Publication Abstracts
Canuto and Fassio-Canuto 1973
, 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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BibTeX Citation
@article{ca09110u, author={Canuto, V. and Fassio-Canuto, L.}, title={Photoneutrino energy losses in strong magnetic fields}, year={1973}, journal={Physical Review D}, volume={7}, pages={1601--1608}, doi={10.1103/PhysRevD.7.1601}, }
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RIS Citation
TY - JOUR ID - ca09110u AU - Canuto, V. AU - Fassio-Canuto, L. PY - 1973 TI - Photoneutrino energy losses in strong magnetic fields JA - Phys. Rev. D JO - Physical Review D VL - 7 SP - 1601 EP - 1608 DO - 10.1103/PhysRevD.7.1601 ER -
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