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Using an effective interaction approach to describe the interactions between the dark matter particle and the light degrees of freedom of the standard model, we calculate the antiproton flux due to the annihilation of the dark matter in the Galactic Halo and compare to the most recent antiproton spectrum of the PAMELA experiment.
G. Bertone, D. Hooper, and J. Silk, “Particle dark matter: Evidence, candidates and constraints,” Phys. Rept. 405
2005
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I. Low, W. Y. Keung and G. Shaughnessy, “When CoGeNT met PAMELA,” arXiv:1010.1774 [hep-ph]
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K. Nakamura et al
2010
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