Sample records for nucleosynthesis bbn offers

  1. Big-Bang Nucleosynthesis verifies classical Maxwell-Boltzmann distribution

    E-Print Network [OSTI]

    S. Q. Hou; J. J. He; A. Parikh; K. Daid; C. Bertulani

    2014-08-15T23:59:59.000Z

    We provide the most stringent constraint to date on possible deviations from the usually-assumed Maxwell-Boltzmann (MB) velocity distribution for nuclei in the Big-Bang plasma. The impact of non-extensive Tsallis statistics on thermonuclear reaction rates involved in standard models of Big-Bang Nucleosynthesis (BBN) has been investigated. We find that the non-extensive parameter $q$ may deviate by, at most, $|\\delta q|$=6$\\times$10$^{-4}$ from unity for BBN predictions to be consistent with observed primordial abundances; $q$=1 represents the classical Boltzmann-Gibbs statistics. This constraint arises primarily from the {\\em super}sensitivity of endothermic rates on the value of $q$, which is found for the first time. As such, the implications of non-extensive statistics in other astrophysical environments should be explored. This may offer new insight into the nucleosynthesis of heavy elements.

  2. Testing a Dilaton Gravity Model using Nucleosynthesis

    E-Print Network [OSTI]

    Sibel Boran; Emre Onur Kahya

    2014-09-05T23:59:59.000Z

    Big Bang Nucleosynthesis (BBN) offers one of the most strict evidences for the Lambda-CDM cosmology at present, as well as the Cosmic Microwave Background (CMB) radiation. In this work, our main aim is to present the outcomes of our calculations related to primordial abundances of light elements, in the context of higher dimensional steady-state universe model in the dilaton gravity. Our results show that abundances of light elements (primordial D, 3He, 4He, T, 7Li) are significantly different for some cases, and a comparison is given between a particular dilaton gravity model and Lambda-CDM in the light of the astrophysical observations.

  3. Big Bang Nucleosynthesis: 2015

    E-Print Network [OSTI]

    Cyburt, Richard H; Olive, Keith A; Yeh, Tsung-Han

    2015-01-01T23:59:59.000Z

    Big-bang nucleosynthesis (BBN) describes the production of the lightest nuclides via a dynamic interplay among the four fundamental forces during the first seconds of cosmic time. We briefly overview the essentials of this physics, and present new calculations of light element abundances through li6 and li7, with updated nuclear reactions and uncertainties including those in the neutron lifetime. We provide fits to these results as a function of baryon density and of the number of neutrino flavors, N_nu. We review recent developments in BBN, particularly new, precision Planck cosmic microwave background (CMB) measurements that now probe the baryon density, helium content, and the effective number of degrees of freedom, n_eff. These measurements allow for a tight test of BBN and of cosmology using CMB data alone. Our likelihood analysis convolves the 2015 Planck data chains with our BBN output and observational data. Adding astronomical measurements of light elements strengthens the power of BBN. We include a ...

  4. Nuclear reaction rates and the primordial nucleosynthesis

    E-Print Network [OSTI]

    Abhishek Mishra; D. N. Basu

    2011-11-15T23:59:59.000Z

    The theoretical predictions of the primordial abundances of elements in the big-bang nucleosynthesis (BBN) are dominated by uncertainties in the input nuclear reaction rates. We investigate the effect of modifying these reaction rates on light element abundance yields in BBN by replacing the thirty-five reaction rates out of the existing eighty-eight. We have studied these yields as functions of evolution time or temperature. We find that using these new reaction rates results in only a little increase in helium mass fraction over that obtained previously in BBN calculations. This allows insights into the role of the nuclear reaction rates in the setting of the neutron-to-proton ratio during the BBN epoch. We observe that even with considerable nuclear physics uncertainties, most of these nuclear reactions have minimal effect on the standard BBN abundance yields of $^6$Li and $^7$Li.

  5. The DARPA WNaN Network Architecture Raytheon BBN Technologies

    E-Print Network [OSTI]

    Ramanathan, Ram

    The DARPA WNaN Network Architecture Jason Redi Raytheon BBN Technologies Cambridge, MA redi@bbn.com Ram Ramanathan Raytheon BBN Technologies Cambridge, MA ramanath@bbn.com Abstract-- The warfighter its goal. WNaN uses networking software from Raytheon BBN Technologies, and radio hardware plus

  6. The NACRE Thermonuclear Reaction Compilation and Big Bang Nucleosynthesis

    E-Print Network [OSTI]

    Richard H. Cyburt; Brian D. Fields; Keith A. Olive

    2001-05-17T23:59:59.000Z

    The theoretical predictions of big bang nucleosynthesis (BBN) are dominated by uncertainties in the input nuclear reaction cross sections. In this paper, we examine the impact on BBN of the recent compilation of nuclear data and thermonuclear reactions rates by the NACRE collaboration. We confirm that the adopted rates do not make large overall changes in central values of predictions, but do affect the magnitude of the uncertainties in these predictions. Therefore, we then examine in detail the uncertainties in the individual reaction rates considered by NACRE. When the error estimates by NACRE are treated as 1\\sigma limits, the resulting BBN error budget is similar to those of previous tabulations. We propose two new procedures for deriving reaction rate uncertainties from the nuclear data: one which sets lower limits to the error, and one which we believe is a reasonable description of the present error budget. We propagate these uncertainty estimates through the BBN code, and find that when the nuclear data errors are described most accurately, the resulting light element uncertainties are notably smaller than in some previous tabulations, but larger than others. Using these results, we derive limits on the cosmic baryon-to-photon ratio $\\eta$, and compare this to independent limits on $\\eta$ from recent balloon-borne measurements of the cosmic microwave background radiation (CMB). We discuss means to improve the BBN results via key nuclear reaction measurements and light element observations.

  7. BBN Technical Memorandum No. TM-2023 Ultra Low Latency MANETs

    E-Print Network [OSTI]

    Ramanathan, Ram

    communication ranges foretell MANETs with very large diameters. Indeed, an architecture where dense low-cost: ramanath@bbn.com Fabrice Tchakountio Mobile Networking Systems Department BBN Technologies Cambridge, MA a MANET to a large number of hops. MANETs are trending toward larger numbers of nodes due to increasing

  8. Refined scenario of standard Big Bang nucleosynthesis allowing for nonthermal nuclear reactions in the primordial plasma

    SciTech Connect (OSTI)

    Voronchev, Victor T.; Nakao, Yasuyuki; Nakamura, Makoto; Tsukida, Kazuki [Institute of Nuclear Physics, Moscow State University, Moscow 119991 (Russian Federation); Department of Applied Quantum Physics and Nuclear Engineering, Kyushu University, Motooka, Fukuoka 819-0395 (Japan); Division of Advanced Plasma Research, Japan Atomic Energy Agency, 2-166 Oaza-Obuchi-Aza-Omotedate, Rokkasho, Kamikita, Aomori 039-3212 (Japan); Department of Applied Quantum Physics and Nuclear Engineering, Kyushu University, Motooka, Fukuoka 819-0395 (Japan)

    2012-11-12T23:59:59.000Z

    The standard scenario of big bang nucleosynthesis (BBN) is generalized to take into account nonthermal nuclear reactions in the primordial plasma. These reactions are naturally triggered in the BBN epoch by fast particles generated in various exoergic processes. It is found that, although such particles can appreciably enhance the rates of some individual reactions, their influence on the whole process of element production is not significant. The nonthermal corrections to element abundances are obtained to be 0.1% ({sup 3}H), -0.03% ({sup 7}Li), and 0.34 %-0.63% (CNO group).

  9. Nucleosynthesis in Thermonuclear Supernovae

    SciTech Connect (OSTI)

    Claudia, Travaglio [Istituto Nazionale di Astrofisica, Osservatorio Astronomico di Torino; Hix, William Raphael [ORNL

    2013-01-01T23:59:59.000Z

    We review our understanding of the nucleosynthesis that occurs in thermonuclear supernovae and their contribution to Galactic Chemical evolution. We discuss the prospects to improve the modeling of the nucleosynthesis within simulations of these events.

  10. BBN And The CMB Constrain Neutrino Coupled Light WIMPs

    E-Print Network [OSTI]

    Nollett, Kenneth M

    2014-01-01T23:59:59.000Z

    (abridged) In the presence of a light WIMP (mass m_chi 35 MeV, equivalent to no light WIMP at all. Without any light WIMP, BBN alone prefers Delta N_nu = 0.50 +- 0.23, favoring neither Delta N_nu = 0, nor a fully thermalized sterile neutrino (Delta N_nu = 1). This result is consistent with the CMB constraint, N_eff = 3.30 +- 0.27, limiting "new physics" between BBN and recombination. Combining BBN and CMB data gives Delta N_nu = 0.35 +- 0.16 and N_eff = 3.40 +- 0.16; while BBN and the CMB combined require Delta N_nu > 0 at ~98% confidence, they disfavor Delta N_nu > 1 at > 99% confidence. Allowing a neutrino-coupled light WIMP extends the allowed range slightly downward for Delta N_nu and slightly upward for N_eff simultaneously, leaving best-fit values unchanged.

  11. Using Big Bang Nucleosynthesis to Extend CMB Probes of Neutrino Physics

    E-Print Network [OSTI]

    M. Shimon; N. J. Miller; C. T. Kishimoto; C. J. Smith; G. M. Fuller; B. G. Keating

    2010-05-10T23:59:59.000Z

    We present calculations showing that upcoming Cosmic Microwave Background (CMB) experiments will have the power to improve on current constraints on neutrino masses and provide new limits on neutrino degeneracy parameters. The latter could surpass those derived from Big Bang Nucleosynthesis (BBN) and the observationally-inferred primordial helium abundance. These conclusions derive from our Monte Carlo Markov Chain (MCMC) simulations which incorporate a full BBN nuclear reaction network. This provides a self-consistent treatment of the helium abundance, the baryon number, the three individual neutrino degeneracy parameters and other cosmological parameters. Our analysis focuses on the effects of gravitational lensing on CMB constraints on neutrino rest mass and degeneracy parameter. We find for the PLANCK experiment that total (summed) neutrino mass $M_{\

  12. Using Big Bang Nucleosynthesis to Extend CMB Probes of Neutrino Physics

    E-Print Network [OSTI]

    Shimon, M; Kishimoto, C T; Smith, C J; Fuller, G M; Keating, B G

    2010-01-01T23:59:59.000Z

    We present calculations showing that upcoming Cosmic Microwave Background (CMB) experiments will have the power to improve on current constraints on neutrino masses and provide new limits on neutrino degeneracy parameters. The latter could surpass those derived from Big Bang Nucleosynthesis (BBN) and the observationally-inferred primordial helium abundance. These conclusions derive from our Monte Carlo Markov Chain (MCMC) simulations which incorporate a full BBN nuclear reaction network. This provides a self-consistent treatment of the helium abundance, the baryon number, the three individual neutrino degeneracy parameters and other cosmological parameters. Our analysis focuses on the effects of gravitational lensing on CMB constraints on neutrino rest mass and degeneracy parameter. We find for the PLANCK experiment that total (summed) neutrino mass $M_{\

  13. Big Bang Nucleosynthesis with Independent Neutrino Distribution Functions

    E-Print Network [OSTI]

    Christel J. Smith; George M. Fuller; Michael S. Smith

    2008-12-06T23:59:59.000Z

    We have performed new Big Bang Nucleosynthesis calculations which employ arbitrarily-specified, time-dependent neutrino and antineutrino distribution functions for each of up to four neutrino flavors. We self-consistently couple these distributions to the thermodynamics, the expansion rate and scale factor-time/temperature relationship, as well as to all relevant weak, electromagnetic, and strong nuclear reaction processes in the early universe. With this approach, we can treat any scenario in which neutrino or antineutrino spectral distortion might arise. These scenarios might include, for example, decaying particles, active-sterile neutrino oscillations, and active-active neutrino oscillations in the presence of significant lepton numbers. Our calculations allow lepton numbers and sterile neutrinos to be constrained with observationally-determined primordial helium and deuterium abundances. We have modified a standard BBN code to perform these calculations and have made it available to the community.

  14. Nucleosynthesis Without a Computer

    E-Print Network [OSTI]

    V. Mukhanov

    2003-03-04T23:59:59.000Z

    I derive completely analytically the time evolution and final abundances of the light elements (up to Be-7) formed in the big-bang nucleosynthesis.This highlights an interesting physics taking place during the formation of light elements in the early universe.

  15. REVISED BIG BANG NUCLEOSYNTHESIS WITH LONG-LIVED, NEGATIVELY CHARGED MASSIVE PARTICLES: UPDATED RECOMBINATION RATES, PRIMORDIAL {sup 9}Be NUCLEOSYNTHESIS, AND IMPACT OF NEW {sup 6}Li LIMITS

    SciTech Connect (OSTI)

    Kusakabe, Motohiko; Kim, K. S. [School of Liberal Arts and Science, Korea Aerospace University, Goyang 412-791 (Korea, Republic of); Cheoun, Myung-Ki [Department of Physics, Soongsil University, Seoul 156-743 (Korea, Republic of); Kajino, Toshitaka [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Kino, Yasushi [Department of Chemistry, Tohoku University, Sendai 980-8578 (Japan); Mathews, Grant J., E-mail: motohiko@kau.ac.kr, E-mail: kyungsik@kau.ac.kr, E-mail: cheoun@ssu.ac.kr, E-mail: kajino@nao.ac.jp, E-mail: y.k@m.tohoku.ac.jp, E-mail: gmathews@nd.edu [Center for Astrophysics, Department of Physics, University of Notre Dame, Notre Dame, IN 46556 (United States)

    2014-09-01T23:59:59.000Z

    We extensively reanalyze the effects of a long-lived, negatively charged massive particle, X {sup –}, on big bang nucleosynthesis (BBN). The BBN model with an X {sup –} particle was originally motivated by the discrepancy between the {sup 6,} {sup 7}Li abundances predicted in the standard BBN model and those inferred from observations of metal-poor stars. In this model, {sup 7}Be is destroyed via the recombination with an X {sup –} particle followed by radiative proton capture. We calculate precise rates for the radiative recombinations of {sup 7}Be, {sup 7}Li, {sup 9}Be, and {sup 4}He with X {sup –}. In nonresonant rates, we take into account respective partial waves of scattering states and respective bound states. The finite sizes of nuclear charge distributions cause deviations in wave functions from those of point-charge nuclei. For a heavy X {sup –} mass, m{sub X} ? 100 GeV, the d-wave ? 2P transition is most important for {sup 7}Li and {sup 7,} {sup 9}Be, unlike recombination with electrons. Our new nonresonant rate of the {sup 7}Be recombination for m{sub X} = 1000 GeV is more than six times larger than the existing rate. Moreover, we suggest a new important reaction for {sup 9}Be production: the recombination of {sup 7}Li and X {sup –} followed by deuteron capture. We derive binding energies of X nuclei along with reaction rates and Q values. We then calculate BBN and find that the amount of {sup 7}Be destruction depends significantly on the charge distribution of {sup 7}Be. Finally, updated constraints on the initial abundance and the lifetime of the X {sup –} are derived in the context of revised upper limits to the primordial {sup 6}Li abundance. Parameter regions for the solution to the {sup 7}Li problem and the primordial {sup 9}Be abundances are revised.

  16. Explosive Nucleosynthesis: Prospects

    E-Print Network [OSTI]

    David Arnett

    1999-08-16T23:59:59.000Z

    Explosive nucleosynthesis is a combination of the nuclear physics of thermonuclear reactions, and the hydrodynamics of the plasma in which the reactions occur. It depends upon the initial conditions---the stellar evolution up to the explosive instability, and the nature of the explosion mechanism. Some key issues for explosive nucleosynthesis are the interaction of burning with hydrodynamics, the degree of microscopic mixing in convective zones, and the breaking of spherical symmetry by convection and rotation. Recent experiments on high intensity lasers provides new opportunities for laboratory testing of astrophysical hydrodynamic codes. Implications of SN1987A, SN1998bw (GRB980425?), and eta Carina are discussed, as well as the formation of black holes or neutron stars.

  17. Primordial nucleosynthesis and neutrino physics

    E-Print Network [OSTI]

    Smith, Christel Johanna

    2009-01-01T23:59:59.000Z

    A Brief History of and Introduction to Neutrino Physics . 13Nucleosynthesis and Neutrino Physics A dissertationdensity depend on new neutrino physics in di?erent ways. In

  18. STANDARD BIG BANG NUCLEOSYNTHESIS UP TO CNO WITH AN IMPROVED EXTENDED NUCLEAR NETWORK

    SciTech Connect (OSTI)

    Coc, Alain [Centre de Spectrometrie Nucleaire et de Spectrometrie de Masse (CSNSM), CNRS/IN2P3, Universite Paris Sud, UMR 8609, Batiment 104, F-91405 Orsay Campus (France); Goriely, Stephane; Xu, Yi [Institut d'Astronomie et d'Astrophysique, Universite Libre de Bruxelles, CP 226, Boulevard du Triomphe, B-1050 Bruxelles (Belgium); Saimpert, Matthias; Vangioni, Elisabeth [Institut d'Astrophysique de Paris, UMR 7095 CNRS, Universite Pierre et Marie Curie, 98 bis Boulevard Arago, Paris 75014 (France)

    2012-01-10T23:59:59.000Z

    Primordial or big bang nucleosynthesis (BBN) is one of the three strong pieces of evidence for the big bang model together with the expansion of the universe and cosmic microwave background radiation. In this study, we improve the standard BBN calculations taking into account new nuclear physics analyses and enlarge the nuclear network up to sodium. This is, in particular, important to evaluate the primitive value of CNO mass fraction that could affect Population III stellar evolution. For the first time we list the complete network of more than 400 reactions with references to the origin of the rates, including Almost-Equal-To 270 reaction rates calculated using the TALYS code. Together with the cosmological light elements, we calculate the primordial beryllium, boron, carbon, nitrogen, and oxygen nuclei. We performed a sensitivity study to identify the important reactions for CNO, {sup 9}Be, and boron nucleosynthesis. We re-evaluated those important reaction rates using experimental data and/or theoretical evaluations. The results are compared with precedent calculations: a primordial beryllium abundance increase by a factor of four compared to its previous evaluation, but we note a stability for B/H and for the CNO/H abundance ratio that remains close to its previous value of 0.7 Multiplication-Sign 10{sup -15}. On the other hand, the extension of the nuclear network has not changed the {sup 7}Li value, so its abundance is still 3-4 times greater than its observed spectroscopic value.

  19. A revised thermonuclear rate of $^{7}$Be($n$,$\\alpha$)$^{4}$He relevant to Big-Bang nucleosynthesis

    E-Print Network [OSTI]

    Hou, S Q; Kubono, S; Chen, Y S

    2015-01-01T23:59:59.000Z

    In the standard Big-Bang nucleosynthesis (BBN) model, the primordial $^7$Li abundance is overestimated by about a factor of 2--3 comparing to the astronomical observations, so called the pending cosmological lithium problem. The $^7$Be($n$,$\\alpha$)$^4$He reaction, which may affect the $^7$Li abundance, was regarded as the secondary important reaction in destructing the $^7$Be nucleus in BBN. However, the thermonuclear rate of $^7$Be($n$,$\\alpha$)$^4$He has not been well studied so far. This reaction rate was firstly estimated by Wagoner in 1969, which has been generally adopted in the current BBN simulations and the reaction rate library. This simple estimation involved only a direct-capture reaction mechanism, but the resonant contribution should be also considered according to the later experimental results. In this work, we have revised this rate based on the indirect cross-section data available for the $^4$He($\\alpha$,$n$)$^7$Be and $^4$He($\\alpha$,$p$)$^7$Li reactions, with the charge symmetry and deta...

  20. A revised thermonuclear rate of $^{7}$Be($n$,$?$)$^{4}$He relevant to Big-Bang nucleosynthesis

    E-Print Network [OSTI]

    S. Q. Hou; J. J. He; S. Kubono; Y. S. Chen

    2015-02-13T23:59:59.000Z

    In the standard Big-Bang nucleosynthesis (BBN) model, the primordial $^7$Li abundance is overestimated by about a factor of 2--3 comparing to the astronomical observations, so called the pending cosmological lithium problem. The $^7$Be($n$,$\\alpha$)$^4$He reaction, which may affect the $^7$Li abundance, was regarded as the secondary important reaction in destructing the $^7$Be nucleus in BBN. However, the thermonuclear rate of $^7$Be($n$,$\\alpha$)$^4$He has not been well studied so far. This reaction rate was firstly estimated by Wagoner in 1969, which has been generally adopted in the current BBN simulations and the reaction rate library. This simple estimation involved only a direct-capture reaction mechanism, but the resonant contribution should be also considered according to the later experimental results. In this work, we have revised this rate based on the indirect cross-section data available for the $^4$He($\\alpha$,$n$)$^7$Be and $^4$He($\\alpha$,$p$)$^7$Li reactions, with the charge symmetry and detailed-balance principle. Our new result shows that the previous rate (acting as an upper limit) is overestimated by about a factor of ten. The BBN simulation shows that the present rate leads to a 1.2\\% increase in the final $^7$Li abundance compared to the result using the Wagoner rate, and hence the present rate even worsens the $^7$Li problem. By the present estimation, the role of $^7$Be($n$,$\\alpha$)$^4$He in destroying $^7$Be is weakened from the secondary importance to the third, and the $^7$Be($d$,$p$)2$^4$He reaction becomes of secondary importance in destructing $^7$Be.

  1. Nucleosynthesis in Type II Supernovae

    E-Print Network [OSTI]

    K. Nomoto; M. Hashimoto; T. Tsujimoto; F. -K. Thielemann; N. Kishimoto; Y. Kubo

    1997-06-03T23:59:59.000Z

    Presupernova evolution and explosive nucleosynthesis in massive stars for main-sequence masses from 13 $M_\\odot$ to 70 $M_\\odot$ are calculated. We examine the dependence of the supernova yields on the stellar mass, $^{12}C(\\alpha, \\gamma) ^{16}O}$ rate, and explosion energy. The supernova yields integrated over the initial mass function are compared with the solar abundances.

  2. Big-Bang Nucleosynthesis and Gamma-Ray Constraints on Cosmic Strings with a large Higgs condensate

    E-Print Network [OSTI]

    H. F. Santana Mota; Mark Hindmarsh

    2015-01-06T23:59:59.000Z

    We consider constraints on cosmic strings from their emission of Higgs particles, in the case that the strings have a Higgs condensate with amplitude of order the string mass scale, assuming that a fraction of the energy of condensate can be turned into radiation near cusps. The injection of energy by the decaying Higgs particles affects the light element abundances predicted by standard Big-Bang Nucleosynthesis (BBN), and also contributes to the Diffuse Gamma-Ray Background (DGRB) in the universe today. We examine the two main string scenarios (Nambu-Goto and field theory), and find that the primordial Helium abundance strongly constrains the string tension and the efficiency of the emission process in the NG scenario, while the strongest BBN constraint in the FT scenario comes from the Deuterium abundance. The Fermi-LAT measurement of the DGRB constrains the field theory scenario even more strongly than previously estimated from EGRET data, requiring that the product of the string tension {\\mu} and Newton's constant G is bounded by G{\\mu} < 2.7x10^{-11}{\\beta}_{ft}^{-2}, where {\\beta}_{ft}^2 is the fraction of the strings' energy going into Higgs particles.

  3. Neutrino-induced nucleosynthesis of A>64 nuclei: The nu p-process

    E-Print Network [OSTI]

    C. Fröhlich; G. Martínez-Pinedo; M. Liebendörfer; F. -K. Thielemann; E. Bravo; W. R. Hix; K. Langanke; N. T. Zinner

    2005-11-12T23:59:59.000Z

    We present a new nucleosynthesis process, that we denote nu p-process, which occurs in supernovae (and possibly gamma-ray bursts) when strong neutrino fluxes create proton-rich ejecta. In this process, antineutrino absorptions in the proton-rich environment produce neutrons that are immediately captured by neutron-deficient nuclei. This allows for the nucleosynthesis of nuclei with mass numbers A >64. Making this process a possible candidate to explain the origin of the solar abundances of 92,94Mo and 96,98Ru. This process also offers a natural explanation for the large abundance of Sr seen in an hyper-metal-poor star.

  4. Nucleosynthesis in Early Neutrino Driven Winds

    SciTech Connect (OSTI)

    Hoffman, R; Fisker, J; Pruet, J; Woosley, S; Janka, H; Buras, R

    2008-01-09T23:59:59.000Z

    Two recent issues related to nucleosynthesis in early proton-rich neutrino winds are investigated. In the first part we investigate the effect of nuclear physics uncertainties on the synthesis of {sup 92}Mo and {sup 94}Mo. Based on recent experimental results, we find that the proton rich winds of the model investigated here can not be the only source of the solar abundance of {sup 92}Mo and {sup 94}Mo. In the second part we investigate the nucleosynthesis from neutron rich bubbles and show that they do not contribute to the nucleosynthesis integrated over both neutron and proton-rich bubbles and proton-rich winds.

  5. Precise Nucleosynthesis Limits on Neutrino Masses

    E-Print Network [OSTI]

    Kimmo Kainulainen

    1996-08-02T23:59:59.000Z

    A computation of nucleosynthesis bounds on the masses of long-lived Dirac and Majorana neutrinos is reviewed. In particular an explicit treatment of the ``differential heating'' of the $\

  6. Neutrino Nucleosynthesis of radioactive nuclei in supernovae

    E-Print Network [OSTI]

    Sieverding, A; Langanke, K; Martínez-Pinedo, G; Heger, A

    2015-01-01T23:59:59.000Z

    We study the neutrino-induced production of nuclides in explosive supernova nucleosynthesis for progenitor stars with solar metallicity and initial main sequence masses between 15 M$_\\odot$ and 40 M$_\\odot$. We improve previous investigations i) by using a global set of partial differential cross sections for neutrino-induced charged- and neutral-current reactions on nuclei with charge numbers $Z < 76 $ and ii) by considering modern supernova neutrino spectra which have substantially lower average energies compared to those previously adopted in neutrino nucleosynthesis studies. We confirm the production of $^7$Li, $^{11}$B, $^{138}$La, and $^{180}$Ta by neutrino nucleosynthesis, albeit at slightly smaller abundances due to the changed neutrino spectra. We find that for stars with a mass smaller than 20 M$_\\odot$, $^{19}$F is produced mainly by explosive nucleosynthesis while for higher mass stars it is produced by the $\

  7. Nucleosynthesis in O-Ne-Mg Supernovae

    SciTech Connect (OSTI)

    Hoffman, R D; Janka, H; Muller, B

    2007-12-18T23:59:59.000Z

    We have studied detailed nucleosynthesis in the shocked surface layers of an oxygen-neon-magnesium core collapse supernova with an eye to determining whether the conditions are suitable for r-process nucleosynthesis. We find no such conditions in an unmodified model, but do find overproduction of N=50 nuclei (previously seen in early neutron-rich neutrino winds) in amounts that, if ejected, would pose serious problems for Galactic chemical evolution.

  8. Nucleosynthesis in Type Ia Supernovae

    E-Print Network [OSTI]

    K. Nomoto; K. Iwamoto; N. Nakasato; F. -K. Thielemann; F. Brachwitz; T. Tsujimoto; Y. Kubo; N. Kishimoto

    1997-06-03T23:59:59.000Z

    Among the major uncertainties involved in the Chandrasekhar mass models for Type Ia supernovae are the companion star of the accreting white dwarf (or the accretion rate that determines the carbon ignition density) and the flame speed after ignition. We present nucleosynthesis results from relatively slow deflagration (1.5 - 3 % of the sound speed) to constrain the rate of accretion from the companion star. Because of electron capture, a significant amount of neutron-rich species such as ^{54}Cr, ^{50}Ti, ^{58}Fe, ^{62}Ni, etc. are synthesized in the central region. To avoid the too large ratios of ^{54}Cr/^{56}Fe and ^{50}Ti/^{56}Fe, the central density of the white dwarf at thermonuclear runaway must be as low as \\ltsim 2 \\e9 \\gmc. Such a low central density can be realized by the accretion as fast as $\\dot M \\gtsim 1 \\times 10^{-7} M_\\odot yr^{-1}$. These rapidly accreting white dwarfs might correspond to the super-soft X-ray sources.

  9. Supernova neutrinos and explosive nucleosynthesis

    SciTech Connect (OSTI)

    Kajino, T. [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan and Department of Astronomy, Graduate School of Science, The University of Tokyo, Hongo 7-3-1, Bunkyo-ku, Tokyo 113-0033 (Japan); Aoki, W. [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Cheoun, M.-K. [Department of Physics, Soongsil University, Seoul 156-743 (Korea, Republic of); Hayakawa, T. [Japan Atomic Energy Agency, Shirakara-Shirane 2-4, Tokai-mura, Ibaraki 319-1195 (Japan); Hidaka, J.; Hirai, Y.; Shibagaki, S. [National Astronomical Observatory, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Mathews, G. J. [Center for Astrophysics, Department of Physics, University of Notre Dame, Notre Dame, IN 46556 (United States); Nakamura, K. [Faculty of Science and Engineering, Waseda University, Ohkubo 3-4-1, Shinjuku, Tokyo 169-8555 (Japan); Suzuki, T. [Department of Physics, College of Humanities and Sciences, Nihon University, Sakurajosui 3-25-40, Setagaya-ku, Tokyo 156-8550 (Japan)

    2014-05-09T23:59:59.000Z

    Core-collapse supernovae eject huge amount of flux of energetic neutrinos. We studied the explosive nucleosyn-thesis in supernovae and found that several isotopes {sup 7}Li, {sup 11}B, {sup 92}Nb, {sup 138}La and {sup 180}Ta as well as r-process nuclei are affected by the neutrino interactions. The abundance of these isotopes therefore depends strongly on the neutrino flavor oscillation due to the Mikheyev-Smirnov-Wolfenstein (MSW) effect. We discuss first how to determine the neutrino temperatures in order to explain the observed solar system abundances of these isotopes, combined with Galactic chemical evolution of the light nuclei and the heavy r-process elements. We then study the effects of neutrino oscillation on their abundances, and propose a novel method to determine the still unknown neutrino oscillation parameters, mass hierarchy and ?{sub 13}, simultaneously. There is recent evidence that SiC X grains from the Murchison meteorite may contain supernova-produced light elements {sup 11}B and {sup 7}Li encapsulated in the presolar grains. Combining the recent experimental constraints on ?{sub 13}, we show that our method sug-gests at a marginal preference for an inverted neutrino mass hierarchy. Finally, we discuss supernova relic neutrinos that may indicate the softness of the equation of state (EoS) of nuclear matter as well as adiabatic conditions of the neutrino oscillation.

  10. Neutron-capture nucleosynthesis in the first stars

    SciTech Connect (OSTI)

    Roederer, Ian U. [Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI 48109 (United States); Preston, George W.; Thompson, Ian B.; Shectman, Stephen A. [Carnegie Observatories, 813 Santa Barbara Street, Pasadena, CA 91101 (United States); Sneden, Christopher, E-mail: iur@umich.edu [Department of Astronomy, University of Texas at Austin, 1 University Station C1400, Austin, TX 78712 (United States)

    2014-04-01T23:59:59.000Z

    Recent studies suggest that metal-poor stars enhanced in carbon but containing low levels of neutron-capture elements may have been among the first to incorporate the nucleosynthesis products of the first generation of stars. We have observed 16 stars with enhanced carbon or nitrogen using the MIKE Spectrograph on the Magellan Telescopes at Las Campanas Observatory and the Tull Spectrograph on the Smith Telescope at McDonald Observatory. We present radial velocities, stellar parameters, and detailed abundance patterns for these stars. Strontium, yttrium, zirconium, barium, europium, ytterbium, and other heavy elements are detected. In four stars, these heavy elements appear to have originated in some form of r-process nucleosynthesis. In one star, a partial s-process origin is possible. The origin of the heavy elements in the rest of the sample cannot be determined unambiguously. The presence of elements heavier than the iron group offers further evidence that zero-metallicity rapidly rotating massive stars and pair instability supernovae did not contribute substantial amounts of neutron-capture elements to the regions where the stars in our sample formed. If the carbon- or nitrogen-enhanced metal-poor stars with low levels of neutron-capture elements were enriched by products of zero-metallicity supernovae only, then the presence of these heavy elements indicates that at least one form of neutron-capture reaction operated in some of the first stars.

  11. High-energy break-up of 6Li as a tool to study the Big-Bang nucleosynthesis reaction 2H(alpha,gamma)6Li

    E-Print Network [OSTI]

    F. Hammache; M. Heil; S. Typel; D. Galaviz; K. Sümmerer; A. Coc; F. Uhlig; F. Attallah; M. Caamano; D. Cortina; H. Geissel; M. Hellström; N. Iwasa; J. Kiener; P. Koczon; B. Kohlmeyer; P. Mohr; E. Schwab; K. Schwarz; F. Schümann; P. Senger; O. Sorlin; V. Tatischeff; J. P. Thibaud; E. Vangioni; A. Wagner; W. Walus

    2010-11-29T23:59:59.000Z

    The recently claimed observations of non-negligible amounts of 6Li in old halo stars have renewed interest in the Big-Bang Nucleosynthesis (BBN) of 6Li. One important ingredient in the predicted BBN abundance of 6Li is the low-energy 2H(alpha,gamma)6Li cross section. Up to now, the only available experimental result for this cross section showed an almost constant astrophysical S-factor below 400 keV, contrary to theoretical expectations. We report on a new measurement of the 2H(alpha,gamma)6Li reaction using the break-up of 6Li at 150 A MeV. Even though we cannot separate experimentally the Coulomb contribution from the nuclear one, we find clear evidence for Coulomb-nuclear interference by analyzing the scattering-angular distributions. This is in-line with our theoretical description which indicates a drop of the S_24-factor at low energies as predicted also by most other models. Consequently, we find even lower upper limits for the calculated primordial 6Li abundance than before.

  12. NUCLEAR ASPECTS OF STELLAR AND EXPLOSIVE NUCLEOSYNTHESIS

    E-Print Network [OSTI]

    Rauscher, Thomas

    NUCLEAR ASPECTS OF STELLAR AND EXPLOSIVE NUCLEOSYNTHESIS Thomas Rauscher 1 , Friedrich. of Astron. and Astroph., Univ. of California, Santa Cruz, CA 95064 Abstract The majority of nuclear­Feshbach). The global parametrizations of the nuclear properties needed for predictions far off stability probe our

  13. Modeling The Nucleosynthesis Of Massive Stars

    E-Print Network [OSTI]

    T. Rauscher

    2003-09-09T23:59:59.000Z

    This overview discusses issues relevant to modeling nucleosynthesis in type II supernovae and implications of detailed studies of the ejecta. After a brief presentation of the most common approaches to stellar evolution and parameterized explosions, the relevance of a number of nuclei to obtain information on the evolution and explosion mechanisms is discussed. The paper is concluded by an outlook on multi-dimensional simulations.

  14. Effect of nuclear structure on Type Ia supernova nucleosynthesis

    E-Print Network [OSTI]

    D. J. Dean

    2000-12-08T23:59:59.000Z

    The relationship among nuclear structure, the weak processes in nuclei, and astrophysics becomes quite apparent in supernova explosion and nucleosynthesis studies. In this brief article, I report on progress made in the last few years on calculating electron capture and beta-decay rates in iron-group nuclei. I also report on applications of these rates to Type-Ia nucleosynthesis studies.

  15. Primordial Nucleosynthesis Constraints on Z' Properties

    E-Print Network [OSTI]

    Vernon Barger; Paul Langacker; Hye-Sung Lee

    2003-02-13T23:59:59.000Z

    In models involving new TeV-scale Z' gauge bosons, the new U(1)' symmetry often prevents the generation of Majorana masses needed for a conventional neutrino seesaw, leading to three superweakly interacting ``right-handed'' neutrinos nu_R, the Dirac partners of the ordinary neutrinos. These can be produced prior to big bang nucleosynthesis by the Z' interactions, leading to a faster expansion rate and too much ^4He. We quantify the constraints on the Z' properties from nucleosynthesis for Z' couplings motivated by a class of E_6 models parametrized by an angle theta_E6. The rate for the annihilation of three approximately massless right-handed neutrinos into other particle pairs through the Z' channel is calculated. The decoupling temperature, which is higher than that of ordinary left-handed neutrinos due to the large Z' mass, is evaluated, and the equivalent number of new doublet neutrinos Delta N_nu is obtained numerically as a function of the Z' mass and couplings for a variety of assumptions concerning the Z-Z' mixing angle and the quark-hadron transition temperature T_c. Except near the values of theta_E6 for which the Z' decouples from the right-handed neutrinos, the Z' mass and mixing constraints from nucleosynthesis are much more stringent than the existing laboratory limits from searches for direct production or from precision electroweak data, and are comparable to the ranges that may ultimately be probed at proposed colliders. For the case T_c = 150 MeV with the theoretically favored range of Z-Z' mixings, Delta N_nu 4.3 TeV for any value of theta_E6. Larger mixing or larger T_c often lead to unacceptably large Delta N_nu except near the nu_R decoupling limit.

  16. Type Ia Supernovae: Simulations and Nucleosynthesis

    E-Print Network [OSTI]

    E. F. Brown; A. C. Calder; T. Plewa; P. M. Ricker; K. Robinson; J. B. Gallagher

    2005-05-19T23:59:59.000Z

    We present our first nucleosynthesis results from a numerical simulation of the thermonuclear disruption of a static cold Chandrasekhar-mass C/O white dwarf. The two-dimensional simulation was performed with an adaptive-mesh Eulerian hydrodynamics code, FLASH, that uses as a flame capturing scheme the evolution of a passive scaler. To compute the isotopic yields and their velocity distribution, 10,000 massless tracer particles are embedded in the star. The particles are advected along streamlines and provide a Lagrangian description of the explosion. We briefly describe our verification tests and preliminary results from post-processing the particle trajectories with a modest (214 isotopes) reaction network.

  17. Constraining spacetime noncommutativity with primordial nucleosynthesis

    SciTech Connect (OSTI)

    Horvat, Raul [Physics Division, Rudjer Boskovic Institute, Zagreb (Croatia); Trampetic, Josip [Theoretical Physics Division, Rudjer Boskovic Institute, Zagreb (Croatia)

    2009-04-15T23:59:59.000Z

    We discuss a constraint on the scale {lambda}{sub NC} of noncommutative (NC) gauge field theory arising from consideration of the big bang nucleosynthesis of light elements. The propagation of neutrinos in the NC background described by an antisymmetric tensor {theta}{sup {mu}}{sup {nu}} does result in a tree-level vectorlike coupling to photons in a generation-independent manner, raising thus a possibility to have an appreciable contribution of three light right-handed (RH) fields to the energy density of the Universe at nucleosynthesis time. Considering elastic scattering processes of the RH neutrinos off charged plasma constituents at a given cosmological epoch, we obtain for a conservative limit on an effective number of additional doublet neutrinos {delta}N{sub {nu}}=1, a bound {lambda}{sub NC} > or approx. 3 TeV. With a more stringent requirement, {delta}N{sub {nu}} < or approx. 0.2, the bound is considerably improved, {lambda}{sub NC} > or approx. 10{sup 3} TeV. For our bounds the {theta} expansion of the NC action stays always meaningful, since the decoupling temperature of the RH species is perseveringly much less than the inferred bound for the scale of noncommutativity.

  18. Green Power Offer (Maine)

    Broader source: Energy.gov [DOE]

    This chapter establishes requirements, standards and procedures and a competitive bidding process to implement the green power offer program. The program is designed to make renewable energy...

  19. Electron capture cross sections for stellar nucleosynthesis

    E-Print Network [OSTI]

    Giannaka, P G

    2015-01-01T23:59:59.000Z

    In the first stage of this work, we perform detailed calculations for the cross sections of the electron capture on nuclei under laboratory conditions. Towards this aim we exploit the advantages of a refined version of the proton-neutron quasi-particle random-phase approximation (pn-QRPA) and carry out state-by-state evaluations of the rates of exclusive processes that lead to any of the accessible transitions within the chosen model space. In the second stage of our present study, we translate the above mentioned $e^-$-capture cross sections to the stellar environment ones by inserting the temperature dependence through a Maxwell-Boltzmann distribution describing the stellar electron gas. As a concrete nuclear target we use the $^{66}Zn$ isotope, which belongs to the iron group nuclei and plays prominent role in stellar nucleosynthesis at core collapse supernovae environment.

  20. Effects of a torsion field on Big Bang nucleosynthesis

    E-Print Network [OSTI]

    M. Brüggen

    1999-06-25T23:59:59.000Z

    In this paper it is investigated whether torsion, which arises naturally in most theories of quantum gravity, has observable implications for the Big Bang nucleosynthesis. Torsion can lead to spin flips amongst neutrinos thus turning them into sterile neutrinos. In the early Universe they can alter the helium abundance which is tightly constrained by observations. Here I calculate to what extent torsion of the string theory type leads to a disagreement with the Big Bang nucleosynthesis predictions.

  1. Challenges in explosive nucleosynthesis of heavy elements

    SciTech Connect (OSTI)

    Pinedo, Gabriel Martinez; Fischer, T.; Lohs, A.; Huther, L. [Institut fuer Kernphysik, Technische Universitaet Darmstadt, Schlossgartenstrasse 2, 64289 Darmstadt, Germany and GSI Helmholtzzentrum fuer Schwerioneneforschung, Planckstrasse 1, 64291 Darmstadt (Germany); GSI Helmholtzzentrum fuer Schwerioneneforschung, Planckstrasse 1, 64291 Darmstadt, Germany and Institut fuer Kernphysik, Technische Universitaet Darmstadt, Schlossgartenstrasse 2, 64289 Darmstadt (Germany); Institut fuer Kernphysik, Technische Universitaet Darmstadt, Schlossgartenstrasse 2, 64289 Darmstadt (Germany)

    2012-10-20T23:59:59.000Z

    We show that a treatment of charged-current neutrino interactions in hot and dense matter that is consistent with the nuclear equation of state has a strong impact on the spectra of the neutrinos emitted during the deleptonization period of a protoneutron star formed in a core-collapse supernova. We compare results of simulations including and neglecting mean field effects on the neutrino opacities. Their inclusion reduces the luminosities of all neutrino flavors and enhances the spectral differences between electron neutrino and antineutrino. The magnitude of the difference depends on the equation of state and in particular on the symmetry energy at sub-nuclear densities. These modifications reduce the proton-to-nucleon ratio of the neutrino-driven outflow, increasing slightly their entropy. They are expected to have a substantial impact on the nucleosynthesis in neutrino-driven winds, even though they do not result in conditions that favor an r-process. Contrarily to previous findings, our simulations show that the spectra of electron neutrinos remain substantially different from those of other (anti)neutrino flavors during the entire deleptonization phase of the protoneutron star. The obtained luminosity and spectral changes are also expected to have important consequences for neutrino flavor oscillations and neutrino detection on Earth.

  2. Sport Management Academic Offerings

    E-Print Network [OSTI]

    Mather, Patrick T.

    production and programming of events; marketing and public relations; technological operations management including (but not limited to) digital advertising, media law, new media business, operations managementSport Management Academic Offerings M.S. In Sport Venue And Event Management GRADUATE Chad Mc

  3. Heavy element nucleosynthesis in jets from collapsars

    SciTech Connect (OSTI)

    Fujimoto, Shin-ichirou [Department of Electronic Control, Kumamoto National College of Technology, Kumamoto 861-1102 (Japan); Institut d'Astronomie et d'Astrophysique, Universite libre de Bruxelles, CP226 Boulevard du Triomphe, B-1050 Brussels (Belgium); Hashimoto, Masa-aki [Department of Physics, School of Sciences, Kyushu University, Fukuoka 810-8560 (Japan); Kotake, Kei [Division of Theoretical Astronomy, National Astronomical Observatory Japan, 2-21-1, Osawa, Mitaka, Tokyo, 181-8588 (Japan); Yamada, Shoichi [Science and Engineering, Waseda University, 3-4-1 Okubo, Shinjuku, Tokyo 169-8555 (Japan); Advanced Research Institute for Science and Engineering, Waseda University, 3-4-1 Okubo, Shinjuku, Tokyo 169-8555 (Japan)

    2007-02-26T23:59:59.000Z

    We investigate nucleosynthesis in collapsars, based on long-term, magnetohydrodynamic simulations of a rapidly rotating massive star of 40M{center_dot} during the core collapse. We have calculated detailed composition of magnetically driven jets ejected from the collapsars, in which the magnetic fields before the collapse, are uniform and parallel to the rotational axis of the star and the magnitudes of the fields, B0, are 1010 G or 1012 G. We follow the evolution of chemical composition up to about 4000 nuclides inside the jets from the collapse phase to the ejection phase through the jet generation phase with use of a large nuclear reaction network. We find that the r-process successfully operates in the jets from the collapsar of B0 = 1012 G, so that U and Th are synthesized abundantly. Abundance pattern inside the jets is similar to that of r-elements in the solar system. Furthermore, we find that p-nuclei are produced without seed nuclei: not only light p-nuclei, such as 74Se, 78Kr, 84Sr, and 92Mo, but also heavy p-nuclei, 113In, 115Sn, and 138La, can be abundantly synthesized in the jets. The amounts of p-nuclei in the ejecta are much greater than those in core-collapse supernovae (SNe). In particular, 92Mo, 113In, 115Sn, and 138La deficient in the SNe, are significantly produced in the ejecta. On the other hand, in the jets from the collapsar of B0 = 1010 G, the r-process cannot operate and 56Ni, 28Si, 32S, and 4He are abundantly synthesized in the jets, as in ejecta from inner layers of Type II supernovae. An amount of 56Ni is much smaller than that from SN 1987A.

  4. Neutrinos and nucleosynthesis in core-collapse supernovae

    SciTech Connect (OSTI)

    Fröhlich, C.; Casanova, J. [Department of Physics, North Carolina State University, Raleigh, NC, 27695 (United States); Hempel, M.; Liebendörfer, M. [Departement für Physik, Universität Basel, CH-4056 Basel (Switzerland); Melton, C. A. [Department of Physics, North Carolina State University, Raleigh, NC 27695 (United States); Perego, A. [Institut für Kernphysik, Technische Universität Darmstadt, D-64289 Darmstadt (Germany)

    2014-01-01T23:59:59.000Z

    Massive stars (M > 8-10 M{sub ?}) undergo core collapse at the end of their life and explode as supernova with ~ 10?¹ erg of kinetic energy. While the detailed supernova explosion mechanism is still under investigation, reliable nucleosynthesis calculations based on successful explosions are needed to explain the observed abundances in metal-poor stars and to predict supernova yields for galactic chemical evolution studies. To predict nucleosynthesis yields for a large number of progenitor stars, computationally efficient explosion models are required. We model the core collapse, bounce and subsequent explosion of massive stars assuming spherical symmetry and using detailed microphysics and neutrino physics combined with a novel method to artificially trigger the explosion (PUSH). We discuss the role of neutrinos, the conditions in the ejecta, and the resulting nucleosynthesis.

  5. Statistical Methods for Thermonuclear Reaction Rates and Nucleosynthesis Simulations

    E-Print Network [OSTI]

    Iliadis, Christian; Coc, Alain; Timmes, F X; Champagne, Art E

    2014-01-01T23:59:59.000Z

    Rigorous statistical methods for estimating thermonuclear reaction rates and nucleosynthesis are becoming increasingly established in nuclear astrophysics. The main challenge being faced is that experimental reaction rates are highly complex quantities derived from a multitude of different measured nuclear parameters (e.g., astrophysical S-factors, resonance energies and strengths, particle and gamma-ray partial widths). We discuss the application of the Monte Carlo method to two distinct, but related, questions. First, given a set of measured nuclear parameters, how can one best estimate the resulting thermonuclear reaction rates and associated uncertainties? Second, given a set of appropriate reaction rates, how can one best estimate the abundances from nucleosynthesis (i.e., reaction network) calculations? The techniques described here provide probability density functions that can be used to derive statistically meaningful reaction rates and final abundances for any desired coverage probability. Examples ...

  6. Nucleosynthesis in the accretion disks of Type II collapsars

    E-Print Network [OSTI]

    Indrani Banerjee; Banibrata Mukhopadhyay

    2013-05-08T23:59:59.000Z

    We investigate nucleosynthesis inside the gamma-ray burst (GRB) accretion disks formed by the Type II collapsars. In these collapsars, the core collapse of massive stars first leads to the formation of a proto-neutron star and a mild supernova explosion is driven. However, this supernova ejecta lack momentum and falls back onto the neutron star which gets transformed to a stellar mass black hole. In order to study the hydrodynamics and nucleosynthesis of such an accretion disk formed from the fallback material of the supernova ejecta, we use the well established hydrodynamic models. In such a disk neutrino cooling becomes important in the inner disk where the temperature and density are higher. Higher the accretion rate (dot{M}), higher is the density and temperature in the disks. In this work we deal with accretion disks with relatively low accretion rates: 0.001 M_sun s^{-1} \\lesssim dot{M} \\lesssim 0.01 M_sun s^{-1} and hence these disks are predominantly advection dominated. We use He-rich and Si-rich abundances as the initial condition of nucleosynthesis at the outer disk, and being equipped with the disk hydrodynamics and the nuclear network code, we study the abundance evolution as matter inflows and falls into the central object. We investigate the variation in the nucleosynthesis products in the disk with the change in the initial abundance at the outer disk and also with the change in the mass accretion rate. We report the synthesis of several unusual nuclei like {31}P, {39}K, {43}Sc, {35}Cl, and various isotopes of titanium, vanadium, chromium, manganese and copper. We also confirm that isotopes of iron, cobalt, nickel, argon, calcium, sulphur and silicon get synthesized in the disk, as shown by previous authors. Much of these heavy elements thus synthesized are ejected from the disk via outflows and hence they should leave their signature in observed data.

  7. Nucleosynthesis and Remnants in Massive Stars of Solar Metallicity

    E-Print Network [OSTI]

    Woosley, S E

    2007-01-01T23:59:59.000Z

    Hans Bethe contributed in many ways to our understanding of the supernovae that happen in massive stars, but, to this day, a first principles model of how the explosion is energized is lacking. Nevertheless, a quantitative theory of nucleosynthesis is possible. We present a survey of the nucleosynthesis that occurs in 32 stars of solar metallicity in the mass range 12 to 120 solar masses. The most recent set of solar abundances, opacities, mass loss rates, and current estimates of nuclear reaction rates are employed. Restrictions on the mass cut and explosion energy of the supernovae based upon nucleosynthesis, measured neutron star masses, and light curves are discussed and applied. The nucleosynthetic results, when integrated over a Salpeter initial mass function (IMF), agree quite well with what is seen in the sun. We discuss in some detail the production of the long lived radioactivities, 26Al and 60Fe, and why recent model-based estimates of the ratio 60Fe/26Al are overly large compared with what satelli...

  8. Statistical Methods for Thermonuclear Reaction Rates and Nucleosynthesis Simulations

    E-Print Network [OSTI]

    Christian Iliadis; Richard Longland; Alain Coc; F. X. Timmes; Art E. Champagne

    2014-09-19T23:59:59.000Z

    Rigorous statistical methods for estimating thermonuclear reaction rates and nucleosynthesis are becoming increasingly established in nuclear astrophysics. The main challenge being faced is that experimental reaction rates are highly complex quantities derived from a multitude of different measured nuclear parameters (e.g., astrophysical S-factors, resonance energies and strengths, particle and gamma-ray partial widths). We discuss the application of the Monte Carlo method to two distinct, but related, questions. First, given a set of measured nuclear parameters, how can one best estimate the resulting thermonuclear reaction rates and associated uncertainties? Second, given a set of appropriate reaction rates, how can one best estimate the abundances from nucleosynthesis (i.e., reaction network) calculations? The techniques described here provide probability density functions that can be used to derive statistically meaningful reaction rates and final abundances for any desired coverage probability. Examples are given for applications to s-process neutron sources, core-collapse supernovae, classical novae, and big bang nucleosynthesis.

  9. Offered: Offered: Position(s): Position(s)

    E-Print Network [OSTI]

    New Hampshire, University of

    Company: Industry: Website: Majors: Offered: Offered: Position(s): Position(s): Description the future for streamlined operations. B2W Software solutions effectively leverage the latest technologies into a unified system approach for estimating and bidding, field tracking and analysis, resource planning

  10. Revisiting shock-driven exploding pushers: Insights into plasma flows and fields, stopping power, nucleosynthesis, and

    E-Print Network [OSTI]

    topics such as nucleosynthesis and kinetic and/or multi-ion fluid phenomena. For nucleosynthesis the fuel plasma density is sufficiently low and the temperature sufficiently high. Such conditions lend domain, the issue of multi-ion fluid effects, as opposed to the "average" single-ion fluid approximation

  11. Collaborative Research: Neutrinos & Nucleosynthesis in Hot Dense Matter

    SciTech Connect (OSTI)

    Reddy, Sanjay

    2013-09-06T23:59:59.000Z

    It is now firmly established that neutrinos, which are copiously produced in the hot and dense core of the supernova, play a role in the supernova explosion mechanism and in the synthesis of heavy elements through a phenomena known as r-process nucleosynthesis. They are also detectable in terrestrial neutrino experiments, and serve as a probe of the extreme environment and complex dynamics encountered in the supernova. The major goal of the UW research activity relevant to this project was to calculate the neutrino interaction rates in hot and dense matter of relevance to core collapse supernova. These serve as key input physics in large scale computer simulations of the supernova dynamics and nucleosynthesis being pursued at national laboratories here in the United States and by other groups in Europe and Japan. Our calculations show that neutrino production and scattering rate are altered by the nuclear interactions and that these modifications have important implications for nucleosynthesis and terrestrial neutrino detection. The calculation of neutrino rates in dense matter are difficult because nucleons in the dense matter are strongly coupled. A neutrino interacts with several nucleons and the quantum interference between scattering off different nucleons depends on the nature of correlations between them in dense matter. To describe these correlations we used analytic methods based on mean field theory and hydrodynamics, and computational methods such as Quantum Monte Carlo. We found that due to nuclear effects neutrino production rates at relevant temperatures are enhanced, and that electron neutrinos are more easily absorbed than anti-electron neutrinos in dense matter. The latter, was shown to favor synthesis of heavy neutron-rich elements in the supernova.

  12. Big Bang nucleosynthesis and the baryonic content of the universe

    E-Print Network [OSTI]

    T. X. Thuan; Y. I. Izotov

    2000-12-18T23:59:59.000Z

    A review of the latest measurements of the primordial abundances of the light nuclei D, 3He, 4He and 7Li is given. We discuss in particular the primordial abundance Yp of 4He as measured in blue compact dwarf galaxies. We argue that the best measurements now give a ``high'' value of Yp along with a ``low'' value of D/H, and that the two independent measurements are consistent within the framework of standard Big Bang nucleosynthesis with a number of light neutrino species Nnu = 3.0+/-0.3 (2sigma).

  13. Nucleosynthesis in the Outflow from Gamma Ray Burst Accretion Disks

    E-Print Network [OSTI]

    R. Surman; G. C. McLaughlin; W. R. Hix

    2005-09-13T23:59:59.000Z

    We examine the nucleosynthesis products that are produced in the outflow from rapidly accreting disks. We find that the type of element synthesis varies dramatically with the degree of neutrino trapping in the disk and therefore the accretion rate of the disk. Disks with relatively high accretion rates such as 10 M_solar/s can produce very neutron rich nuclei that are found in the r process. Disks with more moderate accretion rates can produce copious amounts of Nickel as well as the light elements such as Lithium and Boron. Disks with lower accretion rates such as 0.1 M_solar/s produce large amounts of Nickel as well as some unusual nuclei such as Ti-49, Sc-45, Zn-64, and Mo-92. This wide array of potential nucleosynthesis products is due to the varying influence of electron neutrinos and antineutrinos emitted from the disk on the neutron-to-proton ratio in the outflow. We use a parameterization for the outflow and discuss our results in terms of entropy and outflow acceleration.

  14. Neutrino-driven wind simulations and nucleosynthesis of heavy elements

    E-Print Network [OSTI]

    A. Arcones; F. -K. Thielemann

    2012-07-11T23:59:59.000Z

    Neutrino-driven winds, which follow core-collapse supernova explosions, present a fascinating nuclear astrophysics problem that requires understanding advanced astrophysics simulations, the properties of matter and neutrino interactions under extreme conditions, the structure and reactions of exotic nuclei, and comparisons against forefront astronomical observations. The neutrino-driven wind has attracted vast attention over the last 20 years as it was suggested to be a candidate for the astrophysics site where half of the heavy elements are produced via the r-process. In this review, we summarize our present understanding of neutrino-driven winds from the dynamical and nucleosynthesis perspectives. Rapid progress has been made during recent years in understanding the wind with improved simulations and better micro physics. The current status of the fields is that hydrodynamical simulations do not reach the extreme conditions necessary for the r-process and the proton or neutron richness of the wind remains to be investigated in more detail. However, nucleosynthesis studies and observations point already to neutrino-driven winds to explain the origin of lighter heavy elements, such as Sr, Y, Zr.

  15. Primordial Lithium Abundance in Catalyzed Big Bang Nucleosynthesis

    E-Print Network [OSTI]

    Chris Bird; Kristen Koopmans; Maxim Pospelov

    2008-05-19T23:59:59.000Z

    There exists a well known problem with the Li7+Be7 abundance predicted by standard big bang nucleosynthesis being larger than the value observed in population II stars. The catalysis of big bang nucleosynthesis by metastable, \\tau_X \\ge 10^3 sec, charged particles X^- is capable of suppressing the primordial Li7+Be7, abundance and making it consistent with the observations. We show that to produce the correct abundance, this mechanism of suppression places a requirement on the initial abundance of X^- at temperatures of 4\\times 10^8 K to be on the order of or larger than 0.02 per baryon, which is within the natural range of abundances in models with metastable electroweak-scale particles. The suppression of Li7+Be7, is triggered by the formation of (Be7X^-), compound nuclei, with fast depletion of their abundances by catalyzed proton reactions, and in some models by direct capture of X^- on Be7. The combination of Li7+Be7 and Li6 constraints favours the window of lifetimes, 1000s \\la tau_X \\leq 2000 s.

  16. Comprehensive nucleosynthesis analysis for ejecta of compact binary mergers

    E-Print Network [OSTI]

    Just, Oliver; Pulpillo, Ricard Ardevol; Goriely, Stephane; Janka, H -Thomas

    2015-01-01T23:59:59.000Z

    We present a comprehensive study of r-process element nucleosynthesis in the ejecta of compact binary mergers (CBMs) and their relic black-hole (BH)-torus systems. The evolution of the BH-accretion tori is simulated for seconds with a Newtonian hydrodynamics code including viscosity effects, pseudo-Newtonian gravity for rotating BHs, and an energy-dependent two-moment closure scheme for the transport of electron neutrinos and antineutrinos. The investigated cases are guided by relativistic double neutron star (NS-NS) and NS-BH merger models, producing ~3-6 Msun BHs with rotation parameters of A~0.8 and tori of 0.03-0.3 Msun. Our nucleosynthesis analysis includes the dynamical (prompt) ejecta expelled during the CBM phase and the neutrino and viscously driven outflows of the relic BH-torus systems. While typically ~20-25% of the initial accretion-torus mass are lost by viscously driven outflows, neutrino-powered winds contribute at most another ~1%, but neutrino heating enhances the viscous ejecta significantl...

  17. Explosive Nucleosynthesis in GRB Jets Accompanied by Hypernovae

    SciTech Connect (OSTI)

    Nagataki, Shigehiro; /Kyoto U., Yukawa Inst., Kyoto /KIPAC, Menlo Park; Mizuta, Akira; /Garching, Max Planck Inst.; Sato, Katsuhiko; /Tokyo U. /Tokyo U., RESCEU

    2006-09-21T23:59:59.000Z

    Two-dimensional hydrodynamic simulations are performed to investigate explosive nucleosynthesis in a collapsar using the model of MacFadyen and Woosley (1999). It is shown that {sup 56}Ni is not produced in the jet of the collapsar sufficiently to explain the observed amount of a hypernova when the duration of the explosion is {approx} 10 sec, which is considered to be the typical timescale of explosion in the collapsar model. Even though a considerable amount of {sup 56}Ni is synthesized if all explosion energy is deposited initially, the opening angles of the jets become too wide to realize highly relativistic outflows and gamma-ray bursts in such a case. From these results, it is concluded that the origin of {sup 56}Ni in hypernovae associated with GRBs is not the explosive nucleosynthesis in the jet. We consider that the idea that the origin is the explosive nucleosynthesis in the accretion disk is more promising. We also show that the explosion becomes bi-polar naturally due to the effect of the deformed progenitor. This fact suggests that the {sup 56}Ni synthesized in the accretion disk and conveyed as outflows are blown along to the rotation axis, which will explain the line features of SN 1998bw and double peaked line features of SN 2003jd. Some fraction of the gamma-ray lines from {sup 56}Ni decays in the jet will appear without losing their energies because the jet becomes optically thin before a considerable amount of {sup 56}Ni decays as long as the jet is a relativistic flow, which may be observed as relativistically Lorentz boosted line profiles in future. We show that abundance of nuclei whose mass number {approx} 40 in the ejecta depends sensitively on the energy deposition rate, which is a result of incomplete silicon burning and alpha-rich freezeout. So it may be determined by observations of chemical composition in metal poor stars which model is the proper one as a model of a gamma-ray burst accompanied by a hypernova.

  18. Offered jointly with International Business

    E-Print Network [OSTI]

    Offered jointly with Master in International Business #12;.02 Welcome to Barcelona Welcome to UPF Pompeu Fabra (UPF), in the very heart of Barcelona. UPF is a public institution established in 1990, and is integrated into the urban fabric of the city, contributing to and participating in its dynamism. The UPF has

  19. technology offer Who we are

    E-Print Network [OSTI]

    Szmolyan, Peter

    and the requirement of liquid nitrogen cooled detectors. The proposed sensor system only measures the IR absorbance spectrum between 2 and 20 µm, requiring liquid nitrogen cooling the proposed sensor system only recordstechnology offer Who we are: Vienna University of Technology, Research and Transfer Support Tel

  20. Nucleosynthesis of heavy elements in gamma ray bursts

    E-Print Network [OSTI]

    ,

    2015-01-01T23:59:59.000Z

    The ultrarelativistic jets responsible for prompt and afterglow emission in gamma ray bursts are presumably driven by a central engine that consists of a dense accretion disk around a spinning black hole. We consider such engine, composed of free nucleons, electron-positron pairs, Helium nuclei, and cooled by neutrino emission. A significant number density of neutrons in the disk provide conditions for neutron rich plasma in the outflows and jets. Heavy nuclei are also formed in the accretion flow, at the distances 150-250 gravitational radii from the black hole. We study the process of nucleosynthesis in the GRB engine, depending on its physical properties. Our results may have important observational implications for the jet deceleration process and heavy elements observed in the spectra of GRB afterglows.

  1. Beta decay rates for nuclei with 115 < A < 140 for r-process nucleosynthesis

    E-Print Network [OSTI]

    Kamales Kar; Soumya Chakravarti; V. R. Manfredi

    2006-03-19T23:59:59.000Z

    For r-process nucleosynthesis the beta decay rates for a number of neutron-rich intermediate heavy nuclei are calculated. The model for the beta strength function is able to reproduce the observed half~lives quite well.

  2. Sharyland Utilities- Residential Standard Offer Program

    Broader source: Energy.gov [DOE]

    Sharyland Utilities offers the Residential and "Hard-to-Reach" Standard Offer Programs, which encourage residential customers to pursue energy saving measures and equipment upgrades in their homes....

  3. Sharyland Utilities- Commercial Standard Offer Program (Texas)

    Broader source: Energy.gov [DOE]

    Sharyland Utilities offers the Residential and "Hard-to-Reach" Standard Offer Programs, which encourage residential customers to pursue energy saving measures and equipment upgrades in their homes....

  4. Supernova nucleosynthesis and the physics of neutrino oscillation

    SciTech Connect (OSTI)

    Kajino, Toshitaka [National Astronomical Observatory, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan) and Department of Astronomy, Graduate School of Science, University of Tokyo, Hongo 7-3-1, Bunkyo-ku, Tokyo 113-0033 (Japan)

    2012-11-20T23:59:59.000Z

    We studied the explosive nucleosynthesis in core-collapse supernovae and found that several isotopes of rare elements like {sup 7}Li, {sup 11}B, {sup 138}La, {sup 180}Ta and others are predominantly produced by the neutrino interactions with several abundant nuclei. These isotopes are strongly affected by the neutrino flavor oscillation due to the MSW (Mikheyev-Smirnov-Wolfenstein) effect. We here first study how to know the suitable average neutrino temperatures in order to explain the observed solar system abundances of these isotopes, combined with Galactic chemical evolution of the light nuclei and the heavy r-process elements. We then study the neutrino oscillation effects on their abundances, and propose a new novel method to determine the neutrino oscillation parameters, {theta}{sub 13} and mass hierarchy, simultaneously. There is recent evidence that some SiC X grains from the Murchison meteorite may contain supernova-produced neutrino-process {sup 11}B and {sup 7}Li encapsulated in the grains. Combining the recent experimental constraints on {theta}{sub 13}, we show that although the uncertainties are still large, our method hints at a marginal preference for an inverted neutrino mass hierarchy for the first time.

  5. The r-process nucleosynthesis: Nuclear physics challenges

    SciTech Connect (OSTI)

    Goriely, S. [Institut d'Astronomie et d'Astrophysique, Universite Libre de Bruxelles Campus de la Plaine, CP 226, 1050 Brussels (Belgium)

    2012-10-20T23:59:59.000Z

    About half of the nuclei heavier than iron observed in nature are produced by the socalled rapid neutron capture process, or r-process, of nucleosynthesis. The identification of the astrophysics site and the specific conditions in which the r-process takes place remains, however, one of the still-unsolved mysteries of modern astrophysics. Another underlying difficulty associated with our understanding of the r-process concerns the uncertainties in the predictions of nuclear properties for the few thousands exotic neutron-rich nuclei involved and for which essentially no experimental data exist. The present contribution emphasizes some important future challenges faced by nuclear physics in this problem, particularly in the determination of the nuclear structure properties of exotic neutron-rich nuclei as well as their radiative neutron capture rates and their fission probabilities. These quantities are particularly relevant to determine the composition of the matter resulting from the r-process. Their impact on the r-abundance distribution resulting from the decompression of neutron star matter is discussed.

  6. Pasta Nucleosynthesis: Molecular dynamics simulations of nuclear statistical equilibrium

    E-Print Network [OSTI]

    M. E. Caplan; A. S. Schneider; C. J. Horowitz; D. K. Berry

    2014-12-29T23:59:59.000Z

    Background: Exotic non-spherical nuclear pasta shapes are expected in nuclear matter at just below saturation density because of competition between short range nuclear attraction and long range Coulomb repulsion. Purpose: We explore the impact of nuclear pasta on nucleosynthesis, during neutron star mergers, as cold dense nuclear matter is ejected and decompressed. Methods: We perform classical molecular dynamics simulations with 51200 and 409600 nucleons, that are run on GPUs. We expand our simulation region to decompress systems from an initial density of 0.080 fm^{-3} down to 0.00125 fm^{-3}. We study proton fractions of Y_P=0.05, 0.10, 0.20, 0.30, and 0.40 at T =0.5, 0.75, and 1.0 MeV. We calculate the composition of the resulting systems using a cluster algorithm. Results: We find final compositions that are in good agreement with nuclear statistical equilibrium models for temperatures of 0.75 and 1 MeV. However, for proton fractions greater than Y_P=0.2 at a temperature of T = 0.5 MeV, the MD simulations produce non-equilibrium results with large rod-like nuclei. Conclusions: Our MD model is valid at higher densities than simple nuclear statistical equilibrium models and may help determine the initial temperatures and proton fractions of matter ejected in mergers.

  7. The Effects of Thermonuclear Reaction Rate Variations on Nova Nucleosynthesis: A Sensitivity Study

    E-Print Network [OSTI]

    Christian Iliadis; Art Champagne; Jordi Jose; Sumner Starrfield; Paul Tupper

    2002-06-03T23:59:59.000Z

    We investigate the effects of thermonuclear reaction rate uncertainties on nova nucleosynthesis. One-zone nucleosynthesis calculations have been performed by adopting temperature-density-time profiles of the hottest hydrogen-burning zone (i.e., the region in which most of the nucleosynthesis takes place). We obtain our profiles from 7 different, recently published, hydrodynamic nova simulations covering peak temperatures in the range from Tpeak=0.145-0.418 GK. For each of these profiles, we individually varied the rates of 175 reactions within their associated errors and analyzed the resulting abundance changes of 142 isotopes in the mass range below A=40. In total, we performed 7350 nuclear reaction network calculations. We use the most recent thermonuclear reaction rate evaluations for the mass ranges A=1-20 and A=20-40. For the theoretical astrophysicist, our results indicate the extent to which nova nucleosynthesis calculations depend on presently uncertain nuclear physics input, while for the experimental nuclear physicist our results represent at least a qualitative guide for future measurements at stable and radioactive ion beam facilities. We find that present reaction rate estimates are reliable for predictions of Li, Be, C and N abundances in nova nucleosynthesis. However, rate uncertainties of several reactions have to be reduced significantly in order to predict more reliable O, F, Ne, Na, Mg, Al, Si, S, Cl and Ar abundances. Results are presented in tabular form for each adopted nova simulation.

  8. Sensitivity study of explosive nucleosynthesis in Type Ia supernovae: I. Modification of individual thermonuclear reaction rates

    E-Print Network [OSTI]

    Eduardo Bravo; Gabriel Martínez-Pinedo

    2012-04-09T23:59:59.000Z

    We explore the sensitivity of the nucleosynthesis due to type Ia supernovae with respect to uncertainties in nuclear reaction rates. We have adopted a standard one-dimensional delayed detonation model of the explosion of a Chandrasekhar-mass white dwarf, and have post-processed the thermodynamic trajectories of every mass-shell with a nucleosynthetic code, with increases (decreases) by a factor of ten on the rates of 1196 nuclear reactions. We have computed as well hydrodynamic models for different rates of the fusion reactions of 12C and of 16O. For selected reactions, we have recomputed the nucleosynthesis with alternative prescriptions for their rates taken from the JINA REACLIB database, and have analyzed the temperature ranges where modifications of their rates have the strongest effect on nucleosynthesis. The nucleosynthesis resulting from the Type Ia supernova models is quite robust with respect to variations of nuclear reaction rates, with the exception of the reaction of fusion of 12C nuclei. The energy of the explosion changes by less than \\sim4%. The changes in the nucleosynthesis due to the modification of the rates of fusion reactions are as well quite modest, for instance no species with a mass fraction larger than 0.02 experiences a variation of its yield larger than a factor of two. We provide the sensitivity of the yields of the most abundant species with respect to the rates of the most intense reactions with protons, neutrons, and alphas. In general, the yields of Fe-group nuclei are more robust than the yields of intermediate-mass elements. Among the charged particle reactions, the most influential on supernova nucleosynthesis are 30Si + p \\rightleftarrows 31P + {\\gamma}, 20Ne + {\\alpha} \\rightleftarrows 24Mg + {\\gamma}, and 24Mg + {\\alpha} \\rightleftarrows 27Al + p. The temperatures at which a modification of their rate has a larger impact are in the range 2 < T < 4 GK. (abridged)

  9. Lithium in cool stellar atmospheres: Big bang nucleosynthesis and extrasolar planets

    E-Print Network [OSTI]

    Lithium in cool stellar atmospheres: Big bang nucleosynthesis and extrasolar planets Matthias Steffen and Elisabetta Caffau Sternphysik In metal-poor stellar atmospheres, the Lithium line at 6707 Ã?-NLTE, respectively. The accurate spectroscopic determination of the Lithium abundance and in particular the 6Li/7Li

  10. Denton Municipal Electric- Standard Offer Rebate Program

    Broader source: Energy.gov [DOE]

    Within the GreenSense program, Denton Municipal Electric's Standard Offer Program provides rebates to large commercial and industrial customers for lighting retrofits, HVAC upgrades and motor...

  11. Savings by Design (Offered by five Utilities)

    Broader source: Energy.gov [DOE]

    In conjunction with the California Department of Public Utilities, Savings by Design offers services and incentives to help owners and designers of commercial buildings raise energy performance....

  12. ORIGINAL ARTICLE Offer Shai Efim Mohr

    E-Print Network [OSTI]

    Shai, Offer

    ORIGINAL ARTICLE Offer Shai Æ Efim Mohr Transforming engineering knowledge through graph introduces an approach for trans- forming methods and knowledge between different engineering fields through ways of conducting engineering research by enabling a systematic derivation of engineering knowledge

  13. Plant Diagnostic Clinic Services Offered & Fees

    E-Print Network [OSTI]

    Plant Diagnostic Clinic Services Offered & Fees Make the Most of a Beneficial Facility Visual without notice. Location Jefferson County Plant Diagnostic Clinic 15200 West 6th Avenue, Unit C Golden, CO

  14. Effects of neutrino oscillations on nucleosynthesis and neutrino signals for an 18 M supernova model

    E-Print Network [OSTI]

    Wu, Meng-Ru; Martinez-Pinedo, Gabriel; Fischer, Tobias; Huther, Lutz

    2014-01-01T23:59:59.000Z

    In this paper, we explore the effects of neutrino flavor oscillations on supernova nucleosynthesis and on the neutrino signals. Our study is based on detailed information about the neutrino spectra and their time evolution from a spherically-symmetric supernova model for an 18 M progenitor. We find that collective neutrino oscillations are not only sensitive to the detailed neutrino energy and angular distributions at emission, but also to the time evolution of both the neutrino spectra and the electron density profile. We apply the results of neutrino oscillations to study the impact on supernova nucleosynthesis and on the neutrino signals from a Galactic supernova. We show that in our supernova model, collective neutrino oscillations enhance the production of rare isotopes 138La and 180Ta but have little impact on the nu p-process nucleosynthesis. In addition, the adiabatic MSW flavor transformation, which occurs in the C/O and He shells of the supernova, may affect the production of light nuclei such as 7L...

  15. Nucleosynthesis in Fast Expansions of High-Entropy, Proton Rich Matter

    E-Print Network [OSTI]

    G. C. Jordan IV; B. S. Meyer

    2004-06-29T23:59:59.000Z

    We demonstrate that nucleosynthesis in rapid, high-entropy expansions of proton-rich matter from high temperature and density can result in a wider variety of abundance patterns than heretofore appreciated. In particular, such expansions can produce iron-group nuclides, p-process nuclei, or even heavy, neutron-rich isotopes. Such diversity arises because the nucleosynthesis enters a little explored regime in which the free nucleons are not in equilibrium with the abundant alpha particles. This allows nuclei significantly heavier than iron to form in t he presence of abundant free nucleons early in the expansion. As the temperature drops, nucleons increasingly assemble into alpha particles and heavier nuclei. If the assembly is efficient, the resulting depletion of free neutrons allows disintegrat ion flows to drive nuclei back down to iron and nickel. If this assembly is inefficient, then the large abundance of free nucleons prevents the disintegration flows and leaves a distribution of heavy nuclei after reaction freezeout. For cases in between, an intermediate abundance distribution, enriched in p-process isotopes, is frozen out. These last expansions may contribute to the solar system's supply of the p-process nuclides if mildly proton-rich, high-entropy matter is ejected from proto-neutron stars winds or other astrophysical sites. Also sign ificant is the fact that, because the nucleosynthesis is primary, the signature of this nucleosyn thesis may be evident in metal poor stars.

  16. The Karlsruhe Astrophysical Database of Nucleosynthesis in Stars Project - Status and Prospects

    E-Print Network [OSTI]

    Iris Dillmann; Tamas Szücs; Zsolt Fülöp; Ralf Plag; Franz Käppeler; Thomas Rauscher

    2014-08-16T23:59:59.000Z

    The KADoNiS (Karlsruhe Astrophysical Database of Nucleosynthesis in Stars) project is an astrophysical online database for cross sections relevant for nucleosynthesis in the $s$ process and the $\\gamma$ process. The $s$-process database (www.kadonis.org) was started in 2005 and is presently facing its 4th update (KADoNiS v1.0). The $\\gamma$-process database (KADoNiS-p, www.kadonis.org/pprocess) was recently revised and re-launched in March 2013. Both databases are compilations for experimental cross sections with relevance to heavy ion nucleosynthesis. For the $s$ process recommended Maxwellian averaged cross sections for $kT$= 5-100~keV are given for more than 360 isotopes between $^{1}$H and $^{210}$Bi. For the $\\gamma$-process database all available experimental data from $(p,\\gamma), (p,n), (p,\\alpha), (\\alpha,\\gamma), (\\alpha,n)$, and $(\\alpha,p)$ reactions between $^{70}$Ge and $^{209}$Bi in or close to the respective Gamow window were collected and can be compared to theoretical predictions. The aim of both databases is a quick and user-friendly access to the available data in the astrophysically relevant energy regions.

  17. Attachment 2: Solicitation for Offers with New and Revised Green...

    Office of Environmental Management (EM)

    2: Solicitation for Offers with New and Revised Green Lease Text Attachment 2: Solicitation for Offers with New and Revised Green Lease Text Solicitation for Offers Paragraphs with...

  18. Appreciative Leadership Development Offered in Canada!

    E-Print Network [OSTI]

    Pulfrey, David L.

    Appreciative Leadership Development Offered in Canada! November 18, 19, 25, 26 Vancouver, British Columbia The Appreciative Leadership Development Program is an innovative strengths-based learning process during which you discover and build upon your Leadership Positive Core -- your unique strengths, skills

  19. OFFER TO LEASE SPACE IN RESPONSE TO

    E-Print Network [OSTI]

    . OTHER 1b. BUILDING ADDRESS sq. ft sq. ft sq. ft 1c. CITY 1d. STATE 4. LIVE FLOOR LOAD 5. MEASUREMENT _______________ - ____________ lbs./sq. ft SECTION II - SPACE OFFERED AND RATES INITIAL TERM RENEWAL OPTION TYPE OF SPACE FLOOR Full(F)/Partial

  20. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may;Note: This syllabus may represent a past offering of this course and future course offerings may differ

  1. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may, #12;Note: This syllabus may represent a past offering of this course and future course offerings may

  2. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may: This syllabus may represent a past offering of this course and future course offerings may differ. Course

  3. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may: This syllabus may represent a past offering of this course and future course offerings may differ. Course;Note: This syllabus may represent a past offering of this course and future course offerings may differ

  4. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may;Note: This syllabus may represent a past offering of this course and future course offerings may differHutchinson Style: #12;Note: This syllabus may represent a past offering of this course and future course offerings

  5. R-Process Nucleosynthesis in Dynamically Ejected Matter of Neutron Star Mergers

    E-Print Network [OSTI]

    Stephane Goriely; Andreas Bauswein; H. -Thomas Janka

    2011-08-09T23:59:59.000Z

    Although the rapid neutron-capture process, or r-process, is fundamentally important for explaining the origin of approximately half of the stable nuclei with A > 60, the astrophysical site of this process has not been identified yet. Here we study r-process nucleosynthesis in material that is dynamically ejected by tidal and pressure forces during the merging of binary neutron stars (NSs) and within milliseconds afterwards. For the first time we make use of relativistic hydrodynamical simulations of such events, defining consistently the conditions that determine the nucleosynthesis, i.e., neutron enrichment, entropy, early density evolution and thus expansion timescale, and ejecta mass. We find that 10^{-3}-10^{-2} solar masses are ejected, which is enough for mergers to be the main source of heavy (A > 140) galactic r-nuclei for merger rates of some 10^{-5} per year. While asymmetric mergers eject 2-3 times more mass than symmetric ones, the exact amount depends weakly on whether the NSs have radii of ~15 km for a "stiff" nuclear equation of state (EOS) or ~12 km for a "soft" EOS. R-process nucleosynthesis during the decompression becomes largely insensitive to the detailed conditions because of efficient fission recycling, producing a composition that closely follows the solar r-abundance distribution for nuclei with mass numbers A > 140. Estimating the light curve powered by the radioactive decay heating of r-process nuclei with an approximative model, we expect high emission in the B-V-R bands for 1-2 days with potentially observable longer duration in the case of asymmetric mergers because of the larger ejecta mass.

  6. Nucleosynthesis in the outflows associated with accretion disks of Type II collapsars

    E-Print Network [OSTI]

    Indrani Banerjee; Banibrata Mukhopadhyay

    2013-09-04T23:59:59.000Z

    We investigate nucleosynthesis inside the outflows from gamma-ray burst (GRB) accretion disks formed by the Type II collapsars. In these collapsars, massive stars undergo core collapse to form a proto-neutron star initially and a mild supernova explosion is driven. The supernova ejecta lack momentum and subsequently this newly formed neutron star gets transformed to a stellar mass black hole via massive fallback. The hydrodynamics and the nucleosynthesis in these accretion disks has been studied extensively in the past. Several heavy elements are synthesized in the disk and much of these heavy elements are ejected from the disk via winds and outflows. We study nucleosynthesis in the outflows launched from these disks by using an adiabatic, spherically expanding outflow model, to understand which of these elements thus synthesized in the disk survive in the outflow. While studying this we find that many new elements like isotopes of titanium, copper, zinc etc. are present in the outflows. 56Ni is abundantly synthesized in most of the cases in the outflow which implies that the outflows from these disks in a majority of cases will lead to an observable supernova explosion. It is mainly present when outflow is considered from the He-rich, 56Ni/54Fe rich zones of the disks. However, outflow from the Si-rich zone of the disk remains rich in silicon. Although, emission lines of many of these heavy elements have been observed in the X-ray afterglows of several GRBs by Chandra, BeppoSAX, XMM-Newton etc., Swift seems to have not detected these lines yet.

  7. NUCLEOSYNTHESIS IN THE OUTFLOWS ASSOCIATED WITH ACCRETION DISKS OF TYPE II COLLAPSARS

    SciTech Connect (OSTI)

    Banerjee, Indrani; Mukhopadhyay, Banibrata, E-mail: indrani@physics.iisc.ernet.in, E-mail: bm@physics.iisc.ernet.in [Department of Physics, Indian Institute of Science, Bangalore 560 012 (India)

    2013-11-20T23:59:59.000Z

    We investigate nucleosynthesis inside the outflows from gamma-ray burst (GRB) accretion disks formed by the Type II collapsars. In these collapsars, massive stars undergo core collapse to form a proto-neutron star initially, and a mild supernova (SN) explosion is driven. The SN ejecta lack momentum, and subsequently this newly formed neutron star gets transformed to a stellar mass black hole via massive fallback. The hydrodynamics and the nucleosynthesis in these accretion disks have been studied extensively in the past. Several heavy elements are synthesized in the disk, and much of these heavy elements are ejected from the disk via winds and outflows. We study nucleosynthesis in the outflows launched from these disks by using an adiabatic, spherically expanding outflow model, to understand which of these elements thus synthesized in the disk survive in the outflow. While studying this, we find that many new elements like isotopes of titanium, copper, zinc, etc., are present in the outflows. {sup 56}Ni is abundantly synthesized in most of the cases in the outflow, which implies that the outflows from these disks in a majority of cases will lead to an observable SN explosion. It is mainly present when outflow is considered from the He-rich, {sup 56}Ni/{sup 54}Fe-rich zones of the disks. However, outflow from the Si-rich zone of the disk remains rich in silicon. Although emission lines of many of these heavy elements have been observed in the X-ray afterglows of several GRBs by Chandra, BeppoSAX, XMM-Newton, etc., Swift seems to have not yet detected these lines.

  8. Low-mass helium star models for type Ib supernovae - Light curves, mixing, and nucleosynthesis

    SciTech Connect (OSTI)

    Shigeyama, Toshikazu; Nomoto, Kenichi; Tsujimoto, Takuji; Hashimoto, Masaki (Tokyo Univ. (Japan) Kyushu Univ., Fukuoka (Japan))

    1990-09-01T23:59:59.000Z

    The applicability of theoretical models of He-star explosions to type Ib SN explosions is explored. Particular attention is given to light curves and mixing, Rayleigh-Taylor instabilities and mixing, and nucleosynthesis and the mass of Ni-56. Typical numerical results are presented in graphs, and it is concluded that the explosions of SN 1983N and SN 1983I can be accurately represented in terms of explosions of He stars with M(alpha) of 3-4 solar mass. A strong M(alpha) dependence of light-curve shape, photospheric velocity, and Ni-56 mass is found. 44 refs.

  9. Astrophysical S-factor for destructive reactions of lithium-7 in big bang nucleosynthesis

    SciTech Connect (OSTI)

    Komatsubara, Tetsuro; Kwon, YoungKwan; Moon, JunYoung; Kim, Yong-Kyun [Rare Isotope Science Project, Institute for Basic Science, Daejeon (Korea, Republic of); Moon, Chang-Bum [Hoseo University, Asan, Chungnam (Korea, Republic of); Ozawa, Akira; Sasa, Kimikazu; Onishi, Takahiro; Yuasa, Toshiaki; Okada, Shunsuke; Saito, Yuta [Division of Physics, University of Tsukuba, Tsukuba, Ibaraki (Japan); Hayakawa, Takehito; Shizuma, Toshiyuki [Japan Atomic Energy Agency, Shirakata Shirane, Tokai, Ibaraki (Japan); Kubono, Shigeru [RIKEN, Hirosawa, Wako, Saitama (Japan); Kusakabe, Motohiko [School of Liberal Arts and Science, Korea Aerospace University (Korea, Republic of); Kajino, Toshitaka [National Astronomical Observatory, Osawa, Mitaka, Tokyo (Japan)

    2014-05-02T23:59:59.000Z

    One of the most prominent success with the Big Bang models is the precise reproduction of mass abundance ratio for {sup 4}He. In spite of the success, abundances of lithium isotopes are still inconsistent between observations and their calculated results, which is known as lithium abundance problem. Since the calculations were based on the experimental reaction data together with theoretical estimations, more precise experimental measurements may improve the knowledge of the Big Bang nucleosynthesis. As one of the destruction process of lithium-7, we have performed measurements for the reaction cross sections of the {sup 7}L({sup 3}He,p){sup 9}Be reaction.

  10. On the introduction of {sup 17}O+p reaction rates evaluated through the THM in AGB nucleosynthesis calculations

    SciTech Connect (OSTI)

    Palmerini, S.; Sergi, M. L.; La Cognata, M.; Pizzone, R. G. [I.N.F.N. Laboratori Nazionali del Sud, via Santa Sofia 62, Catania (Italy); Lamia, L.; Spitaleri, C. [Dipartimento di Fisica e Astronomia, Universitá degli Studi di Catania (Italy)

    2014-05-09T23:59:59.000Z

    The rates for the {sup 17}O(p,??{sup 14}N, {sup 17}O(p,?){sup 18}F and {sup 18}O(p,?){sup 15}N reactions deduced trough the Trojan Horse Method (THM) have been introduced into a state-of-the-art asymptotic giant branch (AGB) models for proton-capture nucleosynthesis and cool bottom process. The predicted abundances have been compared with isotopic compositions provided by geochemical analysis of presolar grains. As a result, an improved agreement is found between the models and the isotopic mix of oxide grains of AGB origins, whose composition is the signature of low-temperature proton-capture nucleosynthesis.

  11. Peptoid Nanosheets Offer a Diversity of Functionalities

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC)IntegratedSpeeding accessPeptoid Nanosheets Offer a Diversity of Functionalities

  12. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may: This syllabus may represent a past offering of this course and future course offerings may differ. Course to Seidman, pp.7­14, Weiss, Chap.1 -- #12;Note: This syllabus may represent a past offering of this course

  13. Statement of Work - Optional Service Offerings for Contractor...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Work - Optional Service Offerings for Contractor-Identified Project Statement of Work - Optional Service Offerings for Contractor-Identified Project Spreadsheet features optional...

  14. POLICY GUIDANCE MEMORANDUM #29 Employment Offers Letters Performance...

    Energy Savers [EERE]

    9 Employment Offers Letters Performance Management POLICY GUIDANCE MEMORANDUM 29 Employment Offers Letters Performance Management This memorandum is to ensure compliance with DOE...

  15. New rocket propellant and motor design offer high-performance...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    New rocket propellant and motor design offer high-performance and safety New rocket propellant and motor design offer high-performance and safety Scientists recently flight tested...

  16. UNICOR Renewable Energy Group Solar Program and Service Offerings...

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    UNICOR Renewable Energy Group Solar Program and Service Offerings UNICOR Renewable Energy Group Solar Program and Service Offerings Presentation-for the Federal Utility Partnership...

  17. Department of Energy Offers Vehicle Production Group Nearly ...

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    Department of Energy Offers Vehicle Production Group Nearly 50 Million Conditional Loan Commitment Department of Energy Offers Vehicle Production Group Nearly 50 Million...

  18. Promising Inspection Technique for Vehicle Welding Offers Efficient...

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    Promising Inspection Technique for Vehicle Welding Offers Efficient Alternative Promising Inspection Technique for Vehicle Welding Offers Efficient Alternative April 22, 2015 -...

  19. Energy Department Offers Conditional Commitment to Support Nevada...

    Energy Savers [EERE]

    Energy Department Offers Conditional Commitment to Support Nevada Geothermal Development with Recovery Act Funds Energy Department Offers Conditional Commitment to Support Nevada...

  20. Department of Energy Offers Conditional Commitment for a Loan...

    Office of Environmental Management (EM)

    Department of Energy Offers Conditional Commitment for a Loan Guarantee to Support World's Largest Wind Project Department of Energy Offers Conditional Commitment for a Loan...

  1. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may) with your progress report (PDF). (1-3 pages) #12;Note: This syllabus may represent a past offering

  2. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may-class participation (required) #12;Note: This syllabus may represent a past offering of this course and future course

  3. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may will design and build a #12;Note: This syllabus may represent a past offering of this course and future course

  4. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may discussions): 20% #12;Note: This syllabus may represent a past offering of this course and future course

  5. Non-Extensive Statistics, New Solution to the Cosmological Lithium Problem

    E-Print Network [OSTI]

    J. J. He; S. Q. Hou; A. Parikh; D. Kahl; C. A. Bertulani; other collaborators

    2014-12-22T23:59:59.000Z

    In the primordial Big Bang nucleosynthesis (BBN), only the lightest nuclides (D, $^3$He, $^4$He, and $^7$Li) were synthesized in appreciable quantities, and these relics provide us a unique window on the early universe. Currently, BBN simulations give acceptable agreement between theoretical and observed abundances of D and $^4$He, but it is still difficult to reconcile the predicted $^7$Li abundance with the observation for the Galactic halo stars. The BBN model overestimates the primordial $^7$Li abundance by about a factor of three, so called the cosmological lithium problem, a long-lasting pending issue in BBN. Great efforts have been paid in the past decades, however, the conventional nuclear physics seems unable to resolve such problem. It is well-known that the classical Maxwell-Boltzmann (MB) velocity distribution has been usually assumed for nuclei in the Big-Bang plasma. In this work, we have thoroughly investigated the impact of non-extensive Tsallis statistics (deviating from the MB) on thermonuclear reaction rates involved in standard models of BBN. It shows that the predicted primordial abundances of D, $^4$He, and $^7$Li agree very well with those observed ones by introducing a non-extensive parameter $q$. It is discovered that the velocities of nuclei in a hot Big-Bang plasma indeed violate the classical Maxwell-Boltzmann (MB) distribution in a very small deviation of about 6.3--8.2%. Thus, we have for the first time found a new solution to the cosmological lithium problem without introducing any mysterious theories. Furthermore, the implications of non-extensive statistics in other exotic high-temperature and density astrophysical environments should be explored, which might offer new insight into the nucleosynthesis of heavy elements.

  6. Aspherical nucleosynthesis in a core-collapse supernova with 25 M {sub ?} standard progenitor

    SciTech Connect (OSTI)

    Popov, M. V. [École Normale Supérieure de Lyon, CRAL (UMR CNRS 5574), Université de Lyon 1, 46 allée d'Italie, F-69007 Lyon (France); Filina, A. A.; Baranov, A. A.; Chardonnet, P. [LAPTh, Université de Savoie, 9, Chemin de Bellevue BP 110, F-74941 Annecy-le-Vieux Cedex (France); Chechetkin, V. M. [Keldysh Institute of Applied Mathematics RAS, Miusskaya sq. 4, 125047 Moscow (Russian Federation)

    2014-03-01T23:59:59.000Z

    The problem of nucleosynthesis was studied within an aspherical supernova model. The explosive burning was computed in a star of 25 M {sub ?} initial mass on its final stage of evolution. The chemical composition of a presupernova was taken from realistic evolutionary computations. A piecewise parabolic method on a local stencil was applied to simulate the hydrodynamics of the explosion. The gravity was recomputed by a Poisson solver on a fine grid as the explosion developed. A detailed yield of chemical elements was performed as a post-processing step using the tracer particles method. The produced nuclei formed a layer-like structure enclosing large fragments of nickel and iron-group isotopes that were pushed away from the central region by an explosion along the polar direction. The light nuclei were preferentially moving along the equatorial plane forming a torus-like structure.

  7. Beta-decay spectroscopy relevant to the r-process nucleosynthesis

    SciTech Connect (OSTI)

    Nishimura, Shunji [RIKEN Nishina Center, 2-1 Hirosawa, Wako, Saitama 351-0198 (Japan); Collaboration: RIBF Decay Collaboration

    2012-11-12T23:59:59.000Z

    A scientific program of beta-decay spectroscopy relevant to r-process nucleosynthesis has been started using high intensity U-beam at the RIBF. The first results of {beta}-decay half-lives of very neutron-rich Kr to Tc nuclides, all of which lie close to the r-process path, suggest a systematic enhancement of the the {beta}-decay rates of the Zr and Nb isotopes around A110 with respect to the predictions of the deformed quasiparticle-random-phase-approximation model (FRDM + QRPA). An impact of the results on the astrophysical r-process is discussed together with the future perspective of the {beta}-decay spectroscopy with the EURICA.

  8. The neutrino-induced neutron source in helium shell and r-process nucleosynthesis

    E-Print Network [OSTI]

    D. K. Nadyozhin; I. V. Panov; S. I. Blinnikov

    1998-07-06T23:59:59.000Z

    The huge neutrino pulse that occurs during the collapse of a massive stellar core, is expected to contribute to the origination of a number of isotopes both of light chemical elements and heavy ones. It is shown that, in general, the heating of stellar matter due to the neutrino scattering off electrons and the heat released from the neutrino-helium breakup followed by the thermonuclear reactions should be taken into account. On the base of kinetic network, using all the important reactions up to Z=8, the main features and the time-dependent character of the neutrino- driven neutron flux are investigated. The time-dependent densities of free neutrons produced in helium breakup, Y_n(t), were used to calculate the r-process nucleosynthesis with another full kinetic network for 3200 nuclides. It was found that in the case of metal-deficient stars, Z neutrons seems to be high enough to drive the r-process efficiently under favorable conditions. But it is impossible to obtain a sufficient amount of heavy nuclei in neutrino-induced r-process in a helium shell at radii R > R_cr \\approx 10^9 cm. We speculate that to make the neutrino-induced r-process work efficiently in the shell, one has to invoke nonstandard presupernova models in which helium hopefully is closer to the collapsed core owing, for instance, to a large scale mixing or/and rotation and magnetic fields. Apart from this exotic possibility, the neutrino-induced nucleosynthesis in the helium shell is certainly not strong enough to explain the observed solar r-process abundances.

  9. s-Process Nucleosynthesis in Advanced Burning Phases of Massive Stars

    E-Print Network [OSTI]

    Lih-Sin The; Mounib F. El Eid; Bradley S. Meyer

    2006-09-28T23:59:59.000Z

    We present a detailed study of s-process nucleosynthesis in massive stars of solar-like initial composition and masses 15, 20,25, and 30 Msun. We update our previous results of s-process nucleosynthesis during the core He-burning of these stars and then focus on an analysis of the s-process under the physical conditions encountered during the shell-carbon burning. We show that the recent compilation of the Ne22(alpha,n)Mg25 rate leads to a remarkable reduction of the efficiency of the s-process during core He-burning. In particular, this rate leads to the lowest overproduction factor of Kr80 found to date during core He-burning in massive stars. The s-process yields resulting from shell carbon burning turn out to be very sensitive to the structural evolution of the carbon shell. This structure is influenced by the mass fraction of C12 attained at the end of core helium burning, which in turn is mainly determined by the C12(alpha,gamma)O16 reaction. The still present uncertainty in the rate for this reaction implies that the s-process in massive stars is also subject to this uncertainty. We identify some isotopes like Zn70 and Rb87 as the signatures of the s-process during shell carbon burning in massive stars. In determining the relative contribution of our s-only stellar yields to the solar abundances, we find it is important to take into account the neutron exposure of shell carbon burning. When we analyze our yields with a Salpeter Initial Mass Function, we find that massive stars contribute at least 40% to s-only nuclei with mass A 90, massive stars contribute on average ~7%, except for Gd152, Os187, and Hg198 which are ~14%, \\~13%, and ~11%, respectively.

  10. THE IMPACT OF HELIUM-BURNING REACTION RATES ON MASSIVE STAR EVOLUTION AND NUCLEOSYNTHESIS

    SciTech Connect (OSTI)

    West, Christopher; Heger, Alexander [Minnesota Institute for Astrophysics, School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455 (United States); Austin, Sam M., E-mail: west0482@umn.edu, E-mail: alexander.heger@monash.edu, E-mail: austin@nscl.msu.edu [Joint Institute for Nuclear Astrophysics, Notre Dame, IN 46556 (United States)

    2013-05-20T23:59:59.000Z

    We study the sensitivity of presupernova evolution and supernova nucleosynthesis yields of massive stars to variations of the helium-burning reaction rates within the range of their uncertainties. The current solar abundances from Lodders are used for the initial stellar composition. We compute a grid of 12 initial stellar masses and 176 models per stellar mass to explore the effects of independently varying the {sup 12}C({alpha}, {gamma}){sup 16}O and 3{alpha} reaction rates, denoted R{sub {alpha},12} and R{sub 3{alpha}}, respectively. The production factors of both the intermediate-mass elements (A = 16-40) and the s-only isotopes along the weak s-process path ({sup 70}Ge, {sup 76}Se, {sup 80}Kr, {sup 82}Kr, {sup 86}Sr, and {sup 87}Sr) were found to be in reasonable agreement with predictions for variations of R{sub 3{alpha}} and R{sub {alpha},12} of {+-}25%; the s-only isotopes, however, tend to favor higher values of R{sub 3{alpha}} than the intermediate-mass isotopes. The experimental uncertainty (one standard deviation) in R{sub 3{alpha}}(R{sub {alpha},12}) is approximately {+-}10%({+-}25%). The results show that a more accurate measurement of one of these rates would decrease the uncertainty in the other as inferred from the present calculations. We also observe sharp changes in production factors and standard deviations for small changes in the reaction rates, due to differences in the convection structure of the star. The compactness parameter was used to assess which models would likely explode as successful supernovae, and hence contribute explosive nucleosynthesis yields. We also provide the approximate remnant masses for each model and the carbon mass fractions at the end of core-helium burning as a key parameter for later evolution stages.

  11. Primordial Helium And the Cosmic Background Radiation

    E-Print Network [OSTI]

    Gary Steigman

    2010-04-29T23:59:59.000Z

    The products of primordial nucleosynthesis and the cosmic microwave background (CMB) photons are relics from the early evolution of the Universe whose observations probe the standard model of cosmology and provide windows on new physics beyond the standard models of cosmology and of particle physics. In the standard, hot big bang cosmology, long before any stars have formed a significant fraction (~25%) of the baryonic mass in the Universe should be in the form of helium-4 nuclei. Since current 4He observations are restricted to low redshift regions where stellar nucleosynthesis has occurred, observations of high redshift, prestellar 4He would constitute a fundamental test of the hot, big bang cosmology. At recombination, long after big bang nucleosynthesis (BBN) has ended, the temperature anisotropy spectrum imprinted on the CMB depends on the 4He abundance through its connection to the electron density and the effect of the electron density on Silk damping. Since the relic abundance of 4He is relatively insensitive to the universal density of baryons, but is sensitive to a non-standard, early Universe expansion rate, the primordial mass fraction of 4He, Yp, offers a test of the consistency of the standard models of BBN and the CMB and, provides constraints on non-standard physics. Here, the WMAP seven year data (supplemented by other CMB experiments), which lead to an indirect determination of Yp at high redshift, are compared to the BBN predictions and to the independent, direct observations of 4He in low redshift, extragalactic HII regions. At present, given the very large uncertainties in the CMB-determined primordial 4He abundance (as well as for the helium abundances inferred from H II region observations), any differences between the BBN predictions and the CMB observations are small, at a level < 1.5 sigma.

  12. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may Tuesday Introduction to course Introduction to user assistance (UA) #12;Note: This syllabus may represent: This syllabus may represent a past offering of this course and future course offerings may differ. Thursday

  13. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may%) 15% #12;Note: This syllabus may represent a past offering of this course and future course offerings Introduction, Overview Syllabus review Introductions User-Centered Design Requirements 2 Ways of Thinking About

  14. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may Week 3 A A. Lecture: Constructive criticism & evaluation rubric #12;Note: This syllabus may represent sources #12;Note: This syllabus may represent a past offering of this course and future course offerings

  15. Impact of neutrino flavor oscillations on the neutrino-driven wind nucleosynthesis of an electron-capture supernova

    E-Print Network [OSTI]

    Pllumbi, Else; Wanajo, Shinya; Janka, H -Thomas; Huedepohl, Lorenz

    2014-01-01T23:59:59.000Z

    Neutrino oscillations, especially to light sterile states, can affect the nucleosynthesis yields because of their possible feedback effect on the electron fraction (Ye). For the first time, we perform nucleosynthesis calculations for neutrino-driven wind trajectories from the neutrino-cooling phase of an 8.8 Msun electron-capture supernova, whose hydrodynamic evolution was computed in spherical symmetry with sophisticated neutrino transport and whose Ye evolution was post-processed by including neutrino oscillations both between active and active-sterile flavors. We also take into account the alpha-effect as well as weak magnetism and recoil corrections in the neutrino absorption and emission processes. We observe effects on the Ye evolution which depend in a subtle way on the relative radial positions of the sterile MSW resonances, of collective flavor transformations, and on the formation of alpha-particles. For the adopted supernova progenitor, we find that neutrino oscillations, also to a sterile state wi...

  16. Lowest l=0 proton resonance in {sup 26}Si and implications for nucleosynthesis of {sup 26}Al

    SciTech Connect (OSTI)

    Peplowski, P. N.; Baby, L. T.; Wiedenhoever, I.; Diffenderfer, E.; Hoeflich, P.; Rojas, A.; Volya, A. [Physics Department, Florida State University, Tallahassee, Florida 32306 (United States); Dekat, S. E.; Gay, D. L. [Department of Chemistry and Physics, University of North Florida, Jacksonville, Florida 32224 (United States); Grubor-Urosevic, O. [Department of Chemistry and Physics, Purdue University Calumet, Hammond, Indiana 46323 (United States); Kaye, R. A. [Department of Chemistry and Physics, Purdue University Calumet, Hammond, Indiana 46323 (United States); Department of Physics and Astronomy, Ohio Wesleyan University, Delaware, Ohio 43015 (United States); Keeley, N. [Department of Nuclear Reactions, Andrezj Soltan Institute for Nuclear Studies, PL-00681 Warsaw (Poland)

    2009-03-15T23:59:59.000Z

    Using a beam of the radioactive isotope {sup 25}Al, produced with the new RESOLUT facility, we measured the direct (d,n) proton-transfer reaction leading to low-lying proton resonances in {sup 26}Si. We observed the lowest l=0 proton resonance, identified with the 3{sup +} state at 5.914-MeV excitation energy. This result eliminates the largest uncertainty in astrophysical reaction rates involved in the nucleosynthesis of {sup 26}Al.

  17. Indianapolis Offers a Lesson on Driving Demand | Department of...

    Energy Savers [EERE]

    Indianapolis Offers a Lesson on Driving Demand Indianapolis Offers a Lesson on Driving Demand The flier for EcoHouse, with the headline 'Save energy, save money, improve your home'...

  18. Geothermal Discovery Offers Hope for More Potential Across the...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Discovery Offers Hope for More Potential Across the Country Geothermal Discovery Offers Hope for More Potential Across the Country October 17, 2012 - 12:50pm Addthis The solution...

  19. Department of Energy Offers $102 Million Conditional Commitment...

    Office of Environmental Management (EM)

    Offers 102 Million Conditional Commitment for Loan Guarantee to U.S. Geothermal Inc. Department of Energy Offers 102 Million Conditional Commitment for Loan Guarantee to U.S....

  20. SunShot Incubator Awardee Helps Companies Offer Discount Solar...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    SunShot Incubator Awardee Helps Companies Offer Discount Solar as Employee Perk SunShot Incubator Awardee Helps Companies Offer Discount Solar as Employee Perk March 31, 2015 -...

  1. ESPC Standard Financing Offer Template (IDIQ Attachment J-12)

    Broader source: Energy.gov [DOE]

    Document features a template to help communicate a finance offer as part of an energy savings performance contract (ESPC).

  2. The Effects of Variations in Nuclear Interactions on Nucleosynthesis in Thermonuclear Supernovae

    E-Print Network [OSTI]

    Anuj Parikh; Jordi Jose; Ivo R. Seitenzahl; Friedrich K. Roepke

    2013-06-25T23:59:59.000Z

    The impact of nuclear physics uncertainties on nucleosynthesis in thermonuclear supernovae has not been fully explored using comprehensive and systematic studies with multiple models. To better constrain predictions of yields from these phenomena, we have performed a sensitivity study by post-processing thermodynamic histories from two different hydrodynamic, Chandrasekhar-mass explosion models. We have individually varied all input reaction and, for the first time, weak interaction rates by a factor of ten and compared the yields in each case to yields using standard rates. Of the 2305 nuclear reactions in our network, we find that the rates of only 53 reactions affect the yield of any species with an abundance of at least 10^-8 M_sun by at least a factor of two, in either model. The rates of the 12C(a,g), 12C+12C, 20Ne(a,p), 20Ne(a,g) and 30Si(p,g) reactions are among those that modify the most yields when varied by a factor of ten. From the individual variation of 658 weak interaction rates in our network by a factor of ten, only the stellar 28Si(b+)28Al, 32S(b+)32P and 36Ar(b+)36Cl rates significantly affect the yields of species in a model. Additional tests reveal that reaction rate changes over temperatures T > 1.5 GK have the greatest impact, and that ratios of radionuclides that may be used as explosion diagnostics change by a factor of less than two from the variation of individual rates by a factor of 10. Nucleosynthesis in the two adopted models is relatively robust to variations in individual nuclear reaction and weak interaction rates. Laboratory measurements of a limited number of reactions would help to further constrain predictions. As well, we confirm the need for a consistent treatment for relevant stellar weak interaction rates since simultaneous variation of these rates (as opposed to individual variation) has a significant effect on yields in our models.

  3. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may to its cultural relevance and effectiveness 50% Week 9 #12;Note: This syllabus may represent a past

  4. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may the original total point value. Work more than 5 days late will receive zero credit. #12;Note: This syllabus

  5. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may Participation 10% Major Figure 15% Group Web 25% Final Paper 40% #12;Note: This syllabus may represent a past

  6. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may is a part of your class grade and that it includes many components. #12;Note: This syllabus may represent

  7. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may and prototype files can be in the format most convenient for you. #12;Note: This syllabus may represent a past

  8. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may argumentation around the concept of crowdsourcing/crowd work. #12;Note: This syllabus may represent a past

  9. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may your professional identity using multiple avenues (i.e., #12;Note: This syllabus may represent a past

  10. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may management project OR 55% Due Week 8b #12;Note: This syllabus may represent a past offering of this course - Cultural adaptation WEEK 3A ­ JULY 5TH Localization Engineering and Tools #12;Note: This syllabus may

  11. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may Course Schedule: MW, 1:30-3:20pm; or TTh, 10:30am-12:20pm *DISCLAIMER: This syllabus represents computational thinking, including: #12;Note: This syllabus may represent a past offering of this course

  12. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may with empirical research. #12;Note: This syllabus may represent a past offering of this course and future course of this syllabus) and short "discussion idea" postings to the course blog in order to stimulate discussion about

  13. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may.9 ­ 1.1 D 0.7 ­ 0.8 D- 0.0 E #12;Note: This syllabus may represent a past offering of this course

  14. Explosive nucleosynthesis: nuclear physics impact using neutrino-driven wind simulations

    E-Print Network [OSTI]

    A. Arcones; G. Martinez-Pinedo

    2010-12-14T23:59:59.000Z

    We present nucleosynthesis studies based on hydrodynamical simulations of core-collapse supernovae and their subsequent neutrino-driven winds. Although the conditions found in these simulations are not suitable for the rapid neutron capture (r-process) to produce elements heavier than A$\\sim$130, this can be solved by artificially increasing the wind entropy. In this way one can mimic the general behavior of an ejecta where the r-process occurs. We study the impact of the long-time dynamical evolution and of the nuclear physics input on the final abundances and show that different nuclear mass models lead to significant variations in the abundances. These differences can be linked to the behavior of nuclear masses far from stability. In addition, we have analyzed in detail the effect of neutron capture and beta-delayed neutron emission when matter decays back to stability. In all our studied cases, freeze out effects are larger than previously estimated and produce substantial changes in the post freeze out abundances.

  15. A New Study of s-Process Nucleosynthesis in Massive Stars

    E-Print Network [OSTI]

    L. -S. The; M. F. El Eid; B. S. Meyer

    1998-12-11T23:59:59.000Z

    We present a comprehensive study of s-process nucleosynthesis in 15, 20, 25, and 30 $\\msun$ stellar models having solar-like initial composition. The stars are evolved up to ignition of central neon with a 659 species network coupled to the stellar models. In this way, the initial composition from one burning phase to another is consistently determined, especially with respect to neutron capture reactions. The aim of our calculations is to gain a full account of the s-process yield from massive stars. In the present work, we focus primarily on the s-process during central helium burning and illuminate some major uncertainties affecting the calculations. We briefly show how advanced burning can significantly affect the products of the core helium burning s-process and, in particular, can greatly deplete $^{80}$Kr that was strongly overproduced in the earlier core helium burning phase; however, we leave a complete analysis of the s-process during the advanced evolutionary phases (especially in shell carbon burning) to a subsequent paper. Our results can help to constrain the yield of the s-process material from massive stars during their pre-supernova evolution.

  16. Nucleosynthesis and mixing on the Asymptotic Giant Branch. III. Predicted and observed s-process abundances

    E-Print Network [OSTI]

    M. Busso; R. Gallino; D. L. Lambert; C. Travaglio; V. V. Smith

    2001-04-26T23:59:59.000Z

    We present the results of s-process nucleosynthesis calculations for AGB stars of different metallicities and initial masses. The computations were based on previously published stellar evolutionary models that account for the III dredge up phenomenon occurring late on the AGB. Neutron production is driven by the 13C(alpha,n)16O reaction during the interpulse periods in a tiny layer in radiative equilibrium at the top of the He- and C-rich shell. The s-enriched material is subsequently mixed with the envelope by the III dredge up, and the envelope composition is computed after each thermal pulse. We follow the changes in the photospheric abundance of the Ba-peak elements (heavy s, or `hs') and that of the Zr-peak ones (light s, or `ls'), whose logarithmic ratio [hs/ls] has often been adopted as an indicator of the s-process efficiency. The theoretical predictions are compared with published abundances of s elements for Galactic AGB giants of classes MS, S, SC, post-AGB supergiants, and for various classes of binary stars. The observations in general confirm the complex dependence of n captures on metallicity. They suggest that a moderate spread exists in the abundance of 13C that is burnt in different stars. Although additional observations are needed, a good understanding has been achieved of s-process operation in AGB. The detailed abundance distribution including the light elements (CNO) of a few s-enriched stars at different metallicity are examined.

  17. Lithium in Very Metal-poor Dwarf Stars - Problems for Standard Big Bang Nucleosynthesis?

    E-Print Network [OSTI]

    David L. Lambert

    2004-10-18T23:59:59.000Z

    The standard model of primordial nucleosynthesis by the Big Bang as selected by the WMAP-based estimate of the baryon density ($\\Omega_bh^2$) predicts an abundance of $^7$Li that is a factor of three greater than the generally reported abundance for stars on the Spite plateau, and an abundance of $^6$Li that is about a thousand times less than is found for some stars on the plateau. This review discusses and examines these two discrepancies. They can likely be resolved without major surgery on the standard model of the Big Bang. In particular, stars on the Spite plateau may have depleted their surface lithium abundance over their long lifetime from the WMAP-based predicted abundances down to presently observed abundances, and synthesis of $^6$Li (and $^7$Li) via $\\alpha + \\alpha$ fusion reactions may have occurred in the early Galaxy. Yet, there remain fascinating ways in which to remove the two discrepancies involving aspects of a new cosmology, particularly through the introduction of exotic particles.

  18. Business Energy Efficiency Rebate (Offered by 11 Utilities)

    Broader source: Energy.gov [DOE]

    Rebates are offered for a variety of efficient technologies and measures including: compressed air system efficiency, HVAC, lighting, VFDs, cooking equipment, and custom projects.  Rebates vary f...

  19. assistance program offers: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    majoring in programs offered by the College Chemistry Websites Summary: College of Engineering and Computer Science These scholarships have been established to assist...

  20. Partnering With Utilities to Offer Energy Efficiency Programs Webinar Transcript

    Broader source: Energy.gov [DOE]

    Partnering With Utilities to Offer Energy Efficiency Programs Webinar Transcript, from the U.S. Department of Energy Technical Assistance Program (TAP).

  1. CenterPoint Energy- Commercial and Industrial Standard Offer Program

    Broader source: Energy.gov [DOE]

    CenterPoint Energy's Commercial and Industrial Standard Offer Program pays incentives to service providers who install energy efficiency measures in commercial or industrial facilities that are...

  2. Department of Energy Offers $2.1 Billion Conditional Commitment...

    Office of Environmental Management (EM)

    .1 Billion Conditional Commitment Loan Guarantee to Support California Solar Thermal Power Plant Department of Energy Offers 2.1 Billion Conditional Commitment Loan Guarantee to...

  3. Energy Department Offers Conditional Commitment to Cape Wind...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Cape Wind Offshore Wind Generation Project Energy Department Offers Conditional Commitment to Cape Wind Offshore Wind Generation Project July 1, 2014 - 9:23am Addthis News Media...

  4. DOE Offers Loan Guarantees to Geothermal Projects in Nevada and...

    Broader source: Energy.gov (indexed) [DOE]

    a geothermal power plant. DOE recently offered loan guarantees for geothermal power projects located in northwestern Nevada and southeastern Oregon, drawing on funds from the...

  5. DOE Offers $15 Million Geothermal Heat Recovery Opportunity ...

    Office of Environmental Management (EM)

    15 Million Geothermal Heat Recovery Opportunity DOE Offers 15 Million Geothermal Heat Recovery Opportunity August 25, 2010 - 11:11am Addthis Photo of geothermal power plant....

  6. Improved understanding of protein complex offers insight into...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Improved understanding of protein complex offers insight into DNA replication initiation mechanism basics By Angela Hardin * March 18, 2015 Tweet EmailPrint Argonne, Ill. - A...

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    Broader source: Energy.gov [DOE]

    Bright Energy Solutions offers energy efficiency cash incentive programs to residential and business customers of municipal utilities that are members of Missouri River Energy Services. In Iowa,...

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    Broader source: Energy.gov [DOE]

    Video explains how the Federal Energy Management Program offers International Association for Continuing Education and Training (IACET) continuing education units for eTraining core courses.

  9. BEST OFFER EVER ACCELERATED TEXAS UPGRADES | Department of Energy

    Energy Savers [EERE]

    combination of radio, newspaper, and online advertisements; mass mailings; testimonial videos; features on its website; and outreach at local events to publicize the Best Offer...

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    Broader source: Energy.gov [DOE]

    Associated Electric Cooperative and many of its member cooperatives offer rebates to residential customers who purchase and install energy efficient equipment for the home. Eligible equipment...

  11. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future is a virtue ­ your insight, clarity of thought, #12;Note: This syllabus may represent

  12. Wind energy offers considerable promise; the wind itself is free,

    E-Print Network [OSTI]

    Langendoen, Koen

    Wind energy offers considerable promise; the wind itself is free, wind power is clean. One of these sources, wind energy, offers considerable promise; the wind itself is free, wind power is clean, and it is virtually inexhaustible. In recent years, research on wind energy has accelerated

  13. Optimal Power Flow Based Demand Response Offer Price Optimization

    E-Print Network [OSTI]

    Lavaei, Javad

    Optimal Power Flow Based Demand Response Offer Price Optimization Zhen Qiu 1 Introduction-time energy balance. Demand response programs are offered by the utility companies to reduce the load response cost in exchange for load reduction. A considerable amount of papers have discussed the demand

  14. ENGINEERING PHYSICS An Interdisciplinary Program Jointly Offered by the

    E-Print Network [OSTI]

    Lozano-Robledo, Alvaro

    ENGINEERING PHYSICS An Interdisciplinary Program Jointly Offered by the School of Engineering in engineering fundamentals, but also an understanding of the physical principles of the underlying mechanisms is required. The goal of the Engineering Physics Program is to offer students a solid background

  15. Letter-of-Offer Attachment Work Authorization Documentation --I-9

    E-Print Network [OSTI]

    Sheridan, Jennifer

    Letter-of-Offer Attachment Work Authorization Documentation -- I-9 This offer of employment is contingent upon verification of the appropriate identity and employment eligibility documentation on the Form and the list of acceptable documents, please see the Forms section of the U.S. Citizenship and Immigration

  16. Nonperturbative dynamics of reheating after inflation: A review

    E-Print Network [OSTI]

    Amin, Mustafa A.

    Our understanding of the state of the universe between the end of inflation and big bang nucleosynthesis (BBN) is incomplete. The dynamics at the end of inflation are rich and a potential source of observational signatures. ...

  17. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may of the environmental, economic, and social impact of engineering work. #12;Note: This syllabus may represent a past and project overview Syllabus introduction Introductions Assignment introductions: · Sustainability project

  18. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may Role plays and simulations Short speeches and presentations #12;Note: This syllabus may represent Introduction to HCDE 461: syllabus, goals, rules, and tips to success Warm-up activities: Self

  19. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may for a small system and plan and perform a usability evaluation #12;Note: This syllabus may represent a past in UCD Week 11 Project Presentations L11: Course Wrap-Up Finals Online Final Exam #12;Note: This syllabus

  20. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may reading 5% Participation in discussion 10% ____________ 100% #12;Note: This syllabus may represent a past (2) --- HW: Summary (2) due Mon. 9:00 a.m.; Prep. for mini-presentation (2) #12;Note: This syllabus

  1. Note: This syllabus may represent a past offering of this course and future course offerings may differ.

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future/Wednesdays Course URL: http://faculty.washington.edu/farkas/TC407/syllabus.html Course Description will be deducted for not posting. #12;Note: This syllabus may represent a past offering

  2. UConn Extension offers Bedding Plant Program for Greenhouse The University of Connecticut Cooperative Extension is offering Bedding Plants

    E-Print Network [OSTI]

    Alpay, S. Pamir

    UConn Extension offers Bedding Plant Program for Greenhouse Growers The University of Connecticut Cooperative Extension is offering Bedding Plants - Spring 2015! This educational program will feature, University of Connecticut, Storrs, CT · Diseases of Spring Crops and Their Management, Yonghao Li, Plant

  3. New Nuclear Reaction Flow during r-Process Nucleosynthesis in Supernovae: Critical Role of Light Neutron-Rich Nuclei

    E-Print Network [OSTI]

    M. Terasawa; K. Sumiyoshi; T. Kajino; G. J. Mathews; I. Tanihata

    2001-07-19T23:59:59.000Z

    We study the role of light neutron-rich nuclei during r-process nucleosynthesis in supernovae. Most previous studies of the r-process have concentrated on the reaction flow of heavy unstable nuclei. Although the nuclear reaction network includes a few thousand heavy nuclei, only limited reaction flow through light-mass nuclei near the stability line has been used in those studies. However, in a viable scenario of the r-process in neutrino-driven winds, the initial condition is a high-entropy hot plasma consisting of neutrons, protons, and electron-positron pairs experiencing an intense flux of neutrinos. In such environments light-mass nuclei as well as heavy nuclei are expected to play important roles in the production of seed nuclei and r-process elements. Thus, we have extended our fully implicit nuclear reaction network so that it includes all nuclei up to the neutron drip line for Z $ \\leq 10$, in addition to a larger network for Z $ \\geq 10$. In the present nucleosynthesis study, we utilize a wind model of massive SNeII explosions to study the effects of this extended network. We find that a new nuclear-reaction flow path opens in the very light neutron-rich region. This new nuclear reaction flow can change the final heavy-element abundances by as much as an order of magnitude.

  4. DNR offers 284 tracts in lease Sale 40

    SciTech Connect (OSTI)

    Not Available

    1983-11-01T23:59:59.000Z

    The State of Alaska's Department of Natural Resources, Division of Minerals and Energy Management, offered 284 tracts of submerged lands in Cook Inlet and uplands on Kalgin Island, the Kenai Peninsula, the west side of Cook Inlet and in the lower Susitna Valley. State geologists classify the area as low in its potential for commercial discoveries of oil, but many companies feel that Cook Inlet has some promise. Major oil companies offered the highest cash bonus bids, but independents and speculators managed to pick up the bulk of the 284 tracts offered.

  5. DOE Offers $150 Million Conditional Commitment for a Loan Guarantee...

    Office of Environmental Management (EM)

    Solar Manufacturing Process June 17, 2011 - 12:00am Addthis Washington D.C. - U.S. Energy Secretary Steven Chu today announced the offer of a conditional commitment for a 150...

  6. Oncor Electric Delivery- Solar Photovoltaic Standard Offer Program

    Broader source: Energy.gov [DOE]

    The 2013 Oncor Solar Photovoltaic Standard Offer Program Guidelines are now [https://www.oncoreepm.com/SolarPV.aspx available]. The application period for both the residential and non-residential...

  7. Department of Energy Offers $102 Million Conditional Commitment...

    Office of Environmental Management (EM)

    02 Million Conditional Commitment for Loan Guarantee to U.S. Geothermal, Inc. Department of Energy Offers 102 Million Conditional Commitment for Loan Guarantee to U.S. Geothermal,...

  8. Department of Energy Offers Conditional Loan Guarantee Commitment...

    Broader source: Energy.gov (indexed) [DOE]

    -- U.S. Energy Secretary Steven Chu today announced the offer of a conditional commitment for a 359.1 million loan guarantee to Mesquite Solar 1, LLC to support the development of...

  9. Entergy Texas- Residential and Small Commercial Standard Offer Program

    Broader source: Energy.gov [DOE]

    The Hard to Reach and Residential Standard Offer Programs provides incentives for the retrofit or new construction installation of a wide range of energy efficiency measures. The program does not...

  10. Obama Administration Offers $59 Million in Conditional Loan Guarantees...

    Energy Savers [EERE]

    expansion of its assembly plant in Pocatello, Idaho, to produce its one megawatt wind turbine. Beacon Power, an energy storage company, has been offered 43 million to support the...

  11. Residential Energy Efficiency Rebates (Offered by 11 Utilities)

    Broader source: Energy.gov [DOE]

    Bright Energy Solutions offers energy efficiency cash incentive programs to residential and [http://www.dsireusa.org/incentives/incentive.cfm?Incentive_Code=SD60F&re... business customers] of...

  12. Residential Energy Efficiency Rebates (Offered by 11 Utilities)

    Broader source: Energy.gov [DOE]

    Bright Energy Solutions offers energy efficiency cash incentive programs to [http://www.dsireusa.org/incentives/incentive.cfm?Incentive_Code=SD60F&re... residential] and business customers of...

  13. technology offer Non-Intrusive Remote Oscillator Measurement for

    E-Print Network [OSTI]

    Szmolyan, Peter

    technology offer Non-Intrusive Remote Oscillator Measurement for Distributed Systems based on Flex are quite intrusive: they require physical access to each single node and might interrupt system operation

  14. Note: This syllabus may represent a past offering of this course and future course offerings may differ. HCDE 418: User Experience Design

    E-Print Network [OSTI]

    Note: This syllabus may represent a past offering of this course and future course offerings may the trade-offs #12;Note: This syllabus may represent a past offering of this course and future course

  15. New neutron capture and total cross section measurements on {sup 88}Sr and their impact on s-process nucleosynthesis

    SciTech Connect (OSTI)

    Koehler, P.E.; Spencer, R.R.; Guber, K.H. [and others

    1998-11-01T23:59:59.000Z

    The authors have made new and improved measurements of the neutron capture and total cross sections of {sup 88}Sr at the Oak Ridge Electron Linear Accelerator (ORELA). Improvements over previous measurements include a wider incident neutron energy range, the use of metallic rather than carbonate samples, better background subtraction, reduced sensitivity to sample-dependent backgrounds, and better pulse-height weighting functions. Because of its small cross section, the {sup 88}Sr(n,{gamma}) reaction is an important bottleneck during the s-process nucleosynthesis. Hence, an accurate determination of this rate is needed to better constrain the neutron exposure in s-process models and to more fully exploit the recently discovered isotopic anomalies in certain meteorites. They describe the experimental procedures, compare the results to previous data, and discuss their astrophysical impact.

  16. The Sensitivity of Nucleosynthesis in Type I X-ray Bursts to Thermonuclear Reaction-Rate Variations

    E-Print Network [OSTI]

    Anuj Parikh; Jordi Jose; Fermin Moreno; Christian Iliadis

    2008-06-18T23:59:59.000Z

    We examine the sensitivity of nucleosynthesis in Type I X-ray bursts to variations in nuclear rates. As a large number of nuclear processes are involved in these phenomena -with the vast majority of reaction rates only determined theoretically due to the lack of any experimental information- our results can provide a means for determining which rates play significant roles in the thermonuclear runaway. These results may then motivate new experiments. For our studies, we have performed a comprehensive series of one-zone post-processing calculations in conjunction with various representative X-ray burst thermodynamic histories. We present those reactions whose rate variations have the largest effects on yields in our studies.

  17. New Constraints on Radiative Decay of Long-Lived Particles in Big Bang Nucleosynthesis with New $^4$He Photodisintegration Data

    E-Print Network [OSTI]

    Motohiko Kusakabe; Toshitaka Kajino; Takashi Yoshida; Tatsushi Shima; Yasuki Nagai; Toshiteru Kii

    2009-06-11T23:59:59.000Z

    A recent measurement of $^4$He photodisintegration reactions, $^4$He($\\gamma$,$p$)$^3$H and $^4$He($\\gamma$,$n$)$^3$He with laser-Compton photons shows smaller cross sections than those estimated by other previous experiments at $E_\\gamma \\lesssim 30$ MeV. We study big-bang nucleosynthesis with the radiative particle decay using the new photodisintegration cross sections of $^4$He as well as previous data. The sensitivity of the yields of all light elements D, T, $^3$He, $^4$He, $^6$Li, $^7$Li and $^7$Be to the cross sections is investigated. The change of the cross sections has an influence on the non-thermal yields of D, $^3$He and $^4$He. On the other hand, the non-thermal $^6$Li production is not sensitive to the change of the cross sections at this low energy, since the non-thermal secondary synthesis of $^6$Li needs energetic photons of $E_\\gamma \\gtrsim 50$ MeV. The non-thermal nucleosynthesis triggered by the radiative particle decay is one of candidates of the production mechanism of $^6$Li observed in metal-poor halo stars (MPHSs). In the parameter region of the radiative particle lifetime and the emitted photon energy which satisfies the $^6$Li production above the abundance level observed in MPHSs, the change of the photodisintegration cross sections at $E_\\gamma \\lesssim 30$ MeV as measured in the recent experiment leads to $\\sim 10$% reduction of resulting $^3$He abundance, whereas the $^6$Li abundance does not change for this change of the cross sections of $^4$He($\\gamma$,$p$)$^3$H and $^4$He($\\gamma$,$n$)$^3$He. The $^6$Li abundance, however, could show a sizable change and therefore the future precise measurement of the cross sections at high energy $E_\\gamma \\gtrsim$ 50 MeV is highly required.

  18. Impact of neutrino flavor oscillations on the neutrino-driven wind nucleosynthesis of an electron-capture supernova

    E-Print Network [OSTI]

    Else Pllumbi; Irene Tamborra; Shinya Wanajo; H. -Thomas Janka; Lorenz Huedepohl

    2014-06-11T23:59:59.000Z

    Neutrino oscillations, especially to light sterile states, can affect the nucleosynthesis yields because of their possible feedback effect on the electron fraction (Ye). For the first time, we perform nucleosynthesis calculations for neutrino-driven wind trajectories from the neutrino-cooling phase of an 8.8 Msun electron-capture supernova, whose hydrodynamic evolution was computed in spherical symmetry with sophisticated neutrino transport and whose Ye evolution was post-processed by including neutrino oscillations both between active and active-sterile flavors. We also take into account the alpha-effect as well as weak magnetism and recoil corrections in the neutrino absorption and emission processes. We observe effects on the Ye evolution which depend in a subtle way on the relative radial positions of the sterile MSW resonances, of collective flavor transformations, and on the formation of alpha-particles. For the adopted supernova progenitor, we find that neutrino oscillations, also to a sterile state with eV-mass, do not significantly affect the element formation and in particular cannot make the post-explosion wind outflow neutron rich enough to activate a strong r-process. Our conclusions become even more robust when, in order to mimic equation-of-state dependent corrections due to nucleon potential effects in the dense-medium neutrino opacities, four cases with reduced Ye in the wind are considered. In these cases, despite the conversion of neutrinos to sterile neutrinos, Ye increases compared to the values obtained without oscillations and active flavor transformations. This is a consequence of a complicated interplay between sterile-neutrino production, neutrino-neutrino interactions, alpha-effect.

  19. Offering Web-of-Things Connectivity to Building Networks

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    for restricting access. This constellation of devices has led buildings to become "smart" and are now relyingOffering Web-of-Things Connectivity to Building Networks G´er^ome Bovet Telecom ParisTech 46 Avenue Building management systems (BMS) are nowadays present in new and renovated buildings, relying on dedicated

  20. HOUSING: Senior year offers the broadest range of housing options.

    E-Print Network [OSTI]

    Royer, Dana

    SENIOR HOUSING: Senior year offers the broadest range of housing options. Most seniors live in an apartment or wood frame house with a group of friends, although some choose to live in a residence hall or program house. STUDENT STAFF: Senior areas are staffed by Community Advisors. See previous box

  1. Social media offers many ways to grow business

    SciTech Connect (OSTI)

    Madison, Alison L.

    2011-03-13T23:59:59.000Z

    Facebook and Twitter and YouTube, oh my! For some of us the added communications channels offered by social media can feel overwhelming in a hurry. But whether we like it or not, they’re proving to be valuable marketing tools that small and large companies alike are jumping on board to explore.

  2. Nuclear magnetic resonance offers new insights into Pu 239

    E-Print Network [OSTI]

    - 1 - Nuclear magnetic resonance offers new insights into Pu 239 May 29, 2012 Nuclear magnetic signal of plutonium 239's unique nuclear magnetic resonance signature has been detected by scientists on the subject, "Observation of 239 Pu Nuclear Magnetic Resonance," was published in the May 18 issue of Science

  3. Combining daylighting, personal controls, and load shedding offers

    E-Print Network [OSTI]

    Combining daylighting, personal controls, and load shedding offers enormous potential for reducing lighting system to respond to available daylight and demand response control · Allows building occupants--Consider the improved cost-effectiveness of wireless dimming to promote daylighting controls and load- shedding

  4. TRI-MENTORING OFFERS AN EDUCATION BEYOND TRADITIONAL UNIVERSITY

    E-Print Network [OSTI]

    TRI-MENTORING OFFERS AN EDUCATION BEYOND TRADITIONAL UNIVERSITY ENGINEERING CURRICULUM Donna L an education in topics such as these through the recently established Tri-Mentoring Program. The Tri-Mentoring and initial outcomes specifically for the UBC Engineering Tri-Mentoring Program, one of eight tri-mentoring

  5. AMST courses offered Spring 2014 Tulsa Based Classes

    E-Print Network [OSTI]

    Veiga, Pedro Manuel Barbosa

    AMST courses offered Spring 2014 Tulsa Based Classes: Crime, Law & Am Culture (S) AMST 3333 Liang to crime and the law. Arts and American Society: Tulsa's Public Cultures AMST 3550 Gray T 4:30-7:10p T-NCB 104 Topics vary by semester. This course will focus on Tulsa art, architecture and literature

  6. www.chem.pdx.edu Undergraduate Degrees Offered

    E-Print Network [OSTI]

    instrumentation, such as mass spectrometers, is available for chemical research. is includes a new high- resolution time-of-flight mass spectrometer as well as low- and high-field NMR spectrometers (400 & new 600CHEMISTRY www.chem.pdx.edu Undergraduate Degrees Offered: Bachelor of Arts in Chemistry

  7. Unique Energy Management Training Offers Certification and Energy Savings

    E-Print Network [OSTI]

    Ebbage, R.

    2004-01-01T23:59:59.000Z

    is rapidly becoming a mandatory practice in the maintance departments of commercial buildings around the world. Driven by increasing utility rates and shrinking budgets, energy-cost savings are often a requirement rather that just a good idea. Managers... the key to selecting the right project, stretching maintenance dollars and maximizing return on investment. These strict conditions have led commercial building managers and administrators to look for energy training programs that offer personnel...

  8. A Reply to "Comment on 'Big Bang Nucleosynthesis and Active-Sterile Neutrino Mixing: Evidence for Maximal $?_?\\leftrightarrow?_?$ Mixing in Super Kamiokande?'"

    E-Print Network [OSTI]

    Xiangdong Shi; George M. Fuller

    1998-12-17T23:59:59.000Z

    In the paper "Big Bang Nucleosynthesis and Active-Sterile Neutrino Mixing: Evidence for Maximal Muon-Neutrino/Sterile-Neutrino Mixing in Super Kamiokande" (astro-ph/9810075), we suggested that to evade the Big Bang Nucleosynthesis exclusion of the muon neutrino to sterile neutrino oscillation explanation of the Super Kamiokande data, the tau neutrino must have a mass over about 15 eV and it must mix with a lighter sterile neutrino. A stable tau neutrino with this mass is inconsistent with cosmological structure formation. In a comment on our paper (astro-ph/9811067), Foot and Volkas argued that our result is incorrect and that the required tau neutrino mass should be much lower. Here we back up our original result with a more detailed calculation. We show that the argument of Foot and Volkas is invalid, most likely due to an insufficient energy resolution in the low energy part of the neutrino spectrum.

  9. Falk Herwig: Mixing and Nucleosynthesis in IMS 16 Sep 2004 Cat'sEyeNebula,APOD4Sep02,Corradi&Goncalves

    E-Print Network [OSTI]

    Herwig, Falk

    & Lattanzio(partly published, 2003, PASA) Ventura etal (2002) A&A, 393 Herwig (2004), ApJS,155, #12;Falk: Ventura etal 2002 H04: Herwig 2004 average X in ejecta Ventura etal 2002 vs Herwig 2004 #12;Falk Herwig: »Mixing and Nucleosynthesis in IMS« 16 Sep 2004 Ventura etal 2002 vs Herwig 2004 4 He 12 C H04 H04 V02 V02

  10. CMI Offers Webinars on Critical Materials and Rare Earths | Critical

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOnItem NotEnergy,ARMForms About Batteries BatteriesCAES HomeMaterials Institute Offers

  11. NITROGEN ISOTOPES IN ASYMPTOTIC GIANT BRANCH CARBON STARS AND PRESOLAR SiC GRAINS: A CHALLENGE FOR STELLAR NUCLEOSYNTHESIS

    SciTech Connect (OSTI)

    Hedrosa, R. P.; Abia, C.; Dominguez, I.; Palmerini, S. [Departamento de Fisica Teorica y del Cosmos, Universidad de Granada, E-18071 Granada (Spain); Busso, M. [Dipartimento di Fisica, Universita di Perugia, I-06123 Perugia (Italy); Cristallo, S.; Straniero, O. [INAF, Osservatorio di Collurania, I-64100 Teramo (Italy); Plez, B. [Laboratoire Univers et Particules de Montpellier, Universite Montpellier II, CNRS, F-34095 Montpellier (France)

    2013-05-01T23:59:59.000Z

    Isotopic ratios of C, N, Si, and trace heavy elements in presolar SiC grains from meteorites provide crucial constraints to nucleosynthesis. A long-debated issue is the origin of the so-called A+B grains, as of yet no stellar progenitor thus far has been clearly identified on observational grounds. We report the first spectroscopic measurements of {sup 14}N/{sup 15}N ratios in Galactic carbon stars of different spectral types and show that J- and some SC-type stars might produce A+B grains, even for {sup 15}N enrichments previously attributed to novae. We also show that most mainstream grains are compatible with the composition of N-type stars, but in some cases might also descend from SC stars. From a theoretical point of view, no astrophysical scenario can explain the C and N isotopic ratios of SC-, J-, and N-type carbon stars together, as well as those of many grains produced by them. This poses urgent questions to stellar physics.

  12. Binghamton University offers this worksheet to help you compare costs and financial aid offers and calculate the bottom line. Since financial aid offers can vary greatly from school to school, it is recommended that you review them carefully, ask

    E-Print Network [OSTI]

    Suzuki, Masatsugu

    Must be repaid Binghamton University offers this worksheet to help you compare costs and financial is for 1, 2, 3 or 4 years. + + + Fees + + + Room & Board (Housing & Meals) + + + A. ESTIMATED COST (as.TOTALSTUDENTLOANS = = = A. TOTAL COST OF ATTENDANCE = TOTAL OUT-OF-POCKET COSTS = $ $ $ D. TOTAL FINANCIAL AID OFFER

  13. Berkeley Program Offers New Option for Financing Residential PV Systems

    SciTech Connect (OSTI)

    Bolinger, Mark A

    2008-07-06T23:59:59.000Z

    Readily accessible credit has often been cited as a necessary ingredient to open up the market for residential photovoltaic (PV) systems. Though financing does not reduce the high up-front cost of PV, by spreading that cost over some portion of the system's life, financing can certainly make PV systems more affordable. As a result, a number of states have, in the past, set up special residential loan programs targeting the installation of renewable energy systems and/or energy-efficiency improvements and often featuring low interest rates, longer terms and no-hassle application requirements. Historically, these loan programs have had mixed success (particularly for PV), for a variety of reasons, including a historical lack of homeowner interest in PV, a lack of program awareness, a reduced appeal in a low-interest-rate environment, and a tendency for early PV adopters to be wealthy and not in need of financing. Some of these barriers have begun to fade. Most notably, homeowner interest in PV has grown in some states, particularly those that offer solar rebates. The passage of the Energy Policy Act of 2005 (EPAct 2005), however, introduced one additional roadblock to the success of low-interest PV loan programs: a residential solar investment tax credit (ITC), subject to the Federal government's 'anti-double-dipping' rules. Specifically, the residential solar ITC--equal to 30% of the system's tax basis, capped at $2000--will be reduced or offset if the system also benefits from what is known as 'subsidized energy financing', which is likely to include most government-sponsored low-interest loan programs. Within this context, it has been interesting to note the recent flurry of announcements from a number of U.S cities concerning a new type of PV financing program. Led by the city of Berkeley, Calif., these cities propose to offer their residents the ability to finance the installation of a PV system using increased property tax assessments, rather than a more-traditional credit vehicle, to recover both system and administrative costs. This approach has a number of features that should appeal to PV owners, including long-term, fixed-cost, attractive financing; loans that are tied to the tax capacity of the property rather than to the owner's credit standing; a repayment obligation that transfers along with the sale of the property; and a potential ability to deduct the repayment obligation from federal taxable income as part of the local property tax deduction. For these reasons, Berkeley's program, which was first announced on October 23, 2007, has received considerable nationwide attention in both the trade and general press. Since the announcement, cities from throughout California and the broader U.S. have expressed keen interest in the possibility of replicating this type of program. In California alone, the cities of Santa Cruz, Santa Monica and Palm Desert are all reportedly considering similar programs, while the city of San Francisco has recently announced its own program, portions of which closely parallel Berkeley's approach. In addition, a bill (AB 811) that would authorize all cities in California, not just charter cities like Berkeley, to create this type of program was approved by the California General Assembly on January 29 and is currently under consideration in the State Senate. A similar bill in Colorado (HB 1350) was signed into law on May 28. Elsewhere, the city of Tucson, Arizona has also considered this financing approach.

  14. Cosmological solutions to the Lithium problem: Big-bang nucleosynthesis with photon cooling, $X$-particle decay and a primordial magnetic field

    E-Print Network [OSTI]

    Dai G. Yamazaki; Motohiko Kusakabe; Toshitaka Kajino; Grant. J. Mathews; Myung-Ki Cheoun

    2014-06-30T23:59:59.000Z

    The $^7$Li abundance calculated in BBN with the baryon-to-photon ratio fixed from fits to the CMB power spectrum is inconsistent with the observed lithium abundances on the surface of metal-poor halo stars. Previous cosmological solutions proposed to resolve this $^7$Li problem include photon cooling (possibly via the Bose-Einstein condensation of a scalar particle) or the decay of a long-lived $X-$particle (possibly the next-to-lightest supersymmetric particle). In this paper we reanalyze these solutions, both separately and in concert. We also introduce the possibility of a primordial magnetic field (PMF) into these models. We constrain the $X-$particles and the PMF parameters by the observed light element abundances using a likelihood analysis to show that the inclusion of all three possibilities leads to an optimum solution to the lithium problem. We deduce allowed ranges for the $X-$particle parameters and energy density in the PMF that can solve $^7$Li problem.

  15. Carbon-enhanced metal-poor stars: a window on AGB nucleosynthesis and binary evolution. I. Detailed analysis of 15 binary stars with known orbital periods

    E-Print Network [OSTI]

    Abate, C; Karakas, A I; Izzard, R G

    2015-01-01T23:59:59.000Z

    AGB stars are responsible for producing a variety of elements, including carbon, nitrogen, and the heavy elements produced in the slow neutron-capture process ($s$-elements). There are many uncertainties involved in modelling the evolution and nucleosynthesis of AGB stars, and this is especially the case at low metallicity, where most of the stars with high enough masses to enter the AGB have evolved to become white dwarfs and can no longer be observed. The stellar population in the Galactic halo is of low mass ($\\lesssim 0.85M_{\\odot}$) and only a few observed stars have evolved beyond the first giant branch. However, we have evidence that low-metallicity AGB stars in binary systems have interacted with their low-mass secondary companions in the past. The aim of this work is to investigate AGB nucleosynthesis at low metallicity by studying the surface abundances of chemically peculiar very metal-poor stars of the halo observed in binary systems. To this end we select a sample of 15 carbon- and $s$-element-en...

  16. Voluntary Disclosure and Information Asymmetry: Evidence from the 2005 Securities Offering Reform

    E-Print Network [OSTI]

    SHROFF, NEMIT

    In 2005, the Securities and Exchange Commission enacted the Securities Offering Reform (Reform), which relaxes “gun-jumping” restrictions, thereby allowing firms to more freely disclose information before equity offerings. ...

  17. Electronic Resource Management Systems, Part II: Offerings from Serial Vendors and Serial Data Vendors

    E-Print Network [OSTI]

    Duranceau, Ellen

    2005-06-19T23:59:59.000Z

    In the September 2004 issue, I reported on the Electronic Resource Management (ERM) offerings of the major ILS vendors, and promised to follow with a second article covering the ERM tools offered by other kinds of companies, ...

  18. Offering Sign-On and Retention Bonus Payments to Faculty March 12, 2012

    E-Print Network [OSTI]

    Acton, Scott

    Offering Sign-On and Retention Bonus Payments to Faculty March 12, 2012 page 1 Policy on Offering Sign-On and Retention Bonus Payments to Faculty Date: March 12, 2012 Policy ID: 1.600 Status: Final for Policy: This policy was developed to clarify the approval required to offer a sign ­on or retention bonus

  19. Neutrino Physics and the Primordial Elemental Abundances

    E-Print Network [OSTI]

    Christian Y. Cardall; George M. Fuller

    1997-01-31T23:59:59.000Z

    Limits can be placed on nonstandard neutrino physics when big bang nucleosynthesis (BBN) calculations employing standard neutrino physics agree with the observationally inferred primordial abundances of deuterium (D), $^3$He, $^4$He, and $^7$Li. These constraints depend most sensitively on the abundances of D and $^4$He. New observational determinations of the primordial D and/or $^4$He abundances could force revisions in BBN constraints on nonstandard neutrino physics.

  20. Active-Sterile neutrino oscillations and BBN+CMBR constraints

    E-Print Network [OSTI]

    P. Di Bari; R. Foot

    2000-11-13T23:59:59.000Z

    We show how active-sterile neutrino oscillations in the early Universe can play an interesting role in explaining the current observations of CMBR anisotropies and light element abundances. We describe different possible phenomenological scenarios in the interpretation of present data and how active-sterile neutrino oscillations can provide a viable theoretical framework.

  1. Curriculum, Admissions, & Contact Information on Back Rochester Institute of Technology offers Masters and

    E-Print Network [OSTI]

    Zanibbi, Richard

    Curriculum, Admissions, & Contact Information on Back Rochester Institute of Technology offers in digital imaging, color instrumentation, colorant formulation, and basic & applied research. Employers

  2. Undergraduate Degrees Offered: Bachelor of Arts in Physics or Environmental Physics

    E-Print Network [OSTI]

    Undergraduate Degrees Offered: Bachelor of Arts in Physics or Environmental Physics Bachelor of Science in Physics or Environmental Physics Minor in Physics Graduate Degrees Offered: Doctor of Philosophy in Environmental Science and Resources: Physics Master of Science in Physics Master of Arts

  3. Special Offer for Indonesian Government DIKTI PhD Scholarship Awardees

    E-Print Network [OSTI]

    Special Offer for Indonesian Government DIKTI PhD Scholarship Awardees Charles Darwin University welcomes applications for PhD degrees from DIKTI scholarship awardees and offers English language must be provided at initial PhD application stage. Tuition fee waiver for a fourth year of study

  4. Neutrino Oscillations and the Early Universe

    E-Print Network [OSTI]

    D. P. Kirilova

    2003-12-21T23:59:59.000Z

    The observational and theoretical status of neutrino oscillations in connection with solar and atmospheric neutrino anomalies is presented in brief. The effect of neutrino oscillations on the early Universe evolution is discussed in detail. A short review is given of the standard Big Bang Nucleosynthesis and the influence of resonant and nonresonant neutrino oscillations on active neutrinos and on primordial nucleosynthesis of He-4. BBN cosmological constraints on neutrino oscillation parameters are discussed.

  5. The George R. Brown School of Engineering Degrees Offered: BA, MStat, MA, PhD

    E-Print Network [OSTI]

    Richards-Kortum, Rebecca

    Introduction to Engineering Computation · STAT 310 Probability and Statistics · STAT 410 Introduction246 Statistics The George R. Brown School of Engineering Degrees Offered: BA, MStat, MA, PhD Course engineering, computational and applied mathematics, managerial studies, mathematics, political science

  6. The George R. Brown School of Engineering Degrees Offered: BA, MStat, MA, PhD

    E-Print Network [OSTI]

    Richards-Kortum, Rebecca

    Introduction to Engineering Computation · STAT 310 Probability and Statistics · STAT 410 Introduction253 Statistics The George R. Brown School of Engineering Degrees Offered: BA, MStat, MA, PhD Course engineering, computational and applied mathematics, managerial studies, mathematics, political science

  7. Environmental Studies The Environmental Studies Program offers several interdisciplinary courses for

    E-Print Network [OSTI]

    Richards-Kortum, Rebecca

    185 Environmental Studies The Environmental Studies Program offers several interdisciplinary courses for students interested in broadening their understanding of environmental issues. These courses in an environmental program have 3 options: environmental science (see below), environmental engineering sciences (see

  8. Environmental Studies The Environmental Studies Program offers several interdisciplinary courses for

    E-Print Network [OSTI]

    Richards-Kortum, Rebecca

    177 Environmental Studies The Environmental Studies Program offers several interdisciplinary courses for students interested in broadening their understanding of environmental issues. These courses in an environmental program have 3 options: environmental science (see below), environmental engineering sciences (see

  9. Why Should I Study Engineering? Georgia Southern offers three engineering disciplines Civil, Electrical and Mechanical.

    E-Print Network [OSTI]

    Hutcheon, James M.

    , Electrical and Mechanical. Engineers plan, design, develop, test and analyze infrastructure components (CivilWhy Should I Study Engineering? Georgia Southern offers three engineering disciplines ­ Civil), electronic systems (Electrical), and systems with moving parts (Mechanical) that affect and improve people

  10. Customer Response to RTP in Competitive Markets: A Study of Niagara Mohawk's Standard Offer Tariff

    E-Print Network [OSTI]

    Boisvert, Richard N.; Cappers, Peter; Goldman, Charles; Neenan, Bernie; Hopper, Nicole

    2006-01-01T23:59:59.000Z

    Niagara Mohawk’s Standard Offer Tariff * Richard N. BoisvertThis default-service commodity tariff (“SC-3A Option One”)electricity usage data, tariff history, basic customer

  11. FEMP Offers Training on Federal On-Site Renewable Power Purchase...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Training on Federal On-Site Renewable Power Purchase Agreements FEMP Offers Training on Federal On-Site Renewable Power Purchase Agreements March 30, 2015 - 2:16pm Addthis The U.S....

  12. DENTAL CLINIC PROPERTIES FOR SALE OFFERED BY THE UNIVERSITY OF NEVADA, LAS VEGAS

    E-Print Network [OSTI]

    Hemmers, Oliver

    DENTAL CLINIC PROPERTIES FOR SALE OFFERED BY THE UNIVERSITY OF NEVADA, LAS VEGAS PROPERTY ADDRESSES Clinics 818 E. Sahara 2 parcels 0.45 acre Building 2,346 gsf Const Yr. 1966 864 E. Sahara 2 parcels 0

  13. Success at Sea: Maritime Votive Offerings and Naval Dedications in Antiquity

    E-Print Network [OSTI]

    Streuding, Jaclyn Haley

    2014-06-26T23:59:59.000Z

    , as well as explore the relationship between dedicant and dedicatee. Also, I consider the geographical location of a site or maritime sanctuary, and the impact it may have had on the types of objects offered. Following a thorough investigation...

  14. The University of Mississippi-Grenada offers graduate degree programs geared to working adults, including

    E-Print Network [OSTI]

    Tchumper, Gregory S.

    and Instruction (MACI) is for students who currently hold a bachelor's degree in a field other than education-Grenada ITC Building Find us on Facebook! #12;UM/ School District Bank Hours The UM School of Education offers

  15. The Impact on the New Mexico Budget of Offering Domestic Partnerships to Same-Sex Couples

    E-Print Network [OSTI]

    Sears, Brad

    2010-01-01T23:59:59.000Z

    same-sex couples in New Mexico who choose to celebrate theirThe Impact on the New Mexico Budget of Offering DomesticCommittee of the New Mexico Senate Presented by Professor

  16. Jefferson Lab Offers Science Enrichment Program for 5th, 6th...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Jefferson Lab Offers Science Enrichment Program for 5th, 6th & 8th Grade Teachers; Registration Deadline is Sept. 12 Jefferson Lab Open House For many teachers who enroll in...

  17. Reaction rates of $^{64}$Ge($p,?$)$^{65}$As and $^{65}$As($p,?$)$^{66}$Se and the extent of nucleosynthesis in type I X-ray bursts

    E-Print Network [OSTI]

    Y. H. Lam; J. J. He; A. Parikh; B. A. Brown; M. Wang; B. Guo; Y. H. Zhang; X. H. Zhou; H. S. Xu

    2015-05-09T23:59:59.000Z

    The extent of nucleosynthesis in models of type I X-ray bursts and the associated impact on the energy released in these explosive events are sensitive to nuclear masses and reaction rates around the $^{64}$Ge waiting point. Using a recent high precision mass measurement of $^{65}$As along with large-scale shell model calculations, we have determined new thermonuclear rates of the $^{64}$Ge($p$,$\\gamma$)$^{65}$As and $^{65}$As($p$,$\\gamma$)$^{66}$Se reactions. We examine the impact of available rates for these two reactions through a representative one-zone X-ray burst model. We find that our recommended rates may strongly suppress the flow of abundances toward $A\\approx100$, in sharp contrast to recent work claiming that $^{64}$Ge is not a significant $rp$-process waiting point. Indeed, the summed mass fractions for species with $A > 70$ varies by about factors of 3 or 2 depending upon the adopted $^{64}$Ge($p$,$\\gamma$)$^{65}$As or $^{65}$As($p$,$\\gamma$)$^{66}$Se rates, respectively. Furthermore, the predictions for nuclear energy generation rate E$_\\mathrm{gen}$ at late times during the burst varies rather significantly between the models using the different rates, with differences as large as about a factor of 2.

  18. 9/18/09 2:55 PMScienceNology: Big Wave Theory Offers Alternative to Dark Energy Page 1 of 5http://sciencenology.blogspot.com/2009/08/big-wave-theory-offers-alternative-to.html

    E-Print Network [OSTI]

    Temple, Blake

    9/18/09 2:55 PMScienceNology: Big Wave Theory Offers Alternative to Dark Energy Page 1 of 5http Offers Alternative to Dark Energy Page 2 of 5http://sciencenology.blogspot.com/2009/08/big-wave-theory-offers-alternative://sciencenology.blogspot.com/2009/08/big-wave-theory-offers-alternative-to.html home posts rss comments rss edit Home Applied

  19. 9/18/09 2:09 PM'Big Wave' Theory Offers Alternative to Dark Energy -Physical Science Page 1 of 3http://scienceblips.dailyradar.com/story/big_wave_theory_offers_alternative_to_dark_energy/

    E-Print Network [OSTI]

    Temple, Blake

    9/18/09 2:09 PM'Big Wave' Theory Offers Alternative to Dark Energy - Physical Science Page 1 of 3http://scienceblips.dailyradar.com/story/big_wave_theory_offers_alternative_to_dark_energy/ Gadget.com - 30 days ago 'Big Wave' Theory Offers Alternative to Dark Energy -- Mathematicians have proposed

  20. 9/18/09 2:12 PM'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 4http://digg.com/general_sciences/Big_Wave_Theory_Offers_Alternative_to_Dark_Energy

    E-Print Network [OSTI]

    Temple, Blake

    9/18/09 2:12 PM'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 4http://digg.com/general_sciences/Big_Wave_Theory_Offers_Alternative_to_Dark_Energy show profanity settings Digg is a place Offers Alternative to Dark Energy space.com -- Mathematicians have proposed an alternative explanation

  1. The Drafting Technology Program offers a certificate or associate of applied science in drafting technology. The certificate program

    E-Print Network [OSTI]

    Ickert-Bond, Steffi

    DRAFTING TECHNOLOGY The Drafting Technology Program offers a certificate or associate of applied science in drafting technology. The certificate program offers a choice of six areas of emphasis: architectural drafting; civil drafting; information technology; mechanical and electrical drafting; process

  2. EXPLOSIVE NUCLEOSYNTHESIS IN THE NEUTRINO-DRIVEN ASPHERICAL SUPERNOVA EXPLOSION OF A NON-ROTATING 15 M{sub sun} STAR WITH SOLAR METALLICITY

    SciTech Connect (OSTI)

    Fujimoto, Shin-ichiro [Kumamoto National College of Technology, 2659-2 Suya, Goshi, Kumamoto 861-1102 (Japan); Kotake, Kei [Division of Theoretical Astronomy, National Astronomical Observatory Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Hashimoto, Masa-aki; Ono, Masaomi [Department of Physics, School of Sciences, Kyushu University, Fukuoka 810-8560 (Japan); Ohnishi, Naofumi, E-mail: fujimoto@ec.knct.ac.jp [Department of Aerospace Engineering, Tohoku University, 6-6-01 Aramaki-Aza-Aoba, Aoba-ku, Sendai 980-8579 (Japan)

    2011-09-01T23:59:59.000Z

    We investigate explosive nucleosynthesis in a non-rotating 15 M{sub sun} star with solar metallicity that explodes by a neutrino-heating supernova (SN) mechanism aided by both standing accretion shock instability (SASI) and convection. To trigger explosions in our two-dimensional hydrodynamic simulations, we approximate the neutrino transport with a simple light-bulb scheme and systematically change the neutrino fluxes emitted from the protoneutron star. By a post-processing calculation, we evaluate abundances and masses of the SN ejecta for nuclei with a mass number {<=}70, employing a large nuclear reaction network. Aspherical abundance distributions, which are observed in nearby core-collapse SN remnants, are obtained for the non-rotating spherically symmetric progenitor, due to the growth of a low-mode SASI. The abundance pattern of the SN ejecta is similar to that of the solar system for models whose masses range between (0.4-0.5) M{sub sun} of the ejecta from the inner region ({<=}10, 000 km) of the precollapse core. For the models, the explosion energies and the {sup 56}Ni masses are {approx_equal} 10{sup 51}erg and (0.05-0.06) M{sub sun}, respectively; their estimated baryonic masses of the neutron star are comparable to the ones observed in neutron-star binaries. These findings may have little uncertainty because most of the ejecta is composed of matter that is heated via the shock wave and has relatively definite abundances. The abundance ratios for Ne, Mg, Si, and Fe observed in the Cygnus loop are reproduced well with the SN ejecta from an inner region of the 15 M{sub sun} progenitor.

  3. Fact #857 January 26, 2015 Number of Partner Workplaces Offering Electric Vehicle Charging More Than Tripled Since 2011 – Dataset

    Broader source: Energy.gov [DOE]

    Excel file with dataset for Number of Partner Workplaces Offering Electric Vehicle Charging More Than Tripled Since 2011

  4. MedicineUndergradUate stUdy We offer many opportunities for you to

    E-Print Network [OSTI]

    Guo, Zaoyang

    MedicineUndergradUate stUdy #12;Visit us We offer many opportunities for you to visit us and find;Medicine is based in our Wolfson Medical School Building on the main campus. #12;Medicine Medicine is about-centredlearning,andhasaspiral course structure. This means that you will revisit topics on several occasions as you progress through

  5. The Glass Box offers a unique environment to support research, development and evaluation of software

    E-Print Network [OSTI]

    The Glass Box offers a unique environment to support research, development and evaluation of software products used by workers performing real computer- based tasks. The Glass Box instrumentation and to retrieve, store, and share Glass Box data. · Test Bed environment­Glass Box serves as a test bed

  6. What is Personal Training? Personal Training offers a one-on-one

    E-Print Network [OSTI]

    McConnell, Terry

    PERSONAL TRAINING What is Personal Training? Personal Training offers a one-on-one private workout program, your Personal Trainer will help you reach your goals. Learn the different weight training will begin your Personal Training program with a fitness assessment, which will give the trainer

  7. technology offer SandTES -High Temperature Sand Thermal Energy Storage

    E-Print Network [OSTI]

    Szmolyan, Peter

    technology offer SandTES - High Temperature Sand Thermal Energy Storage key words: High Temperature Energy Storage | Fluidized Bed | Sand | The invention consists of a fluidized bed with internal heat together with Dr. Eisl of ENRAG GmbH. Background Thermal energy storage (TES) systems are essential

  8. The George R. Brown School of Engineering Degrees Offered: BA, MStat, MA, PhD

    E-Print Network [OSTI]

    Richards-Kortum, Rebecca

    211Introduction to Engineering Computation · STAT310Probability and Statistics · STAT410Introduction263 Statistics The George R. Brown School of Engineering Degrees Offered: BA, MStat, MA, PhD Course engineering, computational and applied mathematics, managerial studies, mathematics, political science

  9. Who can help me? The Safety Office offers ergonomic assessments for

    E-Print Network [OSTI]

    Martin, Jeff

    Who can help me? The Safety Office offers ergonomic assessments for all University of Winnipeg employees. Call 786.9894 to arrange an appointment. For more information on ergonomics, visit the Safety Office website at www. uwinnipeg.ca/index/safety-safety. ERGONOMICS OFFICE What is ergonomics? Ergonomics

  10. Environmental Studies The Environmental Studies Program offers several interdisciplinary courses for

    E-Print Network [OSTI]

    Richards-Kortum, Rebecca

    171 Environmental Studies The Environmental Studies Program offers several interdisciplinary courses for students interested in broadening their understanding of environmental issues. These courses are often team-taught by faculty from various areas of study. Students wishing to major in an environmental

  11. Environmental Studies The Environmental Studies Program offers several interdisciplinary courses for

    E-Print Network [OSTI]

    Richards-Kortum, Rebecca

    173 Environmental Studies The Environmental Studies Program offers several interdisciplinary courses for students interested in broadening their understanding of environmental issues. These courses are often team-taught by faculty from various areas of study. Students wishing to major in an environmental

  12. Environmental Studies The Environmental Studies Program offers several interdisciplinary courses for

    E-Print Network [OSTI]

    Richards-Kortum, Rebecca

    Environmental Studies The Environmental Studies Program offers several interdisciplinary courses for students interested in broadening their understanding of environmental issues. These courses often are team-taught by faculty from various areas of study. Students wishing to major in an environmental program have three

  13. Environmental Health Minor Students interested in the Environmental Health Minor offered by the Department of

    E-Print Network [OSTI]

    Massachusetts at Lowell, University of

    Environmental Health Minor Students interested in the Environmental Health Minor offered.252 Physiological Chemistry II + lab (Gened SCL) 4 credits 31.313 Principles of Environmental Health 3 credits or 2 of the following courses (3 credits each): 31.316 Environmental Health in Practice 31.371 Food

  14. Environmental Studies The Environmental Studies Program offers several interdisciplinary courses for

    E-Print Network [OSTI]

    Richards-Kortum, Rebecca

    1 Environmental Studies The Environmental Studies Program offers several interdisciplinary courses for students interested in broadening their understanding of environmental issues. These courses often are team-taught by faculty from various areas of study. Students wishing to major in an environmental program have three

  15. Madrid, Spain *This program is offered every Summer, Spring and Fall

    E-Print Network [OSTI]

    Ponce, V. Miguel

    Madrid, Spain *This program is offered every Summer, Spring and Fall To view the most recent information about the Spanish Language Immersion Program in Spain please go to the SDSU College of Extended 2009 Gloria Cossio and Jose Alberto Martinez Spain Summer 2008 Experience by Rodolfo Nubes My

  16. Erasmus Student Work Placement Offer in Spanish educational institutions in the Canary Islands

    E-Print Network [OSTI]

    Robbiano, Lorenzo

    Erasmus Student Work Placement Offer in Spanish educational institutions in the Canary Islands on the Regional Ministry of Education and Universities of the Canary Islands Government (Spain). Its objective Erasmus students on their placements. Placements available for Erasmus students In the Canary Islands

  17. Course offer (1/2) Hydrology II (1st Sem. MSc)

    E-Print Network [OSTI]

    Giger, Christine

    1 Course offer (1/2) · Hydrology II (1st Sem. MSc) · advanced engineering hydrology course focused on hydrological monitoring, processunderstanding and new analysis and modelling techniques · Fluvial Systems (1st management and riverine ecosystem sustainability · Hydrology of Glaciers (2nd Sem. MSc) · study of ice

  18. EU Gives Japan Until End-June to Accept Nuclear-Project Offer

    E-Print Network [OSTI]

    must begin this year. The EU made the partnership offer in November to break a deadlock in which China of negotiations.'' ITER, which would generate ``clean'' energy by fusing together light atoms such as hydrogen reach an agreement. ``Only on a political level is it possible to get a solution quickly,'' he said

  19. Degrees Offered: MS Rice University introduced the professional master's degree in environmental

    E-Print Network [OSTI]

    Richards-Kortum, Rebecca

    in the Environment(F) CEVE536Environmental Biotechnology and Bioremediation(S) CEVE 550 Environmental Organic1 Degrees Offered: MS Rice University introduced the professional master's degree in environmental.Asaninterdisciplinaryprogram, it aims to give students the ability to predict environmental problems, not just solve them. It emphasizes

  20. Unique among undergraduate programs offered nationally, the major in Latin American, Caribbean and

    E-Print Network [OSTI]

    Saldin, Dilano

    Unique among undergraduate programs offered nationally, the major in Latin American, Caribbean and U.S. Latino Studies (LACUSL) integrates the study of the Latin American and Caribbean region knowledge of U.S. Latino, Latin American and Caribbean history and culture · develop analytical and critical

  1. DIESEL/HEAVY The diesel/heavy equipment certificate offers training in maintenance

    E-Print Network [OSTI]

    Ickert-Bond, Steffi

    DIESEL/HEAVY EQUIPMENT The diesel/heavy equipment certificate offers training in maintenance and repair of heavy equipment and trucks. Students will learn to work on electrical and air systems, diesel · Small Engines · Automotive Maintenance · Welding · Training for entry level heavy diesel equipment

  2. Science Highlight August 2010 New State of Topological Insulators Offers New Opportunities

    E-Print Network [OSTI]

    Wechsler, Risa H.

    Science Highlight ­ August 2010 New State of Topological Insulators Offers New Opportunities Three dimensional topological insulators are a new state of quantum matter with a bulk gap and odd number insulator enters the insulating masive Dirac fermion state, a state that harbors striking topological

  3. inverters, offering less weight, higher efficiency, and lower-cost installations.

    E-Print Network [OSTI]

    Johnson, Eric E.

    inverters, offering less weight, higher efficiency, and lower- cost installations. The electrical. These locking connectors will also soon appear on most, if not all, PV modules--although they are only required when the PV array wiring is operating above 30 volts and is readily accessible. Another 2008 NEC

  4. Deregulating Residential Electricity Markets: What's on Offer? Catherine Waddams Price1

    E-Print Network [OSTI]

    Feigon, Brooke

    Deregulating Residential Electricity Markets: What's on Offer? Catherine Waddams Price1 ESRC Centre on Electricity Pricing, 16 August 2007 1. Introduction The Australian Energy Markets Commission is considering the development of the gas and electricity markets in Victoria, and in particular the role of the safety net

  5. Computer Science The computer science program offers a foundation in the

    E-Print Network [OSTI]

    Miles, Will

    Computer Science The computer science program offers a foundation in the fundamentals of computer, the entertainment industry or government, the computer science major, which emphasizes the theory and application in computer science, students develop expertise in systems analysis, software development, networking

  6. As the BPM marketplace continues its rapid evolution, there is an increasing array of technology offerings

    E-Print Network [OSTI]

    van der Aalst, Wil

    As the BPM marketplace continues its rapid evolution, there is an increasing array of technology) the increasing diversity of offerings that fall under the BPM technology umbrella, and (2) the complexity. As illustrated in Figure 1, the potential range of tech- nologies on which a BPM solution might be based

  7. A method for classifying offer strategies observed in an electricity market

    E-Print Network [OSTI]

    characteristics of software agents that were designed based on the outcome of human subject experiments, in some sense, their behaviors are roughly identical. Our experiments with trained humans have shown as a replacement for the human agents used in the real world to offer energy into a market. Well-designed software

  8. BEE 4900/AEM 6900. Biofuels: The Economic and Environmental Interactions (offered Spring 2008)

    E-Print Network [OSTI]

    Walter, M.Todd

    BEE 4900/AEM 6900. Biofuels: The Economic and Environmental Interactions (offered Spring 2008 and Economics of BioFuels. Questions addressed include the environmental and economic impacts of biofuel use and whether the use of biofuels justifies public policy intervention. The class will consist of a colloquium

  9. technology offer Vienna University of Technology | Research and Transfer Support | Claudia Doubek

    E-Print Network [OSTI]

    Szmolyan, Peter

    technology offer Vienna University of Technology | Research and Transfer Support | Claudia Doubek will retain biomass and media components in the fermentation broth and therefore reduce media costs and vitamins are removed as well and have to be added again, at high costs. The problem to solve was to find

  10. technology offer Vienna University of Technology | Research and Transfer Support | Claudia Doubek

    E-Print Network [OSTI]

    Szmolyan, Peter

    technology offer Vienna University of Technology | Research and Transfer Support | Claudia Doubek. Researchers focused on low building costs, easy assembly and long service life. Investment costs as well as control and maintenance costs are extremely reduced in relation to state of the art expansion joints. Long

  11. Digital Arts The digital arts major offers coursework on a range of topics including

    E-Print Network [OSTI]

    Miles, Will

    Florida's growing digital media industry and world-famous tourism industry. Our relationshipDigital Arts The digital arts major offers coursework on a range of topics including image in these departments should consider the digital arts minor as a way to investigate the creative applications

  12. CHEMICAL ENGINEERING Page 1 of 9 SEMESTER OFFERED COURSE PRE-and/or CO-REQUISITES

    E-Print Network [OSTI]

    Calgary, University of

    CHEMICAL ENGINEERING Page 1 of 9 1st YEAR SEMESTER OFFERED COURSE PRE- and/or CO-REQUISITES FALL 1 Mechanics of Solids ENGG 202 or 205; AMAT 217 9 ENCH 315 Chemical Engineering Process Calculations Pre. All complementary studies courses must be taken prior to graduation. Chemical Engineering: Regular

  13. 718.982.3619 The Math Tutorial Lab offers walk-in tutoring for all

    E-Print Network [OSTI]

    Rosen, Jay

    , math, Core, psychology, computer science, physics, chemistry, engineering science, geology, astronomy-on-one and group tutoring for students enrolled in cinema and communications. 718.982.2850 Tutoring is offered by appointment or on a walk-in basis in all 100 and 200-level computer science courses. Tutors can assist

  14. Evaluation of Public Service Electric & Gas Company`s standard offer program, Volume I

    SciTech Connect (OSTI)

    Goldman, C.A.; Kito, M.S.; Moezzi, M.M.

    1995-07-01T23:59:59.000Z

    In May 1993, Public Service Electric and Gas (PSE&G), the largest investor-owned utility in New Jersey, initiated the Standard Offer program, an innovative approach to acquiring demand-side management (DSM) resources. In this program, PSE&G offers longterm contracts with standard terms and conditions to project sponsors, either customers or third-party energy service companies (ESCOs), on a first-come, first-serve basis to fill a resource block. The design includes posted, time-differentiated prices which are paid for energy savings that will be verified over the contract term (5, 10, or 15 years) based on a statewide measurement and verification (M&V) protocol. The design of the Standard Offer differs significantly from DSM bidding programs in several respects. The eligibility requirements and posted prices allow ESCOs and other energy service providers to market and develop projects among customers with few constraints on acceptable end use efficiency technologies. In contrast, in DSM bidding, ESCOs typically submit bids without final commitments from customers and the utility selects a limited number of winning bidders who often agree to deliver a pre-specified mix of savings from various end uses in targeted markets. The major objectives of the LBNL evaluation were to assess market response and customer satisfaction; analyze program costs and cost-effectiveness; review and evaluate the utility`s administration and delivery of the program; examine the role of PSE&G`s energy services subsidiary (PSCRC) in the program and the effect of its involvement on the development of the energy services industry in New Jersey; and discuss the potential applicability of the Standard Offer concept given current trends in the electricity industry (i.e., increasing competition and the prospect of industry restructuring).

  15. 9/18/09 2:43 PM'Big Wave' Theory Offers Alternative to Dark Energy // Current Page 1 of 11http://current.com/items/90718274_big-wave-theory-offers-alternative-to-dark-energy.htm

    E-Print Network [OSTI]

    Temple, Blake

    9/18/09 2:43 PM'Big Wave' Theory Offers Alternative to Dark Energy // Current Page 1 of 11http://current.com/items/90718274_big-wave-theory-offers-alternative-to-dark-energy.htm login | register |home tv shows schedule to Dark Energy // Current Page 2 of 11http://current.com/items/90718274_big-wave-theory-offers-alternative-to-dark-energy

  16. Marketplace Training Marketplace offers several training opportunities below. To request a dedicated training for your department or group, or for

    E-Print Network [OSTI]

    Tsien, Roger Y.

    Marketplace Training Marketplace offers several training opportunities below. To request a dedicated training for your department or group, or for general questions about Marketplace please contact

  17. Meeting Offers Opportunity to Discuss EM Cleanup with China | Department of

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the.pdfBreaking ofOil & GasTechnical PublicationsDepartmentEnergy Meeting Offers

  18. DOT Offers nearly $25 Million for More Zero-Emission Buses | Department of

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the YouTube| Department ofDepartment9-92January 20,Department of(JulyEnergy Offers

  19. Solid waste management of temple floral offerings by vermicomposting using Eisenia fetida

    SciTech Connect (OSTI)

    Singh, Akanksha, E-mail: bhuaks29@gmail.com [Department of Botany, Banaras Hindu University, Varanasi 221 005 (India); Jain, Akansha, E-mail: akansha007@rediffmail.com [Department of Botany, Banaras Hindu University, Varanasi 221 005 (India); Sarma, Birinchi K., E-mail: birinchi_ks@yahoo.com [Department of Mycology and Plant Pathology, Institute of Agricultural Sciences, Banaras Hindu University, Varanasi 221 005 (India); Abhilash, P.C., E-mail: pca.iesd@bhu.ac.in [Institute for Environment and Sustainable Development, Banaras Hindu University, Varanasi 221 005 (India); Singh, Harikesh B., E-mail: hbs1@rediffmail.com [Department of Mycology and Plant Pathology, Institute of Agricultural Sciences, Banaras Hindu University, Varanasi 221 005 (India)

    2013-05-15T23:59:59.000Z

    Highlights: ? Effective management of temple floral offerings using E. fetida. ? Physico-chemical properties in TW VC were better especially EC, C/N, C/P and TK. ? TW VC as plant growth promoter at much lower application rates than KW and FYW VC. - Abstract: Recycling of temple waste (TW) mainly comprising of floral offerings was done through vermitechnology using Eisenia fetida and its impact on seed germination and plant growth parameters was studied by comparing with kitchen waste (KW) and farmyard waste (FYW) vermicompost (VC). The worm biomass was found to be maximum in TW VC compared to KW and FYW VCs at both 40 and 120 days old VCs. Physico-chemical analysis of worm-worked substrates showed better results in TW VC especially in terms of electrical conductivity, C/N, C/P and TK. 10% TW VC–water extract (VCE) showed stimulatory effect on germination percentage of chickpea seeds while KW and FYW VCE proved effective at higher concentration. Variation in growth parameters was also observed with change in the VC–soil ratio and TW VC showed enhanced shoot length, root length, number of secondary roots and total biomass at 12.5% VC compared to KW and FYW VC.

  20. OIL and GAS ENGINEERING Page 1 of 2 SEMESTER OFFERED COURSE PRE-and/or CO-REQUISITES

    E-Print Network [OSTI]

    Calgary, University of

    OIL and GAS ENGINEERING Page 1 of 2 1st Year SEMESTER OFFERED COURSE PRE- and/or CO-REQUISITES FALL-req: AMAT 219 2nd Year Oil and Gas Engineering: Regular Program SEMESTER OFFERED COURSE PRE- and/or CO Mechanics of Solids ENGG 202 or 205; AMAT 217 3rd Year Oil and Gas Engineering: Regular Program SEMESTER

  1. Santander Master's Scholarship The University of Stirling is pleased to offer nine 5,000 taught postgraduate scholarships

    E-Print Network [OSTI]

    Little, Tony

    Santander Master's Scholarship The University of Stirling is pleased to offer nine £5,000 taught annually? 4 scholarships - Stirling Master of Business Administration (MBA) 2 scholarships - MSc have accepted an offer of a place to study one of the named programmes at the University of Stirling

  2. Large neutrino asymmetries from neutrino oscillations

    E-Print Network [OSTI]

    R. Foot; M. J. Thomson; R. R. Volkas

    1995-09-19T23:59:59.000Z

    We re-examine neutrino oscillations in the early universe. Contrary to previous studies, we show that large neutrino asymmetries can arise due to oscillations between ordinary neutrinos and sterile neutrinos. This means that the Big Bang Nucleosynthesis (BBN) bounds on the mass and mixing of ordinary neutrinos with sterile neutrinos can be evaded. Also, it is possible that the neutrino asymmetries can be large (i.e. $\\stackrel{>}{\\sim} 10\\%$), and hence have a significant effect on BBN through nuclear reaction rates.

  3. Precision Cosmology and the Density of Baryons in the Universe

    E-Print Network [OSTI]

    M. Kaplinghat; M. S. Turner

    2000-11-14T23:59:59.000Z

    Big-bang Nucleosynthesis (BBN) and Cosmic Microwave Background (CMB) anisotropy measurements give independent, accurate measurements of the baryon density and can test the framework of the standard cosmology. Early CMB data are consistent with the longstanding conclusion from BBN that baryons constitute a small fraction of matter in the Universe, but may indicate a slightly higher value for the baryon density. We clarify precisely what the two methods determine, and point out that differing values for the baryon density can indicate either an inconsistency or physics beyond the standard models of cosmology and particle physics. We discuss other signatures of the new physics in CMB anisotropy.

  4. Niger, with new oil legislation, offers little drilled acreage for exploration

    SciTech Connect (OSTI)

    Bruneton, A. (Beicip, Rueil-Malmaison (FR))

    1991-09-16T23:59:59.000Z

    This paper reports on the Ministry of Mines and Energy of Niger has released acreage in East Niger to the international oil industry. Four blocks will be opened in a first step with no fixed time schedule for offers. The blocks are largely underexplored and are near significant oil indications. Niger, between Algeria and Nigeria, represents a transitional link between North Africa and Central Africa. The Republic of Niger, with the exception of its capital Niamey, is sparsely populated with 7 million people on a 1.3 million sq mile territory. Easy communications exist with neighboring Nigeria, Mali, and Chad. The arid climate allows for year round working conditions and easy access to opened areas.

  5. Fruit and Vegetable Servings in Local Farm-Sourced and Standard Lunches Offered to Children in a Head Start Program

    E-Print Network [OSTI]

    Johnson, Amy M.

    2010-04-25T23:59:59.000Z

    . Independent-samples t-tests were performed using SPSS. There were no significant differences in either fruit or vegetable consumption between conventional lunches and locally-sourced lunches. Even though there was more variety of fruit and vegetable offerings...

  6. Here is a list of all the categories (Subject and Event types) that UBCevents currently offers: Subject -Aboriginal

    E-Print Network [OSTI]

    Schluter, Dolph

    Here is a list of all the categories (Subject and Event types) that UBCevents currently offers - Graduation Subject - International Subject - Learning And Research - Arts, Humanities And Social Sciences Subject - Learning And Research - Business Subject - Learning And Research - Community Subject - Learning

  7. Certificate in Geographic Information Science The Environmental Science programs and the Departments of Earth Sciences and Biology offer

    E-Print Network [OSTI]

    Adl, Sina

    Certificate in Geographic Information Science The Environmental Science programs and the Departments of Earth Sciences and Biology offer a Certificate in Geographic Information Science information science. This Certificate can be completed by a student in a BSc program, in addition

  8. The North Carolina Solar Center offers free and fee-based technical services for manufacturers and other

    E-Print Network [OSTI]

    The North Carolina Solar Center offers free and fee- based technical services for manufacturers Training. Renewable Energy Assessments The Solar Center's renewable energy assessments focus on practical ways companies can incorporate renewable energy into their facilities and existing energy systems

  9. Techno-Economic Analysis of BEV Service Providers Offering Battery Swapping Services: Preprint

    SciTech Connect (OSTI)

    Neubauer, J.; Pesaran, A.

    2013-03-01T23:59:59.000Z

    Battery electric vehicles (BEVs) offer the potential to reduce both oil imports and greenhouse gas emissions, but high upfront costs, battery-limited vehicle range, and concern over high battery replacement costs may discourage potential buyers. A subscription model in which a service provider owns the battery and supplies access to battery swapping infrastructure could reduce upfront and replacement costs for batteries with a predictable monthly fee, while expanding BEV range. Assessing the costs and benefits of such a proposal are complicated by many factors, including customer drive patterns, the amount of required infrastructure, battery life, etc. The National Renewable Energy Laboratory has applied its Battery Ownership Model to compare the economics and utility of BEV battery swapping service plan options to more traditional direct ownership options. Our evaluation process followed four steps: (1) identifying drive patterns best suited to battery swapping service plans, (2) modeling service usage statistics for the selected drive patterns, (3) calculating the cost-of-service plan options, and (4) evaluating the economics of individual drivers under realistically priced service plans. A service plan option can be more cost-effective than direct ownership for drivers who wish to operate a BEV as their primary vehicle where alternative options for travel beyond the single-charge range are expensive, and a full-coverage-yet-cost-effective regional infrastructure network can be deployed. However, when assumed cost of gasoline, tax structure, and absence of purchase incentives are factored in, our calculations show the service plan BEV is rarely more cost-effective than direct ownership of a conventional vehicle.

  10. Techno-Economic Analysis of BEV Service Providers Offering Battery Swapping Services

    SciTech Connect (OSTI)

    Neubauer, J. S.; Pesaran, A.

    2013-01-01T23:59:59.000Z

    Battery electric vehicles (BEVs) offer the potential to reduce both oil imports and greenhouse gas emissions, but high upfront costs, battery-limited vehicle range, and concern over high battery replacement costs may discourage potential buyers. A subscription model in which a service provider owns the battery and supplies access to battery swapping infrastructure could reduce upfront and replacement costs for batteries with a predictable monthly fee, while expanding BEV range. Assessing the costs and benefits of such a proposal are complicated by many factors, including customer drive patterns, the amount of required infrastructure, battery life, etc. The National Renewable Energy Laboratory has applied its Battery Ownership Model to compare the economics and utility of BEV battery swapping service plan options to more traditional direct ownership options. Our evaluation process followed four steps: (1) identifying drive patterns best suited to battery swapping service plans, (2) modeling service usage statistics for the selected drive patterns, (3) calculating the cost-of-service plan options, and (4) evaluating the economics of individual drivers under realistically priced service plans. A service plan option can be more cost-effective than direct ownership for drivers who wish to operate a BEV as their primary vehicle where alternative options for travel beyond the single-charge range are expensive, and a full-coverage-yet-cost-effective regional infrastructure network can be deployed. However, when assumed cost of gasoline, tax structure, and absence of purchase incentives are factored in, our calculations show the service plan BEV is rarely more cost-effective than direct ownership of a conventional vehicle.

  11. Yes No Offered Yes No Offered

    E-Print Network [OSTI]

    Snider, Barry B.

    2011 The Commonwealth of Massachusetts Executive Office of Health and Human Services Division of Health and the Division of Revenue as required by state regulation 114.5 CMR 18.00. Employee Signature Employee Affidavit for the full costs of all medical treatment, that I may forfeit all or a portion of my Massachusetts personal

  12. Reaction rates of $^{64}$Ge($p,\\gamma$)$^{65}$As and $^{65}$As($p,\\gamma$)$^{66}$Se and the extent of nucleosynthesis in type I X-ray bursts

    E-Print Network [OSTI]

    Lam, Y H; Parikh, A; Brown, B A; Wang, M; Guo, B; Zhang, Y H; Zhou, X H; Xu, H S

    2015-01-01T23:59:59.000Z

    The extent of nucleosynthesis in models of type I X-ray bursts and the associated impact on the energy released in these explosive events are sensitive to nuclear masses and reaction rates around the $^{64}$Ge waiting point. Using a recent high precision mass measurement of $^{65}$As along with large-scale shell model calculations, we have determined new thermonuclear rates of the $^{64}$Ge($p$,$\\gamma$)$^{65}$As and $^{65}$As($p$,$\\gamma$)$^{66}$Se reactions. We examine the impact of available rates for these two reactions through a representative one-zone X-ray burst model. We find that our recommended rates may strongly suppress the flow of abundances toward $A\\approx100$, in sharp contrast to recent work claiming that $^{64}$Ge is not a significant $rp$-process waiting point. Indeed, the summed mass fractions for species with $A > 70$ varies by about factors of 3 or 2 depending upon the adopted $^{64}$Ge($p$,$\\gamma$)$^{65}$As or $^{65}$As($p$,$\\gamma$)$^{66}$Se rates, respectively. Furthermore, the predi...

  13. A Secure Content Network in Space Craig Partridge

    E-Print Network [OSTI]

    Strayer, William Timothy

    A Secure Content Network in Space Craig Partridge Raytheon BBN Technologies craig@bbn.com Robert Walsh Raytheon BBN Technologies rwalsh@bbn.com Matthew Gillen Raytheon BBN Technologies mgillen@bbn.com Gregory Lauer Raytheon BBN Technologies glauer@bbn.com John Lowry Raytheon BBN Technologies jlowry

  14. The beauty of the intricate shapes of spider webs fascinates people, but webs offer more than aesthetic appeal for

    E-Print Network [OSTI]

    Blackledge, Todd

    1937 The beauty of the intricate shapes of spider webs fascinates people, but webs offer more than aesthetic appeal for biological research. The silk fibers used to construct webs have long been a favorite spun by only a few species of spiders, all of which construct similar types of orb webs. Orb webs, flat

  15. The Stark Center offers fieldwork positions for 327L students. The breadth of materials and ongoing projects at

    E-Print Network [OSTI]

    Patzek, Tadeusz W.

    The Stark Center offers fieldwork positions for 327L students. The breadth of materials and ongoing projects at the Stark Center provides for a variety of intern tasks and responsibilities pertaining during the long semester. Possible Intern Responsibilities: - Work on one major project throughout

  16. Important Resources for Transfer Students Office of Transfer Academic Services--offers academic and procedural assistance to Franklin

    E-Print Network [OSTI]

    Arnold, Jonathan

    Important Resources for Transfer Students Office of Transfer Academic Services--offers academic and procedural assistance to Franklin College transfer students adjusting to a new campus by providing resources, and preparing for exams. You'll find them at http://tutor.uga.edu/ or call 706-542-7575 Disability Resource

  17. OIL and GAS ENGINEERING Page 1 of 3 SEMESTER OFFERED COURSE PRE-REQUISITES listed in this column.

    E-Print Network [OSTI]

    Calgary, University of

    OIL and GAS ENGINEERING Page 1 of 3 1st Year SEMESTER OFFERED COURSE PRE-REQUISITES listed and Magnetism AMAT 217; MATH 211; recommended co-req: AMAT 219 2nd Year Oil and Gas Engineering: Regular Program correct. 2013/2014 Curriculum (Updated June 18, 2013) #12;OIL and GAS ENGINEERING Page 2 of 3 3rd Year Oil

  18. Internship Opportunities Thank you for contacting us about offering an internship to students at Murray Edwards College,

    E-Print Network [OSTI]

    Goldschmidt, Christina

    Internship Opportunities Thank you for contacting us about offering an internship to students of internship/work placement Position title and department: Length of internship and time of year the College is very willing to support shorter unpaid internships and work placements we also encourage

  19. Certificate in Geospatial Technology The School of Earth, Environment, and Society offers a graduate certificate in Geospatial

    E-Print Network [OSTI]

    Moore, Paul A.

    Certificate in Geospatial Technology The School of Earth, Environment, and Society offers a graduate certificate in Geospatial Technology. The purpose of the certificate program is to provide graduate students with training in geospatial theory, research design, and its application in fields

  20. Digital Eyes has the potential to be a transformative technology offering practical capabilities as a navigational aid for the visually

    E-Print Network [OSTI]

    Gray, Jeffrey G.

    Digital Eyes has the potential to be a transformative technology offering practical capabilities million preschool-age children and approximately twelve million school-age children. To put those numbers with a need for an alternative guide. There is a deep need for new research that can advance the technology

  1. Welcome to Union County Extension. The service offered to the citizens of Union County is a part-

    E-Print Network [OSTI]

    Jawitz, James W.

    education continues to be a Tri-County initiative through Bradford, Baker and Union County. This pro- gramWelcome to Union County Extension. The service offered to the citizens of Union County is a part- nership between Union County Board of County Commissioners and the University of Florida/IFAS. The mission

  2. Welcome to Union County Extension. The ser-vice offered to the citizens of Union County is a

    E-Print Network [OSTI]

    Jawitz, James W.

    Education: Pesticide education continues to be a Tri-County initiative through Bradford, Baker and UnionWelcome to Union County Extension. The ser- vice offered to the citizens of Union County is a partnership between Union County Board of County Commissioners and the University of Florida/IFAS. The mission

  3. Department of World Economy, St. Petersburg State University offers a position at the global PhD partnership programme

    E-Print Network [OSTI]

    Knobloch,Jürgen

    Department of World Economy, St. Petersburg State University offers a position at the global Ph and the global economy. The programme combines integrated training workshops and internship opportunities across: international relations, international political economy, area studies and new qualitative methods. Fluency

  4. 01MK4032 R6/13 Your student health insurance coverage, offered by Blue Cross and

    E-Print Network [OSTI]

    of Louisiana, may not meet the minimum standards required by the health care reform law for the restrictions01MK4032 R6/13 Your student health insurance coverage, offered by Blue Cross and Blue Shield and individual health insurance coverage are $1.25 million for policy years before September 23, 2012; and $2

  5. UC Davis Minors in Energy: Energy Science and Technology Minor (EEST) Offered by the Department of Biological and Agricultural Engineering

    E-Print Network [OSTI]

    Schladow, S. Geoffrey

    . Clean-tech and green-tech markets including energy are some of the fastest growing of new investment1 UC Davis Minors in Energy: Energy Science and Technology Minor (EEST) Offered by the Department There is an urgent need to develop and commercialize technologies for the sustainable conversion and use of energy

  6. Career opportunities Dental hygiene is routinely listed as one of today's top-ten career fields, offering

    E-Print Network [OSTI]

    Career opportunities Dental hygiene is routinely listed as one of today's top-ten career fields for all other occupations. Dental hygiene at Wichita State Wichita State is the only school in the state of Kansas to offer bachelor's degrees in dental hygiene and provides two programs for students to choose

  7. Computer Science Programs Available at FAU's Treasure Coast Campus Florida Atlantic University's College of Engineering and Computer Science offers exciting

    E-Print Network [OSTI]

    Fernandez, Eduardo

    Computer Science Programs Available at FAU's Treasure Coast Campus Florida Atlantic University's College of Engineering and Computer Science offers exciting degree programs in computer science.I.E.T.) and bachelor in computer science. The innovative B.I.E.T. degree program provides more hands-on, practical

  8. Performance Optimization of Battery-Super Capacitor Hybrid System Electrochemical capacitors (ultracapacitors) offer high power density when compared to battery

    E-Print Network [OSTI]

    Popov, Branko N.

    Performance Optimization of Battery-Super Capacitor Hybrid System Electrochemical capacitors a decreased value of power and energy densities for the hybrid system. Figure 1shows the fractional capacity (ultracapacitors) offer high power density when compared to battery systems and also have a relatively large energy

  9. Operating agricultural equipment accurately can be difficult, tedious, or even hazardous. Automatic control offers many potential advantages over human

    E-Print Network [OSTI]

    Stanford University

    , and automatic control. CDGPS-based control systems have been utilized in a number of applications, including. An automatic control system was developed, simulated in software using a simple kinematic vehicle model. Automatic control offers many potential advantages over human control; however, previous efforts to automate

  10. OIL and GAS ENGINEERING Page 1 of 3 SEMESTER OFFERED PRE-REQUISITES are listed in this column.

    E-Print Network [OSTI]

    Calgary, University of

    OIL and GAS ENGINEERING Page 1 of 3 1st Year SEMESTER OFFERED PRE-REQUISITES are listed AMAT 217 and MATH 211; recommended co-req: AMAT 219 2nd Year Oil and Gas Engineering: Regular Program will be deemed correct. 2014/2015 Curriculum (Updated June 13, 2014) #12;OIL and GAS ENGINEERING Page 2 of 3 3rd

  11. Recruitment Visit Support Guidelines The University Graduate School will support campus visits for students being offered the following

    E-Print Network [OSTI]

    Indiana University

    reimbursements for departments who are recruiting students as an SAA only; the offers must include at least one in excess of 3000 For students within 250 miles, a maximum of $200 will be paid (at the IU rate shown above living between 250-500 miles from Bloomington, a maximum of $350 will be paid (at the IU rate per shown

  12. Making the Most of your Internship: * Look for an Internship Offering a Substantial Learning Opportunity: The best opportunities are those

    E-Print Network [OSTI]

    Bertini, Robert L.

    Making the Most of your Internship: * Look for an Internship Offering a Substantial Learning. * Set Personal Goals: Some internships are project-oriented or structured, some are not. With the help to accomplish or skills you would like to acquire. Setting intentions before beginning your internship

  13. National Diabetes Prevention Program The University of Florida/IFAS Extension Bay County office is offering the Center for Disease

    E-Print Network [OSTI]

    Jawitz, James W.

    National Diabetes Prevention Program (NDPP) The University of Florida/IFAS Extension Bay County office is offering the Center for Disease Control-led National Diabetes Prevention Program (NDPP). The purpose of the NDPP Program is to reach individuals before they acquire diabetes. This is an evidence

  14. University Awards California State University, Fullerton offers a number of university-wide awards to students each year.

    E-Print Network [OSTI]

    de Lijser, Peter

    University Awards California State University, Fullerton offers a number of university-wide awards are a faculty member, we welcome your nomination of deserving students for whichever award you feel would Association Outstanding Graduate Student Award Amount: $1,000 Established by: This award was established

  15. Graduate Admissions * At this time the Petroleum Engineering Program offers two master degrees options. The master of petroleum

    E-Print Network [OSTI]

    Glowinski, Roland

    Graduate Admissions * At this time the Petroleum Engineering Program offers two master degrees options. The master of petroleum engineering requires courses only and known as the non-thesis option. The Master of Science in petroleum engineering requires fewer courses but also a thesis and is known

  16. Earth SciEncEUndErgradUatE StUdy We offer many opportunities for you to

    E-Print Network [OSTI]

    Guo, Zaoyang

    1 Earth SciEncEUndErgradUatE StUdy #12;Visit us We offer many opportunities for you to visit usUniversities&CollegesAdmissionsServices(UCAS), tel: 0871 468 0468 or see their website www.ucas.com OnE Of thE wOrld'S tOP 1% UniVErSitiES #12;Earth SciEncE Earth science is the study of the Earth, its structure, composition, history and resources

  17. 9/18/09 2:42 PM'Big Wave' Theory Offers Alternative to Dark Energy -Tech Support Forum Page 1 of 4http://www.techsupportforum.com/relaxation-room/offline/406161-big-wave-theory-offers-alternative-dark-energy.html

    E-Print Network [OSTI]

    Temple, Blake

    9/18/09 2:42 PM'Big Wave' Theory Offers Alternative to Dark Energy - Tech Support Forum Page 1 of 4http://www.techsupportforum.com/relaxation-room/offline/406161-big-wave-theory-offers-alternative-dark-energy' Theory Offers Alternative to Dark Energy User Name Remember Me? Password Log in Site Map Register Donate

  18. Brief History Degrees Offered

    E-Print Network [OSTI]

    Wang, Xiaorui "Ray"

    Technology Park · Provision Center for Proton Therapy · Nuclear Fuels and Materials · Nuclear Security · Radiological Sciences and Health Physics · Nuclear I&C, Reliability, and Safety · Nuclear Fuel Cycles Report at www.engr.utk.edu/nuclear or contact us at utne@tennessee.edu NE Welcomes New Faculty Dr. Jamie

  19. OFFERS THREE COMPLETION OPTIONS

    E-Print Network [OSTI]

    O'Toole, Alice J.

    Management Degree 28 Months · MBA (Product Lifecycle and Supply Chain Emphasis) 28 Months · CONVENIENT environment, it is crucial for executives to make decisions from an informed workplace. The Product Lifecycle to production, marketing to service, distribution to disposal, each step in the product lifecycle and supply

  20. SOLICITATION, OFFER AND AWARD

    National Nuclear Security Administration (NNSA)

    the aggregate for each nuclear incident or precautionary evacuation occurring within the United States or 500 million in the aggregate for each nuclear incident occurring outside...

  1. SOLICITATION, OFFER AND AWARD

    National Nuclear Security Administration (NNSA)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn AprilA Approved:AdministrationAnalysis andBHoneywell9/%2ARequest forMod0/%2A en

  2. SOLICITATION, OFFER AND AWARD

    National Nuclear Security Administration (NNSA)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn AprilA Approved:AdministrationAnalysis andBHoneywell9/%2ARequest forMod0/%2A en

  3. SOLICITATION, OFFER AND AWARD

    National Nuclear Security Administration (NNSA)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn AprilA Approved:AdministrationAnalysis andBHoneywell9/%2ARequest forMod0/%2A en

  4. Education in anesthesia for nurses entered a new era in Michigan in September 1963. Nine registered nurses entered the program in anesthesia offered by Detroit Receiving

    E-Print Network [OSTI]

    Berdichevsky, Victor

    History Education in anesthesia for nurses entered a new era in Michigan in September 1963. Nine registered nurses entered the program in anesthesia offered by Detroit Receiving Hospital in collaborationD., the Wayne State University Nurse Anesthesia Program (WSUNAP), became the first in the country to offer

  5. The University of Stirling Vietnam Award This award offers a fee waiver of 1,000 for the first year and 500 for years two,

    E-Print Network [OSTI]

    Little, Tony

    The University of Stirling Vietnam Award This award offers a fee waiver of £1,000 for the first-time undergraduate or postgraduate (taught or research) degree. The University of Stirling wishes to offer this award at Stirling and add to our already diverse international community on campus. Students do not have to apply

  6. FansyRoute: Adaptive Fan-Out for Variably Intermittent Challenged Networks

    E-Print Network [OSTI]

    Ramanathan, Ram

    Raytheon BBN Technologies 10 Moulton Street, Cambridge, MA 02138 dabideen@bbn.com Ram Ramanathan Raytheon

  7. Sierra Designs 20 degrees F Wild Bill Climashield Sleeping Bag ClimashieldTM HL, a high-loft continuous filament insulation, offers excellent thermal

    E-Print Network [OSTI]

    Walker, Lawrence R.

    -loft continuous filament insulation, offers excellent thermal efficiency, durability and water resistance Chest to create a pillow; no need for a pillow to take up valuable space in your backpack Insulated draft tube

  8. German Company Offers to Transform Sofia Waste to Energy The German company AlphaKat has filed a bid at Sofia municipality to construct an

    E-Print Network [OSTI]

    Columbia University

    and might be used for vehicles and heating. AlphaKat explained that under that technology 1liter of diesel of the offered technology include the fact that there would be no need for waste depots and baling systems

  9. Sale information 1.1. The description of each lot offered for sale is believed to be accurate, but is not

    E-Print Network [OSTI]

    been subject to a full tariff and offered for a lump sum. In all other respects the Purchaser is deemed estimates have been derived from a full Tariff unless otherwise stated. Tariff sheets may be inspected

  10. 50-Plus Ways to Be Water Smart 1. If your local water utility offers water-saving incentives or in-home water audits, take advantage

    E-Print Network [OSTI]

    50-Plus Ways to Be Water Smart BEHAVIORS 1. If your local water utility offers water-saving incentives or in-home water audits, take advantage of these programs. 2. Don't let water run while brushing

  11. Advances in r-Process Nucleosynthesis

    E-Print Network [OSTI]

    John J. Cowan; Christopher Sneden

    2003-09-29T23:59:59.000Z

    During the last several decades, there have been a number of advances in understanding the rapid neutron-capture process (i.e., the r-process). These advances include large quantities of high-resolution spectroscopic abundance data of neutron-capture elements, improved astrophysical models, and increasingly more precise nuclear and atomic physics data. The elemental abundances of the heavy neutron-capture elements, from Ba through the third r-process peak, in low-metallicity ([Fe/H] = 56 the r-process is robust--appearing to operate in a relatively consistent manner over the history of the Galaxy--and place stringent constraints on r-process models. While not yet identified, neutron-rich ejecta outside of the core in a collapsing (Type II, Ib) supernova continues to be a promising site for the r-process. Neutron star binary mergers might also be a possible alternative site. Abundance comparisons of lighter n-capture elements in halo stars show variations with the scaled solar r-process curve and might suggest either multiple r-process sites, or, at least, different synthesis conditions in the same astrophysical site. Constraints on r-process models and clues to the progenitors of the halo stars--the earliest generations of Galactic stars--are also provided by the star-to-star abundance scatter of [Eu/Fe] at low metallicities in the early Galaxy. Finally, abundance observations of long-lived radioactive elements (such as Th and U) produced in the r-process can be used to determine the chronometric ages of the oldest stars, placing constraints on the lower limit age estimates of the Galaxy and the Universe.

  12. Verification of Maxwell-Boltzmann distribution with Big-Bang Nucleosyntheis theory

    E-Print Network [OSTI]

    S. Q. Hou; J. J. He; others

    2014-06-18T23:59:59.000Z

    The current Big-Bang Nucleosynthesis (BBN) model has been constructed based on a nuclear reaction network operating with thermal reactivities of Maxwell-Boltzmann (MB) distribution plasma. However, does the classical MB distribution still hold for the extremely high-temperature (in order of 10$^9$ K) plasma involved in the Big-Bang environment? In this work, we have investigated the impact of non-extensive Tsallis statistics (in $q$-Guassian distribution) on the thermonuclear reaction rates. We show for the first time that the reverse rates are extremely sensitive to the non-extensive $q$ parameter. Such sensitivity does not allow a large deviation of non-extensive distribution from the usual MB distribution. With a newly developed BBN code, the impact of primordial light-element abundances on $q$ values has been studied by utilizing the most recent BBN cosmological parameters and the available nuclear cross-section data. For the first time, we have accurately verified the microscopic MB distribution with the macroscopic BBN theory and bservation. By comparing the recent observed primordial abundances with our predictions, only a tiny deviation of $\\pm$6$\\times$10$^{-4}$ at most can be allowed for the MB distribution. However, validity of the classical statistics needs to be studied further for the self-gravitating stars and binaries of high-density environment, with the extreme sensitivity of reverse rate on $q$ found here.

  13. 9/18/09 2:29 PM'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 6http://www.mastersconnection.com/index.php/articles/452-wave

    E-Print Network [OSTI]

    Temple, Blake

    9/18/09 2:29 PM'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 6http;9/18/09 2:29 PM'Big Wave' Theory Offers Alternative to Dark Energy Page 2 of 6http:29 PM'Big Wave' Theory Offers Alternative to Dark Energy Page 4 of 6http

  14. 10/14/09 2:29 PM'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 3http://www.thirdeyeconcept.com/news/index.php?topic=10126.0

    E-Print Network [OSTI]

    Temple, Blake

    10/14/09 2:29 PM'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 3http > Forum > Duality > The Eye > 'Big Wave' Theory Offers Alternative to Dark Energy Pages: [1] Go Down SEND THIS TOPIC | PRINT Author Topic: 'Big Wave' Theory Offers Alternative to Dark Energy (Read 59 times) 'Big

  15. 9/18/09 2:17 PM'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 20http://www.freerepublic.com/focus/f-chat/2319699/posts

    E-Print Network [OSTI]

    Temple, Blake

    9/18/09 2:17 PM'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 20http' Theory Offers Alternative to Dark Energy Space.com ^ | 8/18/09 | Clara Moskowitz Posted on August 19'Big Wave' Theory Offers Alternative to Dark Energy Page 2 of 20http

  16. A loophole to the universal photon spectrum in electromagnetic cascades: application to the "cosmological lithium problem"

    E-Print Network [OSTI]

    Poulin, Vivian

    2015-01-01T23:59:59.000Z

    The standard theory of electromagnetic cascades onto a photon background predicts a quasi-universal shape for the resulting non-thermal photon spectrum. This has been applied to very disparate fields, including non-thermal big bang nucleosynthesis (BBN). However, once the energy of the injected photons falls below the pair-production threshold the spectral shape is very different, a fact that has been overlooked in past literature. This loophole may have important phenomenological consequences, since it generically alters the BBN bounds on non-thermal relics: for instance it allows to re-open the possibility of purely electromagnetic solutions to the so-called "cosmological lithium problem", which were thought to be excluded by other cosmological constraints. We show this with a proof-of-principle example and a simple particle physics model, compared with previous literature.

  17. A loophole to the universal photon spectrum in electromagnetic cascades: application to the "cosmological lithium problem"

    E-Print Network [OSTI]

    Vivian Poulin; Pasquale D. Serpico

    2015-03-04T23:59:59.000Z

    The standard theory of electromagnetic cascades onto a photon background predicts a quasi-universal shape for the resulting non-thermal photon spectrum. This has been applied to very disparate fields, including non-thermal big bang nucleosynthesis (BBN). However, once the energy of the injected photons falls below the pair-production threshold the spectral shape is very different, a fact that has been overlooked in past literature. This loophole may have important phenomenological consequences, since it generically alters the BBN bounds on non-thermal relics: for instance it allows to re-open the possibility of purely electromagnetic solutions to the so-called "cosmological lithium problem", which were thought to be excluded by other cosmological constraints. We show this with a proof-of-principle example and a simple particle physics model, compared with previous literature.

  18. Online Training Now Available -We are proud to offer EPA Accredited Lead-Safe Work Practices training online, which can take the place of the 6 hour classroom

    E-Print Network [OSTI]

    Tennessee, University of

    Online Training Now Available - We are proud to offer EPA Accredited Lead-Safe Work Practices training online, which can take the place of the 6 hour classroom instruction for the Lead RRP certification. Please note that a two hour hands-on training session is still required before you can obtain

  19. List of East Texas Forestry Vendors This list of forestry vendors that offer services in East Texas is divided into four groups

    E-Print Network [OSTI]

    Behmer, Spencer T.

    List of East Texas Forestry Vendors This list of forestry vendors that offer services in East Texas. It is provided as a service to landowners seeking assistance with forestry practices on their land. Forestland@earthlink.net www.superiorwaterfront.com MO, MW Acorn Forestry Justin Penick P. O. Box 151537 Lufkin, TX 759151537

  20. Migration: An engine for social change The movement of people into societies that offer a better way of life is a more powerful driver of cultural

    E-Print Network [OSTI]

    Richerson, Peter J.

    Migration: An engine for social change The movement of people into societies that offer a better way of life is a more powerful driver of cultural evolution than conflict and conquest, say Peter effect on how societies evolve cul- turally because it is selective. People move to societies

  1. The Area of Energy, Economics and Law offers two academic credentials: the Energy Commerce degree and the Certificate in Energy. Students learn industry

    E-Print Network [OSTI]

    Westfall, Peter H.

    The Area of Energy, Economics and Law offers two academic credentials: the Energy Commerce degree and publication, our faculty bring a wealth of industry and legal experience to the classroom. AREA OF ENERGY on the importance of energy in the era of globalization." Terry McInturff, J.D. Professor of Practice; Area

  2. With its international student body, world-class faculty and strategic location at the gateway to the Pacific Rim, the USC Marshall School of Business offers an

    E-Print Network [OSTI]

    Southern California, University of

    to the Pacific Rim, the USC Marshall School of Business offers an unparalleled, hands-on education in global, informa- tion systems, marketing, management, operations, real estate and statistics. USC Marshall fosters. Founded in 1920, USC Marshall is one of the nation's oldest and most prominent business schools. Through

  3. Rutgers Business School's Undergraduate Program in New Brunswick offers a minor in Business Administration. The goals of the Rutgers Business School minor in Business Administration are

    E-Print Network [OSTI]

    Lin, Xiaodong

    Rutgers Business School's Undergraduate Program in New Brunswick offers a minor in Business Administration. The goals of the Rutgers Business School minor in Business Administration are: · To acquire an understanding of the theories, principles, and practices in the foundations of business (accounting, finance

  4. Subject-specific Study and Examination Regulations for the advanced English language Master's Online Program "Advanced Oncology" offered by the Medical

    E-Print Network [OSTI]

    Ulm, Universität

    's Online Program "Advanced Oncology" offered by the Medical Faculty of Ulm University of 6 February 2012Subject-specific Study and Examination Regulations for the advanced English language Master At the proposal of the Medical Faculty, the Senate of Ulm University, in its meeting of 19 January 2012, adopted

  5. Environmental Sciences Career Snapshot Environmental Sciences (ES) is a joint major offered by the College of Natural Resources (B.S.) and

    E-Print Network [OSTI]

    Wildermuth, Mary C

    Environmental Sciences Career Snapshot Environmental Sciences (ES) is a joint major offered by the Environmental Sciences Program (ES): http://environmentalsciences.berkeley.edu Key Skills Develop a broad of the Environmental Sciences degree, our graduates are well prepared for a myriad of career options, ranging from

  6. Shale Webinar Series to Start September 13th The Penn State Marcellus Education Team will be offering a new monthly Shale webinar series beginning

    E-Print Network [OSTI]

    Shale Webinar Series to Start September 13th The Penn State Marcellus Education Team will be offering a new monthly Shale webinar series beginning Thursday, September 13th from 1:00 to 2:00 PM. Tom the series with an overview of trends and updates on shale development. Tom will provide an analysis of shale

  7. Nuclear Research & Consultancy Group (NRG) develops and provides sustainable nuclear technology for energy, environment, and health. NRG offers a wide range of services to energy

    E-Print Network [OSTI]

    Vuik, Kees

    of overheating of the nuclear reactor core during a severe accident, large amount of hydrogen are generatedNuclear Research & Consultancy Group (NRG) develops and provides sustainable nuclear technology for energy, environment, and health. NRG offers a wide range of services to energy utilities, government

  8. The School offers the Bachelor of Science (B.S.) and Bachelor of Arts (B.A) degrees in computer science.

    E-Print Network [OSTI]

    Thomas, Andrew

    The School offers the Bachelor of Science (B.S.) and Bachelor of Arts (B.A) degrees in computer science. Computer science is the foundation of computing and information technology. Computer scientists and services. The required course work in computer science provides the student with an understanding

  9. Retirement Guidance One-on-One Consultations As part of our comprehensive benefits program, the Texas Tech University System offers complimentary one-

    E-Print Network [OSTI]

    Rock, Chris

    . Before closing or consolidating accounts always consider all applicable fees, features, and benefits program, the Texas Tech University System offers complimentary one- on-one planning sessions with each. This is your opportunity to get answers to any questions about the Texas Tech University System's Retirement

  10. The University of Oklahoma is an equal opportunity institution. The University of Oklahoma offers a wide variety of scholarship opportunities to admitted transfer students based on criteria

    E-Print Network [OSTI]

    Oklahoma, University of

    The University of Oklahoma is an equal opportunity institution. The University of Oklahoma offersTraditions Square and the Residence Halls for this award. TOTAL AWARD AMOUNT $3,000 for Oklahoma residents $7,000 for nonresidents $1,500 for Oklahoma residents $3,500 for nonresidents $1,500 for Oklahoma residents $3

  11. Maine Maritime Academy is a co-educational, public college in Castine, Maine offering 18 degree programs in engineering, management, science and

    E-Print Network [OSTI]

    Bustamante, Fabián E.

    Maine Maritime Academy is a co-educational, public college in Castine, Maine offering 18 degree.edu. Maine Maritime Academy currently seeks to fill the following position in the Loeb-Sullivan School. Appropriate research and service are required which may include Academy Committees, Department Committees

  12. In order to contribute to the development of a human society that coexists with the natural environment, and to establish efficient clean energy systems, we offer education

    E-Print Network [OSTI]

    Takada, Shoji

    environment, and to establish efficient clean energy systems, we offer education and conduct research on the generation, conversion, control and utilization of various kinds of energy from the perspectives of science and engineering. GraduateScho ol of Energy Science, Kyoto University GraduateScho ol of Energy Science, Kyoto

  13. List of Texas Fuel Mitigation Vendors This list of fuel mitigation vendors that offer services in Texas is divided into two groups

    E-Print Network [OSTI]

    Behmer, Spencer T.

    List of Texas Fuel Mitigation Vendors This list of fuel mitigation vendors that offer services as a service to communities and landowners seeking assistance with fuel mitigation practices on their land Service Area Mu, Be, CP, Sc, Mo, FB Page 1 of 4Last updated on 10/16/2013 #12;List of Fuel Mitigation

  14. The Landscape Architecture field of study --both the two-year and three-year programs --offers the ideal context for producing tomorrow's leaders in ecological

    E-Print Network [OSTI]

    Edwards, Paul N.

    The Landscape Architecture field of study -- both the two-year and three-year programs -- offers programs, you will learn to be a designer who authentically employs ecological principles in sustainable in the program. "Our program recognizes that design must celebrate culture if it is to sustain ecological

  15. Dear Student, You have been offered a place at Trinity College Dublin for entry into a Postgraduate Programme for 2010/2011. Please find

    E-Print Network [OSTI]

    O'Mahony, Donal E.

    1 Dear Student, You have been offered a place at Trinity College Dublin for entry. This is important especially for the period between your departure from home and before you register at Trinity which have not been addressed. We look forward to meeting you when you arrive in Dublin! TRINITY COLLEGE

  16. Adopt a Book Thank you for your kind offer to Adopt a Book at the University of Stirling.Your gift will be used to

    E-Print Network [OSTI]

    Little, Tony

    Adopt a Book Thank you for your kind offer to Adopt a Book at the University of Stirling.Your gift my cheque/Charities Aid Voucher for £30.00 payable to `University of Stirling' I wish to make my different from above): Bookplates To recognise your gift, Stirling will put a dedicate bookplate into a book

  17. The DFG PhD Research Training Group 1261 "Critical Junctures of Globalization" at the Centre for Area Studies (CAS) of the University of Leipzig is offering

    E-Print Network [OSTI]

    Schüler, Axel

    The DFG PhD Research Training Group 1261 "Critical Junctures of Globalization" at the Centre for Area Studies (CAS) of the University of Leipzig is offering 9 PhD positions (65% of a TVL E 13 post April 2012 to 31 March 2014 The PhD Research Training Group, which was established in 2006, is devoted

  18. Offered: Offered: Position(s): Position(s)

    E-Print Network [OSTI]

    New Hampshire, University of

    in house. We are not an ordinary company and are always open for new opportunities and changes. That is why we can develop some fine applications that save lives, decrease the ecological footprint and increase

  19. Offered: Offered: Position(s): Position(s)

    E-Print Network [OSTI]

    New Hampshire, University of

    processes and procedures, and providing technical expertise/support to manufacturing. Additional tasks may with engineering tasks including participating in new product/process development, establishing manufacturing involvement, and product studies. www.tbvc.com Manufacturing Company Overview: Degree: Paid Fall, Spring

  20. Offered: Offered: Position(s): Position(s)

    E-Print Network [OSTI]

    New Hampshire, University of

    in Southern New England from six offices: two in Connecticut, three in Massachusetts and one in New Hampshire, energetic, enthusiastic men and women who thrive on the challenge of engineering consulting. Related

  1. Offered: Offered: Position(s): Position(s)

    E-Print Network [OSTI]

    New Hampshire, University of

    & Statistics Yes Entry LevelInternships Energy Project Intern Whittemore Center New Hampshire Office of Energy to gather comprehensive data on the ARRA-funded energy projects that OEP oversaw. A final product -- 12:00-4:00pm No The Office of Energy and Planning (OEP) is part of the Executive Department within

  2. Offered: Offered: Position(s): Position(s)

    E-Print Network [OSTI]

    New Hampshire, University of

    in Westchester, Ohio and its field sales offices located across the United States. The company operates with bleach plants, a groundwood mill, a wood processing facility, utilities, two black liquor recovery boilers, a multi fuel boiler, 95 megawatts of steam generated electrical capacity, 25 megawatts

  3. Offered: Offered: Position(s): Position(s)

    E-Print Network [OSTI]

    New Hampshire, University of

    and services that surpass expectations. The Gorton's brand in the U.S. (and the BlueWater brand in Canada

  4. Offered: Offered: Position(s): Position(s)

    E-Print Network [OSTI]

    New Hampshire, University of

    development lifecycle: High Level Avionics System Requirements/Architecture Design and Development Software Performance Software team as a Software Engineer will enable you to participate in the design and development Detailed Design/Development Software Debug/Integration Formal and Informal Software Test Development

  5. Offered: Offered: Position(s): Position(s)

    E-Print Network [OSTI]

    New Hampshire, University of

    a wide variety of car leasing, vanpooling, car sharing and hourly rental programs and local car rental -- 12:00-4:00pm Yes Entry Level Management Trainee Enterprise Rent-A-Car is a privately held company stewardship and long-term commitment to the sustainability of the car rental business. All majors Yes Entry

  6. MERRIMACK COUNTY CLUB PROJECT OFFERINGS Location Club Project Offerings

    E-Print Network [OSTI]

    New Hampshire, University of

    , Crafts, Sewing, Cooking, Shooting Sports, Woodworking, Youth Leadership Epsom Merrimack River Valley Dairy Citizenship & Government, Dairy Cattle, Youth Leadership Loudon Happy Hill Community Service

  7. Offered: Offered: Position(s): Position(s)

    E-Print Network [OSTI]

    New Hampshire, University of

    -- 12:00-4:00pm Yes Sales Consultant Trainee As a leading employee benefits provider, Unum helps protect more than 25 million working people and their families in the event of illness or injury. We show of your training. As a Sales Consultant, your compensation is based on a semi-monthly draw plus bonus

  8. Special Offer: Subscribe to the

    E-Print Network [OSTI]

    Rogers, John A.

    OF SCIENCE. Comets and asteroids made of similar stuff, a bird needs more than plumage to pick a mate AN ODD COMET For planetary scientists studying comets and asteroids, our solar system gets curiouser interstellar dust, which would open a window on the environment in which the solar system was born. Instead

  9. Donald Ostdiek Degree Offered: BA

    E-Print Network [OSTI]

    Richards-Kortum, Rebecca

    Palaeoclimate and Human Response ARCH 313 Sustainable Architecture BIOS 323 Conservation Biology BIOS 325 Ecology CEVE 201 Introduction to Environmental Systems CEVE 306 Global Environmental Law and Sustainable

  10. 9/18/09 2:07 PMSPACE.com --'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 8http://www.space.com/scienceastronomy/090817-dark-energy-alternative.html

    E-Print Network [OSTI]

    Temple, Blake

    9/18/09 2:07 PMSPACE.com -- 'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 8http://www.space.com/scienceastronomy/090817-dark-energy-alternative.html What is Dark Energy? Universe Might Be Bigger and Older Than Expected In New? Register: Join Now! 'Big Wave' Theory Offers Alternative to Dark Energy By Clara Moskowitz Staff

  11. 8/24/09 11:48 AMSPACE.com --'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 10http://www.space.com/scienceastronomy/090817-dark-energy-alternative.html#comments

    E-Print Network [OSTI]

    Temple, Blake

    8/24/09 11:48 AMSPACE.com -- 'Big Wave' Theory Offers Alternative to Dark Energy Page 1 of 10http://www.space.com/scienceastronomy/090817-dark-energy-alternative.html#comments What is Dark Energy? Universe Might Be Bigger and Older Than In New? Register: Join Now! 'Big Wave' Theory Offers Alternative to Dark Energy By Clara Moskowitz Staff

  12. Formation of super-heavy elements in astrophysical nucleosynthesis

    SciTech Connect (OSTI)

    Zagrebaev, V. I.; Karpov, A. V.; Mishustin, I. N.; Greiner, Walter [Flerov Laboratory of Nuclear Reactions, JINR, Dubna, Moscow Region (Russian Federation); Frankfurt Institute for Advanced Studies, J.W. Goethe-Universitaet, Frankfurt (Germany)

    2012-10-20T23:59:59.000Z

    The unexplored area of heavy neutron-rich nuclides is extremely important for the understanding of the r process of astrophysical nucleogenesis. For elements with Z>100 only neutron deficient isotopes (located to the left of the stability line) have been synthesized so far. The 'north-east' area of the nuclear map can be reached neither in fusion reactions nor in fragmentation processes. Low energy multi-nucleon transfer reactions are quite promising for the production and study of neutron-rich heavy nuclei including those located at the superheavy (SH) island of stability [1]. The neutron capture process is considered here as an alternative method for the production of SH nuclei. Requirements for the pulsed reactors of the next generation that could be used for the synthesis of long-living neutron rich SH nuclei are formulated. Formation of SH nuclei in supernova explosions is also discussed and the abundance of SH elements in nature is estimated.

  13. Experimental techniques to investigate the p process of nucleosynthesis

    E-Print Network [OSTI]

    Zilges, Andreas

    ) 127 #12;Activation measurement HPG Decay of 147,149Nd HPGe detector activated -: 147Nd147Pm -: 149Nd149Pm Shielding activated target : 149Nd149Pm Nd ­ X-rays Energy [keV] Reaction Yield: d

  14. Neutrinos and Nucleosynthesis in Gamma-Ray Burst Accretion Disks

    E-Print Network [OSTI]

    R. Surman; G. C. McLaughlin

    2003-11-24T23:59:59.000Z

    We calculate the nuclear composition of matter in accretion disks surrounding stellar mass black holes as are thought to accompany gamma-ray bursts (GRBs). We follow a mass element in the accretion disk starting at the point of nuclear dissociation and calculate the evolution of the electron fraction due to electron, positron, electron neutrino and electron antineutrino captures. We find that the neutronization of the disk material by electron capture can be reversed by neutrino interactions in the inner regions of disks with accretion rates of 1 M_solar/s and higher. For these cases the inner disk regions are optically thick to neutrinos, and so to estimate the emitted neutrino fluxes we find the surface of last scattering for the neutrinos (the equivalent of the proto-neutron star neutrinosphere) for each optically thick disk model. We also estimate the influence of neutrino interactions on the neutron-to-proton ratio in outflows from GRB accretion disks, and find it can be significant even when the disk is optically thin to neutrinos.

  15. Constraints on Supersymmetric Models from Catalytic Primordial Nucleosynthesis of Beryllium

    E-Print Network [OSTI]

    Maxim Pospelov; Josef Pradler; Frank Daniel Steffen

    2008-10-27T23:59:59.000Z

    The catalysis of nuclear reactions by negatively charged relics leads to increased outputs of primordial ^6Li and ^9Be. In combination with observational constraints on the primordial fractions of ^6Li and ^9Be, this imposes strong restrictions on the primordial abundance and the lifetime of charged relics. We analyze the constraints from the catalysis of ^9Be on supersymmetric models in which the gravitino is the lightest supersymmetric particle and a charged slepton--such as the lighter stau--the next-to-lightest supersymmetric particle (NLSP). Barring the special cases in which the primordial fraction of the slepton NLSP is significantly depleted, we find that the ^9Be data require a slepton NLSP lifetime of less than 6x10^3 seconds. We also address the issue of the catalytic destruction of ^6Li and ^9Be by late forming bound states of protons with negatively charged relics finding that it does not lead to any significant modification of the limit on the slepton lifetime.

  16. Nucleosynthesis in type Ia supernovae driven by asymmetric thermonuclear ignition

    SciTech Connect (OSTI)

    Maeda, Keiichi [Institute for the Physics and Mathematics of the Universe (IPMU), Todai Institutes for Advanced Study (TODIAS), University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583 (Japan)

    2012-11-12T23:59:59.000Z

    Type Ia Supernovae (SNe Ia) are believed to be thermonuclear explosions of a white dwarf. They can be used as mature cosmological standardized candles, leading to the discovery of the accelerating expansion of the Universe. However, the explosion mechanism has not yet been fully clarified. In this paper, we first present nucleosynthetic features of a leading explosion scenario, namely a delayed-detonation scenario. Based on this, we propose a new and strong observational constraint on the explosion mechanism through emission lines from neutron-rich Fe-peaks. Especially, we show that an asymmetry in the explosion is likely a generic feature. We further argue that the diversity arising from various viewing angles can be an origin of observational diversities of SNe Ia seen in their spectral features (suspected possible biases in cosmology) and colors (related to the extinction estimate in cosmology). Using these new insights could open up a possibility of using SNe Ia as more precise distance indicators than currently employed.

  17. The Faculty of Fine Arts understands the integral role of new technologies in today's society and offers instruction that focuses on the creative and technical aspects of New Media in an artistic and

    E-Print Network [OSTI]

    Seldin, Jonathan P.

    and offers instruction that focuses on the creative and technical aspects of New Media in an artistic and critical milieu. The Bachelor of Fine Arts (New Media) (formerly Multimedia) provides an environment where stu- dents develop an understanding of the diverse aspects of New Media, and the skills to create art

  18. MECHANICAL ENGINEERING at PORTLAND STATE UNIVERSITYMECHANICAL ENGINEERING at PORTLAND STATE UNIVERSITY The Mechanical and Materials Engineering Department at Portland State University offers a Bachelor of Science in Mechanical Engineering (BSME).

    E-Print Network [OSTI]

    Bertini, Robert L.

    UNIVERSITY The Mechanical and Materials Engineering Department at Portland State University offers a Bachelor of Science in Mechanical Engineering (BSME). Our undergraduate program is accredited by ABET and is focused on Mechanical Engineering design with application in the thermal and fluid sciences and in machinery

  19. The Department of Communication at the University of Delaware offers a strong theory and research-based program coupled with skills training in oral communication, video production, broadcast journalism, and public

    E-Print Network [OSTI]

    Firestone, Jeremy

    The Department of Communication at the University of Delaware offers a strong theory and research-based program coupled with skills training in oral communication, video production, broadcast journalism, and public relations. Students also study intercultural communication, principles in advertising, media

  20. Health Insurance Options for Part-Time Faculty/Staff/Adjunct Faculty and Dependents While the Commonwealth of Virginia and George Mason University do not formally offer health insurance to

    E-Print Network [OSTI]

    Health Insurance Options for Part-Time Faculty/Staff/Adjunct Faculty and Dependents While the Commonwealth of Virginia and George Mason University do not formally offer health insurance to part-time employees, health insurance options do exist for employees and their dependents who wish to purchase

  1. UKAEA Discounts is available on-line to all employees of UKAEA. UKAEA Discounts is a free to use benefit, paid for by UKAEA, and offers numerous opportunities to regularly save

    E-Print Network [OSTI]

    benefit, paid for by UKAEA, and offers numerous opportunities to regularly save money on normal everyday shopping. It has the potential to save you many £10s or even £100s per year. The 3 main ways of saving using UKAEA Discounts are: Re-loadable gift cards Re-loadable gift cards typically save you between 5

  2. The role of DCU Sport Heart Smart in Civic Engagement Overall, the strength of DCU Sport's commitment to civic engagement lies in the diversity of programmes on offer to the community.

    E-Print Network [OSTI]

    Humphrys, Mark

    The role of DCU Sport Heart Smart in Civic Engagement Overall, the strength of DCU Sport's commitment to civic engagement lies in the diversity of programmes on offer to the community. Heart Smart most vulnerable. The fact that three of the biggest hospitals in Dublin view Heart Smart

  3. The UN Standing Committee on Nutrition (UNSCN) offers a new internship position. Are you interested in experiencing nutrition at a global level while working in Geneva with a dynamic

    E-Print Network [OSTI]

    Mullins, Dyche

    The UN Standing Committee on Nutrition (UNSCN) offers a new internship position. Are you interested in experiencing nutrition at a global level while working in Geneva with a dynamic and international team related field) who is seeking work experience within the UN system. The main focus of this internship

  4. Thermal Distributions, Saha Equation, Weak Interactions This chapter deals with some background issues important to modeling the BBN as well as

    E-Print Network [OSTI]

    Washington at Seattle, University of - Department of Physics, Electroweak Interaction Research Group

    Chapter 3 Thermal Distributions, Saha Equation, Weak Interactions This chapter deals with some · the Saha equation · low-energy weak interactions 3.1 Thermal distributions The thermal distributions to be considered: the Saha equation discussion will il- lustrate this.) The parameter µ, the chemical potential

  5. On the Universal Generation of Mobility Models Alberto Medina

    E-Print Network [OSTI]

    On the Universal Generation of Mobility Models Alberto Medina Raytheon BBN Technologies amedina@bbn.com Gonca Gursun Computer Science Dept. Boston University goncag@cs.bu.edu Prithwish Basu Raytheon BBN

  6. Algorithms for Channel Assignment in Mobile Wireless Networks using Temporal Coloring

    E-Print Network [OSTI]

    Ramanathan, Ram

    of New York Graduate Center New York, NY, 10016, USA amotz@sci.brooklyn.cuny.edu Prithwish Basu Raytheon BBN Technologies Cambridge, MA, 02138, USA pbasu@bbn.com Ram Ramanathan Raytheon BBN Technologies

  7. Steptoe Butte Offer Clues to State's Past

    SciTech Connect (OSTI)

    Reidel, Steve P.

    2004-11-21T23:59:59.000Z

    This is a column for a Tri-City Herald column that I write called Northwest Geology. This week's column is on Steptoe Butte near Colfax

  8. Vermont Standard Offer for Qualifying SPEED Resources

    Broader source: Energy.gov [DOE]

    '''''Note: The first RFP for the new competitive award process has passed; applications were accepted through May 1, 2013. See the program web site for information regarding future solicitations. '...

  9. Research Overview The Mechanical Engineering Department offers

    E-Print Network [OSTI]

    the Colorado Fuel Cell Center at the Colorado Graduate student Jen Labs attending to laser diagnostics facility community, and industry partners. Particle-laden flame Robotic welding instrument Fuel cells from

  10. Working with JLT to offer employees

    E-Print Network [OSTI]

    University College London

    of external prosthesis ­ up to £5,000 per year. Purchase of wigs ­ up to £150 per year. Provision of external prosthesis ­ up to £5,000 per year. Purchase of wigs ­ up to £150 per year. Provision of external prosthesis ­ up to £5,000 per year. Purchase of wigs ­ up to £150 per year. Provision of external prosthesis ­ up

  11. ORIGINAL PAPER Offer Shai Yoram Reich

    E-Print Network [OSTI]

    Shai, Offer

    examples that demonstrate the details of infused design. Keywords Collaboration Æ Concurrent engineering Æ and effectively. Concurrent engineering (CE) (Prasad 1996; Reich and Subrahmanian 1992; Walton 1991) is seen, this interface has been the focal point of many studies attempting to support the concurrent work of engineers

  12. Eight National Labs Offer Streamlined Partnership Agreements...

    Broader source: Energy.gov (indexed) [DOE]

    Oak Ridge National Laboratory Pacific Northwest National Laboratory Savannah River National Laboratory DOE's laboratories have a long tradition of working with...

  13. Advanced Graduate Courses offered by the Mathematics ...

    E-Print Network [OSTI]

    1910-10-41T23:59:59.000Z

    study of the foundations of Mathematics and Computer Science. ... Logic, which in its simplicity provides a a good picture of the methods and goals of Logic. ... of partial differential equations in applied mathematics, science and engineering.

  14. My Amazing Future tour offers career options.

    ScienceCinema (OSTI)

    Idaho National Laboratory

    2010-01-08T23:59:59.000Z

    Girls from several Idaho high schools attended this event at INL where they learned about career opportunities in the science and technology fields.

  15. Experts Offer Marines Energy-Efficiency Advice

    Broader source: Energy.gov [DOE]

    As an early adopter of cutting-edge technologies, the United States military is pioneering energy efficiency and renewable energy technologies in the field. Recently, the Commandant of the United States Marine Corps sent a team to visit bases and camps in Afghanistan to assess and make recommendations on the supply and use of energy and water.

  16. Photoswitchable Nanoprobes Offer Unlimited Brightness in Frequency...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    from none frequencydependent interference or noise using photoswitchingenabled Fourier transformation (PFT). As a result, the light-modulated probes can be made super...

  17. Peptoid Nanosheets Offer a Diversity of Functionalities

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    field. Just as the properties of peptoids can be chemically customized through robotic synthesis, the properties of peptoid nanosheets can also be engineered for specific...

  18. Underbalanced drilling with air offers many pluses

    SciTech Connect (OSTI)

    Shale, L. [Baker Hughes Inteq, Houston, TX (United States)

    1995-06-26T23:59:59.000Z

    A pressure overbalance during conventional drilling can cause significant fluid filtrate invasion and lost circulation. Fluid invasion into the formation can lead to formation damage, high mud costs, a need for expensive completions, and well productivity impairment. Because underbalanced drilling creates a natural tendency for fluid and gas to flow from the formation to the borehole, successful underbalanced drilling depends upon the appropriate selection of circulating fluid. The use of a compressible fluid in the circulating system, referred to as air drilling, lowers the downhole pressure, allowing drilling into and beyond these sensitive formations. The paper discusses the equipment needed; well control; downhole air requirements; air drilling techniques using dry air, air-mist, stable foam, stiff foam, and aerated-fluid; downhole fires; directional air drilling; and well completions.

  19. Upton bill offers clean-up incentives

    SciTech Connect (OSTI)

    Black, B. [Weinberg & Green, Baltimore, MD (United States)

    1994-07-01T23:59:59.000Z

    Like castor oil, the Superfund law can be difficult medicine to swallow, and no one wants to volunteer for a dose. Indeed, the law`s harsh and unbending liability scheme sometimes hinders the cleanup of contaminated property. Confronted with the choice of redeveloping an old {open_quotes}brownfield{close_quotes} urban industrial site or building at a pristine new {open_quotes}greenfield{close_quotes} location, most companies opt for the latter. The brownfield problem is especially troubling because the law often prevents voluntary cleanups at relatively low priority sites that usually don`t get caught up in the Superfund program. This paper describes the Upton Bill which would require the US EPA to establish cleanup standards for hazrdous substances, allow for public comment on a proposed response plan, and require a voluntary party to submit detailed annual reports and maintain records.

  20. ERASMUS Placement Offer Form EMPLOYER INFORMATION

    E-Print Network [OSTI]

    Herrmann, Samuel

    ) Humanities and Arts Arts Arts (broad programmes) Fine arts Music and performing arts Audio-visual techniques) Wholesale and retail sales Marketing and advertising Finance, banking, insurance Accounting and taxation work Electricity and energy Electronics and automation Chemical and process Motor vehicles, ships

  1. Peptoid Nanosheets Offer a Diversity of Functionalities

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What's Possible for RenewableSpeedingBiomassPPPO WebsitePalms Village95-1999)PaulPeer

  2. Peptoid Nanosheets Offer a Diversity of Functionalities

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What's Possible for RenewableSpeedingBiomassPPPO WebsitePalms Village95-1999)PaulPeerPeptoid Nanosheets

  3. Peptoid Nanosheets Offer a Diversity of Functionalities

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What's Possible for RenewableSpeedingBiomassPPPO WebsitePalms Village95-1999)PaulPeerPeptoid

  4. Peptoid Nanosheets Offer a Diversity of Functionalities

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What's Possible for RenewableSpeedingBiomassPPPO WebsitePalms Village95-1999)PaulPeerPeptoidPeptoid

  5. Peptoid Nanosheets Offer a Diversity of Functionalities

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC)IntegratedSpeeding access

  6. Fermilab | Newsroom | Press Releases | National laboratories offer

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOEThe Bonneville Power AdministrationField8,Dist.New Mexico Feb. 13, 2013Focus GroupDownreport

  7. Solicitation, Offer and Award (SF-33)

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels DataDepartment of Energy Your Density Isn'tOriginEducationVideo »UsageSecretary ofSmallConfidential,2Cycle SelectionDepartment

  8. Optical Furnace offers improved semiconductor device processing

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What's Possible for RenewableSpeeding accessSpeedingOctoberResearchOpen→and

  9. High energy cosmic rays experiments inspired by noncommutative quantum field theory

    E-Print Network [OSTI]

    Josip Trampetic

    2012-10-19T23:59:59.000Z

    Phenomenological analysis of the covariant theta-exact noncommutative (NC) gauge field theory (GFT), inspired by high energy cosmic rays experiments, is performed in the framework of the inelastic neutrino-nucleon scatterings, plasmon and $Z$-boson decays into neutrino pair, the Big Bang Nucleosynthesis (BBN) and the Reheating Phase After Inflation (RPAI), respectively. Next we have have found neutrino two-point function and shows a closed form decoupling of the hard ultraviolet (UV) divergent term from softened ultraviolet/infrared (UV/IR) mixing term and from the finite terms as well. For a certain choice of the noncommutative parameter theta which preserves unitarity, problematic UV divergent and UV/IR mixing terms vanish. Non-perturbative modifications of the neutrino dispersion relations are assymptotically independent of the scale of noncommutativity in both the low and high energy limits and may allow superluminal propagation.

  10. Sterile Neutrinos with Secret Interactions - Lasting Friendship with Cosmology

    E-Print Network [OSTI]

    Chu, Xiaoyong; Kopp, Joachim

    2015-01-01T23:59:59.000Z

    Sterile neutrinos with mass ~1 eV and order 10% mixing with active neutrinos have been proposed as a solution to anomalies in neutrino oscillation data, but are tightly constrained by cosmological limits. It was recently shown that these constraints are avoided if sterile neutrinos couple to a new MeV-scale gauge boson A'. However, even this scenario is restricted by structure formation constraints when A'-mediated collisional processes lead to efficient active-to-sterile neutrino conversion after neutrinos have decoupled. In view of this, we reevaluate in this paper the viability of sterile neutrinos with such "secret" interactions. We carefully dissect their evolution in the early Universe, including the various production channels and the expected modifications to large scale structure formation. We argue that there are two regions in parameter space - one at very small A' coupling, one at relatively large A' coupling - where all constraints from big bang nucleosynthesis (BBN), cosmic microwave background ...

  11. Grit Denker, Ph.D. SRI International

    E-Print Network [OSTI]

    Denker, Grit

    and countermeasures of cognitive radios. PI of subcontract to Raytheon BBN Technologies architecture for MANET clusters in space applications designed by Raytheon BBN. PI

  12. Cosmic Minivoids in the Intergalactic Medium

    E-Print Network [OSTI]

    Avery Meiksin

    1996-11-01T23:59:59.000Z

    The Gunn-Peterson effect, absorption of Lya photons by a homogeneous component of the intergalactic medium (IGM), potentially provides a test of Big Bang Nucleosynthesis (BBN). With a lower limit on the UV radiation field estimated from the contribution due to QSOs, a measurement of the Lya opacity of the intergalactic medium would permit the derivation of a lower bound to the baryonic density of the universe. The effect, however, has continually eluded a convincing detection, both in HI and HeII, despite extensive searches. Recent cosmological hydrodynamical simulations of structure formation in the intergalactic medium suggest an explanation for its absence. In a Cold Dark Matter dominated cosmology, the fragmentation of the baryons is nearly complete, leaving a negligible remnant to comprise a smoothly distributed component. The fragmentation extends even into regions that are underdense, where it gives rise to most of the optically thin HI systems and nearly all of the HeII systems, both thin and saturated. The result is a Lya opacity from a smooth IGM that is suppressed by over two orders of magnitude from the BBN value.

  13. Sinks of Light Elements in Stars - Part II

    E-Print Network [OSTI]

    Marc H. Pinsonneault; Corinne Charbonnel; Constantine P. Deliyannis

    2000-06-20T23:59:59.000Z

    The fragile light elements lithium, beryllium, and boron are easily destroyed in stellar interiors, and are thus superb probes of physical processes occuring in the outer stellar layers. The light elements are also excellent tracers of the chemical evolution of the Galaxy, and can test big bang nucleosynthesis (BBN). These inter-related topics are reviewed with an emphasis on stellar physics. In Part I (presented by CPD), an overview is given of the physical processes which can modify the surface abundances of the light elements, with emphasis on Population I dwarfs - convection; gravitational settling, thermal diffusion, and radiative levitation; slow mixing induced by gravity waves or rotation. We will discuss the increasingly large body of data which begin to enable us to discern the relative importance of these mechanisms in Population I main sequence stars. In Part II (presented by MHP), discussion is extended to the issue of whether or not the halo Li plateau is depleted, and includes the following topics: Li dispersion in field and globular cluster stars, Li production vs. destruction in Li-rich halo stars, and constraints from 6Li. Also discussed are trends with metal abundance and Teff and implications for chemical evolution and BBN. In Part III (presented by CC), evidence is reviewed that suggests that in situ mixing occurs in evolved low mass Population I and Population II stars. Theoretical mechanisms that can create such mixing are discussed, as well as their implications in stellar yields.

  14. Sinks of Light Elements in Stars - Part III

    E-Print Network [OSTI]

    Corinne Charbonnel; Constantine P. Deliyannis; Marc H. Pinsonneault

    2000-06-20T23:59:59.000Z

    The fragile light elements lithium, beryllium, and boron are easily destroyed in stellar interiors, and are thus superb probes of physical processes occuring in the outer stellar layers. The light elements are also excellent tracers of the chemical evolution of the Galaxy, and can test big bang nucleosynthesis (BBN). These inter-related topics are reviewed with an emphasis on stellar physics. In Part I (presented by CPD), an overview is given of the physical processes which can modify the surface abundances of the light elements, with emphasis on Population I dwarfs - convection; gravitational settling, thermal diffusion, and radiative levitation; slow mixing induced by gravity waves or rotation. We will discuss the increasingly large body of data which begin to enable us to discern the relative importance of these mechanisms in Population I main sequence stars. In Part II (presented by MHP), discussion is extended to the issue of whether or not the halo Li plateau is depleted, and includes the following topics: Li dispersion in field and globular cluster stars, Li production vs. destruction in Li-rich halo stars, and constraints from 6Li. Also discussed are trends with metal abundance and Teff and implications for chemical evolution and BBN. In Part III (presented by CC), evidence is reviewed that suggests that in situ mixing occurs in evolved low mass Population I and Population II stars. Theoretical mechanisms that can create such mixing are discussed, as well as their implications in stellar yields.

  15. The Primordial Lithium Problem

    E-Print Network [OSTI]

    Brian D. Fields

    2012-03-15T23:59:59.000Z

    Big-bang nucleosynthesis (BBN) theory, together with the precise WMAP cosmic baryon density, makes tight predictions for the abundances of the lightest elements. Deuterium and 4He measurements agree well with expectations, but 7Li observations lie a factor 3-4 below the BBN+WMAP prediction. This 4-5\\sigma\\ mismatch constitutes the cosmic "lithium problem," with disparate solutions possible. (1) Astrophysical systematics in the observations could exist but are increasingly constrained. (2) Nuclear physics experiments provide a wealth of well-measured cross-section data, but 7Be destruction could be enhanced by unknown or poorly-measured resonances, such as 7Be + 3He -> 10C^* -> p + 9B. (3) Physics beyond the Standard Model can alter the 7Li abundance, though D and 4He must remain unperturbed; we discuss such scenarios, highlighting decaying Supersymmetric particles and time-varying fundamental constants. Present and planned experiments could reveal which (if any) of these is the solution to the problem.

  16. Cosmological and supernova neutrinos

    SciTech Connect (OSTI)

    Kajino, T. [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan Department of Astronomy, University of Tokyo, Hongo 7-3-1, Bunkyo-ku, Tokyo 113-0033 (Japan); Aoki, W. [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Balantekin, A. B. [Department of Physics, University of Wisconsin - Madison, Wisconsin 53706 (United States); Cheoun, M.-K. [Department of Physics, Soongsil University, Seoul 156-743 (Korea, Republic of); Hayakawa, T. [Japan Atomic Energy Agency, Shirakara-Shirane 2-4, Tokai-mura, Ibaraki 319-1195 (Japan); Hidaka, J. [National Astronomical Observatory, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Hirai, Y.; Shibagaki, S. [National Astronomical Observatory, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan and Department of Astronomy, University of Tokyo, Hongo 7-3-1, Bunkyo-ku, Tokyo 113-0033 (Japan); Kusakabe, M. [School of Liberal Arts and Science, Korea Aerospace University, Goyang 412-791 (Korea, Republic of); Mathews, G. J. [Department of Physics, University of Notre Dame, IN 46556 (United States); Nakamura, K. [Waseda University, Ohkubo 3-4-1, Shinjuku, Tokyo 169-8555 (Japan); Pehlivan, Y. [Mimar Sinan GSÜ, Department of Physics, ?i?li, ?stanbul 34380 (Turkey); Suzuki, T. [Nihon University, Sakurajosui 3-25-40, Setagaya-ku, Tokyo 156-8550 (Japan)

    2014-06-24T23:59:59.000Z

    The Big Bang nucleosynthesis (BBN) and the cosmic microwave background (CMB) anisotropies are the pillars of modern cosmology. It has recently been suggested that axion which is a dark matter candidate in the framework of the standard model could condensate in the early universe and induce photon cooling before the epoch of the photon last scattering. Although this may render a solution to the overproduction problem of primordial {sup 7}Li abundance, there arises another serious difficulty of overproducing D abundance. We propose a hybrid dark matter model with both axions and relic supersymmetric (SUSY) particles to solve both overproduction problems of the primordial D and {sup 7}Li abundances simultaneously. The BBN also serves to constrain the nature of neutrinos. Considering non-thermal photons produced in the decay of the heavy sterile neutrinos due to the magnetic moment, we explore the cosmological constraint on the strength of neutrino magnetic moment consistent with the observed light element abundances. Core-collapse supernovae eject huge flux of energetic neutrinos which affect explosive nucleosynthesis of rare isotopes like {sup 7}Li, {sup 11}B, {sup 92}Nb, {sup 138}La and {sup 180}Ta and r-process elements. Several isotopes depend strongly on the neutrino flavor oscillation due to the Mikheyev-Smirnov-Wolfenstein (MSW) effect. Combining the recent experimental constraints on ?{sub 13} with predicted and observed supernova-produced abundance ratio {sup 11}B/{sup 7}Li encapsulated in the presolar grains from the Murchison meteorite, we show a marginal preference for an inverted neutrino mass hierarchy. We also discuss supernova relic neutrinos (SRN) that may indicate the softness of the equation of state (EoS) of nuclear matter and adiabatic conditions of the neutrino oscillation.

  17. The directory of United States coal & technology export resources. Profiles of domestic US corporations, associations and public entities, nationwide, which offer products or services suitable for export, relating to coal and its utilization

    SciTech Connect (OSTI)

    Not Available

    1994-01-01T23:59:59.000Z

    The purpose of this directory is to provide a listing of available U.S. coal and coal related resources to potential purchasers of those resources abroad. The directory lists business entities within the US which offer coal related resources, products and services for sale on the international market. Each listing is intended to describe the particular business niche or range of product and/or services offered by a particular company. The listing provides addresses, telephones, and telex/fax for key staff in each company committed to the facilitation of international trade. The content of each listing has been formulated especially for this directory and reflects data current as of the date of this edition. The directory listings are divided into four primary classifications: coal resources; technology resources; support services; and financing and resource packaging. The first three of which are subdivided as follows: Coal Resources -- coal derivatives, coal exporters, and coal mining; Technology Resources -- advanced utilization, architects and engineers, boiler equipment, emissions control and waste disposal systems, facility construction, mining equipment, power generation systems, technical publications, and transport equipment; Support Services -- coal transport, facility operations, freight forwarders, sampling services and equipment, and technical consultants. Listings for the directory were solicited on the basis of this industry breakdown. Each of the four sections of this directory begins with a matrix illustrating which companies fall within the particular subclassifications specific to that main classification. A general alphabetical index of companies and an index by product/service classification are provided following the last section of the directory.

  18. bu.edu/eng4 ACCESS DENIED

    E-Print Network [OSTI]

    , Deutsche Telekom and Raytheon BBN Technologies; and one academic partner, Warwick University. The ECE

  19. Please Note: The Speaking Test--$80. This test will ONLY be offered to those who are successful on the General Test. The Speaking Test is held two weeks after the dates listed above. You will be notified if you are eligible.

    E-Print Network [OSTI]

    Saskatchewan, University of

    CanTEST Please Note: The Speaking Test--$80. This test will ONLY be offered to those who are successful on the General Test. The Speaking Test is held two weeks after the dates listed above. You: ____________________________________ Have you ever taken the CanTEST? q No q Yes If yes, date of test: I request that an official score

  20. It is a unique programme of its kind not only in this country but also in the whole of South East Asian region. Besides offering M.Tech and Ph.D degrees in the area of Nuclear Engineering & Technology, the programme provides research and development exper

    E-Print Network [OSTI]

    Srivastava, Kumar Vaibhav

    Asian region. Besides offering M.Tech and Ph.D degrees in the area of Nuclear Engineering & TechnologyDepartmentofAtomicEnergy. Contact Head Nuclear Engineering & Technology Programme Indian Institute of Technology Kanpur Kanpur - 208.iitk.ac.in/net/ Nuclear Engineering & Technology Programme IITK Indian Institute of Technology Kanpur 3D Tomographic

  1. [Environmental Hazards Assessment Program annual report, June 1992--June 1993]. Proposal for a new program leading to the Master of Science degree in environmental studies to be offered jointly by the Medical University of South Carolina and the University of Charleston, South Carolina

    SciTech Connect (OSTI)

    Not Available

    1993-12-01T23:59:59.000Z

    The Medical University of South Carolina (MUSC) and the University of Charleston, South Carolina (UCSC) propose to offer the degree of Master of Science in Environmental Studies. The proposed starting date is August 1994. The purpose of this interdisciplinary program is to offer nationally and internationally recognized graduate level training in the areas of environmental policy, science, and health risk assessment. Special emphasis will be placed on human health. Included in this proposal are a needs assessment for environmental science professionals along with employment projections and salary expectations. The Environmental Science program is described and its relationship to other programs within MUSC and UCSC, as well as its relation to similar programs at other institutions are examined. Enrollment is discussed, admission requirements and standards outlined, and the curriculum is described. Academic and physical resources are examined and estimated costs are given.

  2. Heavy sterile neutrinos, entropy and relativistic energy production, and the relic neutrino background

    E-Print Network [OSTI]

    George M. Fuller; Chad T. Kishimoto; Alexander Kusenko

    2011-10-28T23:59:59.000Z

    We explore the implications of the existence of heavy neutral fermions (i.e., sterile neutrinos) for the thermal history of the early universe. In particular, we consider sterile neutrinos with rest masses in the 100 MeV to 500 MeV range, with couplings to ordinary active neutrinos large enough to guarantee thermal and chemical equilibrium at epochs in the early universe with temperatures T > 1 GeV, but in a range to give decay lifetimes from seconds to minutes. Such neutrinos would decouple early, with relic densities comparable to those of photons, but decay out of equilibrium, with consequent prodigious entropy generation prior to, or during, Big Bang Nucleosynthesis (BBN). Most of the ranges of sterile neutrino rest mass and lifetime considered are at odds with Cosmic Microwave Background (CMB) limits on the relativistic particle contribution to energy density (e.g., as parameterized by N_eff). However, some sterile neutrino parameters can lead to an acceptable N_eff. These parameter ranges are accompanied by considerable dilution of the ordinary background relic neutrinos, possibly an adverse effect on BBN, but sometimes fall in a range which can explain measured neutrino masses in some particle physics models. A robust signature of these sterile neutrinos would be a measured N_eff not equal to 3 coupled with no cosmological signal for neutrino rest mass when the detection thresholds for these probes are below laboratory-established neutrino mass values, either as established by the atmospheric neutrino oscillation scale or direct measurements with, e.g., KATRIN or neutrino-less double beta decay experiments.

  3. Reconciling thermal leptogenesis with the gravitino problem in SUSY models with mixed axion/axino dark matter

    SciTech Connect (OSTI)

    Baer, Howard; Lessa, Andre [Dept. of Physics and Astronomy, University of Oklahoma, 440 West Brooks, Norman, OK 73019 (United States); Kraml, Sabine [Laboratoire de Physique Subatomique et de Cosmologie, UJF Grenoble 1, CNRS/IN2P3, INPG, 53 Avenue des Martyrs, F-38026 Grenoble (France); Sekmen, Sezen, E-mail: baer@nhn.ou.edu, E-mail: sabine.kraml@lpsc.in2p3.fr, E-mail: lessa.a.p@gmail.com, E-mail: sezen.sekmen@cern.ch [Dept. of Physics, Florida State University, 513 Keen Bldg., Tallahassee, FL 32306 (United States)

    2010-11-01T23:59:59.000Z

    Successful implementation of thermal leptogenesis requires re-heat temperatures T{sub R}?>2 × 10{sup 9} GeV, in apparent conflict with SUSY models with TeV-scale gravitinos, which require much lower T{sub R} in order to avoid Big Bang Nucleosynthesis (BBN) constraints. We show that mixed axion/axino dark matter can reconcile thermal leptogenesis with the gravitino problem in models with m{sub G-tilde}?>30 TeV, a rather high Peccei-Quinn breaking scale and an initial mis-alignment angle ?{sub i} < 1. We calculate axion and axino dark matter production from four sources, and impose BBN constraints on long-lived gravitinos and neutralinos. Moreover, we discuss several SUSY models which naturally have gravitino masses of the order of tens of TeV. We find a reconciliation difficult in Yukawa-unified SUSY and in AMSB with a wino-like lightest neutralino. However, T{sub R} ? 10{sup 10}?10{sup 12} GeV can easily be achieved in effective SUSY and in models based on mixed moduli-anomaly mediation. Consequences of this scenario include: 1. an LHC SUSY discovery should be consistent with SUSY models with a large gravitino mass, 2. an apparent neutralino relic abundance ?{sub Z-tilde} {sub 1}h{sup 2}?<1, 3. no WIMP direct or indirect detection signals should be found, and 4. the axion mass should be less than ? 10{sup ?6} eV, somewhat below the conventional range which is explored by microwave cavity axion detection experiments.

  4. Sterile Neutrinos and Light Dark Matter Save Each Other

    E-Print Network [OSTI]

    Chiu Man Ho; Robert J. Scherrer

    2013-03-13T23:59:59.000Z

    Short baseline neutrino experiments such as LSND and MiniBooNE seem to suggest the existence of light sterile neutrinos. Meanwhile, current cosmic microwave background (CMB) and big bang nucleosynthesis (BBN) measurements place an upper bound on the effective number of light neutrinos, $N_{eff}$ and the PLANCK satellite will measure $N_{eff}$ to a much higher accuracy and further constrain the number of sterile neutrinos allowed. We demonstrate that if an MeV dark matter particle couples more strongly to electrons and/or photons than to neutrinos, then p-wave annihilation after neutrino decoupling can reduce the value of $N_{eff}$ inferred from BBN and PLANCK. This mechanism can accommodate two eV sterile neutrinos even if PLANCK observes $N_{eff}$ as low as the standard model theoretical value of 3.046, and a large neutrino asymmetry is not needed to obtain the correct primordial element abundances. The dark matter annihilation also weakens the cosmological upper bounds on the neutrino masses, and we derive a relationship between the change in these bounds and the corresponding change in $N_{eff}$. Dark matter with an electric dipole moment or anapole moment is a natural candidate that exhibits the desired properties for this mechanism. Coincidentally, a dark matter particle with these properties and lighter than 3 MeV is precisely one that can explain the 511 keV gamma-ray line observed by INTEGRAL. We show that the addition of two eV sterile neutrinos allows this kind of dark matter to be lighter than 3 MeV, which is otherwise ruled out by the CMB bound on $N_{eff}$ if only active neutrinos are considered.

  5. Study of {sup 24}Mg resonances relevant for carbon burning nucleosynthesis

    SciTech Connect (OSTI)

    Toki?, V.; Soi?, N.; Blagus, S.; Fazini?, S.; Jelavi?-Malenica, D.; Miljani?, D.; Prepolec, L.; Skukan, N.; Szilner, S.; Uroi?, M. [Ru?er Boškovi? Institute, Bijeni?ka cesta 54, 10000 Zagreb (Croatia); Milin, M. [Faculty of Science, University of Zagreb, Bijeni?ka cesta 32, 10000 Zagreb (Croatia); Di Pietro, A.; Figuera, P.; Fisichella, M.; Lattuada, M.; Scuderi, V.; Strano, E.; Torresi, D. [INFN-Laboratori Nazionali del Sud, via S.Sofia 62, 95125 Catania (Italy); Freer, M.; Ziman, V. [School of Physics and Astronomy, University of Birmingham, Birmingham B15 2TT (United Kingdom); and others

    2014-05-09T23:59:59.000Z

    We have studied decays of resonances in {sup 24}Mg at excitation energies above the {sup 12}C+{sup 12}C decay threshold, using {sup 12}C({sup 16}O,?){sup 24}Mg* reaction. This experiment has been performed at INFNLNS, using Tandem accelerator beam of 16O at E = 94 MeV. Some preliminary results are presented.

  6. NUCLEOSYNTHESIS IN INTERMEDIATE MASS STARS JOHN C. LATTANZIO AND CHERYL A. FROST

    E-Print Network [OSTI]

    Lattanzio, John

    are primarily taken from the data base of Thielemann et al (1987). There are some notable exceptions. (All masses given are in units of M fi .) 2.1. CORE HYDROGEN BURNING AND FIRST DREDGE­UP Following core in 13 C at the cost of 12 C. The same region shows a decrease in the 15 N due to 15 N(p,ff) 12 C

  7. Nucleosynthesis of Nickel-56 from Gamma-Ray Burst Accretion Disks

    E-Print Network [OSTI]

    R. Surman; G. C. McLaughlin; N. Sabbatino

    2011-12-12T23:59:59.000Z

    We examine the prospects for producing Nickel-56 from black hole accretion disks, by examining a range of steady state disk models. We focus on relatively slowly accreting disks in the range of 0.05 - 1 solar masses per second, as are thought to be appropriate for the central engines of long-duration gamma-ray bursts. We find that significant amounts of Nickel-56 are produced over a wide range of parameter space. We discuss the influence of entropy, outflow timescale and initial disk position on mass fraction of Nickel-56 which is produced. We keep careful track of the weak interactions to ensure reliable calculations of the electron fraction, and discuss the role of the neutrinos.

  8. Possible signature of hypernova nucleosynthesis in a beryllium rich halo dwarf

    E-Print Network [OSTI]

    R. Smiljanic; L. Pasquini; F. Primas; P. Mazzali; D. Galli; G. Valle

    2008-01-07T23:59:59.000Z

    As part of a large survey of halo and thick disc stars, we found one halo star, HD 106038, exceptionally overabundant in beryllium. In spite of its low metallicity, [Fe/H] = -1.26, the star has log(Be/H) = -10.60, which is similar to the solar meteoritic abundance, log(Be/H) = -10.58. This abundance is more than ten times higher the abundance of stars with similar metallicity and cannot be explained by models of chemical evolution of the Galaxy that include the standard theory of cosmic-ray spallation. No other halo star exhibiting such a beryllium overabundance is known. In addition, overabundances of Li, Si, Ni, Y, and Ba are also observed. We suggest that all these chemical peculiarities, but the Ba abundance, can be simultaneously explained if the star was formed in the vicinity of a hypernova.

  9. Experimental study of beta-delayed proton decay of (23)Al for nucleosynthesis in novae

    E-Print Network [OSTI]

    Saastamoinen, A.; Trache, L.; Banu, A.; Bentley, M. A.; Davinson, T.; Hardy, John C.; Iacob, V. E.; McCleskey, M.; Roeder, B. T.; Simmons, E.; Tabacaru, G.; Tribble, Robert E.; Woods, P. J.; Aysto, J.

    2011-01-01T23:59:59.000Z

    The beta-delayed gamma and proton decay of (23)Al has been studied with an alternative detector setup at the focal plane of the momentum achromat recoil separator MARS at Texas AandM University. We could detect protons down to an energy of 200 ke...

  10. Neutrino-nucleus reactions and their role for supernova dynamics and nucleosynthesis

    E-Print Network [OSTI]

    Balasi, K G; Martínez-Pinedo, G

    2015-01-01T23:59:59.000Z

    The description of nuclear reactions induced by supernova neutrinos has witnessed significant progress during the recent years. At the energies and momentum transfers relevant for supernova neutrinos neutrino-nucleus cross sections are dominated by allowed transitions, however, often with non-negligible contributions from (first) forbidden transitions. For several nuclei allowed Gamow-Teller strength distributions could be derived from charge-exchange reactions and from inelastic electron scattering data. Importantly the diagonalization shell model has been proven to accurately describe these data and hence became the appropriate tool to calculate the allowed contributions to neutrino-nucleus cross sections for supernova neutrinos. Higher multipole contributions are usually calculated within the framework of the Quasiparticle Random Phase Approximation, which describes the total strength and the position of the giant resonances quite well. This manuscript reviews the recent progress achieved in calculating su...

  11. Experimental study of beta-delayed proton decay of (23)Al for nucleosynthesis in novae 

    E-Print Network [OSTI]

    Saastamoinen, A.; Trache, L.; Banu, A.; Bentley, M. A.; Davinson, T.; Hardy, John C.; Iacob, V. E.; McCleskey, M.; Roeder, B. T.; Simmons, E.; Tabacaru, G.; Tribble, Robert E.; Woods, P. J.; Aysto, J.

    2011-01-01T23:59:59.000Z

    The beta-delayed gamma and proton decay of (23)Al has been studied with an alternative detector setup at the focal plane of the momentum achromat recoil separator MARS at Texas AandM University. We could detect protons down to an energy of 200 ke...

  12. The effect of 12C + 12C rate uncertainties on the evolution and nucleosynthesis of

    E-Print Network [OSTI]

    Herwig, Falk

    Contact: M. E. Bennett, Keele University, meb@astro.keele.ac.uk Published: Bennet et al., Monthly Notices

  13. Clues on the evolution of abundance gradients and on AGB nucleosynthesis

    E-Print Network [OSTI]

    Stasinska, G; Bresolin, F; Tsamis, Yi

    2013-01-01T23:59:59.000Z

    We have obtained deep spectra of 26 planetary nebulae (PNe) and 9 compact HII regions in the nearby spiral galaxy NGC 300, and analyzed them together with those of the giant HII regions previously observed. We have determined the physical properties of all these objects and their He, N, O, Ne, S and Ar abundances in a consistent way. We find that, globally, compact HII regions have abundance ratios similar to those of giant HII regions, while PNe have systematically larger N/O ratios and similar Ne/O and Ar/O ratios. We demonstrate that the nitrogen enhancement in PNe cannot be only due to second dredge-up in the progenitor stars, since their initial masses are around 2--2.5\\,\\msun. An extra mixing process is required, perhaps driven by stellar rotation. Concerning the radial abundance distribution, PNe behave differently from HII regions: in the central part of the galaxy their average O/H abundance ratio is 0.15 dex smaller. Their abundance dispersion at any galactocentric radius is significantly larger tha...

  14. Nucleosynthesis at the proton drip line a challenge for nuclear physics

    E-Print Network [OSTI]

    Rauscher, Thomas

    are thermonuclear flashes on the surface of accreting neutron stars [1--3] (see also the review article [4 in a thermonuclear runaway. Helium is burned via the 3ff­reaction and the ffp­process (a sequence of (ff,p) and (p fuel to power the second burst and can therefore not be explained by the simple #12; thermonuclear

  15. Unveiling secret interactions among sterile neutrinos with big-bang nucleosynthesis

    E-Print Network [OSTI]

    Ninetta Saviano; Ofelia Pisanti; Gianpiero Mangano; Alessandro Mirizzi

    2014-11-15T23:59:59.000Z

    Short-baseline neutrino anomalies suggest the existence of low-mass ( m \\sim O(1)~eV) sterile neutrinos \

  16. Big-bang nucleosynthesis with a long-lived CHAMP including He4 spallation process

    E-Print Network [OSTI]

    Toshifumi Jittoh; Kazunori Kohri; Masafumi Koike; Joe Sato; Kenichi Sugai; Masato Yamanaka; Koichi Yazaki

    2012-09-10T23:59:59.000Z

    We propose helium-4 spallation processes induced by long-lived stau in supersymmetric standard models, and investigate an impact of the processes on light elements abundances. We show that, as long as the phase space of helium-4 spallation processes is open, they are more important than stau-catalyzed fusion and hence constrain the stau property. This talk is based on works (Jittoh et al., 2011).

  17. nu-Process Nucleosynthesis in Population III Core-Collapse Supernovae

    E-Print Network [OSTI]

    Takashi Yoshida; Hideyuki Umeda; Ken'ichi Nomoto

    2007-10-01T23:59:59.000Z

    We investigate the effects of neutrino-nucleus interactions (the nu-process) on the production of iron-peak elements in Population III core-collapse supernovae. The nu-process and the following proton and neutron capture reactions produce odd-Z iron-peak elements in complete and incomplete Si burning region. This reaction sequence enhances the abundances of Sc, Mn, and Co in the supernova ejecta. The supernova explosion models of 15 M_sol and 25 M_sol stars with the nu-process well reproduce the averaged Mn/Fe ratio observed in extremely metal-poor halo stars. In order to reproduce the observed Mn/Fe ratio, the total neutrino energy in the supernovae should be 3 - 9 x 10^{53} ergs. Stronger neutrino irradiation and other production sites are necessary to reproduce the observed Sc/Fe and Co/Fe ratios, although these ratios increase by the nu-process.

  18. Quark mass variation constraints from Big Bang nucleosynthesis | SciTech

    Office of Scientific and Technical Information (OSTI)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn AprilAElectronicCurvesSpeedingScientificof ScientificQ LA-UR- " "

  19. Microsoft Word - XX 13 Science and education grants offered by...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Falls, Idaho 2,813.38 for multifaceted research field trips and classroom projects focused on power generation and impacts to communities and river ecology for ninth and 10th...

  20. New nano-mechanical plasmonic phase modulator offers electronics...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    and the University of Colorado at Colorado Springs, has demonstrated a nano-mechanical plasmon phase modulator that can control and manipulate the flow of plasmons at the nanoscale...

  1. GovEnergy 2011 Offers Federal Energy Professionals Strategies...

    Office of Environmental Management (EM)

    and military energy professionals participated in GovEnergy last month - an annual trade show held in Cincinnati, Ohio cosponsored by the Energy Department along with several...

  2. Smart Meters Offer 'Instant Gratification;' Help Houston Homeowners...

    Broader source: Energy.gov (indexed) [DOE]

    Diorio explains to KPRC Local 2 News how much she's saved with her recently installed smart meter, which allows her to see her savings in real time. Houston resident Ruth...

  3. technology offer Research and Transfer Support | DI Karin Hofmann

    E-Print Network [OSTI]

    Szmolyan, Peter

    is the usage of a cyclone collector in the form of an axial hydro cyclone to separate the unwanted sediment://www.rt.tuwien.ac.at Sediment Removal by an Axial Hydro Cyclone key words: desilting | axial cyclone | pressure pipe| hydropower by implementing an axial hydro cyclone. This device produces a heavy swirling flow, the particles are carried

  4. Storage tank insulation panels that offer fire protection

    SciTech Connect (OSTI)

    Stancroff, M. [Pittsburgh Corning Corp., Houston, TX (United States)

    1995-12-31T23:59:59.000Z

    Many fluids require storage temperatures of over several hundred degrees above ambient. As a result of these elevated storage temperatures many storage tanks require insulation to help in both energy conservation and in maintaining a uniform fluid temperature distribution. Since these fluids are typically flammable these storage tanks also often require some sort of fire protection. One of the most commonly used methods of fire protection is a deluge system. Actively operated deluge systems, although effective when working properly, have several drawbacks. A cellular glass insulation panel system can provide not only excellent insulation value but also passive fire protection without the concern of an active system failure.

  5. Labor Department Offers $500 Million for Clean Energy Job Training...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    five grant competitions, totaling 500 million, to fund projects that prepare workers for green jobs in the energy efficiency and renewable energy industries. Four of the...

  6. Department of Energy Offers $245 Million Conditional Loan Guarantee...

    Office of Environmental Management (EM)

    proportion of industrial mercury emissions. The plant will use state-of-the-art air pollution control equipment to reduce its own emissions of volatile organic compounds,...

  7. www.geology.pdx.edu Undergraduate Degrees Offered

    E-Print Network [OSTI]

    , geomorphology, geomechanics, engineering geology, and teaching and learning. e PSU program serves geology majors Glaciology Geomechanics Environmental and engineering geology K-12 education In addition to their work

  8. NREL: Energy Systems Integration - NREL's ESIF Offers Equipment...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    of the first attempts to aggregate control of smart inverters in the US, he added. Other ground-breaking research on behind-the-meter power storage and bidirectional power flow is...

  9. Fact #830: July 21, 2014 Diesel Light Vehicle Offerings Expand...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    fotw830web.xlsx More Documents & Publications Fact 849: December 1, 2014 Midsize Hybrid Cars Averaged 51% Better Fuel Economy than Midsize Non-Hybrid Cars in 2014 -...

  10. active ingredients offered: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Sciences Websites Summary: Stuffed Bell Peppers Ingredients: 1 pound ground turkey 12 onion 15 ounces low sodium tomato sauce 14 cup water 18 teaspoon pepper 12 cup...

  11. Department of Energy Offers Conditional Commitment for $1.187...

    Office of Environmental Management (EM)

    Ranch project will help lower the cost of solar power and encourage more utility-scale solar deployment," said Secretary Chu. "The project will also create hundreds of jobs and...

  12. University of East Anglia technology offering Fluid mechanics

    E-Print Network [OSTI]

    Matthews, Adrian

    · Financial indemnity e.g.· marine insurance Renewable energy, oil and· gas e.g. determining mass flow rate containers. Aerodynamics and acoustics:· Receptivity and boundary layer transition; ground effect; ultrasound

  13. RMOTC offers unique test facility to oil industry

    SciTech Connect (OSTI)

    Opsal, C.M. [Fluor Daniel NPOSR-CUW, Inc., Casper, WY (United States). Rocky Mountain Oilfield Testing Center

    1998-12-31T23:59:59.000Z

    Testing laboratory developed new tools and techniques in actual field conditions before commercialization has long been a significant problem. Working lab models may fail in the first field applications because of handling, incompatibility with existing equipment, or natural elements such as wind, humidity, or temperature. Further, the risk of damage to the operators wellbore, production, or other operations can be costly and embarrassing. As research dollars are becoming harder to obtain, a neutral, non-competitive, and user friendly test site is needed. This type of facility has been developed at the US Department of Energy`s Naval Petroleum Reserve No. 3 (NPR-3), near Casper, Wyoming, through the Rocky Mountain Oilfield Testing Center (RMOTC). New technologies and processes field tested at this facility include those related to drilling production/lifting costs, P and A methods, and environmental control and remediation.

  14. Department of Energy Offers Abengoa Bioenergy a Conditional Commitment...

    Energy Savers [EERE]

    is part of the Administration's commitment to expand our advanced domestic biofuels industry," said Secretary Chu. "Investments like these will create jobs and decrease the...

  15. Energy Department Offers $50 Million to Advance Fuel Efficient...

    Energy Savers [EERE]

    plug-in electric vehicles (PEVs) as affordable and convenient to own and drive as today's gasoline-powered vehicles within the next 10 years. The funding will support a wide range...

  16. Energy Department Offers $10 Million for Energy-Saving Lighting...

    Energy Savers [EERE]

    technologies. This funding will help accelerate the development of high-quality light-emitting diode (LED) and organic light-emitting diode (OLED) products with the potential to...

  17. We offer a full range of surgical expertise. Bariatric Surgery

    E-Print Network [OSTI]

    Mohaghegh, Shahab

    with the latest technologies available, including the DaVinci surgical robot. Our flagship hospital in Morgantown-293-1253 Ruth Fitzgerald, Dept. Manager - 304-293-1616 Sharon Bartholomew, Administrative Assistant 304

  18. technology offer Research and Transfer Support | Tanja Sovic

    E-Print Network [OSTI]

    Szmolyan, Peter

    in bubbling regime by operating the secon- dary reactor in turbulent or fast flui- dization regime. It allows gas-solid con- tact over the whole height of the reactor and potentially allows operation with lower combustion/ref orming oxygen and heat transport high in both reactors, no gas phase conversion without solids

  19. BPA offering grants in science and energy education

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    on hydroelectricity, wind and other sources of electric power, methods of conserving electricity, studies of energy and environment, programs on engineering and technology...

  20. Unprecedented detail of intact neuronal receptor offers blueprint...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Argonne, Ill.- Scientists succeeded in obtaining an unprecedented view of a type of brain-cell receptor that is implicated in a range of neurological illnesses, including...

  1. Global Safeguards and Security Educational Center Course Offerings

    E-Print Network [OSTI]

    ) POC: Michael Whitaker, 865.576.1682, whitakerjm@ornl.gov Facility Systems for Accounting and Control) POC: Brian Cowell, 865.574.0656, cowellbs@ornl.gov Radiological Controls Radiological Protection (Radiological) ­ Course (25 days) POC: Bill Toth, 865.675.3738, tothwj@ornl.gov Materials of Concern

  2. MuniHELPS- Offered by 17 Utilities through the MMWEC

    Broader source: Energy.gov [DOE]

    The Massachusetts Municipal Wholesale Electric Company (MMWEC) provides the Home Energy Loss Prevention Services (HELPS) Program to seventeen municipal utilities in Massachusetts.

  3. Sample Statement of Work - Standard Service Offerings forContractor...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    of Measurement and Verification Activities Investment-Grade Audit Kickoff Meeting With ESCO - Sample Agenda Best Practices and Lessons Learned for Federal Agency ESPC Projects...

  4. CERN Offers UN Advice on Bringing Women into Science

    Broader source: Energy.gov [DOE]

    In CERN’s first opportunity to engage directly with a UN organization since it gained observer status, grad students suggested ways to improve the situation of women in science.

  5. Program Offers New Spin on Traditional Marketing | Department...

    Energy Savers [EERE]

    troop. Known as the "Cleveland Boys" around the neighborhood, this group of seven high school seniors performed at eight community outreach events for CPW this past summer. For...

  6. FEMP Offers Training on Distributed-Scale Renewable Energy Projects...

    Energy Savers [EERE]

    be able to: Plan facility renewable energy projects using available screening tools for renewable energy resources, savings to investment ratio analysis, and feasibility studies...

  7. Shoulder injury reduction with post-offer testing

    E-Print Network [OSTI]

    Harbina, Gary L.; Shenoy, Catherine; Garcia, Amy; Olson, John C.

    2011-06-21T23:59:59.000Z

    . Methods: A physical capacity evaluation based testing protocol was utilized to determine if each new employee had the physical work capacity to perform the job for which they were hired. Injuries to the shoulder were specifically scrutinized...

  8. Secretaries Chu and Salazar Lead Administration Team Offering...

    Office of Environmental Management (EM)

    and fluid flows." "Putting our best scientific minds together with BP's deepwater drilling engineers will enable these dedicated professionals to examine every feasible means...

  9. Energy Department Offers Conditional Commitment to Alcoa to Support...

    Energy Savers [EERE]

    largest wind farms, and several of the world's largest solar generation and thermal energy storage systems. Addthis Related Articles Financing the Growing American Auto...

  10. DOE Offers Support for Innovative Manufacturing Plant That Will...

    Broader source: Energy.gov (indexed) [DOE]

    of traditional polysilicon purification processes, which will reduce the overall cost of solar modules and panels. At full production, the manufacturing plant is expected to...

  11. Berkeley Program Offers New Option for Financing Residential PV Systems

    E-Print Network [OSTI]

    Bolinger, Mark A

    2009-01-01T23:59:59.000Z

    Vehicle for Residential PV Installations: Opportunities andfor Financing Residential PV Systems Mark Bolinger, Lawrencefor residential photovoltaic (PV) systems. Though financing

  12. FEMP Offers New Training on Photovoltaic Operations and Maintenance...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    The instructors for this seminar are Brad Gustafson, P.E., CEM, LEED AP, supervisor of customer services for DOE FEMP, and Andy Walker, P.E., Ph.D., principal engineer at the...

  13. FEMP Offers Updated Training on the Guiding Principles for High...

    Broader source: Energy.gov (indexed) [DOE]

    Energy's Federal Energy Management Program (FEMP) presents an updated series of training courses focused on the Guiding Principles for Federal Leadership in High-Performance and...

  14. Technology Offer High-throughput Algorithm for Automated

    E-Print Network [OSTI]

    reliability enables the same LC-MS analyses with less human resources as manual correction is not necessary Chemical industry: identification and quantitation of chemical composition of various analytes, e.g. oils

  15. RESEARCH PROPOSAL Riemann Hypothesis A proof is offered of ...

    E-Print Network [OSTI]

    2014-09-22T23:59:59.000Z

    The project is the result of special circumstances resulting from the second ... On graduation however he chose to go on to graduate school in mathematics,.

  16. Table of Contents Degrees Offered and Associated Departments 338

    E-Print Network [OSTI]

    Varela, Carlos

    359 Computer Science at Harford 369 Earth and Environmental Sciences 371 Mathematical Sciences 378 Biochemistry and Biophysics 398 Bioinformatics and Molecular Biology 403 Environmental Science 407 are meeting the high demand for scientists in these areas. A new Center for Biotechnology

  17. Table of Contents Degrees Offered and Associated Departments 334

    E-Print Network [OSTI]

    Varela, Carlos

    356 Computer Science at Harford 365 Earth and Environmental Sciences 367 Mathematical Sciences 374 Biochemistry and Biophysics 394 Bioinformatics and Molecular Biology 399 Environmental Science 402 technology are meeting the high demand for scientists in these areas. A new Center for Biotechnology

  18. Voices of Experience: New Guide Offers Utilities' Insights on...

    Energy Savers [EERE]

    the Power Over Energy campaign to empower consumers to make smart decisions about their electricity consumption. For additional information about national efforts to modernize...

  19. Cutting-Edge Building Technologies Offer Big Energy Savings Potential...

    Energy Savers [EERE]

    gas and heat energy from the surrounding air. It is also designed to help reduce peak electricity consumption during the summer. Similar to S-Ram Dynamic's heat pump,...

  20. agents offered cash: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    JADE uses an agent model and Java implementation that allow good runtime efficiency, software reuse, agent mobility and the realization of different agent architectures. 1....

  1. Cooperation Among Balancing Authorities Offers Greater Use of...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    1, 2012 - 3:10pm Addthis This is an excerpt from the Second Quarter 2012 edition of the Wind Program R&D Newsletter. Since February 2010, the Variable Generation Subcommittee at...

  2. USDA Offers Renewable Energy Feasibility Studies for Rural Businesses...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Initiative DOE and USDA Select Projects for more than 24 Million in Biomass Research and Development Grants USDA and DOE Fund Genomics Projects For Bioenergy Fuels Research...

  3. Department of Energy Offers $2 Billion in Conditional Loan Guarantee...

    Office of Environmental Management (EM)

    capacity and displace a total of 40 percent of the output from a typical 500MW coal-fired plant. Abengoa Solar Inc., the Mojave Solar project sponsor, estimates that project will...

  4. technology offer Research and Transfer Support | Tanja Sovic

    E-Print Network [OSTI]

    Szmolyan, Peter

    by the production route of the master alloy. The master alloy can be produced by water atomizing of high carbon for high mechanical loads. These parts are produced by powder mixes, axially pressed and sintered. Carbon containing iron melt, which reduced markedly the melting temperature. By special heat treatment the hardness

  5. Department Of Energy Offers $60 Million to Spur Industry Engagement...

    Energy Savers [EERE]

    two years (FY'07-'08), to engage industry experts in the conceptual design of the initial nuclear fuel recycling center and advanced recycling reactor as part of President Bush's...

  6. Wood-based Energy Technologies Michigan offers some significant advantages

    E-Print Network [OSTI]

    quality stan- dards. Wood pellets are an attractive alternative for home heating or for larger individual--ground wood. Pellet storage area. #12;distributed through a District Energy grid. Efficiencies are high on municipal solid waste. Both district heating and CHP plants can also pro- duce pellets for local housing

  7. The new Integrated Biorefinery Research Facility (IBRF) offers an unprecedented

    E-Print Network [OSTI]

    Advance Commercial Success of Thin-Film PV Cells The thin-film solar cells in use today could not function and are used to form the front of the solar cell. Improving the quality and properties of TCOs is widely of flexibility for NREL's science and technology experts to develop cost-effec- tive biofuels processes and move

  8. Department of Energy Offers Conditional Loan Guarantee Commitments...

    Office of Environmental Management (EM)

    commitment for a loan guarantee to AV Solar Ranch 1, LLC to support the Antelope Valley Solar Ranch 1 project. The 230 megawatt (MW) project will be located in the Antelope...

  9. ORNL superhydrophobic glass coating offers clear benefits | ornl...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Jellison, Pooran Joshi, Ilia Ivanov, Tao Liu, Peng Wang, Rajesh Menon, Rosa Trejo, Edgar Lara-Curzio, Scott Hunter, John Simpson, Parans Paranthaman and David Christen. The...

  10. automated container offering: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    technology, we propose a solution for real-time automated detection Terms-- rootkits, stealth malware, intrusion, con- tainment,virtual machines I. INTRODUCTION Despite to...

  11. Department of Energy Offers Conditional Commitment for a Loan...

    Broader source: Energy.gov (indexed) [DOE]

    in America by 2035." The Record Hill project will avoid over 70,000 tons of carbon pollution annually, equivalent to the annual greenhouse gas emissions from over 13,000...

  12. Sandia National Laboratories: Sandia Offers Approach to Help...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Laboratories. A report released recently by Sandia National Laboratories, the Electric Power Research Institute (EPRI), and the Georgia Institute of Technology provides a...

  13. Spotlight on Austin, Texas: Best Offer Ever Produces Upgrades...

    Energy Savers [EERE]

    and Refrigeration Institute certificate, and any other documentation (i.e. load calculation, test reports, andor drawings from contractor as needed) 3) Verify the...

  14. CHEMISTRY COURSE OFFERINGS, FALL, 2013 (Updated 8/1/13)

    E-Print Network [OSTI]

    Kounaves, Samuel P.

    in Chemistry 61. Techniques in synthesis, spectroscopy, and reactivity studies. Applications of inorganic compounds in synthesis, catalysis, materials sciences, and biology. One laboratory, one lecture, one and chemistry of materials. Three lectures, one laboratory, one recitation. Only one of Chemistry 1, 11, or 16

  15. Site in the Sky: Climate Facility Offers New Observational Capabilities

    SciTech Connect (OSTI)

    Roeder, Lynne R.

    2010-06-01T23:59:59.000Z

    This article is intended for publication in the trade journal, Meteorological Technology International. Its purpose is to introduce the audience to the ARM Climate Research Facility by describing its key capabilities (fixed, mobile and aerial facilities) with examples of field campaigns using each. It also summarizes coming enhancements to the facility through the American Recovery and Reinvestment Act of 2009, and mentions the data archive and proposal opportunities to use the facility.

  16. Silicon Ink Technology Offers Path to Higher Efficiency Solar...

    Broader source: Energy.gov (indexed) [DOE]

    equity investments. The Incubator program provides early-stage assistance to help startup companies cross technological barriers to commercialization while encouraging private...

  17. Department of Energy Offers $90.6 Million Conditional Commitment...

    Office of Environmental Management (EM)

    invested 17.5 million in seven companies in its first round of funding -- and those companies have gone on to attract more than 1.6 billion of private financing as they...

  18. Department of Energy Offers Conditional Commitment for Loan Guarantee...

    Energy Savers [EERE]

    jobs right here in Nevada," said U.S. Senate Majority Leader Harry Reid. "Innovative companies like SolarReserve are helping ensure that Nevada can lead the nation in clean...

  19. ROSE Process Offers Energy Savings for Solvent Extraction 

    E-Print Network [OSTI]

    Gearheart, J. A.; Nelson, S. R.

    1983-01-01T23:59:59.000Z

    -McGee has a bench scale pilot plant available for feedstock evaluation. Four commercial ROSE units and a large pilot plant have been placed into operation during the past five years. Two additional units are under construction and others are in various...

  20. THE OFFER OF ACTIVITIES AND SERVICES CAN BE FOUND

    E-Print Network [OSTI]

    Geffner, Hector

    activities boards w on the UPF website (www.upf.edu) w on the Student participation website (www.upf.edu/participacio) w on Canal UPF w on Facebook and Twitter WHERE CAN I FIND FURTHER INFORMATION ABOUT THESE ACTIVITIES Support Centre (CAU) (https://cau.upf.edu/sacu/). WHO SHOULD I ASK FOR FURTHER INFORMATION? THE UNIVERSITY

  1. ROSE Process Offers Energy Savings for Solvent Extraction

    E-Print Network [OSTI]

    Gearheart, J. A.; Nelson, S. R.

    1983-01-01T23:59:59.000Z

    of solvent is dictated by the nature of the feedstock and the desired specifications for the materials to be produced. In addi tion to residual feedstocks der ived from crude petroleum, oil from tar sands and oil shales, pyrolysis tar residues and tall...

  2. 16-Month Program Starting in August Offered Everywhere in Canada

    E-Print Network [OSTI]

    Ellis, Randy

    with the United Nations Global Compact. Thought Leadership Queen's School of Business has an impressive record

  3. Comprehensive phonon map offers direction for engineering new...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    power plants, laptops, and many other machines produce heat when they operate. Waste heat is an unavoidable energy loss, a trade-off in order to produce the kind of...

  4. Department of Energy Offers First Conditional Commitment for...

    Broader source: Energy.gov (indexed) [DOE]

    reflects this Administration's commitment to promoting the development of advanced biofuels," said Secretary Chu. "Strong biofuels projects like Diamond Green Diesel can help to...

  5. PNNL offers 'virtual tour' of Shallow Underground Laboratory...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    science research such as the search for dark matter in the universe or neutrinoless double-beta decay. The virtual tour allows visitors to witness the development of gas...

  6. Sandia Energy - Magnetically Stimulated Flow Patterns Offer Strategy...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    said, the technology could be practical in problems ranging from reactor cooling to microfluidics, a multidisciplinary field used, for example, in designing systems that handle...

  7. El Paso Electric Company- SCORE Plus Standard Offer Program

    Broader source: Energy.gov [DOE]

    The El Paso Electric (EPE) SCORE Plus Program is designed to help participants identify energy efficiency opportunities in existing and newly planned facilities and to provide monetary incentives...

  8. Innovative High Energy Density Capacitor Design Offers Potential...

    Broader source: Energy.gov (indexed) [DOE]

    provided 75,000 as part of an initial cooperative research and development agreement (CRADA) that allowed TroyCap to engage with LLNL. By the end of the CRADA, TroyCap had...

  9. PPPL, Princeton launch hunt for Big Bang particles offering clues...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Universe Massive Neutrino Yield." Ptolemy was an ancient Greek astronomer who lived in Egypt during the first century. Darkest, coldest conditions achievable The task calls for...

  10. Microsoft Word - REPSIA template as offered to IOUs.doc

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    REP SETTLEMENTIMPLEMENTATION AGREEMENT PRODUCTION TEMPLATE Contract No. PB- DRAFT September, 2011 RESIDENTIAL EXCHANGE PROGRAM SETTLEMENT IMPLEMENTATION AGREEMENT...

  11. Secretary Chu Offers $117 Million Conditional Commitment for...

    Office of Environmental Management (EM)

    project in Kahuku, Hawaii. Kahuku Wind Power, LLC will install twelve 2.5 MW wind turbine generators along with a battery energy storage system for electricity load stability....

  12. technology offer Research and Transfer Support | Tanja Sovic-Gasser

    E-Print Network [OSTI]

    Szmolyan, Peter

    to the substantial noise level and the space requirements a compressor cooling does not represent the ideal device

  13. Department of Energy Offers Severstal Dearborn, LLC a $730 Million...

    Office of Environmental Management (EM)

    Department of Energy Finalizes a 967 Million Loan Guarantee to Support the Agua Caliente Solar Project Department of Energy Conditional Loan Guarantee Commitment to Support the...

  14. Quantum Alloys Offer Prospects for CO2 Management Technologies...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    radical new catalysts capable of converting CO2 emissions into fuels, chemicals, and plastics. Their unique discovery involves shrinking gold into a system consisting of just 25...

  15. Cutting-Edge Building Technologies Offer Big Energy Savings Potential |

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33 1112011AT&T,Office of Policy, OAPM | Department of Energy Current TrendsDepartment

  16. Energy Department Offers $50 Million to Advance Fuel Efficient Autos |

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the YouTube|6721 Federal RegisterHydrogen and Fuel Cellof EnergyDepartmentDepartment of

  17. Energy Department Offers Conditional Commitment to Alcoa to Support

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the YouTube|6721 Federal RegisterHydrogen and Fuel Cellof EnergyDepartmentDepartment

  18. Energy Department Offers Conditional Commitment to Cape Wind Offshore Wind

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

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  19. Energy Department Offers Conditional Commitment to Support Nevada

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

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  20. Obama Administration Offers $59 Million in Conditional Loan Guarantees to

    Energy Savers [EERE]

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