High-energy cosmic ray electrons interaction with Dark Matter particles are considered. In particular, a weakening of energy spectrum of cosmic electrons is predicted resulting from inelastic electron scattering on hyper-pions in the hypercolor extension of the Standard Model. Corresponding cross section and angular distributions of secondary neutrino are calculated and studied. We also briefly discuss some effects of scattering processes of such type.

On the scattering of a high-energy cosmic ray electrons off the dark matter

High-energy cosmic ray electrons interaction with Dark Matter particles is considered. In particular, a weakening of energy spectrum of cosmic electrons is predicted resulting from inelastic electr...

Scattering of high-energy cosmic ray electrons off the Dark Matter

Analysis of branon dark matter and extra-dimensional models with AMS-02

Dark matter is one of the main goals of neutrino astronomy. At present, there are two big neutrino telescopes based on the Cherenkov technique in ice and water: IceCube at the South Pole and ANTARES in the northern hemisphere. Both telescopes are performing an indirect search for Dark Matter by looking for a statistical excess of neutrinos coming from astrophysical massive objects. This excess could be an evidence of the possible annihilation of dark matter particles in the centre of these objects. In one of the most popular scenarios the Dark Matter is composed of WIMP particles. The analysis and results of the ANTARES neutrino telescope for the indirect detection of Dark Matter fluxes from the Sun are here presented, as well as the latest IceCube published sensitivity results, for different Dark Matter models.

/pdf/indirect-dark-matter-search-with-large-neutrino-telescopes-2y62dpthr0.pdf

Indirect dark matter search with large neutrino telescopes

Indirect Dark Matter search with large neutrino telescopes

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Indirect dark matter search with large neutrino telescopes

Indirect Dark Matter search with large neutrino telescopes