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 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008dmap.conf..122r&link_type=abstract

DARK MATTER IN ASTROPARTICLE AND PARTICLE PHYSICS. Proceedings of the 6th International Heidelberg Conference. Held 24-28 Septem

Physics

Dark Matter, Neutralino, Neutrino Telescopes, Amanda/Icecube, South Pole

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 are presented from searches for neutralinos accumulated in the Sun, using AMANDA-II data from 2001, and in the centre of the Earth, using AMANDA-II data from 2001 to 2003. Future perspectives, in view of higher statistics data samples acquired during recent years and by the combined AMANDA-IceCube detector, are also discussed.

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