2008/06/04 by Jacco Vink · 2 citations
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Dark Matter and Cosmic Phenomena #Relativity and Gravitational Theory #astro-ph
paper · pdf · doi:10.1051/0004-6361:200809669
To be published as a research note in A & A
openalex publication_date 2008/06/04 · arxiv created 2008/06/26 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/01
Aims. We investigate the shape of the electron cosmic ray spectrum in the range up to ~1000 keV, assuming that the acceleration process at the shock results in a power law in momentum, and that downstream of the shock the spectrum is affected by Coulomb interactions with background electrons only.