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- W2506773516 abstract "The possibility of amplification of the annihilation signal from dark matter in the Galaxy halo due to its clusterization into small-mass clumps (about the Moon’s or Earth’s mass) is discussed. Formation of dark-matter clumps is considered within the conventional cosmological model taking into account their hierarchical clustering and tidal destruction. It is shown that the amplification factor of γ rays from dark-matter annihilation due to small-mass clumps in the Galaxy may range from 10 to 1000." @default.
- W2506773516 created "2016-08-23" @default.
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- W2506773516 date "2010-10-01" @default.
- W2506773516 modified "2023-10-16" @default.
- W2506773516 title "DARK MATTER ANNIHILATION IN THE GALAXY" @default.
- W2506773516 doi "https://doi.org/10.1142/9789814329682_0046" @default.
- W2506773516 hasPublicationYear "2010" @default.
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