Angular, spectral, and time distributions of highest energy protons and associated secondary gamma-rays and neutrinos propagating through extragalactic magnetic and radiation fields

A.Y. Prosekin; F.A. Aharonian; S.R. Kelner

arxiv: 1006.1045 · v1 · pith:FVH3UH7Enew · submitted 2010-06-05 · 🌌 astro-ph.HE

Angular, spectral, and time distributions of highest energy protons and associated secondary gamma-rays and neutrinos propagating through extragalactic magnetic and radiation fields

F.A. Aharonian , S.R. Kelner , A.Y. Prosekin This is my paper

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keywords angularenergyfieldsgamma-rayshighestmagneticneutrinospropagating

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The angular, spectral and temporal features of the highest energy protons and accompanying them secondary neutrinos and synchrotron gamma-rays propagating through the intergalactic magnetic and radiation fields are studied using the analytical solutions of the Boltzmann transport equation obtained in the limit of the small-angle and continuous-energy-loss approximation.

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