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- W3105438863 endingPage "217" @default.
- W3105438863 startingPage "194" @default.
- W3105438863 abstract "Weakly interacting massive particles (WIMPs) remain a prime candidate for the cosmological dark matter (DM), even in the absence of current collider signals that would unambiguously point to new physics below the TeV scale. The self-annihilation of these particles in astronomical targets may leave observable imprints in cosmic rays of various kinds. In this review, we focus on gamma rays which we argue to play a pronounced role among the various possible messengers. We discuss the most promising spectral and spatial signatures to look for, give an update on the current state of gamma-ray searches for DM and an outlook concerning future prospects. We also assess in some detail the implications of a potential signal identification for particle DM models as well as for our understanding of structure formation. Special emphasis is put on the possible evidence for a 130 GeV line-like signal that was recently identified in the data of the Fermi gamma-ray space telescope." @default.
- W3105438863 created "2020-11-23" @default.
- W3105438863 creator A5021706010 @default.
- W3105438863 creator A5038806090 @default.
- W3105438863 date "2012-11-01" @default.
- W3105438863 modified "2023-10-03" @default.
- W3105438863 title "Gamma ray signals from dark matter: Concepts, status and prospects" @default.
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