Cosmological Large Scale Anisotropies in the high-energy cosmic rays and gamma-ray sky

Details Cosmological Large Scale Anisotropies in the high-energy cosmic rays and gamma-ray sky Cosmological Large Scale Anisotropies in the high-energy cosmic rays and gamma-ray sky

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007nuphs.168..280c&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 168, p. 280-282.

Physics

Nuclear Physics

Scientific paper

The interactions that characterize the propagation of γ photons in the TeV energy range and of the Ultra High-Energy cosmic rays at energies >10eV both introduce a cosmological horizon at the distance of few hundreds Mpc, implying a correlation with the local Large Scale Structures. We provide detailed predictions of the expected anisotropies based on the map of the local universe from the PSCz astronomical catalogue. We discuss the chances to detect the predicted signal with the forthcoming observatories like Auger for the UHECRs or the satellite Glast for γ-rays.

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