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- W3100485584 abstract "Recently, self-annihilation of dark matter particles is proposed to explain the WMAP Haze and excess of energetic positrons and electrons in ATIC and PAMELA results. If self-annihilation of dark matter occurs around the recombination of cosmic plasma, energy release from self-annihilation of dark matter delays the recombination, and hence affects CMB anisotropy. By using the recent CMB data, we have investigated the self-annihilation of dark matter particles. In this investigation, we do not find statistically significant evidence, and impose an upper bound on <sigma v> / m_chi. The upcoming data from Planck surveyor and the Fermi Gamma-ray telescope will allow us to break some of parameter degeneracy and improve constraints on self-annihilation of dark matter particles." @default.
- W3100485584 created "2020-11-23" @default.
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- W3100485584 date "2010-01-01" @default.
- W3100485584 modified "2023-09-23" @default.
- W3100485584 title "CMB data constraint on self-annihilation of dark matter particles" @default.
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- W3100485584 doi "https://doi.org/10.1063/1.3462637" @default.
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