| Limits on WIMP Dark Matter using Sapphire Cryogenic Detectors (2002) | |||||||||
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Abstract | |||||||||
| 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. | |||||||||
Details der Publikation | |||||||||
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