Chou et al. 1978
Chou, C.K., L. Fassio-Canuto, and V. Vanuto, 1978: 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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Chou, C.K., Fassio-Canuto, L., and Vanuto, V.: Photoneutrino reactions in a superstrong magnetoactive plasma, Astrophys. J., 227, 974-986, doi:10.1086/156806, 1978.
Chou, C.K., L. Fassio-Canuto, and V. Vanuto (1978), Photoneutrino reactions in a superstrong magnetoactive plasma, Astrophys. J., 227, 974-986, doi:10.1086/156806.
Chou, C.K., L. Fassio-Canuto, and V. Vanuto, 1978: Photoneutrino reactions in a superstrong magnetoactive plasma. Astrophys. J., 227, 974-986, doi:10.1086/156806.
Chou, C.K., Fassio-Canuto, L., & Vanuto, V. 1978, Astrophys. J., 227, 974, doi:10.1086/156806.
Chou CK, Fassio-Canuto L, Vanuto V. Photoneutrino reactions in a superstrong magnetoactive plasma, Astrophys J 1978;227:974-986. doi:10.1086/156806.
C.K. Chou, L. Fassio-Canuto, V. Vanuto, Astrophys. J. 227, 974-986, doi:10.1086/156806 (1978).
