The CRESST Dark Matter Search Status and Future; DARK 2002

Dettagli Bibliografici
Parent link:	DARK 2002.— 2002.— [P. 517-523]
Altri autori:	Seidel W. Wolfgang, Altmann M., Angloher G., Bucci C., Cooper S., Cozzini C., Feilitzsch F. von, Frank T., Hauff D., Jagemann Th., Jochum J., Keeling R., Kraus H., Macallister J., Probst F., Ramachers Y., Rulofs A., Stark M., Stodolsky L., Uchaykin S. V. Sergey Victorovich, Wulandari H.
Riassunto:	Title screen Data taken by CRESST in 2000 with a cryogenic detector system based on 262 g sapphire crystals is used to place limits on WIMP dark matter in the Galactic Halo. The detector is especially sensitive for low-mass WIMPS with spin-dependent cross sections and improves on existing limits in this region. CRESST is now preparing for a second phase, which will use a 10 kg detector consisting of 300 g CaWO4 crystals with simultaneous detection of phonons and scintillation light to reduce background Режим доступа: по договору с организацией-держателем ресурса
Lingua:	inglese
Pubblicazione:	2002
Soggetti:	электронный ресурс труды учёных ТПУ Dark matter Темная Материя детекторы
Accesso online:	http://link.springer.com/chapter/10.1007%2F978-3-642-55739-2_48
Natura:	Elettronico Capitolo di libro
KOHA link:	https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=637171

Descrizione
Riassunto:	Title screen Data taken by CRESST in 2000 with a cryogenic detector system based on 262 g sapphire crystals is used to place limits on WIMP dark matter in the Galactic Halo. The detector is especially sensitive for low-mass WIMPS with spin-dependent cross sections and improves on existing limits in this region. CRESST is now preparing for a second phase, which will use a 10 kg detector consisting of 300 g CaWO4 crystals with simultaneous detection of phonons and scintillation light to reduce background Режим доступа: по договору с организацией-держателем ресурса

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