The CRESST Dark Matter Search Status and Future; DARK 2002

The CRESST Dark Matter Search Status and Future; DARK 2002

Sonraí bibleagrafaíochta
Parent link:DARK 2002.— 2002.— [P. 517-523]
Rannpháirtithe: 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.
Achoimre: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
Teanga:Béarla
Foilsithe / Cruthaithe: 2002
Ábhair:
электронный ресурс
труды учёных ТПУ
Dark matter
Темная Материя
детекторы
Rochtain ar líne:http://link.springer.com/chapter/10.1007%2F978-3-642-55739-2_48
Formáid: Leictreonach Caibidil leabhair
KOHA link:https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=637171

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