Publication Abstracts
Canuto and Fassio-Canuto 1973
, and L. Fassio-Canuto, 1973: Pair annihilation into neutrinos in strong magnetic fields. Phys. Rev. D, 7, 1593-1600, doi:10.1103/PhysRevD.7.1593.
The production of a pair of neutrinos via annihilation of an electron and a positron is computed in the presence of a strong magnetic field typical of neutron stars. The results are compared with the zero-field case, and it is shown that the neutrino luminosity QH is greater than Q0 for temperatures up to T ≅ 3×108 K and densities up to 106 g/cm3. For temperatures exceeding T=3.85×108 °K, QH < Q0 at any density. Since it was previously established that electromagnetic losses are systematically losses are systematically enhanced, the thermal history of the star will therefore result from a delicate balance between electromagnetic and neutrino energy losses.
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BibTeX Citation
@article{ca07110b, author={Canuto, V. and Fassio-Canuto, L.}, title={Pair annihilation into neutrinos in strong magnetic fields}, year={1973}, journal={Physical Review D}, volume={7}, pages={1593--1600}, doi={10.1103/PhysRevD.7.1593}, }
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RIS Citation
TY - JOUR ID - ca07110b AU - Canuto, V. AU - Fassio-Canuto, L. PY - 1973 TI - Pair annihilation into neutrinos in strong magnetic fields JA - Phys. Rev. D JO - Physical Review D VL - 7 SP - 1593 EP - 1600 DO - 10.1103/PhysRevD.7.1593 ER -
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