Fine-scale anisotropy of the cosmic γ-ray background to identify the underlying generation process

Details Fine-scale anisotropy of the cosmic γ-ray background to identify the underlying generation process Fine-scale anisotropy of the cosmic γ-ray background to identify the underlying generation process

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989nuphs..10..228c&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 10, Issue 2, p. 228-233.

Physics

Nuclear Physics

Scientific paper

The study of the intrinsic anisotropies of the extragalactic γ-ray background is of cosmological importance. As the first step to investigate the anisotropies, we introduce new evolution results of the active galaxies, and calculate the fine-scale anisotropy due to the possible contribution from the active galactic nuclei (AGN) model. By use of Monte Carlo simulations, we discuss the fine-scale fluctuation patterns, and propose that these patterns or anisotropies form a unique test for the AGN generation mechanism.
We also suggest that the best energy range to test the AGN model is Eo ~ 10 MeV.

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