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

Bibliografische gegevens
Parent link:	Astroparticle Physics: Scientific Journal Vol. 18, iss. 1.— 2002.— [P. 43-55]
Andere auteurs:	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.
Samenvatting:	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
Taal:	Engels
Gepubliceerd in:	2002
Onderwerpen:	электронный ресурс труды учёных ТПУ
Online toegang:	http://www.sciencedirect.com/science/article/pii/S092765050200111
Formaat:	Elektronisch Hoofdstuk
KOHA link:	https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=637172

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