ikuro Sato; Stephen Wallace

2005-06-01T23:59:59.000Z

134

Measurement of $\\psi(2S)$ decays to baryon pairs  

E-Print Network (OSTI)

A sample of 3.95M $\\psi(2S)$ decays registered in the BES detector are used to study final states containing pairs of octet and decuplet baryons. We report branching fractions for $\\psi(2S)\\to p\\bar{p}$, $\\Lambda\\bar{\\Lambda}$, $\\Sigma^0\\bar{\\Sigma}{}^0$, $\\Xi^-\\bar{\\Xi}{}^+$, $\\Delta^{++}\\bar{\\Delta}{}^{--}$, $\\Sigma^+(1385)\\bar{\\Sigma}{}^-(1385 )$, $\\Xi^0(1530)\\bar{\\Xi}{}^0(1530)$, and $\\Omega^-\\bar{\\Omega}{}^+$. These results are compared to expectations based on the SU(3)-flavor symmetry, factorization, and perturbative QCD.

Bai, J Z; Bian, J G; Blum, I K; Chen, A D; Chen, G P; Chen, H F; Chen, H S; Chen, J; Chen Jia Chao; Chen, X D; Chen, Y; Chen, Y B; Cheng Bao Sen; Choi, J B; Cui, X Z; Ding, H L; Dong, L Y; Du, Z Z; Dunwoodie, W M; Gao, C S; Gao, M L; Gao, S Q; Gratton, P; Gu, J H; Gu, S D; Gu, W X; Guo, Y N; Guo, Z J; Han, S W; Han, Y; Harris, F A; He, J; He, J T; He, K L; He, M; Heng, Y K; Hitlin, D G; Hu, G Y; Hu, H M; Hu, J L; Hu, Q H; Hu, T; Huang, G S; Huang, X P; Huang, Y Z; Izen, J M; Jiang, C H; Jin, Y; Jones, B D; Ju, X; Kang, J S; Ke, Z J; Kelsey, M H; Kim, B K; Kim, H J; Kim, S K; Kim, T Y; Kong, D; Lai, Y F; Lang, P F; Lankford, A J; Li, C G; Li, D; Li, H B; Li, J; Li, J C; Li, P Q; Li, W; Li, W G; Li, X H; Li Xiao Nan; Li Xue Qian; Li Zhong Chao; Liu, B; Liu, F; Liu Feng; Liu, H M; Liu, J; Liu, J P; Liu, R G; Liu, Y; Liu, Z X; Lou, X C; Lowery, B; Lu, G R; Lu, F; Lu, J G; Luo, X L; Ma, E C; Ma, J M; Malchow, R L; Mao, H S; Mao, Z P; Meng, X C; Mo, X H; Nie, J; Olsen, S L; Oyang, J Y T; Paluselli, D; Pan, L J; Panetta, J; Park, H; Porter, F; Qi, N D; Qi, X R; Qian, C D; Qiu, J F; Qu, Y H; Que, Y K; Rong, G; Schernau, M; Shao, Y Y; Shen, B W; Shen, D L; Shen, H; Shen, H Y; Shen, X Y; Shi, F; Shi, H Z; Song, X F; Standifird, J; Suh, J Y; Sun, H S; Sun, L F; Sun, Y Z; Tang, S Q; Toki, W; Tong, G L; Varner, G S; Wang, F; Wang, L; Wang, L S; Wang, L Z; Wang, P; Wang, P L; Wang, S M; Wang, Y Y; Wang, Z Y; Weaver, M; Wei, C L; Wu, N; Wu, Y G; Xi, D M; Xia, X M; Xie, Y; Xie, Y H; Xu, G F; Xue, S T; Yan, J; Yan, W G; Yang, C M; Yang, C Y; Yang, H X; Yang, W; Yang, X F; Ye, M H; Ye Shu Wei; Ye, Y X; Yu, C S; Yu, C X; Yu, G W; Yu Yu Hei; Yu, Z Q; Yuan, C Z; Yuan, Y; Zhang Bing Yun; Zhang, C; Zhang, C C; Zhang, D H; De Hong Zhang; Zhang, H L; Zhang, J; Zhang, J W; Zhang, L; Zhang Lei; Zhang, L S; Zhang, P; Zhang, Q J; Zhang, S Q; Zhang, X Y; Zhang, Y Y; Zhao, D X; Zhao, H W; Jia Wei Zhao; Zhao Jia Wei; Zhao, M; Zhao Wei Ren; Zhao, Z G; Zheng Jian Ping; Zheng Lin Sheng; Zheng Zhi Peng; Zhou, B Q; Zhou, L; Zhu, K J; Zhu, Q M; Zhu, Y C; Zhu, Y S; Zhu, Z A; Zhuang, B A

2001-01-01T23:59:59.000Z

135

Meson properties in a nonlocal SU(3) chiral quark model at finite temperature  

SciTech Connect

Finite temperature meson properties are studied in the context of a nonlocal SU(3) quark model which includes flavor mixing and the coupling of quarks to the Polyakov loop (PL). We analyze the behavior of scalar and pseudoscalar meson masses and mixing angles, as well as quark-meson couplings and pseudoscalar meson decay constants.

Contrera, G. A. [CONICET, Rivadavia 1917, 1033 Buenos Aires (Argentina); Physics Department, Centro Atomico Constituyentes, Buenos Aires (Argentina); Gomez Dumm, D. [CONICET, Rivadavia 1917, 1033 Buenos Aires (Argentina); IFLP, Dpto. de Fisica, Universidad Nacional de La Plata, C.C. 67, (1900) La Plata (Argentina); Scoccola, N. N. [CONICET, Rivadavia 1917, 1033 Buenos Aires (Argentina); Universidad Favaloro, Solis 453, 1078 Buenos Aires (Argentina)

2010-11-12T23:59:59.000Z

136

Large N QCD in two dimensions with a baryonic chemical potential  

E-Print Network (OSTI)

We consider large N gauge theory on a two dimensional lattice in the presence of a baryonic chemical potential. We work with one copy of naive fermion and argue that reduction holds even in the presence of a chemical potential. Analytical arguments supported by numerical studies show that there is no phase transition as a function of the baryonic chemical potential.

Galvez, Richard; Narayanan, Rajamani

2008-01-01T23:59:59.000Z

137

A Study of Double-Charm and Charm-Strange Baryons inElectron-Positron Annihilations  

SciTech Connect

In this dissertation I describe a study of double-charm and charm-strange baryons based on data collected with the BABAR Detector at the Stanford Linear Accelerator Center. In this study I search for new baryons and make precise measurements of their properties and decay modes. I seek to verify and expand upon double-charm and charm-strange baryon observations made by other experiments. The BABAR Detector is used to measure subatomic particles that are produced at the PEP-II storage rings. I analyze approximately 300 million e+e- {yields} c{bar c} events in a search for the production of double-charm baryons. I search for the double-charm baryons {Xi}{sup +}{sub cc} (containing the quarks ccd) and {Xi}{sup ++}{sub cc} (ccu) in decays to {Lambda}{sup +}{sub c}K{sup -}{pi}{sup +} and {Lambda}{sup +}{sub c}K{sup -}{pi}{sup +}{pi}{sup +}, respectively. No statistically significant signals for their production are found, and upper limits on their production are determined. Statistically significant signals for excited charm-strange baryons are observed with my analysis of approximately 500 million e+e- {yields} c{bar c} events. The charged charm-strange baryons {Xi}{sub c}(2970){sup +}, {Xi}{sub c}(3055){sup +}, {Xi}{sub c}(3123){sup +} are found in decays to {Lambda}{sup +}{sub c}K{sup -}{pi}{sup +}, the same decay mode used in the {Xi}{sup +}{sub cc} search. The neutral charm-strange baryon {Xi}{sub c}(3077){sup 0} is observed in decays to {Lambda}{sup +}{sub c}K{sub 8}{pi}{sup -}. I also search for excited charm-strange baryon decays to {Lambda}{sup +}{sub c}K{sub 8}, {Lambda}{sup +}{sub c}K{sup -}, {Lambda}{sup +}{sub c}K{sub 8}{pi}{sup -}{pi}{sup +}, and {Lambda}{sup +}{sub c}K{sup -}{pi}{sup -}{pi}{sup +}. No significant charm-strange baryon signals a f h these decay modes. For each excited charm-strange baryon state that I observe, I measure its mass, natural width (lifetime), and production rate. The properties of these excited charm-strange baryons and their decay modes provide constraints for phenomenological models of quark interactions through quantum chromodynamics. My discovery of the two new charm-strange baryons {Xi}{sub c}(3055){sup +} and {Xi}{sub c}(3123){sup +} influences our theoretical understanding of charm-strange baryon states.

Edwards, Adam J.; /SLAC

2007-10-15T23:59:59.000Z

138

The Baryon Oscillation Spectroscopic Survey of SDSS-III  

E-Print Network (OSTI)

The Baryon Oscillation Spectroscopic Survey (BOSS) is designed to measure the scale of baryon acoustic oscillations (BAO) in the clustering of matter over a larger volume than the combined efforts of all previous spectroscopic surveys of large scale structure. BOSS uses luminous galaxies to measure BAO to redshifts z<0.7 and observations of neutral hydrogen in the Lyman alpha forest in quasar spectra to constrain BAO over the redshift range 2.15

Dawson, Kyle S; Ahn, Christopher P; Anderson, Scott F; Aubourg, Eric; Bailey, Stephen; Barkhouser, Robert H; Bautista, Julian E; Beifiori, Alessandra; Berlind, Andreas A; Bhardwaj, Vaishali; Bizyaev, Dmitry; Blake, Cullen H; Blanton, Michael R; Blomqvist, Michael; Bolton, Adam S; Borde, Arnaud; Bovy, Jo; Brandt, W N; Brewington, Howard; Brinkmann, Jon; Brown, Peter J; Brownstein, Joel R; Bundy, Kevin; Busca, N G; Carithers, William; Carnero, Aurelio R; Carr, Michael A; Chen, Yanmei; Comparat, Johan; Connolly, Natalia; Cope, Frances; Croft, Rupert A C; Cuesta, Antonio J; da Costa, Luiz N; Davenport, James R A; Delubac, Timothee; de Putter, Roland; Dhital, Saurav; Ealet, Anne; Ebelke, Garrett L; Eisenstein, Daniel J; Escoffier, S; Fan, Xiaohui; Ak, N Filiz; Finley, Hayley; Font-Ribera, Andreu; Genova-Santos, R; Gunn, James E; Guo, Hong; Haggard, Daryl; Hall, Patrick B; Hamilton, Jean-Christophe; Harris, Ben; Harris, David W; Ho, Shirley; Hogg, David W; Holder, Diana; Honscheid, Klaus; Huehnerhoff, Joe; Jordan, Beatrice; Jordan, Wendell P; Kauffmann, Guinevere; Kazin, Eyal A; Kirkby, David; Klaene, Mark A; Kneib, Jean-Paul; Goff, Jean-Marc Le; Lee, Khee-Gan; Long, Daniel C; Loomis, Craig P; Lundgren, Britt; Lupton, Robert H; Maia, Marcio A G; Makler, Martin; Malanushenko, Elena; Malanushenko, Viktor; Mandelbaum, Rachel; Manera, Marc; Maraston, Claudia; Margala, Daniel; Masters, Karen L; McBride, Cameron K; McDonald, Patrick; McGreer, Ian D; Mena, Olga; Miralda-Escude, Jordi; Montero-Dorta, Antonio D; Montesano, Francesco; Muna, Demitri; Myers, Adam D; Naugle, Tracy; Nichol, Robert C; Noterdaeme, Pasquier; Olmstead, Matthew D; Oravetz, Audrey; Oravetz, Daniel J; Owen, Russell; Padmanabhan, Nikhil; Palanque-Delabrouille, Nathalie; Pan, Kaike; Parejko, John K; Paris, Isabelle; Percival, Will J; Perez-Fournon, Ismael; Perez-Rafols, Ignasi; Petitjean, Patrick; Pfaffenberger, Robert; Pforr, Janine; Pieri, Matthew M; Prada, Francisco; Price-Whelan, Adrian M; Raddick, M Jordan; Rebolo, Rafael; Rich, James; Richards, Gordon T; Rockosi, Constance M; Roe, Natalie A; Ross, Ashley J; Ross, Nicholas P; Rossi, Graziano; Rubino-Martin, J A; Samushia, Lado; Sanchez, Ariel G; Sayres, Conor; Schmidt, Sarah J; Schneider, Donald P; Scoccola, C G; Seo, Hee-Jong; Shelden, Alaina; Sheldon, Erin; Shen, Yue; Shu, Yiping; Slosar, Anze; Smee, Stephen A; Snedden, Stephanie A; Stauffer, Fritz; Steele, Oliver; Strauss, Michael A; Suzuki, Nao; Swanson, Molly E C; Tal, Tomer; Tanaka, Masayuki; Thomas, Daniel; Tinker, Jeremy L; Tojeiro, Rita; Tremonti, Christy A; Magana, M Vargas; Verde, Licia; Viel, Matteo; Wake, David A; Watson, Mike; Weaver, Benjamin A; Weinberg, David H; Weiner, Benjamin J; West, Andrew A; White, Martin; Wood-Vasey, W M; Yeche, Christophe; Zehavi, Idit; Zhao, Gong-Bo; Zheng, Zheng

2012-01-01T23:59:59.000Z

139

Transport properties of a meson gas  

E-Print Network (OSTI)

We present recent results on a systematic method to calculate transport coefficients for a meson gas (in particular, we analyze a pion gas) at low temperatures in the context of Chiral Perturbation Theory. Our method is based on the study of Feynman diagrams with a power counting which takes into account collisions in the plasma by means of a non-zero particle width. In this way, we obtain results compatible with analysis of Kinetic Theory with just the leading order diagram. We show the behavior with temperature of electrical and thermal conductivities and shear and bulk viscosities, and we discuss the fundamental role played by unitarity. We obtain that bulk viscosity is negligible against shear viscosity near the chiral phase transition. Relations between the different transport coefficients and bounds on them based on different theoretical approximations are also discussed. We also comment on some applications to heavy-ion collisions.

D. Fernandez-Fraile; A. Gomez Nicola

2007-06-25T23:59:59.000Z

140

Delta, iota and other meson spectroscopies  

Science Conference Proceedings (OSTI)

This talk is given from the point of view of an experimentalist. Meson spectroscopy in the 1 to 3 GeV region is interesting because experiments exploring this region, in particular radiative psi decay, have found a rich structure of resonances too complicated to unravel with any one experiment, and not easily interpreted with any one theoretical model. None of the theoretical calculations predicting all kinds of interesting and exotic objects in this region is very convincing or reliable. Additional input from anti pp annihilation can be very useful in helping to find the answers to the following open questions: what exactly is this spectrum, what are the masses and quantum numbers of the resonances, as determined from analysis of data without theoretical prejudices; how is this spectrum described by QCD, is there evidence for new kinds of states like glue-balls, hybrids, axions, Higgses or multiquark exotics, and is there any evidence for new physics beyond QCD. 20 refs.

Lipkin, H.J.

1986-05-01T23:59:59.000Z

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141

Hydrogen like classification for light nonstrange mesons  

E-Print Network (OSTI)

The recent experimental results on the spectrum of highly excited light nonstrange mesons are known to reveal a high degree of degeneracy among different groups of states. We revise some suggestions about the nature of the phenomenon and put the relevant ideas into the final shape. The full group of approximate mass degeneracies is argued to be $SU(2)_f\\times I\\times O(4)$, where $I$ is the degeneracy of isosinglets and isotriplets and O(4) is the degeneracy group of the relativistic hydrogen atom. We discuss the dynamical origin and consequences of considered symmetry with a special emphasis on distinctions of this symmetry from the so-called chiral symmetry restoration scenario.

S. S. Afonin

2007-09-27T23:59:59.000Z

142

Helicity Probabilities For Heavy Quark Fragmentation Into Excited Mesons  

E-Print Network (OSTI)

In the fragmentation of a heavy quark into a heavy meson whose light degrees of freedom have angular momentum $3/2$, all the helicity probabilities are completely determined in the heavy quark limit up to a single probability $w_{3/2}$. We point out that this probability depends on the longitudinal momentum fraction $z$ of the meson and on its transverse momentum $p_\\bot$ relative to the jet axis. We calculate $w_{3/2}$ as a function of scaling variables corresponding to $z$ and $p_\\bot$ for the heavy quark limit of the perturbative QCD fragmentation functions for $b$ quark to fragment into $(b \\bar c)$ mesons. In this model, the light degrees of freedom prefer to have their angular momentum aligned transverse to, rather than along, the jet axis. Implications for the production of excited heavy mesons, like $D^{**}$ and $B^{**}$, are discussed.

Tzu Chiang Yuan

1994-07-20T23:59:59.000Z

143

The Photoproduction of Hybrid Mesons from Cebaf to HERA  

E-Print Network (OSTI)

Decay widths, branching ratios and production dynamics of some recently discovered $J^{PC} = 1^{-+}, 0^{-+}$,$1^{--}$ and $2^{-+}$ mesons are found to be in remarkable agreement with the predicted properties of hybrid mesons. We propose tests for this new dynamics, emphasise the critical role of $\\pi b_1$ or $\\pi h_1$ decay channels in discriminating hybrids from conventional states, and suggest that photoproduction may offer special opportunities for isolation and confirmation of hybrids.

F. E. Close; P. R. Page

1994-12-15T23:59:59.000Z

144

Search for the ?-N bound state from ?meson subthreshold production  

E-Print Network (OSTI)

The subthreshold photoproduction of \\phi mesons from heavy nuclear targets has been suggested as a candidate to search for the \\phi-N bound state, a quantum chromodynamics molecular state. In this Brief Report, we present detailed Monte Carlo studies to demonstrate the feasibility of this technique. Further, we show that proton-induced subthreshold production of \\phi meson from heavy nuclear targets is also suitable for such a search.

S. Liska; H. Gao; W. Chen; X. Qian

2007-07-06T23:59:59.000Z

145

Hadronic Production of the Doubly Heavy Baryon $?_{bc}$ at LHC  

E-Print Network (OSTI)

We investigate the hadronic production of the doubly heavy baryon $\\Xi_{bc}$ at the large hadron collider (LHC), where contributions from the four $(bc)$-diquark states $(bc)_{\\bf\\bar{3},6}[^1S_0]$ and $(bc)_{\\bf\\bar{3},6}[^3S_1]$ have been taken into consideration. Numerical results show that under the condition of $p_T>4$ GeV and $|y|energy $\\sqrt{S}=7$ TeV and $\\sqrt{S}=14$ TeV respectively. For experimental usage, the total and the interested differential cross-sections are estimated under some typical $p_T$- and $y$- cuts for the LHC detectors CMS, ATLAS and LHCb. Main uncertainties are discussed and a comparative study on the hadronic production of $\\Xi_{cc}$, $\\Xi_{bc}$ and $\\Xi_{bb}$ at LHC are also presented.

Jia-Wei Zhang; Xing-Gang Wu; Tao Zhong; Yao Yu; Zhen-Yun Fang

2011-01-06T23:59:59.000Z

146

$?$ baryon strong decays in a chiral quark model  

E-Print Network (OSTI)

The strong decays of $\\Xi$ baryons up to N=2 shell were studied in a chiral quark model. The strong decay properties of these well-established ground decuplet baryons were reasonably described. We found that (i) $\\Xi(1690)$ and $\\Xi(1820)$ could be assigned to the spin-parity $J^P=1/2^-$ state $|70,^{2}{8},1,1,1/2^->$ and the spin-parity $J^P=3/2^-$ state $|70,^{2}{8},1,1,3/2^->$, respectively. Slight configuration mixing might exist in these two negative parity states. (ii) $\\Xi(1950)$ might correspond to several different $\\Xi$ resonances. The broad states ($\\Gamma\\sim 100$ MeV) observed in the $\\Xi\\pi$ channel could be classified as the pure $J^P=5/2^-$ octet state $\\Xi^0|70,^{4}8,1,1,5/2^->$ or the mixed state $|\\Xi 1/2^->_3 $ with $J^P=1/2^-$. The $\\Xi$ resonances with moderate width ($\\Gamma\\sim 60$ MeV) observed in the $\\Xi\\pi$ channel might correspond to the $J^P=1/2^+$ excitation $|56,^{4}10,2,2,1/2^+>$. The second orbital excitation $|56,^{4}10,2,2,3/2^+>$ and the mixed state $|\\Xi 1/2^->_1$ might be candidates for the narrow width state observed in the $\\Lambda \\bar{K}$ channel, however, their spin-parity numbers are incompatible with the moment analysis of the data. (iii) $\\Xi(2030)$ could not be assigned to either any spin-parity $J^P=7/2^+$ states or any pure $J^P=5/2^+$ configurations. It seems to favor the $|70,^{2}8,2,2,3/2^+>$ assignment, however, its spin conflicts with the moment analysis of the data. To find more $\\Xi$ resonances, the observations in the $\\Xi(1530)\\pi$ and $\\Sigma(1385) \\bar{K}$ channels are necessary.

Li-Ye Xiao; Xian-Hui Zhong

2013-02-01T23:59:59.000Z

147

THE BARYON OSCILLATION SPECTROSCOPIC SURVEY OF SDSS-III  

Science Conference Proceedings (OSTI)

The Baryon Oscillation Spectroscopic Survey (BOSS) is designed to measure the scale of baryon acoustic oscillations (BAO) in the clustering of matter over a larger volume than the combined efforts of all previous spectroscopic surveys of large-scale structure. BOSS uses 1.5 million luminous galaxies as faint as i = 19.9 over 10,000 deg{sup 2} to measure BAO to redshifts z < 0.7. Observations of neutral hydrogen in the Ly{alpha} forest in more than 150,000 quasar spectra (g < 22) will constrain BAO over the redshift range 2.15 < z < 3.5. Early results from BOSS include the first detection of the large-scale three-dimensional clustering of the Ly{alpha} forest and a strong detection from the Data Release 9 data set of the BAO in the clustering of massive galaxies at an effective redshift z = 0.57. We project that BOSS will yield measurements of the angular diameter distance d{sub A} to an accuracy of 1.0% at redshifts z = 0.3 and z = 0.57 and measurements of H(z) to 1.8% and 1.7% at the same redshifts. Forecasts for Ly{alpha} forest constraints predict a measurement of an overall dilation factor that scales the highly degenerate D{sub A} (z) and H {sup -1}(z) parameters to an accuracy of 1.9% at z {approx} 2.5 when the survey is complete. Here, we provide an overview of the selection of spectroscopic targets, planning of observations, and analysis of data and data quality of BOSS.

Dawson, Kyle S.; Ahn, Christopher P.; Bolton, Adam S. [Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 (United States); Schlegel, David J.; Bailey, Stephen [Lawrence Berkeley National Laboratory, One Cyclotron Road, Berkeley, CA 94720 (United States); Anderson, Scott F.; Bhardwaj, Vaishali [Department of Astronomy, University of Washington, Box 351580, Seattle, WA 98195 (United States); Aubourg, Eric; Bautista, Julian E. [APC, University of Paris Diderot, CNRS/IN2P3, CEA/IRFU, Observatoire de Paris, Sorbonne Paris Cite (France); Barkhouser, Robert H. [Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218 (United States); Beifiori, Alessandra [Max-Planck-Institut fuer Extraterrestrische Physik, Giessenbachstrasse, D-85748 Garching (Germany); Berlind, Andreas A. [Department of Physics and Astronomy, Vanderbilt University, VU Station 1807, Nashville, TN 37235 (United States); Bizyaev, Dmitry; Brewington, Howard [Apache Point Observatory, P.O. Box 59, Sunspot, NM 88349 (United States); Blake, Cullen H. [Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544 (United States); Blanton, Michael R. [Center for Cosmology and Particle Physics, Department of Physics, New York University, 4 Washington Place, New York, NY 10003 (United States); Blomqvist, Michael [Department of Physics and Astronomy, University of California, Irvine, CA 92697 (United States); Borde, Arnaud [CEA, Centre de Saclay, Irfu/SPP, F-91191 Gif-sur-Yvette (France); Bovy, Jo [Institute for Advanced Study, Einstein Drive, Princeton, NJ 08540 (United States); Brandt, W. N., E-mail: kdawson@astro.utah.edu [Department of Astronomy and Astrophysics, 525 Davey Laboratory, The Pennsylvania State University, University Park, PA 16802 (United States); and others

2013-01-01T23:59:59.000Z

148

Nuclear modification factors of phi mesons in d+Au, Cu+Cu and Au+Au collisions at sqrt(S_NN)=200 GeV  

E-Print Network (OSTI)

The PHENIX experiment at the Relativistic Heavy Ion Collider (RHIC) has performed systematic measurements of phi meson production in the K+K- decay channel at midrapidity in p+p, d+Au, Cu+Cu and Au+Au collisions at sqrt(S_NN)=200 GeV. Results are presented on the phi invariant yield and the nuclear modification factor R_AA for Au+Au and Cu+Cu, and R_dA for d+Au collisions, studied as a function of transverse momentum (1phi exhibits a suppression relative to expectations from binary scaled p+p results. The amount of suppression is smaller than that of the neutral pion and the eta meson in the intermediate p_T range (2--5 GeV/c); whereas at higher p_T the phi, pi^0, and eta show similar suppression. The baryon (protons and anti-protons) excess observed in central Au+Au collisions at intermediate p_T is not observed for the phi meson despite the similar mass of the proton and the phi. This suggests that the excess is linked to the number of constituent quarks rather than the hadron mass. The difference gradually disappears with decreasing centrality and for peripheral collisions the R_AA values for both particles are consistent with binary scaling. Cu+Cu collisions show the same yield and suppression as Au+Au collisions for the same number of N_part. The R_dA of phi shows no evidence for cold nuclear effects within uncertainties.

PHENIX Collaboration; A. Adare; S. Afanasiev; C. Aidala; N. N. Ajitanand; Y. Akiba; H. Al-Bataineh; J. Alexander; A. Al-Jamel; A. Angerami; K. Aoki; L. Aphecetche; Y. Aramaki; R. Armendariz; S. H. Aronson; J. Asai; E. T. Atomssa; R. Averbeck; T. C. Awes; B. Azmoun; V. Babintsev; M. Bai; G. Baksay; L. Baksay; A. Baldisseri; K. N. Barish; P. D. Barnes; B. Bassalleck; A. T. Basye; S. Bathe; S. Batsouli; V. Baublis; F. Bauer; C. Baumann; A. Bazilevsky; S. Belikov; R. Belmont; R. Bennett; A. Berdnikov; Y. Berdnikov; J. H. Bhom; A. A. Bickley; M. T. Bjorndal; D. S. Blau; J. G. Boissevain; J. S. Bok; H. Borel; N. Borggren; K. Boyle; M. L. Brooks; D. S. Brown; D. Bucher; H. Buesching; V. Bumazhnov; G. Bunce; J. M. Burward-Hoy; S. Butsyk; S. Campbell; A. Caringi; N. Cassano; J. -S. Chai; B. S. Chang; J. -L. Charvet; C. -H. Chen; S. Chernichenko; J. Chiba; C. Y. Chi; M. Chiu; I. J. Choi; J. B. Choi; R. K. Choudhury; P. Christiansen; T. Chujo; P. Chung; A. Churyn; O. Chvala; V. Cianciolo; Z. Citron; C. R. Cleven; Y. Cobigo; B. A. Cole; M. P. Comets; Z. Conesa del Valle; M. Connors; P. Constantin; M. Csanad; T. Csorgo; T. Dahms; S. Dairaku; I. Danchev; K. Das; A. Datta; G. David; M. K. Dayananda; M. B. Deaton; K. Dehmelt; H. Delagrange; A. Denisov; D. d'Enterria; A. Deshpande; E. J. Desmond; K. V. Dharmawardane; O. Dietzsch; A. Dion; M. Donadelli; L. D Orazio; J. L. Drachenberg; O. Drapier; A. Drees; K. A. Drees; A. K. Dubey; J. M. Durham; A. Durum; D. Dutta; V. Dzhordzhadze; S. Edwards; Y. V. Efremenko; J. Egdemir; F. Ellinghaus; W. S. Emam; T. Engelmore; A. Enokizono; H. En'yo; B. Espagnon; S. Esumi; K. O. Eyser; B. Fadem; D. E. Fields; M. Finger Jr.; M. Finger; F. Fleuret; S. L. Fokin; B. Forestier; Z. Fraenkel; J. E. Frantz; A. Franz; A. D. Frawley; K. Fujiwara; Y. Fukao; S. -Y. Fung; T. Fusayasu; S. Gadrat; I. Garishvili; F. Gastineau; M. Germain; A. Glenn; H. Gong; M. Gonin; J. Gosset; Y. Goto; R. Granier de Cassagnac; N. Grau; S. V. Greene; G. Grim; M. Grosse Perdekamp; T. Gunji; H. -A. Gustafsson; T. Hachiya; A. Hadj Henni; C. Haegemann; J. S. Haggerty; M. N. Hagiwara; K. I. Hahn; H. Hamagaki; J. Hamblen; J. Hanks; R. Han; H. Harada; E. P. Hartouni; K. Haruna; M. Harvey; E. Haslum; K. Hasuko; R. Hayano; M. Heffner; T. K. Hemmick; T. Hester; J. M. Heuser; X. He; H. Hiejima; J. C. Hill; R. Hobbs; M. Hohlmann; M. Holmes; W. Holzmann; K. Homma; B. Hong; T. Horaguchi; D. Hornback; S. Huang; M. G. Hur; T. Ichihara; R. Ichimiya; H. Iinuma; Y. Ikeda; K. Imai; M. Inaba; Y. Inoue; D. Isenhower; L. Isenhower; M. Ishihara; T. Isobe; M. Issah; A. Isupov; D. Ivanischev; Y. Iwanaga; B. V. Jacak; J. Jia; X. Jiang; J. Jin; O. Jinnouchi; B. M. Johnson; T. Jones; K. S. Joo; D. Jouan; D. S. Jumper; F. Kajihara; S. Kametani; N. Kamihara; J. Kamin; M. Kaneta; J. H. Kang; H. Kanou; J. Kapustinsky; K. Karatsu; M. Kasai; T. Kawagishi; D. Kawall; M. Kawashima; A. V. Kazantsev; S. Kelly; T. Kempel; A. Khanzadeev; K. M. Kijima; J. Kikuchi; A. Kim; B. I. Kim; D. H. Kim; D. J. Kim; E. J. Kim; E. Kim; Y. -J. Kim; Y. -S. Kim; E. Kinney; A. Kiss; E. Kistenev; A. Kiyomichi; J. Klay; C. Klein-Boesing; L. Kochenda; V. Kochetkov; B. Komkov; M. Konno; J. Koster; D. Kotchetkov; D. Kotov; A. Kozlov; A. Kral; A. Kravitz; P. J. Kroon; J. Kubart; G. J. Kunde; N. Kurihara; K. Kurita; M. Kurosawa; M. J. Kweon; Y. Kwon; G. S. Kyle; R. Lacey; Y. S. Lai; J. G. Lajoie; A. Lebedev; Y. Le Bornec; S. Leckey; D. M. Lee; J. Lee; K. B. Lee; K. S. Lee; M. K. Lee; T. Lee; M. J. Leitch; M. A. L. Leite; B. Lenzi; P. Lichtenwalner; P. Liebing; H. Lim; L. A. Linden Levy; T. Liska; A. Litvinenko; H. Liu; M. X. Liu; X. Li; X. H. Li; B. Love; D. Lynch; C. F. Maguire; Y. I. Makdisi; A. Malakhov; M. D. Malik; V. I. Manko; E. Mannel; Y. Mao; L. Masek; H. Masui; F. Matathias; M. C. McCain; M. McCumber; P. L. McGaughey; N. Means; B. Meredith; Y. Miake; T. Mibe; A. C. Mignerey; P. Mikes; K. Miki; T. E. Miller; A. Milov; S. Mioduszewski; G. C. Mishra; M. Mishra; J. T. Mitchell; M. Mitrovski; A. K. Mohanty; H. J. Moon; Y. Morino; A. Morreale; D. P. Morrison; J. M. Moss; T. V. Moukhanova; D. Mukhopadhyay; T. Murakami; J. Murata; S. Nagamiya; Y. Nagata; J. L. Nagle; M. Naglis; M. I. Nagy; I. Nakagawa; Y. Nakamiya; K. R. Nakamura; T. Nakamura; K. Nakano; S. Nam; J. Newby; M. Nguyen; M. Nihashi; B. E. Norman; R. Nouicer; A. S. Nyanin; J. Nystrand; C. Oakley; E. O'Brien; S. X. Oda; C. A. Ogilvie; H. Ohnishi; I. D. Ojha; K. Okada; M. Oka; O. O. Omiwade; Y. Onuki; A. Oskarsson; I. Otterlund; M. Ouchida; K. Ozawa; R. Pak; D. Pal; A. P. T. Palounek; V. Pantuev; V. Papavassiliou; I. H. Park; J. Park; S. K. Park; W. J. Park; S. F. Pate; H. Pei; J. -C. Peng; H. Pereira; V. Peresedov; D. Yu. Peressounko; R. Petti; C. Pinkenburg; R. P. Pisani; M. Proissl; M. L. Purschke; A. K. Purwar; H. Qu; J. Rak; A. Rakotozafindrabe; I. Ravinovich; K. F. Read; S. Rembeczki; M. Reuter

2010-04-20T23:59:59.000Z

149

Propagation of B mesons in the atmosphere  

E-Print Network (OSTI)

Collisions of cosmic rays in the atmosphere may produce heavy hadrons of very high energy. The decay length of a $B$ meson of energy above $10^7$ GeV is larger than 1 km, implying that such a particle tends to interact in the air before it decays. We show that the fraction of energy deposited in these interactions is much smaller than in proton and pion collisions. We parameterize their elasticity and determine the average number of interactions and the atmospheric depth at the decay point for different initial energies. We find that the profile of a $3\\times 10^9$ GeV bottom shower may be very different from the profile of a proton shower of the same energy, defining either a very deep maximum, or two maxima, or other features that cannot be parameterized with a single Gaisser-Hillas function. Finally, we discuss under what conditions a bottom hadron inside the parent air shower may provide observable effects.

A. Bueno; A. Gascon; J. I. Illana; M. Masip

2011-09-20T23:59:59.000Z

150

Formation of the intermediate baryon systems in hadron-nuclear and nuclear-nuclear interactions  

E-Print Network (OSTI)

The centrality experiments indicate regime change and saturation in the behavior of some characteristics of the secondary particles emitted in hadron-nuclear and nuclear-nuclear interactions at high energies. The phenomenon has a critical character. The simple models do not explain the effect. We suppose that the responsible mechanism to explain the phenomenon could be the formation and decay of the intermediate baryon systems. Such systems could be formed as a result of nucleon percolation in compressed baryonic matter. Formation of big percolation cluster may change the properties of the medium, e.g., it could lead to the changing its transparency. This could be used to get a signal of the intermediate baryonic system formation. We consider two signals to identify the formation of the intermediate baryon systems: the critical changing of transparency of the strongly interacting matter and the enhancement of light nuclei production with increase in centrality.

M. K. Suleymanov; E. U. Khan; A Kravchakova; Mahnaz Q. Haseeb; S. M. Saleem; Y. H. Huseynaliyev; S Vokal; A. S. Vodopianov; O. B. Abdinov

2007-12-17T23:59:59.000Z

151

HEAVY BARYONS: A COMBINED LARGE Nc AND HEAVY QUARK EXPANSION FOR ELECTROWEAK CURRENTS  

E-Print Network (OSTI)

The combined large Nc and heavy quark limit for baryons containing a single heavy quark is discussed. The combined large Nc and heavy quark expansion of the heavy quark bilinear operators is obtained. In the combined expansion the corrections proportional to mN/mQ are summed to all orders. In particular, the combined expansion can be used to determine semileptonic form factors of heavy baryons in the combined limit. 1

Boris A. Gelman

2002-01-01T23:59:59.000Z

152

The Catalysis of Nuclear Reactions by mu Mesons  

DOE Green Energy (OSTI)

In the course of a recent experiment involving the stopping of negative K mesons in a 10-inch liquid hydrogen bubble chamber, an interesting new reaction was observed to take place. The chamber is traversed by many more negative {mu} mesons than K mesons, so that in the last 75,000 photographs, approximately 2500 {mu}{sup -} decays at rest have been observed. In the same pictures, several hundred {pi}{sup -} mesons have been observed to disappear at rest, presumably by one of the ''Panofsky reactions''. For tracks longer than 10 cm, it is possible to distinguish a stopping {mu} meson from a stopping {pi} meson by comparing its curved path (in a field of 11,000 gauss) with that of a calculated template. In addition to the normal {pi}{sup -} and {mu}{sup -} stoppings, we have observed 15 cases in which what appears (from curvature measurement) to be a {mu}{sup -} meson comes to rest in the hydrogen, and then gives rise to a secondary negative particle of 1.7 cm range, which in turn decays by emitting an electron. (A 4.1-Mev {mu} meson from {pi} - {mu} decay has a range of 1.0 cm.) The energy spectrum of the electrons from these 15 secondary particles looks remarkably like that of the {mu} meson. There are four electrons in the energy range 50 to 55 Mev, and none higher; the other electrons have energies varying from 50 Mev to 13 Mev. The most convincing proof that the primary particle actually comes to rest, and does not--for example--have a large resonant cross section for scattering at a residual range of 1.7 cm, is the following: In five of the 15 special events, there is a large gap between the last bubble of the primary track and the first bubble of the secondary track. This gap is a real effect, and not merely a statistical fluctuation in the spacing of the bubbles, since in some cases the tracks form a letter X, and in another case the secondary track is parallel to the primary, but displaced transversely by about 1 mm at the end of the primary. These real gaps appear also (although perhaps less frequently) between some otherwise normal-looking {mu}{sup -} endings and the subsequent decay electron; they are thought to be the distance traveled by the small neutral mesic atom.

Alvarez, L.W.; Bradner, H.; Crawford Jr, F.S.; Crawford, J.A.; Falk-Vairant, P.; Good, M.L.; Gow, J.D.; Hosenfeld, A.R.; Solmitz, F.; Stevenson, M.L.; Ticho, H.K.; Tripp, H.D.

1956-12-10T23:59:59.000Z

153

$?$ meson exchange effect on nonmesonic hypernuclear weak decay observables  

E-Print Network (OSTI)

We analyze the influence of $\\sigma$ meson exchange on the main nonmesonic hypernuclear weak decay observables: the total rate, $\\Gamma_{NM}$, the neutron-to-proton branching ratio, $\\Gamma_{n/p}$, and the proton asymmetry parameter, $a_\\Lambda$. The $\\sigma$ meson exchange is added to the standard strangeness-changing weak $\\Lambda N\\to NN$ transition potential, which includes the exchange of the complete pseudoscalar and vector mesons octet ($\\pi$, $\\eta$, $K$, $\\rho$, $\\omega$, $K^*$). Using a shell model formalism, the $\\sigma$ meson weak coupling constants are adjusted to reproduce the recent $\\Gamma_{NM}$ and $\\Gamma_{n/p}$ experimental data for $^5_{\\Lambda}He$. Numerical results for the remaining observables of $^5_{\\Lambda}He$ and all the observables of $^{12}_{\\Lambda}C$ decays are presented. They clearly show that the addition of the $\\sigma$ meson, in spite of improving some observables values, is not enough to reproduce simultaneously all the measurements, and the puzzle posed by the experimental data remains unexplained.

C. Barbero; A. Mariano

2005-09-15T23:59:59.000Z

154

Hadronic production of eta--mesons: recent results and open questions  

E-Print Network (OSTI)

I review recent insights and open questions connected with the production of eta--mesons from hadrons.

C. Hanhart

2005-11-17T23:59:59.000Z

155

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Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Contents" ,"Colorado Natural Gas Repressuring (MMcf)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description"," Of Series","Frequency","Latest...

206

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Contents" ,"California Natural Gas Repressuring (MMcf)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description"," Of Series","Frequency","Latest...

207

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Contents" ,"Nevada Natural Gas Residential Consumption (MMcf)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description"," Of Series","Frequency","Latest...

208

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Contents" ,"Oregon Natural Gas Residential Consumption (MMcf)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description"," Of Series","Frequency","Latest...

209

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Workbook Contents" ,"Texas Natural Gas Repressuring (MMcf)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description"," Of Series","Frequency","Latest...

210

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Contents" ,"Pennsylvania Natural Gas Repressuring (MMcf)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description"," Of Series","Frequency","Latest...

211

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Workbook Contents" ,"South Dakota Natural Gas Repressuring (MMcf)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description"," Of Series","Frequency","La...

212

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Workbook Contents" ,"South Dakota Price of Natural Gas Sold to Commercial Consumers (Dollars per Thousand Cubic Feet)" ,"Click worksheet name or tab at bottom for data"...

213

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Workbook Contents" ,"Natural Gas Delivered to Consumers in South Dakota (Including Vehicle Fuel) (MMcf)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet...

214

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Workbook Contents" ,"Natural Gas Citygate Price in South Dakota (Dollars per Thousand Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet...

215

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Workbook Contents" ,"South Dakota Natural Gas Withdrawals from Oil Wells (MMcf)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description"," Of...

216

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Workbook Contents" ,"South Dakota Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" ,"Click worksheet name or tab at bottom for data"...

217

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Workbook Contents" ,"Percent of Commercial Natural Gas Deliveries in South Dakota Represented by the Price (%)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet...

218

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Workbook Contents" ,"South Dakota Natural Gas Withdrawals from Gas Wells (MMcf)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description"," Of...

219

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Workbook Contents" ,"South Dakota Natural Gas Gross Withdrawals from Coalbed Wells (MMcf) " ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","...

220

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Workbook Contents" ,"Percentage of Total Natural Gas Residential Deliveries included in Prices " ,"Click worksheet name or tab at bottom for data" ,"Worksheet...

Note: This page contains sample records for the topic "mesons contents baryons" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


221

Universal Short-Range Repulsion in the Baryon System Originating from the Confinement --Approach in String-Junction Model--  

E-Print Network (OSTI)

We show a way to unifiedly understand the origins of the repulsive core of baryon-baryon interaction and the universal repulsion of three-baryon interaction needed to avoid dramatic softening of the equation of state of neutron stars due to hyperon mixing. For this aim we adopt the string-junction model which embodies the essential aspects of the confinement in the baryon system confirmed by recent lattice QCD calculations. Key concept of this study lies in the recognition that baryonic short-range repulsion appears as the latent effect implying the energy necessary for full overlap of baryons, for the confinement to persist at such situation. Numerical results are shown and related problems are discussed.

Ryozo Tamagaki

2008-01-15T23:59:59.000Z

222

Kinetic Description of a Finite Temperature Meson Gas  

E-Print Network (OSTI)

A transport model based on the mean free path approach for an interacting meson system at finite temperatures is discussed. A transition to a quark gluon plasma is included within the framework of the bag model. We discuss some calculations for a pure meson gas where the Hagedorn limiting temperature is reproduced when including the experimentally observed resonances. Next we include the possibility for a QGP formation based on the MIT bag model. The results obtained compare very well with Lattice QCD calculations. In particular the cross over to the QGP at about 175 MeV temperature is nicely reproduced.

Zhi Guang Tan; Dai-Mei Zhou; S. Terranova; A. Bonasera

2006-06-28T23:59:59.000Z

223

Meson production in high-energy electron-nucleus scattering  

E-Print Network (OSTI)

Experimental studies of meson production through two-photon fusion in inelastic electron-nucleus scattering is now under way. A high-energy photon radiated by the incident electron is fused with a soft photon radiated by the nucleus. The process takes place in the small-angle-Coulomb region of nuclear scattering. We expound the theory for this production process as well as its interference with coherent-radiative-meson production. In particular, we investigate the distortion of the electron wave function due to multiple-Coulomb scattering.

Göran Fäldt

2010-06-09T23:59:59.000Z

224

D meson hadronic decays at CLEO-c  

SciTech Connect

The recent CLEO-c results on hadronic decays of D and D{sub s} mesons are presented. First the absolute branching fractions for D and D{sub s} mesons using a double tag technique are discussed, then are the Cabibbo suppressed decays and doubly Cabibbo suppressed decays. Finally, I present the inclusive and rare decay modes and other measurements from CLEO-c. These decays illuminate a wide range of physics. A brief theoretical introduction is given before the corresponding discussion on measurement.

Yang, Fan; /Fermilab

2011-01-01T23:59:59.000Z

225

Update analysis of two-body charmed $B$ meson decays  

E-Print Network (OSTI)

The charmed B decays, $B\\to DP, ~D^*P$ and $DV$, are re-analyzed using the latest experimental data, where $P$ and $V$ denote the pseudoscalar meson and vector meson, respectively. We perform global fits under the assumption of flavor SU(3) symmetry. The size of the decay amplitudes and the strong phases between the topologically distinct amplitudes are studied. Predictions of the related $B_s$ decay rates are made based upon the fitted results. We also note a serious SU(3) symmetry breaking or inconsistency in the $DV$ sector.

Chiang, C W; Chiang, Cheng-Wei; Senaha, Eibun

2007-01-01T23:59:59.000Z

226

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"9302013 5:41:19 AM" "Back to Contents","Data 1: Natural...

227

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"1092013 12:45:25 PM" "Back to Contents","Data 1: Natural...

228

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"9302013 5:47:49 AM" "Back to Contents","Data 1: Oklahoma...

229

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"9302013 5:47:48 AM" "Back to Contents","Data 1: Ohio...

230

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"9302013 5:40:49 AM" "Back to Contents","Data 1: Natural...

231

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"9302013 5:47:39 AM" "Back to Contents","Data 1: Indiana...

232

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"9302013 5:41:58 AM" "Back to Contents","Data 1: Natural...

233

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"9302013 5:44:37 AM" "Back to Contents","Data 1: Nebraska...

234

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"9302013 5:50:33 AM" "Back to Contents","Data 1:...

235

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Workbook Contents" ,"U.S. Price of Natural Gas Pipeline Exports by Point of Exit " ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description"," Of...

236

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Workbook Contents" ,"U.S. Price of Natural Gas Pipeline Imports by Point of Entry " ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description"," Of...

237

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,,"(202) 586-8800",,,"9302013 9:14:27 AM" "Back to Contents","Data 1: Wisconsin Price of Natural Gas Sold to Commercial Consumers (Dollars per Thousand Cubic Feet)"...

238

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,,"(202) 586-8800",,,"9302013 9:13:24 AM" "Back to Contents","Data 1: Wisconsin Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic...

239

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,,"(202) 586-8800",,,"9302013 5:40:28 AM" "Back to Contents","Data 1: Wisconsin Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010WI2" "Date","Wisconsin...

240

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,,"(202) 586-8800",,,"9302013 5:43:56 AM" "Back to Contents","Data 1: Wisconsin Natural Gas Industrial Consumption (MMcf)" "Sourcekey","N3035WI2" "Date","Wisconsin...

Note: This page contains sample records for the topic "mesons contents baryons" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


241

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,,"(202) 586-8800",,,"9302013 5:45:05 AM" "Back to Contents","Data 1: Wisconsin Natural Gas Deliveries to Electric Power Consumers (MMcf)" "Sourcekey","N3045WI2"...

242

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,,"(202) 586-8800",,,"9302013 5:45:04 AM" "Back to Contents","Data 1: Wisconsin Natural Gas Deliveries to Electric Power Consumers (MMcf)" "Sourcekey","N3045WI2"...

243

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

AM" "Back to Contents","Data 1: Percent of Commercial Natural Gas Deliveries in Pennsylvania Represented by the Price (%)" "Sourcekey","N3020PA4" "Date","Percent of Commercial...

244

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,,"(202) 586-8800",,,"9302013 9:13:15 AM" "Back to Contents","Data 1: Pennsylvania Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"...

245

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,,"(202) 586-8800",,,"9302013 9:14:13 AM" "Back to Contents","Data 1: Pennsylvania Price of Natural Gas Sold to Commercial Consumers (Dollars per Thousand Cubic Feet)"...

246

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

586-8800",,,"9302013 9:16:27 AM" "Back to Contents","Data 1: Natural Gas Citygate Price in Pennsylvania (Dollars per Thousand Cubic Feet)" "Sourcekey","N3050PA3"...

247

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

586-8800",,,"9302013 9:16:28 AM" "Back to Contents","Data 1: Natural Gas Citygate Price in Pennsylvania (Dollars per Thousand Cubic Feet)" "Sourcekey","N3050PA3"...

248

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,,"(202) 586-8800",,,"172014 2:49:36 PM" "Back to Contents","Data 1: Idaho Price of Natural Gas Sold to Commercial Consumers (Dollars per Thousand Cubic Feet)"...

249

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,,"(202) 586-8800",,,"172014 2:48:16 PM" "Back to Contents","Data 1: Idaho Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010ID2" "Date","Idaho...

250

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

72014 2:54:14 PM" "Back to Contents","Data 1: Natural Gas Citygate Price in Idaho (Dollars per Thousand Cubic Feet)" "Sourcekey","N3050ID3" "Date","Natural Gas Citygate...

251

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

72014 2:54:52 PM" "Back to Contents","Data 1: Natural Gas Delivered to Consumers in Idaho (Including Vehicle Fuel) (MMcf)" "Sourcekey","N3060ID2" "Date","Natural Gas Delivered...

252

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,,"(202) 586-8800",,,"172014 2:53:12 PM" "Back to Contents","Data 1: Idaho Natural Gas Deliveries to Electric Power Consumers (MMcf)" "Sourcekey","N3045ID2"...

253

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

72014 2:54:13 PM" "Back to Contents","Data 1: Natural Gas Citygate Price in Idaho (Dollars per Thousand Cubic Feet)" "Sourcekey","N3050ID3" "Date","Natural Gas Citygate...

254

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

2:49:37 PM" "Back to Contents","Data 1: Percent of Commercial Natural Gas Deliveries in Idaho Represented by the Price (%)" "Sourcekey","N3020ID4" "Date","Percent of Commercial...

255

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,,"(202) 586-8800",,,"172014 2:51:34 PM" "Back to Contents","Data 1: Idaho Natural Gas Industrial Consumption (MMcf)" "Sourcekey","N3035ID2" "Date","Idaho...

256

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

72014 2:54:53 PM" "Back to Contents","Data 1: Natural Gas Delivered to Consumers in Idaho (Including Vehicle Fuel) (MMcf)" "Sourcekey","N3060ID2" "Date","Natural Gas Delivered...

257

Spectral Content  

NLE Websites -- All DOE Office Websites (Extended Search)

Spectral Content of the NLC Bunch Train due to Long Range Wakefields Peter Tenenbaum LCC-Note-0015 10-May-1999 Abstract The functional specifications of the sub-train position...

258

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

2:08:06 PM" "Back to Contents","Data 1: Price of Liquefied U.S. Natural Gas Exports to Brazil (Dollars per Thousand Cubic Feet)" "Sourcekey","NGMEPG0PNGNUS-NBRDMCF"...

259

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

2:08:07 PM" "Back to Contents","Data 1: Price of Liquefied U.S. Natural Gas Exports to Brazil (Dollars per Thousand Cubic Feet)" "Sourcekey","NGMEPG0PNGNUS-NBRDMCF"...

260

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

132014 2:06:54 PM" "Back to Contents","Data 1: Liquefied U.S. Natural Gas Exports to Brazil (MMcf)" "Sourcekey","NGMEPG0ENGNUS-NBRMMCF" "Date","Liquefied U.S. Natural Gas...

Note: This page contains sample records for the topic "mesons contents baryons" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


261

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

312013 3:21:41 PM" "Back to Contents","Data 1: Natural Gas Gross Withdrawals from Shale Gas Wells (Summary) " "Sourcekey","NGMEPG0FGSNUSMMCF","NGMEPG0FGSR3FMMMCF","NG...

262

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

312013 3:21:40 PM" "Back to Contents","Data 1: Natural Gas Gross Withdrawals from Shale Gas Wells (Summary) " "Sourcekey","NGMEPG0FGSNUSMMCF","NGMEPG0FGSR3FMMMCF","NG...

263

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

4:58:30 PM" "Back to Contents","Data 1: Liquefied U.S. Natural Gas Exports to South Korea (MMcf)" "Sourcekey","NGMEPG0ENGNUS-NKSMMCF" "Date","Liquefied U.S. Natural Gas...

264

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

2:08:11 PM" "Back to Contents","Data 1: Alaska Liquefied Natural Gas Exports Price to China (Dollars per Thousand Cubic Feet)" "Sourcekey","NGMEPG0PNGSAK-NCHDMCF"...

265

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

2:08:07 PM" "Back to Contents","Data 1: Price of Liquefied U.S. Natural Gas Exports to China (Dollars per Thousand Cubic Feet)" "Sourcekey","NGMEPG0PNGNUS-NCHDMCF"...

266

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

132014 2:06:55 PM" "Back to Contents","Data 1: Liquefied U.S. Natural Gas Exports to China (MMcf)" "Sourcekey","NGMEPG0ENGNUS-NCHMMCF" "Date","Liquefied U.S. Natural Gas...

267

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

2:08:12 PM" "Back to Contents","Data 1: Alaska Liquefied Natural Gas Exports Price to China (Dollars per Thousand Cubic Feet)" "Sourcekey","NGMEPG0PNGSAK-NCHDMCF"...

268

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,,"(202) 586-8800",,,"11252013 9:01:19 AM" "Back to Contents","Data 1: Total Crude Oil and Products Imports from All Countries" "Sourcekey","MTTIPP11","MTTIPP21","MTTIPP31",...

269

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"9302013 5:41:31 AM" "Back to Contents","Data 1:...

270

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"9302013 6:13:51 AM" "Back to Contents","Data 1:...

271

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

,,"(202) 586-8800",,,"172014 2:58:22 PM" "Back to Contents","Data 1: Federal Offshore--Gulf of Mexico Natural Gas Gross Withdrawals (MMcf)" "Sourcekey","N9010FX2"...

272

Gluonic profile of the static baryon at finite temperature  

E-Print Network (OSTI)

The gluon flux distribution of a static three quark system has been revealed at finite temperature in the pure SU(3) Yang-Mills theory. An action density operator is correlated with three Polyakov loops representing the baryonic state at a temperatures near the end of the QCD plateau, T/T_c = 0.8, and another just before the deconfinement point, T/T_c = 0.9. The flux distributions at short distance separations between the quarks display an action-density profile consistent with a filled Delta shape iso-surface. However the Delta-shaped action iso-surface distributions are found to persist even at large inter-quark separations for both temperatures. The action density distribution in the quark plane exhibits a nonuniform pattern for all quark separations considered. This result contrasts the well-known Y-shaped uniform action density gluonic-flux profile obtained using the Wilson-loop as a quark source operator at zero temperature. We systematically measure and compare the main aspects of the profile of the flux distribution at the two considered temperature scales for three sets of isosceles triangle quark configurations. The radii, amplitudes and rate of change of the width of the flux distribution are found to reverse their behavior as the temperature increase from the end of the QCD plateau region towards the deconfinement point. Remarkably, we find the mean square width of the flux distribution shrinks and localizes for quark separations larger than 1.0 fm at T/T_c = 0.8 which results in an identifiable Y-shaped radius profile. Near the deconfinement point, the action-density delocalizes and the width broadens linearly at large quark separations.

Ahmed S. Bakry; Derek B. Leinweber; Anthony G. Williams

2011-07-01T23:59:59.000Z

273

The Effect of Vector Meson Decays on Dihadron Fragmentation Functions  

E-Print Network (OSTI)

Dihadron Fragmentation Functions (DFF) provide a vast amount of information on the intricate details of the parton hadronization process. Moreover, they provide a unique access to the "clean" extraction of nucleon transversity parton distribution functions in semi inclusive deep inelastic two hadron production process with a transversely polarised target. On the example of the u \\to \\pi^+ \\pi^-, we analyse the properties of unpolarised DFFs using their probabilistic interpretation. We use both the NJL-jet hadronization model and PYTHIA 8.1 event generator to explore the effect of the strong decays of the vector mesons produced in the quark hadronization process on the pseudoscalar DFFs. Our study shows that, even though it is less probable to produce vector mesons in the hadronization process than pseudo scalar mesons of the same charge, the products of their strong decays drastically affect the DFFs for pions because of the large combinatorial factors. Thus, an accurate description of both vector meson production and decays are crucial for theoretical understanding of DFFs.

Hrayr H. Matevosyan; Anthony W. Thomas; Wolfgang Bentz

2013-07-30T23:59:59.000Z

274

Study of scalar mesons in chiral Lagrangian frameworks  

E-Print Network (OSTI)

sigma model the pseudoscalar and scalar mesons appear together since the model is constructed from the 3× 3 matrix field M = S + i?, (9) where S = S† represents a scalar nonet and ? = ?† a pseudoscalar nonet. Under a chiral transformation qL ? ULqL, qR...

Black, Deirdre; Gaunt, Jonathan R

275

Light Vector Mesons from dAu in PHENIX  

E-Print Network (OSTI)

A first measurement of the e+e-decay rate of phi mesons in dAu collisions from the PHENIX detector at RHIC and its comparison to the K+K- decay channel is described. The comparison of the two decay channels can be sensitive to chiral symmetry restoration.

Richard Seto

2004-04-01T23:59:59.000Z

276

CEDR Content  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

CEDR Content" CEDR Content" "The Consolidated Energy Data Report (CEDR) consists of 27 worksheets that should be completed by each site, as applicable, and included as part each site's SSP in a MS Excel electronic format. The CEDR is due to the SPO no later than December 9th." "Worksheet",,"Overview","Action" 1.1,"Content","Stand-alone overview of the CEDR tabs.","None" 2.1,"Funds, Meters, Training","Collects information on energy and water spending, and metering status.","If applicable, complete cells highlighted in orange. Edited and new data cells should be highlighted in light blue." 3.1,"BTU & Gal Key","Reference tab containing all factors and dropdown menu information for all tabs starting with ""3"". If you need to divide up the CEDR, please keep all tabs starting with ""3"" together to ensure calculation links are not broken. ","None"

277

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Workbook Contents" Workbook Contents" ,"U.S. State-to-State capacity" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","Units of Measurement","Frequency","Updated Date" ,"Pipeline State-to-State Capacity","State-to-State capacity","Million cubic feet per day (MMcf/d)","Quarterly","application/vnd.ms-excel" ,"State Inflow Capacity","Inflow capacity from other States","Million cubic feet per day (MMcf/d)","Quarterly","application/vnd.ms-excel" ,"State Outflow Capacity","Outflow capacity to other States","Million cubic feet per day (MMcf/d)","Quarterly","application/vnd.ms-excel"

278

Baryon Resonances in the Double Pion Channel at Jefferson Lab (CEBAF): Experimental and Physical Analysis Status and Perspectives  

E-Print Network (OSTI)

Decay of light quark excited baryons in the double pion channel is discussed, as a particular way of investigating poorly know baryon resonances and searching for "missing states" predicted by quark models. A possible approach to the data analysis is discussed and some preliminary data from the CLAS collaboration at Jefferson Laboratory are presented.

Marco Ripani

1999-02-18T23:59:59.000Z

279

Exotic State Searches at the SPring-8: Observation of a Pentaquark State Theta^+ Baryon  

E-Print Network (OSTI)

A narrow resonance peak was observed at 1.54 +/- 0.01 GeV as an exotic baryon with strangeness S = +1 in the gamma + n going to K^+ + K^- + n reaction on Carbon. The new state have a width smaller than 0.025 GeV and a Gaussian significance of 4.6 sigma. It can not be interpreted as three quark state and is consistent with the lightest member of an antidecuplet of baryons predicted by the chiral soliton model.

Yuji Ohashi

2004-02-02T23:59:59.000Z

280

Rotational-vibrational coupling in the BPS Skyrme model of baryons  

E-Print Network (OSTI)

We calculate the rotational-vibrational spectrum in the BPS Skyrme model for the hedgehog skyrmion with baryon number one. The resulting excitation energies for the nucleon and delta Roper resonances are slightly above their experimental values. Together with the fact that in the standard Skyrme model these excitation energies are significantly lower than the experimental ones, this provides strong evidence for the conjecture that the inclusion of the BPS Skyrme model is necessary for a successful quantitative description of physical properties of baryons and nuclei.

Adam, C; Sanchez-Guillen, J; Wereszczynski, A

2013-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "mesons contents baryons" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


281

CEBAF-TH-93-18 Quasi-Two-Body Decays of Nonstrange Baryons  

E-Print Network (OSTI)

(1440)?, and ?2 (1600)?, in a relativized pair-creation ( 3P0) model which has been developed in a previous study of the N? decays of the same baryon states. As it is our goal to provide a guide for the possible discovery of new baryon states at CEBAF and elsewhere, we examine the decays of resonances which have already been seen in the partial-wave analyses, along with those of states which are predicted by the quark model but which remain undiscovered. The level of agreement between our calculation and the available widths from the partial-wave analyses is encouraging. Typeset Using REVTEX

Simon Capstick; Winston Roberts

1993-01-01T23:59:59.000Z

282

Electric properties of the baryon anti-decuplet in the SU(3) chiral quark-soliton model  

E-Print Network (OSTI)

We investigate the electric form factors and charge radii of the pentaquark baryons within the framework of the chiral quark-soliton model. We consider the rotational $1/N_c$ and linear $m_s$ corrections, assuming isospin symmetry and employing the symmetry-conserving quantization. The flavor-decomposed charge densities of the $\\Theta^+$ are presented. The electric form factors and charge radii of the charged pentaquark baryons turn out to be very similar to those of the corresponding octet baryons. The charge radii of the neutral pentaquark baryons are obtained to be very tiny and positive. The strange electric form factor of the pentaquark proton is shown to be larger than the corresponding one of the proton by around 20%. We also present the charge radii of the baryon decuplet for comparison.

Tim Ledwig; Hyun-Chul Kim; Antonio Silva; Klaus Goeke

2006-03-16T23:59:59.000Z

283

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

586-8800",,,"12122013 6:56:58 PM" "Back to Contents","Data 1: U.S. Liquefied Natural Gas Imports by Point of Entry " "Sourcekey","N9103US2","NGAEPG0IMLYCAM-Z00MMCF","NAEP...

284

POLICY CONTENT  

E-Print Network (OSTI)

March 31, 1999. It lists in alphabetical order the National Customs Rulings (NCR) that were made since the Memorandum was published. 2. Appendix B – Supplement 1 is a supplement to Appendix B of Memorandum D11-11-2. It presents the policy content of the more recent NCRs, which are listed by numerical order of tariff items for greater ease of reference.

Um D; National Customs Rulings (ncrs

1999-01-01T23:59:59.000Z

285

Observation of the Omega(b)- Baryon and Measurement of the Properties of the Xi(b)- and Omega(b)- Baryons  

SciTech Connect

The authors report the observation of the bottom, doubly-strange baryon {Omega}{sub b}{sup -} through the decay chain {Omega}{sub b}{sup -} {yields} J/{psi}{Omega}{sup -}, where J/{psi} {yields} {mu}{sup +} {mu}{sup -}, {Omega}{sup -} {yields} {Lambda}K{sup -}, and {Lambda} {yields} p {pi}{sup -}, using 4.2 fb{sup -1} of data from p{bar p} collisions at {radical}s = 1.96 TeV, and recorded with the Collider Detector at Fermilab. A signal is observed whose probability of arising from a background fluctuation is 4.0 x 10{sup -8}, or 5.5 Gaussian standard deviations. The {Omega}{sub b}{sup -} mass is measured to be 6054.4 {+-} 6.8(stat.) {+-} 0.9(syst.) MeV/c{sup 2}. The lifetime of the {Omega}{sub b}{sup -} baryon is measured to be 1.13{sub -0.40}{sup +0.53}(stat.) {+-} 0.02(syst.) ps. In addition, for the {Xi}{sub b}{sup -} baryon they measure a mass of 5790.9 {+-} 2.6(stat.) {+-} 0.8(syst.) MeV/c{sup 2} and a lifetime of 1.56{sub -0.25}{sup +0.27}(stat.) {+-} 0.02(syst.) ps.

Aaltonen, T.; /Helsinki Inst. of Phys.; Adelman, Jahred A.; /Chicago U., EFI; Akimoto, T.; /Tsukuba U.; Alvarez Gonzalez, B.; /Cantabria Inst. of Phys.; Amerio, S.; /INFN, Padua; Amidei, Dante E.; /Michigan U.; Anastassov, A.; /Northwestern U.; Annovi, Alberto; /Frascati; Antos, Jaroslav; /Comenius U.; Apollinari, G.; /Fermilab; Apresyan, A.; /Purdue U. /Waseda U.

2009-05-01T23:59:59.000Z

286

Evidence for new nucleon resonances from electromagnetic meson production  

Science Conference Proceedings (OSTI)

The study of nucleon resonances in electromagnetic meson production with the CLAS detector is discussed. The electromagnetic interaction is complementary to pion scattering in the exploration of the nucleon excitation spectrum. Higher mass states often decouple from the N{pi} channel and are not seen in {pi} N --> {pi} N. Photoproduction of mesons, such as K {Lambda}, {omega} p and {eta}' p may be more sensitive to many of these states. The CLAS detector, combined with the use of energy-tagged polarized photons and polarized electrons, as well as po- larized targets and the measurement of recoil polarization, are the tools needed for a comprehensive nucleon resonance program. Some of the recently published high statistics data sets had significant impact on further clarifying the nucleon excitation spectrum.

Volker Burkert

2012-12-01T23:59:59.000Z

287

Meson Photoproduction off the Deuteron and off {sup 3}He  

SciTech Connect

Photoproduction of mesons off the deuteron and He nuclei has been studied at the tagged photon facilities of the Bonn ELSA accelerator and the Mainz MAMI accelerator with the Crystal/ setup (Mainz). Meson photoproduction off the neutron has been investigated for different final states ({pi}{sup o}, {pi}{sup o} {pi}{sup o}, {pi}{sup o} {pi}{sup -}, {eta}, {eta}{sup '}, {eta}{pi}{sup o}). A surprising finding was a narrow structure in the {gamma}n{yields}n{eta} excitation function, which is not seen in the proton case. Photoproduction off {sup 3}He has provided further evidence for the formation of an h-mesic state.

Krusche, B. [Department of Physics, University of Basel, Klingelbergstrasse. 82 Basel (Switzerland)

2010-08-05T23:59:59.000Z

288

Dynamical instabilities of warm npe matter: {delta} meson effects  

Science Conference Proceedings (OSTI)

The effects of {delta} mesons on the dynamical instabilities of cold and warm nuclear and stellar matter at subsaturation densities are studied in the framework of relativistic mean-field hadron models (NL3, NL{rho}, and NL{rho}{delta}) with the inclusion of the electromagnetic field. The distillation effect and the spinodals for all the models considered are discussed. The crust-core transition density and pressure are obtained as a function of temperature for {beta}-equilibrium matter with and without neutrino trapping. An estimation of the size of the clusters formed in the nonhomogeneous phase and the corresponding growth rates are made. It is shown that cluster sizes increase with temperature. The effects of the {delta} meson on the instability region are larger for low temperatures, very asymmetric matter, and densities close to the spinodal surface. It increases the distillation effect above {approx}0.4{rho}{sub 0} and has the opposite effect below that density.

Pais, Helena; Santos, Alexandre; Providencia, Constanca [Centro de Fisica Computacional, Department of Physics, University of Coimbra, 3004-516 Coimbra (Portugal)

2009-10-15T23:59:59.000Z

289

Static-light mesons on a dynamical anisotropic lattice  

E-Print Network (OSTI)

We present results for the spectrum of static-light mesons from Nf=2 lattice QCD. These results were obtained using all-to-all light quark propagators on an anisotropic lattice, yielding an improved signal resolution when compared to more conventional lattice techniques. In particular, we consider the inversion of orbitally-excited multiplets with respect to the `standard ordering', which has been predicted by some quark models.

Justin Foley; Alan O Cais; Mike Peardon; Sinead M Ryan

2006-10-09T23:59:59.000Z

290

Symposium Summary and Outlook: Twenty Years of Meson Factory Physics  

E-Print Network (OSTI)

The opening of the meson factories twenty years ago provided nuclear physics with new beams, higher momentum transfers, and new opportunities for precision measurements. The resulting changes in nuclear physics were substantial, altering not only the range of physics issues identified with the field but also the manner and size of the collaborations that do nuclear physics. Inspired by the talks of this symposium, I discuss some of the accomplishments as well as some of the goals not yet reached.

W. C. Haxton

1997-04-24T23:59:59.000Z

291

A calculation of the QCD phase diagram at finite temperature, and baryon and isospin chemical potentials  

E-Print Network (OSTI)

We study the phases of a two-flavor Nambu-Jona-Lasinio model at finite temperature $T$, baryon and isospin chemical potentials: $\\mu_{B}=(\\mu_{u}+\\mu_{d})/2$, $\\mu_{I}=(\\mu_{u}-\\mu_{d})/2$. This study completes a previous analysis where only small isospin chemical potentials $\\mu_{I}$ were considered

A. Barducci; R. Casalbuoni; G. Pettini; L. Ravagli

2004-02-10T23:59:59.000Z

292

Baryonic triplet P-wave dominant superfluidity under combined pion condensation with delta-mixing  

E-Print Network (OSTI)

We study baryonic superfluidity under the combined pion condensation with delta-mixing, where both condensates of the neutral and charged pions take place in neutron stars. Outline of formulation treating such superfluidity is presented and energy gap calculations show the possibility that critical temperatures are higher than about 1x10^9 K.

R. Tamagaki; T. Takatsuka

2005-11-28T23:59:59.000Z

293

Production of spin-3 mesons in diffractive DIS  

E-Print Network (OSTI)

We calculate the amplitudes of J^{PC}=3^{--} meson production in diffractive DIS within the k_t-factorization approach, with a particular attention paid to the rho_3(1690) meson. We find that at all Q^2 the rho_3(1690) production cross section is 2-5 times smaller than the rho(1700) production cross section, which is assumed to be a pure D-wave state. Studying sigma_L and sigma_T separately, we observe domination of rho_3 in sigma_L and domination of rho(1700) in sigma_T and offer an explanation of this behavior in simple terms. We also find very strong contributions -- sometimes even domination -- of the s-channel helicity violating amplitudes. The typical color dipole sizes probed in rho_3 production are shown to be larger than those in the ground state rho production, and the energy dependence of rho_3 cross section turns out to be much flatter than the rho production cross section. All the conclusions about the relative behavior of rho_3(1690) and rho(1700) mesons are numerically stable against variations of input parameters.

F. Caporale; I. P. Ivanov

2005-04-16T23:59:59.000Z

294

Eta(547) and Eta(958) Meson Photoproduction on the Proton  

DOE Green Energy (OSTI)

Photoproduction of {eta} and {eta}{prime} mesons has been studied at the Continuous Electron Beam Accelerator Facility (CEBAF) Large Acceptance Spectrometer (CLAS) using a tagged photon beam incident on a hydrogen target with photon energies from the respective production thresholds up to 2.4 GeV. The photoproduced mesons were identified via missing mass reconstruction using recoil proton momentum and time of flight information. Data were obtained in a range of {radical}s from threshold to 2.2 GeV for each meson. In this study, differential cross-section measurements for the {gamma}p {yields} p{eta} and {gamma}p {yields} p{eta}{prime} reactions are presented, and the results compared to recent data. An isobar analysis of the differential cross-sections is performed. The predicted differential cross-sections from the isobar analysis are used to predict behavior in unmeasured regions of phase space, and to infer total cross sections. For the {gamma}p {yields} p{eta} reaction, a value of the S{sub 11}(1535) proton helicity amplitude also was extracted and compared to recent analyses. The data presented greatly extends the energy and angle coverage for differential cross-sections of {eta} photoproduction, and significantly improves the accuracy with which {eta}{prime} cross sections are known.

Michael Dugger

2001-12-01T23:59:59.000Z

295

Meson production in two-photon interactions at energies available at CERN Large Hadron Collider  

E-Print Network (OSTI)

The meson production cross sections are estimated considering photon-photon interactions in hadron - hadron collisions at CERN LHC energies. We consider a large number of mesons with photon-photon partial decay width well constrained by the experiment and some mesons which are currently considered as hadronic molecule and glueball candidates. Our results demonstrate that the experimental analysis of these states is feasible at CERN - LHC.

V. P. Goncalves; D. T. da Silva; W. K. Sauter

2012-09-04T23:59:59.000Z

296

Marriage à-la-MOND: Baryonic dark matter in galaxy clusters and the cooling flow puzzle  

E-Print Network (OSTI)

I start with a brief introduction to MOND phenomenology and its possible roots in cosmology--a notion that may turn out to be the most far reaching aspect of MOND. Next I discuss the implications of MOND for the dark matter (DM) doctrine: MOND's successes imply that baryons determine everything. For DM this would mean that the puny tail of leftover baryons in galaxies wags the hefty DM dog. This has to occur in many intricate ways, and despite the haphazard construction history of galaxies--a very tall order. I then concentrate on galaxy clusters in light of MOND, which still requires some yet undetected cluster dark matter, presumably in some baryonic form (CBDM). This CBDM might contribute to the heating of the x-ray emitting gas and thus alleviate the cooling-flow puzzle. MOND, qua theory of dynamics, does not directly enter the microphysics of the gas; however, it does force a new outlook on the role of DM in shaping the cluster gasdynamics: MOND tells us that the cluster DM is not cold dark matter, is not so abundant, and is not expected in galaxies; it is thus not subject to constraints on baryonic DM in galaxies. The mass in CBDM required in a whole cluster is, typically, similar to that in hot gas, but is rather more centrally concentrated, totally dominating the core. The CBDM contribution to the baryon budget in the universe is thus small. Its properties, deduced for isolated clusters, are consistent with the observations of the ``bullet cluster''. Its kinetic-energy reservoir is much larger than that of the hot gas in the core, and would suffice to keep the gas hot for many cooling times. Heating can be effected in various ways depending on the exact nature of the CBDM, from very massive black holes to cool, compact gas clouds.

Mordehai Milgrom

2007-12-27T23:59:59.000Z

297

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","ngm_epg0_fgc_sky_mmcfa.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/ngm_epg0_fgc_sky_mmcfa.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:59:11 AM" "Back to Contents","Data 1: Kentucky Natural Gas Gross Withdrawals from Coalbed Wells (MMcf) " "Sourcekey","NGM_EPG0_FGC_SKY_MMCF" "Date","Kentucky Natural Gas Gross Withdrawals from Coalbed Wells (MMcf) "

298

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040ks2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040ks2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:36 AM" "Back to Contents","Data 1: Kansas Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040KS2" "Date","Kansas Natural Gas Vented and Flared (MMcf)" 35079,63 35110,63 35139,63 35170,61 35200,62 35231,57 35261,57 35292,55 35323,56

299

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040nv2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040nv2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:41 AM" "Back to Contents","Data 1: Nevada Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040NV2" "Date","Nevada Natural Gas Vented and Flared (MMcf)" 33253,0 33284,0 33312,0 33343,0 33373,0 33404,0 33434,0 33465,0 33496,0 33526,0

300

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040ms2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040ms2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:38 AM" "Back to Contents","Data 1: Mississippi Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040MS2" "Date","Mississippi Natural Gas Vented and Flared (MMcf)" 35079,217 35110,199 35139,223 35170,219 35200,237 35231,234 35261,239

Note: This page contains sample records for the topic "mesons contents baryons" from the National Library of EnergyBeta (NLEBeta).
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301

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9103us3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9103us3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/13/2013 3:54:18 PM" "Back to Contents","Data 1: Price of U.S. Natural Gas LNG Imports (Dollars per Thousand Cubic Feet)" "Sourcekey","N9103US3" "Date","Price of U.S. Natural Gas LNG Imports (Dollars per Thousand Cubic Feet)" 31228,4.6 31593,4.62 32324,2.71

302

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9130us3m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9130us3m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/13/2013 2:23:24 PM" "Back to Contents","Data 1: Price of U.S. Natural Gas Exports (Dollars per Thousand Cubic Feet)" "Sourcekey","N9130US3" "Date","Price of U.S. Natural Gas Exports (Dollars per Thousand Cubic Feet)" 32523,2.69 32554,2.4

303

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040tx2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040tx2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:44 AM" "Back to Contents","Data 1: Texas Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040TX2" "Date","Texas Natural Gas Vented and Flared (MMcf)" 24653,129403 25019,124584 25384,111499 25749,100305 26114,70222 26480,59821 26845,36133 27210,34431

304

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010al2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010al2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:07 PM" "Back to Contents","Data 1: Alabama Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010AL2" "Date","Alabama Natural Gas Residential Consumption (MMcf)" 24653,45543 25019,51708 25384,54804 25749,55779 26114,54867 26480,53397 26845,55685

305

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010mi2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010mi2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:33 PM" "Back to Contents","Data 1: Michigan Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010MI2" "Date","Michigan Natural Gas Residential Consumption (MMcf)" 24653,302472 25019,315694 25384,333264 25749,340033 26114,343773 26480,355266

306

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010co3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010co3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:12 PM" "Back to Contents","Data 1: Colorado Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010CO3" "Date","Colorado Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

307

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010wa3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010wa3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:05 PM" "Back to Contents","Data 1: Washington Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010WA3" "Date","Washington Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

308

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ak2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ak2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:05 PM" "Back to Contents","Data 1: Alaska Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010AK2" "Date","Alaska Natural Gas Residential Consumption (MMcf)" 24653,1958 25019,2293 25384,4573 25749,6211 26114,6893 26480,8394 26845,5024

309

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ar2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ar2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:08 PM" "Back to Contents","Data 1: Arkansas Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010AR2" "Date","Arkansas Natural Gas Residential Consumption (MMcf)" 24653,52777 25019,56346 25384,58322 25749,59792 26114,48737 26480,47387

310

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2010 Annual",2010 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040ok2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040ok2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:42 AM" "Back to Contents","Data 1: Oklahoma Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040OK2" "Date","Oklahoma Natural Gas Vented and Flared (MMcf)" 24653,126629 25019,129408 25384,130766 25749,129629 26114,39799 26480,38797 26845,36411

311

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3020us4m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3020us4m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:23:38 PM" "Back to Contents","Data 1: Percent of Commercial Natural Gas Deliveries in U.S. Total Represented by the Price (%)" "Sourcekey","N3020US4" "Date","Percent of Commercial Natural Gas Deliveries in U.S. Total Represented by the Price (%)"

312

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ak3m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ak3m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:06 PM" "Back to Contents","Data 1: Alaska Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010AK3" "Date","Alaska Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

313

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ca3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ca3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:11 PM" "Back to Contents","Data 1: California Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010CA3" "Date","California Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

314

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040la2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040la2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:37 AM" "Back to Contents","Data 1: Louisiana Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040LA2" "Date","Louisiana Natural Gas Vented and Flared (MMcf)" 33253,1788 33284,1684 33312,1571 33343,1593 33373,1807 33404,1690 33434,2042

315

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040tn2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040tn2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:44 AM" "Back to Contents","Data 1: Tennessee Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040TN2" "Date","Tennessee Natural Gas Vented and Flared (MMcf)" 33253,0 33284,0 33312,0 33343,0 33373,0 33404,0 33434,0 33465,0 33496,0

316

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010wi2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010wi2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:06 PM" "Back to Contents","Data 1: Wisconsin Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010WI2" "Date","Wisconsin Natural Gas Residential Consumption (MMcf)" 24653,90994 25019,93425 25384,101124 25749,105208 26114,109758 26480,104648

317

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3020us4a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3020us4a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:23:38 PM" "Back to Contents","Data 1: Percent of Commercial Natural Gas Deliveries in U.S. Total Represented by the Price (%)" "Sourcekey","N3020US4" "Date","Percent of Commercial Natural Gas Deliveries in U.S. Total Represented by the Price (%)"

318

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010nh3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010nh3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:43 PM" "Back to Contents","Data 1: New Hampshire Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010NH3" "Date","New Hampshire Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

319

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010in2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010in2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:24 PM" "Back to Contents","Data 1: Indiana Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010IN2" "Date","Indiana Natural Gas Residential Consumption (MMcf)" 24653,139519 25019,145955 25384,156699 25749,158699 26114,162747 26480,169267

320

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3020ct3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3020ct3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:23 PM" "Back to Contents","Data 1: Connecticut Price of Natural Gas Sold to Commercial Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3020CT3" "Date","Connecticut Price of Natural Gas Sold to Commercial Consumers (Dollars per Thousand Cubic Feet)"

Note: This page contains sample records for the topic "mesons contents baryons" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


321

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010mo3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010mo3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:36 PM" "Back to Contents","Data 1: Missouri Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010MO3" "Date","Missouri Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

322

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040la2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040la2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:36 AM" "Back to Contents","Data 1: Louisiana Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040LA2" "Date","Louisiana Natural Gas Vented and Flared (MMcf)" 24653,161849 25019,166439 25384,158852 25749,154089 26114,103564 26480,63667 26845,102091

323

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040ut2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040ut2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:46 AM" "Back to Contents","Data 1: Utah Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040UT2" "Date","Utah Natural Gas Vented and Flared (MMcf)" 34592,646 34834,696 34865,4590 34895,4767 34926,4382 34957,4389 34987,4603 35018,4932

324

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010az2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010az2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:09 PM" "Back to Contents","Data 1: Arizona Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010AZ2" "Date","Arizona Natural Gas Residential Consumption (MMcf)" 24653,25376 25019,26681 25384,28426 25749,29679 26114,32619 26480,34259 26845,36280

325

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ak3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ak3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:06 PM" "Back to Contents","Data 1: Alaska Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010AK3" "Date","Alaska Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

326

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9132us3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9132us3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/13/2013 2:23:27 PM" "Back to Contents","Data 1: Price of U.S. Natural Gas Pipeline Exports (Dollars per Thousand Cubic Feet)" "Sourcekey","N9132US3" "Date","Price of U.S. Natural Gas Pipeline Exports (Dollars per Thousand Cubic Feet)" 31228,3.92 31593,2.35

327

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010id3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010id3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:23 PM" "Back to Contents","Data 1: Idaho Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010ID3" "Date","Idaho Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

328

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010me2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010me2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:32 PM" "Back to Contents","Data 1: Maine Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010ME2" "Date","Maine Natural Gas Residential Consumption (MMcf)" 24653,3967 25019,3571 25384,4910 25749,5247 26114,5591 26480,6036 26845,6027 27210,6174

329

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ne3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ne3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:42 PM" "Back to Contents","Data 1: Nebraska Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010NE3" "Date","Nebraska Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

330

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040wy2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040wy2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:47 AM" "Back to Contents","Data 1: Wyoming Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040WY2" "Date","Wyoming Natural Gas Vented and Flared (MMcf)" 24653,1498 25019,13038 25384,17632 25749,18419 26114,3860 26480,8376 26845,6618 27210,6102

331

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010mn3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010mn3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:34 PM" "Back to Contents","Data 1: Minnesota Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010MN3" "Date","Minnesota Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

332

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ca2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ca2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:10 PM" "Back to Contents","Data 1: California Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010CA2" "Date","California Natural Gas Residential Consumption (MMcf)" 24653,522122 25019,517636 25384,562127 25749,552544 26114,630998 26480,637289

333

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040sd2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040sd2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:43 AM" "Back to Contents","Data 1: South Dakota Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040SD2" "Date","South Dakota Natural Gas Vented and Flared (MMcf)" 33253,384 33284,350 33312,382 33343,380 33373,382 33404,376 33434,405

334

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040nm2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040nm2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:41 AM" "Back to Contents","Data 1: New Mexico Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040NM2" "Date","New Mexico Natural Gas Vented and Flared (MMcf)" 35079,236 35110,220 35139,240 35170,230 35200,241 35231,229 35261,217

335

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010co2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010co2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:11 PM" "Back to Contents","Data 1: Colorado Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010CO2" "Date","Colorado Natural Gas Residential Consumption (MMcf)" 24653,75351 25019,78371 25384,81068 25749,82595 26114,84864 26480,89187

336

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Daily","12/17/2013" Daily","12/17/2013" ,"Release Date:","12/18/2013" ,"Next Release Date:","12/27/2013" ,"Excel File Name:","rngc2d.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngc2d.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/18/2013 12:22:40 PM" "Back to Contents","Data 1: Natural Gas Futures Contract 2 (Dollars per Million Btu)" "Sourcekey","RNGC2" "Date","Natural Gas Futures Contract 2 (Dollars per Million Btu)" 34346,2.13 34347,2.072 34348,2.139 34351,2.196 34352,2.131

337

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ar3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ar3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:08 PM" "Back to Contents","Data 1: Arkansas Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010AR3" "Date","Arkansas Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

338

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040mo2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040mo2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:38 AM" "Back to Contents","Data 1: Missouri Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040MO2" "Date","Missouri Natural Gas Vented and Flared (MMcf)" 33253,0 33284,0 33312,0 33343,0 33373,0 33404,0 33434,0 33465,0 33496,0

339

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Daily","12/17/2013" Daily","12/17/2013" ,"Release Date:","12/18/2013" ,"Next Release Date:","12/27/2013" ,"Excel File Name:","rngc4d.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngc4d.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/18/2013 12:22:29 PM" "Back to Contents","Data 1: Natural Gas Futures Contract 4 (Dollars per Million Btu)" "Sourcekey","RNGC4" "Date","Natural Gas Futures Contract 4 (Dollars per Million Btu)" 34323,1.894 34324,1.83 34325,1.859 34326,1.895 34330,1.965

340

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9010us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9010us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:55:17 AM" "Back to Contents","Data 1: U.S. Natural Gas Gross Withdrawals (MMcf)" "Sourcekey","N9010US2" "Date","U.S. Natural Gas Gross Withdrawals (MMcf)" 26679 26710 26738 26769 26799 26830 26860 26891 26922 26952 26983 27013 27044 27075 27103

Note: This page contains sample records for the topic "mesons contents baryons" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


341

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040ut2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040ut2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:45 AM" "Back to Contents","Data 1: Utah Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040UT2" "Date","Utah Natural Gas Vented and Flared (MMcf)" 24653,3000 25019,2906 25384,2802 25749,2852 26114,2926 26480,5506 26845,7664 27210,5259 27575,1806

342

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ak2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ak2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:06 PM" "Back to Contents","Data 1: Alaska Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010AK2" "Date","Alaska Natural Gas Residential Consumption (MMcf)" 32523,1793 32554,2148 32582,1566 32613,1223 32643,858 32674,638

343

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040nd2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040nd2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:39 AM" "Back to Contents","Data 1: North Dakota Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040ND2" "Date","North Dakota Natural Gas Vented and Flared (MMcf)" 24653,25795 25019,22050 25384,22955 25749,19862 26114,2686 26480,20786 26845,22533

344

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010al3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010al3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:07 PM" "Back to Contents","Data 1: Alabama Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010AL3" "Date","Alabama Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

345

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ar3m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ar3m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:09 PM" "Back to Contents","Data 1: Arkansas Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010AR3" "Date","Arkansas Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

346

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010va2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010va2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:02 PM" "Back to Contents","Data 1: Virginia Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010VA2" "Date","Virginia Natural Gas Residential Consumption (MMcf)" 24653,41495 25019,43582 25384,46663 25749,49554 26114,49488 26480,55427

347

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040co2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040co2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:33 AM" "Back to Contents","Data 1: Colorado Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040CO2" "Date","Colorado Natural Gas Vented and Flared (MMcf)" 35079,112 35110,77 35139,78 35170,91 35200,100 35231,89 35261,100 35292,106

348

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ga2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ga2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:17 PM" "Back to Contents","Data 1: Georgia Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010GA2" "Date","Georgia Natural Gas Residential Consumption (MMcf)" 24653,80322 25019,84072 25384,87878 25749,87359 26114,88319 26480,85256 26845,86191

349

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3020hi2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3020hi2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:33 PM" "Back to Contents","Data 1: Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in Hawaii (MMcf)" "Sourcekey","N3020HI2" "Date","Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in Hawaii (MMcf)"

350

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3020ga2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3020ga2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:31 PM" "Back to Contents","Data 1: Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in Georgia (MMcf)" "Sourcekey","N3020GA2" "Date","Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in Georgia (MMcf)"

351

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3020ar2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3020ar2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:14 PM" "Back to Contents","Data 1: Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in Arkansas (MMcf)" "Sourcekey","N3020AR2" "Date","Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in Arkansas (MMcf)"

352

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ct2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ct2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:12 PM" "Back to Contents","Data 1: Connecticut Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010CT2" "Date","Connecticut Natural Gas Residential Consumption (MMcf)" 24653,26177 25019,26437 25384,29048 25749,31187 26114,31878 26480,32879

353

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010dc3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010dc3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:14 PM" "Back to Contents","Data 1: District of Columbia Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010DC3" "Date","District of Columbia Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

354

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ri3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ri3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:54 PM" "Back to Contents","Data 1: Rhode Island Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010RI3" "Date","Rhode Island Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

355

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010sd3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010sd3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:56 PM" "Back to Contents","Data 1: South Dakota Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010SD3" "Date","South Dakota Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

356

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3020de2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3020de2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:26 PM" "Back to Contents","Data 1: Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in Delaware (MMcf)" "Sourcekey","N3020DE2" "Date","Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in Delaware (MMcf)"

357

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010tn3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010tn3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:58 PM" "Back to Contents","Data 1: Tennessee Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010TN3" "Date","Tennessee Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

358

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ny3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ny3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:48 PM" "Back to Contents","Data 1: New York Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010NY3" "Date","New York Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

359

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010or2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010or2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:51 PM" "Back to Contents","Data 1: Oregon Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010OR2" "Date","Oregon Natural Gas Residential Consumption (MMcf)" 24653,13427 25019,15126 25384,20507 25749,19742 26114,21217 26480,23331 26845,22271

360

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9140us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9140us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:33:47 PM" "Back to Contents","Data 1: U.S. Natural Gas Total Consumption (MMcf)" "Sourcekey","N9140US2" "Date","U.S. Natural Gas Total Consumption (MMcf)" 36906,2676998 36937,2309464 36965,2246633 36996,1807170 37026,1522382 37057,1444378

Note: This page contains sample records for the topic "mesons contents baryons" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


361

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Daily","12/17/2013" Daily","12/17/2013" ,"Release Date:","12/18/2013" ,"Next Release Date:","12/27/2013" ,"Excel File Name:","rngc1d.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngc1d.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/18/2013 12:22:45 PM" "Back to Contents","Data 1: Natural Gas Futures Contract 1 (Dollars per Million Btu)" "Sourcekey","RNGC1" "Date","Natural Gas Futures Contract 1 (Dollars per Million Btu)" 34347,2.194 34348,2.268 34351,2.36 34352,2.318 34353,2.252

362

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010fl3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010fl3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:16 PM" "Back to Contents","Data 1: Florida Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010FL3" "Date","Florida Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

363

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3035us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3035us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:25:08 PM" "Back to Contents","Data 1: U.S. Natural Gas Industrial Consumption (MMcf)" "Sourcekey","N3035US2" "Date","U.S. Natural Gas Industrial Consumption (MMcf)" 36906,686540 36937,640026 36965,664918 36996,622054 37026,576532 37057,536820

364

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040fl2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040fl2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:34 AM" "Back to Contents","Data 1: Florida Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040FL2" "Date","Florida Natural Gas Vented and Flared (MMcf)" 26114,355 26480,284 27941,837 28306,607 29402,677 29767,428 30132,435 30497,198 30863,34

365

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ok2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ok2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:50 PM" "Back to Contents","Data 1: Oklahoma Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010OK2" "Date","Oklahoma Natural Gas Residential Consumption (MMcf)" 24653,67395 25019,74782 25384,75310 25749,77460 26114,75238 26480,77608

366

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040ar2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040ar2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:31 AM" "Back to Contents","Data 1: Arkansas Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040AR2" "Date","Arkansas Natural Gas Vented and Flared (MMcf)" 24653,997 25019,895 25384,1326 25749,226 26114,1734 26480,2649 26845,1947 27210,1716 27575,1318

367

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010me3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010me3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:32 PM" "Back to Contents","Data 1: Maine Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010ME3" "Date","Maine Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

368

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3060us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3060us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:27:25 PM" "Back to Contents","Data 1: Natural Gas Delivered to Consumers in the U.S. (MMcf)" "Sourcekey","N3060US2" "Date","Natural Gas Delivered to Consumers in the U.S. (MMcf)" 36906,2505011 36937,2156873 36965,2086568 36996,1663832

369

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010us2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010us2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:00 PM" "Back to Contents","Data 1: U.S. Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010US2" "Date","U.S. Natural Gas Residential Consumption (MMcf)" 11139,295700 11504,294406 11870,298520 12235,283197 12600,288236 12965,313498 13331,343346

370

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010in3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010in3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:25 PM" "Back to Contents","Data 1: Indiana Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010IN3" "Date","Indiana Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

371

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9011us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9011us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:55:36 AM" "Back to Contents","Data 1: U.S. Natural Gas Gross Withdrawals from Gas Wells (MMcf)" "Sourcekey","N9011US2" "Date","U.S. Natural Gas Gross Withdrawals from Gas Wells (MMcf)" 33253,1482053 33526,1363737 33984,1452098 34015,1305490

372

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3020us3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3020us3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:23:37 PM" "Back to Contents","Data 1: U.S. Price of Natural Gas Sold to Commercial Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3020US3" "Date","U.S. Price of Natural Gas Sold to Commercial Consumers (Dollars per Thousand Cubic Feet)"

373

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010nv3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010nv3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:46 PM" "Back to Contents","Data 1: Nevada Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010NV3" "Date","Nevada Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

374

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9133us3m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9133us3m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/13/2013 2:23:31 PM" "Back to Contents","Data 1: Price of Liquefied U.S. Natural Gas Exports (Dollars per Thousand Cubic Feet)" "Sourcekey","N9133US3" "Date","Price of Liquefied U.S. Natural Gas Exports (Dollars per Thousand Cubic Feet)"

375

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010sc3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010sc3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:55 PM" "Back to Contents","Data 1: South Carolina Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010SC3" "Date","South Carolina Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

376

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010vt2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010vt2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:03 PM" "Back to Contents","Data 1: Vermont Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010VT2" "Date","Vermont Natural Gas Residential Consumption (MMcf)" 29402,1301 29767,1290 30132,1278 30497,1252 30863,1352 31228,1456 31593,1595

377

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Weekly","12/13/2013","1/10/1997" Weekly","12/13/2013","1/10/1997" ,"Data 2","Futures Prices",4,"Weekly","12/13/2013","12/24/1993" ,"Release Date:","12/18/2013" ,"Next Release Date:","12/27/2013" ,"Excel File Name:","ng_pri_fut_s1_w.xls" ,"Available from Web Page:","http://www.eia.gov/dnav/ng/ng_pri_fut_s1_w.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.gov" ,,"(202) 586-8800",,,"12/18/2013 12:22:18 PM" "Back to Contents","Data 1: Spot Price" "Sourcekey","RNGWHHD" "Date","Weekly Henry Hub Natural Gas Spot Price (Dollars per Million Btu)"

378

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040in2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040in2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:35 AM" "Back to Contents","Data 1: Indiana Natural Gas Vented and Flared (Million Cubic Feet)" "Sourcekey","N9040IN2" "Date","Indiana Natural Gas Vented and Flared (Million Cubic Feet)" 33253,0 33284,0 33312,0 33343,0 33373,0

379

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3020ga3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3020ga3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:32 PM" "Back to Contents","Data 1: Georgia Price of Natural Gas Sold to Commercial Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3020GA3" "Date","Georgia Price of Natural Gas Sold to Commercial Consumers (Dollars per Thousand Cubic Feet)"

380

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010hi3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010hi3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:20 PM" "Back to Contents","Data 1: Hawaii Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010HI3" "Date","Hawaii Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

Note: This page contains sample records for the topic "mesons contents baryons" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


381

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ks2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ks2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:26 PM" "Back to Contents","Data 1: Kansas Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010KS2" "Date","Kansas Natural Gas Residential Consumption (MMcf)" 24653,84912 25019,89372 25384,94320 25749,97317 26114,98644 26480,100720 26845,96468

382

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9100us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9100us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/13/2013 3:53:50 PM" "Back to Contents","Data 1: U.S. Natural Gas Imports (MMcf)" "Sourcekey","N9100US2" "Date","U.S. Natural Gas Imports (MMcf)" 26679,92694 26710,83870 26738,91581 26769,88407 26799,85844 26830,79121 26860,79428 26891,84400 26922,81157

383

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ga3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ga3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:18 PM" "Back to Contents","Data 1: Georgia Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010GA3" "Date","Georgia Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

384

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9133us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9133us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/13/2013 2:23:31 PM" "Back to Contents","Data 1: Liquefied U.S. Natural Gas Exports (MMcf)" "Sourcekey","N9133US2" "Date","Liquefied U.S. Natural Gas Exports (MMcf)" 35445,5604 35476,5596 35504,5675 35535,5660 35565,3812 35596,3786 35626,3756 35657,7532

385

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9170us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9170us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:33:48 PM" "Back to Contents","Data 1: U.S. Natural Gas Pipeline & Distribution Use (MMcf)" "Sourcekey","N9170US2" "Date","U.S. Natural Gas Pipeline & Distribution Use (MMcf)" 36906,76386 36937,65770 36965,63626 36996,50736

386

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","na1504_nus_4a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/na1504_nus_4a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:46:13 PM" "Back to Contents","Data 1: U.S. Natural Gas % of Total Residential - Sales (%)" "Sourcekey","NA1504_NUS_4" "Date","U.S. Natural Gas % of Total Residential - Sales (%)" 32689,99.9 33054,99.2 33419,99.2 33785,99.1 34150,99.1 34515,99.1

387

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ct3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ct3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:13 PM" "Back to Contents","Data 1: Connecticut Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010CT3" "Date","Connecticut Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

388

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010us3m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010us3m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:01 PM" "Back to Contents","Data 1: U.S. Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010US3" "Date","U.S. Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

389

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040fl2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040fl2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:34 AM" "Back to Contents","Data 1: Florida Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040FL2" "Date","Florida Natural Gas Vented and Flared (MMcf)" 35079 35110 35139 35170 35200 35231 35261 35292 35323 35353 35384 35414 35445,0

390

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040mi2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040mi2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:37 AM" "Back to Contents","Data 1: Michigan Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040MI2" "Date","Michigan Natural Gas Vented and Flared (MMcf)" 24653,1861 25019,1120 25384,808 25749,809 26480,1032 26845,1117 27210,1268 27575,1612

391

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ar2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ar2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:08 PM" "Back to Contents","Data 1: Arkansas Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010AR2" "Date","Arkansas Natural Gas Residential Consumption (MMcf)" 32523,6774 32554,7118 32582,6736 32613,3835 32643,1927 32674,1402

392

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010la3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010la3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:29 PM" "Back to Contents","Data 1: Louisiana Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010LA3" "Date","Louisiana Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

393

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9100us3m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9100us3m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/13/2013 3:53:51 PM" "Back to Contents","Data 1: Price of U.S. Natural Gas Imports (Dollars per Thousand Cubic Feet)" "Sourcekey","N9100US3" "Date","Price of U.S. Natural Gas Imports (Dollars per Thousand Cubic Feet)" 32523,1.72 32554,1.88

394

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040ne2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040ne2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:40 AM" "Back to Contents","Data 1: Nebraska Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040NE2" "Date","Nebraska Natural Gas Vented and Flared (MMcf)" 24653,0 25019,0 25384,0 25749,0 26114,1558 26480,1263 26845,834 27210,2137 27575,1398 27941,797

395

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9020us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9020us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:13 AM" "Back to Contents","Data 1: U.S. Natural Gas Repressuring (MMcf)" "Sourcekey","N9020US2" "Date","U.S. Natural Gas Repressuring (MMcf)" 26679 26710 26738 26769 26799 26830 26860 26891 26922 26952 26983 27013 27044 27075 27103 27134 27164

396

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2010 Annual",2010 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040pa2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040pa2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:43 AM" "Back to Contents","Data 1: Pennsylvania Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040PA2" "Date","Pennsylvania Natural Gas Vented and Flared (MMcf)" 24653,0 25019,0 25384,0 25749,0 26114,0 26480,0 26845,0 27210,98 27575,96 27941,99

397

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010oh2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010oh2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:48 PM" "Back to Contents","Data 1: Ohio Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010OH2" "Date","Ohio Natural Gas Residential Consumption (MMcf)" 24653,442360 25019,444964 25384,456414 25749,459972 26114,460820 26480,478331 26845,439212

398

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040ca2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040ca2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:32 AM" "Back to Contents","Data 1: California Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040CA2" "Date","California Natural Gas Vented and Flared (MMcf)" 24653,3565 25019,2780 25384,3074 25749,2499 26114,575 26845,1999 27210,1560 27575,1537

399

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010us3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010us3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:01 PM" "Back to Contents","Data 1: U.S. Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010US3" "Date","U.S. Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

400

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","11/2013" Monthly","11/2013" ,"Release Date:","12/18/2013" ,"Next Release Date:","12/27/2013" ,"Excel File Name:","rngc1m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngc1m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/18/2013 12:22:41 PM" "Back to Contents","Data 1: Natural Gas Futures Contract 1 (Dollars per Million Btu)" "Sourcekey","RNGC1" "Date","Natural Gas Futures Contract 1 (Dollars per Million Btu)" 34349,2.347 34380,2.355 34408,2.109 34439,2.111 34469,1.941

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401

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010az3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010az3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:09 PM" "Back to Contents","Data 1: Arizona Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010AZ3" "Date","Arizona Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

402

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3045us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3045us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:26:13 PM" "Back to Contents","Data 1: U.S. Natural Gas Deliveries to Electric Power Consumers (MMcf)" "Sourcekey","N3045US2" "Date","U.S. Natural Gas Deliveries to Electric Power Consumers (MMcf)" 36906,340292 36937,312843 36965,362843

403

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010pa2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010pa2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:52 PM" "Back to Contents","Data 1: Pennsylvania Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010PA2" "Date","Pennsylvania Natural Gas Residential Consumption (MMcf)" 24653,279817 25019,285978 25384,295027 25749,297022 26114,304327

404

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Bcf)" Bcf)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","# Of Series","Frequency","Latest Data for" ,"Data 1","U.S. Dry Natural Gas Production (Bcf)",1,"Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9070us1m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9070us1m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:33:14 PM" "Back to Contents","Data 1: U.S. Dry Natural Gas Production (Bcf)"

405

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","na1504_nus_4m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/na1504_nus_4m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:46:14 PM" "Back to Contents","Data 1: U.S. Natural Gas % of Total Residential - Sales (%)" "Sourcekey","NA1504_NUS_4" "Date","U.S. Natural Gas % of Total Residential - Sales (%)" 37271,98.3 37302,98.5 37330,98.4 37361,98.1

406

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n5050us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n5050us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:29:09 PM" "Back to Contents","Data 1: U.S. Total Natural Gas Injections into Underground Storage (MMcf)" "Sourcekey","N5050US2" "Date","U.S. Total Natural Gas Injections into Underground Storage (MMcf)" 26679 26710 26738 26769 26799

407

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010hi2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010hi2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:19 PM" "Back to Contents","Data 1: Hawaii Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010HI2" "Date","Hawaii Natural Gas Residential Consumption (MMcf)" 29402,1416 29767,1289 30132,1197 30497,1121 30863,1048 31228,625 31593,579 31958,591

408

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010tx2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010tx2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:59 PM" "Back to Contents","Data 1: Texas Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010TX2" "Date","Texas Natural Gas Residential Consumption (MMcf)" 24653,201407 25019,211763 25384,220728 25749,232189 26114,237387 26480,240662

409

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040nd2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040nd2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:40 AM" "Back to Contents","Data 1: North Dakota Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040ND2" "Date","North Dakota Natural Gas Vented and Flared (MMcf)" 35079,232 35110,193 35139,232 35170,176 35200,230 35231,258 35261,269

410

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010de3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010de3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:15 PM" "Back to Contents","Data 1: Delaware Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010DE3" "Date","Delaware Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

411

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3020fl2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3020fl2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:29 PM" "Back to Contents","Data 1: Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in Florida (MMcf)" "Sourcekey","N3020FL2" "Date","Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in Florida (MMcf)"

412

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3020ct2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3020ct2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:23 PM" "Back to Contents","Data 1: Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in Connecticut (MMcf)" "Sourcekey","N3020CT2" "Date","Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in Connecticut (MMcf)"

413

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3020az2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3020az2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:17 PM" "Back to Contents","Data 1: Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in Arizona (MMcf)" "Sourcekey","N3020AZ2" "Date","Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in Arizona (MMcf)"

414

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3020ca2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3020ca2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:19 PM" "Back to Contents","Data 1: Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in California (MMcf)" "Sourcekey","N3020CA2" "Date","Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in California (MMcf)"

415

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3020dc2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3020dc2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:24 PM" "Back to Contents","Data 1: Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in the District of Columbia (MMcf)" "Sourcekey","N3020DC2" "Date","Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in the District of Columbia (MMcf)"

416

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3020co2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3020co2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:21 PM" "Back to Contents","Data 1: Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in Colorado (MMcf)" "Sourcekey","N3020CO2" "Date","Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in Colorado (MMcf)"

417

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010md2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010md2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:30 PM" "Back to Contents","Data 1: Maryland Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010MD2" "Date","Maryland Natural Gas Residential Consumption (MMcf)" 24653,77130 25019,79015 25384,84406 25749,86811 26114,87617 26480,89042

418

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040or2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040or2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:43 AM" "Back to Contents","Data 1: Oregon Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040OR2" "Date","Oregon Natural Gas Vented and Flared (MMcf)" 35079 35110 35139 35170 35200 35231 35261 35292 35323 35353 35384 35414 35445,0

419

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010wv3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010wv3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:07 PM" "Back to Contents","Data 1: West Virginia Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010WV3" "Date","West Virginia Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

420

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010la2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010la2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:28 PM" "Back to Contents","Data 1: Louisiana Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010LA2" "Date","Louisiana Natural Gas Residential Consumption (MMcf)" 24653,74386 25019,77762 25384,82965 25749,86148 26114,79893 26480,82847

Note: This page contains sample records for the topic "mesons contents baryons" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


421

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010al3m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010al3m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:07 PM" "Back to Contents","Data 1: Alabama Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010AL3" "Date","Alabama Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

422

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010nm3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010nm3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:45 PM" "Back to Contents","Data 1: New Mexico Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010NM3" "Date","New Mexico Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

423

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010id2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010id2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:22 PM" "Back to Contents","Data 1: Idaho Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010ID2" "Date","Idaho Natural Gas Residential Consumption (MMcf)" 24653,6179 25019,6545 25384,6980 25749,7711 26114,8455 26480,10887 26845,9947 27210,9652

424

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010wa2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010wa2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:05 PM" "Back to Contents","Data 1: Washington Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010WA2" "Date","Washington Natural Gas Residential Consumption (MMcf)" 24653,23160 25019,26342 25384,30479 25749,31929 26114,33934 26480,38631

425

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040ok2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040ok2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:42 AM" "Back to Contents","Data 1: Oklahoma Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040OK2" "Date","Oklahoma Natural Gas Vented and Flared (MMcf)" 35079 35110 35139 35170 35200 35231 35261 35292 35323 35353 35384 35414 35445,0

426

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9132us3m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9132us3m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/13/2013 2:23:27 PM" "Back to Contents","Data 1: Price of U.S. Natural Gas Pipeline Exports (Dollars per Thousand Cubic Feet)" "Sourcekey","N9132US3" "Date","Price of U.S. Natural Gas Pipeline Exports (Dollars per Thousand Cubic Feet)" 35445,4.08

427

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040nm2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040nm2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:40 AM" "Back to Contents","Data 1: New Mexico Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040NM2" "Date","New Mexico Natural Gas Vented and Flared (MMcf)" 24653,5992 25019,5987 25384,4058 25749,2909 26114,2823 26480,5696 26845,3791 27210,1227

428

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040sd2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040sd2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:43 AM" "Back to Contents","Data 1: South Dakota Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040SD2" "Date","South Dakota Natural Gas Vented and Flared (MMcf)" 24653,0 25019,0 25384,0 25749,0 26114,0 26480,0 26845,0 27210,0 27575,4 27941,5

429

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040co2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040co2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:33 AM" "Back to Contents","Data 1: Colorado Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040CO2" "Date","Colorado Natural Gas Vented and Flared (MMcf)" 24653,2656 25019,1514 25384,1326 25749,7126 26114,2843 26480,4758 26845,3008 27210,2957

430

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3035us4a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3035us4a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:25:09 PM" "Back to Contents","Data 1: Percent of Industrial Natural Gas Deliveries in U.S. Total Represented by the Price (%)" "Sourcekey","N3035US4" "Date","Percent of Industrial Natural Gas Deliveries in U.S. Total Represented by the Price (%)"

431

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040ny2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040ny2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:41 AM" "Back to Contents","Data 1: New York Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040NY2" "Date","New York Natural Gas Vented and Flared (MMcf)" 33253,0 33284,0 33312,1 33343,0 33373,0 33404,0 33434,0 33465,0 33496,0

432

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ma2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ma2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:29 PM" "Back to Contents","Data 1: Massachusetts Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010MA2" "Date","Massachusetts Natural Gas Residential Consumption (MMcf)" 24653,73471 25019,74919 25384,78451 25749,82646 26114,83434 26480,86171

433

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040mt2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040mt2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:39 AM" "Back to Contents","Data 1: Montana Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040MT2" "Date","Montana Natural Gas Vented and Flared (MMcf)" 35079,32 35110,38 35139,34 35170,40 35200,43 35231,27 35261,63 35292,59 35323,60

434

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040us2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040us2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:45 AM" "Back to Contents","Data 1: U.S. Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040US2" "Date","U.S. Natural Gas Vented and Flared (MMcf)" 13331,392528 13696,526159 14061,649106 14426,677311 14792,655967 15157,630212 15522,626782 15887,684115

435

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040mi2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040mi2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:38 AM" "Back to Contents","Data 1: Michigan Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040MI2" "Date","Michigan Natural Gas Vented and Flared (MMcf)" 35079,277 35110,277 35139,277 35170,277 35200,277 35231,277 35261,277

436

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012,"6/30/1997" Annual",2012,"6/30/1997" ,"Data 2","Futures Prices",4,"Annual",2012,"6/30/1993" ,"Release Date:","12/18/2013" ,"Next Release Date:","12/27/2013" ,"Excel File Name:","ng_pri_fut_s1_a.xls" ,"Available from Web Page:","http://www.eia.gov/dnav/ng/ng_pri_fut_s1_a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.gov" ,,"(202) 586-8800",,,"12/18/2013 12:22:13 PM" "Back to Contents","Data 1: Spot Price" "Sourcekey","RNGWHHD","NGM_EPG0_PLC_NUS_DMMBTU" "Date","Henry Hub Natural Gas Spot Price (Dollars per Million Btu)","U.S. Natural Gas Liquid Composite Price (Dollars per Million Btu)"

437

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9012us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9012us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:55:55 AM" "Back to Contents","Data 1: U.S. Natural Gas Gross Withdrawals from Oil Wells (MMcf)" "Sourcekey","N9012US2" "Date","U.S. Natural Gas Gross Withdrawals from Oil Wells (MMcf)" 33253,475614 33526,500196 33984,513068 34015,462218

438

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040ne2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040ne2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:40 AM" "Back to Contents","Data 1: Nebraska Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040NE2" "Date","Nebraska Natural Gas Vented and Flared (MMcf)" 33253,0 33284,0 33312,0 33343,0 33373,0 33404,0 33434,0 33465,0 33496,0

439

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040pa2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040pa2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:43 AM" "Back to Contents","Data 1: Pennsylvania Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040PA2" "Date","Pennsylvania Natural Gas Vented and Flared (MMcf)" 33253,0 33284,0 33312,0 33343,0 33373,0 33404,0 33434,0 33465,0

440

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9050us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9050us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:57:04 AM" "Back to Contents","Data 1: U.S. Natural Gas Marketed Production (MMcf)" "Sourcekey","N9050US2" "Date","U.S. Natural Gas Marketed Production (MMcf)" 26679,1948000 26710,1962000 26738,1907000 26769,1814000 26799,1898000 26830,1839000

Note: This page contains sample records for the topic "mesons contents baryons" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


441

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

mbbl_a.xls" mbbl_a.xls" ,"Available from Web Page:","http://www.eia.gov/dnav/pet/pet_crd_crpdn_adc_mbbl_a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.gov" ,,"(202) 586-8800",,,"11/27/2013 9:07:23 AM" "Back to Contents","Data 1: Crude Oil Production" "Sourcekey","MCRFPUS1","MCRFPP11","MCRFPFL1","MCRFPNY1","MCRFPPA1","MCRFPVA1","MCRFPWV1","MCRFPP21","MCRFPIL1","MCRFPIN1","MCRFPKS1","MCRFPKY1","MCRFP_SMI_1","MCRFPMO1","MCRFPNE1","MCRFPND1","MCRFPOH1","MCRFPOK1","MCRFPSD1","MCRFPTN1","MCRFPP31","MCRFPAL1","MCRFPAR1","MCRFPLA1","MCRFPMS1","MCRFPNM1","MCRFPTX1","MCRFP3FM1","MCRFPP41","MCRFPCO1","MCRFPMT1","MCRFPUT1","MCRFPWY1","MCRFPP51","MCRFPAK1","MCRFPAKS1","MANFPAK1","MCRFPAZ1","MCRFPCA1","MCRFPNV1","MCRFP5F1"

442

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3020al2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3020al2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:11 PM" "Back to Contents","Data 1: Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in Alabama (MMcf)" "Sourcekey","N3020AL2" "Date","Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in Alabama (MMcf)"

443

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9100us3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9100us3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/13/2013 3:53:51 PM" "Back to Contents","Data 1: Price of U.S. Natural Gas Imports (Dollars per Thousand Cubic Feet)" "Sourcekey","N9100US3" "Date","Price of U.S. Natural Gas Imports (Dollars per Thousand Cubic Feet)" 31228,3.21 31593,2.43 31958,1.95 32324,1.84

444

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/18/2013" ,"Next Release Date:","12/27/2013" ,"Excel File Name:","rngc1a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngc1a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/18/2013 12:22:41 PM" "Back to Contents","Data 1: Natural Gas Futures Contract 1 (Dollars per Million Btu)" "Sourcekey","RNGC1" "Date","Natural Gas Futures Contract 1 (Dollars per Million Btu)" 34515,1.934 34880,1.692 35246,2.502 35611,2.475 35976,2.156 36341,2.319

445

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9130us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9130us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/13/2013 2:23:23 PM" "Back to Contents","Data 1: U.S. Natural Gas Exports (MMcf)" "Sourcekey","N9130US2" "Date","U.S. Natural Gas Exports (MMcf)" 26679,5808 26710,6079 26738,4021 26769,8017 26799,8741 26830,4131 26860,5744 26891,8726 26922,6403 26952,5473

446

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ks3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ks3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:26 PM" "Back to Contents","Data 1: Kansas Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010KS3" "Date","Kansas Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

447

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040ca2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040ca2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:33 AM" "Back to Contents","Data 1: California Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040CA2" "Date","California Natural Gas Vented and Flared (MMcf)" 35079,97 35110,103 35139,109 35170,107 35200,107 35231,104 35261,108

448

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9103us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9103us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/13/2013 3:54:17 PM" "Back to Contents","Data 1: U.S. Liquefied Natural Gas Imports (MMcf)" "Sourcekey","N9103US2" "Date","U.S. Liquefied Natural Gas Imports (MMcf)" 35445,9977 35476,7667 35504,2530 35535,2557 35565,5007 35596,5059 35626,5026 35657,7535

449

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040mt2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040mt2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:39 AM" "Back to Contents","Data 1: Montana Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040MT2" "Date","Montana Natural Gas Vented and Flared (MMcf)" 24653,5022 25019,12551 25384,26458 25749,5203 26114,4917 26480,4222 26845,3691 27210,3901

450

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040tx2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040tx2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:44 AM" "Back to Contents","Data 1: Texas Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040TX2" "Date","Texas Natural Gas Vented and Flared (MMcf)" 33253,2478 33284,2147 33312,2113 33343,2353 33373,3203 33404,2833 33434,3175

451

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9130us3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9130us3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/13/2013 2:23:24 PM" "Back to Contents","Data 1: Price of U.S. Natural Gas Exports (Dollars per Thousand Cubic Feet)" "Sourcekey","N9130US3" "Date","Price of U.S. Natural Gas Exports (Dollars per Thousand Cubic Feet)" 31228,4.77 31593,2.81 31958,3.07 32324,2.74

452

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040ny2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040ny2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:41 AM" "Back to Contents","Data 1: New York Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040NY2" "Date","New York Natural Gas Vented and Flared (MMcf)" 24653,0 25019,0 25384,0 25749,0 26114,0 26480,0 26845,0 27210,0 27575,0 27941,0 28306,0 28671,0

453

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040ks2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040ks2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:35 AM" "Back to Contents","Data 1: Kansas Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040KS2" "Date","Kansas Natural Gas Vented and Flared (MMcf)" 24653,2630 25019,2529 25384,2666 25749,2713 26114,2669 26480,2681 26845,2377 27210,889 27575,846

454

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040ar2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040ar2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:32 AM" "Back to Contents","Data 1: Arkansas Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040AR2" "Date","Arkansas Natural Gas Vented and Flared (MMcf)" 33253,23 33284,13 33312,12 33343,7 33373,13 33404,28 33434,28 33465,30

455

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010de2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010de2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:15 PM" "Back to Contents","Data 1: Delaware Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010DE2" "Date","Delaware Natural Gas Residential Consumption (MMcf)" 24653,6844 25019,7068 25384,7475 25749,7843 26114,8172 26480,8358 26845,7514

456

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

mbblpd_a.xls" mbblpd_a.xls" ,"Available from Web Page:","http://www.eia.gov/dnav/pet/pet_crd_crpdn_adc_mbblpd_a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.gov" ,,"(202) 586-8800",,,"11/27/2013 9:07:25 AM" "Back to Contents","Data 1: Crude Oil Production" "Sourcekey","MCRFPUS2","MCRFPP12","MCRFPFL2","MCRFPNY2","MCRFPPA2","MCRFPVA2","MCRFPWV2","MCRFPP22","MCRFPIL2","MCRFPIN2","MCRFPKS2","MCRFPKY2","MCRFP_SMI_2","MCRFPMO2","MCRFPNE2","MCRFPND2","MCRFPOH2","MCRFPOK2","MCRFPSD2","MCRFPTN2","MCRFPP32","MCRFPAL2","MCRFPAR2","MCRFPLA2","MCRFPMS2","MCRFPNM2","MCRFPTX2","MCRFP3FM2","MCRFPP42","MCRFPCO2","MCRFPMT2","MCRFPUT2","MCRFPWY2","MCRFPP52","MCRFPAK2","MCRFPAKS2","MANFPAK2","MCRFPAZ2","MCRFPCA2","MCRFPNV2","MCRFP5F2"

457

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","ngm_epg0_fgc_sky_mmcfm.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/ngm_epg0_fgc_sky_mmcfm.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:59:11 AM" "Back to Contents","Data 1: Kentucky Natural Gas Gross Withdrawals from Coalbed Wells (MMcf) " "Sourcekey","NGM_EPG0_FGC_SKY_MMCF" "Date","Kentucky Natural Gas Gross Withdrawals from Coalbed Wells (MMcf) "

458

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3020hi3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3020hi3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:34 PM" "Back to Contents","Data 1: Hawaii Price of Natural Gas Sold to Commercial Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3020HI3" "Date","Hawaii Price of Natural Gas Sold to Commercial Consumers (Dollars per Thousand Cubic Feet)"

459

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

poe2_dcu_nus-z00_a.xls" poe2_dcu_nus-z00_a.xls" ,"Available from Web Page:","http://www.eia.gov/dnav/ng/ng_move_poe2_dcu_nus-z00_a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.gov" ,,"(202) 586-8800",,,"12/12/2013 6:58:44 PM" "Back to Contents","Data 1: U.S. Total Exports " "Sourcekey","N9132US2","N9132US3","N9133US2","N9133US3" "Date","U.S. Natural Gas Pipeline Exports (MMcf)","Price of U.S. Natural Gas Pipeline Exports (Dollars per Thousand Cubic Feet)","Liquefied U.S. Natural Gas Exports (MMcf)","Price of Liquefied U.S. Natural Gas Exports (Dollars per Thousand Cubic Feet)"

460

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040ms2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040ms2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:38 AM" "Back to Contents","Data 1: Mississippi Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040MS2" "Date","Mississippi Natural Gas Vented and Flared (MMcf)" 24653,7098 25019,5910 25384,8097 25749,7233 26114,5090 26480,3672 26845,10767 27210,10787

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they are not comprehensive nor are they the most current set.
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461

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ok3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ok3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:50 PM" "Back to Contents","Data 1: Oklahoma Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010OK3" "Date","Oklahoma Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

462

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010nd3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010nd3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:40 PM" "Back to Contents","Data 1: North Dakota Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010ND3" "Date","North Dakota Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

463

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040or2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040or2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:42 AM" "Back to Contents","Data 1: Oregon Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040OR2" "Date","Oregon Natural Gas Vented and Flared (MMcf)" 35246 35611,0 35976,0 36341,0 36707,0 37072,0 37437,0 37802,0 38168,0 38533,0 38898,0 39263,0

464

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ky2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ky2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:27 PM" "Back to Contents","Data 1: Kentucky Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010KY2" "Date","Kentucky Natural Gas Residential Consumption (MMcf)" 24653,69542 25019,75824 25384,83815 25749,86473 26114,84197 26480,85881

465

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9160us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9160us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:33:48 PM" "Back to Contents","Data 1: U.S. Natural Gas Lease and Plant Fuel Consumption (MMcf)" "Sourcekey","N9160US2" "Date","U.S. Natural Gas Lease and Plant Fuel Consumption (MMcf)" 29235,93000 29266,87000 29295,93000 29326,85000

466

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9030us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9030us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:28 AM" "Back to Contents","Data 1: U.S. Nonhydrocarbon Gases Removed from Natural Gas (MMcf)" "Sourcekey","N9030US2" "Date","U.S. Nonhydrocarbon Gases Removed from Natural Gas (MMcf)" 26679 26710 26738 26769 26799 26830 26860 26891

467

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010mi3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010mi3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:33 PM" "Back to Contents","Data 1: Michigan Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010MI3" "Date","Michigan Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

468

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9070us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9070us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:57:08 AM" "Back to Contents","Data 1: U.S. Dry Natural Gas Production (MMcf)" "Sourcekey","N9070US2" "Date","U.S. Dry Natural Gas Production (MMcf)" 35445,1617923 35476,1465907 35504,1627602 35535,1551268 35565,1610527 35596,1525325

469

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9102us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9102us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/13/2013 3:53:55 PM" "Back to Contents","Data 1: U.S. Natural Gas Pipeline Imports (MMcf)" "Sourcekey","N9102US2" "Date","U.S. Natural Gas Pipeline Imports (MMcf)" 35445,268310 35476,232878 35504,254455 35535,235621 35565,236725 35596,227059 35626,230567

470

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010wy2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010wy2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:08 PM" "Back to Contents","Data 1: Wyoming Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010WY2" "Date","Wyoming Natural Gas Residential Consumption (MMcf)" 24653,11939 25019,12592 25384,16592 25749,17984 26114,19463 26480,22242 26845,13868

471

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3020ak2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3020ak2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:09 PM" "Back to Contents","Data 1: Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in Alaska (MMcf)" "Sourcekey","N3020AK2" "Date","Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in Alaska (MMcf)"

472

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:00 PM" "Back to Contents","Data 1: U.S. Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010US2" "Date","U.S. Natural Gas Residential Consumption (MMcf)" 26679,843900 26710,747331 26738,648504 26769,465867 26799,326313

473

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010mt2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010mt2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:38 PM" "Back to Contents","Data 1: Montana Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010MT2" "Date","Montana Natural Gas Residential Consumption (MMcf)" 24653,19756 25019,19711 25384,21463 25749,24794 26114,25379 26480,23787 26845,24923

474

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9103us3m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9103us3m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/13/2013 3:54:18 PM" "Back to Contents","Data 1: Price of U.S. Natural Gas LNG Imports (Dollars per Thousand Cubic Feet)" "Sourcekey","N9103US3" "Date","Price of U.S. Natural Gas LNG Imports (Dollars per Thousand Cubic Feet)" 35445,3 35476,3

475

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9132us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9132us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/13/2013 2:23:27 PM" "Back to Contents","Data 1: U.S. Natural Gas Pipeline Exports (MMcf)" "Sourcekey","N9132US2" "Date","U.S. Natural Gas Pipeline Exports (MMcf)" 35445,6424 35476,6846 35504,10601 35535,8211 35565,6284 35596,5741 35626,6380 35657,10101

476

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3035us4m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3035us4m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:25:10 PM" "Back to Contents","Data 1: Percent of Industrial Natural Gas Deliveries in U.S. Total Represented by the Price (%)" "Sourcekey","N3035US4" "Date","Percent of Industrial Natural Gas Deliveries in U.S. Total Represented by the Price (%)"

477

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010wi3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010wi3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:06 PM" "Back to Contents","Data 1: Wisconsin Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010WI3" "Date","Wisconsin Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

478

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040al2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040al2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:31 AM" "Back to Contents","Data 1: Alabama Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040AL2" "Date","Alabama Natural Gas Vented and Flared (MMcf)" 35079,194 35110,200 35139,140 35170,132 35200,106 35231,82 35261,205 35292,152

479

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040wv2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040wv2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:46 AM" "Back to Contents","Data 1: West Virginia Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040WV2" "Date","West Virginia Natural Gas Vented and Flared (MMcf)" 33253,0 33284,0 33312,0 33343,0 33373,0 33404,0 33434,0 33465,0

480

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013","1/15/1993" Monthly","9/2013","1/15/1993" ,"Release Date:","11/27/2013" ,"Next Release Date:","Last Week of December 2013" ,"Excel File Name:","pet_pnp_pct_dc_nus_pct_m.xls" ,"Available from Web Page:","http://www.eia.gov/dnav/pet/pet_pnp_pct_dc_nus_pct_m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.gov" ,,"(202) 586-8800",,,"11/25/2013 11:23:48 AM" "Back to Contents","Data 1: U.S. Refinery Yield" "Sourcekey","MLRRYUS3","MGFRYUS3","MGARYUS3","MKJRYUS3","MKERYUS3","MDIRYUS3","MRERYUS3","MNFRYUS3","MOTRYUS3","MNSRYUS3","MLURYUS3","MWXRYUS3","MCKRYUS3","MAPRYUS3","MSGRYUS3","MMSRYUS3","MPGRYUS3"

Note: This page contains sample records for the topic "mesons contents baryons" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


481

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3020us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3020us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:23:36 PM" "Back to Contents","Data 1: Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in the U.S. (MMcf)" "Sourcekey","N3020US2" "Date","Natural Gas Deliveries to Commercial Consumers (Including Vehicle Fuel through 1996) in the U.S. (MMcf)"

482

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","9/2013" Monthly","9/2013" ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040us2m.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040us2m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:45 AM" "Back to Contents","Data 1: U.S. Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040US2" "Date","U.S. Natural Gas Vented and Flared (MMcf)" 26679 26710 26738 26769 26799 26830 26860 26891 26922 26952 26983 27013 27044 27075 27103

483

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Monthly","11/2013","1/15/1997" Monthly","11/2013","1/15/1997" ,"Data 2","Futures Prices",4,"Monthly","11/2013","12/15/1993" ,"Release Date:","12/18/2013" ,"Next Release Date:","12/27/2013" ,"Excel File Name:","ng_pri_fut_s1_m.xls" ,"Available from Web Page:","http://www.eia.gov/dnav/ng/ng_pri_fut_s1_m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.gov" ,,"(202) 586-8800",,,"12/18/2013 12:22:17 PM" "Back to Contents","Data 1: Spot Price" "Sourcekey","RNGWHHD","NGM_EPG0_PLC_NUS_DMMBTU"

484

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010pa3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010pa3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:52 PM" "Back to Contents","Data 1: Pennsylvania Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010PA3" "Date","Pennsylvania Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

485

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010ut3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010ut3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:02 PM" "Back to Contents","Data 1: Utah Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010UT3" "Date","Utah Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

486

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010dc2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010dc2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:13 PM" "Back to Contents","Data 1: District of Columbia Natural Gas Residential Consumption (MMcf)" "Sourcekey","N3010DC2" "Date","District of Columbia Natural Gas Residential Consumption (MMcf)" 29402,13730 29767,13686 30132,13041 30497,13007

487

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010tx3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010tx3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:00 PM" "Back to Contents","Data 1: Texas Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010TX3" "Date","Texas Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

488

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012,"6/30/1993" Annual",2012,"6/30/1993" ,"Release Date:","9/27/2013" ,"Next Release Date:","9/26/2014" ,"Excel File Name:","pet_stoc_typ_d_nus_skn_mbbl_a.xls" ,"Available from Web Page:","http://www.eia.gov/dnav/pet/pet_stoc_typ_d_nus_skn_mbbl_a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.gov" ,,"(202) 586-8800",,,"11/25/2013 11:41:29 AM" "Back to Contents","Data 1: U.S. Natural Gas Processing Plant " "Sourcekey","MAOSNUS1","MPPSNUS1","MLPSNUS1","METSNUS1","MPRSNUS1","MBNSNUS1","MBISNUS1"

489

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n9040az2a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n9040az2a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/19/2013 6:56:32 AM" "Back to Contents","Data 1: Arizona Natural Gas Vented and Flared (MMcf)" "Sourcekey","N9040AZ2" "Date","Arizona Natural Gas Vented and Flared (MMcf)" 26114,347 26480,367 26845,277 27210,26 27575,47 27941,32 29036,101 29402,143 29767,106 30132,162

490

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3020ca3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3020ca3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:20 PM" "Back to Contents","Data 1: California Price of Natural Gas Sold to Commercial Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3020CA3" "Date","California Price of Natural Gas Sold to Commercial Consumers (Dollars per Thousand Cubic Feet)"

491

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3010oh3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3010oh3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:21:49 PM" "Back to Contents","Data 1: Ohio Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3010OH3" "Date","Ohio Price of Natural Gas Delivered to Residential Consumers (Dollars per Thousand Cubic Feet)"

492

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012 Annual",2012 ,"Release Date:","12/12/2013" ,"Next Release Date:","1/7/2014" ,"Excel File Name:","n3020fl3a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/n3020fl3a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 5:22:30 PM" "Back to Contents","Data 1: Florida Price of Natural Gas Sold to Commercial Consumers (Dollars per Thousand Cubic Feet)" "Sourcekey","N3020FL3" "Date","Florida Price of Natural Gas Sold to Commercial Consumers (Dollars per Thousand Cubic Feet)"

493

Masses of mesons with charm valence quarks from 2+1+1 flavor twisted mass lattice QCD  

E-Print Network (OSTI)

We present preliminary results of an ongoing lattice QCD computation of the spectrum of $D$ mesons and $D_s$ mesons and of charmonium using 2+1+1 flavors of twisted mass sea and valence quarks.

Martin Kalinowski; Marc Wagner

2013-04-30T23:59:59.000Z

494

Emergency Operations Table of Contents  

E-Print Network (OSTI)

Table of Contents..................................................................................................... ii

unknown authors

2012-01-01T23:59:59.000Z

495

An experimental review of the decays of the D/sub S/ meson  

SciTech Connect

In this paper I review the current experimental knowledge of the decays of the D/sub s/ meson. I compare D/sub s/ properties to those predicted from recent comprehensive D meson decay models that are based on the better measured charmed isodoublet (D/sup 0/,D/sup +/). 12 refs., 5 figs., 2 tabs.

Schindler, R.H.

1989-06-01T23:59:59.000Z

496

Handbook of Higher Twist Distribution Amplitudes of Vector Mesons in QCD  

E-Print Network (OSTI)

We give a summary of existing results on higher twist distribution amplitudes of vector mesons in QCD. Special attention is payed to meson mass corrections which turn out to be large. A ``shopping list'' is presented of most important nonperturbative parameters which enter distribution amplitudes.

Patricia Ball; V. M. Braun

1998-08-05T23:59:59.000Z

497

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

capwork_a_(na)_8sw0_mbbl_a.xls" capwork_a_(na)_8sw0_mbbl_a.xls" ,"Available from Web Page:","http://www.eia.gov/dnav/pet/pet_pnp_capwork_a_(na)_8sw0_mbbl_a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.gov" ,,"(202) 586-8800",,,"6/20/2013 4:20:16 PM" "Back to Contents","Data 1: Total " "Sourcekey","8_NA_8SW0_NUS_MBBL","8_NA_8SW0_R10_MBBL","8_NA_8SW0_R20_MBBL","8_NA_8SW0_R30_MBBL","8_NA_8SW0_R40_MBBL","8_NA_8SW0_R50_MBBL" "Date","U.S. Refinery Working Storage Capacity as of January 1 (Thousand Barrels)","East Coast (PADD 1) Refinery Working Storage Capacity as of January 1 (Thousand Barrels)","Midwest (PADD 2) Refinery Working Storage Capacity as of January 1 (Thousand Barrels)","Gulf Coast (PADD 3) Refinery Working Storage Capacity as of January 1 (Thousand Barrels)","Rocky Mountain (PADD 4) Refinery Working Storage Capacity as of January 1 (Thousand Barrels)","West Coast (PADD 5) Refinery Working Storage Capacity as of January 1 (Thousand Barrels)"

498

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

mbblpd_m.xls" mbblpd_m.xls" ,"Available from Web Page:","http://www.eia.gov/dnav/pet/pet_cons_psup_dc_nus_mbblpd_m.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.gov" ,,"(202) 586-8800",,,"11/25/2013 7:26:11 AM" "Back to Contents","Data 1: U.S. Product Supplied for Crude Oil and Petroleum Products" "Sourcekey","MTTUPUS2","MCRUPUS2","MNGUPUS2","MPPUPUS2","MLPUPUS2","METUPUS2","MPRUPUS2","MBNUPUS2","MBIUPUS2","MOLUPUS2","MOHUPUS2","MUOUPUS2","MBCUPUS2","MO1UP_NUS_2","MO5UP_NUS_2","MBAUPUS2","MTPUPUS2","MGFUPUS2","MGRUPUS2","MG4UP_NUS_2","MGAUPUS2","MKJUPUS2","MKEUPUS2","MDIUPUS2","MD0UP_NUS_2","MD1UP_NUS_2","MDGUPUS2","MREUPUS2","MPCUP_NUS_2","MNFUPUS2","MOTUPUS2","MNSUPUS2","MLUUPUS2","MWXUPUS2","MCKUPUS2","MCMUP_NUS_2","MCOUP_NUS_2","MAPUPUS2","MSGUPUS2","MMSUPUS2"

499

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

capshell_a_(na)_8ss0_mbbl_a.xls" capshell_a_(na)_8ss0_mbbl_a.xls" ,"Available from Web Page:","http://www.eia.gov/dnav/pet/pet_pnp_capshell_a_(na)_8ss0_mbbl_a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.gov" ,,"(202) 586-8800",,,"6/20/2013 4:17:24 PM" "Back to Contents","Data 1: Total " "Sourcekey","8_NA_8SS0_NUS_MBBL","8_NA_8SS0_R10_MBBL","8_NA_8SS0_R20_MBBL","8_NA_8SS0_R30_MBBL","8_NA_8SS0_R40_MBBL","8_NA_8SS0_R50_MBBL" "Date","U.S. Refinery Shell Storage Capacity as of January 1 (Thousand Barrels)","East Coast (PADD 1) Refinery Shell Storage Capacity as of January 1 (Thousand Barrels)","Midwest (PADD 2) Refinery Shell Storage Capacity as of January 1 (Thousand Barrels)","Gulf Coast (PADD 3) Refinery Shell Storage Capacity as of January 1 (Thousand Barrels)","Rocky Mountain (PADD 4) Refinery Shell Storage Capacity as of January 1 (Thousand Barrels)","West Coast (PADD 5) Refinery Shell Storage Capacity as of January 1 (Thousand Barrels)"

500

Workbook Contents  

U.S. Energy Information Administration (EIA) Indexed Site

Annual",2012,"6/30/1936" Annual",2012,"6/30/1936" ,"Release Date:","9/27/2013" ,"Next Release Date:","9/26/2014" ,"Excel File Name:","pet_pnp_refp_dc_nus_mbbl_a.xls" ,"Available from Web Page:","http://www.eia.gov/dnav/pet/pet_pnp_refp_dc_nus_mbbl_a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.gov" ,,"(202) 586-8800",,,"11/25/2013 11:25:40 AM" "Back to Contents","Data 1: U.S. Refinery and Blender Net Production" "Sourcekey","MTTRPUS1","MLPRPUS1","METRPUS1","MENRPUS1","MEYRPUS1","MPRRPUS1","MPARP_NUS_1","MPLRPUS1","MBNRPUS1","MBURPUS1","MBYRPUS1","MBIRPUS1","MIIRPUS1","MIYRPUS1","MGFRPUS1","MGRRPUS1","MG1RP_NUS_1","M_EPM0RO_YPR_NUS_MBBL","MG4RP_NUS_1","MG5RP_NUS_1","M_EPM0CAL55_YPR_NUS_MBBL","M_EPM0CAG55_YPR_NUS_MBBL","MG6RP_NUS_1","MGARPUS1","MKJRPUS1","MKERPUS1","MDIRPUS1","MD0RP_NUS_1","MD1RP_NUS_1","MDGRPUS1","MRERPUS1","MRLRPUS1","MRMRPUS1","MRGRPUS1","MPCRPUS1","MNFRPUS1","MOTRPUS1","MNSRPUS1","MLURPUS1","MWXRPUS1","MCKRPUS1","MCMRPUS1","MCORPUS1","MAPRPUS1","MSGRPUS1","MMSRPUS1","MPGRPUS1"