English

Dark Matter through the Axion Portal

High Energy Physics - Phenomenology 2010-04-28 v2 Astrophysics High Energy Physics - Theory

Abstract

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 anti-proton 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 model implementing this scenario, where both the Higgsino and dark matter obtain masses from the same source of TeV-scale spontaneous symmetry breaking.

Keywords

Cite

@article{arxiv.0810.5397,
  title  = {Dark Matter through the Axion Portal},
  author = {Yasunori Nomura and Jesse Thaler},
  journal= {arXiv preprint arXiv:0810.5397},
  year   = {2010}
}

Comments

5 pages; reference added

R2 v1 2026-06-21T11:36:25.492Z