The CRESST Dark Matter Search Status and Future

Bibliographic Details
Parent link:	DARK 2002: Proceedings of the 4th International Conference (4–9 February 2002, Cape Town, South Africa). [P. 517-523].— , 2002
Other Authors:	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.
Summary:	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
Published:	2002
Subjects:	электронный ресурс труды учёных ТПУ Dark matter Темная Материя детекторы
Online Access:	http://link.springer.com/chapter/10.1007%2F978-3-642-55739-2_48
Format:	Electronic Book Chapter
KOHA link:	https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=637171

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