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Cosmic ray propagation and interactions in the Galaxy

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arxiv 1412.0863 v1 pith:AWREPQH5 submitted 2014-12-02 astro-ph.HE

V.N.Zirakashvili This is my paper · ORCID
classification astro-ph.HE
keywords propagationcosmicgalaxymodelsalfvanisotropyconsiderdetermines
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Cosmic ray propagation in the Galaxy is shortly reviewed. In particular we consider the self-consistent models of CR propagation. In these models CR streaming instability driven by CR anisotropy results in the Alfv\'enic turbulence which in turn determines the scattering and diffusion of particles.

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  1. Constraints on Primordial Black Holes from Galactic Diffuse Synchrotron Emissions

    hep-ph 2026-01 conditional novelty 5.0 of 10

    Galactic synchrotron emissions above 20 MHz can set tighter upper limits on the abundance of primordial black holes with masses above 10^16 grams than previous cosmic-ray electron data.

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