Dark matter search with a low temperature sapphire bolometer

被引：46

作者：

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

机构：

[1] INST ASTROPHYS, CNRS, F-75014 PARIS, FRANCE

[2] COLL FRANCE, PHYS CORPUSCULAIRE LAB, F-75231 PARIS 05, FRANCE

[3] INST PHYS NUCL, F-69622 VILLEURBANNE, FRANCE

[4] UNIV LYON 1, IN2P3, CNRS, F-69622 VILLEURBANNE, FRANCE

[5] CEA, CTR ETUD SACLAY, DRECAM, SERV PHYS ETAT CONDENSE, F-91191 GIF SUR YVETTE, FRANCE

[6] CEA, CTR ETUD SACLAY, DAPNIA, SERV PARTICLE PHYS, F-91191 GIF SUR YVETTE, FRANCE

[7] CEA, CNRS, LAB SOUTERRAIN MODANE, F-73500 MODANE, FRANCE

[8] UNIV PARIS 11, IN2P3 CNRS, CTR SPECTROMETRIE NUCL & SPECTROMETRIE MASSE, F-91405 ORSAY, FRANCE

[9] UNIV PARIS 11, INST ASTROPHYS SPATIALE, F-91405 ORSAY, FRANCE

来源：

ASTROPARTICLE PHYSICS | 1996年 / 6卷 / 01期

关键词：

dark matter; WIMP; bolometer;

D O I：

10.1016/S0927-6505(96)00040-0

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A dark matter detection experiment using a low temperature 24 g sapphire bolometer is presented, The low radioactive background cryogenic facility, installed in a deep underground site, is described, as well as the low-noise read-out electronics and the data analysis, From the energy spectrum, measured down to 4 keV, exclusion plots are derived for WIMPs having coherent vector coupling or axial coupling to ordinary matter.

引用

页码：35 / 43

页数：9

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