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1.
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Les Houches 2011: Physics at TeV Colliders New Physics Working Group Report
/ Brooijmans, G. (Columbia U.) ; Gripaios, B. (Cambridge U.) ; Moortgat, F. (Zurich, ETH) ; Santiago, J. (CAFPE, Granada ; Granada U., Theor. Phys. Astrophys.) ; Skands, P. (CERN) ; Albornoz Vásquez, D. (Paris, Inst. Astrophys.) ; Allanach, B.C. (Cambridge U., DAMTP) ; Alloul, A. (Strasbourg, IPHC ; Strasbourg, IReS) ; Arbey, A. (CERN ; Lyon, IPN ; Lyon Observ.) ; Azatov, A. (INFN, Rome ; Rome U.) et al.
We present the activities of the 'New Physics' working group for the 'Physics at TeV Colliders' workshop (Les Houches, France, 30 May-17 June, 2011). Our report includes new agreements on formats for interfaces between computational tools, new tool developments, important signatures for searches at the LHC, recommendations for presentation of LHC search results, as well as additional phenomenological studies..
arXiv:1203.1488; FERMILAB-CONF-12-924-T.-
2012 - 243 p.
- Published in : , pp. 221-463
Fermilab Library: PDF; Fulltext: PDF; External link: Fermilab Library
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2.
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Nonthermal production of WIMPs, cosmic e± excesses, and γ rays from the Galactic Center
/ Bi, Xiao-Jun (Beijing, Inst. High Energy Phys. ; Peking U.) ; Brandenberger, Robert (McGill U. ; Beijing, Inst. High Energy Phys. ; TPCSF, Beijing ; Beijing, KITPC ; CERN) ; Gondolo, Paolo (Utah U. ; Beijing, KITPC) ; Li, Tian-jun (Beijing, Inst. Theor. Phys. ; Texas A-M ; Beijing, KITPC) ; Yuan, Qiang (Beijing, Inst. High Energy Phys.) ; Zhang, Xin-min (Beijing, Inst. High Energy Phys. ; TPCSF, Beijing ; Beijing, KITPC)
In this paper we propose a dark matter model and study aspects of its phenomenology. Our model is based on a new dark matter sector with a U(1)′ gauge symmetry plus a discrete symmetry added to the standard model of particle physics. [...]
arXiv:0905.1253; CERN-PH-TH-2009-082.-
2009 - 23 p.
- Published in : Phys. Rev. D 80 (2009) 103502
APS Published version, local copy: PDF; Fulltext: PDF; External link: Preprint
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3.
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The case for a directional dark matter detector and the status of current experimental efforts
/ Ahlen, S ; Afshordi, N ; Battat, J B R ; Billard, J ; Bozorgnia, N ; Burgos, S ; Caldwell, T ; Carmona, J M ; Cebrián, S ; Colas, P et al.
We present the case for a dark matter detector with directional sensitivity. This document was developed at the 2009 CYGNUS workshop on directional dark matter detection, and contains contributions from theorists and experimental groups in the field. [...]
arXiv:0911.0323.-
2010 - 48 p.
- Published in : Int. J. Mod. Phys. A 25 (2010) 1-51
External link: Preprint
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4.
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Ultra-cold WIMPs: relics of non-standard pre-BBN cosmologies
/ Gelmini, Graciela B. (UCLA) ; Gondolo, Paolo (Utah U.)
Weakly interacting massive particles (WIMPs) constitute one of very few probes of cosmology before big bang nucleosynthesis (BBN). We point out that in scenarios in which the Universe evolves in a non-standard manner during and after WIMP kinetic decoupling, the horizon mass scale at decoupling can be smaller and the dark matter WIMPs can be colder than in standard cosmology. [...]
arXiv:0803.2349; CERN-PH-TH-2008-052; CERN-PH-TH-2008-052.-
2008 - 6 p.
- Published in : JCAP 0810 (2008) 002
Fulltext: PDF; External link: Fulltext
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5.
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AGAPE, an experiment to detect MACHO's in the direction of the andromeda galaxy
/ Ansari, R ; Aurière, M ; Baillon, Paul ; Bouquet, A ; Coupinot, G ; Ghesquière, C ; Giraud-Héraud, Yannick ; Gondolo, P ; Hecquet, J ; Kaplan, J et al.
1994
In : 17th Texas Symposium on Relativistic Astrophysics and Cosmology, Munich, Germany, 11 - 16 Dec 1994, pp.608-611
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6.
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7.
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Variable stars towards the bulge of M31: the AGAPE catalogue
/ Ansari, R. (Orsay, LAL) ; Auriere, M. (Midi-Pyrenees Observ., Tarbes) ; Baillon, P. (CERN) ; Bouquet, A. (College de France) ; Coupinot, G. (Midi-Pyrenees Observ., Tarbes) ; Coutures, Ch. (DAPNIA, Saclay) ; Ghesquiere, C. (College de France) ; Giraud-Heraud, Y. (College de France) ; Gillieron, D. (Midi-Pyrenees Observ., Tarbes) ; Gondolo, P. (Utah U.) et al.
We present the AGAPE astrometric and photometric catalogue of 1579 variable stars in a 14'x10' field centred on M31. This work is the first survey devoted to variable stars in the bulge of M31. [...]
astro-ph/0405402.-
2004
- Published in : Astron. Astrophys. 421 (2004) 509-518
Access to fulltext document: PDF; External link: AAEJA
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8.
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Pixel Lensing
/ Ansari, R ; Aurière, M ; Baillon, Paul ; Bouquet, A ; Coupinot, G ; Coutures, C ; Ghesquière, C ; Giraud-Héraud, Yannick ; Gondolo, P ; Hecquet, J et al.
PCC-97-55-CONF.
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1997. - 107 p.
IN2P3 Publications database
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9.
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AgapeZ1 : a Large Amplification Microlensing Event or an Odd Variable Star Towards the Inner Bulge of M31
/ Ansari, R. (Orsay, LAL) ; Auriere, M. (Pic du Midi Observ.) ; Baillon, P. (CERN) ; Bouquet, A. (College de France) ; Coupinot, G. (Pic du Midi Observ.) ; Coutures, Ch. (DAPNIA, Saclay) ; Ghesquiere, C. (College de France) ; Giraud-Heraud, Y. (College de France) ; Gondolo, P. (Munich, Max Planck Inst.) ; Hecquet, J. (Midi-Pyrenees Observ.) et al.
AgapeZ1 is the brightest and the shortest duration microlensing candidate event found in the Agape data. It occured only 42" from the center of M31. [...]
astro-ph/9812334; PCC-98-23; PCC-98-23.-
Paris : Collège de France. Lab. Phys. Corpusc. Cosmol., 1999 - 4 p.
- Published in : Astron. Astrophys. 344 (1999) L49
Access to fulltext document: PDF; External link: astro-ph/9812334 PDF
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10.
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AGAPEROS : Searches for microlensing in the LMC with the Pixel Method; 2, Selection of possible microlensing events
/ Melchior, A.L. (Queen Mary, U. of London ; College de France) ; Afonso, C (CEA, DSM, Saclay ; DAPNIA, Saclay) ; Ansari, R (Orsay, LAL) ; Aubourg, E. (CEA, DSM, Saclay ; DAPNIA, Saclay) ; Baillon, P. (CERN) ; Bareyre, P. (CEA, DSM, Saclay ; DAPNIA, Saclay) ; Bauer, F. (CEA, DSM, Saclay ; DAPNIA, Saclay) ; Beaulieu, J.-Ph. (Paris, Inst. Astrophys.) ; Bouquet, A. (College de France) ; Brehin, S. (CEA, DSM, Saclay ; DAPNIA, Saclay) et al.
We apply the pixel method of analysis (sometimes called ``pixel lensing'') to a small subset of the EROS-1 microlensing observations of the bar of the Large Magellanic Cloud (LMC). The pixel method is designed to find microlensing events of unresolved source stars and had heretofore been applied only to M31 where essentially all sources are unresolved. [...]
astro-ph/9804321.-
1998 - 14 p.
- Published in : Astron. Astrophys. 339 (1998) 658
Access to fulltext document: PDF; External link: astro-ph/9804321 PDF
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