Expanded calculation of weak-interaction-mediated neutrino cooling rates due to 56Ni in stellar matter

@article{Nabi2010ExpandedCO,
  title={Expanded calculation of weak-interaction-mediated neutrino cooling rates due to 56Ni in stellar matter},
  author={Jameel-Un Nabi},
  journal={Physica Scripta},
  year={2010},
  volume={81},
  pages={025901}
}
  • J. Nabi
  • Published 15 January 2010
  • Physics
  • Physica Scripta
An accurate estimate of the neutrino cooling rates is required in order to study the various stages of stellar evolution of massive stars. Neutrino losses from proto-neutron stars play a crucial role in deciding whether these stars would be crushed into black holes or explode as supernovae. Both pure leptonic and weak-interaction processes contribute to the neutrino energy losses in stellar matter. At low temperatures and densities, the characteristics of the early phase of presupernova… 

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