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

来源：

PHYSICS OF ATOMIC NUCLEI | 2004年 / 67卷 / 11期

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

页码：2027 / 2031

页数：5

共 25 条

[1] Exclusion limits on the WIMP-nucleon cross section from the cryogenic dark matter search [J].

Abrams, D ;

Akerib, DS ;

Armel-Funkhouser, MS ;

Baudis, L ;

Bauer, DA ;

Bolozdynya, A ;

Brink, PL ;

Bunker, R ;

Cabrera, B ;

Caldwell, DO ;

Castle, JP ;

Chang, CL ;

Clarke, RM ;

Crisler, MB ;

Dixon, R ;

Driscoll, D ;

Eichblatt, S ;

Gaitskell, RJ ;

Golwala, SR ;

Haller, EE ;

Hellmig, J ;

Holmgren, D ;

Huber, ME ;

Kamat, S ;

Lu, A ;

Mandic, V ;

Martinis, JM ;

Meunier, P ;

Nam, SW ;

Nelson, H ;

Perera, TA ;

Isaac, MCP ;

Rau, W ;

Ross, RR ;

Saab, T ;

Sadoulet, B ;

Sander, J ;

Schnee, RW ;

Shutt, T ;

Smith, A ;

Sonnenschein, AH ;

Spadafora, AL ;

Wang, G ;

Yellin, S ;

Young, BA .

PHYSICAL REVIEW D, 2002, 66 (12)

[2] Exclusion limits on the WIMP-nucleon cross section from the Cryogenic Dark Matter Search [J].

Abusaidi, R ;

Akerib, DS ;

Barnes, PD ;

Bauer, DA ;

Bolozdynya, A ;

Brink, PL ;

Bunker, R ;

Cabrera, B ;

Caldwell, DO ;

Castle, JP ;

Clarke, RM ;

Colling, P ;

Crisler, MB ;

Cummings, A ;

Silva, AD ;

Davies, AK ;

Dixon, R ;

Dougherty, BL ;

Driscoll, D ;

Eichblatt, S ;

Emes, J ;

Gaitskell, RJ ;

Golwala, SR ;

Hale, D ;

Haller, EE ;

Hellmig, J ;

Huber, ME ;

Irwin, KD ;

Jochum, J ;

Lipschultz, FP ;

Lu, A ;

Mandic, V ;

Martinis, JM ;

Nam, SW ;

Nelson, H ;

Neuhauser, B ;

Penn, MJ ;

Perera, TA ;

Isaac, MCP ;

Pritychenko, B ;

Ross, RR ;

Saab, T ;

Sadoulet, B ;

Schnee, RW ;

Seitz, DN ;

Shestople, P ;

Shutt, T ;

Smith, A ;

Smith, GW ;

Sonnenschein, AH .

PHYSICAL REVIEW LETTERS, 2000, 84 (25) :5699-5703

[3] 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

[4] First results of the EDELWEISS WIMP search using a 320 g heat-and-ionization Ge detector [J].

Benoit, A ;

Bergé, L ;

Broniatowski, A ;

Chambon, B ;

Chapellier, M ;

Chardin, G ;

Charvin, P ;

De Jésus, M ;

Di Stefano, P ;

Drain, D ;

Dumoulin, L ;

Gascon, J ;

Gerbier, G ;

Goldbach, C ;

Goyot, M ;

Gros, M ;

Hadjout, JP ;

Juillard, A ;

de Lesquen, A ;

Loidl, M ;

Mallet, J ;

Marnieros, S ;

Martineau, O ;

Mirabolfathi, N ;

Mosca, L ;

Miramonti, L ;

Navick, XF ;

Nollez, G ;

Pari, P ;

Stern, M ;

Vagneron, L .

PHYSICS LETTERS B, 2001, 513 (1-2) :15-22

[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]

Bernabei R, 2003, RIV NUOVO CIMENTO, V26, P1

[7]

Broniatowski A, 2002, AIP CONF PROC, V605, P521, DOI 10.1063/1.1457700

[8]

BRONIATOWSKI A, 2003, IN PRESS NUCL INSTRU

[9] What is the big-bang-nucleosynthesis prediction for the baryon density and how reliable is it? art. no. 063512 [J].

Burles, S ;

Nollett, KM ;

Turner, MS .

PHYSICAL REVIEW D, 2001, 63 (06)

[10]

CHARDIN G, 2003, P 4 INT WORKSH ID DA, P470, DOI DOI 10.1142/9789812791313_FMATTER

← 1 2 3 →