Propagation of Cosmic Rays and their Secondaries in the Intracluster Medium
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Pre-published on:
July 22, 2019
Published on:
July 02, 2021
Abstract
We present results of the propagation of high-energy cosmic rays (CRs) in the intracluster medium (ICM). To this end, we employ three-dimensional cosmological magnetohydrodynamical simulations of the turbulent intergalactic medium to explore the propagation of CRs with energies between $10^{14}$ and $10^{19}$ eV. We study the interaction of test particles with this environment and compute the associated fluxes of CRs and neutrinos using a Monte Carlo simulations.
DOI: https://doi.org/10.22323/1.358.0081
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.