Evolution of cosmic ray electron spectra in magnetohydrodynamical simulations
Evolution of cosmic ray electron spectra in magnetohydrodynamical simulations
Cosmic ray (CR) electrons reveal key insights into the non-thermal physics of the interstellar medium, galaxies, galaxy clusters, and active galactic nuclei by means of their inverse Compton {\gamma}-ray emission and synchrotron emission in magnetic fields. While magnetohydrodynamical (MHD) simulations with CR protons capture their dynamical impact on these systems, …