General Relativistic Augmentation of Neutrino Pair Annihilation Energy Deposition Near Neutron Stars

2); (2) University of Calivornia; Davis); James R. Wilson (1) ((1) Lawrence Livermore National Laboratory; Jay D. Salmonson (1

General Relativistic Augmentation of Neutrino Pair Annihilation Energy Deposition Near Neutron Stars

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arxiv astro-ph/9908017 v1 pith:M5ZH3RXR submitted 1999-08-03 astro-ph

General Relativistic Augmentation of Neutrino Pair Annihilation Energy Deposition Near Neutron Stars

Jay D. Salmonson (1 , 2) , James R. Wilson (1) ((1) Lawrence Livermore National Laboratory , (2) University of Calivornia , Davis) This is my paper

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General relativistic calculations are made of neutrino-antineutrino annihilation into electron-positron pairs near the surface of a neutron star. It is found that the efficiency of this process is enhanced over the Newtonian values up to a factor of more than 4 in the regime applicable to Type II supernovae and by up to a factor of 30 for collapsing neutron stars.

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Scattering, Hawking Radiation and Neutrino Energy Deposition in Euler-Heisenberg Black Holes Surrounded by Perfect Fluid Dark Matter
gr-qc 2026-06 unverdicted novelty 5.0

Computes quasinormal modes via 13th-order WKB with Padé, greybody factors by numerical integration, and Hawking/neutrino spectra for Euler-Heisenberg plus perfect fluid dark matter black holes, finding PFDM increases ...