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- W2100059055 abstract "If non‐baryonic dark matter exists in the form of neutralinos, it may accumulate in massive celestial bodies, leading to a neutrino flux from the decay products of neutralino pair annihilation. Such fluxes can be detected with high energy neutrino telescopes. We will present current results from searches for neutrino signals of neutralinos accumulated in the Earth and the Sun, using AMANDA data taken in 1997–1999 and 2001 respectively. We also discuss the improvements expected from a combined analysis of several years of newer data and the prospects for the 1 km 3 IceCube detector." @default.
- W2100059055 created "2016-06-24" @default.
- W2100059055 creator A5008310294 @default.
- W2100059055 date "2007-01-01" @default.
- W2100059055 modified "2023-10-16" @default.
- W2100059055 title "Search for Dark Matter with the AMANDA detector" @default.
- W2100059055 doi "https://doi.org/10.1063/1.2735257" @default.
- W2100059055 hasPublicationYear "2007" @default.
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