作者: G. Angloher , Y. Ramachers , F. von Feilitzsch , I. Sergeyev , W. Seidel
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摘要: Data taken by CRESST in 2000 with a cryogenic detector system based on 262 g sapphire crystals is used to place limits WIMP dark matter the Galactic Halo. The especially sensitive for low-mass WIMPS spin-dependent cross sections and improves existing this region. now preparing second phase, which will use 10 kg consisting of 300 CaWO4 simultaneous detection phonons scintillation light reduce background.