Results of CRESST phase I

Results of CRESST phase I

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 sapphi...

詳細記述

書誌詳細
主要な著者: Probst, F, Angloher, G, Bruckmayer, M, Bucci, C, Cooper, S, Di Stefano, P, von Feilitzsch, F, Frank, T, Hauff, D, Jagemann, T, Jochum, J, Keeling, R, Kraus, H, Marchese, J, Ramachers, Y, Schnagl, J, Seidel, W, Sergeyev, I, Stark, M, Stodolsky, L, Wulandari, H
フォーマット: Conference item
出版事項: 2002
その他の書誌記述
要約: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.

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