Dark Matter Searches
arXiv:astro-ph/0511805 · doi:10.1142/S0217751X06032873
Abstract
More than 90% of matter in the Universe could be composed of heavy particles, which were non-relativistic, or 'cold', when they froze-out from the primordial soup. I will review current searches for these hypothetical particles, both via interactions with nuclei in deep underground detectors, and via the observation of their annihilation products in the Sun, galactic halo and galactic center.
13 pages, 8 figures, latex. To appear in the Proceedings of the XXII International Symposium on Lepton-Photon Interactions (Uppsala, Sweden, 2005)
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Cited by in corpus (10)
- Limits on spin-dependent WIMP-nucleon cross-sections from the XENON10 experiment
- Constraints on inelastic dark matter from XENON10
- Material screening and selection for XENON100
- New Measurement of the Relative Scintillation Efficiency of Xenon Nuclear Recoils Below 10 keV
- Detecting the Milky Way's Dark Disk
- The scintillation and ionization yield of liquid xenon for nuclear recoils
- Limits on the local dark matter density
- A Modified Gravity and its Consequences for the Solar System, Astrophysics and Cosmology
- Composite macro-bolometers for the rejection of surface radioactive background in rare-event experiments
- The XENON10 WIMP Search Experiment at the Gran Sasso Underground Laboratory