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Dependence of the gamma-ray emission from SN 1006 on the astronomical parameters
L. T. Ksenofontov, E. G. Berezhko, H. J. Voelk
We use nonlinear kinetic theory to study the remnant dynamics and the particle acceleration as well as the properties of the nonthermal emission from the supernova remnant SN 1006.…
Confirmation of strong magnetic field amplification and nuclear cosmic ray acceleration in SN 1006
E. G. Berezhko, L. T. Ksenofontov, H. J. Voelk
It is shown that the nonlinear kinetic model of cosmic ray (CR) acceleration in supernova remnants (SNRs) fits the shell-type nonthermal X-ray morphology, obtained in Chandra obser…
Cosmic ray production in supernova remnants including reacceleration: the secondary to primary ratio
E. G. Berezhko, L. T. Ksenofontov, V. S. Ptuskin +2
We study the production of cosmic rays (CRs) in supernova remnants (SNRs), including the reacceleration of background galactic cosmic rays (GCRs) - thus refining the early consider…