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We propose a strategy for how to look for dark matter particles possessing a radiative decay channel and derive constraints on their parameters from observations of x rays from our own Galaxy and its dwarf satellites. When applied to sterile neutrinos in the keV mass range this approach gives a significant improvement to restrictions on neutrino parameters compared with previous works. © 2006 The American Physical Society.
Marco Drewes, Valerie Fiona Domcke, Michele Lucente
Georges Meylan, Bo Li, Yi Wang, Richard Massey