Dark matter annihilation into right-handed neutrinos and the galactic center gamma-ray excess
arXiv:1512.02899 · doi:10.1007/JHEP03(2016)043
Abstract
In this paper, we will discuss a specific case that the dark matter particles annihilate into right-handed neutrinos. We calculate the predicted gamma-ray excess from the galactic center and compare our results with the data from the Fermi-LAT. An approximately 10-60 GeV right-handed neutrino with heavier dark matter particle can perfectly explain the observed spectrum. The annihilation cross section falls within the range -, which is roughly compatible with the WIMP annihilation cross section.
11 pages, 5 figures
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