Rayleigh–Taylor instabilities in Type Ia supernova remnants undergoing cosmic ray particle acceleration – low adiabatic index solutions

@article{Wang2011RayleighTaylorII,
  title={Rayleigh–Taylor instabilities in Type Ia supernova remnants undergoing cosmic ray particle acceleration – low adiabatic index solutions},
  author={Chih-Yueh Wang},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2011},
  volume={415},
  pages={83-92}
}
  • Chih-Yueh Wang
  • Published 13 November 2010
  • Physics
  • Monthly Notices of the Royal Astronomical Society
This study investigates the evolution of Rayleigh-Taylor (R-T) instabilities in Type Ia supernova remnants that are associated with a low adiabatic index γ, where γ < 5/3, which reflects the expected change in the supernova shock structure as a result of cosmic ray particle acceleration. Extreme cases, such as the case with the maximum compression ratio that corresponds to γ = 1.1, are examined. As γ decreases, the shock compression ratio rises, and an increasingly narrow intershock region with… 
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