The influence of the Alfvénic drift on the shape of cosmic ray spectra in SNRs
arXiv:0807.2754 · doi:10.1063/1.3076675
Abstract
Cosmic ray acceleration in SNRs in the presence of the Alfvénic drift is considered. It is shown that spectra of accelerated particles may be considerably softer in the presence of amplified magnetic fields.
arXiv comment4 pages, 4 figures, poster talk at 4-th Gamma-ray Symposium (Heidelberg, Germany, 7-11th of July 2008)
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