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

Chi tiết về thư mục
Parent link:	New Astronomy Reviews: Scientific Journal Vol. 49, iss. 2-6.— 2005.— [P. 255-258]
Tác giả khác:	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.
Tóm tắt:	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
Ngôn ngữ:	Tiếng Anh
Được phát hành:	2005
Những chủ đề:	электронный ресурс труды учёных ТПУ
Truy cập trực tuyến:	http://www.sciencedirect.com/science/article/pii/S1387647305000369
Định dạng:	Điện tử Chương của sách
KOHA link:	https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=637161

Internet

http://www.sciencedirect.com/science/article/pii/S1387647305000369