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Breit-Wigner Enhancement of Dark Matter Annihilation

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 نشر من قبل Hitoshi Murayama
 تاريخ النشر 2008
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We point out that annihilation of dark matter in the galactic halo can be enhanced relative to that in the early universe due to a Breit-Wigner tail, if the dark matter annihilates through a pole just below the threshold. This provides a new explanation to the boost factor which is suggested by the recent data of the PAMELA, ATIC and PPB-BETS cosmic-ray experiments.



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