Collisionless Shock 5

[HEDS12-01(Invited)] PeV Cosmic Ray Acceleration in the Supernova Blast Wave: Kinetic-magnetohydrodynamic Simulations

*Tsuyoshi Inoue¹ (1. Konan University)

Supernova remnants are believed to be the accelerators of cosmic-rays up to PeV. In this work, using a novel method developed by Inoue (2009), we show that cosmic-ray streaming instability mediated acceleration successfully energize cosmic-rays more than PeV at the supernova shock propagating in the dense circum stellar medium.