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Relic neutralinos produced after the Big Bang are favoured candidates for Dark Matter. They can accumulate at the centre of massive celestial objects like our Sun. Their annihilation can result in a high-energy neutrino ux that could be detectable as a localised emission with earth- based neutrino telescopes like ANTARES.

 

 

 


Instituto de Física Corpuscular (IFIC). Universitat de Valencia (UV), E-46980 Paterna (Valencia), Spain