CRESST cryogenic dark matter search

被引：3

作者：

Cozzini, C ^{[1
]}

Angloher, G

Bucci, C

von Feilitzsch, F

Frank, T

Hauff, D

Henry, S

Jagemann, T

Jochum, J

Kraus, H

Majorovits, B

Ninkovic, J

Petricca, F

Pröbst, F

Ramachers, Y

Rau, W

Razeti, M

Seidel, W

Stark, M

Stodolsky, L

Uchaikin, S

Wulandari, H

机构：

[1] Univ Oxford, Dept Phys, Oxford OX1 3RH, England

[2] Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany

[3] Lab Nazl Gran Sasso, I-67010 Assergi, Italy

[4] Tech Univ Munich, Phys Dept E 15, D-85748 Garching, Germany

来源：

NEW ASTRONOMY REVIEWS | 2005年 / 49卷 / 2-6期

关键词：

dark matter; cryogenic detectors;

D O I：

10.1016/j.newar.2005.01.016

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorbers for direct WIMP (weakly interactive massive particles) detection. The phonon signal in the CaWO4 crystal is registered in coincidence with the light signal, which is measured with a separate cryogenic light detector. The absorber crystal and the silicon light detector are read out by tungsten superconducting phase transition thermometers (W-SPTs). As a result an active discrimination of the electron recoils against nuclear recoils is achieved. Results on the properties of the detector modules and on the WIMP sensitivity are presented. (C) 2005 Published by Elsevier B.V.

引用

页码：255 / 258

页数：4

共 8 条

[1] New results from the Cryogenic Dark Matter Search experiment [J].

Akerib, DS ;

Alvaro-Dean, J ;

Armel, MS ;

Attisha, MJ ;

Baudis, L ;

Bauer, DA ;

Bolozdynya, AI ;

Brink, PL ;

Bunker, R ;

Cabrera, B ;

Caldwell, DO ;

Castle, JP ;

Chang, CL ;

Clarke, RM ;

Crisler, MB ;

Cushman, P ;

Davies, AK ;

Dixon, R ;

Driscoll, DD ;

Duong, L ;

Emes, J ;

Ferril, R ;

Gaitskell, RJ ;

Golwala, SR ;

Haldeman, M ;

Hellmig, J ;

Hennessey, M ;

Holmgren, D ;

Huber, ME ;

Kamat, S ;

Kurylowicz, M ;

Lu, A ;

Mahapatra, R ;

Mandic, V ;

Martinis, JM ;

Meunier, P ;

Mirabolfathi, N ;

Nam, SW ;

Nelson, H ;

Nelson, R ;

Ogburn, RW ;

Perales, J ;

Perera, TA ;

Isaac, MCI ;

Rau, W ;

Reisetter, A ;

Ross, RR ;

Saab, T ;

Sadoulet, B ;

Sander, J .

PHYSICAL REVIEW D, 2003, 68 (08)

[2] Limits on WIMP dark matter using sapphire cryogenic detectors [J].

Angloher, G ;

Bruckmayer, M ;

Bucci, C ;

Bühler, M ;

Cooper, S ;

Cozzini, C ;

DiStefano, P ;

von Feilitzsch, F ;

Frank, T ;

Hauff, D ;

Jagemann, T ;

Jochum, J ;

Jörgens, V ;

Keeling, R ;

Kraus, H ;

Loidl, M ;

Marchese, J ;

Meier, O ;

Nagel, U ;

Pröbst, F ;

Ramachers, Y ;

Rulofs, A ;

Schnagl, J ;

Seidel, W ;

Sergeyev, I ;

Sisti, M ;

Stark, M ;

Uchaikin, S ;

Stodolsky, L ;

Wulandari, H ;

Zerle, L .

ASTROPARTICLE PHYSICS, 2002, 18 (01) :43-55

[3]

ANGLOHER G, 2003, P 10 INT WORKSH LOW

[4] Improved exclusion limits from the EDELWEISS WIMP search [J].

Benoit, A ;

Bergé, L ;

Broniatowski, A ;

Chabert, L ;

Chambon, B ;

Chapellier, M ;

Chardin, G ;

Charvin, R ;

De Jésus, M ;

Di Stefano, P ;

Drain, D ;

Dumoulin, L ;

Gascon, J ;

Gerbier, G ;

Gerlic, E ;

Goldbach, C ;

Goyot, M ;

Gros, M ;

Hadjout, JP ;

Hervé, S ;

Juillard, A ;

de Lesquen, A ;

Loidl, M ;

Mallet, J ;

Marnieros, S ;

Martineau, O ;

Mirabolfathi, N ;

Mosca, L ;

Navick, XF ;

Nollez, G ;

Pari, P ;

Riccio, C ;

Sanglard, V ;

Stern, M ;

Vagneron, L .

PHYSICS LETTERS B, 2002, 545 (1-2) :43-49

[5] Search for WIMP annual modulation signature: Results from DAMA/NaI-3 and DAMA/NaI-4 and the global combined analysis [J].

Bernabei, R ;

Belli, P ;

Cerulli, R ;

Montecchia, F ;

Amato, M ;

Ignesti, G ;

Incicchitti, A ;

Prosperi, D ;

Dai, CJ ;

He, HL ;

Kuang, HH ;

Ma, JM .

PHYSICS LETTERS B, 2000, 480 (1-2) :23-31

[6]

FRANK T, 2001, P 7 INT C ADV TECH P

[7]

PETRICCA F, 2003, P 10 INT WORKSH LOW

[8]

Wulandari H., 2004, HEPEX0401032

← 1 →