On the generation mechanism of hard cosmic gamma-ray emission from AGN jets

Astronomy and Astrophysics – Astronomy

Scientific paper

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98.54.Cm, 98.62.Nx

Scientific paper

We consider the mechanism for the generation of high-energy cosmic gamma rays through the inelastic interaction of relativistic protons (due to their velocity dispersion) accelerated by a self-consistent electromagnetic field in an electron-positron jet plasma. The velocity dispersion is explained by the growth of a plasma instability in a relativistic jet.

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