The CRESST Dark Matter Search Status and Future; DARK 2002

The CRESST Dark Matter Search Status and Future; DARK 2002

গ্রন্থ-পঞ্জীর বিবরন
Parent link:DARK 2002.— 2002.— [P. 517-523]
অন্যান্য লেখক: 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.
সংক্ষিপ্ত: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
ভাষা:ইংরেজি
প্রকাশিত: 2002
বিষয়গুলি:
электронный ресурс
труды учёных ТПУ
Dark matter
Темная Материя
детекторы
অনলাইন ব্যবহার করুন:http://link.springer.com/chapter/10.1007%2F978-3-642-55739-2_48
বিন্যাস: বৈদ্যুতিক গ্রন্থের অধ্যায়
KOHA link:https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=637171
বিবরন
সংক্ষিপ্ত: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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