Dark matter and cosmic-ray anomalies

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Abstract

After giving a review of recent cosmic-ray observations such as PAMELA, ATIC/PPB-BETS, Fermi and H.E.S.S, I explain what kind of conditions must be met if the PAMELA/Fermi excesses are due to dark matter. Finally I will give one dark matter model based on a Wino LSP with a tiny R-parity violation.

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