Dark Matter, Cosmic Rays and Neutrinos: status circa 2010

Details Dark Matter, Cosmic Rays and Neutrinos: status circa 2010 Dark Matter, Cosmic Rays and Neutrinos: status circa 2010

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011nuphs.217..237c&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 217, Issue 1, p. 237-242.

Physics

Nuclear Physics

Scientific paper

Dark Matter constitutes more that 80% of the total amount of matter in the Universe, yet almost nothing is known about its nature. A powerful investigation technique is that of searching for the products of annihilations of Dark Matter particles in the galactic halo, on top of the ordinary cosmic rays. Recent data from the PAMELA and FERMI satellites and a number of balloon experiments have reported unexpected excesses in the measured fluxes of cosmic rays. Are these the first direct evidences for Dark Matter? If yes, which DM models and candidates can explain these anomalies (in terms of annihilations) and what do they imply for future searches and model building? What are the constraints from gamma rays and neutrino measurements?

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