arXiv Analytics

Sign in

arXiv:2307.11640 [astro-ph.HE]AbstractReferencesReviewsResources

Charged particles in magnetic fields and cosmic ray transport

Pasquale Blasi

Published 2023-07-21Version 1

The theory of transport of charged particles in cosmic magnetic fields is at the very center of the investigation of non-thermal phenomena in the universe, ranging from our local neighborhood to supernovae, clusters of galaxies or distant active galaxies. It is crucial to understand how particles get energized to non-thermal energies as well as to describe their motion from the sources to an observer or to another location in the universe. Here I summarize some essential, basic aspects of the theory and discuss some topics in the theoretical framework that are currently being developed. I will also discuss some simple applications of the theory of transport to particle acceleration and propagation in the Galaxy.

Comments: 51 Pages, to appear in "Foundations of Cosmic Ray Astrophysics", Proceedings of the International School of Physics "Enrico Fermi", Course 208, Varenna, 24-29 June 2022, edited by F. Aharonian, E. Amato, and P. Blasi
Categories: astro-ph.HE
Related articles: Most relevant | Search more
arXiv:2101.07759 [astro-ph.HE] (Published 2021-01-19)
Cosmic Ray transport in mixed magnetic fields and their role on the observed anisotropies
arXiv:1812.01996 [astro-ph.HE] (Published 2018-12-05)
Cosmic ray transport and radiative processes in nuclei of starburst galaxies
arXiv:1712.07117 [astro-ph.HE] (Published 2017-12-18)
A New Numerical Scheme for Cosmic Ray Transport