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astro-ph2001
A 3D time-dependent model for Galactic cosmic rays and gamma rays
A. W. Strong, I. V. Moskalenko
In studies of cosmic-ray (CR) propagation and diffuse continuum gamma-ray emission from the Galaxy it has usually been assumed that the source function can be taken as smooth and t…
astro-ph2001
Secondary Antiprotons in Cosmic Rays
I. V. Moskalenko, A. W. Strong, J. F. Ormes +2
High energy collisions of cosmic ray (CR) nuclei with interstellar gas are believed to be the mechanism producing the majority of CR antiprotons. The distinguishing spectral shape…