CRESST cryogenic dark matter search; New Astronomy Reviews; Vol. 49, iss. 2-6

CRESST cryogenic dark matter search; New Astronomy Reviews; Vol. 49, iss. 2-6

Dades bibliogràfiques
Parent link:	New Astronomy Reviews: Scientific Journal Vol. 49, iss. 2-6.— 2005.— [P. 255-258]
Altres autors:	Cozzini C., Henry S., Kraus H., Majorovits B., Ramachers Y., Angloher G., Frank T., Hauff D., Ninkovic J., Petricca F., Probst F., Seidel W., Stodolsky L., Uchaykin S. V. Sergey Victorovich, Bucci C., Feilitzsch F. von, Jagemann T., Jochum J., Rau W., Razeti M., Stark M., Wulandari H.
Sumari:	Title screen 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 Режим доступа: по договору с организацией-держателем ресурса
Idioma:	anglès
Publicat:	2005
Matèries:	электронный ресурс труды учёных ТПУ
Accés en línia:	http://www.sciencedirect.com/science/article/pii/S1387647305000369
Format:	Electrònic Capítol de llibre
KOHA link:	https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=637161

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