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Titolo:
INSTALLATION OF THE CRYOGENIC DARK-MATTER SEARCH (CDMS)
Autore:
BARNES PD; DASILVA A; AKERIB DS; BAUER D; BRINK P; CABRERA B; CALDWELL DO; CHUGG B; CLARKE RM; CUMMINGS A; DAVIES A; DIAZ RC; DOUGHERTY BL; EMES J; GOLWALA SR; HALE D; HALLER EE; IRWIN KD; KNOWLTON WB; KUZIMINOV V; LU A; NAM SW; PENN MJ; NOVIKOV V; PRITYCHENKO BV; QUEINNEC F; ROSS RR; SADOULET B; SEITZ D; SHUTT T; SMITH A; SMITH G; SONNENSCHEIN A; STOCKWELL W; TAYLOR JD; THERRIEN R; TRUMBULL TL; WHITE S; WOLGAST RC; YELLIN S; YOUNG BA;
Indirizzi:
UNIV CALIF BERKELEY,CTR PARTICLE ASTROPHYS,301 LE CONTE HALL BERKELEYCA 94720 UNIV CALIF BERKELEY,DEPT PHYS BERKELEY CA 94720 UNIV BRITISH COLUMBIA,DEPT PHYS VANCOUVER BC V5Z 1M9 CANADA UNIV CALIF SANTA BARBARA,DEPT PHYS SANTA BARBARA CA 93106 STANFORD UNIV,DEPT PHYS STANFORD CA 94305 CALTECH,JET PROP LAB PASADENA CA 00000 UNIV CALIF BERKELEY,LAWRENCE BERKELEY NATL LAB BERKELEY CA 94720 UNIV CALIF BERKELEY,DEPT MAT SCI & MINERAL ENGN BERKELEY CA 94720 RUSSIAN ACAD SCI,INST NUCL RES,BAKSAN NEUTRINO OBSERV MOSCOW RUSSIA CARLETON UNIV,CRPP OTTAWA ON K1S 5B6 CANADA MICHIGAN STATE UNIV,DEPT PHYS & ASTRON E LANSING MI 48824 UNIV SANTA CLARA,DEPT PHYS SANTA CLARA CA 95053
Titolo Testata:
Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment
fascicolo: 1, volume: 370, anno: 1996,
pagine: 233 - 236
SICI:
0168-9002(1996)370:1<233:IOTCDS>2.0.ZU;2-M
Fonte:
ISI
Lingua:
ENG
Soggetto:
UNIVERSE; LIMITS;
Tipo documento:
Article
Natura:
Periodico
Settore Disciplinare:
Science Citation Index Expanded
Science Citation Index Expanded
Science Citation Index Expanded
Science Citation Index Expanded
Citazioni:
19
Recensione:
Indirizzi per estratti:
Citazione:
P.D. Barnes et al., "INSTALLATION OF THE CRYOGENIC DARK-MATTER SEARCH (CDMS)", Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment, 370(1), 1996, pp. 233-236

Abstract

We discuss the status of a cryogenic dark matter search beginning operation in the Stanford Underground Facility. The detectors will be cooled in a specially designed cryostat connected to a modified side access Oxford 400 dilution refrigerator. We discuss two detector designs and performance, the cryostat construction and operation, and the multi-level shield surrounding the cryostat. Finally, we will examine the limits which we will be able to set on WIMP dark matter with this experiment.

ASDD Area Sistemi Dipartimentali e Documentali, Università di Bologna, Catalogo delle riviste ed altri periodici
Documento generato il 07/07/20 alle ore 06:20:55