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Results and plans of the CRESST dark matter search

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arxiv astro-ph/0106314 v1 pith:3OTHZX6T submitted 2001-06-18 astro-ph

M. Altmann , G. Angloher , M. Bruckmayer , C. Bucci , S. Cooper , C. Cozzini , P. DiStefano , F. von Feilitzsch
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T. Frank D. Hauff Th. Jagemann J. Jochum R. Keeling H. Kraus J. Macallister F.Proebst Y. Ramachers J. Schnagl W. Seidel I. Sergeyev M. Stark L. Stodolsky H. Wulandari
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keywords cresstdetectorcrystalsdarklimitsmatterbackgroundcawo4
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Data taken by CRESST in 2000 with a cryogenic detector system based on 262 g sapphire crystals is used to place limits on WIMP dark matter in the Galactic Halo. The detector is especially sensitive for low-mass WIMPS with spin-dependent cross sections and improves on existing limits in this region. CRESST is now preparing for a second phase, which will use a 10 kg detector consisting of 300 g CaWO4 crystals with simultaneous detection of phonons and scintillation light to reduce background.

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