Cirelli, M. (2010) Recent developments in theory and phenomenology of Dark Matter. Il nuovo cimento C, 33 (4). pp. 35-42. ISSN 1826-9885
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Abstract
Dark Matter constitutes more than 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 and model building? What are the constraints from gamma-rays measurements and cosmology?
| Item Type: | Article |
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| Uncontrolled Keywords: | Dark matter (stellar, interstellar, galactic, and cosmological) |
| Subjects: | 500 Scienze naturali e Matematica > 530 Fisica |
| Depositing User: | Marina Spanti |
| Date Deposited: | 02 Apr 2020 14:38 |
| Last Modified: | 02 Apr 2020 14:38 |
| URI: | http://eprints.bice.rm.cnr.it/id/eprint/16986 |
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