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When CoGeNT met PAMELA

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arxiv 1010.1774 v2 pith:3YS3ARTI submitted 2010-10-08 hep-ph astro-ph.HE

When CoGeNT met PAMELA

classification hep-ph astro-ph.HE
keywords darkmatterinteractionsanti-protoncogentexcesslightpamela
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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If the excess events from the CoGeNT experiment arise from elastic scatterings of a light dark matter off the nuclei, crossing symmetry implies non-vanishing annihilation cross-sections of the light dark matter into hadronic final states inside the galactic halo, which we confront with the anti-proton spectrum measured by the PAMELA collaboration. We consider two types of effective interactions between the dark matter and the quarks: 1) contact interactions from integrating out heavy particles and 2) long-range interactions due to the electromagnetic properties of the dark matter. The lack of excess in the anti-proton spectrum results in tensions for a scalar and, to a less extent, a vector dark matter interacting with the quarks through the Higgs portal.

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