Status of the EDELWEISS Experiment

被引:11
作者
Berge, L
Berkes, I
Chambon, B
Chapellier, M
Chardin, G
Charvin, P
De Jesus, M
Di Stefano, P
Drain, D
Dumoulin, L
Goldbach, C
Juillard, A
L'Hote, D
Marnieros, S
Miramonti, L
Mosca, L
Navick, XF
Nollez, G
Pari, P
Pastor, C
Pecourt, S
Tourbot, R
Yvon, D
机构
[1] Univ Paris 11, CNRS, IN2P3, Ctr Spectrometrie Nucl & Spectrometrie Masse, F-91405 Orsay, France
[2] Univ Lyon 1, CNRS, IN2P3, F-69622 Villeurbanne, France
[3] Inst Phys Nucl, F-69622 Villeurbanne, France
[4] Ctr Etud Saclay, CEA, DSM,DAPNIA, Serv Phys Particules, F-91191 Gif Sur Yvette, France
[5] CNRS, CEA, Lab Souterrain Modane, F-73500 Modane, France
[6] CNRS, INSU, Inst Astrophys Paris, F-75014 Paris, France
关键词
D O I
10.1016/S0920-5632(98)00390-9
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
The status of the EDELWEISS experiment (underground dark matter search with heat-ionisation bolometers) is reviewed. Auspicious results achieved with a prototype 70 g Ge heat-ionisation detector under a 2 V reverse bias tension are discussed. Based on gamma and neutron calibrations, a best-case rejection factor, over the 15-45 keV range, of 99.7% for gammas, with an acceptance of 94% for neutrons, is presented first. Some operational results of physical interest obtained under poor low radioactivity conditions follow. They include a raw event rate of around 30 events/day/kg/keV over the same energy range, and, after rejection of part of the background, lead to a conservative upper limit on the signal of approximately 1.6 events/day/kg/keV at a 90% confidence level. Performance degrading surface effects of the detector are speculated upon; and planned upgrades are summarized.
引用
收藏
页码:69 / 73
页数:5
相关论文
共 15 条
[1]  
[Anonymous], 1963, KGL DANSKE VIDENSKAB
[2]   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
[3]   The statistics of background rejection in direct detection experiments for dark matter. [J].
Gaitskell, RJ ;
Barnes, PD ;
DaSilva, A ;
Sadoulet, B ;
Shutt, T .
NUCLEAR PHYSICS B, 1996, :279-283
[4]   DETECTABILITY OF CERTAIN DARK-MATTER CANDIDATES [J].
GOODMAN, MW ;
WITTEN, E .
PHYSICAL REVIEW D, 1985, 31 (12) :3059-3063
[5]   Supersymmetric dark matter [J].
Jungman, G ;
Kamionkowski, M ;
Griest, K .
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 1996, 267 (5-6) :195-373
[6]  
LHOTE D, 1997, P 7 INT WORK LOW TEM, P240
[7]   CALORIMETRIC IONIZATION DETECTOR [J].
LUKE, PN ;
BEEMAN, J ;
GOULDING, FS ;
LABOV, SE ;
SILVER, EH .
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 1990, 289 (03) :406-409
[8]  
MARNIEROS S, 1997, P 7 INT WORKSH LOW T, P134
[9]  
Mosca L., 1996, Surveys in High Energy Physics, V9, P275, DOI 10.1080/01422419608223782
[10]   THERMAL DETECTORS AS X-RAY SPECTROMETERS [J].
MOSELEY, SH ;
MATHER, JC ;
MCCAMMON, D .
JOURNAL OF APPLIED PHYSICS, 1984, 56 (05) :1257-1262