Detectability of gamma-rays from clumps of dark matter

Details Detectability of gamma-rays from clumps of dark matter Detectability of gamma-rays from clumps of dark matter

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990natur.346...39l&link_type=abstract

Nature (ISSN 0028-0836), vol. 346, July 5, 1990, p. 39, 40. Research supported by NSF.

Astronomy and Astrophysics

Astronomy

26

Annihilation Reactions, Dark Matter, Energetic Particles, Gamma Ray Astronomy, Particle Interactions, Galactic Evolution, Gamma Ray Observatory, Particle Mass, Radiation Sources, Spatial Distribution, Spectral Signatures, Weak Interactions (Field Theory)

Scientific paper

The possibility of using the Gamma Ray Observatory (GRO) to detect
gamma-rays from the annihilation of weakly interacting massive particles
in lumps of dark matter in the Galaxy is addressed. An expression is
derived for the expected gamma-ray flux from the nearest lump. Possible
candidates for observations by GRO are considered.

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