Tools for Dark Matter Indirect Detection

Abstract : 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.
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Communication dans un congrès
17th Hellenic School and Workshops on Elementary Particle Physics and Gravity, Sep 2017, Corfu, Greece. PoS, CORFU2017, pp.117, 2018, 〈10.22323/1.318.0117〉
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https://hal.archives-ouvertes.fr/hal-01871990
Contributeur : Inspire Hep <>
Soumis le : mardi 11 septembre 2018 - 15:00:53
Dernière modification le : mardi 18 septembre 2018 - 14:52:38

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Marco Cirelli. Tools for Dark Matter Indirect Detection. 17th Hellenic School and Workshops on Elementary Particle Physics and Gravity, Sep 2017, Corfu, Greece. PoS, CORFU2017, pp.117, 2018, 〈10.22323/1.318.0117〉. 〈hal-01871990〉

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