Neutrino-pair emission due to electron-phonon scattering in a neutron star crust

@inproceedings{Yakovlev1996NeutrinopairED,
  title={Neutrino-pair emission due to electron-phonon scattering in a neutron star crust},
  author={Dmitry G. Yakovlev and Alexander Kaminker and Ioffe},
  year={1996}
}
Neutrino-pair bremsstrahlung radiation is considered due to electron–phonon scattering of degenerate, relativistic electrons in a lattice of spherical atomic nuclei in a neutron star crust. The neutrino energy generation rate is calculated taking into account exact spectrum of phonons, the Debye–Waller factor, and the nuclear form–factor in the density… CONTINUE READING