Search for neutralino Dark Matter with the AMANDA neutrino telescope and prospects for IceCube

Details Search for neutralino Dark Matter with the AMANDA neutrino telescope and prospects for IceCube Search for neutralino Dark Matter with the AMANDA neutrino telescope and prospects for IceCube

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1115...42r&link_type=abstract

THE DARK SIDE OF THE UNIVERSE: 4th International Workshop on the Dark Side of the Universe. AIP Conference Proceedings, Volume

Statistics

Dark Matter, Supersymmetry, Molecular And Chemical Processes And Interactions

Scientific paper

If non-baryonic dark matter exists in the form of neutralinos, a neutrino flux is expected from the decay of neutralino pair annihilation products inside heavy celestial bodies. Data taken with the AMANDA-II neutrino telescope located at the South Pole, have been used in a search for this indirect dark matter signal. Results will be presented from searches for neutralinos accumulated in the Sun, using AMANDA-II data of 2001 and 2003, and in the centre of the Earth, using AMANDA-II data of 2001 to 2003. Future perspectives, achieved by higher statistics data samples acquired during recent years and by the combined AMANDA-IceCube detector, will also be discussed.

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