Dark matter through the axion portal

Yasunori Nomura and Jesse Thaler
Phys. Rev. D 79, 075008 – Published 15 April 2009

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

  • Received 10 November 2008

DOI:https://doi.org/10.1103/PhysRevD.79.075008

©2009 American Physical Society

Authors & Affiliations

Yasunori Nomura and Jesse Thaler

  • Berkeley Center for Theoretical Physics, University of California, Berkeley, California 94720, USA, and Theoretical Physics Group, Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA

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Issue

Vol. 79, Iss. 7 — 1 April 2009

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