Vela as the Source of Galactic Cosmic Rays above 100 TeV
M. Bouyahiaoui*, M. Kachelriess and D. Semikoz
Pre-published on:
July 22, 2019
Published on:
July 02, 2021
Abstract
We modeled the contribution of the young supernova remant Vela to the local cosmic rays taking into account the effect of the Local superBubble and an anistropic diffusion. We recovered the knee observed in the CR spectrum at energy of 3-5 PeV. By the contribution of Vela and an older local source of 2-3 Myr supernova we were able to explain the CR spectrum from TeV to 100 PeV.
DOI: https://doi.org/10.22323/1.358.0039
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