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

Bibliografiske detaljer
Parent link:	New Astronomy Reviews: Scientific Journal Vol. 49, iss. 2-6.— 2005.— [P. 255-258]
Andre forfattere:	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.
Summary:	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
Sprog:	engelsk
Udgivet:	2005
Fag:	электронный ресурс труды учёных ТПУ
Online adgang:	http://www.sciencedirect.com/science/article/pii/S1387647305000369
Format:	Electronisk Book Chapter
KOHA link:	https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=637161

Internet