Neutronization and the Physics of Quasi-equilibrium

  • Raphael Hix
  • Published 1995

Abstract

As the ultimate stage of stellar nucleosynthesis, and the source of the iron peak nuclei, silicon burning is important to our understanding of the evolution of massive stars and supernovae. Our reexamination of silicon burning, using results gleaned from simulation work done with a large nuclear network (299 nuclei and more than 3000 reactions) and from… (More)

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Cite this paper

@inproceedings{Hix1995NeutronizationAT, title={Neutronization and the Physics of Quasi-equilibrium}, author={Raphael Hix}, year={1995} }