PoS - Proceedings of Science
Volume 358 - 36th International Cosmic Ray Conference (ICRC2019) - CRD - Cosmic Ray Direct
Core-collapse Supernovae as Cosmic Ray Sources
V. Dwarkadas*, A. Marcowith, M. Renaud, V. Tatischeff and G. Giacinti
Full text: pdf
Pre-published on: July 22, 2019
Published on: July 02, 2021
Core-collapse supernovae produce fast shocks which expand into the dense circumstellar medium (CSM) of the stellar progenitor. Cosmic rays (CRs) accelerated at these shocks can induce the growth of electromagnetic fluctuations in the pre-shock medium. Using a self-similar description for the shock evolution, we calculate the growth time-scales of CR driven instabilities for SNe in general, and SN 1993J in particular. We find that extended SN shocks can trigger fast intra-day instabilities, strong magnetic field amplification, and CR acceleration. In particular, the non-resonant streaming instability can contribute to about 50 per cent of the magnetic field intensity deduced from radio data. This results in the acceleration of CR particles to energies of 1-10 PeV within a few days after the shock breakout.
DOI: https://doi.org/10.22323/1.358.0065
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