skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Photon spectra from WIMP annihilation

Journal Article · · Physical Review. D, Particles Fields
 [1]; ; ;  [2];  [3]
  1. William I. Fine Theoretical Physics Institute, University of Minnesota, Minneapolis, Minnesota 55455 (United States) and School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455 (United States)
  2. Departamento de Fisica Teorica I, Universidad Complutense de Madrid, E-28040 Madrid (Spain)
  3. INFN sezione di Torino, I-10122 Torino, Italy and Dipartimento di Fisica Teorica, Universita di Torino, I-10122 Torino (Italy)

If the present dark matter in the Universe annihilates into standard model particles, it must contribute to the fluxes of cosmic rays that are detected on the Earth and, in particular, to the observed gamma-ray fluxes. The magnitude of such a contribution depends on the particular dark matter candidate, but certain features of the produced photon spectra may be analyzed in a rather model-independent fashion. In this work we provide the complete photon spectra coming from WIMP annihilation into standard model particle-antiparticle pairs obtained by extensive Monte Carlo simulations. We present results for each individual annihilation channel and provide analytical fitting formulas for the different spectra for a wide range of WIMP masses.

OSTI ID:
21541448
Journal Information:
Physical Review. D, Particles Fields, Vol. 83, Issue 8; Other Information: DOI: 10.1103/PhysRevD.83.083507; (c) 2011 American Institute of Physics; ISSN 0556-2821
Country of Publication:
United States
Language:
English