Publication Abstracts

Chou et al. 1979

Chou, C.K., L. Fassio-Canuto, and V. Canuto, 1979: Photoneutrino reactions in a superstrong magnetoactive plasma. Astrophys. J., 227, 974-986, doi:10.1086/156806.

The neutrino luminosity due to the photoneutrino process in the presence of a superstrong magnetoactive electron plasma appropriate for neutron stars is computed. The results indicate that for relatively low temperatures, between 108 ≲ T < 5×108 K the energy loss rate is significantly reduced both in the low-density regime ρ ≲ 107 g/cm3 (by the magnetic field) and in the high-density regime ρ ≳ 107 g/cm3 (by plasmon excitations). These effects are temperature dependent, and they are less pronounced when the temperature is in the range from 5×108 ≤ T ≤ 109 K.

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BibTeX Citation

@article{ch06500y,
  author={Chou, C. K. and Fassio-Canuto, L. and Canuto, V.},
  title={Photoneutrino reactions in a superstrong magnetoactive plasma},
  year={1979},
  journal={Astrophys. J.},
  volume={227},
  pages={974--986},
  doi={10.1086/156806},
}

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RIS Citation

TY  - JOUR
ID  - ch06500y
AU  - Chou, C. K.
AU  - Fassio-Canuto, L.
AU  - Canuto, V.
PY  - 1979
TI  - Photoneutrino reactions in a superstrong magnetoactive plasma
JA  - Astrophys. J.
VL  - 227
SP  - 974
EP  - 986
DO  - 10.1086/156806
ER  -

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