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.
Original language | English |
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Pages (from-to) | 43-55 |
Number of pages | 13 |
Journal | Astroparticle Physics |
Volume | 18 |
Issue number | 1 |
DOIs | |
Publication status | Published - 5 Jul 2002 |
Externally published | Yes |
ASJC Scopus subject areas
- Astronomy and Astrophysics