Dark Matter through the Axion Portal

  title={Dark Matter through the Axion Portal},
  author={Yasunori Nomura and Jesse Thaler},
  journal={Physical Review D},
Motivated by the galactic positron excess seen by PAMELA and ATIC/PPB-BETS, we propose that dark matter is a TeV-scale particle that annihilates into a pseudoscalar 'axion'. The positron excess and the absence of an antiproton or gamma ray excess constrain the axion mass and branching ratios. In the simplest realization, the axion is associated with a Peccei-Quinn symmetry, in which case it has a mass around 360-800 MeV and decays into muons. We present a simple and predictive supersymmetric… 

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        arXiv:0807.1427 [hep-ex]

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        • Phys. 29,
        • 2008

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