Indirect detection of neutralino dark matter

Details Indirect detection of neutralino dark matter Indirect detection of neutralino dark matter

1999-02-11

arxiv.org/abs/astro-ph/9902172v1

Astronomy and Astrophysics

Astrophysics

7 pages, epsfig and aipproc macros. Invited talk at Cosmo-98, Asilomar, CA, to appear in the Proceedings (ed. D. Caldwell)

Scientific paper

10.1063/1.59414

Dark matter detection experiments are getting ever closer to the sensitivity needed to detect the primary particle physics candidates for nonbaryonic dark matter. Indirect detection methods include searching for antimatter and gamma rays, in particular gamma ray lines, in cosmic rays and high-energy neutrinos from the centre of the Earth or Sun caused by accretion and annihilation of dark matter particles. A review is given of recent progress, both on the theoretical and experimental sides.

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