TH Cosmo Coffee

The cosmic-ray positron excess and possible Dark Matter interpretations

by Dr Marco Taoso (U. Padova)

→ Europe/Zurich
1/1-025 (CERN)

1/1-025

CERN

20
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Description
Recent results from PAMELA and FERMI suggest an excess in the electrons and positrons cosmic-ray spectra which have been tentatively interpreted in terms of Dark Matter annihilations or decays. I will review the required properties of Dark Matter models needed in order to explain these cosmic-ray observations and I will underline possible difficulties such models have to face with. I will then show astrophysical and cosmological constraints on these interpretations. References: e-Print: arXiv:0905.0636 [astro-ph.HE] e-Print: arXiv:0905.0480 [hep-ph] e-Print: arXiv:0811.3744 [astro-ph] e-Print: arXiv:0901.3582 [hep-ph]
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Geraldine Servant