Photon spectra from WIMP annihilation
- 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)
- Departamento de Fisica Teorica I, Universidad Complutense de Madrid, E-28040 Madrid (Spain)
- 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
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Related Subjects
ANNIHILATION
ANTIPARTICLES
COMPUTERIZED SIMULATION
COSMIC RADIATION
GAMMA RADIATION
MASS
MONTE CARLO METHOD
NONLUMINOUS MATTER
PHOTONS
SPECTRA
STANDARD MODEL
UNIVERSE
WEAK INTERACTIONS
ANTIMATTER
BASIC INTERACTIONS
BOSONS
CALCULATION METHODS
ELECTROMAGNETIC RADIATION
ELEMENTARY PARTICLES
FIELD THEORIES
GRAND UNIFIED THEORY
INTERACTIONS
IONIZING RADIATIONS
MASSLESS PARTICLES
MATHEMATICAL MODELS
MATTER
PARTICLE INTERACTIONS
PARTICLE MODELS
QUANTUM FIELD THEORY
RADIATIONS
SIMULATION
UNIFIED GAUGE MODELS