Publication Abstracts

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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BibTeX Citation

  author={Canuto, V. and Fassio-Canuto, L.},
  title={Photoneutrino energy losses in strong magnetic fields},
  journal={Physical Review D},

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RIS Citation

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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