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

Manylion Llyfryddiaeth
Parent link:	Astroparticle Physics: Scientific Journal Vol. 18, iss. 1.— 2002.— [P. 43-55]
Awduron Eraill:	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.
Crynodeb:	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
Iaith:	Saesneg
Cyhoeddwyd:	2002
Pynciau:	электронный ресурс труды учёных ТПУ
Mynediad Ar-lein:	http://www.sciencedirect.com/science/article/pii/S092765050200111
Fformat:	Electronig Pennod Llyfr
KOHA link:	https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=637172

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