http://arxiv.org/abs/1507.06200
An unidentified 3.5 keV line from X-ray observations of galaxy clusters has been reported recently. Although still under scrutiny, decaying dark matter could be responsible for this signal. We investigate whether an axino with a mass of 7 keV could explain the line, keeping the discussion as model independent as possible. We point out several obstacles, which were overlooked in the literature, and which make the axino an unlikely candidate.
S. Colucci, H. Dreiner, F. Staub, et. al.
Thu, 23 Jul 15
23/39
Comments: 4 pages
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