Limits on WIMP Dark Matter using Sapphire Cryogenic Detectors

Bibliografiset tiedot
Parent link:	Astroparticle Physics: Scientific Journal Vol. 18, iss. 1.— 2002.— [P. 43-55]
Muut tekijät:	Angloher G., Bruckmayer M., Bucci C., Buhler M., Cooper S., Cozzini C., Stefano P. Di, Feilitzsch F. von, Frank T., Hauff D., Jagemann T., Jochum J., Jorgens V., Keeling R., Kraus H., Loidl M., Marchese J., Meier O., Nagel U., Probst F., Ramachens Y., Rulofs A., Schnagl J., Seidel W., Sergeyev I., Sisti M., Stark M., Uchaykin S. V. Sergey Victorovich, Stodolsky L., Wulandari H., Zerle L.
Yhteenveto:	Title screen Data taken by CRESST with a cryogenic detector system based on 262 g sapphire crystals has been used to place limits on WIMP dark matter in the Galactic Halo. The experiment was especially sensitive for low-mass WIMPs with spin-dependent cross sections and improves on existing limits in this region Режим доступа: по договору с организацией-держателем ресурса
Julkaistu:	2002
Aiheet:	электронный ресурс труды учёных ТПУ
Linkit:	http://www.sciencedirect.com/science/article/pii/S092765050200111
Aineistotyyppi:	Elektroninen Kirjan osa
KOHA link:	https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=637172

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