How to find a dark matter sterile neutrino?

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.


Published in:
Phys. Rev. Lett., 97, 261302
Year:
2006
Other identifiers:
Scopus: 2-s2.0-33846371551
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 Record created 2010-09-07, last modified 2018-12-03

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