Looking for SUSY with EDELWEISS-I and -II

被引:0
作者
Gerbier, G [1 ]
Benoît, A
Bergé, L
Broniatowski, A
Chabert, L
Chambon, B
Chardin, B
Chapellier, M
Charvin, P
De Jésus, M
Deschamps, H
Di Stefano, P
Drain, D
Dumoulin, L
Fiorucci, S
Gascon, J
Gerlic, E
Goldbach, C
Goyot, M
Gros, M
Hadjout, JP
Hervé, S
Juillard, A
de Lesquen, A
Mallet, J
Marnieros, S
Martineau, O
Mosca, L
Navick, XF
Nollez, G
Pari, P
Riccio, C
Sanglard, V
Schoeffel, L
Stern, M
Vagneron, L
机构
[1] Ctr Etud Nucl Saclay, CEA, DAPNIA, DSM, F-91191 Gif Sur Yvette, France
[2] CNRS, Ctr Rech Tres Basses Temp, SPM, Grenoble, France
[3] Univ Paris 11, CNRS, Ctr Spectrometrie Nucl & Spectrometrie Masse, Orsay, France
[4] CNRS, UCBL, Inst Phys Nucl Lyon, Lyon, France
[5] Ctr Etud Nucl Saclay, CEA, DRECAM, DSM, F-91191 Gif Sur Yvette, France
[6] CNRS, CEA, Lab Souterrain Modane, Modane, France
[7] CNRS, INSU, Inst Astrophys Paris, Paris, France
关键词
D O I
10.1134/1.1825523
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
The latest results obtained by the EDELWEISS WIMP (weakly interacting massive particles) direct detection experiment using three heat- and -ionization 320-g germanium bolometers are given. Presently the most sensitive WIMP direct detection experiment for WIMP mass >30 GeV, EDELWEISS-I is testing a first region of SUSY models compatible with accelerator constraints. The status and main characteristics of EDELWEISS-II, involving in a first stage 28 germanium bolometers and able to accommodate up to 120 detectors, are briefly presented, together with neutron background estimates. (C) 2004 MAIK "Nauka/Interperiodica".
引用
收藏
页码:2027 / 2031
页数:5
相关论文
共 25 条
[11]   Comparing interaction rate detectors for weakly interacting massive particles with annual modulation detectors [J].
Copi, CJ ;
Krauss, LM .
PHYSICAL REVIEW D, 2003, 67 (10)
[12]   Dark matter search with a low temperature sapphire bolometer [J].
deBellefon, A ;
Berkes, I ;
Bobin, C ;
Broszkiewicz, D ;
Chambon, B ;
Chaellier, M ;
Chardin, G ;
Charvin, P ;
Chazal, V ;
Coron, N ;
DeJesus, M ;
Drain, D ;
Dumoulin, L ;
GiraudHeraud, Y ;
Goldbach, C ;
Guerier, G ;
Hadjout, JP ;
Leblanc, J ;
Marchand, D ;
Massaq, M ;
Messous, Y ;
Navick, X ;
Nollez, G ;
Pari, P ;
Pastor, C ;
PerilloIsaac, MC ;
Prostakov, I ;
Yvon, D .
ASTROPARTICLE PHYSICS, 1996, 6 (01) :35-43
[13]   Background discrimination capabilities of a heat and ionization germanium cryogenic detector [J].
Di Stefano, P ;
Bergé, L ;
Chambon, B ;
Chapellier, M ;
Chaumont, J ;
Chardin, G ;
Charvin, P ;
De Jésus, M ;
Drain, D ;
Dumoulin, L ;
Forget, P ;
Garoche, P ;
Gascon, J ;
Goldbach, C ;
L'Hôte, D ;
Mallet, J ;
Mangin, J ;
Marnieros, S ;
Miramonti, L ;
Mosca, L ;
Navick, XF ;
Nollez, G ;
Pari, P ;
Pécourt, S ;
Simon, E ;
Stab, L ;
Torre, JP ;
Tourbot, R ;
Yvon, D .
ASTROPARTICLE PHYSICS, 2001, 14 (04) :329-337
[14]   Re-evaluation of the elastic scattering of supersymmetric dark matter [J].
Ellis, J ;
Ferstl, A ;
Olive, KA .
PHYSICS LETTERS B, 2000, 481 (2-4) :304-314
[15]  
Kim YG, 2002, J HIGH ENERGY PHYS
[16]  
KURYLOV A, HEPPH0307185
[17]   Review of mathematics, numerical factors, and corrections for dark matter experiments based on elastic nuclear recoil [J].
Lewin, JD ;
Smith, PF .
ASTROPARTICLE PHYSICS, 1996, 6 (01) :87-112
[18]   LOW-ENERGY X-RAY RESPONSE OF GE DETECTORS WITH AMORPHOUS-GE ENTRANCE CONTACTS [J].
LUKE, PN ;
ROSSINGTON, CS ;
WESELA, MF .
IEEE TRANSACTIONS ON NUCLEAR SCIENCE, 1994, 41 (04) :1074-1079
[19]  
LUKE PN, LBNL33980
[20]  
MARNIEROS S, 2003, IN PRESS NUCL INSTRU