Limits on WIMP Dark Matter using Sapphire Cryogenic Detectors; Astroparticle Physics; Vol. 18, iss. 1

Limits on WIMP Dark Matter using Sapphire Cryogenic Detectors; Astroparticle Physics; Vol. 18, iss. 1

Bibliographic Details
Parent link:	Astroparticle Physics: Scientific Journal Vol. 18, iss. 1.— 2002.— [P. 43-55]
Other Authors:	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.
Summary:	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
Language:	English
Published:	2002
Subjects:	электронный ресурс труды учёных ТПУ
Online Access:	http://www.sciencedirect.com/science/article/pii/S092765050200111
Format:	Electronic Book Chapter
KOHA link:	https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=637172

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