Ponente
Miguel Campos
(King's College London)
Descripción
The best strategy for indirect detection of dark matter depends entirely on its annihilation processes. In this work we discuss a model independent probe for dark matter annihilations into right-handed neutrinos in the GeV-TeV mass range, using dwarf spheroidal galaxies and the galactic center observations performed by Fermi-LAT and H.E.S.S., respectively. We exclude the thermal annihilation cross section for dark matter masses below 200 GeV.
