Role of Ejecta Clumping and Back-reaction of Accelerated Cosmic Rays in the Evolution of Type Ia Supernova Remnants

@article{Orlando2012RoleOE,
  title={Role of Ejecta Clumping and Back-reaction of Accelerated Cosmic Rays in the Evolution of Type Ia Supernova Remnants},
  author={Salvatore Orlando and Fabrizio Bocchino and Marco Miceli and O Petruk and Maria Letizia Pumo},
  journal={The Astrophysical Journal},
  year={2012},
  volume={749},
  pages={156}
}
We investigate the role played by initial clumping of ejecta and by efficient acceleration of cosmic rays (CRs) in determining the density structure of the post-shock region of a Type Ia supernova remnant (SNR) through detailed three-dimensional MHD modeling. Our model describes the expansion of an SNR through a magnetized interstellar medium, including the initial clumping of ejecta and the effects on shock dynamics due to back-reaction of accelerated CRs. The model predictions are compared to… 

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