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1

Morocco  

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

XIV. Morocco (Including Western Sahara and Mauritania) EIA/ARI World Shale Gas and Shale Oil Resource Assessment XIV. Morocco (Including Western Sahara and Mauritania) EIA/ARI World Shale Gas and Shale Oil Resource Assessment May 17, 2013 XIV-1 XIV. MOROCCO (INCLUDING WESTERN SAHARA AND MAURITANIA) SUMMARY In addition to large accumulations of Late-Cretaceous immature oil shale (kerogen) at depths suitable for surface mining 1 , Morocco and its two neighboring countries, Mauritania and Western Sahara, also possess organic-rich Silurian- and Devonian-age shale gas and shale oil potential in the Tindouf and Tadla basins, Figure XIV-1. Mapping and resource characterization of these shales is challenging because regional deformation, erosion and subsidence of the shale deposits have led to their discontinuous and complex present day distribution. Figure XIV-1. Shale Gas Basins of Morocco, Western Sahara and Mauritania

2

Immosolar Morocco | Open Energy Information  

Open Energy Info (EERE)

Immosolar Morocco Immosolar Morocco Name Immosolar Morocco Place Casablanca, Morocco Sector Solar Product Solar energy systems Phone number (+212) 22 40 89 50 Website http://www.immosolar.com/ Coordinates 33.605381°, -7.631949° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":33.605381,"lon":-7.631949,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

3

Shell Morocco | Open Energy Information  

Open Energy Info (EERE)

Morocco Morocco Jump to: navigation, search Logo: Shell Morocco Name Shell Morocco Address Immeuble Le Zenith II Place Casablanca, Morocco Zip 20190 Product Production and Distribution of Lubricants for motorists and industries; Storage and Distribution of Oils and LPG; Marine and Aviation; Off-Shore Exploration Year founded 1922 Phone number +212 (0) 522 972727 Website http://www.shell.com/home/cont Coordinates 38.959732°, -77.3419799° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":38.959732,"lon":-77.3419799,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

4

Morocco: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Morocco: Energy Resources Morocco: Energy Resources Jump to: navigation, search Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"TERRAIN","zoom":5,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"390px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":32,"lon":-5,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

5

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

Open Energy Info (EERE)

CSP programs of five countries in the Middle East and North Africa: Algeria, Egypt, Jordan, Morocco, and Tunisia." References "Middle East and North Africa Regional Program...

6

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

Open Energy Info (EERE)

Morocco-Facilitating Implementation and Readiness for Mitigation (FIRM) Morocco-Facilitating Implementation and Readiness for Mitigation (FIRM) Jump to: navigation, search Logo: Morocco-Facilitating Implementation and Readiness for Mitigation (FIRM) Name Morocco-Facilitating Implementation and Readiness for Mitigation (FIRM) Agency/Company /Organization United Nations Environment Programme (UNEP) Partner Global Environment Facility (GEF), Government of Denmark Sector Climate, Energy, Land Topics Adaptation, Co-benefits assessment, - Environmental and Biodiversity, Finance, Implementation, Low emission development planning Website http://www.unep.org/climatecha Program Start 2011 Program End 2013 Country Morocco UN Region Central America References Facilitating Implementation and Readiness for Mitigation (FIRM)[1] "The Government of Denmark will provide US$6 million to the new programme

7

Morocco-UNEP Green Economy Advisory Services | Open Energy Information  

Open Energy Info (EERE)

Morocco-UNEP Green Economy Advisory Services Morocco-UNEP Green Economy Advisory Services Jump to: navigation, search Logo: Morocco-UNEP Green Economy Advisory Services Name Morocco-UNEP Green Economy Advisory Services Agency/Company /Organization United Nations Environment Programme (UNEP) Partner German Agency for International Cooperation (GIZ), Global Green Growth Knowledge Platform (GGKP), Green Jobs Initiative, United Nations Development Programme (UNDP), United Nations Department of Economic and Social Affairs (UNDESA) Sector Climate, Energy, Land, Water Focus Area People and Policy Topics Co-benefits assessment, Low emission development planning, -LEDS Country Morocco Northern Africa References UNEP Green Economy Advisory Services[1] Overview "UNEP Green Economy Advisory Services consist of policy advice, technical

8

Morocco-UNEP Risoe Technology Needs Assessment Program | Open Energy  

Open Energy Info (EERE)

Morocco-UNEP Risoe Technology Needs Assessment Program Morocco-UNEP Risoe Technology Needs Assessment Program Jump to: navigation, search Name Morocco-UNEP Risoe-Technology Needs Assessment Program Agency/Company /Organization UNEP-Risoe Centre Sector Energy Topics Background analysis, Low emission development planning, -Roadmap, Pathways analysis Website http://tech-action.org/ Country Morocco Northern Africa References UNEP Risoe-Technology Needs Assessment Program[1] Abstract UNEP DTIE in collaboration with the UNEP Risoe Centre will provide targeted financial, technical and methodological support to assist a total of 35 to 45 countries to conduct TNA projects Overview "Technology needs assessment (TNA) is a set of country-driven activities that identifies and determines the mitigation and adaptation technology

9

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

Open Energy Info (EERE)

report on climate change impacts on crop yields in Morocco. It is part of a larger study led by the World Bank and the Government of Morocco on climate change and agriculture. The...

10

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 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 Agricultural Sector Agency/Company /Organization World Bank Sector Land Focus Area Agriculture Topics Co-benefits assessment, Background analysis Resource Type Lessons learned/best practices Website http://www.fao.org/nr/climpag/ Country Morocco UN Region Northern Africa References Morocco Study on the Impact of Climate Change on the Agricultural Sector[1] Summary "The present document is an interim report on climate change impacts on crop yields in Morocco. It is part of a larger study led by the World Bank and the Government of Morocco on climate change and agriculture. The yield

11

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

Open Energy Info (EERE)

Morocco-Low Carbon Development Planning in the Power Sector Morocco-Low Carbon Development Planning in the Power Sector Jump to: navigation, search Logo: Morocco-Low Carbon Development Planning in the Power Sector Name Morocco-Low Carbon Development Planning in the Power Sector Agency/Company /Organization Energy Sector Management Assistance Program of the World Bank Sector Energy Topics Low emission development planning Website http://www.esmap.org/esmap/nod Country Morocco UN Region Northern Africa References ESMAP[1] Overview "This new program was initiated in 2010 and aims to provide clients with analytical support to develop capacity for low-carbon development in power sector planning. It employs a learning-by doing approach with pilot activities in two countries in the initial stage (Nigeria and Morocco -

12

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

Open Energy Info (EERE)

Morocco-The World Bank Partnership for Market Readiness (PMR) Morocco-The World Bank Partnership for Market Readiness (PMR) Jump to: navigation, search Logo: Morocco-The World Bank Partnership for Market Readiness (PMR) Name Morocco-The World Bank Partnership for Market Readiness (PMR) Agency/Company /Organization World Bank Partner Australia, Denmark, EC, Germany, Japan, Netherlands, Norway Spain, Switzerland, UK, and US Sector Climate, Energy Focus Area Non-renewable Energy, Buildings, Economic Development, Energy Efficiency, Goods and Materials, Greenhouse Gas, Grid Assessment and Integration, Industry, Offsets and Certificates, People and Policy, Transportation Topics Baseline projection, Finance, GHG inventory, Implementation, Low emission development planning, Market analysis, Policies/deployment programs

13

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

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

2011 Summary: , Algeria, Bahrain, Bangladesh, Egypt, Eritrea, Indonesia, Iran, Iraq, Jordan, Kuwait, Lebanon, Libya... , Morocco, North Korea, Oman, Pakistan, Qatar, Saudi...

14

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

15

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

Open Energy Info (EERE)

Morocco-Enhancing Low-carbon Development by Greening the Economy: Policy Morocco-Enhancing Low-carbon Development by Greening the Economy: Policy Dialogue, Advisory Services, Benchmarking Jump to: navigation, search Name Morocco-Enhancing Low-carbon Development by Greening the Economy: Policy Dialogue, Advisory Services, Benchmarking Agency/Company /Organization Deutsche Gesellschaft für Internationale Zusammenarbeit (GIZ) GmbH Sector Climate Focus Area Renewable Energy Topics Low emission development planning, -LEDS, -NAMA, -Roadmap, Market analysis, Pathways analysis Program Start 2011 Program End 2014 Country Morocco Northern Africa References Deutsche Gesellschaft für Internationale Zusammenarbeit (GIZ)[1] Program Overview The project will promote Green Economy in developing countries and emerging economies as a realistic approach towards low-carbon development. It will

16

Evaluation of the impacts of climate changes on the coastal Chaouia aquifer, Morocco, using numerical modeling  

Science Journals Connector (OSTI)

The aquifer of the Chaouia Coast, Morocco constitutes an example of groundwater resources subjected to intensive and uncontrolled withdrawals in a semi-arid region. The analysis of the trends of precipitation ...

J. Moustadraf; M. Razack; M. Sinan

2008-11-01T23:59:59.000Z

17

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

18

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

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

International Training International Training REAC/TS Provides International Radiation Emergency Medical Response Training for Emergency Responders In support of the National Nuclear Security Administration's international approach to nuclear and radiological incident response, REAC/TS staff provide training to physicians, nurses and emergency responders in multiple countries each year. REAC/TS has conducted radiation emergency medical response training in Iraq, Kuwait, Morocco, Singapore, South Africa, and Thailand. "As one of the world's primary responders to nuclear and radiological accidents, it's critical that REAC/TS help prepare a variety of health care professionals for the medical management of radiation accidents," said REAC/TS Medical/Technical Director Dr. Albert Wiley. "Our medical

19

Morocco-NREL Energy Activities | Open Energy Information  

Open Energy Info (EERE)

NREL Cooperation NREL Cooperation Name Morocco-NREL Cooperation Agency/Company /Organization National Renewable Energy Laboratory Partner Center for Development of Renewable Energy (CDER) Sector Energy Focus Area Energy Efficiency Topics Background analysis Program Start "1980" is not in the list of possible values (2013, 2012, 2011, 2010, 2009, 2008, 2007, 2006, 2005, 2004, 2003, 2002, 2001, 2000, 1999, 1998, 1997, 1996, 1995, 1994, 1993, 1992, 1991, 1990, 1989, 1988, 1987, 1986, 1985, 1984, 1983, 1982, 1981) for this property."1980" is not in the list of possible values (2013, 2012, 2011, 2010, 2009, 2008, 2007, 2006, 2005, 2004, 2003, 2002, 2001, 2000, 1999, 1998, 1997, 1996, 1995, 1994, 1993, 1992, 1991, 1990, 1989, 1988, 1987, 1986, 1985, 1984, 1983, 1982, 1981) for this property.

20

FIANTD200725 arXiv:0712.3526v2  

E-Print Network (OSTI)

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

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

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

Open Energy Info (EERE)

Morocco-Joint Programme on Resource Efficient and Cleaner Production (RECP) Morocco-Joint Programme on Resource Efficient and Cleaner Production (RECP) in Developing and Transition Countries Jump to: navigation, search Name Morocco-Joint Programme on Resource Efficient and Cleaner Production (RECP) in Developing and Transition Countries Agency/Company /Organization United Nations Industrial Development Organization (UNIDO), United Nations Environment Programme (UNEP) Partner Ministry of Energy, Ministry of Planning, Ministry of Finance, Ministry of Environment, Ministry of Industry Sector Climate, Energy, Water Focus Area Renewable Energy, Non-renewable Energy, Agriculture, Economic Development, Goods and Materials, Industry, People and Policy, Water Conservation Topics Background analysis, Co-benefits assessment, - Environmental and Biodiversity, - Health, - Macroeconomic, Finance, GHG inventory, Implementation, Low emission development planning, -LEDS, -NAMA, -Roadmap, -TNA, Market analysis, Pathways analysis, Policies/deployment programs, Resource assessment, Technology characterizations

22

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

Open Energy Info (EERE)

Morocco-EU-UNDP Low Emission Capacity Building Programme (LECBP) Morocco-EU-UNDP Low Emission Capacity Building Programme (LECBP) Jump to: navigation, search Name Morocco-EU-UNDP Low Emission Capacity Building Programme (LECBP) Agency/Company /Organization The European Union (EU), United Nations Development Programme (UNDP), German Federal Ministry for the Environment, Nature Conservation and Nuclear Safety (BMU), Australian Department of Climate Change and Energy Efficiency (DCCEE), Australian Agency for International Development (AusAID) Partner Multiple Ministries Sector Climate Focus Area Renewable Energy, Non-renewable Energy, Agriculture, Biomass, Buildings, Economic Development, Energy Efficiency, Forestry, Geothermal, Goods and Materials, Greenhouse Gas, Industry, Land Use, Offsets and Certificates, People and Policy, Solar, Transportation, Water Power, Wind

23

New late Pleistocene seismites in a shoreline series including eolianites, north of Rabat (Morocco)  

Science Journals Connector (OSTI)

...Atlantic coast of High Atlas in Morocco: implications...in some ancient wind-blown sand deposits...NW Red Sea and Gulf of Suez. - Quatern. Internat...northern Red Sea and Gulf of Suez (Egyptian coast...Red Sea coast and Gulf of Suez. In: B.H...

Jean-Claude Plaziat; Mhamed Aberkan; Jean-Louis Reyss

24

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

25

Understanding CDM potential in the Mediterranean basin: A country assessment of Egypt and Morocco  

Science Journals Connector (OSTI)

Abstract The Mediterranean basin countries on the one hand are considered a climate change vulnerability hotspot, while on the other they obtain a substantial potential for the implementation of clean development mechanism (CDM) projects and especially for North Africa region. Abatement of greenhouse gas emissions can mainly be achieved through utilizing renewable energy sources in the region, implementing energy efficiency measures and substituting oil with natural gas in energy generation. However, with few exceptions, the majority of these countries have a limited track record in the CDM pipeline. The aim of this paper is to investigate possibilities for CDM projects and indentify the main challenges for the promotion of CDM activities in the Mediterranean region. In this respect, an assessment of the current state of related institutional and policy setting, CDM potential and barriers related to the implementation of a CDM project in two representative case study countries of the Mediterranean basin, namely Egypt and Morocco was elaborated. The analysis indicated that the overall CDM potential in Egypt and Morocco are almost equal and both countries demonstrate the same tendencies, the key problem, however, remains on how to deal with the political instability and regulatory barriers the region face.

Charikleia Karakosta; John Psarras

2013-01-01T23:59:59.000Z

26

OSTI Announces Alert Service for arXiv Patrons | OSTI, US Dept of Energy,  

Office of Scientific and Technical Information (OSTI)

Announces Alert Service for arXiv Patrons Announces Alert Service for arXiv Patrons March 2005 Oak Ridge, TN - The Office of Scientific and Technical Information (OSTI) is pleased to announce implementation of an Alert Service that serves patrons of arXiv, a source in the fields of physics, mathematics, non-linear science, computer science, and quantitative biology. ArXiv, a service of Cornell University Library System, is one of the sources included in OSTI's E-print Network. Through this Alert Service, patrons can subscribe to be automatically notified of the latest information posted on arXiv, as well as other e-print sources in the E-print Network. A special interface is provided for arXiv patrons through the E-print Network. E-print Network is a vast, integrated network of electronic scientific and

27

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

28

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

29

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

30

Near Miscible CO2 Application to Improve Oil Recovery  

E-Print Network (OSTI)

...................................................................................................................... XIV 1 INTRODUCTION AND LITERATURE REVIEW ....................................................................... 1 1.1 THE BASICS OF CO2 EOR... ....................................................................................................................................... 104 APPENDICES ....................................................................................................................................... 107 vii LIST OF FIGURES FIGURE 1-1 GAS INJECTION EOR IN U.S [1...

Bui, Ly H.

2010-07-26T23:59:59.000Z

31

Carbon dioxide emissions, economic growth, industrial structure, and technical efficiency: Empirical evidence from Ghana, Senegal, and Morocco on the causal dynamics  

Science Journals Connector (OSTI)

This paper investigated the short-run causal relationships and the long-run equilibrium relationships among carbon dioxide emissions, economic growth, technical efficiency, and industrial structure for three African countries. Using Bounds cointegration approach the result showed evidence of multiple long-run equilibrium relationships for Ghana and Senegal but a one-way long-run equilibrium relationship for Morocco. The result from the Toda and Yomamoto granger causality test showed a mix of bidirectional, unidirectional, and neutral relationships for all countries. Whilst in Senegal carbon dioxide emission was not found to be a limiting factor to economic growth; it was found to act as a limiting factor to economic growth in Morocco and Ghana. Lastly, the result from the variance decomposition analysis revealed that economic growth contributes largely to changes in future carbon dioxide emissions in Senegal and Morocco whilst in Ghana technical efficiency contributes largely to changes in future variations in carbon dioxide emissions. These results have important policy implications for these countries' energy efficiency systems.

Philip Kofi Adom; William Bekoe; Franklin Amuakwa-Mensah; Justice Tei Mensah; Ebo Botchway

2012-01-01T23:59:59.000Z

32

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.

33

arXiv:hepex/9905010 Towards Low-Threshold, Real-Time Solar Neutrino  

E-Print Network (OSTI)

of qualitatively new experimental tools. According to the SSM the solar neutrino ux is dominated by the low energy energy resolution. The main obstacle in achieving these goals comes from the formidable backgrounds fromarXiv:hep­ex/9905010 v1 6 May 1999 Towards Low-Threshold, Real-Time Solar Neutrino Detectors G

Gratta, Giorgio

34

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

35

arXiv:cond-mat/0506493v120Jun2005 Statistics of cycles in large networks  

E-Print Network (OSTI)

arXiv:cond-mat/0506493v120Jun2005 Statistics of cycles in large networks Konstantin Klemm and Peter corresponds to energy such that the length histogram is obtained as the density of states from Metropolis approximations, and comparisons with real-world networks have been difficult so far, since an efficient method

Stadler, Peter F.

36

arXiv:condmat/0506493 Statistics of cycles in large networks  

E-Print Network (OSTI)

arXiv:cond­mat/0506493 v1 20 Jun 2005 Statistics of cycles in large networks Konstantin Klemm corresponds to energy such that the length histogram is obtained as the density of states from Metropolis checks of the analytical approximations, and comparisons with real-world networks have been di?cult so

Stadler, Peter F.

37

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

38

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

39

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

40

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

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: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

42

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

43

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

44

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

45

arXiv:nucl-th/010204116Feb2001 JLAB-THY-01-07  

E-Print Network (OSTI)

arXiv:nucl-th/010204116Feb2001 WM-01-103 JLAB-THY-01-07 The stability of the scalar 2 interaction, the simple sum of bubble diagrams for the propagation of a single particle leads to a stable ground state] (see also Ref. [4]). Both the simple bubble summation and the quenched calculations do not exhibit

Thomas Jefferson National Accelerator Facility

46

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

47

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

48

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

49

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.

50

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

51

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

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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

52

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

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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

53

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

54

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

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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

55

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

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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

56

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

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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

57

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

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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

58

arXiv:hepph/9903516 hepph/9903516 BNLHET99/6  

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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

59

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

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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

60

arXiv:1208.5325v1[math.PR]27Aug2012 THE COMBINATORIAL APPROACH TO THE ISING  

E-Print Network (OSTI)

arXiv:1208.5325v1[math.PR]27Aug2012 THE COMBINATORIAL APPROACH TO THE ISING MODEL: FOUNDATIONS is a beautiful way to rigorously study the two-dimensional Ising model with no external field. In this paper, we in the literature. We also demonstrate how the method can be applied to prove some classical results about the Ising

Meester, Ronald

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61

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

62

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

63

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

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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

64

arXiv:1011.0897v1[math.NA]3Nov2010 EFFICIENT NUMERICAL STABILITY ANALYSIS OF DETONATION  

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arXiv:1011.0897v1[math.NA]3Nov2010 EFFICIENT NUMERICAL STABILITY ANALYSIS OF DETONATION WAVES­Stewart and Short­Stewart, the numerical evaluation of linear stability of planar detonation waves problem. Planar detonation waves can often change stability as physical parameters are varied, undergoing

Humpherys, Jeffrey

65

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

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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

66

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

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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

67

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

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

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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

69

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

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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

70

arXiv:1109.6695v1[hep-ph]29Sep2011 LU TP 11-32  

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arXiv:1109.6695v1[hep-ph]29Sep2011 LU TP 11-32 September 2011 Drell-Yan diffraction: breakdown Ciencias e Ingenier´ia; and Centro Cient´ifico-Tecnol´ogico de Valpara´iso; Casilla 110-V, Valpara´iso

Lunds Universitet,

71

arXiv:1305.4430v3[hep-ph]14Dec2013 LU TP 13-17  

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arXiv:1305.4430v3[hep-ph]14Dec2013 LU TP 13-17 USM-TH-312 December 2013 Quantum Gravity effect´ecnica Federico Santa Mar´ia Casilla 110-V, Valpara´iso, Chile Roman Pasechnik Theoretical High Energy Physics

Lunds Universitet,

72

arXiv:1204.6477v1[hep-ph]29Apr2012 LU TP 12-14  

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arXiv:1204.6477v1[hep-ph]29Apr2012 LU TP 12-14 April 2012 Diffractive gauge bosons production´ia; and Centro Cient´ifico-Tecnol´ogico de Valpara´iso; Casilla 110-V, Valpara´iso, Chile Abstract We discuss

Lunds Universitet,

73

arXiv:1403.2014v2[hep-ph]24May2014 LU TP 13-38  

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arXiv:1403.2014v2[hep-ph]24May2014 LU TP 13-38 USM-TH-322 May 2014 Higgsstrahlung at forward Santa Mar�ia; and Centro Cient�ifico-Tecnol�ogico de Valpara�iso, Avda. Espa~na 1680, Valpara�iso, Chile

Lunds Universitet,

74

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

75

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

E-Print Network (OSTI)

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

76

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

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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

77

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

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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

78

arXiv:astro-ph/0503398v117Mar2005 Development of Bubble Chambers With Enhanced Stability and Sensitivity to  

E-Print Network (OSTI)

arXiv:astro-ph/0503398v117Mar2005 Development of Bubble Chambers With Enhanced Stability Fermi National Accelerator Laboratory, Batavia, IL, USA The viability of using a Bubble Chamber for rare stability in such a detector are described. Results from prototype trials indicate that sensitivity to low

Collar, Juan I.

79

arXiv:astro-ph/0602147v17Feb2006 Likelihood Methods for Cluster Dark Energy Surveys  

E-Print Network (OSTI)

arXiv:astro-ph/0602147v17Feb2006 Likelihood Methods for Cluster Dark Energy Surveys Wayne Hu1 and J on both the dark energy equation of state and the mass selection function required to extract it-mass relations allows for a joint extraction of dark energy and cluster structural parameters. I. INTRODUCTION

Hu, Wayne

80

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

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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:gr-qc/0609089v121Sep2006 Scattering of cosmic strings by black holes: loop formation  

E-Print Network (OSTI)

the gravitational wave background produced by oscillating string loops [9] 1 . The scattering of a long cosmicarXiv:gr-qc/0609089v121Sep2006 Scattering of cosmic strings by black holes: loop formation Florian: September 22, 2006) We study the deformation of a long cosmic string by a nearby rotating black hole. We

Boyer, Edmond

83

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

84

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

85

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

E-Print Network (OSTI)

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

86

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... 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...

Wendy F. Kasinec

2005-01-01T23:59:59.000Z

87

arXiv:hep-ph/0110320 v3 18 Sep 2002  

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

4 4 November 2001 Detecting and Studying Higgs Bosons in Two-Photon Collisions at a Linear Collider David M. Asner, Jeffery B. Gronberg, Lawrence Livermore National Laboratory Livermore, California John F. Gunion University of California at Davis Davis, California November 2001 Abstract: We examine the potential for detecting and studying Higgs bosons in two-photon collisions at a future linear collider. Our study incorporates realistic two-photon spectra based on the most probable available laser technology. Results include detector simulations. We study the cases of: a) an SM-like Higgs boson; b) the heavy MSSM Higgs bosons; c) a Higgs boson with no WW/ZZ couplings from a general two Higgs doublet model. arXiv:hep-ph/0110320 v3 18 Sep 2002

88

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

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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

89

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

90

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

91

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

92

Reply to "Isotropy of Speed of Light" by Castano and Hawkins, arXiv:1103.1620  

E-Print Network (OSTI)

In "Isotropy of Speed of Light" by Castano and Hawkins, arXiv:1103.1620, it is claimed, using a flawed theoretical argument, that the speed of light must necessarily be isotropic, independent even of experiment. The key false assumption made is that the round trip time must always be invariant wrt change of direction of the light path. This is shown to be false. More importantly the anisotropy of the speed of light has been repeatedly detected in experiments, beginning with Michelson and Morley in 1887, and with the most recent data being from spacecraft earth-flyby Doppler shift data. Similar misunderstandings critically affect the designs for LIGO and LISA.

Reginald T. Cahill

2011-03-10T23:59:59.000Z

93

arXiv:0912.3816v1[astro-ph.CO]18Dec2009 Testable dark energy predictions from current data  

E-Print Network (OSTI)

and early dark energy. Barring additional systematic errors hiding in the data, such a discovery wouldarXiv:0912.3816v1[astro-ph.CO]18Dec2009 Testable dark energy predictions from current data Michael a class of dark energy models, constraints from one set of cosmic acceleration observables make

Hu, Wayne

94

arXiv:1101.0723v1[q-bio.MN]4Jan2011 Bistability of an In Vitro Synthetic Autoregulatory Switch  

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synthetic DNA strands and three enzymes, bacteriophage T7 RNA polymerase, Escherichia coli ribonuclease of a synthetic DNA switch regulated by its RNA output acting as a transcription activator. We verifiedarXiv:1101.0723v1[q-bio.MN]4Jan2011 Bistability of an In Vitro Synthetic Autoregulatory Switch

Winfree, Erik

95

arXiv:1103.2923v1[math.OC]15Mar2011 Estimation of Saturation of Permanent-Magnet  

E-Print Network (OSTI)

effects such as cross-coupling and permanent magnet demagnetization can introduce large errorsarXiv:1103.2923v1[math.OC]15Mar2011 Estimation of Saturation of Permanent-Magnet Synchronous Motors a parametric model of the saturated Permanent-Magnet Synchronous Motor (PMSM) together with an estimation

Paris-Sud XI, Université de

96

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

97

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

98

arXiv:1204.1240v1[cs.IT]5Apr2012 1 Optimal Save-Then-Transmit Protocol for Energy  

E-Print Network (OSTI)

arXiv:1204.1240v1[cs.IT]5Apr2012 1 Optimal Save-Then-Transmit Protocol for Energy Harvesting a fraction of time (dubbed the save-ratio) is devoted exclusively to energy harvesting, with the remaining to validate our proposed study. Index Terms Energy harvesting, save-then-transmit protocol, outage

Lim, Teng Joon

99

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

100

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

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101

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

102

arXiv:astro-ph/0401559v126Jan2004 Self-Calibration of Cluster Dark Energy Studies: Counts in Cells  

E-Print Network (OSTI)

arXiv:astro-ph/0401559v126Jan2004 Self-Calibration of Cluster Dark Energy Studies: Counts in Cells of Chicago, Chicago IL 60637 Cluster number counts can constrain the properties of dark energy if and only be measured from the survey without additional observational cost. It can minimize the degradation in dark

Hu, Wayne

103

arXiv:1211.7167v1[q-bio.BM]30Nov2012 Polymer uncrossing and knotting in protein folding, and their  

E-Print Network (OSTI)

folding is a structural transformation, from a disordered-polymer conformational ensemble to an orderedarXiv:1211.7167v1[q-bio.BM]30Nov2012 1 Polymer uncrossing and knotting in protein folding, optimal trajectories or pathways for a protein to fold. This involves recording all unphysical crossing

Plotkin, Steven S.

104

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.

105

arXiv:1311.6414v1[astro-ph.EP]25Nov2013 Astronomy & Astrophysics manuscript no. lithium c ESO 2013  

E-Print Network (OSTI)

arXiv:1311.6414v1[astro-ph.EP]25Nov2013 Astronomy & Astrophysics manuscript no. lithium c ESO 2013 on the atmospheric Li abundance of planet host stars. Methods. In this work we present new determinations of lithium. 2008) showed the significant metallicity excess of the planet-host sample com- pared with the sample

106

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

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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

107

arXiv:1011.4739v2[math.GR]16Dec2010 APPROXIMATING THE FIRST L2-BETTI NUMBER OF RESIDUALLY  

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arXiv:1011.4739v2[math.GR]16Dec2010 APPROXIMATING THE FIRST L2-BETTI NUMBER OF RESIDUALLY FINITE GROUPS W. L¨UCK, D. OSIN Abstract. We show that the first L2 -betti number of a finitely generated residually finite group can be estimated from below by using ordinary first betti numbers of finite index

Lück, Wolfgang

108

arXiv:1204.3298v2[math.GT]9May2012 ON THE GROWTH OF BETTI NUMBERS IN p-ADIC ANALYTIC  

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arXiv:1204.3298v2[math.GT]9May2012 ON THE GROWTH OF BETTI NUMBERS IN p-ADIC ANALYTIC TOWERS NICOLAS BERGERON, PETER LINNELL, WOLFGANG L¨UCK, AND ROMAN SAUER Abstract. We study the asymptotic growth of Betti and statement of results This paper is mainly concerned with the asymptotic growth of Betti numbers in a tower

Lück, Wolfgang

109

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

110

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

111

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

112

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

E-Print Network (OSTI)

() 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

113

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

114

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

E-Print Network (OSTI)

. The content of the paper is 1) the definition of the interface free energy from first principlesarXiv:0911.5232v1[cond-mat.stat-mech]27Nov2009 Interface Free Energy or Surface Tension: definition energy is the contribution to the free energy of a system due to the presence of an interface separating

Pfister, Charles

115

arXiv:1004.1985v1[cond-mat.mes-hall]12Apr2010 Current correlations of an on-demand electron source as an  

E-Print Network (OSTI)

arXiv:1004.1985v1[cond-mat.mes-hall]12Apr2010 Current correlations of an on-demand electron source to characterize an on-demand electron source consisting of a quantum dot connected to a conductor via a tunable of the electron emission time, which we call quantum jitter. In optimum op- erating conditions of the source

Plaçais, Bernard

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

FRENCH UNIVERSITY MISSION TO MOROCCO  

Science Journals Connector (OSTI)

...which expired on October 1 of this year, be extended...be received up to November 1. As pro-vided under the...thereof not exceed-ing 1,500 words. Such summary must...grant them a 50 per cent. rebate on its railway and Lake Titicaca...

1924-09-19T23:59:59.000Z

118

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

119

arXiv:1306.4564v1[math.GT]19Jun2013 Bitwist manifolds and two-bridge knots  

E-Print Network (OSTI)

arXiv:1306.4564v1[math.GT]19Jun2013 Bitwist manifolds and two-bridge knots J. W. CANNON W. J. FLOYD, explicit, and simple face-pairing descriptions of all of the branched cyclic covers of S3 branched over two-bridge for F1 , S1 , K+ , and K- 7. Surgery diagrams for the general two-bridge knot 8. Continued Fractions 9

Purcell, Jessica

120

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

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121

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

122

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

123

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

124

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

125

Comment on 'A Scaling law beyond Zipf's law and its relation to Heaps' law' [arXiv:1303.0705  

E-Print Network (OSTI)

It is shown that the scaling law for the text-length dependence of word-frequency distributions proposed by Font-Clos et al in 2013 [New J. Phys. 15 093033, arXiv:1303.0705] is fundamentally impossible and leads to incorrect conclusions. Instead the text-length-dependence can be connected to the general properties of a random book with consistent agreement. It is pointed out that this finding has strong implications, when deciding between two conceptually different views on word-frequency distributions, i.e. the `Zipf's-view' and the `Randomness-view', as is discussed. It is also noticed that the text-length transformation of a random book does have an exact scaling property precisely for the power-law index $\\gamma=1$, as opposed to the Zipf's exponent $\\gamma=2$ and the implication of this exact scaling property is discussed. However a real text has $\\gamma>1$ and as a consequence $\\gamma$ increases when shortening a real text, contrary to the claim by Font-Clos et al in 2013 New J. Phys. 15 093033. The con...

Yan, Xiao-Yong

2014-01-01T23:59:59.000Z

126

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

127

Frictional Phenomena. XIV  

Science Journals Connector (OSTI)

IN this chapter technical applications of the solid friction concept in four different fields are discussed. These are: (1) mechanical engineering (a) damping of unwanted vibrations in machineryfor instance crank?shaft vibrations (b) vibrations excited by internal frictionfor instance whirl of rotating shafts; (2) metallurgy in which damping measurement promises to be a useful new tool; (3) rubber technology as applied to automobile tires with regard to the heat generated therein; and (4) electrical engineering specifically dielectric losses in electrical insulating materials.

Andrew Gemant

1943-01-01T23:59:59.000Z

128

Phylum XIV. Bacteroidetes phyl. nov.  

Science Journals Connector (OSTI)

The phylum Bacteroidetes is a phenotypically diverse group of Gram-stain-negative rods that do not form endospores. They are circumscribed for this volume on the basis of phylogenetic analysis of 16S rRNA gene se...

Noel R. Krieg; Wolfgang Ludwig; Jean Euzby

2010-01-01T23:59:59.000Z

129

Religiosity, Freedom of Expression and Lebanon and Morocco  

E-Print Network (OSTI)

Abstract: This study addresses the relationship between religiosity and freedom of speech. While a growing body of research advances the now established notion that Islam as a religion in practice at the individual level ...

Byers III, Ward

2014-05-31T23:59:59.000Z

130

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

131

hst-2001_arXiv.dvi  

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

to to ApJ: April 9, 2010 Preprint typeset using L A T E X style emulateapj v. 2/16/10 SPECTRA AND HST LIGHT CURVES OF SIX TYPE IA SUPERNOVAE AT 0.511 < Z < 1.12 AND THE Union2 COMPILATION ∗ R. Amanullah 1,2 , C. Lidman 2 , D. Rubin 4,6 , G. Aldering 4 , P. Astier 5 , K. Barbary 4,6 , M. S. Burns 7 , A. Conley 8 , K. S. Dawson 24 , S. E. Deustua 9 , M. Doi 10 , S. Fabbro 11 , L. Faccioli 4,12 , H. K. Fakhouri 4,6 , G. Folatelli 13 , A. S. Fruchter 9 , H. Furusawa 26 , G. Garavini 1 , G. Goldhaber 4,6 , A. Goobar 1,2 , D. E. Groom 4 , I. Hook 14,25 , D. A. Howell 3,22 , N. Kashikawa 26 , A. G. Kim 4 , R. A. Knop 15 , M. Kowalski 23 , E. Linder 12 , J. Meyers 4,6 , T. Morokuma 26,27 , S. Nobili 1,2 , J. Nordin 1,2 , P. E. Nugent 4 , L. ¨ Ostman 1,2 , R. Pain 5 , N. Panagia 9,17,18 , S. Perlmutter 4,6 , J. Raux 5 , P. Ruiz-Lapuente 16 , A. L. Spadafora 4 , M. Strovink 4,6 , N. Suzuki 4 , L. Wang 19 , W. M. Wood-Vasey 20 , N. Yasuda 21 (The Supernova Cosmology Project)

132

DESY 05116 arXiv:hepph/0507137  

E-Print Network (OSTI)

phenomeno- logical point of view. We ask ourselves the question whether and how (i) the particles present particles are the four neutralinos, two charginos, and a gluino. Since all squarks are very heavy lifts the light Higgs mass considerably above the LEP limit, solving another problem of the MSSM. Still

133

DESY05158 arXiv:hepph/0509107  

E-Print Network (OSTI)

-158 AZIMUTHAL DEPENDENCE IN DIFFRACTIVE PROCESSES a M. DIEHL Deutsches Elektronen-Synchroton DESY, 22603 Hamburg

134

DESY 06119 arXiv:hepph/0608037  

E-Print Network (OSTI)

fragmentation functions Alessandro Bacchetta #3; Theory Group, Deutsches Elektronen-Synchroton DESY, D-22603

135

DESY05256 arXiv:hepph/0512201  

E-Print Network (OSTI)

Generalized parton distributions: recent results #3; M. Diehl Deutsches Elektronen-Synchroton DESY, 22603

136

DESY05214 arXiv:hepph/0511047  

E-Print Network (OSTI)

Elektronen­Synchroton DESY, 22603 Hamburg, Germany Abstract Diffractive reactions involving a hard scale can

137

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

138

DESY 06173 arXiv:heplat/0610015  

E-Print Network (OSTI)

flavours of quarks with maximally twisted mass Karl Jansen #3; John von Neumann Institute for Computing, NIC, Platanenallee 6, D­15738 Zeuthen, Germany E­mail: Karl.Jansen@desy.de Carsten Urbach #3

139

Chapter XIV A Framework for Understanding  

E-Print Network (OSTI)

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

Dascalu, Sergiu

140

The Path of Carbon in Photosynthesis XIV.  

DOE R&D Accomplishments (OSTI)

It seems hardly necessary to repeat to an audience of this kind the importance of the process known as photosynthesis in the interaction and the interdependence of organisms and in the very existence of life as we know it. This process by which green plants are able to capture electromagnetic energy in the form of sunlight and transform it into stored chemical energy in the form of a wide variety of reduced (relative to carbon dioxide) carbon compounds provides the only major source of energy for the maintenance and propagation of all life.

Calvin, Melvin; Bassham, J. A.; Benson, A. A.; Kawaguchi, S.; Lynch, V. H.; Stepka, W.; Tolbert, N. E.

1951-06-30T23:59:59.000Z

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
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141

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

142

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

143

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

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

2007 page 1 Summary: Darussalam Cambodia Congo Cyprus Eritrea Gabon Gambia* Israel Jordan Kazakhstan Kyrgyzstan Libyan Arab... Jamahiriya* Malawi Maldives Mauritius Moldova...

144

Modelling and simulation of a Jurassic carbonate ramp outcrop, Amellago, High Atlas Mountains, Morocco  

Science Journals Connector (OSTI)

...information about environments of deposition (EOD), rock types and reservoir quality is...discrete rock description properties include EOD, facies types and diagenetic features...environments of deposition (EODs). Each EOD has a unique mode of sediment production...

R. Shekhar; I. Sahni; G. Benson; S. Agar; F. Amour; S. Toms; N. Christ; R. Alway; M. Mutti; A. Immenhauser; Z. Karcz; L. Kabiri

145

Autonomous Desalination and Cooperation. The Experience in Morocco Within the ADIRA Project  

Science Journals Connector (OSTI)

Fresh water supply in the world, particularly in developing countries, is becoming a more and more challenging problem and affects many multidisciplinary aspects, such as security, health, development, economics ...

Vicente J. Subiela; Baltasar Peate

2011-01-01T23:59:59.000Z

146

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

147

Abstract 1813: Frequency and risk factors of male breast cancer in Egypt and Morocco  

Science Journals Connector (OSTI)

...A103: Breast cancer molecular subtype analysis in Egypt reveals high prevalence of Luminal A: Implications...Institute, Phoenix, AZ 2Cairo University, Cairo, Egypt 3Minya University, Minya, Egypt 4The Van Andel Research Institute, Grand Rapids...

Meaghen Quinlan-Davidson; Ashley Strahley; Mohab Eissa; Abdellatif Benider; Noureddine Benjaafar; Ahmed Hablas; Mehdi Karkouri; Mohammad Ramadan; Ibrahim Seif Eldein; Anwar Nayera; Kathy Toy; Sofia D. Merajver; Amr S. Soliman

2010-04-15T23:59:59.000Z

148

Analysis & Projections - U.S. Energy Information Administration (EIA) -  

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

Full report (64.9 mb) Full report (64.9 mb) Overview (2.14 mb) Chapter breakdowns by country: I-III - Canada, Mexico, Australia (15.0 mb) IV-VII - N. South America, Argentina, Brazil, Other S. South America (8.33 mb) VIII-XIII - Poland, Russia, Eastern Europe, United Kingdom, Spain, Northern and Western Europe (13.5 mb) XIV-XIX - Morocco, Algeria, Tunisia, Libya, Egypt, South Africa (14.3 mb) XX-XXVI - China, Mongolia, Thailand, Indonesia, India/Pakistan, Jordan, Turkey (13.0 mb) Previous Report April 5, 2011 (16.8 mb) Technically Recoverable Shale Oil and Shale Gas Resources: An Assessment of 137 Shale Formations in 41 Countries Outside the United States Release date: June 10, 2013 Updated: June 13, 2013 Table 5 corrected Executive summary This report provides an initial assessment of shale oil resources and

149

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

150

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 [

151

arXiv:hepph/0504175 DESY 05-061  

E-Print Network (OSTI)

in the transverse plane and generalized transversity distributions M. Diehl Deutsches Elektronen-Synchroton DESY

152

DESY 08110 arXiv:0808.0970v1  

E-Print Network (OSTI)

Physics: from HERA to LHC #3; Markus Diehl Deutsches Elektronen-Synchroton DESY 22603 Hamburg - Germany I

153

arXiv:hepph/0501074 DESY-05-005  

E-Print Network (OSTI)

of pentaquarks in the scaling regime #3; M. Diehl a , B. Pire by L. Szymanowski c a Deutsches Elektronen-Synchroton

154

DESY 07117 arXiv:0708.1121v1  

E-Print Network (OSTI)

corrections in exclusive meson production M. Diehl and W. Kugler Deutsches Elektronen-Synchroton DESY, 22603

155

DESY 07105 arXiv:0707.3372v1  

E-Print Network (OSTI)

Gary R. Goldstein, 3, z and Asmita Mukherjee 4, x 1 Theory Group, Deutsches Elektronen-Synchroton DESY

156

arXiv:hepph/0611368 Leptogenesis and Gravitino Dark Matter  

E-Print Network (OSTI)

Wilfried Buchmüller Deutsches Elektronen­Synchroton DESY, 22607 Hamburg, Germany Abstract. We study

157

DESY 08111 arXiv:0808.0972v1  

E-Print Network (OSTI)

Generalised Parton Distributions #3; Markus Diehl Deutsches Elektronen-Synchroton DESY 22603 Hamburg - Germany

158

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

159

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

160

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 Institute, Wurenlingen and Villigen, 5232 Villigen PSI, Switzerland guedel@astro.phys.ethz.ch, audard, but are more numerous. Previous analyses of ares in light-curves of active stars have shown that this index

Guedel, Manuel

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161

arXiv:astroph/0503546 submitted to The Astrophysical Journal  

E-Print Network (OSTI)

Scherrer Institut, Wurenlingen and Villigen, CH-5232 Villigen PSI, Switzerland Marc Audard Columbia Astrophysics Laboratory, Mail code 5247, 550 West 120 th Street, New York, NY 10027 Jan-Uwe Ness Department; #25; 2:2 2:8, in excellent agreement with values previously derived from light curves of magnetically

Guedel, Manuel

162

2706 -XIV Encuentro de Latinoamericanistas Espaoles EL PROCESO DE EMPODERAMIENTO  

E-Print Network (OSTI)

en las condiciones materiales de vida es acompañada por un conjunto de logros (competencias ejercen el poder, o, por el contrario, oponen resistencia a la opresión; por último se presentan las

Paris-Sud XI, Université de

163

arXiv:hepph/0302225 LU TP 03{03  

E-Print Network (OSTI)

Abstract Particles are either bosons or fermions, which obey Bose{Einstein (BE) or Fermi{Dirac statistics mesons are the most common products in high-energy collisions. In the phenomenological Lund Model thought of the world as consisting of indivisible parts called atoms, we today associate matter and forces

Lunds Universitet,

164

arXiv:nuclth/0111056 MODERN SHELL-MODEL CALCULATIONS  

E-Print Network (OSTI)

of this approach, we have also performed calculations within the framework of the usual Brueckner G of the Brueckner G matrix has become feasible while the so-called folded- diagram series for the e#11;ective

Itaco, Nunzio

165

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

166

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

167

Revised Version arXiv:0810.0300v2  

E-Print Network (OSTI)

twisted mass fermions in the epsilon regime K. Jansen, A. Nube, DESY Zeuthen, Platanenallee 6 D­15738 Zeuthen, Germany E­mail: karl.jansen@desy.de,annube@ifh.de A. Shindler #3; Theoretical Physics Division

168

Revised Version DESY 06152 arXiv:heplat/0609012  

E-Print Network (OSTI)

­152 Status Report on ILDG activities Karl Jansen John von Neumann­Institute for Computing NIC, DESY, Platanenallee 6, D­15738 Zeuthen, Germany E­mail: Karl.Jansen@desy.de A status report about the International to about 10--20% of this computer power. #3; Present members are R. Brower (USA), K. Jansen (Germany

169

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

170

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

171

arXiv:hepex/0111033 An O -Axis Neutrino Beam  

E-Print Network (OSTI)

to that of the proton beam. 5. At what energy E #23;;peak does the neutrino spectrum peak for #18; = 0? 6. Compare by the \\horn". The main source of neutrinos is then the decay #25; + ! #22; + #23; #22; . 1. Give a simple estimate of the relative number of other types of neutrinos than #23; #22; in the beam. 2. If the decay

McDonald, Kirk

172

arXiv:astroph/0509330 The IceCube Collaboration  

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los Heros q , D. Pieloth d , A.C. Pohl f , R. Porrata i , J. Pretz l , P.B. Price i , G.T. Przybylski , A. Karle o , H. Kawai y , J.L. Kelley o , M. Kestel h , N. Kitamura o , S.R. Klein g , S. Klepser d

Woschnagg, Kurt

173

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

174

arXiv:astroph/0202057 Accepted to AJ  

E-Print Network (OSTI)

@astro.columbia.edu K. O'Neil Arecibo Observatory, HC03 Box 53995, Arecibo, PR 00612 koneil@naic.edu and G. D. Bothun indicating the true range in disk galaxy properties) and b) the presence of at least some red, gas poor, LSB galaxies fainter than the natural sky brightness have been discovered. It has now become clear

O'Neil, Karen

175

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

176

Revised Version DESY 06063 arXiv:astroph/0605198  

E-Print Network (OSTI)

, cosmologically distinguishing dynamic Dark Energy from Dark Gravity will require a weak lensing shear survey more ACCELERATION: DARK ENERGY OR MODIFIED GRAVITY? Sidney Bludman #3; DESY, 22607 Hamburg, Germany (Dated: June 12, 2006) The recently observed accelerating cosmological expansion or "dark energy" may be either

177

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

178

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

179

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

180

Deterioration processes on archaeological sites of Chellah and Oudayas (world cultural heritage, Rabat, Morocco): restoration test and recommendations  

Science Journals Connector (OSTI)

...abundant and variable in shape and size. Plasters (often one superimposed over another...mineralogical composition between the outer plasters (samples S-27 and S-28; tab. 5...phyllosilicates (tab. 6) employed to colour the plaster used for restoration. Sample S-42...

Lahcen Asebriy; Taj-Eddine Cherkaoui; Iz-Eddine El Amrani El Hassani; Roberto Franchi; Francesco Guerrera; Manuel Martn-Martn; Claudia Guerrera Patama; Giuliana Raffaelli; Pedro Robles-Marn; Julian Tejera De Leon; Francisco J. Alcal

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181

PPS-27, 2011, 27th World Congress of the Polymer Processing Society, May 10-14, Marrakech, Morocco  

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of the nanocomposite structure is still an open question. Depending on the nanoclay state (from intercalated to fully-like behavior is associated to the presence of a 3D structure where the nanoclay platelets and tactoids form

Paris-Sud XI, Université de

182

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

183

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

184

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

185

Moldova-UNEP Green Economy Advisory Services | Open Energy Information  

Open Energy Info (EERE)

Armenia, Azerbaijan, Barbados, Burkina Faso, China, Egypt, Ghana, Indonesia, Jordan, Kenya, Korea, Mali, Mexico, Moldova, Mongolia, Montenegro, Morocco, Namibia, Nepal,...

186

Russian-UNEP Green Economy Advisory Services | Open Energy Information  

Open Energy Info (EERE)

Armenia, Azerbaijan, Barbados, Burkina Faso, China, Egypt, Ghana, Indonesia, Jordan, Kenya, Korea, Mali, Mexico, Moldova, Mongolia, Montenegro, Morocco, Namibia, Nepal,...

187

Ghana-UNEP Green Economy Advisory Services | Open Energy Information  

Open Energy Info (EERE)

Armenia, Azerbaijan, Barbados, Burkina Faso, China, Egypt, Ghana, Indonesia, Jordan, Kenya, Korea, Mali, Mexico, Moldova, Mongolia, Montenegro, Morocco, Namibia, Nepal,...

188

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

189

Mineralogy and crystal structure of bouazzerite from Bou Azzer, Anti-Atlas, Morocco: Bi-As-Fe nanoclusters containing Fe3+ in trigonal prismatic coordination  

Science Journals Connector (OSTI)

...associated with quartz, chalcopyrite, native gold, erythrite, talmessite/roselite-beta, Cr-bearing yukonite, alumopharmacosiderite...associated with quartz, chalcopyrite, native gold, erythrite, talmessite/roselite-beta, Cr-bearing yukonite, alumopharmacosiderite...

Jol Brugger; Nicolas Meisser; Sergey Krivovichev; Thomas Armbruster; Georges Favreau

190

Nickeltalmessite, Ca2Ni(AsO4)2 2H2O, a new mineral species of the fairfieldite group, Bou Azzer, Morocco  

Science Journals Connector (OSTI)

Nickeltalmessite, Ca2Ni(AsO4)2 2H2O, a new mineral species of the fairfieldite group, has been found in association with annabergite, nickelaustinite, pecoraite, calcite, and a mineral of the chromite-manganoch...

N. V. Chukanov; A. A. Mukhanova; S. Mckel; D. I. Belakovsky

2010-12-01T23:59:59.000Z

191

arXiv:astro-ph/0005123 v3 2 Oct 2000  

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005123 005123 v3 2 Oct 2000 Draft version June 4, 2005 Preprint typeset using L A T E X style emulateapj v. 26/01/00 MAXIMA-1: A MEASUREMENT OF THE COSMIC MICROWAVE BACKGROUND ANISOTROPY ON ANGULAR SCALES OF 10 TO 5 ◦ S. Hanany 1,2 , P. Ade 3 , A. Balbi 4,2,15 , J. Bock 5,6 , J. Borrill 2,7 , A. Boscaleri 8 , P. de Bernardis 9 , P. G. Ferreira 10,11 , V. V. Hristov 6 , A. H. Jaffe 2 , A. E. Lange 2,6 , A. T. Lee 14,15,2 , P. D. Mauskopf 12 , C. B. Netterfield 13 , S. Oh 2 , E. Pascale 8 , B. Rabii 2,14 , P. L. Richards 2,14 , G. F. Smoot 2,14,15,16 , R. Stompor 2,16,17 , C. D. Winant 2,14 , J. H. P. Wu 18 Draft version June 4, 2005 ABSTRACT We present a map and an angular power spectrum of the anisotropy of the cosmic microwave back- ground (CMB) from the first flight of MAXIMA. MAXIMA is a balloon-borne experiment with an array of 16 bolometric photometers operated at 100 mK. MAXIMA observed a 124 deg 2 region of the sky with 10 resolution

192

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

193

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

194

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

195

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

196

POLYSACCHARIDE AND GLYCOLIPID SYNTHESIS BY CELL-FREE PREPARATIONS FROM TYPE XIV PNEUMOCOCCUS  

Science Journals Connector (OSTI)

...were processed through the electrodialysis step described in the table...treated as follows: no further treatment (unincubated endogenous...from the butanol phase with water, dilute NaHCO3, or dilute...were essentially insoluble in water, but soluble in many organic...

Jack Distler; Saul Roseman

1964-01-01T23:59:59.000Z

197

Revised Version DESY 07195 arXiv:0711.2184v2  

E-Print Network (OSTI)

Elektronen-Synchroton DESY, 22603 Hamburg, Germany Abstract: We study the evolution behavior of generalized

198

Revised Version DESY 08023 arXiv:0803.0227v3  

E-Print Network (OSTI)

a , Piet J. Mulders b a Theory Group, Deutsches Elektronen-Synchroton DESY, 22603 Hamburg, Germany b Dept

199

Revised Version DESY 07194 arXiv:0711.1077v2  

E-Print Network (OSTI)

-194 Implications of HERA measurements for LHC #3; M. Diehl Deutsches Elektronen-Synchroton DESY, 22603 Hamburg

200

Revised Version DESY 07093 arXiv:0706.3139v2  

E-Print Network (OSTI)

Production at NLO Markus Diehl and Wolfgang Kugler Deutsches Elektronen-Synchroton DESY 22603 Hamburg

Note: This page contains sample records for the topic "xiv-1 xiv morocco" from the National Library of EnergyBeta (NLEBeta).
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201

Revised Version DESY 06204 arXiv:hepph/0611265v2  

E-Print Network (OSTI)

, Marc Schlegel b a Theory Group, Deutsches Elektronen-Synchroton DESY, 22603 Hamburg, Germany b Institut

202

Revised Version DESY 07028 arXiv:hepph/0703153v2  

E-Print Network (OSTI)

'Alesio, 3 Piet J. Mulders, 2 and Francesco Murgia 3 1 Theory Group, Deutsches Elektronen-Synchroton DESY

203

arXiv:0911.3317v1 DESY 09-204  

E-Print Network (OSTI)

into octet meson pairs: symmetry relations in the handbag approach M. Diehl Deutsches Elektronen-Synchroton

204

arXiv:hepph/0504124 Reviewing model calculations of the Collins fragmentation function  

E-Print Network (OSTI)

ur Theoretische Physik II, Ruhr-Universitat Bochum, D-44780 Bochum, Germany 2 Deutsches Elektronen-Synchroton

205

arXiv:hepph/0703265v1 DESY 07-034  

E-Print Network (OSTI)

Pavia, Italy Alessandro Bacchetta z Theory Group, Deutsches Elektronen-Synchroton DESY, D-22603 Hamburg

206

Revised Version DESY07049 arXiv:0704.1565v2  

E-Print Network (OSTI)

a polarized nucleon M. Diehl Deutsches Elektronen-Synchroton DESY, 22603 Hamburg, Germany Abstract: We provide

207

arXiv:acc-phys/9602001v112Feb1996 MUON COLLIDERS  

E-Print Network (OSTI)

, A. Garren3,7 , M. Green3 , S. Kahn1 , H. Kirk1 , Y. Y. Lee1 , F. Mills5 , N. Mokhov5 , G. Morgan1 on upgrades of the FERMILAB machines would also be possible (see second Ref. [4]). Hadron collider energies are limited by their size and technical constraints on bending magnetic fields. At very high energies it would

Wurtele, Jonathan

208

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,

209

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.

210

arXiv:1208.3266v1 [math-ph] 16 Aug 2012  

E-Print Network (OSTI)

Aug 16, 2012 ... Motivated by the synthesization of a novel material [1], we started .... type (b), that is superselection rules, to show that the Eigenvalues are.

2012-08-17T23:59:59.000Z

211

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

E-Print Network (OSTI)

Pereira Souza / 10002721, Renato de Oliveira Santos / 10003410, Rodrigo da Paixao Santos / 10005398 dos Santos / 10000964, Alexsandra da Silva Costa / 10001156, Amâmbia Gonçalves Cordeiro dos Santos, Bianca Isabel Araújo da Boa Morte / 10010997, Bruna Simplicio Santos / 10007547, Carlos Alberto Martins

Maier, Rudolf Richard

212

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

E-Print Network (OSTI)

. HERLEY DA LUZ BRASIL 3. ROBSON DE MAGALH?ES PEREIRA 4. WALTER HENRIQUE VILELA DOS SANTOS GRUPO 3 Sorteio:00 1. AMANDA BEZERRA DE ALMEIDA 2. MAURO C?SAR GARCIA PATINI 3. RODRIGO PARENTE PAIVA BENTEMULLHER 4. DIOGO SOUZA SANTA CECÍLIA 2. EDUARDO SANTOS DA ROCHA PENTEADO 3. EMANUEL JOS? MATIAS GUERRA 4. GILBERTO

Maier, Rudolf Richard

213

arXiv:astroph/0410592 Astronomy & Astrophysics manuscript no. 1201main October 25, 2004  

E-Print Network (OSTI)

, Surrey RH5 6NT, UK 2 Paul Scherrer Institut, W?urenlingen & Villigen, 5232 Villigen PSI, Switzerland 3 Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY 10027, USA 4 material is seen in soft X­ray and extreme ultraviolet emissions, where the light curves are more gradual

Guedel, Manuel

214

arXiv:astroph/0408345 TO APPEAR IN THE ASTROPHYSICAL JOURNAL  

E-Print Network (OSTI)

MENSAE MARC AUDARD Columbia Astrophysics Laboratory, Mail code 5247, 550 West 120 th Street, New York, NY PSI, Switzerland STEPHEN L. SKINNER Center for Astrophysics and Space Astronomy, University in the X­ray light curves, we argue that YY Men's distance and X­ray brightness does not allow us to detect

Guedel, Manuel

215

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

216

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

217

arXiv:hep-ph/0701036v14Jan2007 Braneworld Quintessential Inflation and Sum  

E-Print Network (OSTI)

and quintessence--can occur for a sum of exponentials or cosh potential, a type of potential that arises naturally production and the universe undergoes a transition from primordial inflation to radiation domination well before big bang nucleosynthesis. The transition to an accelerating universe due to quintessence occurs

Gardner, Carl

218

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

219

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

220

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

Note: This page contains sample records for the topic "xiv-1 xiv morocco" from the National Library of EnergyBeta (NLEBeta).
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221

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

222

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.

223

arXiv:astro-ph/0110352 v1 15 Oct 2001  

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

redistributes magnetic helicity (a measure of twistedness and knottedness of magnetic field lines) but conserves its total value. It can be shown that fast and unquenched dynamos...

224

arXiv:submit/0214764[math.NT]17Mar2011 Adelic Openness for Drinfeld Modules  

E-Print Network (OSTI)

Characteristic Anna Devic Richard Pink March 17, 2011 Abstract For any Drinfeld module of special characteristic

Pink, Richard

225

arXiv:cond-mat/0402252v19Feb2004 Europhysics Letters PREPRINT  

E-Print Network (OSTI)

. ­ Biological membranes typically contain various components such as lipid mixtures, sterols, and proteins cases particular proteins [3]. Moreover, cholesterol-rich domains have been directly observed in model with a surrounding background in a liquid-disordered (Ld) state [3]. From a physical viewpoint, a strategy

226

arXiv:astro-ph/0402616v125Feb2004 ASP Conference Series, Vol. XXX, 2004  

E-Print Network (OSTI)

review the design of QUEST as a VO resource, a federated data set and an exemplar of VO standards. 1 of astronomy: data gathering, distribution, reduction, analysis, storage, archiving, dissemination and mining to transients (see section 4) is planned. 3. QUEST and VO technol

Williams, Roy

227

arXiv:0810.1843v1 SFB/CPP-08-82  

E-Print Network (OSTI)

-light meson spectrum from twisted mass lattice QCD Karl Jansen DESY, Platanenallee 6, D-15738 Zeuthen, Germany karl.jansen@desy.de Chris Michael, Andrea Shindler Theoretical Physics Division, Department

228

POS (LATTICE 2008) 242 arXiv:0810.0620v1  

E-Print Network (OSTI)

J. Gonzalez Lopez b;z , K. Jansen #3;z and A. Shindler l b Humboldt­Universität zu Berlin, Institut­mail: jenifer.gonzalez.lopez@desy.de, karl.jansen@desy.de, andrea.shindler@liv.ac.uk The Schrödinger functional Conditions K. Jansen 1. QCD and tmQCD continuum actions in infinite volume In the continuum, the QCD action

229

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

230

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

231

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

232

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.

233

Parent stars of extrasolar planets XIV. Strong evidence of Li abundance deficit  

Science Journals Connector (OSTI)

......to expand our comparison sample used to test whether stars with Doppler-detected giant...The purpose of the present study is to test again the claim that the Li abundances...peer-reviewed literature in order to test the robustness of the results obtained......

G. Gonzalez

2015-01-01T23:59:59.000Z

234

arXiv:hep-ph/0409008v11Sep2004 SCIPP 04/13  

E-Print Network (OSTI)

. However, it is difficult to imagine a fundamental theory of elementary particles and their interactions the data to constrain This work was supported in part by the U.S. DOE grant no. DE-FG03-92ER40689. 1 #12

California at Santa Cruz, University of

235

Revised Version DESY 06230 arXiv:0705.2018v2  

E-Print Network (OSTI)

-230 Neutrino Dark Energy { Revisiting the Stability Issue Ole Eggers Bj#26;lde 1 , Anthony W. Brook#12;eld 2 Oslo, Norway 6 Deutsches Elektron-Synchroton DESY, Hamburg, Notkestr. 85, 22607 Hamburg, Germany 7 and the present energy density and equation of state of dark energy. However, it has been pointed out

236

arXiv:cond-mat/970526626May1997 DYNAMICS AND TRANSPORT  

E-Print Network (OSTI)

of the NATO Advanced Study Institute on Dynamical properties of unconventional magnetic systems, Geilo, Norway by an experimentally measurable energy scale, which van- ishes at g = gc. Convenient choices are an energy gap, if one ¯ is an ultraviolet cutoff, measured in units of energy, z is the dy- namic exponent, and is the correlation length

237

arXiv:hepex/0207037 2002 A DEPARTURE FROM PREDICTION: ELECTROWEAK PHYSICS AT  

E-Print Network (OSTI)

current (NC) to charged current (CC) total cross sections 1 : R #23; #17; #27;(#23; #22; N ! #23; #22; X) #27;(#23; #22; N ! #22; X) = #27; #23; NC #27; #23; CC = g 2 L + r g 2 R = 1 2 sin 2 #18; W + 5 9 (1 + r) sin 4 #18; W R #23; #17; #27;(#23; #22; N ! #23; #22; X) #27;(#23; #22; N ! #22; + X) = #27; #23

238

arXiv:0708.1542v1 [nlin.AO] 11 Aug 2007  

E-Print Network (OSTI)

Aug 11, 2007 ... each individual can produce descendants (offsprings) ac- cording to some ..... J. Rundle, D. Turcotte, and W. Klein (eds), Geo- complexity and...

2007-08-11T23:59:59.000Z

239

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

240

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

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.
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241

Solvent-refined-coal (SRC) process. Volume II. Sections V-XIV. Final report  

SciTech Connect

This report documents the completion of development work on the Solvent Refined Coal Process by The Pittsburgh and Midway Coal Mining Co. The work was initiated in 1966 under Office of Coal Research, US Department of Interior, Contract No. 14-01-0001-496 and completed under US Department of Energy Contract No. DE-AC05-79ET10104. This report discusses work leading to the development of the SRC-I and SRC-II processes, construction of the Fort Lewis Pilot Plant for the successful development of these processes, and results from the operation of this pilot plant. Process design data generated on a 1 ton-per-day Process Development Unit, bench-scale units and through numerous research projects in support of the design of major demonstration plants are also discussed in summary form and fully referenced in this report.

Not Available

1982-05-01T23:59:59.000Z

242

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

243

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

244

arXiv:astro-ph/0411019v131Oct2004 CURRENT STATUS OF THE SUPERWASP PROJECT  

E-Print Network (OSTI)

, The Open University, Milton Keynes, MK7 6AA, UK 3 School of Physics & Astronomy, University of St. Andrews. SuperWASP consists of up to 8 individual cameras using ultra-wide field lenses backed by high

Norton, Andrew J.

245

SOFT X-RAY EMISSION LINES OF S VII-S XIV IN PROCYON  

SciTech Connect

Observational data for cool star Procyon available from the Chandra Data Public Archive are co-added and analyzed with as high a signal-to-noise ratio as possible. The soft X-ray emission lines of highly charged sulfur ions (S VII-S XV) are investigated in the 30-80 A range. A collisional-radiative model is constructed to predict line emissivities of sulfur ions using updated excitation data from the R-matrix method. Theoretical line fluxes and line intensity ratios are calculated, and theoretical spectra are constructed with a Gaussian profile with a line width of 0.06 A. By comparing predicted emission lines with observed ones, several strong emission lines are identified for the first time. Some misassignments of lines in previous works are also corrected. By comparing our results with those from the Chianti (v6) model, this work provides insight into the completeness and accuracy of the atomic data of sulfur ions in the Chianti (v6) database.

Li, F.; Liang, G. Y.; Zhao, G., E-mail: gyliang@bao.ac.cn, E-mail: gzhao@bao.ac.cn [Also at National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China. (China)

2013-01-01T23:59:59.000Z

246

arXiv:astroph/0002191 Star Formation and Tidal Encounters with the Low Surface Brightness Galaxy  

E-Print Network (OSTI)

Observatory, HC03 Box 53995, Arecibo, PR 00612, email:koneil@naic.edu 2 National Radio Astronomy Observatory regions where the column density is above this star formation threshold. The low surface brightness nature of this galaxy could thus be attributed to an insufficient gas surface density, inhibiting star formation

O'Neil, Karen

247

arXiv:astro-ph/0310031v11Oct2003 On the morphogenesis of stellar flows  

E-Print Network (OSTI)

gravitational structures has spring up in many astrophysical domains. The large number and the stability with slow winds. This collision induces a compressed zone where a hot bubble creates the observable bright- lar shells are not directly connected to the hot bubble resulting from the collision [2]. Thus

Nottale, Laurent

248

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

249

Immobilized catalysts. XIV. Influence of sysnthesis conditions on fixation of copper complexes  

SciTech Connect

The influence of conditions of the reaction (concentration relationships, reaction temperature) of the polymeric carrier PE-grafted-poly(acrylic acid) with Cu(OCOCH/sub 3/)/sub 2/ on the amount of Cu(II) bound and the structure of the immobilized complexes was studied. The ''concentration'' dependence is Langmuirian in character and its analysis leads to the evaluation of the stability constant of Cu(II) complexes, equal to 300 liters/mole at 333 degrees K. The constant corresponding to the limiting binding of Cu(II) is equal to 0.35 mole/mole (22.22 mg of Cu(II)/g). By using the labeled atoms technique, a stepwise mechanism of fixation of Cu(II) was shown: binding by means of one (up to 16 mole% with respect to fixated Cu(II), k/sub 1/ = 16.10/sup -//sub 2/ mole/g) and two (k/sub 2/ = 2.54.10/sup -//sub 3/ mole/g) carboxyl groups of the grafted fragments. In the PE-gr-PAA-Cu(II) systems the conditions, viz., an insoluble polymeric substrate - a soluble polymeric functional coating, are modeled, whence the advantages of soluble and three-dimensional cross-linked polymers are shown.

Pomogailo, A.D.; Golubeva, N.D.

1986-02-01T23:59:59.000Z

250

arXiv:astro-ph/0510375v112Oct2005 Comparison of air fluorescence and ionization  

E-Print Network (OSTI)

is maintained similar in shape in all showers, independent of initial energy, aside from the relatively sparsely, Salt Lake City, UT 84112, U.S.A. P. Chen, C. Field , C. Hast, R. Iverson, J.S.T. Ng, A. Odian, K. Reil fluorescence profiles in measuring ultra high energy cosmic rays. Key words: air fluorescence, electromagnetic

251

arXiv:astroph/0510375 Comparison of air uorescence and ionization  

E-Print Network (OSTI)

is maintained similar in shape in all showers, independent of initial energy, aside from the relatively sparsely Univ. of Utah, Salt Lake City, UT 84112, U.S.A. P. Chen, C. Field #3; , C. Hast, R. Iverson, J.S.T. Ng of atmospheric uorescence pro#12;les in measuring ultra high energy cosmic rays. Key words: air uorescence

252

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

E-Print Network (OSTI)

Oct 30, 2009 ... With this, the current complexity status of the problem SDP1 is similar to the one of the .... allows us to write the integral in a more explicit form. ..... energy. Finding the minimal energy is equivalent to finding the value SDPn(LA),.

2009-10-29T23:59:59.000Z

253

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.

254

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

255

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

256

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

257

arXiv:astro-ph/0506614v124Jun2005 Draft version June 24, 2005  

E-Print Network (OSTI)

, substantially more dark energy information can be recovered (Hu 1999). In fact future weak lensing surveys- scope Legacy Survey (CFHTLS4 ) and the Dark Energy Email: mzm@oddjob.uchicago.edu 1 http to less than a factor of 1.5 increase in the dark energy parameter errors. The more stringent requirement

Hu, Wayne

258

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

259

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

260

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

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261

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

262

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

263

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.

264

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

265

arXiv:0902.1105v2 [math.OC] 4 May 2009  

E-Print Network (OSTI)

May 4, 2009 ... We thank Etienne de Klerk and Renata Sotirov for initiating our collaboration and we thank Frank Bowert and Rudolf Scharlau for bringing the...

2009-05-04T23:59:59.000Z

266

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

267

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

268

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.

269

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.

270

Revised Version DESY 09120 arXiv:0908.0878v2  

E-Print Network (OSTI)

on Complex Projective Superspaces Constantin Candu 1 , Vladimir Mitev 1 , Thomas Quella 2 , Hubert Saleur 3

271

E-Print Network 3.0 - archipelago tunisia north Sample Search...  

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

Biology and Medicine 6 Algeria Gambia Nigeria Angola Ghana Reunion Summary: Togo Egypt Mauritius Tunisia Equatorial Guinea Morocco Uganda Eritrea Mozambique Zambia......

272

Meyer-Harms, Bettina, Xabier Irigoien, Robert Head, and Roger ...  

Science Journals Connector (OSTI)

M. Head and Harris (1994) first used this method to describe selective feeding by different size-fractionated zooplankton off the coast of Morocco. A modification...

1999-03-11T23:59:59.000Z

273

E-Print Network 3.0 - alpha spectrometry 232u Sample Search Results  

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

18 DISTRIBUTION OF NATURALLY OCCURRING RADIONUCLIDES (U, Th) IN TIMAHDIT'S BLACK SHALE (MOROCCO) Summary: (2005). 232 U in equilibrium with its daughters has been used as...

274

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

Open Energy Info (EERE)

CSP programs of five countries in the Middle East and North Africa: Algeria, Egypt, Jordan, Morocco, and Tunisia." References "Mexico-CTF Investment Plan" Retrieved from...

275

How to Obtain Authorization to Import and/or Export Natural Gas...  

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

Canada, Chile, Colombia, Dominican Republic, El Salvador, Guatemala, Honduras, Jordan, Mexico, Morocco, Nicaragua, Oman, Panama, Peru, Republic of Korea and Singapore....

276

SAFEGUARD AND SECURE CONTROL VERIFY POLICY  

National Nuclear Security Administration (NNSA)

and their national labora- tories, along with representatives from COEs in Morocco, Jordan, and Japan, attended the workshop. Facilitated by Pacific Northwest National...

277

Sandia National Laboratories: Wind and Water Materials and Structures...  

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

Moldova Monaco Mongolia Montenegro Montserrat Morocco Mozambique Myanmar Namibia Nauru Nepal Netherlands New Zealand Nicaragua Niger Nigeria Norway Northern Mariana Islands Oman...

278

E-Print Network 3.0 - african migrants assessed Sample Search...  

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

arrived migrants were born in Algeria (1,437 people), 15% in Morocco... Sub-Saharan Africa (nearly 40 %) than for migrants from ... Source: Ecole Polytechnique, Centre de...

279

Reports and discussion on preprint arXiv:gr-qc/0511113 On the geometry of cosmological model building  

E-Print Network (OSTI)

, that is in my opinion too negative. Examples: a) While I consider with many colleagues the Dark Energy, the Dark Energy is a mystery, but that makes it very interesting (Planck's radiation law was also mystery as a great discovery pointing to new physics, with an enormous impact both on fundamental physics

Scholz, Erhard

280

Evaluation of the opsonic requirements for phagocytosis of Streptococcus pneumoniae serotypes VII, XIV, and XIX by chemiluminescence assay.  

Science Journals Connector (OSTI)

...also appar- ent in the divergent results of previous investi- gators (Table 2). On the other hand, functional assays of opsonic...be inter- preted with caution, since we and other investi- gators have demonstrated a pronounced varia- bility in CL peak height...

K K Matthay; W C Mentzer; D W Wara; H K Preisler; N B Lameris; A J Ammann

1981-01-01T23:59:59.000Z

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281

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

282

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.

283

arXiv:math/0609728v1[math.AG]26Sep2006 ON CALABI-YAU THREEFOLDS WITH LARGE  

E-Print Network (OSTI)

. To show the last assertion, observe that if the lift of had a fixed point, then the image of that point of four quadrics y1y3(x2 0 + x2 4) - y2 2(x1x7 + x3x5) + (y2 1 + y2 3)x2x6 = 0 y1y3(x2 1 + x2 5) - y2 2(x23(x2 3 + x2 7) - y2 2(x4x2 + x6x0) + (y2 1 + y2 3)x5x1 = 0. This variety has 64 ODP singular points

Borisov, Lev

284

arXiv:astro-ph/0512628v229Dec2005 Multiwavelength Observations of the Blazar Mrk 421 in  

E-Print Network (OSTI)

of Physics and Astronomy, University of Leeds, Leeds, LS2 9JT, Yorkshire, England, UK 5 Department of Physics, USA. 12 Physics Department, McGill University, Montreal, QC H3A 2T8, Canada 13 Fred Lawrence Whipple, Ann Arbor, MI 48109, USA 20 Boltwood Observatory, Ontario, Canada 21 University of California, Davis

285

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

E-Print Network (OSTI)

of Physics and Astronomy, University of Leeds, Leeds LS2 9JT, UK 6 INAF - Osservatorio Astrofisico di Arcetri Council Canada, Herzberg Institute of Astrophysics, 5071 West Saanich Road, Vic- toria, BC V9E 2E7, Canada 10 Department of Physics and Astronomy, University of Victoria, Victoria, BC V8P 1A1, Canada 11

286

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

287

arXiv:0804.3651v2[math.AG]24Apr2008 MONODROMY FILTRATIONS AND THE TOPOLOGY OF  

E-Print Network (OSTI)

of a polyhedral complex. In [H], Hacking proved that if X is a subvariety of (C )n satisfying a certain genericity condition, then the link of the fan Trop(X) only has reduced rational homology in the top dimension. Hacking : Trop(C) that is affine-linear on edges. Our results can be seen as the analogue of Hacking's result

Helm, David

288

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

289

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

290

arXiv:1103.1157v2[cs.AI]9Mar2011 GRASP AND PATH-RELINKING FOR  

E-Print Network (OSTI)

DI MAURO, TERESA M.A. BASILE, STEFANO FERILLI, AND FLORIANA ESPOSITO Abstract. In Artificial of each coalition is given by a characteristic 1 #12;2 N. DI MAURO, T.M.A. BASILE, S. FERILLI, AND F

Di Mauro, Nicola

291

arXiv:1006.5188v1[cs.AI]27Jun2010 Feature Construction for  

E-Print Network (OSTI)

Mauro, Teresa M.A. Basile, Stefano Ferilli, and Floriana Esposito Universit`a degli Studi di Bari algorithms adopting a #12;2 Nicola Di Mauro, Teresa M.A. Basile, Stefano Ferilli, and Floriana Esposito

Di Mauro, Nicola

292

arXiv:0805.4010v1[astro-ph]26May2008 Draft version May 27, 2008  

E-Print Network (OSTI)

. Subject headings: pulsars: general -- radiation mechanisms: non-thermal -- radio continuum: stars -- stars-Hofmeister 1999; Mohanty et al. 2002). Importantly, this reduction in the non-radiative heat- ing of plasma be associated with the decreasing fractional ionization of the photo- sphere and atmosphere with later spectral

293

arXiv:cond-mat/0511322v114Nov2005 Glass transition in a fluidized bed of hard spheres  

E-Print Network (OSTI)

. Fluid flow rate fluctuations are smaller than 0.3%. To obtain a uniform flow, fluid passes. Goldman and Harry L. Swinney Center for Nonlinear Dynamics and Department of Physics, The University motion arrested) by application of a small increase in flow rate. Thus a fluidized bed can serve

Weeks, Eric R.

294

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.

295

arXiv:astro-ph/0307433v124Jul2003 THE AGILE ARCHIVE AND DATA PROCESSING AT  

E-Print Network (OSTI)

of the Gamma Ray Imaging Detector (GRID) and the hard X-ray imager Super-AGILE (SA). GRID, sensitive in the energy range 30 MeV-50 GeV, is made of 12 Si-W planes and the Mini Calorimeter, sensitive in the energy GRID tray. The ASI Science Data Center (ASDC) will host the AGILE Data Center (ADC). The ADC includes

296

Introduction to Theoretical Meterology. Seymour L. Hess. Holt, New York, 1959. xiv + 362 pp. Illus. $8.50  

Science Journals Connector (OSTI)

...defined group of fresh-water algae on a world-wide...to the problems of atmospheric motion. These are...explanation of the gen-eral atmospheric circulation. This...is the treatment of condensation and precipitation prob-lems...techniques of detection, recovery, and identification...

H. E. Landsberg

1960-05-27T23:59:59.000Z

297

arXiv:physics/0302084v124Feb2003 Alignment-to-orientation conversion and nuclear quadrupole resonance  

E-Print Network (OSTI)

, California 94720-1460 (Dated: February 24, 2003) The role of alignment-to-orientation conversion (AOC) in nuclear quadrupole resonance (NQR) is discussed. AOC is shown to be the mechanism responsible are drawn between NQR and AOC in atomic physics. PACS numbers: 76.60.Gv, 32.80.Bx Polarization is a generic

Budker, Dmitry

298

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

299

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

300

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

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While these samples are representative of the content of NLEBeta,
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301

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

302

arXiv:0706.1749v1[astro-ph]12Jun2007 30th International Cosmic Ray Conference  

E-Print Network (OSTI)

¨ue, Argentina 1 Depto de F´isica, Centro At´omico Bariloche, CNEA and CONICET, Argentina mollerach@cab.cnea.gov.ar Abstract: If clustering of the arrival directions of ultra high energy cosmic rays is discovered Auger Observatory as a function of the angular scale and the energy threshold. We compare our results

303

arXiv:0706.1256v1[astro-ph]8Jun2007 30th International Cosmic Ray Conference  

E-Print Network (OSTI)

] spans over 3000 km2 in Malarg¨ue (Argentina), at 1400 m a.s.l., investigating the ultra high energy cos, Argentina 2 Av. San Martin Norte 304 (5613) Malarg¨ue, Prov. de Mendoza, Argentina bertou filled with 12 m3 of water, can detect the putative high energy emis- sion of a GRB (photons down

304

arXiv:0706.3940v1[astro-ph]26Jun2007 30th International Cosmic Ray Conference  

E-Print Network (OSTI)

- high energy cosmic rays. The Southern Auger Observatory in Mendoza province, Argentina, is approaching, Houghton, MI 49931, USA 2 Observatorio Pierre Auger, Av. San Mart´in Norte 304, (5613) Malarg¨ue, Argentina and composition of ultra-high energy cosmic rays up to and beyond the predicted GZK feature. We are obtaining

305

arXiv:0706.1491v1[astro-ph]11Jun2007 30TH INTERNATIONAL COSMIC RAY CONFERENCE  

E-Print Network (OSTI)

¨ue, Mendoza, Argentina C.Bleve@leeds.ac.uk Abstract: The rate of events measured with the surface detector The surface detector (SD) of the Auger Southern Observatory, located in Malarg¨ue, Argentina, is de- signed for the detection of ultra high energy cos- mic rays through the measurement of the signal in- duced by the shower

306

arXiv:1004.0836v1[astro-ph.EP]6Apr2010 DRAFT VERSION APRIL 7, 2010  

E-Print Network (OSTI)

. POLLACCO 15 , FREDERIC PONT 16 , IAN SKILLEN 17 , BARRY SMALLEY 5 , RACHEL A. STREET 18 , STEPHANE UDRY 8, Switzerland 9Institut d'Astrophysique et de Géophysique, Université de Liège, Allée du 6 Août, 17, Bat. B5C from the day side to the night side of the planet. We fit the Spitzer light curves simultaneously

Norton, Andrew J.

307

arXiv:1210.1979v1[astro-ph.IM]6Oct2012 Image Analysis for Cosmology  

E-Print Network (OSTI)

, U.K. tdk@roe.ac.uk 2 Department of Physics and Astronomy, University College London, Gower Street), Switzerland 9 Aalto University, Department of Information and Computer Science, P.O. Box 15400, FI-00076 Aalto, Finland 10 University of Edinburgh, School of Informatics, 10 Crichton Street, Edinburgh, EH8 9AB, United

Storkey, Amos

308

arXiv:0904.1953v1[astro-ph.SR]13Apr2009 DRAFT VERSION APRIL 14, 2009  

E-Print Network (OSTI)

style emulateapj v. 10/09/06 ENERGY DISSIPATION THROUGH QUASI-STATIC TIDES IN WHITE DWARF BINARIES B-static tide approximation. For the shortest period binaries, energy dissipation is therefore expected to take tidal interactions in white dwarf binaries in the limiting case of quasi-static tides, in which

Kalogera, Vicky

309

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.

310

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

311

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

312

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

313

arXiv:1004.4881v1[astro-ph.SR]27Apr2010 Solar Physics  

E-Print Network (OSTI)

observations of the cross helicity. Keywords: Sun: magnetic field ­ Magnetohydrodynamics (MHD) 1. Introduction in the northern (southern) hemisphere. This result is based on a ring-diagram analysis of GONG data. The values

314

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

315

arXiv:cs.NE/0512037v213Dec2005 APS/123-QED Evolving Stochastic Learning Algorithm Based on Tsallis  

E-Print Network (OSTI)

,p - tj,p 2 = P p=1 nL j=1 L netL j + L j - tj,p 2 . (1) where, netL j is for the j-th node in the l

Magoulas, George D.

316

arXiv:submit/0094658[math.NA]19Aug2010 DUALITY-BASED ASYMPTOTIC-PRESERVING METHOD FOR HIGHLY  

E-Print Network (OSTI)

- neutral plasma simulations [10], image processing [37, 38], atmospheric or oceanic flows [36] and so on simulations such as atmospheric plasma [24, 26], internal fusion plasma [4, 12] or plasma thrusters [1) or Neumann boundary conditions (atmospheric plasma for example [5]). For these reasons we propose a strongly

Negulescu, Claudia

317

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.

318

arXiv:1012.1626v1[astro-ph.SR]7Dec2010 **Volume Title**  

E-Print Network (OSTI)

gyrosynchrotron radiation from electrons with much higher energies than typically present in the solar atmosphere´onoma de M´exico, Apartado Postal 3-72, 58090, Morelia, Michoac´an, Mexico Abstract. This splinter session energy release X-rays and radio emission are excellent diagnostic probes to study energy release

Guedel, Manuel

319

arXiv:astroph/0106467 A critical appraisal of ATLAS9 and NextGen 5 model  

E-Print Network (OSTI)

Galileo, Spain, 4 INAOE, Mexico. Abstract. The #12;tting atmosphere parameters (Te#11; , g, and [Fe/H]) by comparing its observed spectral energy distribution with a grid of synthetic spectra. The #12;du- cial best with the solar metallicity model grids of ATLAS9 (3500 #20; T e#11; #20; 50 000 K, 0:0 #20; log g #20; 5

Buzzoni, Alberto

320

arXiv:1312.2923v1[stat.AP]10Dec2013 STATISTICAL SCIENCE RESEARCH REPORT 322  

E-Print Network (OSTI)

, instruments are one of the primary ways of directly observing the ocean currents. For studying the currents Models for Ocean Surface Drifter Trajectories Adam M. Sykulski, Sofia C. Olhede, Jonathan M. Lilly and Eric Danioux Abstract This paper proposes stochastic models for the analysis of ocean surface

Guillas, Serge

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321

arXiv:astro-ph/0411121v14Nov2004 Observations of Diffuse EUV Emission with the Cosmic Hot  

E-Print Network (OSTI)

limit on the emission measure is about 0.0004 cm-6 pc for solar abundance plasma with foreground neutral

322

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

323

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

324

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

325

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

326

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

327

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

328

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

329

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

330

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

331

arXiv:cond-mat/010139425Jan2001 Comment on "Critical spin dynamics of the 2D quantum Heisenberg  

E-Print Network (OSTI)

the crossover into the RC regime. The scaling arguments of [3] predict that R(T) obeys R(T) = A T/(c2u(T)), (2

332

arXiv:1402.3591v2[astro-ph.HE]19Feb2014 Draft version February 21, 2014  

E-Print Network (OSTI)

-rays from the inner part of the accretion disc, ionised winds/absorbers, and Comptonisation. The ionised. INTRODUCTION Matter accreting onto supermassive black holes pro- duces emission from radio­to­X-ray energies and gas which introduces absorp- tion features including a low-energy fall-off from photo- electric

Koch, Christof

333

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

334

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

335

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

E-Print Network (OSTI)

.I. Kravtsov ag , K. Krueger a , M. Krus k , C. Kuhn q , L. Kumar ae , P. Kurnadi f , M.A.C. Lamont c , J aw , V.Yu. Khodyrev ag , D.P. Kikola v , J. Kiryluk v , A. Kisiel ac , S.R. Klein v , A.G. Knospe ba

Llope, William J.

336

arXiv:astro-ph/0508176v18Aug2005 A Potential Supernova Remnant/X-ray Binary Association in  

E-Print Network (OSTI)

@head.cfa.harvard.edu 2 The Department of Physics and Astronomy, The Open University, Walton Hall, Milton Keynes, MK7 6BT been discovered in recent years. Roberts & Colbert (2003) inferred a black hole XRB in the ultra

Barnard, Robin

337

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

E-Print Network (OSTI)

Ongoing studies in nuclear astrophysics are focused on the opposite ends of the energy scale of nuclear, and energy production in stars. A. Nuclear reaction rates Low energy nuclear astrophysics requires the knowl presented at the XXXI Symposium on Nuclear Physics held in the Hacienda Cocoyoc, Mexico, Jan. 7-10, 2008. e

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

338

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

339

arXiv:0810.2276v1[math.ST]13Oct2008 A GENERALIZED PORTMANTEAU TEST  

E-Print Network (OSTI)

.g. Bouhaddioui and Roy (2006), Duchesne and Roy (2003), Eichler (2006), Hallin and Saidi (2005, 2007). Consider

Shao, Xiaofeng

340

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.

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341

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

342

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

343

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

344

arXiv:cond-mat/0703632v123Mar2007 Sideband Transitions and Two-Tone Spectroscopy  

E-Print Network (OSTI)

to a superconducting transmission line resonator. When the Cooper pair box is operated at the optimal charge bias point on a set of Cooper pair boxes strongly coupled to a high quality transmission line resonator [12. A promising route towards the implementation of a scalable solid state quantum information processor [1

Wallraff, Andreas

345

La collaboration littraire sous Louis XIV, expression dune communaut Logique de Port-Royal (1662) et Psych (1671)  

E-Print Network (OSTI)

questionnement quant la collaboration de Mnage ou de Laincit et organis la collaboration scientifique, notammenttroisime partie, la collaboration aurait t plus intime.

Morvant, Eglantine

2009-01-01T23:59:59.000Z

346

Description and crystal structure of maghrebite, MgAl2(AsO4)2(OH)28H2O, from Aghbar, Anti-Atlas, Morocco: first arsenate in the laueite mineral group  

Science Journals Connector (OSTI)

...other minerals include erythrite, talmessite/roselite-beta, wendwilsonite...crystals of roselite-wendwilsonite and talmessite were deposited within dolomite in quartzitic...isolated maghrebite crystal on Co-bearing talmessite. Picture width: 1 mm. 3. Appearance...

Nicolas Meisser; Jol Brugger; Sergey Krivovichev; Thomas Armbruster; Georges Favreau

347

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

348

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

349

Comment on "Efficiency of Isothermal Molecular Machines at Maximum Power"  

E-Print Network (OSTI)

Comment on "Efficiency of Isothermal Molecular Machines at Maximum Power" (PRL 108, 210602 (2012), arXiv:1201.6396)

Yunxin Zhang

2012-06-06T23:59:59.000Z

350

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

351

E-Print Network 3.0 - allergen nickel sulfate Sample Search Results  

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

. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . S66 XIV. Allergens... and patch) and in vitro tests for a wide ... Source: Levetin, Estelle - Department of Biological...

352

Modeling the Logistics Performance in Developing Countries: An exploratory study of Moroccan context  

E-Print Network (OSTI)

1 Modeling the Logistics Performance in Developing Countries: An exploratory study of Moroccan to raise their levels of logistics performance. This article is a research progress; it presents, Technological Practices, Supply Chain performance, Morocco. 1. INTRODUCTION: Logistic in Morocco is still

Paris-Sud XI, Université de

353

Buildings, Group Homology and Lattices.  

E-Print Network (OSTI)

This is the author's PhD thesis, published at the Universitt Mnster, Germany in 2010. It contains a detailed description of the results of arXiv:0903.1989, arXiv:0905.0071 and arXiv:0908.2713.

Jan Essert

354

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

355

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

356

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

357

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

358

arXiv:1101.5347v1[physics.plasm-ph]27Jan2011 Gauge-Free Hamiltonian Structure of the Spin Maxwell-Vlasov Equations  

E-Print Network (OSTI)

of our findings. High energy density plasma physics has become a popular subject (see, e.g., [9 the different approaches). The field of quantum kinetic theory [7] in many ways started with the ambitions for the theory, and present an energy-like theorem that demonstrates that all equilibria with monotonically

Morrison, Philip J.,

359

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

360

arXiv:1004.2880v1[cs.AI]16Apr2010 GRASP for the Coalition Structure Formation Problem  

E-Print Network (OSTI)

Mauro, Teresa M.A. Basile, Stefano Ferilli, and Floriana Esposito University of Bari, Italy, {ndm must search at least 2n - 1 coalition structures. #12;2 Nicola Di Mauro, Teresa M.A. Basile, Stefano

Di Mauro, Nicola

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361

arXiv:1108.1713v1[nucl-th]5Aug2011 The EIC Science case: a report on the joint BNL/INT/JLab program  

E-Print Network (OSTI)

Groningen, The Netherlands M. Diehl, Deutsches Elektronen-Synchroton DESY, Germany R. Milner, Massachusetts. Editors: D. Boer, Universiteit Groningen, The Netherlands M. Diehl, Deutsches Elektronen-Synchroton DESY

Gilfoyle, Jerry

362

The Membranes. Albert J. Dalton and Franoise Haguenau, Eds. Academic Press, New York, 1968. xiv + 224 pp., illus. $12.50. Ultrastructure in Biological Systems, vol. 4  

Science Journals Connector (OSTI)

...technically excel-lent electron micrographs. The other-wise lucidly written paper becomes somewhat confused and hazy in...San Francisco Radiation and Its Effects Radiation Biology. ALIsON P. CASARETT. Prepared under the auspices of the Ameri-can...

Walther Stoeckenius

1969-02-07T23:59:59.000Z

363

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

364

arXiv:1011.0127v2[hep-ex]2Nov2010 Precise Measurements of Direct CP Violation, CPT Symmetry, and Other  

E-Print Network (OSTI)

and Institute of Nuclear and Particle Physics, University of Virginia, Charlottesville, Virginia 22901 12 and CPT symmetry based on the full dataset of K decays collected by the KTeV experiment at Fermi National Accelerator Laboratory during 1996, 1997, and 1999. This dataset contains 16 million K 0 0 and 69

Fermilab

365

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

366

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

367

arXiv:0909.3645v1[astro-ph.CO]20Sep2009 Suzaku Observations of the Radio Galaxy 3C 33  

E-Print Network (OSTI)

. Evans1 , James N. Reeves2 , Martin J. Hardcastle3 , Ralph P. Kraft4 , Julia C. Lee4 , and Shanil N

Evans, Dan

368

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

369

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

370

arXiv:1402.1766v1[astro-ph.SR]7Feb2014 Astronomy & Astrophysics manuscript no. ms c ESO 2014  

E-Print Network (OSTI)

, Switzerland e-mail: thalmann@phys.ethz.ch 2 Astronomical Institute "Anton Pannekoek", University of Amsterdam & Astronomy, College of Charleston, 58 Coming Street, Charleston, SC 29424, USA 11 Astrophysics Department planets in the system. Finally, we find that the bright arc of scattered light we see in direct imaging

Henning, Thomas

371

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.

372

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.

373

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

374

arXiv:0710.1758v1[cond-mat.supr-con]9Oct2007 Particle-hole mixing in the pseudogap state of preformed pairs  

E-Print Network (OSTI)

region in the phase diagram corresponds to the Bogolubov-like quasiparticles and, ultimately whether various ex- perimental studies it is known that HTSC materials have kF momentum normal state pseudogap the mean-field framework to account for these strong quantum fluctuations. To handle such problems we use

Domanski, Tadeusz

375

Plant Communities. A Textbook of Plant Synecology. Rexford Daubenmire. Harper and Row, New York, 1968. xiv + 300 pp., illus. $9.75  

Science Journals Connector (OSTI)

...The rock succession diagram shows principal stages...spruce-shrub belt. The au-thor also makes clear that...Arrowed succes-sional diagrams may be real, or they...speculation in Hartmann's handling of the relation-ship...cogent syn-thesis of the material, it quickly be-comes...

William A. Niering

1968-11-08T23:59:59.000Z

376

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

377

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

378

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

379

arXiv:1304.3175v2[nucl-th]17Apr2013 Microscopic optical potential from chiral nuclear forces  

E-Print Network (OSTI)

numerous theoretical frameworks, in- cluding Brueckner-Hartree-Fock (BHF) theory [5­11], Dirac-Brueckner

Weise, Wolfram

380

arXiv:hep-ex/0310047v315Jan2004 A High Sensitivity Search for e's from the Sun and Other Sources at KamLAND  

E-Print Network (OSTI)

in the Sun and has the characteristic 8 B solar e energy spectrum, we obtain an upper limit of 3.7 � 102 cm-2 State University, Baton Rouge, Louisiana 70803, USA 8 Physics Department, University of New Mexico, Albuquerque, New Mexico 87131, USA 9 Physics Department, Stanford University, Stanford, California 94305, USA

Learned, John

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381

arXiv:hep-ex/0310047v123Oct2003 A High Sensitivity Search for e's from the Sun and Other Sources at KamLAND  

E-Print Network (OSTI)

that all �e flux has its origin in the Sun and has the characteristic 8 B solar e energy spectrum, we of New Mexico, Albuquerque, New Mexico 87131, USA 9 Physics Department, Stanford University, Stanford at Chapel Hill 12 Institute of High Energy Physics, Beijing 100039, People's Republic of China (Dated

Mcdonough, William F.

382

arXiv:1106.5208v3[cond-mat.mes-hall]25Apr2012 Thermoelectric transport with electron-phonon coupling and electron-electron  

E-Print Network (OSTI)

expands the potential of using thermoelectricity for meeting the challenge of being a sustainable energy. Gubernatis,3 Chen Wang,2, 4 and Baowen Li1, 2 1 NUS Graduate School for Integrative Sciences and Engineering for the generation and harvesting of energy. It is well accepted that nanoscale materials en- gineering in principle

Li, Baowen

383

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

384

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

385

arXiv:0709.4029v1[astro-ph]26Sep2007 Self Calibration of Tomographic Weak Lensing for the Physics of Baryons to  

E-Print Network (OSTI)

such as the Dark Energy Survey (DES), the SuperNova/Acceleration Probe (SNAP), and the Large Synoptic Survey lensing surveys to constrain both the internal structures of halos and the properties of the dark energy- ing probes of dark energy is weak gravitational lens- ing. Forthcoming weak lensing surveys expect

Hu, Wayne

386

arXiv:0901.3557v1[astro-ph.IM]22Jan2009 Astronomy & Astrophysics manuscript no. sparsity c ESO 2009 January 22, 2009  

E-Print Network (OSTI)

Survey and the VISTA Kilo-Degree Infrared Galaxy Survey2 (KIDS/VIKING), the Dark Energy Survey3 (DES') is a powerful probe of dark energy and dark matter. A number of current and planned sur- veys are dedicated-STARRS), the SuperNovae Acceleration Probe5 (SNAP), the Large Synoptic Survey Telescope6 (LSST) and the Dark UNiverse

Masci, Frank

387

arXiv:0708.4391v1[astro-ph]31Aug2007 CMB Cluster Lensing: Cosmography with the Longest Lever Arm  

E-Print Network (OSTI)

, such as the South Pole Telescope in conjunction with the Dark Energy Survey, can potentially reach the statistical, and assess the impact future surveys may have on dark energy parame- ter measurements. For illustrative of magnitude higher sensitivity to dark energy parameters, and a decreased sensitivity to photometric redshift

Hu, Wayne

388

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.

389

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

390

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

391

Race to the Stratosphere. Manned Scientific Ballooning in America. David H. DeVorkin. Springer-Verlag, New York, 1989. xiv, 406 pp., illus. $39.50  

Science Journals Connector (OSTI)

...demonstrates. In the volume at hand, David DeVorkin has examined this association in the context of the manned stratospheric balloon flights of the 1930s. By a comparison with Project Apollo, he has illuminated patterns of poli-tics and patronage...

Robert Seidel

1989-09-22T23:59:59.000Z

392

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

393

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

394

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.

395

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

396

arXiv:0812.2106v1[hep-ph]11Dec2008 Preprint typeset in JHEP style -PAPER VERSION hep-th08  

E-Print Network (OSTI)

coupling unification at 2-loops for theories with 5 extra vectorlike SU(5) fundamentals added to the MSSM up into the UV. With 5 or more vectorlike SU(5) fundamentals1 added to the MSSM at the elec- troweak flavors are heavy enough, this statement does not apply. For the case of exactly 5 extra flavors, the mass

California at Santa Cruz, University of

397

arXiv:0708.2925v1[physics.atom-ph]21Aug2007 Using Molecules to Measure Nuclear Spin-Dependent Parity Violation  

E-Print Network (OSTI)

- currents (VeAn). This can be parameterized by two con- stants, C2u,d, which describe the VeAn couplings to up and down quarks. These are suppressed in the Standard Model (SM), making C2u,d difficult of this suppression, even moderately precise measurements of C2u,d could be sensitive to new physics at TeV energy

Kozlov, Mikhail G

398

Alan Weir. Truth through Proof: A Formalist Foundation for Mathematics. Oxford: Clarendon Press, 2010. ISBN 978-0-19-954149-2. Pp.xiv+281  

Science Journals Connector (OSTI)

......Critical Studies/Book Reviews Alan Weir. Truth through Proof: A Formalist Foundation...jburgess@princeton.edu Alan Weir. Truth through Proof: A Formalist Foundation...what in the mathematical case plays the truth-making role that in the Sherlock Holmes......

John P. Burgess

2011-06-01T23:59:59.000Z

399

arXiv:nucl-ex/0309012v115Sep2003 Pion, kaon, proton and anti-proton transverse momentum distributions from p+p and  

E-Print Network (OSTI)

.A. Kuznetsov,10 M.A.C. Lamont,3 J.M. Landgraf,2 S. Lange,12 C.P. Lansdell,36 B. Lasiuk,43 F. Laue,2 J. Lauret,2. Kaplan,7 D. Keane,17 J. Kiryluk,6 A. Kisiel,39 J. Klay,18 S.R. Klein,18 A. Klyachko,13 D.D. Koetke,37 T

Llope, William J.

400

arXiv:0906.2260v1[nucl-ex]12Jun2009 Center of mass energy and system-size  

E-Print Network (OSTI)

. Kumar ad , P. Kurnadi f , M.A.C. Lamont c , J.M. Landgraf c , S. LaPointe ay , J. Lauret c , A. Lebedev. Kettler aw , V.Yu. Khodyrev af , D.P. Kikola u , J. Kiryluk u , A. Kisiel av , S.R. Klein u , A.G. Knospe

Llope, William J.

Note: This page contains sample records for the topic "xiv-1 xiv morocco" from the National Library of EnergyBeta (NLEBeta).
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to obtain the most current and comprehensive results.


401

arXiv:0807.1545v1[astro-ph]9Jul2008 Science with the XEUS High Time Resolution Spectrometer  

E-Print Network (OSTI)

Astrophysik, Karl-Schwarzschild-Str. 1, D-85740 Garching bei Munchen, Germany, and Space Research Institute of XEUS is contained in the mirror spacecraft while the focal plane instruments are contained in the detector spacecraft, which is maintained at the focus of the mirror by formation flying. The main

Miller, Cole

402

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

403

arXiv:cond-mat/0301569v325Aug2003 Radiation-Induced Magnetoresistance Oscillations in a 2D Electron Gas  

E-Print Network (OSTI)

at = c due to heating at the cyclotron resonance. Interest in this phenomenon was heightened when, using on the ratio of radiation frequency to cyclotron frequency. We perform a diagrammatic calculation and find, µ, to the cyclotron frequency, c, these radiation-induced oscillations are controlled by the ratio

404

arXiv:1110.6490v1[cond-mat.supr-con]29Oct2011 Cryomagnetic scanning tunneling spectroscopy study of multi-gap spectra in  

E-Print Network (OSTI)

of superconducting 2H-NbSe2, at 300 mK and in a magnetic field, up to 5 T, applied parallel to the ab core11 . More recent STS mea- surements at ultra low temperatures have indicated that the sub

Wei, John Y.T.

405

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

406

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

E-Print Network (OSTI)

. 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 radiative time constant 16 Planetary wind speed 36 Trojan companions 17,18 Artificial planet-sized objects

Hillenbrand, Lynne

407

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

408

arXiv:1002.0679v1[cond-mat.mes-hall]3Feb2010 Theory of resonant photon drag in monolayer graphene  

E-Print Network (OSTI)

distribution in energy. The drag current essentially depends on the polarization of radiation and, in general, is not parallel to q. The perpendicular current component appears if the in-plain electric field is tilted towards. INTRODUCTION Though the theoretical study of two-dimensional car- bon has a long history [1],[2],[3],[4] only

Shepelyansky, Dima

409

arXiv:1406.2962v1[hep-ph]11Jun2014 Reduction of the proton radius discrepancy by 3  

E-Print Network (OSTI)

. On the one hand, it enters the QED calculations of atomic energy splittings (electronic and muonic [1 of the electric and magnetic Sachs form factors GE(Q2 ) and GM (Q2 ), respectively, that depend on the invariant approach was car- ried out by Hill and Paz [4]. In contrast to their analysis, we do not constrain

410

arXiv:0709.2871v1[astro-ph]18Sep2007 Photometric Redshift Requirements for Self-Calibration of Cluster Dark Energy  

E-Print Network (OSTI)

dark energy constrains by more than 10% for a survey with specifications similar to the South Pole-Calibration of Cluster Dark Energy Studies Marcos Lima1,2 and Wayne Hu2,3 1 Department of Physics, University of Chicago (Dated: September 18, 2007) The ability to constrain dark energy from the evolution of galaxy cluster

Hu, Wayne

411

The study of chemical reactions, absorption and extraction, using apparatuses with serpentine pie for pelliclizing-bubbling, XIV. Hydroperoxidation of 1,3-diisopropylbenzene with oxygen  

Science Journals Connector (OSTI)

Experimental results obtained by thermal hydroperoxidation of 1,3-diisopropylbenzene in the temperature region of 102105C, using a Vodnr-1 type apparatus with discontinuous operation are presented. Based on...

Jnos Vodnr; Sndor Bkssy; Jnos Farkas

1999-11-01T23:59:59.000Z

412

arXiv:0809.3239v4[cond-mat.other]4Nov2009 Discerning Incompressible and Compressible Phases of Cold Atoms in Optical Lattices  

E-Print Network (OSTI)

-body phases forms the basis of quantum condensed matter, quan- tum chemistry and elementary particle physics gaps arise in the pres- ence of (or as a result of) interactions to form many-body states that resist state including zero resistance in supercon- ductors or a dramatic rise in resistance in Mott insula

Scarola, Vito

413

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

414

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

415

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

416

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

417

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

418

arXiv:0705.3777v1[quant-ph]25May2007 Role of interference in quantum state transfer through spin chains  

E-Print Network (OSTI)

. In particular, spin chains can be used as transmission lines for quantum states without the need to have´eorique, IRSAMC, UMR 5152 du CNRS, Universit´e Paul Sabatier, 118, route de Narbonne, 31062 Toulouse, FRANCE We parallel quantum channels [6, 7]. In [8] it was shown that the transmission even through very long chains

Bruder, Christoph

419

arXiv:1104.2573v1[physics.ins-det]13Apr2011 A Monte Carlo simulation of the Sudbury Neutrino  

E-Print Network (OSTI)

, Ontario, Canada. The overburden of the experiment is 5890 meters-water-equivalent [2]. The solar neutrino Department of Physics, University of Alberta, Edmonton, Alberta, T6G 2R3, Canada 2 Center for Experimental, USA 3 Department of Physics, Queen's University, Kingston, Ontario K7L 3N6, Canada 4 Department

Waltham, Chris

420

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

E-Print Network (OSTI)

Astrophysics, University of Oslo, P.O. Box 1029, Blindern, N­0315 Oslo, Norway Abstract. Type-II solar spicules appear as long, thin, highly dynamic strands of field-tied matter that feed significant mass and energy to the corona and solar wind. A recent result is that they exhibit torsional Alfv´en waves in addition

Rutten, Rob

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421

The benefits of taking a big bank into a small woodland  

E-Print Network (OSTI)

$93 billion revenue · bigger than GDP of Vietnam, Bangladesh or Morocco $2.4 trillion assets · bigger to deliver a business project 100 Gave me the knowledge and resources to influence others 100 Helped me

422

After 2015: infectious diseases in a new era of health and development  

Science Journals Connector (OSTI)

...water and sanitation, climate change, energy, employment and the management of natural...interaction is a chance to improve the efficiency of both infectious and non-infectious...are Bolivia, the Dominican Republic, Egypt, Indonesia, Morocco and Peru [50...

2014-01-01T23:59:59.000Z

423

Crops for a Salinized World  

Science Journals Connector (OSTI)

...including Pakistan, India, Egypt, Tunisia, Morocco...tolerate salinity require energy and therefore might...for animals, but also renewable energy (biofuel and biodiesel...traditional raw materials for energy productionoil...

Jelte Rozema; Timothy Flowers

2008-12-05T23:59:59.000Z

424

HIRICH et al. Wastewater reuse in the Mediterranean region: Case  

E-Print Network (OSTI)

HIRICH et al. Wastewater reuse in the Mediterranean region: Case of Morocco Abdelaziz HIRICH expedient. The extended reuse of reclaimed (treated) wastewater could contribute considerably Water Resources Management (IWRM) approach, focusing on the component wastewater reuse for irrigation

Paris-Sud XI, Université de

425

Montana State University College of Arts and Architecture  

E-Print Network (OSTI)

and Architecture School of Architecture Outreach and Engagement 1976-Present 2004-2005 2005-2006 2005-Present 2007 Kukaiau Ranch: Architectural Stewardship Khumbu Climbing School Hyalite Pavilion Morocco: Sustainable

Maxwell, Bruce D.

426

PUBLICATIONS1 I. Publications in journals  

E-Print Network (OSTI)

in Phys.Rev. D84 (2011) 032007 e-Print: arXiv:1107.4272 [astro-ph.HE] 3. Discovery of High-energy GammaPUBLICATIONS1 I. Publications in journals 1. Constraining dark matter models from a combined Review Letters (2011) arXiv e-print (arXiv:1108.3546) 2. Constraints on dark matter models from a Fermi

California at Santa Cruz, University of

427

The analysis and conservation of the Belle footwear assemblage  

E-Print Network (OSTI)

: THE CULTURAL MILIEU OF FRANCE (1661-1684) . . France before Louis XIV (1614-1661) . . . . . . . . . , . . . . . . . . . . . . . . . . . . . . . . . . . . 2 Le Gran Seicle: Reforms and Abuses of Louis XIV . . . . . . . . . . . . . . . 4 The Court of Louis.... They also serve as silent reminders of the lives and skills of contemporary French craftsmen, in this case the cordwainer, or shoemaker. Soldiers and craftsmen of that time lived in a world dominated by the French monarch, Louis XIV. Louis was determined...

Randolph, Anthony G., Jr

2003-01-01T23:59:59.000Z

428

Remarks On A Nicolas Inequality  

E-Print Network (OSTI)

This submission has been withdrawn by arXiv admins because it contains inappropriate, fictitious text in the acknowledgments and the final reference.

B. A. Kupershmidt

2008-06-05T23:59:59.000Z

429

Breathing, Laughing, Sneezing, Coughing: Model and Control of an Anatomically Inspired, Physically-Based Human Torso Simulation  

E-Print Network (OSTI)

xiv Hand-tuned Cough. . . . . . . . . . . . . . . . . . . .in the abdominal wall during a cough, is unmatched. Anotherroles in generating the cough animation seen in Figure 7.1.

DiLorenzo, Paul Carmen

2008-01-01T23:59:59.000Z

430

Tropical Linear Spaces and Applications  

E-Print Network (OSTI)

arXiv:1112.1278. [HKT06] Paul Hacking, Sean Keel, and Jeniaof hyperplane arrange- ments (Hacking, Keel and Tevelev [

Rincon, Edgard Felipe

2012-01-01T23:59:59.000Z

431

Comment on "Quantum Time Crystals": a new paradigm or just another proposal of perpetuum mobile?  

E-Print Network (OSTI)

A Comment on Frank Wilczek's paper "Quantum Time Crystals" (Phys. Rev. Lett. 109, 160401 (2012); arXiv:1202.2539).

Patrick Bruno

2012-10-15T23:59:59.000Z

432

London on the Thames: a Study of the Natural Conditions that Influenced the Birth and Growth of a Great City  

Science Journals Connector (OSTI)

... Political Science: Geographical Studies, No. 3.) Pp. xiv + 189. (London: Sifton, Praed and Co., Ltd., 1923.) 7s. 6d. net.

1924-05-31T23:59:59.000Z

433

updated 11/08 Publication List  

E-Print Network (OSTI)

generated on 11/21/08. Does not include early papers, and some astrophysics and cosmic ray papersXiv:0801.4589 [hep-ex

Learned, John

434

accelerated radiative transfer: Topics by E-print Network  

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

Dominated Outflows Astrophysics (arXiv) Summary: Plasma outflows from gamma-ray bursts (GRB), pulsar winds, relativistic jets, and ultra-intense laser targets radiate...

435

adenovectors induce functional: Topics by E-print Network  

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Luminosity Functions Induced by Relativistic Beaming on Statistics of Cosmological Gamma-Ray Bursts Astrophysics (arXiv) Summary: We study the effects of the beaming-induced...

436

E-Print Network 3.0 - angular correlations observed Sample Search...  

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observed Search Powered by Explorit Topic List Advanced Search Sample search results for: angular correlations observed Page: << < 1 2 3 4 5 > >> 1 arXiv:astroph0411130...

437

Definability in Physics  

E-Print Network (OSTI)

This paper has been withdrawn because the content has been substantially improved in a later paper, arXiv:0806.1165.

David J. BenDaniel

2006-06-26T23:59:59.000Z

438

Electroweak physics and physics beyond the Standard Model  

E-Print Network (OSTI)

We summarize the recent results on electroweak physics and physics beyond the Standard Model that have been presented at the XIV International Workshop on Deep Inelastic Scattering 2006.

L. Bellagamba; E. Sauvan; H. Spiesberger

2006-07-25T23:59:59.000Z

439

E-Print Network 3.0 - anestesia regional experiencia Sample Search...  

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Source: Sen, Pradeep - Electrical and Computer Engineering Department, University of New Mexico Collection: Engineering 77 1426 -XIV Encuentro de Latinoamericanistas Espaoles...

440

7. Twisted_inverse_image.pdf - Department of Mathematics, Purdue ...  

E-Print Network (OSTI)

Feb 20, 2009 ... Suresh Nayak extended Nagata's theorem, and hence the twisted inverse image, to essentially finite-type separated maps [arXiv:0809.1201].

2009-02-22T23:59:59.000Z

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441

Microsoft Word - WFO Boilerplate 1 Non-Federal Sponsor using...  

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PATENT AND COPYRIGHT INFRINGEMENT ARTICLE XIV PATENT RIGHTS - USE OF FACILITIES (CLASS WAIVER) ARTICLE XV RIGHTS IN TECHNICAL DATA - USE OF FACILITY ARTICLE XVI ASSIGNMENT...

442

Andrei Gabrielov Homepage  

E-Print Network (OSTI)

Sep 5, 2014 ... arXiv:0904.1714, April 2009. PDF. A. Gabrielov. Asymmetric Abelian Avalanches and Sandpiles. Preprint 93-65, MSI, Cornell Univ., 1993. PDF.

443

E-Print Network 3.0 - aenderung der aufbewahrungsgenehmigung...  

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BAUSENWEIN. - Aenderung des Peltiereffektes mit der Temperatur 1'ariation de l'effet Peltier avec la... regarde la discussion comme close. ----- ANNALEN DER PHYSIK ; T. XIV, n...

444

A review of "The Performance of Male Nobility in Moliere's Comedies-Ballets: Staging the Courtier" by Gretchen Elizabeth Smith  

E-Print Network (OSTI)

?dies-ballets, beginning with Les F?cheux of 1661. The performance took place at the notorious festival held in Louis XIV?s honor at Nicolas Fouquet?s lavish chateau, Vaux-le-Vicomte. Fouquet?s impolitic display of wealth and cultural capital, reflecting his per- sonal...?dies-ballets, beginning with Les F?cheux of 1661. The performance took place at the notorious festival held in Louis XIV?s honor at Nicolas Fouquet?s lavish chateau, Vaux-le-Vicomte. Fouquet?s impolitic display of wealth and cultural capital, reflecting his per- sonal...

Smith, Jay M.

2007-01-01T23:59:59.000Z

445

E-Print Network 3.0 - asociados al bienestar Sample Search Results  

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Powered by Explorit Topic List Advanced Search Sample search results for: asociados al bienestar Page: << < 1 2 3 4 5 > >> 1 2932 -XIV Encuentro de Latinoamericanistas...

446

Howes et al. Reply  

E-Print Network (OSTI)

Howes et al. Reply to Comment on "Kinetic Simulations of Magnetized Turbulence in Astrophysical Plasmas" arXiv:0711.4355

G. G. Howes; S. C. Cowley; W. Dorland; G. W. Hammett; E. Quataert; A. A. Schekochihin; T. Tatsuno

2008-12-12T23:59:59.000Z

447

amino acid conjugates: Topics by E-print Network  

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the measured distributions. Guang Wu; Shaomin Yan 71 Amino acid classes and the protein folding problem Condensed Matter (arXiv) Summary: We present and implement a...

448

aluminum corrosion study: Topics by E-print Network  

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background in low background experiments HEP - Experiment (arXiv) Summary: Neutrinoless double beta decay would be a key to understanding the nature of neutrino masses. The next...

449

RAPID/Roadmap/8-CA-a | Open Energy Information  

Open Energy Info (EERE)

the California Public Utilities Commission (CPUC) before constructing new transmission lines. Section XIV(b) of General Order 131-D clarifies that regulation of transmission line...

450

The Grillakis-Machedon-Margetis Second order corrections to mean field evolution for weakly interacting Bosons in the case of 3-body interactions  

E-Print Network (OSTI)

This note shows that, with a little modification, the results in arXiv:0904.0158 hold in the 3-body interactions case.

Xuwen Chen

2009-11-21T23:59:59.000Z

451

Microsoft Word - M096 Standard1 Revision.DOC  

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to an earlier estimate, provide reconciliation between estimates. (xiii) Basis of escalation. Page 4 of 9 (xiv) Subcontractor cost estimates, traceable to the WTP cost estimate...

452

E-Print Network 3.0 - accurate quark ckm Sample Search Results  

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Washington University in St. Louis Collection: Physics 11 arXiv:hepph0112008 B Phenomenology Summary: A charged current decay diagram for strange quark decay is shown in...

453

E-Print Network 3.0 - advanced hadron facility Sample Search...  

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Fizyki, Uniwersytet Jagiellonski Collection: Physics 20 arXiv:hepph0112008 B Phenomenology Summary: , facilities for b quark studies, neutral B meson mixing, rare b decays,...

454

MAURO NACINOVICH [1] C. Denson Hill and Mauro Nacinovich. Non completely solvable systems of  

E-Print Network (OSTI)

MAURO NACINOVICH References [1] C. Denson Hill and Mauro Nacinovich. Non completely solvable systems of complex first order pde's. arXiv:1111.1502v2 [math.AP], 2012. [2] Mauro Nacinovich and Egmont, Costantino Medori, and Mauro Nacinovich. Reductive com- pact homogeneous CR manifolds. arXiv:1106.2779v1

Nacinovich, Mauro

455

An action with positive kinetic energy term for general relativity  

E-Print Network (OSTI)

At first, we state some results in arXiv: 0707.2639, and then, using a positive kinetic energy coordinate condition given by arXiv: 0707.2639, we present an action with positive kinetic energy term for general relativity. Based on this action, the corresponding theory of canonical quantization is discussed.

T. Mei

2007-11-02T23:59:59.000Z

456

What Maudlin replied to  

E-Print Network (OSTI)

A recent post by Tim Maudlin to this archive (arXiv:1408.1828) was entitled "Reply to Werner". However, it was not clear to what text this was supposed to be a reply. Here I briefly provide this context, and show that Maudlin's post is as ill-conceived as the original paper (arXiv:1408.1826).

R. F. Werner

2014-11-08T23:59:59.000Z

457

Comment on "Spin-rotation coupling in non-exponential decay of hydrogenlike heavy ions" by G. Lambiase et al  

E-Print Network (OSTI)

I note that the explanation of a recently posted paper by Lambiase et al. [arXiv:0811.2302] for the oscillations in the electron capture decay rate, reported by Litvinov et al.[arXiv:0801.2079], requires the cancellation of a difference by eleven orders of magnitude for the two independent measurements. Such a cancellation is (impossible)^2.

Thomas Faestermann

2009-07-09T23:59:59.000Z

458

Effective Models and Extension of Torsors Over a Discrete Valuation Ring of Unequal Characteristic  

Science Journals Connector (OSTI)

......preprint arXiv:math/ 0601639v1. 20 Saidi M. Torsors under finite and flat group...Zeitschrift (2003) 245(4):695-710. 21 Saidi M. On the existence of a torsor structure...preprint arXiv:Math/0403389v1. 22 Saidi M. On the degeneration of etale and -torsors......

Dajano Tossici

2008-01-01T23:59:59.000Z

459

Measurement of the cross section and angular correlations for associated production of a Z boson with b hadrons in pp collisions at s? = 7 TeV  

E-Print Network (OSTI)

corrections to Zbb production with massive bottom quarks at the Fermilab Tevatron, Phys. Rev. D 78 (2008) 074014 [arXiv:0806.0808] [INSPIRE]. [13] F. Febres Cordero, L. Reina and D. Wackeroth, W- and Z-boson production with a massive bottom-quark pair... at the Large Hadron Collider, Phys. Rev. D 80 (2009) 034015 [arXiv:0906.1923] [INSPIRE]. [14] R. Frederix et al., W and Z/?? boson production in association with a bottom-antibottom pair, JHEP 09 (2011) 061 [arXiv:1106.6019] [INSPIRE]. [15] S. Frixione and B...

Baringer, Philip S.; Bean, Alice; Benelli, Gabriele; Kenney, R. P. III; Murray, Michael J.; Noonan, Danny; Sanders, Stephen J.; Stringer, Robert W.; Wood, Jeffrey Scott; Chatrchyan, S.; Khachatryan, V.; Sirunyan, A. M.; Tumasyan, A.; Adam, W.

2013-12-06T23:59:59.000Z

460

arXiv:1109.6328v2[astro-ph.CO]18Jun2012 Mon. Not. R. Astron. Soc. 000, 114 (2012) Printed 19 June 2012 (MN LATEX style file v2.2)  

E-Print Network (OSTI)

for Astrophysics & Supercomputing, Swinburne University of Technology, P.O. Box 218, Hawthorn, VIC 3122, Australia, Giessenbachstra?e, D-85748 Garching, Germany 14Key Laboratory for Research in Galaxies and Cosmology, Shanghai. The differences between the two inhibit a clean comparison between analyses and leave open the possibility that

Skibba, Ramin A.

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461

arXiv:1007.0777v3[nucl-ex]8Jul2010 Study of the p p reaction with the Crystal Ball detector at the Mainz Microtron  

E-Print Network (OSTI)

, T. Rostomyan9 , S. Schumann4 , M. H. Sikora10 , D. I. Sober17 , A. Starostin2 , I. M. Suarez2 , I of Basel, Switzerland I. INTRODUCTION The N family of nucleon resonances has many well established members

Krusche, Bernd

462

arXiv:1211.1407v1[gr-qc]6Nov2012 November 8, 2012 1:7 WSPC -Proceedings Trim Size: 9.75in x 6.5in icmp2012  

E-Print Network (OSTI)

, it is a symmetric (0, 2) tensor Tµ which satisfies the conservation law µ Tµ = 0. (1) Without gravitation Hamiltonian term which arises from Hamilton-Jacobi analysis of the gravitation action. The reference sur- face Suppose tµ is a constant future-directed timelike unit vector in R3,1 . By con- servation law (1), Tµtµ

Wang, Mu-Tao

463

arXiv:1005.1592v1[astro-ph.EP]10May2010 Astronomy & Astrophysics manuscript no. aa-comet-w3-revised-2 c ESO 2010  

E-Print Network (OSTI)

to comets observed closer to the Sun. The CO to H2O production rate ratio exceeds 220%. The dust to gas/Schwassmann-Wachmann 1, where CO, CO+ , and CN were detected at 6 AU from the Sun, and C/1995 O1 (Hale-Bopp), whose

Naylor, David A.

464

arXiv:0712.0277v1[astro-ph]3Dec2007 Mon. Not. R. Astron. Soc. 000, 000000 (0000) Printed 3 December 2007 (MN LATEX style file v2.2)  

E-Print Network (OSTI)

0HA 2RIKEN Cosmic Radiation Lab, 2-1 Hirosawa, Wakoshi, Saitama 351-0198, Japan 3 December 2007 December 2007 (MN LATEX style file v2.2) The effect of radiation pressure on dusty absorbing gas around AGN ABSTRACT Many Active Galactic Nuclei (AGN) are surrounded by gas which absorbs the radiation pro- duced

Gandhi, Poshak

465

Engineering Aspects of Magnetohydrodynamics. Proceedings of the third annual symposium (Rochester, N.Y.), March 1962. Norman W. Mather and George W. Sutton, Eds. Gordon and Breach, New York, 1964. xiv + 675 pp. Illus. $34.50  

Science Journals Connector (OSTI)

...actually misleading. The maps, diagrams, and bibliographies are helpful...as-pects of magnetohydrodynamics (MHD) held at the University of...an ac-count of the original MHD generator experiments undertaken...Corporation in 1938. In the field of MHD power generation, the paper...

William D. Jackson

1965-07-02T23:59:59.000Z

466

arXiv:1409.0674v1[astro-ph.GA]2Sep2014 Mon. Not. R. Astron. Soc. 000, 116 (2014) Printed 3 September 2014 (MN LATEX style file v2.2)  

E-Print Network (OSTI)

´isica, ´Optica y Electr´onica (INAOE), 72000 Puebla, M´exico ABSTRACT We present mid-infrared (MIR) imaging

467

Radiation Biology. Alison P. Casarett. Prepared under the auspices of the American Institute of Biological Sciences for the U.S. Atomic Energy Commission. Prentice Hall, Englewood Cliffs, N.J., 1968. xiv + 368 pp., illus. $9.25  

Science Journals Connector (OSTI)

...illus., + 83 plates. $6.95. Desalination. Water for the World's Future. Roy...x + 246 pp., illus. $7.50. Economics of Dissent. Ben B. Seligman. Quadrangle...1968. xviii + 430 pp. $10. The Economics of Technological Change. Edwin Mansfield...

L. J. Tolmach

1969-02-07T23:59:59.000Z

468

arXiv:physics/0306019v12Jun2003 Computing in High Energy and Nuclear Physics, La Jolla, California, March 24 -28, 2003 1 Java Physics Generator and Analysis Modules  

E-Print Network (OSTI)

and Asian JLC detector simulation modules have been written for performing comparisons to the American LC For- tran77, and new C++ and Fortran95 software mod- ules for event generation, detector simulation 3 and 4 list the generator and detector simulation modules, respectively. A sim- ple comparison

469

arXiv:0812.2609v2[astro-ph]20Dec2008 Mon. Not. R. Astron. Soc. 000, 000000 (0000) Printed 8 August 2011 (MN LATEX style file v2.2)  

E-Print Network (OSTI)

emitters, presumably due to a low opacity in dust at these early epochs. The model involves zero or even and RR 2003, Balland et al 2003, Xu et al 2003, Lagache et al 2003). Dole et al (2006) used stacking

Rowan-Robinson, Michael

470

The Free Will Theorem and the Flash Ontology implicitly assume the Before-Before Experiment and thereby imply free will. Comment on a note by Nicolas Gisin in arXiv:1002.1392v1  

E-Print Network (OSTI)

It is argued that both the "Free Will Theorem" (FWT) and the "relativistic GRW model with Flash Ontology" (rGRWf) hiddenly assume the result of the before-before experiment, and for this reason both FWT and rGRWf imply free will in the world outside free experimenters.

Antoine Suarez

2010-02-13T23:59:59.000Z

471

arXiv:1106.5685v2[hep-ex]28Dec2011 FERMILAB-PUB-11-304-E Dual baseline search for muon neutrino disappearance at 0.5 eV2  

E-Print Network (OSTI)

-Aunion,3 C. E. Anderson,29 A. O. Bazarko,22 S. J. Brice,9 B. C. Brown,9 L. Bugel,20 J. Cao,21 J. Catala

Sheldon, Nathan D.

472

arXiv:1107.5059v1[astro-ph.CO]25Jul2011 Mon. Not. R. Astron. Soc. 000, 120 (2011) Printed 27 July 2011 (MN LATEX style file v2.2)  

E-Print Network (OSTI)

2011 (MN LATEX style file v2.2) The ATLAS3D Project­ VIII: Modelling the Formation and Evolution Coordinating Facility, European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching, Germany 11 reproduce the fraction of fast and slow rotators as a function of magnitude in the ATLAS3D survey, assuming

Bureau, Martin

473

arXiv:1005.3649v2[astro-ph.CO]21May2010 Mon. Not. R. Astron. Soc. 000, 114 (200X) Printed 24 May 2010 (MN LATEX style file v2.2)  

E-Print Network (OSTI)

2010 (MN LATEX style file v2.2) Wide-angle tail galaxies in ATLAS Minnie Y. Mao1,2,3 , Rob Sharp2 , D National Facility, PO Box 76, Epping, NSW, 1710, Australia 4National Centre for Radio Astrophysics, Tata) radio sources identified in the ATLAS 1.4 GHz radio survey, and new spec- troscopic redshifts for four

Norris, Ray

474

arXiv:1208.2722v1[astro-ph.CO]13Aug2012 Mon. Not. R. Astron. Soc. 000, 117 (200X) Printed 15 August 2012 (MN LATEX style file v2.2)  

E-Print Network (OSTI)

, 1710, Australia 3CSIRO Australia Telescope National Facility, PO Box 76, Epping, NSW, 1710, Australia 4 Telescope Large Area Survey (ATLAS) has surveyed seven square degrees of sky around the Chandra Deep Field South (CDFS) and the European Large Area ISO Survey - South 1 (ELAIS- S1) fields at 1.4 GHz. ATLAS aims

Norris, Ray

475

arXiv:1209.0767v1[astro-ph.CO]4Sep2012 Mon. Not. R. Astron. Soc. 000, 000000 (2012) Printed 6 September 2012 (MN LATEX style file v2.2)  

E-Print Network (OSTI)

: abundances ­ Physical data and processing: gravitational lensing 1 INTRODUCTION Strong gravitational lensing- Based on data from the X-shooter GTO observations collected at the Eu- ropean Southern Observatory VLT

Paris-Sud XI, Université de

476

arXiv:1209.0775v2[astro-ph.CO]10Sep2012 Mon. Not. R. Astron. Soc. 000, 000000 (2012) Printed 11 September 2012 (MN LATEX style file v2.2)  

E-Print Network (OSTI)

-redshift ­ galaxies: evolution ­ galaxies: abundances ­ Physical data and processing: gravitational lensing 1 the X-shooter GTO observations collected at the European Southern Observatory VLT/Kuyuen telescope

Paris-Sud XI, Université de

477

arXiv:0911.2715v1[astro-ph.SR]13Nov2009 APS/123-QED An association between anisotropic plasma heating and instabilities in the solar wind  

E-Print Network (OSTI)

the firehose instability threshold. The increase in Tp is consistent with cyclotron-resonant heating]. Ion heating consistent with an Alfv´en-cyclotron mechanism is also directly observed in interplanetary heating and instabilities in the solar wind J. C. Kasper and B. A. Maruca Harvard-Smithsonian Center

California at Berkeley, University of

478

arXiv:1011.2930v1[cond-mat.supr-con]12Nov2010 Spin waves in the (, 0) magnetically ordered iron chalcogenide Fe1.05Te  

E-Print Network (OSTI)

.D. Christianson,5 Takeshi Egami,1, 5 Nanlin Wang,2 Jiangping Hu,3, 2 and Pengcheng Dai1, 5, 2, 1 The University

Hu, Jiangping

479

arXiv:1006.1627v1[astro-ph.SR]8Jun2010 Discovery of a Low-Mass Companion to a Metal-Rich F Star with the  

E-Print Network (OSTI)

, Jian Liu1, Pengcheng Guo1, Stephen R. Kane1,8, Julian C. van Eyken1,8, Nathan M. De Lee1, Justin R

Barnes, Rory

480

arXiv:0712.2439v1[hep-th]14Dec2007 BU 07-08, MIT-CTP 3910, Isaac Newton Inst. N107074 Electron fractionalization for two-dimensional Dirac fermions  

E-Print Network (OSTI)

gauge field. Charge fractionalization occurs whenever the Higgs field either sup- ports vortices as a function of a parameter in the Dirac Hamiltonian that breaks the spectral energy-reflection symmetry notion of a fractional charge demands that the fermion number is a good quantum number. Second, the Bose

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481

arXiv:0706.1732v2[hep-ph]11Jul2007 NUHEP-TH/07-06 GeV Seesaw, Accidentally Small Neutrino Masses, and Higgs Decays to Neutrinos  

E-Print Network (OSTI)

mixing and will provide important input for interpretation of next-generation neutrinoless double beta decay experiments. Measurement of the mass hierarchy is important input to the search for leptonic CP

482

arXiv:1009.4437v1[cond-mat.supr-con]22Sep2010 Pressure effects in PrT2B2C (T = Co, Ni, Pt): Applied and chemical pressure  

E-Print Network (OSTI)

Ciencias B´asicas, Universidad Ju´arez Aut´onoma de Tabasco. Cunduacan, Tabasco. 86690 A. Postal 24. M

Paris-Sud XI, Université de

483

E-Print Network 3.0 - ap star hd Sample Search Results  

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search results for: ap star hd Page: << < 1 2 3 4 5 > >> 1 arXiv:astroph0405348 Astronomy & Astrophysics manuscript no. OstarsCat October 21, 2004 Summary: of the field O...

484

E-Print Network 3.0 - astronomical infrared spectroscopy Sample...  

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T-ReCS ... Source: De Buizer, James Michael - Stratospheric Observatory for Infrared Astronomy, NASA Ames Research Center Collection: Physics 2 arXiv:astro-ph0402572v124Feb2004...

485

E-Print Network 3.0 - antinucleon reactions Sample Search Results  

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10 arXiv:astro-ph9912303v24Apr2000 Vacuum discharge as a possible source of gamma-ray bursts Summary: -positron pair creations in QED with strong electromagnetic fields...

486

E-Print Network 3.0 - apt project ed Sample Search Results  

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and Information Sciences 11 arXiv:astro-ph9711245v120Nov1997 To be published in "Gamma-Ray Bursts, 4th Huntsville Symposium", 1998, ed. Summary: . The APT is complementary to...

487

E-Print Network 3.0 - aperture grb observatory Sample Search...  

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Collection: Mathematics 8 arXiv:astro-ph9711245v120Nov1997 To be published in "Gamma-Ray Bursts, 4th Huntsville Symposium", 1998, ed. Summary: aperture to the APT, but has a...

488

E-Print Network 3.0 - aist laser-compton gamma-ray Sample Search...  

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laser-compton gamma-ray Search Powered by Explorit Topic List Advanced Search Sample search results for: aist laser-compton gamma-ray Page: << < 1 2 3 4 5 > >> 1 arXiv:physics...

489

E-Print Network 3.0 - antiproton nucleon annihilations Sample...  

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32 arXiv:astro-ph9912303v24Apr2000 Vacuum discharge as a possible source of gamma-ray bursts Summary: will then annihilate with the nucleons at the ambient medium through...

490

E-Print Network 3.0 - antinucleon beams Sample Search Results  

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11 arXiv:astro-ph9912303v24Apr2000 Vacuum discharge as a possible source of gamma-ray bursts Summary: reduces the energy released in -rays alone to be 6 1052 erg 8 due...

491

Comment on 'Discussions on common errors in analyzing sea level accelerations, solar trends and global warming'  

E-Print Network (OSTI)

Comment on Scafetta, Nicola. 'Discussion on Common Errors in Analyzing Sea Level Accelerations, Solar Trends and Global Warming.' arXiv:1305.2812 (May 13, 2013a). doi:10.5194/prp-1-37-2013.

Benestad, R E

2013-01-01T23:59:59.000Z

492

Nuclear astrophysics studies with ultra-peripheral heavy-ion collisions  

E-Print Network (OSTI)

I describe in very simple terms the theoretical tools needed to investigate ultra-peripheral nuclear reactions for nuclear astrophysics purposes. For a more detailed account, see arXiv:0908.4307.

C. A. Bertulani

2009-12-17T23:59:59.000Z

493

Stability in the Stefan problem with surface tension (II)  

E-Print Network (OSTI)

This paper has been withdrawn by the authors due to an error in the proof of Lemma 3.9. The correct proof of global stability is given in arXiv:1101.5177

Mahir Hadzic; Yan Guo

2012-12-12T23:59:59.000Z

494

A review of "Blasphemy: Impious Speech in the West from the Seventeenth to the Nineteenth Century." by Alain Cabantous  

E-Print Network (OSTI)

REVIEWS 133 Alain Cabantous. Blasphemy: Impious Speech in the West from the Seventeenth to the Nineteenth Century. Trans. Eric Rauth. New York: Columbia University Press, 2002. xiv + 288 pp. $29.50. Re- view by MELISSA MOHR, STANFORD UNIVERSITY...

Melissa Mohr

2002-01-01T23:59:59.000Z

495

THE CALCULATION OF AUTOIONIZATION POSITIONS AND WIDTHS WITH APPLICATIONS TO PENNING IONIZATION REACTIONS  

E-Print Network (OSTI)

Jn relative maximum (cf4 Figure :,:lI)4 In. :3 ? rev.iou3the He(2 S)+;1.2 calculations {Cf4 Figure XIV. l Interaction

Isaacson, Alan D.

2011-01-01T23:59:59.000Z

496

Microsoft Word - WFO Boilerplate 2 Non-Federal Sponsor Using...  

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

the possession of the Sponsor pertaining to such claim. ARTICLE XIV. PATENT RIGHTS (CLASS WAIVER DECLINED OR DENIED) 1. The following definitions shall be used for this Article. A....

497

Books Received  

Science Journals Connector (OSTI)

...Nuclear Science and Technology. Vol. 8. Ernest J. Henley and Jeffery Lewins, Eds. Academic Press, New York, 1975. xiv, 350...Solid State Physicists. S. Doniach and E. H. Sondheimer. Benjamin, Reading, Mass., 1975. xx, 266 pp. Cloth, $19; paper...

1975-06-13T23:59:59.000Z

498

alternating magnetic fields: Topics by E-print Network  

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

attention on recent progresses. Massimo Giovannini 2006-12-14 32 Cosmological Magnetic Fields vs. CMB Astrophysics (arXiv) Summary: I present a short review of the effects of a...

499

A review of "Defining the Jacobean Church: the Politics of Religious Controversy, 1603-1625." by Charles W.A. Prior  

E-Print Network (OSTI)

REVIEWS 151 Charles W.A. Prior. Defining the Jacobean Church: the Politics of Religious Controversy, 1603-1625. Cambridge: Cambridge University Press, 2005. xiv + 294 pp. $85.00. Review by GRAHAM PARRY, UNIVERSITY OF YORK. Defining the Jacobean...

Parry, Graham

2006-01-01T23:59:59.000Z

500

A Review of "Archipelagic English: Literature, History and Politics, 1603-1707" by John Kerrigan  

E-Print Network (OSTI)

of Green is a moving, useful, pleasurable read. John Kerrigan. Archipelagic English: Literature, History and Politics 1603- 1707. Oxford: Oxford University Press, 2008. xiv + 599 pp. $49.95. Review by Eugene D. Hill, mount holyoke college. As the title...

Hill, Eugene D.

2009-01-01T23:59:59.000Z