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1

XIV.1-Draft ATTACHMENT XIV  

E-Print Network [OSTI]

oxidation over steam reforming is indicated to be that the reaction is self-sustaining and the only heat

Kentucky, University of

2

Morocco  

Gasoline and Diesel Fuel Update (EIA)

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:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary) " ,"ClickPipelines About U.S.30 2013 Macroeconomic team: Kay616 3.64 1967-2010 ImportsProved ReservesXIV.

3

Shell Morocco | Open Energy Information  

Open Energy Info (EERE)

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 on Office of Inspector GeneralDepartmentAUDIT REPORTOpenWende New EnergyAnatoliaScira OffshoreMediawikiShantou DanMorocco

4

Immosolar Morocco | Open Energy Information  

Open Energy Info (EERE)

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 CenterFranconia, Virginia: Energy Resources Jump to: navigation,Ohio:GreerHiCalifornia:ISI SolarIdanha,Information JumpMorocco Jump to:

5

E-Print Network 3.0 - algeria libya morocco Sample Search Results  

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

algeria libya morocco Search Powered by Explorit Topic List Advanced Search Sample search results for: algeria libya morocco Page: << < 1 2 3 4 5 > >> 1 Algeria Gambia Nigeria...

6

King Hassan II: Morocco's Messenger of Peace  

E-Print Network [OSTI]

, peace is not the first thought that comes to mind. Since the creation of the state of Israel in 1948, Arabs and Israelis have been struggling to co-exist peacefully. If policy makers are aiming at stability in the broader Middle East, it is crucial..., was the protection of the Moroccan throne. 1 In addition to Israel, he created and maintained relations with various countries to create a more balanced Maghreb, (the Arabic name for the area consisting of Algeria, Morocco, Tunisia and sometimes Libya) 2...

Cross, Megan

2007-12-17T23:59:59.000Z

7

Morocco: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

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 Home5b9fcbce19 No revision hasInformation Earth's HeatMexico: EnergyMithun Jump to:Moe WindMontMoraine II WindMorocco: Energy

8

World Bank-Morocco Study on the Impact of Climate Change on the...  

Open Energy Info (EERE)

Morocco Study on the Impact of Climate Change on the Agricultural Sector Jump to: navigation, search Name World Bank-Morocco Study on the Impact of Climate Change on the...

9

PLIO-PLEISTOCENE MAMMALIAN BIOSTRATIGRAPHY OF ATLANTIC MOROCCO Denis GERAADS  

E-Print Network [OSTI]

in North Africa at that time. In Thomas Quarry 1, the earliest archaeological level in Morocco, level L, is probably of lower Pleistocene age. In the same complex of quarries, the faunas of cave fillings, of which, following the stratigraphic studies of Biberson (1961), attention focused on the Thomas Quarries south

Paris-Sud XI, Université de

10

E-Print Network 3.0 - atlas morocco peridotite Sample Search...  

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

. Vidal, 1992. Petrogenesis of the Hercynian Tichka plutonic complex (Western High Atlas, Morocco): Trace... of inetrmediate-depth earthquakes and volcanism in the...

11

E-Print Network 3.0 - atlas mountains morocco Sample Search Results  

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

in Morocco Yildiz Aumeeruddy... the domesticated from the wild is a reality in mountain farming systems which represent an important ... Source: Aumeeruddy-Thomas, Yildiz -...

12

Is Morocco an attractive destination for foreign investors looking to invest in the residential real estate segment?  

E-Print Network [OSTI]

Over the last decade, Morocco has witnessed an accelerated process of political, economic and social reforms aimed at improving the business climate and solidifying the economic indicators. Morocco's structural reforms ...

Oubala, Khadija

2011-01-01T23:59:59.000Z

13

A Muslim Feminist Interpretation of Women's Empowerment and Gender Parity: Case Studies of Morocco and Egypt  

E-Print Network [OSTI]

This research focuses on changes in women's empowerment and gender parity during the reigns of Mohammed VI in Morocco (1999-present) and Hosni Mubarak in Egypt (1981-11 February 2011). Despite the absence of regime change in Morocco, the social...

Feather, Ginger Reeves

2012-05-31T23:59:59.000Z

14

DISTRIBUTION OF NATURALLY OCCURRING RADIONUCLIDES (U, Th) IN TIMAHDIT'S BLACK SHALE (MOROCCO)  

E-Print Network [OSTI]

focused on the use of Moroccan's black oil shales as the raw materials for production of a new type, 1991). These adsorbents were produced from oil shale, which is abundant in Morocco. The choice

Paris-Sud XI, Université de

15

Innovating government : migration, development and the state in Morocco and Mexico, 1963-2005  

E-Print Network [OSTI]

Mexico and Morocco have some of the longest standing and most advanced policies linking the emigration of their low-skilled workers to their national and sub-national economic development. In my dissertation, I examine the ...

Iskander, Natasha N. (Natasha Nefertiti), 1972-

2006-01-01T23:59:59.000Z

16

FIANTD200725 arXiv:0712.3526v2  

E-Print Network [OSTI]

########### FIAN­TD­2007­25 arXiv:0712.3526v2 [hep­th] 26 Jan 2012 FIAN­TD­2007­25 arXiv: 0712.3526

18

Implications of "Neo-Orientalist" conservation in Fez, Morocco : need for an innovative non-profit alternative  

E-Print Network [OSTI]

The exotic and mystical image of Morocco has been imbedded in the minds of outsiders even before the French protectorate was established in the early 20th century. Many countries whose modern history has its origins in an ...

Sutton, Summer Stephanie

2012-01-01T23:59:59.000Z

19

Study of pollution in the El Jadida-Safi Atlantic coastal zone (Morocco) by using PIXE and SSNTD methods  

E-Print Network [OSTI]

region (Morocco). In addition, uranium (238 U) and thorium (232 Th) contents were evaluated in the same enterprise in the world, very little after American IMC Agrico Co. (Group Freeport McMoran). Mining

Boyer, Edmond

20

The arXiv: 14 years of open access scientific communication Simeon Warner  

E-Print Network [OSTI]

/09/14 20:22:09 Abstract The arXiv was started in 1991 as a way for high-energy physicists to share publishing. Lessons learned from this development include the importance of community and critical mass how journal publishers have reacted to the arXiv, and ask what the arXiv reveals about the established

Warner, Simeon

Note: This page contains sample records for the topic "xiv-1 xiv morocco" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


21

Geochemical properties of the Beni Bousera (N. Morocco) peridotites : a field and laboratory approach to understanding melt infiltration and extraction in an orogenic peridotite massif  

E-Print Network [OSTI]

The Beni Bousera ultramafic massif is a tectonically emplaced body of upper mantle material that is exposed over 72 km2 in the Betic-Rif-Tell orogenic belt of northern Morocco. The massif is composed primarily of spinel ...

Manthei, Christian D. (Christian David)

2012-01-01T23:59:59.000Z

22

DESY 07176 arXiv:0710.2602v1  

E-Print Network [OSTI]

########### DESY 07­176 arXiv:0710.2602v1 [hep­ex] 13 Oct 2007 Prospects to Measure the Higgs Boson - Germany The process e + e ! ZH allows to measure the Higgs boson in the recoil mass spectrum against the Z boson without any assumptions on the Higgs boson decay. We performed a full simulation

23

820 -XIV Encuentro de Latinoamericanistas Espaoles ARQUITECTURA NEOCOLONIAL  

E-Print Network [OSTI]

820 - XIV Encuentro de Latinoamericanistas Españoles ARQUITECTURA NEOCOLONIAL EN VENEZUELA primeras declaratorias patrimoniales, asociadas a la arquitectura religiosa del periodo colonial. De la Zawisza, La crítica de la arquitectura en Venezuela durante el siglo XIX, Consejo Nacional de la Cultura

Paris-Sud XI, Université de

24

PVGIS approach for assessing the performances of the first PV grid-connected power plant in Morocco  

E-Print Network [OSTI]

In this paper, we apply the PVGIS method for estimating the performance of the first grid-connected PV micro-power plant in Morocco. PVGIS approach provides analysis and assessment of in-site solar energy resources and predicts with good accuracy the potential of PV systems in term of electricity production. We find that annual total power generation of the micro-power is slightly higher than that initially expected at the installation stage and actually measured. The yearly predicted and measured power production values agree to about 2 %. However, individual monthly production can have larger discrepancy.

Barhdadi, Abdelfettah

2012-01-01T23:59:59.000Z

25

Proceedings of the Fourteenth International Conference on Time-Resolved Vibrational Spectroscopy (TRVS XIV)  

E-Print Network [OSTI]

Abstracts of presentations made at the Fourteenth International Conference on Time-Resolved Vibrational Spectroscopy (TRVS XIV) held May 9-14, 2009 in Meredith, New Hampshire. TRVS is a series of biennial conferences ...

Tokmakoff, Andrei

2011-08-31T23:59:59.000Z

26

arXiv:hep-ph/0301023v321Feb2003 SCIPP 02/37  

E-Print Network [OSTI]

arXiv:hep-ph/0301023v321Feb2003 UCD-02-18 SCIPP 02/37 IUHEX-202 December, 2002 hep-ph/0301023 Higgs-energy supersymmetry . . . . . . . . . . . . . . . . 22 5.1 MSSM Higgs sector at tree level

California at Santa Cruz, University of

27

Reply to the revised Comment [PRL 102, 139601; arXiv:0810.4791] on ''Dynamic Scaling of Non-Euclidean Interfaces''  

E-Print Network [OSTI]

This is the Reply to the revised Comment [Phys. Rev. Lett. 102, 139601; arXiv:0810.4791] by Joachim Krug on our paper: C. Escudero, Phys. Rev. Lett. 100, 116101 (2008); arXiv:0804.1898.

Carlos Escudero

2009-06-05T23:59:59.000Z

28

http://arXiv.org/physics/0507088 Teaching About Nature's Nuclear Reactors  

E-Print Network [OSTI]

http://arXiv.org/physics/0507088 Teaching About Nature's Nuclear Reactors J. Marvin Herndon reactors existed in uranium deposits on Earth long before Enrico Fermi built the first man-made nuclear reactors. The subject of planetocentric nuclear fission reactors can be a jumping off point for stimulating

Learned, John

29

arXiv:math.QA/0212313v122Dec2002 MACDONALD POLYNOMIALS AND ALGEBRAIC  

E-Print Network [OSTI]

arXiv:math.QA/0212313v122Dec2002 MACDONALD POLYNOMIALS AND ALGEBRAIC INTEGRABILITY OLEG CHALYKH1 Abstract. We construct explicitly (non-polynomial) eigenfunctions of the difference operators by Macdonald in case t = qk, k Z. This leads to a new, more elementary proof of several Macdonald conjectures, first

Haase, Markus

30

arXiv:astro-ph/0508261v111Aug2005 THE OPACITY OF SPIRAL GALAXY DISKS  

E-Print Network [OSTI]

Figure 2 shows the stacked radial opacity profile of our entire sample of 32 HST/WFPC2 fields. FromarXiv:astro-ph/0508261v111Aug2005 THE OPACITY OF SPIRAL GALAXY DISKS Dust opacity from calibrated Abstract The opacity of foreground spiral disks can be probed from the number of distant galaxies seen

Kruit, Piet van der

31

arXiv:astro-ph/0106481v126Jun2001 MASSIVE DATASETS IN ASTRONOMY  

E-Print Network [OSTI]

arXiv:astro-ph/0106481v126Jun2001 Chapter 1 MASSIVE DATASETS IN ASTRONOMY Robert J. Brunner, S 21218 USA szalay@pha.jhu.edu Abstract Astronomy has a long history of acquiring, systematizing archives and services representing a new in- formation infrastructure for astronomy of the 21st century

Prince, Thomas A.

32

arXiv:physics/000908727Sep2000 MEASURING AND CONTROLLING ENERGY SPREAD IN CEBAF  

E-Print Network [OSTI]

arXiv:physics/000908727Sep2000 MEASURING AND CONTROLLING ENERGY SPREAD IN CEBAF G. A. Krafft, J spread from a CEBAF-type machine to be relatively small; the measured energy spread from CEBAF at 4 Ge, the various subsystems contributing to the energy spread of a CEBAF-type accel- erator are reviewed, as well

33

arXiv:astro-ph/0509571v119Sep2005 Gamma-Ray Burst Early Afterglows  

E-Print Network [OSTI]

arXiv:astro-ph/0509571v119Sep2005 Gamma-Ray Burst Early Afterglows Bing Zhang Department of Physics's Swift Gamma-Ray Burst Explorer open a new era for the multi-wavelength study of the very early afterglow phase of gamma-ray bursts (GRBs). GRB early afterglow information is essential to explore the unknown

Zhang, Bing

34

arXiv:hep-ph/0602242v67Sep2006 SCIPP-06/01  

E-Print Network [OSTI]

arXiv:hep-ph/0602242v67Sep2006 SCIPP-06/01 hep-ph/0602242 February, 2006 Basis-independent methods care [14, 15] to avoid neutral Higgs-mediated flavor-changing neutral currents (FCNCs) at tree level to completely remove the tree-level FCNC effects. Both the discrete symmetries alluded to above

California at Santa Cruz, University of

35

arXiv:hep-ph/9806331v110Jun1998 SCIPP 98/10  

E-Print Network [OSTI]

arXiv:hep-ph/9806331v110Jun1998 SCIPP 98/10 March 1998 hep-ph/9806331 Probing the MSSM Higgs Sector at tree-level in terms of two Higgs sector parameters. This structure arises due to constraints imposed parameters introduced above are real. Supersymmetry imposes the fol- lowing constraints on the tree

California at Santa Cruz, University of

36

arXiv:hep-ph/9810536v212Nov1998 SLAC-PUB-7853  

E-Print Network [OSTI]

arXiv:hep-ph/9810536v212Nov1998 SLAC-PUB-7853 SCIPP-98/31 FERMILAB-PUB-98/345-T hep-ph/9810536 number conservation in the tree-level supersymmetric theory, it is sufficient to impose one extra

California at Santa Cruz, University of

37

arXiv:hep-ph/001029625Oct2000 JLAB-THY-00-37  

E-Print Network [OSTI]

arXiv:hep-ph/001029625Oct2000 JLAB-THY-00-37 RUB-TPII-17/00 hep-ph/0010296 DVCS amplitude at tree for transverse polarization contains a divergence already at tree level. However, this divergence has zero

Thomas Jefferson National Accelerator Facility

38

arXiv:hep-ph/0207010v529Jan2003 UCD-2002-10  

E-Print Network [OSTI]

arXiv:hep-ph/0207010v529Jan2003 UCD-2002-10 SCIPP-02/10 hep-ph/0207010 July 2002 The CP also been addressed recently in ref. [12]. 2 #12;masses and mixing angles vs. Lagrangian tree

California at Santa Cruz, University of

39

arXiv:hep-ph/0212010v11Dec2002 SCIPP 02/27  

E-Print Network [OSTI]

arXiv:hep-ph/0212010v11Dec2002 SCIPP 02/27 November, 2002 hep­ph/0212010 Decoupling generate an accidental cancellation between tree-level and one-loop terms, resulting in a SM-like Higgs tree- level and one-loop terms, resulting in a SM-like Higgs boson for moderate mA outside

California at Santa Cruz, University of

40

arXiv:astro-ph/0703364v227Aug2007 Electromagnetic dark energy  

E-Print Network [OSTI]

arXiv:astro-ph/0703364v227Aug2007 Electromagnetic dark energy Christian Beck School of MathematicalGill University, Montreal, Quebec, Canada (Dated: August 28, 2007) We introduce a new model for dark energy equations, or more generally with the existence of dark energy. The dark energy density consistent

Wright, Francis

Note: This page contains sample records for the topic "xiv-1 xiv morocco" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


41

arXiv:astro-ph/0512327v27Mar2006 Laboratory tests on dark energy  

E-Print Network [OSTI]

arXiv:astro-ph/0512327v27Mar2006 Laboratory tests on dark energy Christian Beck School of the currently observed dark energy in the universe is completely unclear, and many different theoretical models co-exist. Nevertheless, if dark energy is produced by vac- uum fluctuations then there is a chance

Beck, Christian

42

ECMOR XIV 14th European Conference on the Mathematics of Oil Recovery  

E-Print Network [OSTI]

ECMOR XIV ­ 14th European Conference on the Mathematics of Oil Recovery Catania, Sicily, Italy, 8 respectively. We achieved an increase of 15.2% in the secondary objective for a decrease of 0.5% in the primary of Oil Recovery Catania, Sicily, Italy, 8-11 September 2014 Introduction Various model-based optimization

Van den Hof, Paul

43

arXiv:hepex/0505096 Measurement of the Higgs Boson Mass  

E-Print Network [OSTI]

################ arXiv:hep­ex/0505096 v1 30 May 2005 Measurement of the Higgs Boson Mass for the measurement of the Higgs boson mass. An integrated luminosity of 500 fb 1 is assumed. For Higgs boson masses of 120, 150 and 180 GeV the uncertainty on the Higgs boson mass measurement is estimated to be 40, 65

44

Ultrafast Phenomena XIV, pp. 650-654 , Springer, Berlin (2005). 650 Ultrafast Dynamics of Light Transmission  

E-Print Network [OSTI]

of ultrafast pulse propagation through nano-hole arrays reported a 10-fs delay in transmission [6 of ultrafast light propagation through plasmonic nano-crystals using light pulses much shorter than the SPPUltrafast Phenomena XIV, pp. 650-654 , Springer, Berlin (2005). 650 Ultrafast Dynamics of Light

Peinke, Joachim

45

arXiv:math-ph/0305049v123May2003 Transport and Dissipation in Quantum Pumps  

E-Print Network [OSTI]

arXiv:math-ph/0305049v123May2003 Transport and Dissipation in Quantum Pumps J. E. Avron , A in quantum pumps. The notion of "energy shift", a self-adjoint operator dual to the Wigner time delay, plays in quantum pumps. We discuss the geometric and topological content of adiabatic transport and show

46

arXiv:mathph/0305049 Transport and Dissipation in Quantum Pumps  

E-Print Network [OSTI]

arXiv:math­ph/0305049 v1 23 May 2003 Transport and Dissipation in Quantum Pumps J. E. Avron #3; , A in quantum pumps. The notion of \\energy shift", a self-adjoint operator dual to the Wigner time delay, plays in quantum pumps. We discuss the geometric and topological content of adiabatic transport and show

47

arXiv:condmat/0002194 Geometry, Statistics and Asymptotics of Quantum Pumps  

E-Print Network [OSTI]

arXiv:cond­mat/0002194 v2 31 May 2000 Geometry, Statistics and Asymptotics of Quantum Pumps J. E¨uttiker et. al. (BPT) relating the adiabatically pumped current to the S matrix and its (time) derivatives. We relate the charge in BPT to Berry's phase and the corresponding Brouwer pumping formula

48

arXiv:cond-mat/9707333v131Jul1997 Fingering Instability in Combustion  

E-Print Network [OSTI]

arXiv:cond-mat/9707333v131Jul1997 Fingering Instability in Combustion O. Zik(1) , Z. Olami(2) and E quantitatively verify a model based on diffusion limited transport. Harnessing combustion is a basic element conflagrations is often determined by fundamental issues regarding the stability of combustion fronts. Although

Moses, Elisha

49

arXiv:physics/0603142v117Mar2006 Brownian Motion after Einstein  

E-Print Network [OSTI]

arXiv:physics/0603142v117Mar2006 Brownian Motion after Einstein: Some new applications and new-4000 Roskilde, Denmark 2 Department of Biological Physics, E¨otv¨os Lor´and University (ELTE), H-1117 Budapest, Hungary 3 Max Planck Institute for the Physics of Complex Systems, N¨othnitzer Strasse 38, D

50

arXiv:astro-ph/0009259v219Sep2000 How the Sun Shines  

E-Print Network [OSTI]

arXiv:astro-ph/0009259v219Sep2000 How the Sun Shines John N. Bahcall What makes the sun shine? How does the sun produce the vast amount of energy necessary to support life on earth? These questions 1833 Treatise on Astronomy: The sun's rays are the ultimate source of almost every motion which takes

Walter, Frederick M.

51

A review of "The Dynastic State and the Army under Louis XIV: Royal Service and Private Interest, 1661-1701." by Guy Rowlands  

E-Print Network [OSTI]

society and agriculture, and economic development in early modern England. Guy Rowlands. The Dynastic State and the Army under Louis XIV: Royal Service and Private Interest, 1661-1701. Cambridge: Cambridge University Press, 2002. xxv + 404 pp. $70....00. Review by WENDY F. KASINEC, SOUTHWESTERN UNIVERSITY. This ambitious and provocative book by Guy Rowlands regarding the army during Louis XIV?s rule situates this vital institution within the context of personal and dynastic concerns held by both the king...

Wendy F. Kasinec

2005-01-01T23:59:59.000Z

52

arXiv:hep-ph/0208209v313Dec2002 FERMILAB-Pub-02/114-T  

E-Print Network [OSTI]

arXiv:hep-ph/0208209v313Dec2002 FERMILAB-Pub-02/114-T SCIPP 02/07 hep­ph/0208209 Higgs Boson Theory

California at Santa Cruz, University of

53

arXiv:hep-ph/0103095v19Mar2001 Low-Energy Supersymmetry and its Phenomenology  

E-Print Network [OSTI]

arXiv:hep-ph/0103095v19Mar2001 1 Low-Energy Supersymmetry and its Phenomenology Howard E. Habera for the phenomenology of Higgs bosons and supersymmetric particles at future colliders are discussed. 1. INTRODUCTION

California at Santa Cruz, University of

54

arXiv:nucl-ex/0002003v225Feb2000 Phenomenology of the deuteron electromagnetic form factors  

E-Print Network [OSTI]

arXiv:nucl-ex/0002003v225Feb2000 Phenomenology of the deuteron electromagnetic form factors D. The parameterizations allow a phenomenological characterization of the deuteron electromagnetic struc- ture. They can

Thomas Jefferson National Accelerator Facility

55

arXiv:hep-ex/0211027v111Nov2002 Search for neutrinoless decays involving the K0  

E-Print Network [OSTI]

arXiv:hep-ex/0211027v111Nov2002 1 Search for neutrinoless decays involving the K0 S meson K neutrinoless LFV modes within a model involving heavy Dirac neutrinos. The branching fractions depend

56

arXiv:physics/0401035v19Jan2004 A Didactic Approach to Linear Waves in the Ocean  

E-Print Network [OSTI]

arXiv:physics/0401035v19Jan2004 A Didactic Approach to Linear Waves in the Ocean F. J. Beron conceptual. Accordingly, the equations of motion are simplified as much as possible for didactic purposes

Beron-Vera, Francisco Javier

57

Reply to [arXiv:1105.5653]: "Comment on 'Quasinormal modes in Schwarzschild-de Sitter spacetime: A simple derivation of the level spacing of the frequencies'"  

E-Print Network [OSTI]

We explain why the analysis in our paper [Phys. Rev. D 69, 064033 (2004), arXiv:gr-qc/0311064 ] is relevant and correct.

T. Roy Choudhury; T. Padmanabhan

2011-05-31T23:59:59.000Z

58

arXiv:hep-ph/9901365v121Jan1999 SCIPP 99/06  

E-Print Network [OSTI]

arXiv:hep-ph/9901365v121Jan1999 SCIPP 99/06 January, 1999 hep­ph/9901365 How Well Can We Predict, b) are the corresponding Yukawa couplings. The tree-level physical Higgs spectrum is easily computed| mZ. The maximum tree-level upper bound of mZ is saturated when one of the vevs vanishes (and mA0 > m

California at Santa Cruz, University of

59

arXiv:hep-ph/9906310v110Jun1999 SLAC-PUB-8173  

E-Print Network [OSTI]

arXiv:hep-ph/9906310v110Jun1999 SLAC-PUB-8173 SCIPP-99/24 hep-ph/9906310 June, 1999 Neutrino masses-generation models, three sneutrino-antisneutrino mass splittings are generated at tree-level. In contrast, only one neutrino mass is generated at tree-level; the other two neutrinos acquire masses at one-loop. In many

California at Santa Cruz, University of

60

arXiv:1201.6305v1[hep-ph]30Jan2012 CERNPHTH/2012022  

E-Print Network [OSTI]

arXiv:1201.6305v1[hep-ph]30Jan2012 CERN­PH­TH/2012­022 KA­TP­03­2012 MSSM Higgs Bosons from Stop´isica de Cantabria (CSIC-UC), Santander, Spain 2 PH-TH, CERN, CH­1211 Gen`eve 23, Switzerland 3 Institut f ratios. They are roughly of O(10%) of the tree-level results, but can go up to 30% or higher

Note: This page contains sample records for the topic "xiv-1 xiv morocco" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


61

arXiv:hep-ph/0611168v113Nov2006 SI-HEP-2006-15  

E-Print Network [OSTI]

arXiv:hep-ph/0611168v113Nov2006 SI-HEP-2006-15 November 13, 2006 Inclusive Semi-leptonic B Decays orders in the 1/mb expansion in inclusive semi-leptonic decays at tree level. We reproduce the known 1/m3 b terms and compute the 1/m4 b terms at tree level. The appearing non-perturbative parameters

Siegen, Universität

62

arXiv:hepph/9903516 hepph/9903516 BNLHET99/6  

E-Print Network [OSTI]

arXiv:hep­ph/9903516 v2 28 Dec 1999 hep­ph/9903516 BNL­HET­99/6 DFTT 16/99 UCLA/99/TEP/11 MSUHEP are required: a) n particle production amplitudes at tree level, one loop and two loops; b) n+1 particle production amplitudes at tree level and one loop; c) n + 2 particle production amplitudes at tree level

Schmidt, Carl

63

arXiv:hep-ph/9909335v113Sep1999 SCIPP 98/47  

E-Print Network [OSTI]

arXiv:hep-ph/9909335v113Sep1999 SCIPP 98/47 August, 1999 hep­ph/9909335 Radiative Corrections that MW = MZ cos W at tree level, the one-loop corrections due to virtual charged Higgs bosons always) symmetry" [4]. This symmetry leads to the tree-level relation, M2 W /M2 Z cos2 W = 1, a relation

California at Santa Cruz, University of

64

arXiv:1311.5455v1 NLO QCD Corrections to Electroweak Higgs Boson  

E-Print Network [OSTI]

arXiv:1311.5455v1 [hep­ph] 21 Nov 2013 NLO QCD Corrections to Electroweak Higgs Boson Plus Three.sjodahl@thep.lu.se The implementation of the full next­to­leading order (NLO) QCD corrections to electroweak Higgs boson plus three jet Model (SM) Higgs boson [3, 4, 5, 6]. Further, reports from the ATLAS and CMS Collaborations indicate

Lunds Universitet,

65

arXiv:0803.1146v1[math.CO]5Mar2008 A combinatorial formula for Macdonald polynomials  

E-Print Network [OSTI]

arXiv:0803.1146v1[math.CO]5Mar2008 A combinatorial formula for Macdonald polynomials Arun Ram for Macdonald polynomials for all Lie types. These formulas are generalizations of the formulas of Haglund-Haiman-Loehr for Macdonald polynoimals of type GLn. At q = 0 these formulas specialize to the formula of Schwer

Ram, Arun

66

arXiv:1112.5993v1[hep-ph]27Dec2011 A RADIATIVELY IMPROVED FERMIOPHOBIC  

E-Print Network [OSTI]

arXiv:1112.5993v1[hep-ph]27Dec2011 A RADIATIVELY IMPROVED FERMIOPHOBIC HIGGS BOSON SCENARIO E) Higgs boson search [1] is approaching its completion with the operation of the LHC at a larger Higgs boson. In the latter case, exploring the possibility of a Higgs boson with characteristics

67

arXiv:cond-mat/0408020v12Aug2004 Electric generation of spin in crystals with reduced symmetry  

E-Print Network [OSTI]

arXiv:cond-mat/0408020v12Aug2004 Electric generation of spin in crystals with reduced symmetry of spin accumulation in semiconduc- tors, we propose a way of generating a spin polarization in crystals with strong spin-orbit interac- tions. We show that, in the presence of an electric field, there exists

Niu, Qian

68

arXiv:1201.5447v1[math.DG]26Jan2012 CRITICAL CONFIGURATIONS OF PLANAR ROBOT ARMS  

E-Print Network [OSTI]

arXiv:1201.5447v1[math.DG]26Jan2012 CRITICAL CONFIGURATIONS OF PLANAR ROBOT ARMS G these results to the case of open polygonal chains, or robot arms. We introduce the notion of the oriented area of various special configurations of robot arms modeled by open polygonal chains appears essential in many

Siersma, Dirk

69

arXiv:cond-mat/0208233v418Nov2003 Classical and quantum pumping in closed systems  

E-Print Network [OSTI]

arXiv:cond-mat/0208233v418Nov2003 Classical and quantum pumping in closed systems Doron Cohen version [1], follow up [2]) Pumping of charge (Q) in a closed ring geometry is not quantized even and the adiabatic contributions to Q. As an application we bring examples for classical dissipative pumping

Cohen, Doron

70

arXiv:astro-ph/0501317v117Jan2005 Observation of the Ankle and Evidence for a  

E-Print Network [OSTI]

arXiv:astro-ph/0501317v117Jan2005 Observation of the Ankle and Evidence for a High-Energy Break spectrum gives an ob- servation of a feature known as the "ankle" near 3 ? 1018 eV, and strong evidence

71

arXiv:0906.4351v1[cond-mat.mes-hall]23Jun2009 Interfaces Within Graphene Nanoribbons  

E-Print Network [OSTI]

arXiv:0906.4351v1[cond-mat.mes-hall]23Jun2009 Interfaces Within Graphene Nanoribbons J Wurm1,2 , M the conductance through two types of graphene nanostructures: nanoribbon junctions in which the width changes from that experience from electron gas waveguides does not carry over to graphene nanostructures. The interior

Yanikoglu, Berrin

72

arXiv:0707.4149v1[math.DG]27Jul2007 Test configurations and Geodesic rays  

E-Print Network [OSTI]

arXiv:0707.4149v1[math.DG]27Jul2007 Test configurations and Geodesic rays Xiuxiong Chen , Yudong Tang February 5, 2008 Contents 1 Introduction 2 2 Preliminary 5 2.1 Geodesic rays in K¨ahler potential Relative C1,1 geodesic ray from smooth test configuration 8 3.1 Existence

Chen, Xiuxiong

73

arXiv:hep-ph/961238817Dec1996 Signals from Flavor Changing Scalar Currents at the Future Colliders  

E-Print Network [OSTI]

arXiv:hep-ph/961238817Dec1996 Signals from Flavor Changing Scalar Currents at the Future Colliders Neutral Cur- rents arising at the tree level. The existing constraints mainly affect the couplings (2HDM) with Flavor Changing Neu- tral Currents (FCNC's) allowed at the tree level [1]-[3]. This Model

Thomas Jefferson National Accelerator Facility

74

arXiv:hep-ph/0007006v212Jul2000 FERMILAB-Pub-00/138-T  

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arXiv:hep-ph/0007006v212Jul2000 FERMILAB-Pub-00/138-T FTUAM 99-27 IFT-UAM 00-20 SCIPP 00/22 hep­ph. It is well known that the tree-level couplings of the lightest MSSM Higgs boson (h0 ) to fermion pairs

California at Santa Cruz, University of

75

arXiv:0706.2986v1[astro-ph]20Jun2007 DARK MATTER AND DARK ENERGY  

E-Print Network [OSTI]

arXiv:0706.2986v1[astro-ph]20Jun2007 DARK MATTER AND DARK ENERGY MARC KAMIONKOWSKI California, and/or the introduction of some negative-pressure "dark energy," again, the nature of which remains Press. kamion@tapir.caltech.edu 1 #12;Dark Matter and Dark Energy 2 eries may help us understand the new

Steidel, Chuck

76

arXiv:hep-ph/0010338v26Dec2000 FERMILAB-Conf-00/279-T  

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arXiv:hep-ph/0010338v26Dec2000 FERMILAB-Conf-00/279-T SCIPP 00/37 hep­ph/0010338 October 31, 2000 Working Group Members Michael Albrow (Fermilab) Howard Baer (Florida State) Emanuela Barberis (LBNL) Armando A. Barrientos Bendez´u (Hamburg) Pushpalatha Bhat (Fermilab) Alexander Belyaev (Moscow State

California at Santa Cruz, University of

77

arXiv:hep-ph/0106116v327Feb2002 FERMILAB-Pub-00/334-T  

E-Print Network [OSTI]

arXiv:hep-ph/0106116v327Feb2002 FERMILAB-Pub-00/334-T SCIPP-01/25 UCD-01-23 hep-ph/0106116 and approaches zero in the so-called "decoupling limit" of the model [1]. Experiments at the Fermilab Tevatron [2

California at Santa Cruz, University of

78

arXiv:hep-ph/0412300v121Dec2004 Neutrinoless double beta decay and direct searches for neutrino mass  

E-Print Network [OSTI]

arXiv:hep-ph/0412300v121Dec2004 Neutrinoless double beta decay and direct searches for neutrino (Dated: December 22, 2004) Study of the neutrinoless double beta decay and searches for the manifestation and recommendations on them. · Observation of the neutrinoless double-beta decay (0) would prove that the total lepton

Piepke, Andreas G.

79

arXiv:1003.5447v2[cs.LO]14May2010 Relating Nominal and Higher-order  

E-Print Network [OSTI]

, nominal logic, higher-order abstract syn- tax This work has been supported by INRIA through the "Equipes]. Formalizing speci- fication based on higher-order abstract syntax requires a frame- work with devicesarXiv:1003.5447v2[cs.LO]14May2010 Relating Nominal and Higher-order Abstract Syntax Specifications

Paris-Sud XI, Université de

80

arXiv:cond-mat/9606101v114Jun1996 Relationship Between Structural Fractal and Possible Dynamic Scaling  

E-Print Network [OSTI]

arXiv:cond-mat/9606101v114Jun1996 Relationship Between Structural Fractal and Possible Dynamic dimensionality are obtained for different structures. We then show that there might exist the dynamic scaling with homogeneous structure are obtained. The dynamic critical exponents of the global proteins in folding

Gong, Xingao

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to obtain the most current and comprehensive results.


81

arXiv:1206.2498v2[cond-mat.other]19Nov2012 Quantum vortex reconnections  

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, and parts of the initial vortical tubes can be left behind as vortex threads, which then undergo successivearXiv:1206.2498v2[cond-mat.other]19Nov2012 Quantum vortex reconnections S. Zuccher,1 M. Caliari,1 A with time before and after the vor- tex reconnection. We also compute vortex reconnections using the Biot

Caliari, Marco

82

arXiv:cond-mat/9904034v25Apr1999 Making, probing and understanding Bose-Einstein condensates  

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arXiv:cond-mat/9904034v25Apr1999 Making, probing and understanding Bose-Einstein condensates W-Einstein condensation (BEC) in dilute atomic gases [1, 2, 3, 4, 5] achieved several long-standing goals. First, neutral condensates, refs. [9, 10, 11] contain a more complete account on the cooling and trapping techniques

Hart, Gus

83

arXiv:1205.4241v1[hep-th]18May2012 Self-accelerating Massive Gravity  

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arXiv:1205.4241v1[hep-th]18May2012 Self-accelerating Massive Gravity: Exact solutions for any dominates over other sources of stress energy the cosmological expansion self-accelerates, even when found, including the scylla of incompatibility with Solar System tests [2, 3] and the charybdis of ghost

Hu, Wayne

84

arXiv:1305.2916v1[hep-th]13May2013 Self-accelerating Massive Gravity  

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arXiv:1305.2916v1[hep-th]13May2013 Self-accelerating Massive Gravity: How Zweibeins Walk through that the St¨uckelberg equations of motion on the self-accelerating branch prevent solutions from evolving that the Friedmann-Robertson-Walker (FRW) metric is incompatible with massive gravity, but rather

Hu, Wayne

85

arXiv:heplat/0610083v1 Hadron and Lepton School and Conference, Tehran, Iran, May 19th 2006 1  

E-Print Network [OSTI]

arXiv:hep­lat/0610083v1 13 Oct 2006 Hadron and Lepton School and Conference, Tehran, Iran, May 19th, Iran, May 19th 2006 L (a) (b) L # Figure 1: Two potentially relevant graphs to the h#22;qqi

Lunds Universitet,

86

Comment on arXiv:1104.2019, "Relative locality and the soccer ball problem," by Amelino-Camelia et al  

E-Print Network [OSTI]

It is explained why the argument in arXiv:1104.2019 does not answer the question how to describe multi-particle states in models with a deformed Lorentz-symmetry in momentum space.

Sabine Hossenfelder

2012-02-18T23:59:59.000Z

87

arXiv:0810.3042v1[physics.bio-ph]16Oct2008 Single-domain protein folding: a multi-faceted  

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arXiv:0810.3042v1[physics.bio-ph]16Oct2008 Single-domain protein folding: a multi-faceted problem protein-like models can help to understand many controversial issues. Keywords: Protein folding, energy

Ritort, Felix

88

arXiv:1311.0292v1[astro-ph.EP]1Nov2013 Runaway greenhouse effect on exomoons due to  

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arXiv:1311.0292v1[astro-ph.EP]1Nov2013 Runaway greenhouse effect on exomoons due to irradiation to experience a runaway greenhouse effect. Results. Planetary illumination from a 13-Jupiter-mass planet onto

Barnes, Rory

89

5/14/10 4:32 PMTechnology Review: Blogs: arXiv blog: First Mathematical Model of Cow Behavior Page 1 of 4http://www.technologyreview.com/blog/arxiv/25171/  

E-Print Network [OSTI]

5/14/10 4:32 PMTechnology Review: Blogs: arXiv blog: First Mathematical Model of Cow Behavior Page | auf Deutsch | in Italiano | | in India Home Videos Blogs Briefings Community Magazine Newsletters Events Resources Subscribe Computing Web Communications Energy Materials Biomedicine Business arXiv blog

Bollt, Erik

90

arXiv:1301.3520v1[hep-lat]15Jan2013 Bounds on free energy in QCD  

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arXiv:1301.3520v1[hep-lat]15Jan2013 Bounds on free energy in QCD Axel Maas Institute 10003, USA E-mail: dz2@nyu.edu We derive some exact bounds on the free energy W(J) in QCD, where Jb µ of connected gluon correlators. Among other results, we show that for a static source J(x) = h the free energy

Maas, Axel

91

arXiv:0711.2890v5[hep-ph]10Jun2008 SCIPP-07/16  

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arXiv:0711.2890v5[hep-ph]10Jun2008 SCIPP-07/16 arXiV:0711.2890 [hep-ph] November, 2007 Hard to tree-level supersymmetric relations in the chargino and neutralino sectors that can be as large as 56 the effects of the SUSY-breaking one-loop effects appear as corrections to tree-level relations. For example

California at Santa Cruz, University of

92

arXiv:1002.4996v1[cs.DM]26Feb2010 Triangular Self-Assembly  

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arXiv:1002.4996v1[cs.DM]26Feb2010 Triangular Self-Assembly Lila Kari Shinnosuke Seki Zhi Xu 5B7 {lila, sseki, zhi_xu}@csd.uwo.ca February 27, 2010 Abstract We discuss the self-assembly system in their laboratory by the method of self-assembly. One systematic study on this topic is the self-assembly of squares

Kari, Lila

93

arXiv:1101.4041v1[math.PR]20Jan2011 Randomly biased walks on subcritical trees  

E-Print Network [OSTI]

arXiv:1101.4041v1[math.PR]20Jan2011 Randomly biased walks on subcritical trees G´erard Ben Arous study the time taken for a biased random walk to return to the root of a subcritical Galton-Watson tree by the presence of subcritical trees adjacent to the backbone that may act as traps that detain the walker. Indeed

Goldschmidt, Christina

94

Relationships between Beef Postharvest Biochemical Factors and Warner-Bratzler Shear Force  

E-Print Network [OSTI]

fragmentation index Mg2+ Magnesium mW Milliwatts ?l Microliter ?M Micromolar N Newtons (1 N = 0.102 kg force) Na+ Sodium ppm Parts per million PYG Preliminary Yield grade QG Quality grades viii REA Ribeye area RV Revalor IH + Revalor H rpm... ......................................................................................................... xiv 1. INTRODUCTION .......................................................................................................... 1 2. REVIEW OF LITERATURE ......................................................................................... 4 2.1...

Orozco Hernandez, Pilar

2013-04-01T23:59:59.000Z

95

arXiv:1009.5936v1[quant-ph]29Sep2010 On the environmental stability of quantum chaotic ratchets  

E-Print Network [OSTI]

arXiv:1009.5936v1[quant-ph]29Sep2010 On the environmental stability of quantum chaotic ratchets 30, 2010) The transitory and stationary behavior of a quantum chaotic ratchet consisting of a chaotic attractor. In both cases the temperature quickly stabilizes the ratchet, but in the latter it also

Paris-Sud XI, Universit de

96

arXiv:0908.3746v1[astro-ph.SR]26Aug2009 Analytic modeling of the Moreton wave kinematics  

E-Print Network [OSTI]

arXiv:0908.3746v1[astro-ph.SR]26Aug2009 Analytic modeling of the Moreton wave kinematics M. Temmer expansion of the CME flanks), we calculate the kinematics of the associated Moreton wave signature. Those model input parameters are deter- mined which fit the observed Moreton wave kinematics best. Using

Temmer Manuela

97

arXiv:math-ph/0307020v330Dec2003 Energy spectra of the ocean's internal wave field: theory and observations.  

E-Print Network [OSTI]

with internal wave breaking [4] rather than by the production of cold, dense water by convection at high. Consistent only with linear internal wave kinematics, the GM spectrum was developed as an empirical curve fitarXiv:math-ph/0307020v330Dec2003 Energy spectra of the ocean's internal wave field: theory

Tabak, Esteban G.

98

arXiv:1004.0373v3[physics.ins-det]8May2012 Measurement of scintillation efficiency for nuclear recoils in liquid argon  

E-Print Network [OSTI]

arXiv:1004.0373v3[physics.ins-det]8May2012 Measurement of scintillation efficiency for nuclear results for nuclear recoil energies between 10 and 250 keVr at zero electric field. II. REVIEW OF PHYSICAL University, New Haven, CT (Dated: May 9, 2012) The scintillation light yield of liquid argon from nuclear

Sheldon, Nathan D.

99

arXiv:1208.0640v1[astro-ph.SR]3Aug2012 Contracting and Erupting Components of Sigmoidal Active  

E-Print Network [OSTI]

arXiv:1208.0640v1[astro-ph.SR]3Aug2012 Contracting and Erupting Components of Sigmoidal Active of the Atmospheric Imaging Assembly (AIA) onboard SDO, we are able to identify both the contracting and erupting components of the eruptions: the former is observed in cold AIA chan- nels as the contracting coronal loops

100

arXiv:cond-mat/0307619v231Aug2003 Quantum pumping in closed systems, adiabatic transport, and the Kubo formula  

E-Print Network [OSTI]

arXiv:cond-mat/0307619v231Aug2003 Quantum pumping in closed systems, adiabatic transport pumping in closed systems is considered. We explain that the Kubo formula contains all the physically relevant ingredients for the calculation of the pumped charge (Q) within the frame- work of linear response

Cohen, Doron

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We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


101

arXiv:0706.3330v2[physics.flu-dyn]20Feb2008 Coherent structures in localised and global pipe turbulence  

E-Print Network [OSTI]

arXiv:0706.3330v2[physics.flu-dyn]20Feb2008 Coherent structures in localised and global pipe Walk, Bristol BS8 1TW, United Kingdom The recent discovery of unstable travelling waves (TWs) in pipe in both structure and en- ergy with known TWs using numerical simulations in a long pipe. These only occur

Willis, Ashley

102

arXiv:0905.3759v3[nlin.AO]27Jan2010 Evolving networks and the development of neural  

E-Print Network [OSTI]

arXiv:0905.3759v3[nlin.AO]27Jan2010 Evolving networks and the development of neural systems Samuel Johnson, J. Marro and Joaqu´in J. Torres Departamento de Electromagnetismo y F´isica de la Materia Granada, Spain. E-mail: samuel@onsager.ugr.es, jmarro@ugr.es and jtorres@onsager.ugr.es Abstract

Johnson, Samuel

103

arXiv:1008.2085v3[astro-ph.CO]23Nov2011 Axion physics in a Josephson junction environment  

E-Print Network [OSTI]

arXiv:1008.2085v3[astro-ph.CO]23Nov2011 Axion physics in a Josephson junction environment Christian experiments based on Josephson junctions, SQUIDS, and coupled Josephson qubits have a cosmological inter- actions in a resonant Josephson junction environment can be tested, similar in nature to recent

Beck, Christian

104

arXiv:1110.5871v1[astro-ph.IM]26Oct2011 Testing axion physics in a Josephson junction environment  

E-Print Network [OSTI]

arXiv:1110.5871v1[astro-ph.IM]26Oct2011 Testing axion physics in a Josephson junction environmentNS, UK We suggest that experiments based on Josephson junctions, SQUIDS, and coupled Josephson qubits in which axionic interaction strengths in a Josephson junction environment can be tested, similar in nature

Beck, Christian

105

arXiv:0908.1824v2[physics.comp-ph]24Feb2010 The calculation of longitude and latitude from geodesic measurements  

E-Print Network [OSTI]

arXiv:0908.1824v2[physics.comp-ph]24Feb2010 The calculation of longitude and latitude from geodesic, 2009; revised: February 24, 2010) 1. INTRODUCTION Consider a geodesic line between two points A and B by deriving the fundamental properties of geodesic lines on a spheroid of revolution. Even though aspects

Karney, Charles

106

arXiv:0908.1408v1[astro-ph.CO]10Aug2009 Hiding dark energy transitions at low redshift  

E-Print Network [OSTI]

arXiv:0908.1408v1[astro-ph.CO]10Aug2009 Hiding dark energy transitions at low redshift Michael history. Interestingly, the other place where an order unity transition in the dark energy equation requirements on dark energy, and construct explicit scalar field models of the transition. We discuss

Hu, Wayne

107

arXiv:1004.0395v2[cs.NI]6Apr2010 Estimating Self-Sustainability in Peer-to-Peer Swarming Systems  

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arXiv:1004.0395v2[cs.NI]6Apr2010 Estimating Self-Sustainability in Peer-to-Peer Swarming Systems propose a new metric, namely swarm self-sustainability. A swarm is referred to as self-sustaining if all its blocks are collectively held by peers; the self-sustainability of a swarm is the fraction of time

Massachusetts at Amherst, University of

108

MNRAS 429, 534555 (2013) doi:10.1093/mnras/sts353 The ATLAS3D Project XIV. The extent and kinematics of the molecular  

E-Print Network [OSTI]

MNRAS 429, 534­555 (2013) doi:10.1093/mnras/sts353 The ATLAS3D Project ­ XIV. The extent, D-85478 Garching, Germany 12Space Telescope European Coordinating Facility, European Southern and contrast the extent, surface brightness profiles and kinematics of the molecular gas in CO-rich ATLAS3D

Kuntschner, Harald

109

arXiv:0712.1409v1[astro-ph]10Dec2007 Deep ATLAS Radio Observations of the ELAIS-S1/Spitzer  

E-Print Network [OSTI]

arXiv:0712.1409v1[astro-ph]10Dec2007 Deep ATLAS Radio Observations of the ELAIS-S1/Spitzer Wide Facility, PO Box 76, Epping NSW 1710, Australia Tim J. Cornwell Australia Telescope National Facility, PO Box 76, Epping NSW 1710, Australia Maxim A. Voronkov Australia Telescope National Facility, PO Box 76

Norris, Ray

110

arXiv:1107.4788v1[hep-th]24Jul2011 THE RICCI FLOW ON NONCOMMUTATIVE TWO-TORI  

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arXiv:1107.4788v1[hep-th]24Jul2011 THE RICCI FLOW ON NONCOMMUTATIVE TWO-TORI TANVIR AHAMED BHUYAIN], [42], [44]. 1 #12;2 TANVIR AHAMED BHUYAIN AND MATILDE MARCOLLI The Ricci flow also found many

Marcolli, Matilde

111

arXiv:quant-ph/99050166May1999 A simple formula for ground state energy of a two-electron atom  

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() A simple expression for a ground state energy for a two-electron atom is derived. For this assumption basedarXiv:quant-ph/99050166May1999 A simple formula for ground state energy of a two-electron atom M to calculate energy levels of the He atom. He discussed a model when both electrons of a two-electron atom move

Auzinsh, Marcis

112

arXiv:1301.4731v2[nlin.CD]22Dec2013 Energy and potential enstrophy flux constraints in quasi-geostrophic models  

E-Print Network [OSTI]

, the assumption that the energy and enstrophy fluxes should tend to revert the energy spectrum from a cascadearXiv:1301.4731v2[nlin.CD]22Dec2013 Energy and potential enstrophy flux constraints in quasi University Drive, Edinburg, TX 78539-2999 Abstract We investigate an inequality constraining the energy

Gkioulekas, Eleftherios - Department of Mathematics, University of Texas

113

arXiv:1312.0015v1[astro-ph.IM]29Nov2013 The stochastic nature of stellar population modelling  

E-Print Network [OSTI]

arXiv:1312.0015v1[astro-ph.IM]29Nov2013 The stochastic nature of stellar population modelling of the sky so they will observe different stars; hence, you are sam- pling the sky with nsam elements, each

114

arXiv:1205.5114v1[astro-ph.SR]23May2012 370 Years of Astronomy at Utrecht  

E-Print Network [OSTI]

arXiv:1205.5114v1[astro-ph.SR]23May2012 370 Years of Astronomy at Utrecht ASP Conference Series in eclipse spectra taken in 1973. 1. Utrecht solar physics I spent 50 years in Utrecht astronomy, arriving as a student in the autumn of 1961 and cleaning out my desk at the near-defunct Sterrekundig Instituut Utrecht

Rutten, Rob

115

arXiv:cond-mat/0507220v19Jul2005 Direct Observation of Hydrogen Adsorption Sites and Nano-Cage Formation in  

E-Print Network [OSTI]

of future hydrogen and fuel-cell technolo- gies is critically dependent upon the discovery of new maarXiv:cond-mat/0507220v19Jul2005 Direct Observation of Hydrogen Adsorption Sites and Nano, National Institute of Standards and Technology, Gaithersburg, MD 20899 (Dated: July 8 2005) The hydrogen

Yildirim, Taner

116

arXiv:1102.3709v1[q-bio.PE]17Feb2011 Wright's adaptive landscape versus Fisher's fundamental  

E-Print Network [OSTI]

arXiv:1102.3709v1[q-bio.PE]17Feb2011 Wright's adaptive landscape versus Fisher's fundamental, email: safrank@uci.edu. To appear as: Frank, S. A. 2011. Wright's adaptive landscape versus Fisher. Calsbeek, eds. Oxford University Press. #12;Abstract Two giants of evolutionary theory, Sewall Wright and R

Frank, Steven A.

117

Viability of nuclear $?$-particle condensates A reply to N.T. Zinner and A.S. Jensen, arXiv:nucl/th0712.1191  

E-Print Network [OSTI]

In a recent paper, arXiv0712.1191 [nucl-th], Zinner and Jensen (ZJ) expressed strong doubts about the concept of alpha-particle condensation in finite nuclei. In this article we give a reply which, essentially, is point by point (but not in the order).

Y. Funaki; H. Horiuchi; G. Roepke; P. Schuck; A. Tohsaki; T. Yamada; W. von Oertzen

2008-05-16T23:59:59.000Z

118

arXiv:1003.2138v1[cs.IT]10Mar2010 1 Need-based Communication for Smart Grid: When  

E-Print Network [OSTI]

arXiv:1003.2138v1[cs.IT]10Mar2010 1 Need-based Communication for Smart Grid: When to Inquire Power Price? Husheng Li and Robert C. Qiu Abstract-- In smart grid, a home appliance can adjust its power on smart grid do not consider the cost of communications which cannot be ignored in many situations

Qiu, Robert Caiming

119

arXiv:cond-mat/0007297v118Jul2000 Permanent magnetic moment in mesoscopic metals with spin-orbit interaction  

E-Print Network [OSTI]

arXiv:cond-mat/0007297v118Jul2000 Permanent magnetic moment in mesoscopic metals with spin-orbit interaction and odd number of electrons will have a permanent magnetic moment, even in zero magnetic field an effective single-electron Hamiltonian which accounts for spin-orbit coupling. I. INTRODUCTION Permanent

Serota, Rostislav

120

arXiv:0911.5232v1[cond-mat.stat-mech]27Nov2009 Interface Free Energy or Surface Tension  

E-Print Network [OSTI]

arXiv:0911.5232v1[cond-mat.stat-mech]27Nov2009 Interface Free Energy or Surface Tension: definition. The content of the paper is 1) the definition of the interface free energy from first principles mechanical 1.1 Definition of the interface free energy Consider a physical system at equilibrium in a vessel

Pfister, Charles

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121

arXiv:1401.0597v1[math.DG]3Jan2014 ON THE VALIDITY OF THE DEFINITION OF ANGULAR  

E-Print Network [OSTI]

in comparison to translat- ing Killing field used in the definition of the ADM energy-momentum vector, soarXiv:1401.0597v1[math.DG]3Jan2014 ON THE VALIDITY OF THE DEFINITION OF ANGULAR MOMENTUM IN GENERAL of the definition of the ADM angular momentum without the parity assumption. Explicit examples of asymp- totically

Wang, Mu-Tao

122

arXiv:1105.4207v1[math.RT]21May2011 Affine and degenerate affine BMW algebras: The center  

E-Print Network [OSTI]

arXiv:1105.4207v1[math.RT]21May2011 Affine and degenerate affine BMW algebras: The center Zajj and affine BMW algebras arise naturally in the context of Schur- Weyl duality for orthogonal and symplectic Lie algebras and quantum groups, respectively. Cyclotomic BMW algebras, affine Hecke algebras

Ram, Arun

123

arXiv:cond-mat/0305430v119May2003 Shearing or Compressing a Soft Glass in 2D: Time-concentration superposition  

E-Print Network [OSTI]

arXiv:cond-mat/0305430v119May2003 Shearing or Compressing a Soft Glass in 2D: Time dimensional monolayers should be regarded as being close to a soft glass state. PACS numbers: 68.18.-g, 83.60.bc The rheology of systems with very large surface to vol- ume ratios, such as foams or emulsions

Cicuta, Pietro

124

Comment on "Anomalous temperature dependence of the Casimir force for thin metal films" [arXiv:0712.1395  

E-Print Network [OSTI]

Recently V. A. Yampol'skii, S. Savel'ev, Z. A. Mayselis, S. S. Apostolov, and F. Nori [Phys. Rev. Lett., v.101, 096803 (2008),arXiv:0712.1395] claimed that the Casimir force between a thin metal film described by the Drude model and an ideal metal semispace can decrease with temperature whereas for bulk samples the Casimir force increases with temperature. On this basis the experimental observation of the decreasing temperature dependence of the Casimir force magnitude between a film and a bulk ideal metal was proposed. We demonstrate that, contrary to what is claimed by the authors, the magnitude of the Casimir force decreases with temperature in a wide temperature region for bulk samples described by the Drude model. This decrease is shown to be much larger than that for a thin film and it has already been experimentally excluded.

B. Geyer; G. L. Klimchitskaya; V. M. Mostepanenko

2008-10-17T23:59:59.000Z

125

arXiv:0804.3902v1[cs.DS]24Apr2008 Minimum-energy broadcast in random-grid ad-hoc  

E-Print Network [OSTI]

arXiv:0804.3902v1[cs.DS]24Apr2008 Minimum-energy broadcast in random-grid ad-hoc networks ranges to the nodes of an ad-hoc network in order to guarantee a directed spanning tree from a given in ad-hoc networks. In ad-hoc net- works, nodes are able to vary their transmission ranges in order

Rossi, Gianluca

126

arXiv:1007.3122v2[q-bio.NC]30Jan2013 Robust Short-Term Memory without Synaptic  

E-Print Network [OSTI]

been stored in samuel.johnson@imperial.ac.uk 1 #12;our brains previously (not very credible). Here wearXiv:1007.3122v2[q-bio.NC]30Jan2013 Robust Short-Term Memory without Synaptic Learning Samuel Johnson1,2, , J. Marro3 , and Joaqu´in J. Torres3 1 Department of Mathematics, Imperial College London, SW

Johnson, Samuel

127

arXiv:1408.2487v2[physics.ao-ph]22Aug2014 Ising model for melt ponds on Arctic sea ice  

E-Print Network [OSTI]

arXiv:1408.2487v2[physics.ao-ph]22Aug2014 Ising model for melt ponds on Arctic sea ice Yi-Ping Ma,1, USA The albedo of melting Arctic sea ice, a key parameter in climate modeling, is determined by pools of water on the ice surface. Recent observations show an onset of pond complexity at a critical area

Golden, Kenneth M.

128

arXiv:hep-ph/0105014v217May2001 A Light Higgs Boson Explanation for the g -2 Crisis a  

E-Print Network [OSTI]

arXiv:hep-ph/0105014v217May2001 A Light Higgs Boson Explanation for the g - 2 Crisis a A. Dedes1-even Higgs boson with a mass of around 10 GeV could explain the recent BNL measurement of the muon anomalous) the Upsilon mass. It may be possible to exclude or discover such a Higgs boson by fully analyzing the existing

California at Santa Cruz, University of

129

arXiv:0912.3495v1[hep-ph]17Dec2009 IPPP/09/97, DCTP/09/194  

E-Print Network [OSTI]

arXiv:0912.3495v1[hep-ph]17Dec2009 IPPP/09/97, DCTP/09/194 Edinburgh 2009/17 SI-HEP-2009-16 December 17, 2009 Numerical Evaluation of Feynman Loop Integrals by Reduction to Tree Graphs W. Kilian1a of loop integrals which is based on the Feynman Tree Theorem. The loop integrals are replaced by phase

Siegen, Universität

130

arXiv:0802.2965v1[hep-ex]21Feb2008 Single Top Quark Production at the Fermilab Tevatron Collider  

E-Print Network [OSTI]

arXiv:0802.2965v1[hep-ex]21Feb2008 Single Top Quark Production at the Fermilab Tevatron Collider at the Fermilab Tevatron Collider are s-channel, which involve the exchange of a time-like W boson, and t be created in association with an an on-shell W boson, but this process is negligible at the Fermilab

California at Santa Cruz, University of

131

arXiv:1311.5455v1[hep-ph]21Nov2013 NLO QCD Corrections to Electroweak Higgs Boson  

E-Print Network [OSTI]

arXiv:1311.5455v1[hep-ph]21Nov2013 NLO QCD Corrections to Electroweak Higgs Boson Plus Three Jet.sjodahl@thep.lu.se The implementation of the full next-to-leading order (NLO) QCD corrections to electroweak Higgs boson plus three jet that the new particle exhibits production and decays similar to a Standard Model (SM) Higgs boson [3, 4, 5, 6

Lunds Universitet,

132

arXiv:1205.5608v1[hep-ex]25May2012 Search for Neutrinoless Double-Beta Decay in 136  

E-Print Network [OSTI]

arXiv:1205.5608v1[hep-ex]25May2012 Search for Neutrinoless Double-Beta Decay in 136 Xe with EXO-200: May 28, 2012) We report on a search for neutrinoless double-beta decay of 136 Xe with EXO-200 in the ±1 region of interest. This sets a lower limit on the half-life of the neutrinoless double-beta decay

Gratta, Giorgio

133

arXiv:0710.1988v1[hep-lat]10Oct2007 Deflated BiCGStab for linear equations in QCD  

E-Print Network [OSTI]

arXiv:0710.1988v1[hep-lat]10Oct2007 Deflated BiCGStab for linear equations in QCD problems Abdou M. Abdel-Rehim Department of Physics, Baylor University, Waco, TX 76798-7316, USA. E-mail: Abdou-NonCommercial-ShareAlike Licence. http://pos.sissa.it/ #12;Deflated BiCGStab for linear equations in QCD problems Abdou M. Abdel

Morgan, Ron

134

Note on: Considering the Case for Biodiversity Cycles: Reexamining the Evidence for Periodicity in the Fossil Record, by Lieberman and Melott, arXiv preprint 0704.2896  

E-Print Network [OSTI]

Lieberman and Melott built their recent arXiv preprint 0704.2896 on my published paper and (a preprint of) a subsequent comment by Liebermans associate Cornette. But had this group waited for the Cornette comment to actually appear in print together with the expected Reply, they would have learned that his comment exposes Cornettes confusion that likely was due to journal misprint of my figure. Thus 0704.2896 is baseless. Despite receiving the extended Reply with Errata, these authors still fail to recognize that detrending of paleontological records-which they erroneously promote as a must-is an arbitrary rather than a universal operation.

Omerbashich, M

2007-01-01T23:59:59.000Z

135

Note on: Considering the Case for Biodiversity Cycles: Reexamining the Evidence for Periodicity in the Fossil Record, by Lieberman and Melott, arXiv preprint 0704.2896  

E-Print Network [OSTI]

Lieberman and Melott built their recent arXiv preprint 0704.2896 on my published paper and (a preprint of) a subsequent comment by Liebermans associate Cornette. But had this group waited for the Cornette comment to actually appear in print together with the expected Reply, they would have learned that his comment exposes Cornettes confusion that likely was due to journal misprint of my figure. Thus 0704.2896 is baseless. Despite receiving the extended Reply with Errata, these authors still fail to recognize that detrending of paleontological records-which they erroneously promote as a must-is an arbitrary rather than a universal operation.

M. Omerbashich

2007-06-09T23:59:59.000Z

136

arXiv:1102.3798v1[cond-mat.mes-hall]18Feb2011 Graphene on the carbon face of SiC: electronic structure modification by hydrogen  

E-Print Network [OSTI]

arXiv:1102.3798v1[cond-mat.mes-hall]18Feb2011 Graphene on the carbon face of SiC: electronic that the first C layer on the SiC(0001)(22)C surface already exhibits graphene- like electronic structure transfer mechanism. Here, we study the effects of interface mod- ifications on the graphene layer using

Paris-Sud XI, Universit de

137

Reply to Comment [arXiv:0810.3244v1] by R.S. Decca et al. on "Contribution of drifting carriers to the Casimir-Lifshitz and Casimir-Polder interactions with semiconductor materials"  

E-Print Network [OSTI]

We show that the claims expressed in the Comment arXiv:0810.3244v1 by R.S. Decca et al against our paper, D.A.R. Dalvit and S.K. Lamoreaux, Phys. Rev. Lett. {\\bf 101}, 163203 (2008), are wrong and manifestly inconsistent with basic principles of statistical physics.

Diego A. R. Dalvit; Steve K. Lamoreaux

2008-12-05T23:59:59.000Z

138

Some notes on beam dynamics due to vertical oscillations in an all-electric storage ring  

E-Print Network [OSTI]

A document has recently been posted on the arXiv [1], describing analytical formulas and results of particle tracking simulations, for precision tests of numerical integration algorithms for an EDM (electric dipole moment) storage ring. In the context of an all-electric storage ring, the authors cite theoretical formulas by Orlov [2]. However, the reference to Orlov is to a talk at a workshop in 2012, and is unpublished and difficult for independent researchers to access and validate. This note rederives and generalizes some of Orlov's principal results, using a Hamiltonian formalism, and also corrects some details in both Orlov's note [2] and the arXiv post [1].

Mane, S R

2015-01-01T23:59:59.000Z

139

arXiv:0902.1638v1[cond-mat.mtrl-sci]10Feb2009 Graphene on the C-terminated SiC (000 1) surface: An ab initio F.Varchon,1  

E-Print Network [OSTI]

arXiv:0902.1638v1[cond-mat.mtrl-sci]10Feb2009 Graphene on the C-terminated SiC (000 1) surface and electronic structures of a graphene layer on top of the (2 2) reconstruction of the SiC (0001) surface characteristic of graphene. A small graphene-substrate interaction remains in agreement with scanning tunneling

Paris-Sud XI, Universit de

140

May 19-21, 2010 Marrakech, Morocco.  

E-Print Network [OSTI]

welding of aluminum alloy 6056 Niel Aurelie, Fras Gilles ,Deschaux-Beaume Frederic ,Bordreuil Cyril, such as hot tearing. This study focuses on the analysis of hot tearing in TIG welding on a 6056 aluminum alloy components in many manufacturing industries, such as aeronautic, construction, energy and automotive

Boyer, Edmond

Note: This page contains sample records for the topic "xiv-1 xiv morocco" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


141

Casablanca, Morocco: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

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 on Office of InspectorConcentrating SolarElectricEnergyCTBarreis aCallahanWind Farm Jump to: navigation,Carsten

142

Morocco 1995 Al Akhawayn University, located in Ifrane, Morocco, opened its doors in January, 1995 to  

E-Print Network [OSTI]

is told that it is a simple matter of calling Royal Air Maroc (the Moroccan national airline) in New York, Delta does not know John from Adam! Back with Royal Air Maroc, John discovers that there is a prepaid. Perhaps Royal Air Maroc booked you with Northwest instead.'', the voice on the line states. ``That stupid

Paxton, John

143

PHYSIKALISCHE ZEITSCHRIFT ; T. XIV ; 1913.  

E-Print Network [OSTI]

expliquer les dperditions observes ces altitudes est de 9 J 23 fois suprieure celle dtermine la'nergie dans le spectre, se sert d'une quation ana- logue celle que Debye applique aux corps solides. Il libres dans les mtaux (diffrence de potentiel au contact, effet Peltier, effet Thom- son aux hautes et

Paris-Sud XI, Universit de

144

PHYSIKALISCHE ZEITSCHRIFT; T. XIV; 1913.  

E-Print Network [OSTI]

faites en plein air, le soufre constitue un isolant prfrable l'ambre et l'bonite. On obtient un. Comme pile de charge, G.-C. Simpson se sert d'une batterie d'lments Daniell qu'il a modifis d du sulfate de cuivre dans le sulfate de zinc. Les lectrodes (fils de zinc et de cuivre) plongent

Paris-Sud XI, Universit de

145

Helminthosporium spiciferum, foliar parasite of rice in Morocco  

E-Print Network [OSTI]

; Helminthosporium spiciferum, parasite des feuilles de riz au Maroc. Dans cette étude, le pouvoir pathogène de deux- dies du riz au Maroc. Cas de la pyriculariose dueà P oryzae. Thèse de docteur de troisième cycle, fa) Contributionà l'étude de l'Helminthosporiiose du riz au Maroc due à l'Helminthosporium oryzae. Thèse de 3e cycle

Boyer, Edmond

146

DETERMINANTS OF PRODUCTIVITY IN MOROCCO THE ROLE OF TRADE?  

E-Print Network [OSTI]

of the Southern Mediterranean have been engaged in a process of integration and trade liberalisation to include both EU-Med liberalisation as well as integration between the Mediterranean partners themselves liberalisation on firms and sectors. In particular, the aim was to focus on understanding of the determinants

Sussex, University of

147

ORISE: Radiation Emergency Training for Iraq, South Africa and Morocco  

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:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May JunDatastreamsmmcrcalgovInstrumentsrucLas Conchas recoveryLaboratory |CHEMPACK MappingHistoryMedicalInternational Training REAC/TS

148

Morocco-GTZ Promotion of EERE | Open Energy Information  

Open Energy Info (EERE)

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 on Office of InspectorConcentrating Solar Powerstories onFocus Area EnergyMohawk MunicipalMontvale,GTZ Partner Ministry of

149

Morocco-UNEP Green Economy Advisory Services | Open Energy Information  

Open Energy Info (EERE)

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 on Office of InspectorConcentrating Solar Powerstories onFocus Area EnergyMohawk MunicipalMontvale,GTZ Partner

150

Morocco-UNEP Risoe Technology Needs Assessment Program | Open Energy  

Open Energy Info (EERE)

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 on Office of InspectorConcentrating Solar Powerstories onFocus Area EnergyMohawk MunicipalMontvale,GTZ

151

Morocco-NREL Energy Activities | Open Energy Information  

Open Energy Info (EERE)

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 CenterFranconia, Virginia: Energy Resources Jump to:46 -Energieprojekte3 Climate ZoneMontrose,Stanley Capital Grp IncMoro,

152

Morocco-Clean Technology Fund (CTF) | Open Energy Information  

Open Energy Info (EERE)

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 Home5b9fcbce19 No revision hasInformation Earth's HeatMexico: EnergyMithun Jump to:Moe WindMontMoraine II Wind Farm Jump

153

Morocco-Facilitating Implementation and Readiness for Mitigation (FIRM) |  

Open Energy Info (EERE)

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 Home5b9fcbce19 No revision hasInformation Earth's HeatMexico: EnergyMithun Jump to:Moe WindMontMoraine II Wind Farm

154

Religiosity, Freedom of Expression and Lebanon and Morocco  

E-Print Network [OSTI]

history of existence, than some modern Western democratic nations. Furthermore, as recent14 - ?4 Bellin, 139-141. 8 Samuel P. Huntington, "The Clash of Civilizations?, Foreign Affairs (1993): 22-49.9 Abdou Filali-Ansary, Muslims and Democracy..., Journal of Democracy 10, no. 3 (1999): 18, 19. 10 Ibid., 19.11 Ibid., 20-22.12 This list is cited directly from Abdou Filali-Ansarys, (1999), Muslims and Democracy.13 Both Greece and Portugal, both of which have been under military rule as recent...

Byers III, Ward

2014-05-31T23:59:59.000Z

155

Comments on the report "Indications of anomalous heat energy production in a reactor device containing hydrogen loaded nickel powder" [arXiv:1305.3913] by G.Levi, E.Foschi, T.Hartman, B.Histad, R.Pettersson, L.Tegnr, H.Essn  

E-Print Network [OSTI]

In a recent report titled "Indications of anomalous heat energy production in a reactor device containing hydrogen loaded nickel powder" and published on arXiv, G. Levi and co-workers put forth several claims concerning the operations and performance of the so-called E-Cat of inventor Andrea Rossi. We note first of all that the circumstances and people involved in the test make it far from being an independent one. We examine the claims put forth by the authors and note that in many cases they are not supported by the facts given in the report. We present results from thermal calculations showing that alternative explanations are possible were the authors seem to jump to conclusions fitting pre-conceived ideas. In general we find that much attention is drawn to trivialities, while important pieces of information and investigation are lacking and seem not to have been conducted or considered. We also note that the proposed claims would require new physics in not only one but several areas. Besides a cold-fusion like process without production of any radiation also extreme new material properties would be needed to explain what rather seems to be a problem of correct measurement. Therefore, it is clear to us that a truly independent and scientific investigation of the so called E-Cat device, convincingly demonstrating an "anomalous heat energy production" has not been presented in the arXiv report and is thus, to-date, still lacking.

Gran Ericsson; Stephan Pomp

2013-09-17T23:59:59.000Z

156

List of Tables page xiii Preface xiv  

E-Print Network [OSTI]

a Mass-Losing Star 49 Further Reading 50 Problems 50 3 Solar Heating and Energy Transport 56 3.1 Energy Properties and Lifetimes 16 1.4 Formation of the Solar System 18 Further Reading 19 Problems 20 2 Dynamics 22 to the Second Edition xv Color Plates between pages xvi and 1 1 Introduction 1 1.1 Inventory of the Solar System

Militzer, Burkhard

157

DESY 05137 arXiv:physics/0508046  

E-Print Network [OSTI]

may result in achieving shorter radiation wavelengths for the same electron beam energy. This paper on the source part of the wave equation. Moreover, we #12;nd that such part of the wave equation is presented #12; 1 Introduction In a Free-Electron Laser the electromagnetic #12;eld at the fundamental har- monic

158

Revised Version arXiv:physics/0507002  

E-Print Network [OSTI]

and linearity of a polycrystalline diamond response were done for the diamond-tungsten option. For the heavyCal is a diamond-tungsten sandwich calorimeter. Polycrystalline Chemical Vapour Deposition (pCVD) diamonds have. Sim- ulation studies of the performance have been done for a diamond-tungsten sandwich calorimeter

159

Chapter XIV A Framework for Understanding  

E-Print Network [OSTI]

be surprised? Is this a major, self-sustaining phenomenon?Thischapterproposesaframework for understanding

Dascalu, Sergiu

160

DESY 05032 arXiv:physics/0502120  

E-Print Network [OSTI]

components of the electric #12;eld vector. Calculations of Synchrotron Radiation properties performed Radiation theory Gianluca Geloni, Evgeni Saldin, Evgeni Schneidmiller and Mikhail Yurkov Deutsches's functions in Synchrotron Radiation theory Gianluca Geloni, #3; Evgeni Saldin, Evgeni Schneidmiller

Note: This page contains sample records for the topic "xiv-1 xiv morocco" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


161

arXiv:hepex/0212067 Search for  

E-Print Network [OSTI]

, Kyoto 606-8502, Japan l Physics Division, P-23, Los Alamos National Laboratory, Los Alamos, NM 87544 Department of Physics, University of Maryland, College Park, MD 20742, USA o Department of Physics

Tokyo, University of

162

arXiv:hepex/0101056 LCPHSM2001060  

E-Print Network [OSTI]

of the production of a light Higgs boson with a mass between 120 and 160 GeV in photon­photon collisions included. It is shown that the two­photon width of the Higgs boson can be measured with high statistical \\Gamma1 . From this result the total Higgs boson width can be derived in a model independent way. Key

163

Comments on the report "Indications of anomalous heat energy production in a reactor device containing hydrogen loaded nickel powder" [arXiv:1305.3913] by G.Levi, E.Foschi, T.Hartman, B.H\\"oistad, R.Pettersson, L.Tegn\\'er, H.Ess\\'en  

E-Print Network [OSTI]

In a recent report titled "Indications of anomalous heat energy production in a reactor device containing hydrogen loaded nickel powder" [arXiv:1305.3913], G. Levi and co-workers put forth several claims concerning the operations and performance of the so-called E-Cat of Andrea Rossi. We note first of all that the circumstances and people involved in the test make if far from being an independent one. We examine the claims put forth by the authors and note that in many cases they are not supported by the facts given in the report. The authors seem to jump to conclusions fitting pre-conceived ideas where alternative explanations are possible. In general we find that much attention is drawn to trivialities while important pieces of information and investigation are lacking and seem not to have been conducted or considered. These are characteristics more typically found in pseudo-scientific texts and have no place in a technical/scientific report on this level. We also note that the proposed claims would require...

Ericsson, Gran

2013-01-01T23:59:59.000Z

164

Contrasted morphosedimentary activity of the lower Kert River (northeastern Morocco) during the Late Pleistocene and the  

E-Print Network [OSTI]

, six alluvial units (UF1 to UF6) deposited since about 30,000 years BP have been identified, comprising basse vallée du Kert et 16 datations 14 C ont permis d'identifier six unités alluviales (UF1 à UF6

Paris-Sud XI, Université de

165

The Idealized Nation-State, Globalization, Critical Geopolitics and the Case of Morocco  

E-Print Network [OSTI]

The Moroccan nation-state is a taken-for-granted geopolitical entity that is represented by the Moroccan government and the core of the world system in ways that are consonant with their visions of reality. The primary ...

Struckman, Luke

2009-01-01T23:59:59.000Z

166

E-Print Network 3.0 - arab jamahiriya morocco Sample Search Results  

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

2004. SOLAR RADIATION CLIMATE IN AFRICA Summary: -1990 No Index ESRA 28752875 (Egypt) 28.75 28.75 1981-1990 No Index ESRA29001800 (Libyan Arab Jamahiriya) 29 18......

167

Morocco-Enhancing Low-carbon Development by Greening the Economy: Policy  

Open Energy Info (EERE)

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 on Office of InspectorConcentrating Solar Powerstories onFocus Area EnergyMohawk MunicipalMontvale,

168

Morocco-Low Carbon Development Planning in the Power Sector | Open Energy  

Open Energy Info (EERE)

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 on Office of InspectorConcentrating Solar Powerstories onFocus Area EnergyMohawk MunicipalMontvale,GTZ Partner Ministry

169

Morocco-Joint Programme on Resource Efficient and Cleaner Production (RECP)  

Open Energy Info (EERE)

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 CenterFranconia, Virginia: Energy Resources Jump to:46 -Energieprojekte3 Climate ZoneMontrose,Stanley Capital Grp IncMoro, Oregon:in

170

Morocco-EU-UNDP Low Emission Capacity Building Programme (LECBP) | Open  

Open Energy Info (EERE)

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 Home5b9fcbce19 No revision hasInformation Earth's HeatMexico: EnergyMithun Jump to:Moe WindMontMoraine II Wind Farm JumpEnergy

171

Morocco-The World Bank Partnership for Market Readiness (PMR) | Open Energy  

Open Energy Info (EERE)

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 Home5b9fcbce19 No revision hasInformation Earth's HeatMexico: EnergyMithun Jump to:Moe WindMontMoraine II Wind

172

World Bank-Morocco Study on the Impact of Climate Change on the  

Open Energy Info (EERE)

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 Home5b9fcbce19 NoPublic Utilities Address: 160 East 300 South Place:ReferenceEditWisconsin: Energy ResourcesToolkit

173

Long-term drought severity variations in Morocco Jan Esper,1  

E-Print Network [OSTI]

-term temperature changes, potentially teleconnected with ENSO variability and forced by solar irradiance changes current conditions in the context of the past millennium [Treydte et al., 2006; Cook et al., 2004; Cook et al., 2002], and allowed spatial patterns of moisture anomalies over the past 150 years

174

The Place of Feminism in Religious Revival: Islam, Feminist Groups, and Changing Public Policy in Morocco  

E-Print Network [OSTI]

abortion can only be performed to save a womans life or to preserve her physical and mental health.

2010-01-01T23:59:59.000Z

175

List of Tables xiv List of Figures xvi  

E-Print Network [OSTI]

: Food, Soil, Water, Air, Free Speech 99 5.1 The "Hour Glass" Industrial Agriculture Machine . . . . . . . . . . . . . . . . . . . . . . . . . . . 146 6 Mathematics and Energy 151 6.1 How Much Solar Energy is There? . . . . . . . . . . . . . . . 151 6.2 Solar Energy is There, Do We Know How to Get It? . . . . 154 6.3 Four Falsehoods

Russo, Bernard

176

arXiv:astroph/0208546 Flare Heating in Stellar Coronae  

E-Print Network [OSTI]

J. Drake Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 vkashyap@astro.phys.ethz.ch ABSTRACT An open question in the #12;eld of solar and stellar astrophysics is the source of heating, but are more numerous. Previous analyses of ares in light-curves of active stars have shown that this index

Guedel, Manuel

177

2009 Site environmental report xiv the environmental Protection division field  

E-Print Network [OSTI]

(From left to right) Richard Lagattolla, Robert Metz, and James Milligan (Lawrence Lettieri not pictured) the environmental Information management system group (Front row, left to right) Brian Foley, Susan Young, John Richard Lagattolla Lawrence Lettieri Robert Metz James Milligan Glen Todzia Frank Tramontano biology

178

arXiv:hepph/0101093 IMSc/2001/01/01  

E-Print Network [OSTI]

: Comparison of signatures in water and heavy water detectors G. Dutta, Harish-Chandra Research Institute signals from stellar collapse in heavy water detectors are contrasted with those in water detectors solar, atmospheric and laboratory neutrino experiments. Signals at a heavy water detector, espe- cially

Indumathi, D.

179

DESY 09094 arXiv:0906.5160v1  

E-Print Network [OSTI]

on transversely polarized protons A. Airapetian, 12, 15 N. Akopov, 26 Z. Akopov, 26 E.C. Aschenauer, 6 W

180

Revised Version DESY 05205 arXiv:hepex/0510030  

E-Print Network [OSTI]

-hadron leptoproduction in the nuclear medium A. Airapetian, 16 N. Akopov, 27 Z. Akopov, 27 M. Amarian, 7,27 A. Andrus, 15

Note: This page contains sample records for the topic "xiv-1 xiv morocco" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


181

Revised Version DESY 06142 arXiv:hepex/0609039  

E-Print Network [OSTI]

, 16 N. Akopov, 27 Z. Akopov, 27 A. Andrus, 15 E.C. Aschenauer, 7 W. Augustyniak, 26 R. Avakian, 27 A

182

DESY 09082 arXiv:0906.2478v1  

E-Print Network [OSTI]

of hadrons produced in semi-inclusive deep-inelastic scattering on nuclei. A. Airapetian, 12, 15 N. Akopov, 26 Z. Akopov, 5 E.C. Aschenauer, 6 W. Augustyniak, 25 A. Avetissian, 26 E. Avetisyan, 5 B. Ball, 15 S

183

DESY 07050 arXiv:0704.3270v1  

E-Print Network [OSTI]

-inelastic scattering on nuclei A. Airapetian p , N. Akopov aa , Z. Akopov aa , E.C. Aschenauer g , W. Augustyniak z , R

184

Revised Version DESY05072 arXiv:hepex/0505042  

E-Print Network [OSTI]

polarized hydrogen target A. Airapetian, 18 N. Akopov, 30 Z. Akopov, 30 M. Amarian, 8,30 A. Andrus, 16 E

185

DESY 09143 arXiv:0909.3587v1  

E-Print Network [OSTI]

. Keywords: Lepton-Nucleon Scattering. #12; The HERMES Collaboration A. Airapetian 12;15 , N. Akopov 26 , Z. Akopov 5 , E.C. Aschenauer 6;a , W. Augustyniak 25 , R. Avakian 26 , A. Avetissian 26 , E. Avetisyan 5

186

DESY 09106 arXiv:0907.2596v1  

E-Print Network [OSTI]

. Akopov, 26 Z. Akopov, 5 E.C. Aschenauer, 6 W. Augustyniak, 25 A. Avetissian, 26 E. Avetisyan, 5 B. Ball

187

DESY 09190 arXiv:0911.0091v1  

E-Print Network [OSTI]

. Akopov, 26 Z. Akopov, 5 M. Amarian, 6, 27 E.C. Aschenauer, 6, 28 W. Augustyniak, 25 R. Avakian, 26 A

188

Revised Version arXiv:hepex/0605108v3  

E-Print Network [OSTI]

Asymmetry and Deeply Virtual Compton Scattering A. Airapetian, 17 N. Akopov, 29 Z. Akopov, 29 M. Amarian, 8

189

DESY 06227 arXiv:hepex/0612059v1  

E-Print Network [OSTI]

in the Azimuthal Distribution of Pion Electroproduction A. Airapetian, 16 Z. Akopov, 27 M. Amarian, 7, 27 A. Andrus

190

Revised Version DESY06100 arXiv:hepex/0607004  

E-Print Network [OSTI]

Transfer to the #3; Hyperon in Semi-Inclusive Deep-Inelastic Scattering A. Airapetian, 17 N. Akopov, 30 Z. Akopov, 30 M. Amarian, 8,30 A. Andrus, 16 E.C. Aschenauer, 8 W. Augustyniak, 29 R. Avakian, 30 A

191

3040 -XIV Encuentro de Latinoamericanistas Espaoles AUMENTO DE LA PRODUCTIVIDAD  

E-Print Network [OSTI]

televisiones en blanco-y- negro. Sin embargo, últimamente, podemos encontrar televisores de HD, Digital y 3D televisores chinos son una gran amenaza para los productores en México. El mercado principal de ambos es

Paris-Sud XI, Université de

192

1734 -XIV Encuentro de Latinoamericanistas Espaoles JUSTICIA Y CONFLICTO EN  

E-Print Network [OSTI]

Autodefensas Unidas de Colombia (AUC), para lo cual, el 12 de noviembre de 2002, el entonces comisionado de paz las autodefensas1 . LahistoriadeColombiasehavistomarcadaporguerrasynegociaciones de paz, signadas

Paris-Sud XI, Universit de

193

arXiv:astroph/0308017 Draft version August 1, 2003  

E-Print Network [OSTI]

LETGS observation on 19 March 2003. By this time, it had evolved into the Super Soft X-ray phase during the decay. Strong H-like and He-like lines of oxygen, nitrogen, and carbon were found.O. Box 1312, D-85741 Garching, Germany: burwitz@mpe.mpg.de 4 Harvard-Smithsonian Center for Astrophysics

Ness, Jan-Uwe

194

DESY 07015 arXiv:hepph/0702134v1  

E-Print Network [OSTI]

Institute for Nuclear Studies, Warsaw, Poland Abstract We study pp and p#22;p collisions which lead to the exclusive production of J= or #7; from the pomeron{odderon and the pomeron{photon fusion. We calculate of the phenomenological and theoretical status of the odderon we refer the reader to Ref. [12]. In the present paper, we

195

2278 -XIV Encuentro de Latinoamericanistas Espaoles POLTICA EXTERIOR COMO  

E-Print Network [OSTI]

internacionais. E foi nos governos de Fernando Henrique Cardoso (1995 a 2002) e de Luiz Incio Lula da Silva governo Cardoso. Em terceiro lugar, ser feita uma anlise da questo da poltica externa no governo Lula atravs de comparaes com o governo anterior. E, por ltimo, o artigo analisar qualitativamente um caso

Boyer, Edmond

196

Revised Version DESY05077 arXiv:hepex/0506018  

E-Print Network [OSTI]

.G. Vincter, 1 C. Vogel, 10 M. Vogt, 10 J. Volmer, 8 C. Weiskopf, 10 J. Wendland, 26,27 J. Wilbert, 10 Y. Ye Laboratory, University of Colorado, Boulder, Colorado 80309-0390, USA 7 DESY, 22603 Hamburg, Germany 8 DESY

197

DESY 07036 arXiv:0704.3133v1  

E-Print Network [OSTI]

.G. Vincter, 1 J. Visser, 22 M. Vogt, 8 J. Volmer, 6 C. Weiskopf, 8 J. Wendland, 27, 28 J. Wilbert, 8 T. Wise Nucleare, Sezione di Bari, 70124 Bari, Italy 4 Nuclear Physics Laboratory, University of Colorado, Boulder, Colorado 80309-0390, USA 5 DESY, 22603 Hamburg, Germany 6 DESY, 15738 Zeuthen, Germany 7 Joint Institute

198

arXiv:hepph/0508178 CLNS 05/1922  

E-Print Network [OSTI]

b;c , and Gil Paz b a Center for Theoretical Physics, Massachusetts Institute of Technologyat Heidelberg Philosophenweg 16, D{69120 Heidelberg, Germany Abstract A shape-function independent relation of order #11; 2 s (m b ). Power corrections from phase-space factors are included exactly, while

199

arXiv:hepex/0305080 CLNS 03/1830  

E-Print Network [OSTI]

model uncertainties originating from the form-factor shapes needed to simulate the signal and cross-feed #12;t components 8 . We emphasize that theoretical form factors do not constrain the relative rates fractions listed in Tab. 1 residual theoretical form-factor uncertainties of [

200

Viva Tenaz!: El XIV Festival Internacional de Teatro Chicano Latino  

E-Print Network [OSTI]

); Teatro Bilinge de Houston; Teatro Espejo (Sacramento, California); y el artista solitario Edgard Guillen (Lima, Per). Tambin presentes en lo que ya es el nico festival de teatro latino popular de EE.UU. haba representantes de la Coalicin de... todas las obras se combinaba el espaol con el ingls, incorporando orgnicamente el modo de expresin predominante de la comunidad chicana latina de EE.UU. Los Actores de San Antonio inauguraron el Festival con Roosters es Mucha Snchez...

Frischmann, Donald H.

1990-04-01T23:59:59.000Z

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201

DESY 06214 arXiv:hepex/0612024v1  

E-Print Network [OSTI]

. Pleier 13 , M. Poli 6;31 , V. Popov 22 , D. Pose 11;14 , S. Prystupa 16 , V. Pugatch 16 , Y. Pylypchenko

202

Planck 2015 results. XIV. Dark energy and modified gravity  

E-Print Network [OSTI]

We study the implications of Planck data for models of dark energy (DE) and modified gravity (MG), beyond the cosmological constant scenario. We start with cases where the DE only directly affects the background evolution, considering Taylor expansions of the equation of state, principal component analysis and parameterizations related to the potential of a minimally coupled DE scalar field. When estimating the density of DE at early times, we significantly improve present constraints. We then move to general parameterizations of the DE or MG perturbations that encompass both effective field theories and the phenomenology of gravitational potentials in MG models. Lastly, we test a range of specific models, such as k-essence, f(R) theories and coupled DE. In addition to the latest Planck data, for our main analyses we use baryonic acoustic oscillations, type-Ia supernovae and local measurements of the Hubble constant. We further show the impact of measurements of the cosmological perturbations, such as redshif...

Ade, P A R; Arnaud, M; Ashdown, M; Aumont, J; Baccigalupi, C; Banday, A J; Barreiro, R B; Bartolo, N; Battaner, E; Battye, R; Benabed, K; Benot, A; Benoit-Lvy, A; Bernard, J -P; Bersanelli, M; Bielewicz, P; Bonaldi, A; Bonavera, L; Bond, J R; Borrill, J; Bouchet, F R; Bucher, M; Burigana, C; Butler, R C; Calabrese, E; Cardoso, J -F; Catalano, A; Challinor, A; Chamballu, A; Chiang, H C; Christensen, P R; Church, S; Clements, D L; Colombi, S; Colombo, L P L; Combet, C; Couchot, F; Coulais, A; Crill, B P; Curto, A; Cuttaia, F; Danese, L; Davies, R D; Davis, R J; de Bernardis, P; de Rosa, A; de Zotti, G; Delabrouille, J; Dsert, F -X; Diego, J M; Dole, H; Donzelli, S; Dor, O; Douspis, M; Ducout, A; Dupac, X; Efstathiou, G; Elsner, F; Enlin, T A; Eriksen, H K; Fergusson, J; Finelli, F; Forni, O; Frailis, M; Fraisse, A A; Franceschi, E; Frejsel, A; Galeotta, S; Galli, S; Ganga, K; Giard, M; Giraud-Hraud, Y; Gjerlw, E; Gonzlez-Nuevo, J; Grski, K M; Gratton, S; Gregorio, A; Gruppuso, A; Gudmundsson, J E; Hansen, F K; Hanson, D; Harrison, D L; Heavens, A; Helou, G; Henrot-Versill, S; Hernndez-Monteagudo, C; Herranz, D; Hildebrandt, S R; Hivon, E; Hobson, M; Holmes, W A; Hornstrup, A; Hovest, W; Huang, Z; Huffenberger, K M; Hurier, G; Jaffe, A H; Jaffe, T R; Jones, W C; Juvela, M; Keihnen, E; Keskitalo, R; Kisner, T S; Knoche, J; Kunz, M; Kurki-Suonio, H; Lagache, G; Lhteenmki, A; Lamarre, J -M; Lasenby, A; Lattanzi, M; Lawrence, C R; Leonardi, R; Lesgourgues, J; Levrier, F; Lewis, A; Liguori, M; Lilje, P B; Linden-Vrnle, M; Lpez-Caniego, M; Lubin, P M; Ma, Y -Z; Macas-Prez, J F; Maggio, G; Mandolesi, N; Mangilli, A; Marchini, A; Martin, P G; Martinelli, M; Martnez-Gonzlez, E; Masi, S; Matarrese, S; Mazzotta, P; McGehee, P; Meinhold, P R; Melchiorri, A; Mendes, L; Mennella, A; Migliaccio, M; Mitra, S; Miville-Deschnes, M -A; Moneti, A; Montier, L; Morgante, G; Mortlock, D; Moss, A; Munshi, D; Murphy, J A; Narimani, A; Naselsky, P; Nati, F; Natoli, P; Netterfield, C B; Nrgaard-Nielsen, H U; Noviello, F; Novikov, D; Novikov, I; Oxborrow, C A; Paci, F; Pagano, L; Pajot, F; Paoletti, D; Pasian, F; Patanchon, G; Pearson, T J; Perdereau, O; Perotto, L; Perrotta, F; Pettorino, V; Piacentini, F; Piat, M; Pierpaoli, E; Pietrobon, D; Plaszczynski, S; Pointecouteau, E; Polenta, G; Popa, L; Pratt, G W; Przeau, G; Prunet, S; Puget, J -L; Rachen, J P; Reach, W T; Rebolo, R; Reinecke, M; Remazeilles, M; Renault, C; Renzi, A; Ristorcelli, I; Rocha, G; Rosset, C; Rossetti, M; Roudier, G; Rowan-Robinson, M; Rubio-Martn, J A; Rusholme, B; Salvatelli, V; Sandri, M; Santos, D; Savelainen, M; Savini, G; Schaefer, B M; Scott, D; Seiffert, M D; Shellard, E P S; Spencer, L D; Stolyarov, V; Stompor, R; Sudiwala, R; Sunyaev, R; Sutton, D; Suur-Uski, A -S; Sygnet, J -F; Tauber, J A; Terenzi, L; Toffolatti, L; Tomasi, M; Tristram, M; Tucci, M; Tuovinen, J; Valenziano, L; Valiviita, J; Van Tent, B; Viel, M; Vielva, P; Villa, F; Wade, L A; Wandelt, B D; Wehus, I K; White, M; Yvon, D; Zacchei, A; Zonca, A

2015-01-01T23:59:59.000Z

203

DESY07202 arXiv:0712.2336v1  

E-Print Network [OSTI]

for the design and optimisation of particle detectors. A major example of such programs is Geant4 [2, 3], which is widely used in high energy physics, medicine, and space science. Di#11;erent parts of this tool kit can of the production mechanism of polarised positrons from photons emitted from a helical undulator is now possible

204

arXiv:hepex/9908059 DESY99107 ISSN 04189833  

E-Print Network [OSTI]

26 , V. Boudry 27 , W. Braunschweig 1 , V. Brisson 26 , H.­B. Br?oker 2 , D.P. Brown 21 , W. Br , A. Burrage 18 , G. Buschhorn 25 , D. Calvet 22 , A.J. Campbell 10 , T. Carli 25 , E. Chabert 22 , M of perturbative QCD. The proton structure function F 2 (x; Q 2 ) is determined. An extraction of the u and d quark

205

Revised Version DESY 06090 arXiv:hepph/0603173  

E-Print Network [OSTI]

to the LN violation are processes such as neutrinoless double beta decay (A; Z) ! (A; Z + 2) + e + e (for oscillations, cosmological data and searches of the neutrinoless double beta decay, we have derived

206

DESY 08055 arXiv:0805.1338v1  

E-Print Network [OSTI]

of the neutrinoless double beta decay and the leptogenesis. The prediction of the branching ratio of #22; ! e is also are Majorana particles and we expect the neutrinoless double beta decay which provides the information not only

207

Revised Version DESY 06086 arXiv:hepph/0606072  

E-Print Network [OSTI]

2006 NEUTRINOLESS DOUBLE BETA DECAY: ELECTRON ANGULAR CORRELATION AS A PROBE OF NEW PHYSICS A. Ali electrons in the so-called long range mechanism of the neutrinoless double beta decay (0-right symmetric model, taking into account current phenomenological bounds. 1 Introduction Neutrinoless double

208

arXiv:1006.3396v1 INTERNATIONALLARGEDETECTOR  

E-Print Network [OSTI]

, Saskatchewan, S4S 0A2 Canada Jason M Abernathy, Dean Karlen 1 University of Victoria, Department of Physics and Astronomy, P.O.Box 3055 Stn Csc, Victoria, BC V8W 3P6, Canada Jean­Pierre Martin Universit??e de Montr??eal, D Gif­sur­Yvette, France Jerome Baudot 6 , Auguste Besson 6

209

DESY 07054 arXiv:0704.3195v1  

E-Print Network [OSTI]

generally, such experiments, exploiting high uxes of low-energy photons and/or large electromagnetic #12 low energy incarnations, supergravity and su- persymmetry, predict new heavy, m #29; 100 Ge Telescopes", March 6-9, 2007, Venice, Italy. #12; Figure 1: Schematic illustration of the PVLAS experiment 1

210

Revised Version arXiv:0905.1894v2  

E-Print Network [OSTI]

. In the minimal model there are a single complex Higgs doublet, where the Higgs boson H is the physical neutral and neutral scalar Higgs particles. At moment, the Higgs boson is the only missing, undiscovered component of modern particle physics, so that the search for the Higgs boson is of highest 1 #12; priority

211

Structural style and evolution of a Late Triassic rift basin in the Central High Atlas, Morocco: controls on sediment deposition  

E-Print Network [OSTI]

: controls on sediment deposition CATHERINE BAUDON*, IVAN FABUEL-PEREZ and JONATHAN REDFERN* North Africa, Oxford Road, Williamson Building, Manchester M13 9PL, UK Late Triassic continental sediments deposited dimension, geometry of the half-graben and created the accommodation for sediment deposition. The presence

Demouchy, Sylvie

212

Chasing water: Diverging farmers' strategies to cope with the groundwater crisis in the coastal Chaouia region in Morocco  

E-Print Network [OSTI]

policies, whose efficiency will depend on farmers' strategies. The different strategies adopted by farmers1 Chasing water: Diverging farmers' strategies to cope with the groundwater crisis in the coastal, Meknes, France 4 National School for Agronomic Education (ENFA), Rural Dynamics Research Unit, Toulouse

Paris-Sud XI, Université de

213

Controls on the genesis of hydrothermal cobalt mineralization: insights from the mineralogy and geochemistry of the Bou Azzer deposits, Morocco  

E-Print Network [OSTI]

Controls on the genesis of hydrothermal cobalt mineralization: insights from the mineralogy,Ni,Fe) arsenides and sulpharsenides, with accessory sulphides and gold in a quartz-carbonate gangue. The ore-Ni-Fe, avec des quantités mineures de sulphures et de l'or dans une gangue de quartz- carbonate. Les minerais

214

China Energy Databook -- User Guide and Documentation, Version 7.0  

E-Print Network [OSTI]

Mexico Mongolia Morocco Mozambique Nepal Netherlands New Zealand Nicaragua Nigeria Norway Oman Pakistan Panama Coal &

Fridley, Ed., David

2008-01-01T23:59:59.000Z

215

African Alumni of ISU (ISU-AA) "Statement of Intent"  

E-Print Network [OSTI]

. Most countries in Africa: Kenya, Libya, South Africa, Morocco, Nigeria, Cameroun, Algeria and others

Glass, Ian S.

216

******** PROVISIONAL SYLLABUS SUBJECT TO MODIFICATION ******* Society and Politics of North Africa  

E-Print Network [OSTI]

"farthest west" in Arabic)--encompassing Morocco, Algeria, Tunisia, and Libya--has historically been

217

Oil and Gas CDT Prediction of flow through fractures and maximising recovery  

E-Print Network [OSTI]

fracking. Fractured carbonate formation in Morocco The project aims to tackle the problem of quantifying

Henderson, Gideon

218

Berkeley Emeriti January 2011  

E-Print Network [OSTI]

of Science and Technology in Morocco, and the Universidad Central de Venezuela, Caracas. He also served

Alvarez-Cohen, Lisa

219

Offprint Botanica Marina Vol. 44, 2001, pp. 425 460 2001 by Walter de Gruyter Berlin New York Checklist of Mediterranean Seaweeds.  

E-Print Network [OSTI]

) Libya, (Tn) Tunisia, (Ag) Algeria, (Mo) Morocco. (Gallardo et al. 1993). The Rhodophyceae) Libya, (Tn) Tunisia, (Ag) Algeria, (Mo) Morocco. This work benefited from the suggestions on tax- onomy

Boudouresque, Charles F.

220

Mapping myths of the medina : French colonial urbanism, Oriental brandscapes and the politics of tourism in Marrakesh  

E-Print Network [OSTI]

Before the French Protectorate of Morocco was established in 1912, Marrakesh was both a major trading node in North Africa and one of the royal cities in Morocco. Yet as the number of colonists surged and the pieds noirs ...

Demerdash, Nancy Nabeel Aly

2009-01-01T23:59:59.000Z

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221

PPS27, 2011, 27th World Congress of the Polymer Processing Society, May 1014, Marrakech, Morocco 1 Influence of Twin-Screw Processing Conditions  

E-Print Network [OSTI]

montmorillonite with respective mass fraction of 85/10/5 were prepared with a co-rotating twin-screw extruder Influence of Twin-Screw Processing Conditions on Structure and Properties of Polypropylene - Organoclay such as screw speed, feed rate and barrel temperature on the nanocomposite structure and its consequences

Paris-Sud XI, Université de

222

China Energy Databook - Rev. 4  

E-Print Network [OSTI]

Coal Products ( 0 Exports Imports Laos Lebanon Libya Liechtenstein Macau Malaysia Mauritius Mexico Mongolia (Outer) Morocco Mozambique Nepal Netherlands New

Sinton Editor, J.E.

2010-01-01T23:59:59.000Z

223

inpartnership international  

E-Print Network [OSTI]

. Moreover, the Les intérieurs du Maroc (Inland Morocco) semi- nar was organised in Rabat by the LMI

224

Is the beta phase maximal?  

E-Print Network [OSTI]

55, 2935 (1985). [20] M. Battaglia and L. Gibbons, [arXiv:B 592, 1 (2004). [13] M. Battaglia et al. , [arXiv:hep-

Ferrandis, Javier

2008-01-01T23:59:59.000Z

225

arXiv:hep-ex/0310019v110Oct2003 DESY03160 ISSN 04189833  

E-Print Network [OSTI]

.P.J. Landon19 , W. Lange35 , T. Lastovicka35,30 , P. Laycock18 , A. Lebedev24 , B. Lei?ner1 , R. Lemrani10 , V. Malinovski24 , S. Mangano36 , P. Marage4 , J. Marks13 , R. Marshall21 , H.-U. Martyn1 , J. Martyniak6 , S

Boyer, Edmond

226

arXiv:nucl-ex/0507026v119Jul2005 Optical calibration hardware for the Sudbury  

E-Print Network [OSTI]

in the heavy water and light water, and the angular dependence of the response of the detector to detect Che- renkov light produced by solar neutrino interactions in heavy water (D2O). The accuracy). The determination of light attenuation in the heavy and light water and the PMT response as a function of incident

Waltham, Chris

227

arXiv:gr-qc/9712019v13Dec1997 Lecture Notes on General Relativity  

E-Print Network [OSTI]

-- vectors as derivatives -- coordinate bases -- the tensor transformation law -- partial derivatives. Gravitation the Principle of Equivalence -- gravitational redshift -- gravitation as spacetime cur- vature time -- isometries and Killing vectors #12;ii 6. Weak Fields and Gravitational Radiation the weak

Carroll, Sean M.

228

arXiv:astro-ph/0309647v123Sep2003 Hydra A at Low Radio Frequencies  

E-Print Network [OSTI]

Faraday rota- tion measure (RM) and asymmetry in both the RM and depolarization between the kpc-scale jets suggest an inclination angle of 48 (Taylor & Per- ley 1993), with the northern jet lying closer to us

Taylor, Greg

229

556 -XIV Encuentro de Latinoamericanistas Espaoles LA CIUDAD DE PUEBLA DE LOS  

E-Print Network [OSTI]

alcabalas... los cambios en la administracin del azogue, pero sobre todo a la falta de trato y comercio profana, informe dado a su muy ilustre ayuntamiento el ao de 1746, Centro de Estudios Histricos de

Paris-Sud XI, Universit de

230

2600 -XIV Encuentro de Latinoamericanistas Espaoles EL DERECHO A LA CONSULTA  

E-Print Network [OSTI]

Ejecutivo para implementar el tratado de libre comercio con los Estados Unidos, sin 40. En el Informe de la treintena de personas y cuantiosos daos personales y materiales40 . Diversos informes intentan explicar sus

Boyer, Edmond

231

arXiv:hepph/0208219 nuhep-exp/02-012  

E-Print Network [OSTI]

squark parameters of MSSM Higgs boson production in two-photon colli- sions; Higgs boson decay to two to the trilinear Higgs boson coupling; charged Higgs boson pair production; and we discuss the backgrounds produced of a Standard Model-like Higgs boson of mass in the range 100{130 GeV. The properties of this Higgs boson would

232

PUBLICATIONS OF J. WILLIAM HELTON Preprints plus are available mostly from arXiv  

E-Print Network [OSTI]

matrix functions and Darlington synthesis," Acta. Sci. Math., (Szeged), 34 (1973), 6167. [HHo73] J. W), Lecture notes in Comput. Sci., Vol. 25, 164169. [HHo75] J. W. Helton and R. Howe: "Traces of commutators

Helton, J. William

233

Revised Version DESY 08203 arXiv:0901.0701v2  

E-Print Network [OSTI]

on 1 H and 2 H Targets at 27.5 GeV Beam Energy The HERMES Collaboration A. Airapetian, 16 N. Akopov, 27 Z. Akopov, 27 A. Andrus, 15 E.C. Aschenauer, 7 W. Augustyniak, 26 R. Avakian, 27 A. Avetissian, 27 E

234

arXiv:hepex/0301010 The Time-of-Flight Technique  

E-Print Network [OSTI]

. Airapetian e , N. Akopov e , M. Amarian d;e , H. Avakian b;e , A. Avetissian e , E. Avetisyan b;e , B

235

Revised Version DESY 09117 arXiv:0907.5369v3  

E-Print Network [OSTI]

-Photon Exchange Contribution to Inclusive Deep-Inelastic Scattering A. Airapetian, 12, 15 N. Akopov, 26 Z. Akopov

236

Revised Version DESY 07098 arXiv:0707.0222v2  

E-Print Network [OSTI]

for hard exclusive electroproduction of #25; + mesons on a hydrogen target A. Airapetian, 15 N. Akopov, 25 Z. Akopov, 25 E.C. Aschenauer, 6 W. Augustyniak, 24 A. Avetissian, 25 E. Avetissian, 10 L. Barion, 9

237

Revised Version DESY 07223 arXiv:0803.2993v2  

E-Print Network [OSTI]

on the Deuteron A. Airapetian, 16 N. Akopov, 27 Z. Akopov, 27 A. Andrus, 15 E.C. Aschenauer, 7 W. Augustyniak, 26

238

Revised Version DESY 07225 arXiv:0802.2499v2  

E-Print Network [OSTI]

Electroproduction of Real Photons HERMES Collaboration A. Airapetian 15 , N. Akopov 26 , Z. Akopov 26 , A. Andrus 14

239

LC-DET-2008-nnn arXiv:0711.3561  

E-Print Network [OSTI]

for studying short-lived particles. The Linear Collider Flavour Identification (LCFI) collaboration of bulk radiation damage on the CTI of a CPCCD are studied by simulating the effects of two electron trap particles. The Linear Collider Flavour Identification (LCFI) collaboration is developing Column

240

arXiv:physics/0311019v15Nov2003 Silicon Drift Detector Readout Electronics for  

E-Print Network [OSTI]

Silicon detectors. This detector type has been used for several applications such as a scintillator based gamma-camera [9], holography [10], and spectrometry [11]. Our proto

Siegen, Universitt

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241

Spring :z.ooo Volume XIV, Number 2. Nota Bene ~ News from the Yale Library  

E-Print Network [OSTI]

contexts and in the context of the history of Christianity. The EIKON Image Database for Biblical Studies database and Website, AdHoc: Resources Related to Teaching and Research on the History of Christianity Morrison, Michael Ondaatje, Salman Rushdie, and Derek Walcott. -CAS ~ The EIKON Image Database for Biblical

242

arXiv:astroph/0010129 ASP Conference Series, Vol. **VOLUME**, **PUBLICATION YEAR**  

E-Print Network [OSTI]

as a standard tool, we must observe in the vicinity of natural guide stars. But all current deep surveys of current AO systems, we have begun a sur­ vey around bright stars to study intermediate redshift galaxies.05 and at scales 1.0-- 1.5 kpc at z=1. In this contribution we present the initial results of this project, which

Baker, Andrew J.

243

arXiv:quant-ph/0302114v114Feb2003 An Introduction to Quantum Teleportation  

E-Print Network [OSTI]

Theorem, which prohibits making an exact copy of an unknown quantum state. Yet, in 1993, an international team of six scien- tists including Charles Bennett [1] demonstrated that it is possible to transmit in 1997 [2] was the cover story of many journals, includ- ing "Scientific American" [3], and even

Miranowicz, Adam

244

arXiv:hepex/0106030 SEARCHES FOR NEW PHYSICS AT HERA  

E-Print Network [OSTI]

of Particle and Nuclear Studies, KEK, Tsukuba, 305-0801 Japan (on behalf of the H1 and ZEUS Collaborations, are also investigated, including cases with lepton- avor violation. Finally, the status of events physics include: #15; Resonant states formed by electron-quark fusion. Examples of such states

245

arXiv:0711.0984v1[astro-ph]6Nov2007 **FULL TITLE**  

E-Print Network [OSTI]

. Other orbital parameters only affect the eccentricity oscillation period, Pe P2 b /Ppl (1 - e2 b)3/2 , (1) (Ford, Kozinsky & Rasio 2000) where Ppl and Pb are the orbital periods of the planet

Rasio, Frederic A.

246

arXiv:0710.2437v1[astro-ph]12Oct2007 **FULL TITLE**  

E-Print Network [OSTI]

in the Pleiades, PPl 15 (Basri & Mart´in 1999), raised hope to find many more of these systems in the following a spectroscopic orbital solution has been derived: PPl 15, the very young eclipsing system 2M0535-05 (Stassun

Joergens, Viki

247

arXiv:cond-mat/0610695v125Oct2006 EPJ manuscript No.  

E-Print Network [OSTI]

-dimensional electron gas being at a thermal equilibrium. The magnetization is proportional to a number of electrons in a dot and to a microwave power. Microwave fields of moderate strength create in a one dot of few micron at thermal equilibrium (see e.g. [4]). Thus, the persistent currents have a quantum origin and are relatively

Shepelyansky, Dima

248

arXiv:cs.CC/0508071 Every decision tree has an influential variable  

E-Print Network [OSTI]

. A deter­ ministic decision tree (DDT) for a boolean function f : f1; 1g n ! f1; 1g is a deterministic in Section 3.1). The cost of a DDT on a given input is simply the number of input variables that it reads, and the DDT complexity of a func­ tion f , D(f), is the minimum over all DDT's for f of the maximum cost

Servedio, Rocco

249

arXiv:astro-ph/0604590v127Apr2006 Draft version April 15, 2009  

E-Print Network [OSTI]

in the processing pipeline, and obtaining better empirical temperature and bolometric correction relations) are constructed for comparisons to colors from galaxies and star clusters. Color-temperature transformations are also used in spectral abundance analysis, design of observing strategies, computation of selection

Lee, Hyun-chul

250

arXiv:0911.5286v1 LU TP 09-31  

E-Print Network [OSTI]

, Sweden 1 Introduction Given the current landscape in experimental high-energy physics, these lectures, within the #12;eld of high-energy pp=pp collisions, the emphasis will be on the common aspects of QCD with an outlook on the ongoing generator- development work in section 8. Slides for these and other similar

Lunds Universitet,

251

arXiv:0902.3381v1 [math.OA] 19 Feb 2009  

E-Print Network [OSTI]

Feb 19, 2009 ... aim at introducing the classification problem for (nuclear) C?-algebras, that has been around for the last couple of ...... the modular law that.

2009-02-19T23:59:59.000Z

252

arXiv:hep-ex/0107013v16Jul2001 BABAR-PUB-01/18  

E-Print Network [OSTI]

,16 A. A. Grillo,16 M. Grothe,16 C. A. Heusch,16 R. P. Johnson,16 W. Kroeger,16 W. S. Lockman,16 T. Hitlin,17 S. Metzler,17 J. Oyang,17 A. Ryd,17 A. Samuel,17 M. Weaver,17 S. Yang,17 R. Y. Zhu,17 S. Devmal,19 P. Bloom,19 M. O. Dima,19 S. Fahey,19 W. T. Ford,19 D. R. Johnson,19 U. Nauenberg,19 A. Olivas,19

Jessop, Colin

253

arXiv:hep-th/0703137v114Mar2007 LPTENS-07/13  

E-Print Network [OSTI]

constraints in this setup is clarified. Solvay workshop "Bethe Ansatz: 75 Years Later" Brussels, Belgium-NonCommercial-ShareAlike Licence. http://pos.sissa.it/ hal-00717896,version1-13Jul2012 Author manuscript, published in "PoS Solvay

Paris-Sud XI, Université de

254

arXiv:hepth/0506098 BRST-anti eld Quantization: a Short Review  

E-Print Network [OSTI]

Physique Th#19;eorique et Math#19;ematique, Universit#19;e Libre de Bruxelles, and International Solvay

Maas, Axel

255

arXiv:hep-ph/0508178v224Oct2005 CLNS 05/1922  

E-Print Network [OSTI]

,c , and Gil Pazb a Center for Theoretical Physics, Massachusetts Institute of Technology Cambridge, MA 02139 Philosophenweg 16, D­69120 Heidelberg, Germany Abstract A shape-function independent relation is derived between is obtained up to yet unknown corrections of order 2 s(mb). Power corrections from phase-space factors

256

arXiv:1302.1260v1 [math-ph] 6 Feb 2013  

E-Print Network [OSTI]

Feb 6, 2013 ... the gyroid as well as related cases, such as graphene. ... that this analysis will contribute to understanding of potential applications of gyroid-.

2013-02-07T23:59:59.000Z

257

arXiv:cond-mat/0508028v131Jul2005 A generative model for feedback networks  

E-Print Network [OSTI]

model for constructing net- works that grow via competition between cycle formation and the addition, they may seek a partner completely outside it, thereby adding a new node and expanding it. Another], there has been very little work on net- works of this type. The only exception that we are aware of involves

258

arXiv:physics/0211090v120Nov2002 A Problem in Paleobiology  

E-Print Network [OSTI]

that may drive extinction or species proliferation, nor shall we address the shape of evolutionary trees produce many new species, but any species may also become extinct, and a natural model(h) of `dying'. As- suming independence of speciation and extinction events, if there are n species present

Reed, W.J.

259

arXiv:0801.1059v1 [math.CO] 7 Jan 2008  

E-Print Network [OSTI]

Jan 7, 2008 ... Using a basic inequality between the stability number and the fractional ... computed, thanks to classical results on spherical harmonics.

2008-01-07T23:59:59.000Z

260

arXiv:astro-ph/0503251v213Mar2005 DRAFT VERSION MARCH 13, 2005  

E-Print Network [OSTI]

emission is due to the outflow ejected during the GF energizing a thin shell surrounding a pre 20450, MS 29, Stanford, CA 94309; granot@slac.stanford.edu 2 IAS, Einstein Drive, Princeton, NJ 08540

Taylor, Greg

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261

arXiv:0812.0734v1 DESY-08-180  

E-Print Network [OSTI]

. Piccinini 6 , M. A. Pleier 14 , M. Poli 6;32 , V. Popov 23 , D. Pose 12;15 , S. Prystupa 17 , V. Pugatch 17

262

Comment on paper arXiv:0902.3613 by P. Bicudo et al  

E-Print Network [OSTI]

In the Comment we scrutinized the quartet basis for the Delta resonances, and the high-momentum truncation scheme, suggested by Bicudo et al. Not all the results and claims has been properly justified by the authors.

A. E. Inopin

2009-03-23T23:59:59.000Z

263

arXiv:cond-mat/0402415v116Feb2004 SUPERCONDUCTING QUBITS AND THE PHYSICS OF  

E-Print Network [OSTI]

OF JOSEPHSON JUNCTIONS John M. Martinis1, Kevin Osborne1 1 Introduction Josephson junctions are good candidates of a Josephson quantum computer? In this paper we focus on the physics of the Josephson junction because, being to be restricted to only the two qubit states. The Josephson junction is a remarkable nonlinear element because

Martinis, John M.

264

arXiv:0902.3928v1 [astroph.GA  

E-Print Network [OSTI]

observations this would yield the distribution of mass among the various components (including dark matter GHz methanol masers are indicated with dark blue dots and those from water masers are indicated

Brunthaler, Andreas

265

arXiv:0712.2020v1 [math.OA] 12 Dec 2007  

E-Print Network [OSTI]

Feb 2, 2008 ... We exhibit a unital simple nuclear non-type-I C?-algebra into which the Jiang-Su algebra does not embed unitally. This answers a question of...

2008-02-02T23:59:59.000Z

266

arXiv:math/0008182v1 [math.OA] 23 Aug 2000  

E-Print Network [OSTI]

K0(I) vanishes then E must be QD also. A Hahn-Banach type property for K0 of QD C?-algebras is also formulated. It is shown that every nuclear QD C?-

2008-02-01T23:59:59.000Z

267

arXiv:cond-mat/0507293v113Jul2005 Multicritical Point Relations in  

E-Print Network [OSTI]

-Lattice Ising Spin-Glasses Michael Hinczewski and A. Nihat Berker Department of Physics, Istanbul Technical

Gozuacik, Devrim

268

arXiv:cond-mat/0506716v128Jun2005 Phase Diagrams and Crossover in  

E-Print Network [OSTI]

Aykut Erba¸s,1 Asli Tuncer,1 Burcu Y¨ucesoy,1 and A. Nihat Berker1-3 1 Department of Physics, Istanbul

Gozuacik, Devrim

269

arXiv:astro-ph/9802348v127Feb1998 CONSTRAINTS ON NEUTRON STAR MATTER  

E-Print Network [OSTI]

to the orbital frequencies of the gas. The 360­600 Hz brightness oscillations seen during thermonuclear X (thermonuclear) X-ray bursts (see [18]) and in the persistent, accretion-powered X-ray emission (see [23

Miller, Cole

270

arXiv:astro-ph/9912361v116Dec1999 Extracting Neutron Star Properties from  

E-Print Network [OSTI]

, College Park, MD 20742-2421 Abstract. Many thermonuclear X-ray bursts exhibit brightness oscillations were discovered in RXTE countrate time series data from thermonuclear X-ray bursts in several neutron the speed and type of thermonuclear propagation. In turn, this has impli- cations for strong gravity

Miller, Cole

271

arXiv:astroph/0403450 Submitted to the The Astrophysical Journal  

E-Print Network [OSTI]

: A Gamma-Ray Burst Afterglow Discovered by its Supernova Light 1 Andrew Levan 2;3 , Peter Nugent 4 , Andrew, Berkeley, CA 94720, USA 5 Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019

Nugent, Peter

272

arXiv:0903.3075v1 HU-EP-09/10  

E-Print Network [OSTI]

classical solutions has been fully realized with the discovery of calorons with non-trivial holon- omy

273

arXiv:cond-mat/0702119v16Feb2007 Hole dynamics in an antiferromagnet  

E-Print Network [OSTI]

that the critical point broadens into a non-Fermi liquid `holon metal' phase with fractionalized excitations. The holon metal phase is flanked on both sides by Fermi liquid states with Fermi surfaces enclosing

274

arXiv:math.NA/0309058v13Sep2003 Optimization Strategies in Complex Systems  

E-Print Network [OSTI]

of the theory of financial risk with short-selling included, the choice of the optimal portfolio from of reconstructing an original sequence of 1 from the Millennium Prize Problems list at Clay Mathematics Institute

Bologna, Università di

275

Revised Version Phys. Rept. 461 (2008) 37 arXiv:0707.4093v2  

E-Print Network [OSTI]

of the interaction at that energy scale. The out- standing property of QCD, asymptotic freedom, tells us that the coupling decreases with increasing energies. This allows the usage of perturbation theory to make phe on the energy scale of the considered physical process, and it gives a measure of the strength

276

arXiv:hep-ex/0302021v116Feb2003 Physics Potential and Prospects for the  

E-Print Network [OSTI]

. In this paper we report the physics potential of both stages of the experiment regarding neutrinoless double beta decay of 130Te, WIMP searches and solar axions. Key words: PACS: 23.40.-s; 95.35.+d; 14.80.Mz Key (axions or WIMPs), sup- posedly filling a substantial part of the galactic haloes, or neutrinoless double

277

Revised Version DESY 07141 arXiv:0709.4650v2  

E-Print Network [OSTI]

) in "neutrinoless double beta decay": UT group is involved in Majorana and KamLAND/ZEN experiments. (b) in neutron

278

arXiv:hepph/0501039 NUHEP-TH/05-02  

E-Print Network [OSTI]

, \\Predictions on the neutrinoless double beta decay from the leptogenesis via the LH(u) at direction," Phys

279

arXiv:hep-ex/0202018v322May2002 Modern Physics Letters A,  

E-Print Network [OSTI]

COMMENT ON "EVIDENCE FOR NEUTRINOLESS DOUBLE BETA DECAY" C. E. Aalseth1, F. T. Avignone III2, A. Barabash3) We comment on the recent claim for the experimental observation of neutrinoless double- beta decay for Neutrinoless Double Beta Decay" However, the analysis in KDHK makes an extraordinary claim, and therefore re

Piepke, Andreas G.

280

arXiv:1407.2817v2 [math.OC] 29 Jul 2014  

E-Print Network [OSTI]

Jul 29, 2014 ... Independently, they are useful for mapping the energy ..... for x0 ? Br(x?), v?1 ? Br(v?)?SX and h ? h0, one of the following alternatives are.

2014-07-30T23:59:59.000Z

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While these samples are representative of the content of NLEBeta,
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We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


281

arXiv:0910.5765v1 [math.OC] 30 Oct 2009  

E-Print Network [OSTI]

Oct 30, 2009 ... [9] G.J.O. Jameson, Summing and nuclear norms in Banach space theory, ... the 34th Annual ACM Symposium on Theory of Computing, 2002. ... 699708 in Proceedings of the 39th Annual ACM Symposium on Theory of.

2009-10-29T23:59:59.000Z

282

arXiv:astro-ph/0502506v124Feb2005 IL NUOVO CIMENTO Vol. ?, N. ? ?  

E-Print Network [OSTI]

) Faculty of Mathematics and Physics, University in Ljubljana, Slovenia Summary. -- The 2-m robotic Observatories HETE-2, INTEGRAL and Swift, followed by automated data reduction, analysis, OT identification and has entered the robotic (unmanned) operation phase with an automated scheduler in summer 2004

Gomboc, Andreja

283

arXiv:hep-ph/001031126Oct2000 JLAB-THY-00-35  

E-Print Network [OSTI]

, demonstrating that duality works remarkably well for each of the low-lying resonances, including the elastic structure function in the resonance region (data from a compilation [3] of JLab and SLAC data); solid line

Thomas Jefferson National Accelerator Facility

284

arXiv:math.AG/9903204v11Mar1999 Annals of Mathematics, 149 (1999), 451473  

E-Print Network [OSTI]

filtration on Chow groups CHp (X)Q = F0 CHp (X)Q F1 CHp (X)Q = CHp (X)hom Q . . . Fp+1 CHp (X)Q = 0, so that a corre- spondence X ? Y should induce : Fk CHp (X)Q Fk CHp (Y )Q, where p = p + dim Y - dim , and ii) the induced map Grk : Grk F CHp (X)Q Grk F CHp (Y )Q should vanish when is homologous

Voisin, Claire

285

arXiv:astro-ph/0608427v121Aug2006 Pinwheels in the Quintuplet Cluster  

E-Print Network [OSTI]

spiral model with winding angle 110±10mas/turn and with an inclination of the rotation axis to the line which resolves this debate with the discovery of rotating spiral plumes charac- teristic of colliding-wind character- istic of colliding-wind binary "pinwheel" nebulae. These have previously been reported in dust

Monnier, John D.

286

arXiv:astroph/0505344 Astronomy & Astrophysics manuscript no. aa20052781 May 18, 2005  

E-Print Network [OSTI]

as clumpiness. However, if viewed at low inclination, and at limited temporal sampling, such a wind would, 2005 (DOI: will be inserted by hand later) Asphericity and clumpiness in the winds of Luminous Blue to investigate the geometries of their winds. We find that at least half of our sample show changes

Vink, Jorick

287

arXiv:0705.1259v1 DESY 06-065  

E-Print Network [OSTI]

of the two-photon decay width of the Higgs boson at a Photon Collider K. Monig 1 and A. Rosca 2 1 DESY of the measurement of the two photon decay width times the branching ratio of a Higgs boson with the mass of 120 Ge of the measurement of the two-photon width,(H ! ), times the branching ratio of the Higgs boson, BR(H ! b #22; b

288

arXiv:physics/0505007v26May2005 TAKING NANOTECHNOLOGY TO SCHOOLS  

E-Print Network [OSTI]

industrial revolution. No wonder, total worldwide R&D spending on nanotechnology in 2004 was an estimated USD the fact that "the relatively small number of applications . . . that have made it through to industrial matter and processes at the nanoscale undoubtedly exists in many aca- demic and industrial laboratories

Lakhtakia, Akhlesh

289

ECMOR XIV 14th European Conference on the Mathematics of Oil Recovery  

E-Print Network [OSTI]

and a waterflooding problem in a two-dimensional five-spot reservoir. The results are compared with previous work-11 September 2014 Mo P80 Value of Information in Closed-loop Reservoir Management E.G.D. Barros* (Delft) analysis within a closed- loop reservoir management (CLRM) framework. The workflow combines tools

Van den Hof, Paul

290

arXiv:hep-ex/0307010v15Jul2003 EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH  

E-Print Network [OSTI]

25, 2002 Search for a Higgs Boson Decaying to Weak Boson Pairs at LEP The L3 Collaboration AbstractV. Limits on the branching fraction of the Higgs boson decay into two weak bosons as a function of the Higgs mass are derived. These results are combined with the L3 search for a Higgs boson decaying to photon

Boyer, Edmond

291

arXiv:nucl-th/0607015v213Jul2006 Direct reactions in/for astrophysics  

E-Print Network [OSTI]

. In recent years direct reactions methods have been developed and applied to extract low-energy astrophysical are focused on the opposite ends of the energy scale of nuclear reactions: (a) the very high and (b) the very end of the energy scale are the low energy reactions of importance for stellar evolution. Chains

Bertulani, Carlos A. - Department of Physics and Astronomy, Texas A&M University

292

arXiv:nucl-th/001006118Oct2000 INTERACTIONS, CURRENTS, AND THE STRUCTURE OF  

E-Print Network [OSTI]

form factors, -decays, radiative and weak capture reactions at low energies, inclusive response on two- and three- nucleon interactions and associated electro-weak currents. Low-energy radiative to hadronic and electro-weak probes at intermediate energies. In the present talk, I will review the "nuclear

Thomas Jefferson National Accelerator Facility

293

arXiv:0805.0396v1 REPRESENTATION GROWTH OF LINEAR GROUPS  

E-Print Network [OSTI]

\\Subgroup Growth"|see [LS] and the references therein. Counting subgroups is essentially the same property (CSP, for short), i.e. C() := ker ( \\ G(O S ) ! G( ^ O S )) is #12;nite, then A() can be described in the Proposition is the fact that the CSP implies super-rigidity: If #26; is a #12;nite dimensional complex

Lubotzky, Alex

294

arXiv:0908.3897v1 [astroph.CO  

E-Print Network [OSTI]

Charles Street, Baltimore, MD 21218. 5 Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112, USA 6 European Southern Observatory, Alonso de Cordova 3107, Casilla 19001, Santiago

Dawson, Kyle

295

arXiv:1411.7288v2 [math.OC] 8 Jan 2015  

E-Print Network [OSTI]

Jan 8, 2015 ... ... products that can be easily implemented even in micro-controllers where complex procedures ...... Networks and Systems (MTNS), 2014, pp.

2015-01-08T23:59:59.000Z

296

arXiv:physics/0502056v110Feb2005 Europhysics Letters PREPRINT  

E-Print Network [OSTI]

was originally suggested as a means to achieve Bose- Einstein condensation in atomic hydrogen [1­3]. Its Fig. 1 ­ Schematic view of the optical compressor. Particles begin in region A with characteristic

Niu, Qian

297

arXiv:hepph/9912489 Is BFKL ruled out by the Tevatron gaps between jets data?  

E-Print Network [OSTI]

] and in flp collisions at HERA [ 5, 6]. Such events are unexpected in standard Regge phenomenol­ ogy since

Lunds Universitet,

298

arXiv:physics/0402070v116Feb2004 TAUP 2764-04  

E-Print Network [OSTI]

, The Academic College of Tel Aviv Yaffo, 64044 Tel Aviv, Israel c Department of Particle Physics, Weizmann MHz. The design luminosity of the accel- erator is 1034 cm-2 s-1 . At this luminosity an average of 23

Shamir, Ron

299

arXiv:1101.1529v1 [astroph.IM  

E-Print Network [OSTI]

22 , Suzanne L. Hawley 5 , Frederick R. Hearty 25 , Jonay I. Gonzalez Hernandez 7 , Shirley Ho 12,53 , Dustin Lang 18 , James E. Lawler 54 , Jean-Marc Le Goff 11 , Brian L. Lee 23 , Young Sun Lee 16 , Jarron

Dawson, Kyle

300

arXiv:astro-ph/0005123 v3 2 Oct 2000  

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:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmosphericNuclear SecurityTensile Strain Switched FerromagnetismWaste andAnniversary, partReview of SIRS Data83Mar00Common005123 v3 2

Note: This page contains sample records for the topic "xiv-1 xiv morocco" from the National Library of EnergyBeta (NLEBeta).
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301

arXiv:astro-ph/0110352 v1 15 Oct 2001  

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:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmosphericNuclear SecurityTensile Strain Switched FerromagnetismWaste andAnniversary, partReview of SIRS Data83Mar00Common005123 v3

302

arXiv:astro-ph/0205476 v1 28 May 2002  

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:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmosphericNuclear SecurityTensile Strain Switched FerromagnetismWaste andAnniversary, partReview of SIRS Data83Mar00Common005123

303

arXiv:hep-ph/0403167v2 8 Apr 2004  

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:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary)morphinanInformation InInformation In closing, an National Carbon Capture Center at2/316 PhotovoltaicCapORNL

304

arXiv:hep-ph/0412251v117Dec2004 CERN-2004-005  

E-Print Network [OSTI]

AT THE CLIC MULTI-TeV LINEAR COLLIDER Report of the CLIC Physics Working Group Editors: M. Battaglia, A. De. Barklow (SLAC), M. Battaglia (LBL and UC Berkeley), W. Beenakker (Univ. of Nijmegen), S. Berge (Univ

Sjöstrand, Torbjörn

305

arXiv:hepex/0211055 FERMILAB-PUB-02/304-E  

E-Print Network [OSTI]

, the CDF detector has encountered operational problems and observed high backgrounds which have been associated with Tevatron injection and aborts. 1 In addition, backgrounds in the CDF detector have been

306

arXiv:cs.IT/0602071v120Feb2006 Geographic Gossip: Efficient Aggregation for Sensor  

E-Print Network [OSTI]

in noisy and uncertain envi- ronments. However, gossip algorithms can waste significant energy the energy consumption by a n log n factor over standard gossip algorithms. Categories and Subject, in which each node col- lects a measurement in some modality of interest (e.g., tem- perature, light

Wainwright, Martin J.

307

arXiv:cs.DB/0112011v25Feb2003 Interactive Constrained Association Rule Mining  

E-Print Network [OSTI]

. After this relatively expensive operation, the actual data mining queries issued by the user then amount]. It motivated the idea of a "data mining query language" [8, 9, 12, 13, 19] and was stressed again by Ng, Lakshmanan, Han and Pang [21]. A data mining query language allows the user to ask for specific subsets

Antwerpen, Universiteit

308

arXiv:1302.4385v1 [stat.ML] 18 Feb 2013  

E-Print Network [OSTI]

Feb 18, 2013 ... Page 1 ... separability means that, for each topic, there exists a word associated only with that topic; see [2, 3]. In hyperspectral imaging, where...

2013-02-18T23:59:59.000Z

309

Submitted to the Annals of Applied Probability arXiv: math.PR/0000000  

E-Print Network [OSTI]

are the quickest detection of man- ufacturing defects during product quality assurance, online fault detection at the same time. These problems arise, for example, from managing product quality in manufacturing systems and preventing the spread of infectious diseases. The promptness and accuracy of detection rules improve greatly

Dayanik, Savas

310

TRIBUNAL REGIONAL FEDERAL DA 1 REGIO XIV CONCURSO PBLICO PARA PROVIMENTO DE CARGO DE  

E-Print Network [OSTI]

Cunha / 10009183, Luiz Carlos de Assis Junior / 10004675, Luiz Carlos dos Santos Queiroz / 10003003 Medeiros / 10002307, Leonardo Costa Coscarelli / 10004478, Luiz Otavio Barros Dutra / 10006688, Marco, Jorge Sallaberry Vianna / 10003792, Jose Leandro Teixeira Borba / 10001127, Marcio Aparecido de Sousa

Maier, Rudolf Richard

311

Revised Version DESY09050 arXiv:0904.3876v2  

E-Print Network [OSTI]

. Robmann 41 , B. Roland 4 , R. Roosen 4 , A. Rostovtsev 24 , M. Rotaru 5 , J.E. Ruiz Tabasco 22 , Z.

312

arXiv:gr-qc/0010070v119Oct2000 A List of References on  

E-Print Network [OSTI]

To be published in the Proceedings of the Encuentros Relativistas Espa~noles, September, 2000 (http://hades

Jantzen, Robert T.

313

1500 1564 1600 1642 1700 HistoricalEventsGovernmentScience  

E-Print Network [OSTI]

LOUIS XIV of France Nicolas COPERNICUS Giordano BRUNO Tycho BRAHE Johannes KEPLER William HARVEY Rene

Hemenway, Mary Kay

314

The Role of the ILC in the Study of Cosmic Dark Matter  

E-Print Network [OSTI]

arXiv:hep-ph/0205314]. M. Battaglia, A. Datta, A. De Roeck,arXiv:hep-ph/0403047]. M. Battaglia, I. Hinchli?e and D.arXiv:hep-ph/0503165]. M. Battaglia, arXiv:hep-ph/0410123.

Battaglia, Marco

2009-01-01T23:59:59.000Z

315

The power of the family  

E-Print Network [OSTI]

finland nigeria serbia and montenegro peru tanzania, unitedcroatia serbia and montenegro zimbabwe tanzania, nigerianam georgia serbia and montenegro japan morocco azerbaijan

Alesina, Alberto; Giuliano, Paola

2010-01-01T23:59:59.000Z

316

Review: Human Rights, Suffering, and Aesthetics in Political Prison Literature edited by Yenna Wu and Simona Livescu  

E-Print Network [OSTI]

as China, Egypt, Syria, Uruguay, Morocco, Romania, theIn Remembering Pain in Uruguay: What Memories Mean incivil conflict in 1970s Uruguay. Stefano asks the reader to

Ahmed, Sumayya

2012-01-01T23:59:59.000Z

317

15 Energy for development: solar home systemsin Africa and global carbon emissions  

E-Print Network [OSTI]

Bank Group's Photo- voltaic Market Transformation Initiative (PVMTI) has se- lected Kenya and Morocco, battery charging, and to a lesserextent,generators),SHS mayalsoyield indirect carbon emissions reductions

Kammen, Daniel M.

318

A cultural, customizable and prefabricated housing grammar for Casablanca  

E-Print Network [OSTI]

Proposing an innovative design grammar linking prefabrication, customization and cultural adaptability, this thesis addresses the present day housing deficit and lack of architectural identity in Casablanca, Morocco. The ...

Akkar, Ghita

2011-01-01T23:59:59.000Z

319

E-Print Network 3.0 - africa mediterranean fruit Sample Search...  

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

Africa, clade E1 in the Mediterranean Basin... from the Mediterranean and North Africa (Canary Islands, South Morocco and Hoggar). In olive... the Mediterranean area and...

320

E-Print Network 3.0 - alkaline igneous rocks Sample Search Results  

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

at Dallas Collection: Geosciences 74 Precambrian evolution of the Sirwa Window, Anti-Atlas Orogen, Morocco Summary: The Palaeoproterozoic Zenaga Complex repre- sents the oldest...

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We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


321

"Nested" cryptic diversity in a widespread marine ecosystem engineer: a challenge for detecting biological invasions  

E-Print Network [OSTI]

of P. dalbyi from Western Australia vs. southeasternindices were similar (Western Australia: h = 1.000 0.045,New Zealand, Morocco and Western Australia. However, these

2011-01-01T23:59:59.000Z

322

Understanding Democratic Congruence: A Demand-Supply Perspective  

E-Print Network [OSTI]

Ireland Philippines India Croatia France Argentina Luxemb.S. Korea Domin. R. Jordan Croatia Latvia Morocco BrazilSlovenia Uruguay Mexico Croatia Brazil Domin. R. Cyprus

Welzel, Christian; Klingemann, Hans-Dieter

2007-01-01T23:59:59.000Z

323

analysis establishes mycobacterium: Topics by E-print Network  

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

Morocco. This paper 138 Genetic Diversity of Mycobacterium tuberculosis in Peru and Exploration of Phylogenetic Associations with Drug Physics Websites Summary: Genetic Diversity...

324

Proceedings of the XIV Colloquium on Musical Informatics (XIV CIM 2003), Firenze, Italy, May 8-9-10, 2003 AN INTRODUCTORY CATALOG OF COMPUTER-SYNTHESIZED CONTACT SOUNDS, IN  

E-Print Network [OSTI]

Rolling Roller Dropping Plastic Bottle Sound models Falling, then rolling Ball Falling Coin Rolling & Braking Wheel Squeaking Door Rubbed Glass Walking on Gravel Invisiball Breaking Glass Crumpling Figure 1

Fontana, Federico

325

arXiv:astro-ph/0602399v117Feb2006 SAURON observations of Sa bulges: the formation  

E-Print Network [OSTI]

of a kinematically decoupled core in NGC 5953 Jes´us Falc´on-Barroso1 , R. Bacon2 , M. Bureau3 , M. Cappellari1 , R. Using #12;2 Falc´on-Barroso et al. Fig. 1. The interacting pair formed by NGC 5953 and NGC 5954. Left: B and NGC 5953, see Falc´on-Barroso et al. 2006). NGC 4698 is a well studied galaxy, where the KDC may

Bureau, Martin

326

arXiv:astro-ph/0303484v121Mar2003 Conceptual Design of a Cosmic Ray Detector Operating  

E-Print Network [OSTI]

York, USA July 8, 2004 Abstract For our understanding of the origin of ultra high energy cosmic rays evidence that at these energies, the origin of cosmic rays changes from predominantly Galactic offers, this study will provide crucial information on the origin of ultra high energy cosmic rays

327

arXiv:1112.2133v1[math-ph]9Dec2011 ON WIGNER'S THEOREM  

E-Print Network [OSTI]

In the paper [De-We2] we de#12;ned isomorphisms of parallel transport along #19;etale paths for a certain class of degree zero on a curve X with good reduction over Q p . By [De-We2] we have a continuous, Galois on vector bundles. Besides, we show that it is compatible with the theory for curves in [De-We2] via

Renard, David

328

arXiv:1208.5004v1[astro-ph.SR]24Aug2012 DRAFT VERSION AUGUST 27, 2012  

E-Print Network [OSTI]

1953), the energy flux u3 would be approximately constant in the solar con- vective zone. This issue of Physics, Gustaf H¨allstr¨omin katu 2a (PO Box 64), FI-00064 University of Helsinki, Finland 4Department gradient of kinetic energy density rather than that of momentum, as was previously thought. This result

Brandenburg, Axel

329

arXiv:1402.0212v1[astro-ph.GA]2Feb2014 Simulations of galactic dynamos  

E-Print Network [OSTI]

-10691 Stockholm, Sweden, e-mail: brandenb@nordita.org, Revision: 1.51 1 #12;2 Axel Brandenburg magnetic et al., 2013a,b) that are believed to sustain the canonical values of a root-mean-square turbulent velocity of urms = 10km/s at den- sity = 210-24 gcm-3. The required vertically integrated energy input

Brandenburg, Axel

330

arXiv:astro-ph/9812260v114Dec1998 Galactic cosmic rays and gamma rays: a unified approach  

E-Print Network [OSTI]

. Strong1 and Igor V. Moskalenko1,2 1Max-Planck-Institut f¨ur extraterrestrische Physik, Postfach 1603, D sections based on the observed cosmic-ray abundances (see Webber, Lee, & Gupta 1992). The B/C data is used cross sections. A re-evaluation of the halo size is desirable since new 10Be/ 9Be data are available

Moskalenko, Igor V.

331

arXiv:0803.4162v2[nucl-ex]1Feb2009 High sensitivity measurement of 224  

E-Print Network [OSTI]

, for a 275 tonne D2O assay, which are equivalent to 4?10-16 g Th/g and 3?10-16 g U/g in heavy water. Key scintillation 1. Introduction SNO is a heavy water Cherenkov detector sit- uated at a depth of about 2100 m 2001), salt (May 2001 to September 2003) when 2 tonnes of NaCl were added to the heavy water to improve

332

arXiv:1307.2123v1[math.NA]8Jul2013 ADAPTIVE HETEROGENEOUS MULTISCALE METHODS FOR  

E-Print Network [OSTI]

discretizations of immiscible incompressible two-phase flow. Math. Comp., in press, 2013]. Keywords adaptivity and incom- pressible fluids with highly variable porosity and a highly variable hydraulic conductivity, when it is necessary to resolve the fine scale features of the (rapidly oscillating) hydraulic

333

arXiv:astro-ph/0509202v18Sep2005 TO APPEAR IN THE ASTROPHYSICAL JOURNAL SUPPLEMENTS  

E-Print Network [OSTI]

M?NDEZ 1 , DAVID C. MOORE 2 , M?NICA RUBIO 1 , MARÍA TERESA RUIZ 1 , SUNE TOFT 2,3 , SUKYOUNG K. YI 10

Liu, Charles

334

arXiv:condmat/0607335 Molecular dynamics of shock fronts and their transitions in Lennard-Jonesium and Tin  

E-Print Network [OSTI]

in Lennard-Jonesium and Tin J. M. D. Lane #3; and M. P. Marder y Center for Nonlinear Dynamics, University for shocks in tin which agrees to within 6% with experimental data. We study the strong shock to elastic-plastic shock transition in tin and #12;nd that it is a continuous transition consistent with a transcritical

Texas at Austin. University of

335

arXiv:0802.3463v1[nucl-th]23Feb2008 Nuclear astrophysics from direct reactions  

E-Print Network [OSTI]

, and energy production in stars. A. Nuclear reaction rates Low energy nuclear astrophysics requires the knowl Be(p, ) 8 B plays a major role for the production of high energy neutrinos from the -decay of 8 B Department of Physics, Texas A&M University, Commerce, TX 75429, USA Accurate nuclear reaction rates

Bertulani, Carlos A. - Department of Physics and Astronomy, Texas A&M University

336

arXiv:0706.1212v2[astro-ph]12Jun2007 30th International Cosmic Ray Conference  

E-Print Network [OSTI]

. Cherenkov radiation is emitted in the water by the electrons and the muons as well as by electrons produced.ghia@lngs.infn.it Abstract: The building block of the surface detector of the Pierre Auger Observatory is a water Cherenkov the simulation chain, we compare the simulated signals produced by cosmic muons at various zenith angles

337

arXiv:1108.6203v1[astro-ph.SR]31Aug2011 Noname manuscript No.  

E-Print Network [OSTI]

in approximately the same proportion as major events. We discuss the distributions of flare parameters (e.g., peak . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19 3.3 Origin of power-law distribution . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21 3.4 Nonthermal and thermal spectral parameters

California at Berkeley, University of

338

arXiv:1012.4570v1[astro-ph.GA]21Dec2010 Herschel WISH program  

E-Print Network [OSTI]

. Olberg11 , L. Pagani25 , O. Panic36 , B. Parise16 , J.C. Pearson37 , R. Plume38 , C. Risacher13 , D

339

arXiv:astro-ph/0411406v115Nov2004 Classification and Characterization of Objects from the GALEX  

E-Print Network [OSTI]

internal re- lease, matched to the SDSS catalogs in the overlapping regions, to classify objects@ipac.caltech.edu) 9 Laboratory for Astronomy and Solar Physics, NASA Goddard Space Flight Center, Greenbelt, MD 20771

Bianchi, Luciana

340

arXiv:physics/0607280v130Jul2006 APS/123-QED Energy Dissipation in Fractal-Forced Flow  

E-Print Network [OSTI]

48109 Nikola P. Petrov Department of Mathematics University of Oklahoma, Norman, OK 73019 (Dated: July ) as Re (1) where is the total energy dissipation rate per unit mass, is an integral (large) length the cascade picture of turbulence requires that energy be predominantly injected in a relatively narrow range

Cheskidov, Alexey

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While these samples are representative of the content of NLEBeta,
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341

arXiv:0911.5286v1[hep-ph]27Nov2009 LU TP 09-31  

E-Print Network [OSTI]

Given the current landscape in experimental high-energy physics, these lectures are focused, specifically the potential formation of a quarkgluon plasma. Further, within the field of high-energy pp on hadronization in section 7. The article concludes with an outlook on the ongoing generator- development work

Lunds Universitet,

342

arXiv:cond-mat/0005262v116May2000 Spin transitions in a small Si quantum dot  

E-Print Network [OSTI]

during every tunneling event. PACS numbers: 73.23.Hk, 85.30.Wx, 85.30.Vw, 85.30.Tv, 71.70.Ej The spin, the Coulomb blockade is lifted in the corresponding conduction val- ley at low temperatures. Indeed, valleys

343

arXiv:cond-mat/0508301v112Aug2005 Fate of the Josephson effect in thin-film superconductors  

E-Print Network [OSTI]

sensitive magnetic flux and electromagnetic radiation detectors are SQUIDs (Superconducting Quantum link (e.g. an insulating barrier) between two bulk superconductors, even in the absence of a volt- age detectors to monitor brain activity. Josephson junctions were also a stepping stone in computer technology

344

arXiv:astro-ph/0406317v114Jun2004 Star Formation in Hi Selected Galaxies I: Sample Characteristics  

E-Print Network [OSTI]

are best explained by young mean ages 1 Department of Astronomy, New Mexico State University, Dept. 4500 PO, but this conclusion is somewhat dependent on how the fluxes of these objects are determined. Subject headings effect has been lessened by the advent of more sensi- tive detectors and the use of larger and better

O'Neil, Karen

345

arXiv:1202.0507v1[hep-ph]2Feb2012 Associated Production of Light Gravitinos  

E-Print Network [OSTI]

, and International Solvay Institutes, Pleinlaan 2, B-1050 Brussels, Belgium We study light gravitino productions

346

XIV Simpsio Brasileiro de Informtica na Educao -NCE -IM/UFRJ 2003 A Contradiction-driven Approach of Learning in  

E-Print Network [OSTI]

as Discovery Learning Environments (DLE's). In this paper we are concerned with the design and usage of particular DLE's, within which learning events occur as a consequence of contradiction detection for the design of DLE's, by presenting its exploitation in a real learning situation in Law. Key words: Discovery

Paris-Sud XI, Université de

347

arXiv:1008.3932v2[cs.SY]13Sep2010 Multiple Timescale Dispatch and Scheduling for  

E-Print Network [OSTI]

Reliability in Smart Grids with Wind Generation Integration Miao He and Sugumar Murugesan and Junshan Zhang with integrated wind generation, by leveraging multi-timescale dispatch and scheduling. Specifically, we consider information on wind generation and energy demands, we char- acterize the optimal procurement of the energy

Zhang, Junshan

348

arXiv:adap-org/9803001v110Mar1998 Large-scale evolution and extinction in a hierarchically structured  

E-Print Network [OSTI]

- veloped (Kauffman 1992). The extinction of a single species might cause another species to die out, which might drive a third species into extinction and so on, producing an avalanche that in principle could-law distribution of extinction events can appear even in a system in which species are wiped out solely because

349

arXiv:1108.2840v1[q-bio.NC]14Aug2011 Generalised elastic nets  

E-Print Network [OSTI]

the desire to represent a set of data (cities in the TSP, feature preferences in cortical maps, Washington, DC 20007, US miguel@cns.georgetown.edu, geoff@georgetown.edu Abstract The elastic net, to biological modelling. It has an energy function which trades off a fitness term against a tension term

Goodhill, Geoffrey J.

350

arXiv:astro-ph/0609335v112Sep2006 To appear in the Astrophysical Journal Letters  

E-Print Network [OSTI]

Center Green, Boulder, CO 80301 9 Jet Propulsion Laboratory, 4800 Oak Grove Dr., MS 183-900, Pasadena, CA 91109; john.t.trauger@jpl.nasa.gov 10 Instituto de Astrof´isica de Canarias, 38200 La Laguna, Tenerife

Deeg, Hans-Jörg

351

arXiv:1108.3490v1[astro-ph.SR]17Aug2011 Noname manuscript No.  

E-Print Network [OSTI]

. . . . . . . . . . . . . . . . . . . . . . . . . 21 H. S. Hudson SSL/UC Berkeley Tel.: +1 510-643-0333 E-mail: hhudson@ssl.berkeley.edu Abstract

California at Berkeley, University of

352

arXiv:cond-mat/0311535v221Jan2004 On large deviation properties of Erdos-Renyi  

E-Print Network [OSTI]

the Legendre transform of the Potts free energy with respect to ln q is related to the component generating calculate the number of components, the size of the giant component, the degree distributions inside- gree [2] or power law degree distribution [3, 4] have been investigated. Most of the efforts devoted

Peinke, Joachim

353

arXiv:0905.3291v1[astro-ph.HE]20May2009 DRAFT VERSION MAY 20, 2009  

E-Print Network [OSTI]

. WOOD 3 , B. ZITZER 14 Draft version May 20, 2009 ABSTRACT We present evidence that the very-high-energy wind nebula CXOU J061705.3+222127, both of which are important targets for VHE observations. VERITAS Museum, Chicago, IL 60605, USA 13 Department of Physics and Astronomy, University of Utah, Salt Lake City

354

arXiv:0901.0740v4[hep-ex]16May2009 Measurement of D  

E-Print Network [OSTI]

at s = 200 GeV B. I. Abelev,8 M. M. Aggarwal,30 Z. Ahammed,47 B. D. Anderson,18 D. Arkhipkin,12 G. S

Llope, William J.

355

arXiv:0810.4979v1[nucl-ex]28Oct2008 Energy and system size dependence of  

E-Print Network [OSTI]

+Cu and Au+Au collisions B.I. Abelev i , M.M. Aggarwal ae , Z. Ahammed au , B.D. Anderson s , D. Arkhipkin m

Llope, William J.

356

arXiv:hepex/0603047 Polarization of and in 920 GeV Fixed-Target Proton-Nucleus Collisions  

E-Print Network [OSTI]

. Pleier 13 , M. Poli 6;31 , V. Popov 22 , D. Pose 11;14 , S. Prystupa 16 , V. Pugatch 16 , Y. Pylypchenko

357

arXiv:0709.1823v1[astro-ph]12Sep2007 30th International Cosmic Ray Conference  

E-Print Network [OSTI]

and power is provided by solar panels. The construc- tion of the array is nearly completed and a large than 5 M.cm, up to a depth of 1.2 m. Two solar panels combined with batteries furnish 10 W power stability are presented. The performance of the solar power system and other hardware, as well as the water

358

arXiv:cond-mat/0503226v19Mar2005 Two Superconducting Phases in the d = 3 Hubbard Model  

E-Print Network [OSTI]

Diagram and Specific Heat from Renormalization-Group Calculations Michael Hinczewski and A. Nihat Berker

Gozuacik, Devrim

359

arXiv:cond-mat/0504741v128Apr2005 d = 3 Anisotropic and d = 2 tJ Models  

E-Print Network [OSTI]

, Thermodynamic Properties, and Chemical Potential Shift Michael Hinczewski and A. Nihat Berker Department

Gozuacik, Devrim

360

arXiv:cond-mat/0503631v128Mar2005 Superfluid Weight, Free Carrier Density, and Specific Heat  

E-Print Network [OSTI]

of the d = 3 tJ Model at Finite Temperatures Michael Hinczewski and A. Nihat Berker Department of Physics

Gozuacik, Devrim

Note: This page contains sample records for the topic "xiv-1 xiv morocco" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


361

arXiv:1205.2393v1[astro-ph.SR]10May2012 Solar Physics  

E-Print Network [OSTI]

, Switzerland SOLA: SoPH_DF_final.tex; 14 May 2012; 0:20; p. 1 #12;J.C. Mart´inez-Oliveros et al. timing does of this activity. During flares and CMEs, energy stored in the coronal magnetic field is converted into kinetic energy and thermal energy which are observed as coronal mass movement, and used to heat the plasma

California at Berkeley, University of

362

arXiv:1104.2624v1[astro-ph.SR]13Apr2011 Solar Physics  

E-Print Network [OSTI]

­15 keV, and 15­30 keV energy ranges for each event. In order to extract the height distribution from Northwestern Switzerland, Institute of 4D, Technologies, 5210 Windisch, Switzerland SOLA: paper.tex; 15 April

California at Berkeley, University of

363

arXiv:1203.3907v1[astro-ph.SR]17Mar2012 Solar Physics  

E-Print Network [OSTI]

energy in the attendant seismic emission, suggesting that Lorentz forces can contribute significantly Associates, CORA Division, Boulder, CO USA; email: clindsey@cora.nwra.com SOLA: SP_Alvarado_et_al_2011.tex, driven by solar flares. Sunquakes carry energy and momentum into the solar photosphere and interior from

California at Berkeley, University of

364

arXiv:0903.4141v2[astro-ph.SR]4Apr2009 Solar Physics  

E-Print Network [OSTI]

.zouganelis@lpp.polytechnique.fr SOLA: StereodustSP.tex; 4 April 2009; 15:51; p. 1 #12;Meyer-Vernet et al. 1. Introduction The wave by impacts of micron-sized dust moving at Keplerian speeds. Basically, the energy dissipated upon impact

California at Berkeley, University of

365

arXiv:1012.0344v1[astro-ph.SR]1Dec2010 Solar Physics  

E-Print Network [OSTI]

) on the Solar Dy- namics Observatory (SDO) and the Reuven Ramaty High-Energy Solar Spec- troscopic Imager, Switzerland SOLA: martinez_etal_SoPh_2010.tex; 3 December 2010; 1:08; p. 1 #12;J.C. Mart´inez Oliveros et al phenomenon corresponds to the sudden release of energy stored in the corona via the slow buildup of excess

California at Berkeley, University of

366

arXiv:astro-ph/0012043v12Dec2000 ASP Conference Series, Vol. **VOLUME**, **PUBLICATION YEAR**  

E-Print Network [OSTI]

gravity, high densities, and the propagation of thermonuclear burning. Here we review the evidence for them apparent in timing observations. In § 3 we discuss thermonuclear propagation in X-ray bursts

Miller, Cole

367

arXiv:nucl-th/0109084v128Sep2001 Parity-Violating Interaction Effects I: the Longitudinal  

E-Print Network [OSTI]

in pp Elastic Scattering J. Carlson Theoretical Division, Los Alamos National Laboratory, Los Alamos Institute of Technology, Cambridge, MA 02139 and Department of Physics, University of Maryland, College Park, MD 20742 B.F. Gibson Theoretical Division, Los Alamos National Laboratory, Los Alamos, New Mexico

368

arXiv:hep-ex/0205064v117May2002 DESY-02-059 ISSN 0418-9833  

E-Print Network [OSTI]

. Boudry27 , W. Braunschweig1 , V. Brisson26 , H.-B. Br¨oker2 , D.P. Brown10 , W. Br¨uckner12 , D. Bruncko.J. Campbell10 , S. Caron1 , F. Cassol-Brunner22 , D. Clarke5 , C. Collard4 , J.G. Contreras7,41 , Y.R. Coppens3 , J.A. Coughlan5 , M.-C. Cousinou22 , B.E. Cox21 , G. Cozzika9 , J. Cvach29 , J.B. Dainton18 , W.D

Boyer, Edmond

369

Measurements and calculations of metastable level lifetimes in Fe X, Fe XI, Fe XII, Fe XIII, and Fe XIV  

E-Print Network [OSTI]

Lifetimes of metastable levels in the ground term of Fe ions within the 3s(2)3p(k), k=1-5, isoelectronic sequences have been measured. These measurements were performed utilizing ions that were selected by mass to charge ratio while transported from...

Moehs, D. P.; Bhatti, M. I.; Church, David A.

2001-01-01T23:59:59.000Z

370

arXiv:1008.2116v1[cond-mat.mes-hall]12Aug2010 Circular ac Hall Effect  

E-Print Network [OSTI]

¨oping, Sweden and 4 Chalmers University of Technology, S-41296 G¨oteborg, Sweden (Dated: August 13, 2010) We at room tempera- ture for wavelengths between 90 µm and 280 µm using either a continuous-wave (cw) CH3OH laser or a high power pulsed NH3 laser [10]. For these wavelengths the condition

Ganichev, Sergey

371

arXiv:1404.6964v1[astro-ph.SR]28Apr2014 DRAFT VERSION APRIL 29, 2014  

E-Print Network [OSTI]

Stockholm, Sweden Department of Astronomy, Stockholm University, SE-10691 Stockholm, Sweden (Dated: April 29 by a power law, but the exponent is not the same in all cases. For nonhelical turbulence at large magnetic: accretion disks -- hydrodynamics -- MHD -- shock waves -- turbulence 1. INTRODUCTION One of the central

Brandenburg, Axel

372

arXiv:0903.3075v1[hep-ph]18Mar2009 HU-EP-09/10  

E-Print Network [OSTI]

realized with the discovery of calorons with non-trivial holon- omy by Kraan and van Baal [14] and Lee

373

arXiv:cond-mat/0410750v128Oct2004 A fully fermionic mean field theory of the cuprate superconductors  

E-Print Network [OSTI]

fermion) and a holon (a spin-0 charged boson). The spin-charge separation phenomenon corresponds to the rapid decay of an electron excitation into a spinon and a holon, leading to the lack of quasiparticle points means that, in this k-space region, the spinon and the holon form a bound state. [12, 13] Within

Wen, Xiao-Gang

374

arXiv:0706.2187v2[cond-mat.str-el]18Sep2007 Algebraic charge liquids  

E-Print Network [OSTI]

charge e, no spin, and has Fermi statistics. We shall refer to this fermion as a `holon'. The holon comes stronger effects. We also introduce operators f ± which create holons with charges ±1. ¿From the f± and aµ

375

arXiv:cond-mat/0703101v2[cond-mat.str-el]3Jun2007 The Luttinger liquid kink  

E-Print Network [OSTI]

function is that within Lut- tinger liquid theory, the spinon branch is muted com- pared to the holon

Hu, Jiangping

376

arXiv:cond-mat/0306537v230Jun2003 Absence of U(1) spin liquids in two dimensions  

E-Print Network [OSTI]

, and also with other possible `holon' excitations, via exchange of the gauge boson. We will focus here

377

arXiv:1205.1150v3[math.ST]31May2013 Estimating Omissions from Searches  

E-Print Network [OSTI]

-recapture method was devised by Petersen in 1896 to estimate the number of fish migrating into the Limfjord was independently developed by Petersen (1896) to estimate fish numbers migrating between the German sea

378

arXiv:cond-mat/9609266v127Sep1996 Far-infrared and capacitance spectroscopy of  

E-Print Network [OSTI]

-size semiconductor systems. In these systems, the charge carriers are strongly confined in all three dimensions, so spectroscopy is carried out using standard lock-in technology. For small-scale capacitance probing a bridge

Ludwig-Maximilians-Universitt, Mnchen

379

arXiv:hep-ex/0211071v325Feb2003 A Calorimetric Search on Double Beta Decay  

E-Print Network [OSTI]

and on the neutrinoless double beta decay of 128Te to the ground state of 128Xe are also reported and discussed limit of 2.1? 1023 years has been obtained at the 90 % C.L. on the lifetime for neutrinoless double beta decay of 130Te . In terms of effective neutrino mass this leads to the most restrictive limit in direct

380

arXiv:hep-ph/0403296v26Apr2004 LAPTH-1033/04, IFIC/04-11, PCC-0413  

E-Print Network [OSTI]

-9007(96)01989-8] PACS numbers: 23.40.Hc, 21.10.Tg, 21.60.Cs, 27.40.+z Neutrinoless double beta decay (bb0n) is the most

Paris-Sud XI, Université de

Note: This page contains sample records for the topic "xiv-1 xiv morocco" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


381

arXiv:quant-ph/0311099v217Nov2003 Coupling Efficiencies in Single Photon On-Demand Sources  

E-Print Network [OSTI]

, 13 rely on optical parametric downconversion (PDC), because it produces photons two at a time suppressing the probability of multi-photon generation.13 Most PDC based schemes (including ours) require that the PDC output be collected into a single spatial mode defined by an optical fiber. In order for these PDC

Hart, Gus

382

arXiv:0811.1477v1[stat.AP]10Nov2008 The Annals of Applied Statistics  

E-Print Network [OSTI]

in detail multidimensional scaling applied to a specific dataset: the 2005 United States House United States House of Represen- tatives roll call votes [Office of the Clerk--U.S. House ecological factors scored in the form of presence/absence in 10 km side squares in Belgium there was a strong

383

arXiv:submit/0451583[physics.gen-ph]8Apr2012 Including Nuclear Degrees of Freedom in a Lattice  

E-Print Network [OSTI]

of condensed matter physics. In the Fleischmann­Pons excess heat effect [4, 5], a great deal of energy Institute of Technology, Cambridge, MA 02139, USA E-mail: plh@mit.edu 2 Department of Computer Science and Engineering, University of Engineering and Technology. Lahore, Pakistan Abstract. Motivated by many

Williams, Brian C.

384

arXiv:nucl-th/001006218Oct2000 Electromagnetic Structure of Few-Nucleon Systems: a Critical Review  

E-Print Network [OSTI]

in predicting a number of nuclear properties for systems with mass number A 8, including energy spectra of low-lying states, electromagnetic form factors, and low-energy capture reactions. 2. Interactions and Energy, including energy spectra, electromagnetic form factors, and capture reactions, is critically reviewed within

Thomas Jefferson National Accelerator Facility

385

arXiv:cond-mat/0607317v113Jul2006 Programmable control of nucleation for algorithmic self-assembly  

E-Print Network [OSTI]

a significant reduction in assembly speed. I. INTRODUCTION Molecular self-assembly is an emerging low-cost alter-up fabrication of complex nanostruc- tures. A `program' for growing a desired structure consists of a set toward understanding how algorithmic self-assembly can be performed with low error rates without

Winfree, Erik

386

arXiv:astro-ph/0602622v128Feb2006 Magnetic Fields in the Center of the Perseus Cluster  

E-Print Network [OSTI]

the linearly polarized emission from 3C 84, and from them we determine a Faraday rotation measure (RM) ranging is required to re-heat the gas. Since massive flows of material are not observed, 1 University of New Mexico in modifying the energy transport and dissipation in the center of the cluster (Fabian et al. 2005). Compar

Taylor, Greg

387

arXiv:cond-mat/0307379v28May2004 A Theory of Cooperative Diffusion in Dense Granular Flows  

E-Print Network [OSTI]

) random walks. I. INTRODUCTION In spite of a venerable engineering literature [1, 2, 3], the study, continuum equations for hydrodynamics and heat trans- fer can be formally derived from various modifications. Classical continuum models of dense flows are based on plasticity theory from soil mechanics [1, 2

Weeks, Eric R.

388

arXiv:1209.5252v1[astro-ph.SR]24Sep2012 Solar Physics  

E-Print Network [OSTI]

), bright non-magnetic and dark non-magnetic (inter­network) regions, separately. We use Fourier power that short­period pow- ers are mainly concentrated in dark regions whereas long­period powers at- mosphere is observed at chromospheric heights (Ca ii H and K lines), a bright web-like cellular

389

arXiv:0812.4360v2[cs.AI]15Apr2009 Driven by Compression Progress  

E-Print Network [OSTI]

://www.idsia.ch/juergen Abstract I argue that data becomes temporarily interesting by itself to some self-impro- ving . . . . . . . . . . . . . . . . . . . . . . 5 2 Consequences of the Compression Progress Drive 6 2.1 Compact Internal Representations or Symbols Sources of Fun . . . . . . . . . . . . . . . . . . . . 12 3 Previous Concrete Implementations of Systems

Schmidhuber, Juergen

390

arXiv:0812.4360v1[cs.AI]23Dec2008 Driven by Compression Progress  

E-Print Network [OSTI]

://www.idsia.ch/juergen Abstract I argue that data becomes temporarily interesting by itself to some self-impro- ving Drive 6 2.1 Compact Internal Representations or Symbols as General By-Products of Efficient History Learning . . . . . . . . . . . . . . . 11 3 Previous Concrete Implementations of Systems Driven

Schmidhuber, Juergen

391

arXiv:astro-ph/0609503v118Sep2006 Observations Supporting the Role of Magnetoconvection in  

E-Print Network [OSTI]

Supply to the Quiescent Solar Atmosphere Scott W. McIntosh, Alisdair R. Davey, Donald M. Hassler USA Werner Curdt, Klaus Wilhelm Max Planck Institute for Solar System Research, Max-Planck-Str. 2 mechanisms behind the production and suste- nance of the quiescent solar corona and solar wind poses two

Lin, Gang

392

arXiv:gr-qc/0606067v211Jul2006 How often does the Unruh-DeWitt detector click?  

E-Print Network [OSTI]

-order perturbation theory the instantaneous transition rate of an accelerated Unruh-DeWitt particle detector whose with a temperature proportional to the accel- eration is called the Unruh effect in honour of its discoverer [1 way to address the Unruh effect is in terms of a particle detector model, consisting of a quantum

393

arXiv:0905.1816v1[astro-ph.SR]12May2009 Solar Physics  

E-Print Network [OSTI]

: Coronal mass ejections · Cosmic rays, solar · Energetic particles, accel- eration · Energetic particles network of neutron monitors at Earth with electromagnetic signatures of particle acceleration in the solar corona during the large particle event of 20 January 2005. The intensity-time profile of the relativistic

California at Berkeley, University of

394

arXiv:quant-ph/0403061v18Mar2004 Driven chaotic mesoscopic systems, dissipation and decoherence  

E-Print Network [OSTI]

(quantum dots), as well as in nuclear, atomic and molecular physics. Such systems tend to absorb energy. This irreversible effect is known as dissipation. More generally, x may be a dynamical variable, where the total Hamiltonian is H0(x, p) + H(Q, P; x). In such case the interaction of (x, p) with the environmental degrees

Cohen, Doron

395

arXiv:1101.3744v1[nucl-ex]19Jan2011 Measurement of 30  

E-Print Network [OSTI]

,1 J. Robinson,3 G. Rosner,3 T. Rostomyan,11 S. Schumann,2, 5 M. H. Sikora,8 D. Sober,16 I. Supek,15 resonance region consists of three pairs of N and two pairs of (assuming the existence of the one

Krusche, Bernd

396

arXiv:1306.1243v2[hep-ex]21Aug2013 Measurement of the p K0  

E-Print Network [OSTI]

. Schumann1 , M. H. Sikora15 , D. I. Sober20 , A. Starostin9 , I. I. Strakovsky8 , I. M. Suarez9 , I. Supek19 and universal baryon-resonance parameters from corresponding author, e-mail: ostrick

Krusche, Bernd

397

arXiv:1302.0022v1[astro-ph.SR]31Jan2013 Astronomische Nachrichten, 4 February 2013  

E-Print Network [OSTI]

3 , and the CSI 2264 Team 1 Spitzer Science Center, California Institute of Technology, 1200 E with accretion, disk structure, and accompanying stellar activity, but these processes are challenging to model static geometry, young stars and their disks constitute an incredibly dynamic environment, as borne out

Micela, Giusi

398

arXiv:hep-ex/0609002v24Sep2006 Finding The Charm In 800 GeV/c  

E-Print Network [OSTI]

the luminarias to guide me through. I have had the incredible fortune to meet and know two true gentlemen along

399

arXiv:physics/0408090v214Mar2005 Complex Impedance as a Diagnostic Tool for Characterizing Thermal Detectors  

E-Print Network [OSTI]

the thermometer to a heat sink. The simple model treated in most analytical descrip- tions consists of a lumped and complex de- tectors, along with the thermometer temperature sensi- tivity and thermometer voltage (or16­18 in the thermome- ter and a thermal resistance between the absorber and thermometer. We begin

Wisconsin at Madison, University of

400

5""reuniondu GroupeMarocaindu Permien et du Trias El Jadida,26-29Avril2006. Maroc The first 200 ky of the Early Jurassic in eastern North America and Morocco  

E-Print Network [OSTI]

5""?reuniondu GroupeMarocaindu Permien et du Trias El Jadida,26-29Avril2006. Maroc The first 200 ky, 26-29 Avril2006, Maroc likewise of low taxonomic diversity at the family level consisting almost

Olsen, Paul E.

Note: This page contains sample records for the topic "xiv-1 xiv morocco" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


401

apres irradiation gamma: Topics by E-print Network  

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

2 arXiv:astro-ph9912303v24Apr2000 Vacuum discharge as a possible source of gamma-ray bursts Physics Websites Summary: arXiv:astro-ph9912303v24Apr2000 Vacuum discharge as a...

402

accidental gamma irradiation: Topics by E-print Network  

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

84 arXiv:astro-ph9912303v24Apr2000 Vacuum discharge as a possible source of gamma-ray bursts Physics Websites Summary: arXiv:astro-ph9912303v24Apr2000 Vacuum discharge as a...

403

First results on neutrinoless double beta decay of Te-130 with the calorimetric cuoricino experiment  

E-Print Network [OSTI]

Evidence for Neutrinoless Double Beta Decay arXiv:hep-on Evidence for neutrinoless double beta decay- arXiv:hep-Results on Neutrinoless Double Beta Decay of 130 Te with the

2003-01-01T23:59:59.000Z

404

Field-Dependent BRST-antiBRST Lagrangian Transformations  

E-Print Network [OSTI]

We continue our study of finite BRST-antiBRST transformations for general gauge theories in Lagrangian formalism, initiated in [arXiv:1405.0790[hep-th] and arXiv:1406.0179[hep-th

Pavel Yu. Moshin; Alexander A. Reshetnyak

2014-10-05T23:59:59.000Z

405

Near-barrier Fusion and Transfer/Breakup induced by Weakly Bound and Exotic Halo Nuclei  

E-Print Network [OSTI]

This submission has been withdrawn by arXiv administrators because it is a duplicate of nucl-th/0610004.

C. Beck

2007-01-29T23:59:59.000Z

406

A critical analysis of the GP-B mission. I: on the impossibility of a reliable measurement of the gravitomagnetic precession of the GP-B gyroscopes  

E-Print Network [OSTI]

This submission has been removed because 'G. Forst' is an apparent pseudonym, in violation of arXiv policies.

G. Forst

2008-01-11T23:59:59.000Z

407

An implicit numerical algorithm general relativistic hydrodynamics  

E-Print Network [OSTI]

An implicit numerical algorithm general relativistic hydrodynamics This article has been replaced by arXiv:0801.1017

A. Hujeirat

2008-01-09T23:59:59.000Z

408

Automation in image cytometry : continuous HCS and kinetic image cytometry  

E-Print Network [OSTI]

OF CALIFORNIA, SAN DIEGO Automation in Image Cytometry:xiv Abstract of Dissertation Automation in Image Cytometry:

Charlot, David J.

2012-01-01T23:59:59.000Z

409

Erasmus Mundus Action 2 Strand 1 / Strand 2 (delete as appropriate) PROJECT SUMMARY SHEET  

E-Print Network [OSTI]

____________________________________ Title of proposal EM A2 Strand 1 Lot 1:Algeria, Morocco, Tunisia, Egypt and Libya (EM A2 LOT 1 Al- Fihri Partner 18 Libyan International Medical University Libya Partner 19 Omar Muhktar University Libya TC, Morocco, Tunisia, Egypt and Libya Project duration (months) 48 months #12;Amount requested (EUR) 4

Schenato, Luca

410

HOST UNIVERSITIES: University of Abou Bekr Belkaid Tlemcen,  

E-Print Network [OSTI]

and Maritime Transport, Egypt University of Sirte, Libya Superior Institution of Science and Technology SCHOLARSHIPS FOR STUDY/RESEARCH IN MOROCCO|EGYPT|TUNISIA|ALGERIA|LIBYA AVAILABLE FOR UNDERGRADUATE|MASTER POST Doctorate 1800 Staff 2500 EU FUNDED SCHOLARSHIPS FOR STUDY/RESEARCH IN EU|MOROCCO|EGYPT TUNISIA|ALGERIA|LIBYA

Guidoni, Leonardo

411

Resonant slepton production yields CMS eejj and epTjj excesses  

E-Print Network [OSTI]

. F. Deppisch, T. E. Gonzalo, S. Patra, N. Sahu and U. Sarkar, arXiv:1407.5384 [hep-ph]. [5] M. Heikinheimo, M. Raidal and C. Spethmann, arXiv:1407.6908 [hep-ph]. [6] B. A. Dobrescu and A. Martin, arXiv:1408.1082 [hep-ph]. [7] J. A. Aguilar...

Allanach, Ben; Biswas, Sanjoy; Mondal, Subhadeep; Mitra, Manimala

2015-01-13T23:59:59.000Z

412

arXiv:0811.1672v1[cond-mat.other]11Nov2008 Free-fall expansion of finite-temperature  

E-Print Network [OSTI]

-Einstein condensed gas in the non Thomas-Fermi regime M. Zawada1 , R. Abdoul1 , J. Chwede´nczuk,2 R. Gartman1 , J of a diluted Bose-Einstein condensed gas results in spatial separation of the thermal and condensed phases [7, most of the experimental work on the condensed gases was concentrated on samples with large number

413

arXiv:1108.3866v1[physics.atom-ph]18Aug2011 Universalities in ultracold reactions of alkali polar molecules  

E-Print Network [OSTI]

statistics plays a strong role. An ultracold gas of bosonic molecules can lead to Bose-Einstein condensation and an ultracold sample of fermionic molecules can lead to a Degenerate Fermi gas. Thirdly, two polar molecules can University, 198904, Russia interactions in a gas and depends strongly on the ap- plied electric field [16

Kotochigova, Svetlana

414

arXiv:0801.0249v1[cs.MA]31Dec2007 A MATHEMATICAL FORMALISM FOR AGENT-BASED MODELING  

E-Print Network [OSTI]

Systems: Definitions 12 5.2. Configuration Reachability Problem for SDSs 12 5.3. Turing Machines: A Brief Overview 13 5.4. How SDSs Can Mimic Turing Machines 13 5.5. TRANSIMS related questions 14 6. Mathematical

Tesfatsion, Leigh

415

arXiv:1104.0081v2[math.CO]4Apr2011 CAYLEY GRAPHS OF ORDER 16p ARE HAMILTONIAN  

E-Print Network [OSTI]

is prime. We show that if S is any generating set of G, then there is a hamiltonian cycle.2(1) of [10]. Namely, several of the main results of that paper combine to show: Every connected Cayley graph on G has a hamiltonian cycle if |G| = kp, where p is prime, 1 k

Morris, Joy

416

arXiv:1004.0661v1[cond-mat.soft]5Apr2010 Evolution of shear-induced melting in dusty plasma  

E-Print Network [OSTI]

sound speed. Unexpectedly, coherent longitudinal waves are excited in the flow region. PACS numbers: 52 essentially on a 2D plane include a Wigner lattice of electrons on a liquid-He surface [8], ions confined to a crystalline solid or a liquid [17]. Coulomb repulsion is shielded with a screening length D [27]. Dusty

Goree, John

417

arXiv:0712.2761v1[hep-ph]17Dec2007 Chiral phase transition in the presence of spinodal decomposition  

E-Print Network [OSTI]

phase are discussed for zero and non-zero quark masses. We focus on observables that probe the chiral fluctuations are calculated and analyzed. We show that the specific heat and charge susceptibilities diverge at the isothermal spinodal lines. We determine the scaling behavior and compute the critical exponent of the net

Weise, Wolfram

418

The HARPS search for southern extra-solar planets: XIV. Gl 176b, a super-Earth rather than a Neptune, and at a different period  

E-Print Network [OSTI]

A 10.24 days Neptune-mass planet was recently announced to orbit the nearby M2 dwarf Gl 176, based on 28 radial velocities measured with the HRS spectrograph on the Hobby-Heberly Telescope (HET). We obtained 57 radial velocities of Gl 176 with the ESO 3.6m telescope and the HARPS spectrograph, which is known for its sub-m/s stability. The median photon-noise standard error of our measurements is 1.1 m/s, significantly lower than the 4.7 m/s of the HET velocities, and the 4 years period over which they were obtained has much overlap with the epochs of the HET measurements. The HARPS measurements show no evidence for a signal at the period of the putative HET planet, suggesting that its detection was spurious. We do find, on the other hand, strong evidence for a lower mass 8.4 Mearth planet, in a quasi-circular orbit and at the different period of 8.78 days. The host star has moderate magnetic activity and rotates on a 39-days period, which we confirm through modulation of both contemporaneous photometry and chromospheric indices. We detect that period as well in the radial velocities, but it is well removed from the orbital period and no cause for confusion. This new detection of a super-Earth (2 Mearth < M sin(i) < 10 Mearth) around an M dwarf adds to the growing evidence that such planets are common around very low mass stars: a third of the 20 known planets with M sin(i) < 0.1 Mjup and 3 of the 7 known planets with M sin(i) < 10 Mearth orbit an M dwarf, in contrast to just 4 of the ~300 known Jupiter-mass planets.

T. Forveille; X. Bonfils; X. Delfosse; M. Gillon; S. Udry; F. Bouchy; C. Lovis; M. Mayor; F. Pepe; C. Perrier; D. Queloz; N. Santos; J. -L. Bertaux

2008-09-04T23:59:59.000Z

419

arXiv:1207.3969v1[astro-ph.SR]17Jul2012 Astronomy & Astrophysics manuscript no. hd163296 c ESO 2012  

E-Print Network [OSTI]

in this Herbig disk is confirmed by a line stacking analysis, enabled by the full PACS spectral scan, and by lines seen in Spitzer data. The line fluxes are analyzed using an LTE slab model including line opacity

Henning, Thomas

420

Comment on: How the result of a single coin toss can turn out to be 100 heads (arXiv:1403.2362)  

E-Print Network [OSTI]

The authors of [PRL 113 120404 (2014)] produce a classical measurement scheme that supposedly exhibits `anomalous' weak values. I show that their model is flawed due to an incorrect calculation of the noise parameter that follows from an incorrect definition of the weak value.

Aharon Brodutch

2014-10-30T23:59:59.000Z

Note: This page contains sample records for the topic "xiv-1 xiv morocco" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


421

arXiv:0905.0344v3[nlin.CD]3Sep2009 Regularity and singularity in solutions of the  

E-Print Network [OSTI]

`good' and `bad' intervals of [0, T ] which are interspersed with junction points (neutral) i. For large on the subject where more efficient routes to the construction of suitable weak solutions are in evidence [13, 14 intermittent data. Intermittency is characterized by violent surges or bursts away from averages in the energy

Gibbon, J. D.

422

arXiv:0712.2975v1[astro-ph]18Dec2007 X-ray properties of protostars in the Orion Nebula  

E-Print Network [OSTI]

Chandra Orion Ultradeep Project (COUP) data, we study the X-ray properties of stars in different, deep and almost simultaneous UBVI and JHK images taken, respectively, with WFI@2.2m ESO and ISPI@4m, we select a sample of "bona fide" Class II stars and a set of Class III stars with IR emission

423

arXiv:1104.5041v1[physics.ins-det]26Apr2011 A magnetically-driven piston pump for ultra-clean applications  

E-Print Network [OSTI]

is desirable, and is the subject of this paper. a)Now at Tesla Motors, Palo Alto CA, USA b)Electronic mail

Gratta, Giorgio

424

arXiv:1412.0916v1[quant-ph]2Dec2014 Quantum Trajectories based on the Weak Value  

E-Print Network [OSTI]

-0033, Japan 2 Theory Center, Institute of Particle and Nuclear Studies, High Energy Accelerator Research for an ensemble of parti- cles by combining the weak value of the momentum and the determination of the position of the position disturbs the momentum of the particle rendering the successive determination of the position

Tsutsui, Izumi

425

arXiv:cond-mat/0607335v113Jul2006 Molecular dynamics of shock fronts and their transitions in Lennard-Jonesium and Tin  

E-Print Network [OSTI]

in Lennard-Jonesium and Tin J. M. D. Lane and M. P. Marder Center for Nonlinear Dynamics, University of Texas for shocks in tin which agrees to within 6% with experimental data. We study the strong shock to elastic-plastic shock transition in tin and find that it is a continuous transition consistent with a transcritical

Texas at Austin. University of

426

arXiv:1205.2327v1[math.AP]10May2012 Impact of strong magnetic fields on collision mechanism for  

E-Print Network [OSTI]

applications in plasma physics concerns the energy production through thermo-nuclear fusion. The controlled of Texas at Austin, Texas 78712 USA. E-mail: gamba@math.utexas.edu 1 #12;We add the initial condition f (0

427

arXiv:1201.4607v1[astro-ph.SR]22Jan2012 Hinode Science Meeting: Unsolved Problems and Recent Insights  

E-Print Network [OSTI]

of the solar core energy production (of order 0.1%) could be carried by these particles, if they existed an additional channel for solar energy loss, as do the neutrinos. Axions are created in the solar core via nearly preserves the incident momentum and energy of the axion. The solar axions mostly result from

California at Berkeley, University of

428

arXiv:astro-ph/0612563v119Dec2006 Hard X-rays and Fluorescent Iron Emission from the Embedded  

E-Print Network [OSTI]

results of XMM-Newton X-ray observations of the infrared cluster lying near the NGC 2071 reflection nebula winds. One of the closest regions known to contain young high-mass stars is the infrared cluster near (Anthony-Twarog 1982; Brown et al. 1994). Near-infrared observations by Lada et al. (1991) revealed more

Guedel, Manuel

429

arXiv:0704.2794v1[physics.bio-ph]20Apr2007 Strong far field coherent scattering of ultraviolet radiation by holococcolithophores.  

E-Print Network [OSTI]

radiation by holococcolithophores. R. Quintero-Torres and J.L. Arag´on Centro de F´isica Aplicada y Tecnolog holococcolith structures have the ability to scatter the ultraviolet (UV) radiation. This property may represent and constitute a signifi- cant fraction of the phytoplankton in open ocean environ- ments. They impact greatly

430

arXiv:1311.5074v1[physics.ins-det]20Nov2013 Recent integral cross section validation measurements at the ASP facility  

E-Print Network [OSTI]

elemental foils were carried out using gamma spectrometry in a high efficiency, high-purity germanium (HPGe exposure to high intensity, high energy neutrons produced in such devices is certainly towards, if not at, the top of the list. The absence of avail- able high energy neutron irradiation testing facilities

431

arXiv:cond-mat/0412004v3[cond-mat.stat-mech]29May2006 Power laws, Pareto distributions and Zipf's law  

E-Print Network [OSTI]

. For instance, the distributions of the sizes of cities, earthquakes, solar flares, moon craters, wars an enormous dynamic range, sometimes many orders of magnitude. A classic example of this type of behaviour 000. Clearly this is quite different from what we saw for heights of people. And an even more

Terzi, Evimaria

432

arXiv:0807.4929v2[astro-ph]15Aug2008 Transiting Planets Proceedings IAU Symposium No. 253, 2008  

E-Print Network [OSTI]

radiative time constant 16 Planetary wind speed 36 Trojan companions 17,18 Artificial planet-sized objects. Property Refs. Orbital period 1,2 Planet-planet interactions (short-term) 19,20 Orbital inclination 1,2 Planet-planet interactions (long-term) 21,22 Planetary mass 1,2 Mutual orbital inclinations 20

Hillenbrand, Lynne

433

arXiv:0910.4460v2[math.QA]1Dec2009 LECTURES ON CANONICAL AND CRYSTAL BASES OF HALL  

E-Print Network [OSTI]

] into a geometric one. This geometric lift amounts to replacing the "naive" space of functions on the set MA" Hall algebra (or rather, Hall category) QA and the "algebraic" Hall algebra HA. Such a geometric lift. The relevant language for a general theory is likely to be [TV1]. Rather than embarking on the (probably risky

Proudfoot, Nicholas

434

arXiv:0905.1666v1[nlin.AO]11May2009 Nonlinear preferential rewiring in fixed-size networks as a diffusion process  

E-Print Network [OSTI]

as a diffusion process Samuel Johnson, Joaqu´in J. Torres, and Joaqu´in Marro Departmento de Electromagnetismo y

Johnson, Samuel

435

arXiv:0805.1309v1[cond-mat.dis-nn]9May2008 Functional Optimization in Complex Excitable Networks  

E-Print Network [OSTI]

Samuel Johnson, J. Marro, and Joaqu´in J. Torres Departamento de Electromagnetismo y F´isica de la

Johnson, Samuel

436

arXiv:1012.1813v1[cond-mat.dis-nn]8Dec2010 Enhancing neural-network performance via assortativity  

E-Print Network [OSTI]

Sebastiano de Franciscis, Samuel Johnson, and Joaqu´in J. Torres Departamento de Electromagnetismo y F

Johnson, Samuel

437

arXiv:0910.2940v1[nucl-th]15Oct2009 Structure of even-even nuclei using a mapped collective  

E-Print Network [OSTI]

structure, in the sense that it is well-founded in its methodology and is applicable across the chart of nuclides. The most promising starting point is self-consistent mean-field, but the theory must be extended

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

438

arXiv:1005.4579v1[astro-ph.EP]25May2010 Astronomy & Astrophysics manuscript no. 14717v2 c ESO 2010  

E-Print Network [OSTI]

at a constant resolution of 1.4 GHz across the whole band. The flux from the planet is such that the instrument was operated in"bright source" mode to prevent saturation of the detectors. This was the first successful use) and ground-based (e.g. Lellouch et al, 1991, Krasnopolsky, 2007) show an aver- age abundance of 700 ppm. One

Naylor, David A.

439

arXiv:0711.2528v2[astro-ph]23Jan2008 Production of Neutrinos and Secondary Electrons in Cosmic  

E-Print Network [OSTI]

of secondary electrons in a young shell-type SNR, RX J1713.7-3946, which is a measure of the age, the spectral-mG fields recently invoked to explain the X-ray flux variations are unlikely to extend over a large fractionCube-like detector that are induced by muon neutrinos from high-energy -ray sources such as RX J1713.7-3946, Vela Jr

440

arXiv:1107.3747v1[cond-mat.mes-hall]19Jul2011 Terahertz radiation driven chiral edge currents in graphene  

E-Print Network [OSTI]

in graphene J. Karch,1 C. Drexler,1 P. Olbrich,1 M. Fehrenbacher,1 M. Hirmer,1 M. M. Glazov,2 S. A. Tarasenko photocurrents induced in single layer graphene samples by illumination of the graphene edges with circularly of the conductivity type and the momentum scattering time of the charge carriers in the graphene edge vicinity. PACS

Ganichev, Sergey

Note: This page contains sample records for the topic "xiv-1 xiv morocco" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


441

arXiv:1306.3100v1[astro-ph.EP]13Jun2013 Direct Imaging Search for Extrasolar Planets in the  

E-Print Network [OSTI]

yamamoto@iral.ess.sci.osaka-u.ac.jp shibai@iral.ess.sci.osaka-u.ac.jp konishi@iral.ess.sci.osaka-u.ac.jp sudo@iral.ess.sci.osaka-u.ac.jp misato@iral.ess.sci.osaka-u.ac.jp sumi@iral.ess.sci.osaka-u.ac.jp 2

Henning, Thomas

442

arXiv:0909.3183v1[astro-ph.SR]17Sep2009 Astronomy & Astrophysics manuscript no. dustamorphv5.0 c ESO 2011  

E-Print Network [OSTI]

with the circumstellar disk. We show that the fluxes around 1 AU and ion energies of the present solar wind Zentrum M¨unchen, German Research Center for Environmental Health, Ingolst¨adter Landstra?e 1, 85758, Switzerland Received ... / Accepted ... ABSTRACT Aims. High-energy irradiation of the circumstellar material

Guedel, Manuel

443

arXiv:0904.0799v1[physics.flu-dyn]5Apr2009 Bistability and hysteresis of dipolar dynamos generated by turbu-  

E-Print Network [OSTI]

and it is believed to be responsible for the mag- netic fields of cosmic objects including the sun and most planets distribution TS = T0 - d2 r2 /2 and a gravity field in the form g = -dr, where rd is the length of the posi- tion vector with respect to the center of the sphere. This form of temperature profile alludes

Schmidt, Matthias

444

arXiv:1102.0242v3[astro-ph.SR]24Jun2012 A Bayesian approach to comparing theoretic models to observational data  

E-Print Network [OSTI]

. Gallagher3 ABSTRACT Solar flares are large-scale releases of energy in the solar atmosphere, which thermal energy and/or using non-thermal energy according to the energy release mechanisms (Mariska et al. 1993). In the thermal energy model, heat is unleashed in the coronal portion of the loop (possibly

California at Berkeley, University of

445

arXiv:1006.5247v4[astro-ph.SR]4Dec2011 This is an emulation of Solar Physics ,  

E-Print Network [OSTI]

fields, Corona 1 Space Sciences Laborary, University of California, Berkeley, CA, USA email: fisher@ssl.berkeley.edu, bercik@ssl.berkeley.edu, welsch@ssl.berkeley.edu, hhudson@ssl.berkeley.edu #12;2 G.H. Fisher et al. 1

California at Berkeley, University of

446

arXiv:astro-ph/0409377v115Sep2004 The Search for Anisotropy in the Arrival Directions of Ultra-High Energy  

E-Print Network [OSTI]

Center present in its events with energies around 1018 eV [4]. This result seemed to be corroborated predictions mentioned above. Additionally, over the past decade, the search for sources of Ultra-High Energy-High Energy Cosmic Rays Observed by the High Resolution Fly's Eye Detector in Monocular Mode Benjamin T

447

arXiv:1010.3469v2[cs.IT]19Oct2010 1 Decoding the `Nature Encoded' Messages for  

E-Print Network [OSTI]

generators (DEGs, like solar panels, micro- turbines or wind turbines) and multiple loads. A microgrid can: An illustration of the communication procedure and dynamic system. medium, fading, noise and interference may

Qiu, Robert Caiming

448

arXiv:hep-th/0003076v322Aug2000 Preprint typeset in JHEP style. -PAPER VERSION hep-th/0003076 HUTP-00/A008  

E-Print Network [OSTI]

at long distances and gives rise to scalar anti-gravity. The holographic description shows that at large

Terning, John

449

arXiv:0910.1428v1[hep-ex]8Oct2009 Longitudinal Spin Transfer to and Hyperons in Polarized Proton-Proton  

E-Print Network [OSTI]

-Proton Collisions at s = 200 GeV B. I. Abelev,8 M. M. Aggarwal,30 Z. Ahammed,47 A. V. Alakhverdyants,17 B. D

Llope, William J.

450

arXiv:0907.2721v3[nucl-ex]22Sep2009 Neutral Pion Production in Au+Au Collisions at  

E-Print Network [OSTI]

. I. Abelev,8 M. M. Aggarwal,30 Z. Ahammed,47 A. V. Alakhverdyants,17 B. D. Anderson,18 D. Arkhipkin,3

Llope, William J.

451

arXiv:0812.1063v2[nucl-ex]2Mar2009 Observation of Two-source Interference in the Photoproduction Reaction  

E-Print Network [OSTI]

Reaction AuAu AuAu0 B. I. Abelev,9 M. M. Aggarwal,31 Z. Ahammed,47 B. D. Anderson,19 D. Arkhipkin,13 G. S

Llope, William J.

452

arXiv:0807.3269v1[nucl-ex]21Jul2008 Beam-Energy and System-Size Dependence of Dynamical Net Charge Fluctuations  

E-Print Network [OSTI]

Fluctuations B. I. Abelev,1 M. M. Aggarwal,2 Z. Ahammed,3 B. D. Anderson,4 D. Arkhipkin,5 G. S. Averichev,6 Y

Llope, William J.

453

arXiv:0903.1296v2[nucl-ex]4Aug2009 Pion Interferometry in Au+Au and Cu+Cu Collisions at  

E-Print Network [OSTI]

.4 and 200 GeV B. I. Abelev,8 M. M. Aggarwal,30 Z. Ahammed,47 B. D. Anderson,18 D. Arkhipkin,12 G. S

Llope, William J.

454

arXiv:1308.0623v1[physics.bio-ph]2Aug2013 Asymptotic Cellular Growth Rate as the Effective Information Utilization Rate  

E-Print Network [OSTI]

Information Utilization Rate R. Pugatch,1 N. Barkai,2 and T. Tlusty1 1 School of Natural Sciences, Simons

Tlusty, Tsvi

455

arXiv:1101.0536v1[hep-ph]3Jan2011 The PDF4LHC Working Group Interim Report  

E-Print Network [OSTI]

, Francesco Cerutti7, Amanda Cooper-Sarkar8, Albert de Roeck9, Luigi Del Debbio3, Joel Feltesse10, Stefano.22 Computation of Monte Carlo PDF uncertainties . . . . . . . . . . .

Lunds Universitet,

456

arXiv:1105.4540v3[cs.IT]18Oct2011 On the Limits of Sequential Testing in High  

E-Print Network [OSTI]

distributions f0 and f1. The main contribu- tions are 1) to present a necessary condition for success of any

Nowak, Robert

457

arXiv:1405.1915v1[quant-ph]8May2014 Tunable coupler for superconducting Xmon qubits: Perturbative nonlinear model  

E-Print Network [OSTI]

a single flux-biased Josephson junction and acts as a tunable current divider. We calculate the effective. 1. We begin by discussing the circuit in the harmonic approximation. Josephson junctions (crosses magnetic flux bias. There are four active nodes (black dots) in this circuit. The Josephson junctions

Martinis, John M.

458

arXiv:0811.3640v2[hep-lat]21Dec2008 The B semileptonic form factor from three-flavor lattice  

E-Print Network [OSTI]

particle physics experiments to date, it cannot account for gravity, dark matter and dark energy and R.S. Van de Water1, (Fermilab Lattice and MILC Collaborations) 1 Fermi National Accelerator, or the large matter-antimatter asymmetry of the universe. Thus we know that it is incomplete, and expect new

Bernard, Claude

459

arXiv:0811.3437v1[cond-mat.dis-nn]20Nov2008 Infinitely Robust Order and Local Order-Parameter Tulips  

E-Print Network [OSTI]

. Nihat Berker1,3,5 1 Department of Physics, Ko¸c University, Sariyer 34450, Istanbul, Turkey, 2 Martin

Gozuacik, Devrim

460

arXiv:0811.0025v1[cond-mat.dis-nn]31Oct2008 Quenched-Vacancy Induced Spin-Glass Order  

E-Print Network [OSTI]

¨ulpinar1,3 and A. Nihat Berker2,3,4 1 Department of Physics, Dokuz Eyl¨ul University, Buca 35160, Izmir

Gozuacik, Devrim

Note: This page contains sample records for the topic "xiv-1 xiv morocco" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


461

The VMC Survey - XIV. First results on the look-back time star-formation rate tomography of the Small Magellanic Cloud  

E-Print Network [OSTI]

We analyse deep images from the VISTA survey of the Magellanic Clouds in the YJKs filters, covering 14 sqrdeg (10 tiles), split into 120 subregions, and comprising the main body and Wing of the Small Magellanic Cloud (SMC). We apply a colour--magnitude diagram reconstruction method that returns their best-fitting star formation rate SFR(t), age-metallicity relation (AMR), distance and mean reddening, together with 68% confidence intervals. The distance data can be approximated by a plane tilted in the East-West direction with a mean inclination of 39 deg, although deviations of up to 3 kpc suggest a distorted and warped disk. After assigning to every observed star a probability of belonging to a given age-metallicity interval, we build high-resolution population maps. These dramatically reveal the flocculent nature of the young star-forming regions and the nearly smooth features traced by older stellar generations. They document the formation of the SMC Wing at ages <0.2 Gyr and the peak of star formation ...

Rubele, Stefano; Kerber, Leandro; Cioni, Maria-Rosa L; Piatti, Andres E; Zaggia, Simone; Bekki, Kenji; Bressan, Alessandro; Clementini, Gisella; de Grijs, Richard; Emerson, Jim P; Groenewegen, Martin A T; Ivanov, Valentin D; Marconi, Marcella; Marigo, Paola; Moretti, Maria-Ida; Ripepi, Vincenzo; Subramanian, Smitha; Tatton, Benjamin L; van Loon, Jacco Th

2015-01-01T23:59:59.000Z

462

arXiv:hep-ex/0212067v130Dec2002 Search for e from the Sun at Super-Kamiokande-I  

E-Print Network [OSTI]

Alamos National Laboratory, Los Alamos, NM 87544, USA m Department of Physics and Astronomy, Louisiana Park, MD 20742, USA o Department of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139

Tokyo, University of

463

arXiv:nlin.CD/0607029v114Jul2006 APS/123-QED Modeling Time Series of Real Systems using Genetic Programming  

E-Print Network [OSTI]

Programming Dilip P. Ahalpara Institute for Plasma Research, Near Indira Bridge, Gandhinagar-382428, India

Fernandez, Thomas

464

arXiv:1210.0551v1[physics.atom-ph]1Oct2012 Resonant Few-Photon Excitation of a Single-Ion Oscillator  

E-Print Network [OSTI]

, initially cooled to the Doppler limit, quickly phase locks to the drive and builds up coherent oscillations and experiment, we find that phase-locking behavior allows efficient energy trans- fer to the ion oscillator for state readout. Because the driven oscillator phase locks such that photon scattering transfers maximum

Odom, Brian

465

arXiv:0806.3050v1[physics.flu-dyn]18Jun2008 Rayleigh-Plateau instability causes the crown splash  

E-Print Network [OSTI]

, cooling, and combustion. In the crown splash parameter regime, the splash pattern is highly regular. We the air-sea interface [1], cooling [2], coatings [3], and combus- tion [4]. The spatial pattern and size in Edgerton's iconic photograph Milk Coronet [9], and show that number of secondary droplets is governed

Eggers, Jens

466

arXiv:0706.2031v1[physics.hist-ph]14Jun2007 APS/123-QED Relativity tests by complementary rotating Michelson-Morley experiments  

E-Print Network [OSTI]

of Western Australia, School of Physics M013, 35 Stirling Hwy., Crawley 6009 WA, Australia Peter Wolf LNE Perth, Australia) uses microwave whispering-gallery sapphire resonators. Within the standard model with a first glimpse of effects of a future theory of quantum gravity in the low-energy limit [1, 2, 3]. Since

Peters, Achim

467

arXiv:0709.0838v1[cond-mat.stat-mech]6Sep2007 Modeling long-range cross-correlations in  

E-Print Network [OSTI]

, Rijeka, Croatia bZagreb School of Economics and Management, Zagreb, Croatia cDepartment of Physics, Faculty of Science, University of Zagreb, Zagreb, Croatia dCenter for Polymer Studies and Department

Podobnik, Boris

468

arXiv:1003.1076v1[math-ph]4Mar2010 Rigorous scaling law for the heat current in disordered  

E-Print Network [OSTI]

as the integral over oscillation frequency w of the modes: J(µ) n = (T1 - Tn) R vT µ,n(w)An(w) · · · A1(w)vµ,1(w

Boyer, Edmond

469

arXiv:1005.5094v2[math.DS]15Sep2010 Singular sets of holonomy maps for algebraic  

E-Print Network [OSTI]

group. We cannot hope, for a general algebraic foliation of the plane, that the holon- omy relation can

Deroin, Bertrand

470

arXiv:cond-mat/0007431v57Jan2001 Impurity in a d-wave superconductor: Kondo effect and STM spectra  

E-Print Network [OSTI]

is a localized "holon" which binds the moment of a S = 1/2 "spinon". At larger doping, a related picture can

471

arXiv:hep-ph/0608147v113Aug2006 NUHEP-TH/06-06 Neutrino Phenomenology of Very Low-Energy Seesaws  

E-Print Network [OSTI]

), in order to search for Neutrinoless Double Beta Decay of Te. Runs lasting up to 10 000 h have been

472

arXiv:0808.1702v1[hep-ph]12Aug2008 NUHEP-TH/08-04 Minimally Allowed 0 Rates Within an Anarchical Framework  

E-Print Network [OSTI]

, Evanston, IL 60208, USA Neutrinoless double beta decay (0) is the only realistic probe of the Majorana of the neutrino is an important issue that must be addressed experimentally. Neutrinoless double beta decay (0

473

arXiv:1109.1046v1[physics.ins-det]6Sep2011 Xenon purity analysis for EXO-200 via mass  

E-Print Network [OSTI]

for the neutrinoless double beta decay of 136 Xe[1]. The first such experiment, known as EXO-200, is currently double beta decay half life of 6.4 ? 1025 years, equivalent to a Majorana neutrino mass of order 100 me collecting data at the WIPP facility near Carlsbad, New Mexico[2]. EXO-200 is sensitive to a neutrinoless

Gratta, Giorgio

474

arXiv:math/0510577v1[math.AP]26Oct2005 Regularity of the distance function to the boundary  

E-Print Network [OSTI]

coordinates introduced in section 3 of [1] about a given normal geodesic , going from a point y - 1, and Latin letters i, j range from 1 to n. (ten; en) 1, (2) j (ten; en) 0, (3) #12;3 v (ten; en) 0, vn (ten; en) 1, (4) jvk (ten; en) 0, (5) vj vn (ten; en) 0, (6) jn (ten; en) 0. (7

Li, YanYan

475

arXiv:1410.3874v1[astro-ph.GA]14Oct2014 (To appear in the Astrophysical Journal)  

E-Print Network [OSTI]

using LATEX style emulateapj v. 5/2/11 QUANTIFYING THE HEATING SOURCES FOR MID-INFRARED DUST EMISSIONS spiral galaxy M 81 (NGC 3031): (a) I8 or I24, the surface brightness of the mid-infrared emission dust grains heated by evolved stars, and (c) IH, a nominal surface brightness of the H line emission

Baes, Maarten

476

arXiv:1102.1277v1[cond-mat.mes-hall]7Feb2011 Wigner crystal in snaked nanochannels  

E-Print Network [OSTI]

helium [3], cold ions in radio- frequency traps [4] and dusty plasma in laboratory or in space [5 of charge storage in electrochemical capacitors, or supercapacitors, which start to have important industrial applications [13, 14]. In these systems, charged ions are stored in nanopores at the surface

Shepelyansky, Dima

477

arXiv:1402.4675v2[cs.NI]5Oct2014 IEEE 802.11ah: The Wi-Fi Approach  

E-Print Network [OSTI]

scenarios such as agriculture monitoring, smart metering, industrial automation and animal monitoring, in 2017. The communication technologies currently used for M2M applications can be classified in two and complexity of the applications and en- vironments. As for mobile networks, M2M communications are currently

Bellalta, Boris

478

arXiv:0902.3733v1[physics.flu-dyn]21Feb2009 APS/123-QED Rotating electrohydrodynamic flow in a suspended liquid film  

E-Print Network [OSTI]

film motor, emphasizing that it represents a new type of engine. They also proposed that it could be ex of the liquid film motor [1, 2]. PACS numbers: 47.32.Ef, 68.15.+e, 47.57.jd Keywords: electrohydrodynamic flow), but it can not exist for very thin films. An important general result of our paper is the demonstration

479

arXiv:cond-mat/0504696v126Apr2005 Adsorption and dissociation of hydrogen molecules on bare and functionalized carbon  

E-Print Network [OSTI]

and dissociation into hydrogen atoms to complete the current cycle in the fuel cell to produce the desired numbers: 73.22.-f, 61.46.+w, 68.43.Bc I. INTRODUCTION Fuel cells have been a real challenge for clean. Once hydrogen molecule is chosen as potential fuel, its storage, easy dis- charge for consumption

Yildirim, Taner

480

arXiv:cond-mat/0606426v115Jun2006 Large enhancement of the thermopower in NaxCoO2 at high Na doping  

E-Print Network [OSTI]

or Peltier con- ductivity). Whereas the thermopower S = / is the quantity usually reported, we have found. Crystals of NaxCoO2 grow as either bilayer or tri-layer structures (2 and 3 CoO2 layers per unit cell

Ong, N. P.

Note: This page contains sample records for the topic "xiv-1 xiv morocco" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


481

arXiv:nucl-th/0412037v110Dec2004 Transport Theories for Heavy Ion Collisions in the 1 AGeV  

E-Print Network [OSTI]

. Danielewicz8 , C. Fuchs9 , T. Gaitanos10 , C.M. Ko6 , A. Larionov5 , M. Reiter4 , Gy. Wolf11 , J. Aichelin2 1

Heger, Alexander

482

arXiv:1210.0846v3[physics.atom-ph]21Dec2012 Rb optical resonance inside a random porous medium  

E-Print Network [OSTI]

-size volumes such as hollow-core optical fibers [1,2], wave-guides [3], thin cells [4­8] or interstitial cavities in nano-structures such as opals [9]. Positron- ium atoms were created and observed in porous fluorescence. We call this the "integrating- sphere effect" (ISE) by analogy with an extended de- tector

Paris-Sud XI, Université de

483

arXiv:1107.1270v3[cs.LG]4Mar2012 Journal of Machine Learning Research () Submitted 6/11; Published  

E-Print Network [OSTI]

to a maximum weight spanning tree problem and is thus computationally efficient. However, a general. Willsky willsky@mit.edu Stochastic Systems Group Laboratory for Information and Decision Systems and Jmin is the minimum (absolute) edge potential of the graphical model. The sufficient conditions

Willsky, Alan S.

484

arXiv:0904.0927v1[math.AG]6Apr2009 CALCULATING THE PARABOLIC CHERN CHARACTER OF A  

E-Print Network [OSTI]

characters chP ar 1 (E), chP ar 2 (E) and chP ar 3 (E). The basic idea is to use the formula given in [IS2

Simpson, Carlos

485

arXiv:0801.3991v1[cond-mat.soft]25Jan2008 Superdiffusion and non-Gaussian statistics in a driven-dissipative  

E-Print Network [OSTI]

energy is set by a balance of driving forces and dissipation. Random motion is characterized using, Iowa City, Iowa 52242 (Dated: January 25, 2008) Abstract Anomalous diffusion and non

Goree, John

486

arXiv:hep-ph/0102297v32Mar2001 Preprint typeset in JHEP style. -HYPER VERSION SCIPP-01/10  

E-Print Network [OSTI]

USA E-mail: haber@scipp.ucsc.edu Abstract: A light CP-even Higgs boson with mh 10 GeV could explain Higgs boson limit: cos( - ) = 0 8 3. CESR and LEP constraints on a light Higgs boson 8 4. Final Results

California at Santa Cruz, University of

487

Linear Algebra. By Peter Lax. John Wiley, 1997, xiv + 250 pp., $89.95. ISBN 0-471-11111-2. Reviewed by Mark A. Kon  

E-Print Network [OSTI]

;solving systems of linear equations, finding eigenvalues, and inverting matrices has led to a torrent both every- where and nowhere in advanced mathematics. Though by implication linear algebra focuses on finite dimensional spaces, functional analysis has to an extent co-opted and appropriated much

Kon, Mark

488

arXiv:1404.2350v1[cond-mat.stat-mech]9Apr2014 The two-point resistance of a cobweb with a superconducting  

E-Print Network [OSTI]

with a superconducting boundary Zhi-Zhong Tan Department of Physics, Nantong University, Nantong 226007, China J. W as a single summation. Key words: m ? n cobweb; superconducting boundary, two-point resistance; matrix Laplacian approach [7]. In this paper we consider the cobweb network with a superconducting boundary

Essam, John W.

489

Reply to Benestad's comment on "Discussions on common errors in analyzing sea level accelerations, solar trends and global warming" by Scafetta (2013), arXiv:1306.2011  

E-Print Network [OSTI]

Herein I respond to the criticism and to the complains by Benestad (2013) of Scafetta (2013a) that I found misleading and not tenable. More significantly, Benestad (2013) did not find any physical nor mathematical error in Scafetta (2013a). Thus, Scafetta (2013a) scientific results remain fully confirmed.

Scafetta, Nicola

2013-01-01T23:59:59.000Z

490

arXiv:1401.3007v1[astro-ph.EP]13Jan2014 Astronomy & Astrophysics manuscript no. GChen_wasp43_R1 c ESO 2014  

E-Print Network [OSTI]

Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences host star. We aim at securing a broad-band transmission spectrum and detecting its near and satellites: atmospheres ­ planets and satellites: fundamental parameters ­ techniques: photometric 1

Henning, Thomas

491

arXiv:1009.4194v2[cond-mat.str-el]20Jun2011 Jastrow-Correlated Wavefunctions for Flat-Band Lattices  

E-Print Network [OSTI]

terahertz imaging as a method of screening passengers for explosives at air- ports. For military for the surging demand of high performance terahertz detectors in recent years. Charge transport properties3 the photoexcited carriers with energy h larger than the band-edge offset between the doped emit- ter layer

Scarola, Vito

492

arXiv:1406.4193v1[quant-ph]16Jun2014 Atomic Focusing by Quantum Fields: Entanglement Properties  

E-Print Network [OSTI]

, lithography, single atom manipulation, trace gas analysis and ultracold chemistry [3]. In addition, the area of the electromagnetic field. We extend the analysis of this quantum lens to the study of another essentially quantum the search for the matter wave Gouy phase in different systems: Bose-Einstein condensates [7], electron

Boyer, Edmond

493

A review of "The Bellicose Dove: Claude Brousson and Protestant Resistance to Louis XIV, 1645-1698" by Walter C. Utt and Brian Strayer.  

E-Print Network [OSTI]

246 SEVENTEENTH-CENTURY NEWS society, will do well to reserve for themselves the table nearest the History of Parliament at their favorite library. Walter C. Utt and Brian Strayer. The Bellicose Dove: Claude Brousson and Protestant Resistance.... As edited and completed by Brian Strayer, this work reveals both a Brousson utterly unyielding and indefatigable in his polemics against what he considered the idolatry and the multiplicity of errors of Ca- tholicism, and a Brousson much more changeable...

Thomas Worcester

2004-01-01T23:59:59.000Z

494

arXiv:cond-mat/0611020v2[cond-mat.str-el]3Jun2007 Numerical solution of the Holstein polaron  

E-Print Network [OSTI]

Alamos National Laboratory, Los Alamos, New Mexico 87545, U.S.A. sat@lanl.gov 1 Introduction is the absorption or emission of a phonon by the electron with a simultaneous change of the electron state. From the polaron ground state is still extended allowing, in principle, for coherent transport although

Fehske, Holger

495

1 arXiv:nucl-th/0305016v1 7 May 2003Non-Scissors-Mode Behaviour of Isovector Magnetic Dipole Orbital Transitions Involving Isospin Transfer  

E-Print Network [OSTI]

We study the response of isovector orbital magnetic dipole (IOMD) transitions to the quadrupole-quadrupole (Q Q) interaction, to the isospinconserving pairing interaction (ICP) and to combinations of both. We find qualitatively different behaviours for transitions in which the final isospin differs from the initial isospin versus cases where the two isospins are the same. For N = Z even-even nuclei with J ? = 0 +, T = 0 ground states such as 8Be and 20Ne, the summed T = 0 ? T = 1 IOMD from the ground state to all the J = 1, T = 1 states in the 0h? space does not vanish when the Q Q interaction is turned off. The pairing interaction (ICP) alone leads to a finite transition rate. For nuclei with J = 0 +, T = 1 ground states such 2 as 10Be and 22Ne, the summed T = 1 ? T = 1 IOMD does vanish when the Q Q interaction is turned off, as is expected in a good scissors-mode behaviour. However this is not the case for the corresponding sum of the T = 1 ? T = 2 IOMD transitions. In 22Ne (but not in 10Be) the sum of the T = 1 ? T = 2 IOMD transitions is remarkably insensitive to the strengths of both the Q Q and the ICP interactions. In 22Ne an energy weighted-sum is similarly insensitive. All our calculations were carried out in the 0h? space. I.

S. Aroua; L. Zamick; Y. Y. Sharon; E. Moya De Guerra; M. S. Fayache; P. Sarriguren

2008-01-01T23:59:59.000Z

496

Note on: "Inevitability of Plate Tectonics on Super-Earths" by Valencia, O Connell and Sasselov, arXiv preprint 0710.0699  

E-Print Network [OSTI]

Valencia et al. recently claimed that the mass of a Super-Earth (SE) is a sole factor in determining whether a SE is tectonically active or not. However, mass resolving astrometry is unable to discern between a SE and its moons if any. The fact that no exomoons have been discovered yet is rather a matter of instrumentation imperfection at the present, not of physical absence of exomoons. This, with recently discovered relationships between geometric and physical properties in astronomical bodies (Transiting planets; the Earth) makes it impossible to know yet if the Wageners (here constraining) supposition on somehow-tidally caused tectonics holds universally or not also.

Omerbashich, Mensur

2008-01-01T23:59:59.000Z

497

This is a preprint of a paper which appeared in the Proceedings of RoboCup 2010: Robot Soccer World Cup XIV  

E-Print Network [OSTI]

limited mobility than a wheeled system, like in the small size or mid size leagues. Fur- ther, the camera von Stryk Simulation, Systems Optimization and Robotics Group Department of Computer Science supporting a teammate manipulating the ball is proposed and evaluated. This approach has been derived from

Stryk, Oskar von

498

arXiv:astro-ph/0603630v123Mar2006 X-ray and optical bursts and flares in YSOs: results from a 5-day  

E-Print Network [OSTI]

with similar energy production and emission mechanism), the phenomenol- ogy for CTTS and Class I objects

Micela, Giusi

499

Prostanoids. XIV. (+/-)-11-Deoxy-13,14-dihydro-13-thia-16-aryloxy-17,18,19,20-tetranorprostaglandins-E/sub 1/ - new hybrid prostaglandin analogs  

SciTech Connect (OSTI)

11-Deoxy-13,14-dihydro-13-thia-16-aryloxy-17,18,19,20-tetranorprostaglandin-E/sub 1/ and their diastereomers were synthesized by the conjugate 1,4-addition of 2-hydroxy-3-aryloxypropanethiols to 2-(6-ethoxycarbonylhexyl)-2-cyclopenten-1-one.

Tolstikov, G.A.; Miftakhov, M.S.; Danilova, N.A.; Shitikova, O.V.; Khalilov, L.M.; Panasenko, A.A.

1986-11-10T23:59:59.000Z

500

arXiv:1207.3231v1[math.OC]13Jul2012 1 An Overview of Recent Progress in the Study of  

E-Print Network [OSTI]

(UAVs), unmanned ground vehicles (UGVs) and unmanned underwater vehicles (UUVs), has been a very active journals since 2006. Distributed coordination of multiple vehicles, including unmanned aerial vehicles for controlling a single vehicle, albeit higher-dimensional and complex, has become relatively mature and has

Ren, Wei