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.
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