3-11 July 2007
Merida, Mexico
Mexico/General timezone
- icrc2007@icrc2007.unam.mx
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Contribution Poster (WITHDRAWN)
Speakers
- Mr. Pavel KLIMOV
Primary authors
- Mr. Pavel KLIMOV (Skobeltsyn Institute of Nuclear Physics)
- Dr. Boris KHRENOV (Skobeltsyn Institute of Nuclear Physics)
- Dr. Sergei SHARAKIN (Skobeltsyn Institute of Nuclear Physics)
- Dr. Sergey TROITSKY (Institute of Nuclear Research of Russian Academy of Sciences)
- Dr. Oleg KALASHEV (Institute of Nuclear Research of Russian Academy of Sciences)
Abstract content
A space detector has an advantage of observing during a year the arrival directions of ultra-high-energy (UHE) cosmic-ray (CR) particles from the whole sky. We study the prospects of detecting global asymmetries predicted by two distinct scenarios of the origin of UHECR: the Galactic dipole asymmetry expected in the superheavy dark-matter scenario and asymmetries expected if sources of UHE protons follow the distribution of visible matter in the Universe. The first space-based detector of UHECR particles, TUS, will be able to test the predicted asymmetries.