Hoping to indirectly detect Dark Matter with cosmic rays

Details Hoping to indirectly detect Dark Matter with cosmic rays Hoping to indirectly detect Dark Matter with cosmic rays

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1304..152c&link_type=abstract

EXOTIC NUCLEI AND NUCLEAR/PARTICLE ASTROPHYSICS (III): From Nuclei to Stars. AIP Conference Proceedings, Volume 1304, pp. 152-1

Astronomy and Astrophysics

Astrophysics

Cosmic Rays, Dark Matter, Galaxies, Cosmology, Energy States, Cosmic Rays, Dark Matter, Galactic Halo, Origin And Formation Of The Universe, Composition, Energy Spectra And Interactions

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 experiment 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? What are the constraints from gamma rays measurements and cosmology? [Report number: Saclay T-10/098, CERN-PH-TH/2010-183].

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