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- W1992642247 abstract "There is a considerable interest in the possible detection of dark matter1 through astrophysical observations as well as terrestrial observations.2,3 If dark matter is made up of massive, weakly interacting particles, one of the best indirect signatures would be the detection of annihilation products of these particles.4–7 It has been recently suggested8–12 that if the halo of our Galaxy is made of particles in the mass range 1 GeV to 100 GeV, and if these particles self-annihilate, as most of the potential candidates do, then monoenergetic γ rays should be observed when they annihilate directly into two photons. The energy of these γ's is very nearly equal to the mass of the (non-relativistic: v/c± 10−3) parent particles. Very narrow γ lines in the range 1 GeV to 100 GeV would provide a clear signature for dark matter annihilation, if they stand out above the background." @default.
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- W1992642247 date "1989-12-01" @default.
- W1992642247 modified "2023-09-23" @default.
- W1992642247 title "Searching for Halo Dark Matter through ? Ray Lines" @default.
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- W1992642247 doi "https://doi.org/10.1111/j.1749-6632.1989.tb50631.x" @default.
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