Gamma-ray emission expected from Kepler's SNR

@inproceedings{EGBerezhko2006GammarayEE,
  title={Gamma-ray emission expected from Kepler's SNR},
  author={E.G.Berezhko and L.T.Ksenofontov and H.J.Voelk},
  year={2006}
}
Nonlinear kinetic theory of cosmic ray (CR) acceleration in supernova remnants (SNRs) is used to investigate the properties of Kepler's SNR and, in particular, to predict the gamma-ray spectrum expected from this SNR. Observations of the nonthermal radio and X-ray emission spectra as well as theoretical constraints for the total supernova (SN) explosion energy E_sn are used to constrain the astronomical and particle acceleration parameters of the system. Under the assumption that Kepler's SN is… Expand