摘要: Neutrinos could be key particles to unravel the nature of dark matter Universe. On one hand, sterile neutrinos in minimal extensions Standard Model are excellent candidates, producing potentially observable signals form a line X-ray sky. other annihilation or decay produces, many plausible scenarios, neutrino flux that detected at telescopes, thus providing non-gravitational evidence for matter. More conservatively, non-observation significant excess fluxes with respect expected astrophysical backgrounds can used constrain properties, such as self-annihilation cross section, scattering section nucleons and lifetime.
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