Canuto and Fassio-Canuto 1973
Canuto, V., and L. Fassio-Canuto, 1973: Photoneutrino energy losses in strong magnetic fields. Phys. Rev. D, 7, 1601-1608, doi:10.1103/PhysRevD.7.1601.
The energy losses by photoneutrinos is computed in the presence of a magnetic field of 1013 G, typical of neutron stars. Plasma effects are not included. The results indicate that for T ≥ 108 °K and densities ρ ≥ 104 g/cm3, the presence of a strong H field decreases the energy losses by at the most a factor between ten and a hundred in the region up to ρ ≃ 106 g/cm3. At higher densities the neutrino emissivities are almost identical. These effects are temperature-dependent and they are less and less pronounced when T ≥ 5×108 °K.
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Canuto, V., and Fassio-Canuto, L.: Photoneutrino energy losses in strong magnetic fields, Phys. Rev. D, 7, 1601-1608, doi:10.1103/PhysRevD.7.1601, 1973.
Canuto, V., and L. Fassio-Canuto (1973), Photoneutrino energy losses in strong magnetic fields, Phys. Rev. D, 7, 1601-1608, doi:10.1103/PhysRevD.7.1601.
Canuto, V., and L. Fassio-Canuto, 1973: Photoneutrino energy losses in strong magnetic fields. Phys. Rev. D, 7, 1601-1608, doi:10.1103/PhysRevD.7.1601.
Canuto, V., & Fassio-Canuto, L. 1973, Phys. Rev. D, 7, 1601, doi:10.1103/PhysRevD.7.1601.
Canuto V, Fassio-Canuto L. Photoneutrino energy losses in strong magnetic fields, Phys Rev D 1973;7:1601-1608. doi:10.1103/PhysRevD.7.1601.
V. Canuto, L. Fassio-Canuto, Phys. Rev. D 7, 1601-1608, doi:10.1103/PhysRevD.7.1601 (1973).
