Fitting formulae for photon spectra from WIMP annihilation

Fitting formulae for photon spectra from WIMP annihilation

Annihilation of different dark matter (DM) candidates into Standard Model (SM) particles could be detected through their contribution to the gamma ray fluxes that are measured on the Earth. The magnitude of such contributions depends on the particular DM candidate, but certain imprints of produced p...

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Veröffentlicht in:Journal of physics. Conference series 2011-09, Vol.314 (1), p.012063-4
Hauptverfasser: Cembranos, J A R, de la Cruz-Dombriz, A, Dobado, A, Lineros, R, Maroto, A L
Format: Artikel
Sprache:eng
Schlagworte:
Bosons
Channels
Dark matter
Fittings
Fluxes
Gamma rays
Leptons
Particles (of physics)
Photons
Physics
Spectra
Standard model (particle physics)
Weakly interacting massive particles
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container_title Journal of physics. Conference series
container_volume 314
creator Cembranos, J A R
de la Cruz-Dombriz, A
Dobado, A
Lineros, R
Maroto, A L
description Annihilation of different dark matter (DM) candidates into Standard Model (SM) particles could be detected through their contribution to the gamma ray fluxes that are measured on the Earth. The magnitude of such contributions depends on the particular DM candidate, but certain imprints of produced photon spectra may be analyzed in a model-independent fashion. In this work we provide the fitting formulae for the photon spectra generated by WIMP annihilation into quarks, leptons and gauge bosons channels in a wide range of WIMP masses.
doi_str_mv 10.1088/1742-6596/314/1/012063
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subjects Bosons
Channels
Dark matter
Fittings
Fluxes
Gamma rays
Leptons
Particles (of physics)
Photons
Physics
Spectra
Standard model (particle physics)
Weakly interacting massive particles
title Fitting formulae for photon spectra from WIMP annihilation
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