3 papers
astro-ph.HE2021
Magneto-hydrodynamic simulations of young supernova remnants and their energy-conversion phase
O. Petruk, T. Kuzyo, S. Orlando +2
Supernova remnants (SNRs) can be rich sources of information on the parent SN explosion. Thus investigating the transition from the phase of SN to that of SNR can be crucial to lin…
astro-ph.HE2019
Cosmic-ray acceleration and escape from post-adiabatic Supernova remnants
Robert Brose, Martin Pohl, Iurii Sushch +2
Supernova remnants are known to accelerate cosmic rays on account of their non-thermal emission of radio waves, X-rays, and gamma rays. Although there are many models for the accel…
astro-ph.HE2018
Post-adiabatic supernova remnants in an interstellar magnetic field: oblique shocks and non-uniform environment
O. Petruk, T. Kuzyo, S. Orlando +5
We present very-high-resolution 1D MHD simulations of the late-stage supernova remnants (SNR). In the post-adiabatic stage the magnetic field has an important and significant dynam…