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

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.

Note:

21 pages, 13 figures

98.70.Rz
96.50.sb
98.70.Sa
13.85.Tp
p: cosmic radiation
Boltzmann equation: solution
cosmic radiation: propagation
magnetic field: galaxy
gamma ray: cosmic radiation
cosmic radiation: angular distribution

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