The CRESST Dark Matter Search Status and Future; DARK 2002
| Parent link: | DARK 2002.— 2002.— [P. 517-523] |
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| Altri autori: | , , , , , , , , , , , , , , , , , , , , |
| 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
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| Soggetti: | |
| 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 |
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| 200 | 1 | |a The CRESST Dark Matter Search Status and Future |f W. Seidel [et al.] | |
| 203 | |a Text |c electronic | ||
| 300 | |a Title screen | ||
| 320 | |a [Ref.: p. 523 (17 tit.)] | ||
| 330 | |a 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 | ||
| 333 | |a Режим доступа: по договору с организацией-держателем ресурса | ||
| 463 | 1 | |t DARK 2002 |o Proceedings of the 4th International Conference (4–9 February 2002, Cape Town, South Africa) |h Part 8 |v [P. 517-523] |d 2002 | |
| 610 | 1 | |a электронный ресурс | |
| 610 | 1 | |a труды учёных ТПУ | |
| 610 | 1 | |a Dark matter | |
| 610 | 1 | |a Темная Материя | |
| 610 | 1 | |a детекторы | |
| 701 | 1 | |a Seidel |b W. |g Wolfgang | |
| 701 | 1 | |a Altmann |b M. | |
| 701 | 1 | |a Angloher |b G. | |
| 701 | 1 | |a Bucci |b C. | |
| 701 | 1 | |a Cooper |b S. | |
| 701 | 1 | |a Cozzini |b C. | |
| 701 | 1 | |a Feilitzsch |b F. von | |
| 701 | 1 | |a Frank |b T. | |
| 701 | 1 | |a Hauff |b D. | |
| 701 | 1 | |a Jagemann |b Th. | |
| 701 | 1 | |a Jochum |b J. | |
| 701 | 1 | |a Keeling |b R. | |
| 701 | 1 | |a Kraus |b H. | |
| 701 | 1 | |a Macallister |b J. | |
| 701 | 1 | |a Probst |b F. | |
| 701 | 1 | |a Ramachers |b Y. | |
| 701 | 1 | |a Rulofs |b A. | |
| 701 | 1 | |a Stark |b M. | |
| 701 | 1 | |a Stodolsky |b L. | |
| 701 | 1 | |a Uchaykin |b S. V. |c specialist in the field of non-destructive testing |c Engineer of Tomsk Polytechnic University, Doctor of physical and mathematical sciences |f 1963- |g Sergey Victorovich |3 (RuTPU)RU\TPU\pers\32279 | |
| 701 | 1 | |a Wulandari |b H. | |
| 801 | 2 | |a RU |b 63413507 |c 20150323 |g RCR | |
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