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- W2138522044 abstract "The extragalactic cosmic gamma-ray background (CGB) is expected to provide indirect signatures of the presence of Dark Matter (DM) through gamma-rays produced in DM annihilations. In particular, DM can leave its imprint not only in the CGB energy spectrum but also in the peculiar pattern and intensity of the CGB anisotropies. These are expected to differ significantly with respect to the case of a pure astrophysical origin of the CGB due to the peculiar quadratic dependence µ r 2 c of the DM annihilation signal from the DM density. I will discuss the DM signatures expected in the power spectrum of the CGB anisotropies and the prospect for detection with the forthcoming Fermi/GLAST observatory." @default.
- W2138522044 created "2016-06-24" @default.
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- W2138522044 date "2009-08-24" @default.
- W2138522044 modified "2023-09-24" @default.
- W2138522044 title "Cosmic Gamma-Ray Background Anisotropies and Dark Matter Annihilation" @default.
- W2138522044 doi "https://doi.org/10.22323/1.064.0114" @default.
- W2138522044 hasPublicationYear "2009" @default.
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