Collisionless Shock 3

[HEDS3-06] Cosmic-ray acceleration and maximum energy in a supernova remnant shock propagating in a stellar wind with a wind termination shock

*Shoma F. Kamijima¹, Yutaka Ohira² (1. Yukawa Institute for Theoretical Physics, Kyoto University, 2. The University of Tokyo)

We performed global test particle simulations for cosmic-ray acceleration in core-collapse supernova remnants(SNRs) propagating in the stellar wind and found the cyclic motion between the SNR and wind termination shock, leading to increasing particle energy.