Gamma-Rays and Neutrinos from Dark Matter

Details Gamma-Rays and Neutrinos from Dark Matter Gamma-Rays and Neutrinos from Dark Matter

1996-07-05

arxiv.org/abs/astro-ph/9607037v1

Nucl.Phys.Proc.Suppl. 51B (1996) 199-203

Astronomy and Astrophysics

Astrophysics

5 pages, latex file, Proc. 2nd Intl. Symp. on Sources and Detection of Dark Matter in the Universe, Nucl. Phys. B. Conf. Suppl

Scientific paper

10.1016/S0920-5632(96)00511-7

High energy gamma-rays and neutrinos can be produced both by the annihilation and by the possible slow decay of dark matter particles. We discuss the fluxes and spectra of such secondaries produced by dark matter particles in the universe and their observability in competition with other astrophysical gamma-ray signals and with atmospheric neutrinos. To do this, we work within the assumption that the dark matter particles are neutralinos which are the lightest supersymmetric particles (LSPs) predicted by supersymmetry theory.

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