Massive Stars and their Supernovae

@article{Thielemann2011MassiveSA,
  title={Massive Stars and their Supernovae},
  author={Friedrich-Karl Thielemann and R. Hirschi and M. Liebendorfer and R. Diehl},
  journal={Lecture Notes in Physics},
  year={2011},
  volume={812},
  pages={153-231}
}
  • Friedrich-Karl Thielemann, R. Hirschi, +1 author R. Diehl
  • Published 2011
  • Physics
  • Lecture Notes in Physics
  • Our understanding of stellar evolution and the final explosive endpoints such as supernovae or hypernovae or gamma-ray bursts relies on the combination of (a) (magneto-)hydrodynamics, (b) energy generation due to nuclear reactions accomanying composition changes, (c) radiation transport, (d) thermodynamic properties (such as the equation of state of stellar matter). 
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