학술논문
Role of the radiative stage for cosmic ray acceleration in SNRs
Document Type
Working Paper
Author
Source
Subject
Language
Abstract
We consider diffusive shock acceleration in supernova remnants throughout their evolution including a radiative stage. It is found that a more efficient acceleration and fast exit of particles at the radiative stage results in the hardening of the source cosmic ray proton and electron spectra at energies $\sim 100-500$ GeV. The effect is stronger for cosmic ray electrons.
Comment: 8 pages, 8 figures, accepted to MNRAS. arXiv admin note: text overlap with arXiv:1701.00844
Comment: 8 pages, 8 figures, accepted to MNRAS. arXiv admin note: text overlap with arXiv:1701.00844