Tools for Dark Matter Indirect Detection
Résumé
I discuss ingredients and recipes for computing signals of TeV-scale Dark Matter annihilations and decays in the Galaxy and beyond: the energy spectra of electrons and positrons, antiprotons, antideuterons, gamma rays, neutrinos and antineutrinos e, mu, tau at production, the propagation functions for charged particles in the Galaxy, the energy spectra at the location of the Earth, the gamma ray fluxes from the Galaxy and from beyond. All results discussed here are available in numerical form and ready to be consumed.