Heterogeneity of solid neutron‐star matter: transport coefficients and neutrino emissivity

@article{Jones2004HeterogeneityOS,
  title={Heterogeneity of solid neutron‐star matter: transport coefficients and neutrino emissivity},
  author={P. B. Jones},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2004},
  volume={351},
  pages={956-966}
}
  • P. B. Jones
  • Published 2004
  • Physics
  • Monthly Notices of the Royal Astronomical Society
Calculations of weak-interaction transition rates and of nuclear formation enthalpies show that in isolated neutron stars, the solid phase, above the neutron-drip threshold, is amorphous and heterogeneous in nuclear charge. The neutrino emissivities obtained are very dependent on the effects of proton shell structure but may be several orders of magnitude larger than the electron bremsstrahlung neutrino pair emissivity at temperatures ∼10 9 K. In this phase, electrical and thermal… Expand

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