Results of CRESST phase I; Nuclear Physics B- Proceedings Supplements; Vol. 110, №2

Détails bibliographiques
Parent link:	Nuclear Physics B- Proceedings Supplements: Scientific Journal Vol. 110, №2.— 2002.— [P. 67-69]
Autres auteurs:	Probst F., Angloher G., Bruckmayer M., Bucci C., Cooper S., Stefano P. Di, Feilitzsch T. von, Frank T., Hauff D., Jagemann Th., Jochum J., Keeling R., Kraus H., Marchese J., Ramachers Y., Schnagl J., Seidel W., Sergeyev I., Stark M., Stodolsky L., Wulandari H.
Résumé:	Title screen Results of the CRESST experiment at Gran Sasso using 262 g sapphire calorimeters with tungsten phase transition thermometers are presented. Calibration and analysis methods are described. Data taken in 2000 have been used to place limits on WIMP dark matter particles in the galactic halo. The sapphire detectors are especially sensitive for low-mass WIMPS with spin-dependent interaction and improve on existing limits in this region Режим доступа: по договору с организацией-держателем ресурса
Langue:	anglais
Publié:	2002
Sujets:	электронный ресурс труды учёных ТПУ
Accès en ligne:	http://elibrary.ru/item.asp?id=1234261 http://www.sciencedirect.com/science/article/pii/S0920563202014536
Format:	Électronique Chapitre de livre
KOHA link:	https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=637178

Description
Résumé:	Title screen Results of the CRESST experiment at Gran Sasso using 262 g sapphire calorimeters with tungsten phase transition thermometers are presented. Calibration and analysis methods are described. Data taken in 2000 have been used to place limits on WIMP dark matter particles in the galactic halo. The sapphire detectors are especially sensitive for low-mass WIMPS with spin-dependent interaction and improve on existing limits in this region Режим доступа: по договору с организацией-держателем ресурса

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