General Relativistic Hartree-Fock Calculations for Neutron Star

Fuente: arXiv
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Main Author: Onishi, Naoki
Format: Preprint
Published: 2024
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author Onishi, Naoki
author_facet Onishi, Naoki
contents We investigate the global structures of neutron stars within the framework of general relativity, treating the entire star as a quantum-degenerate system. Rather than relying on the Tolman-Oppenheimer-Volkoff (TOV) equation, we solve the Einstein-Cartan (EC) field equations self-consistently, incorporating the energy-momentum tensor contributions from neutrons. Neutron wave functions are obtained by solving the Dirac equation in a curved spacetime with both torsion and curvature effects. Given that neutron stars contain about 10^57 particles, we adopt a scaled h-bar approach to efficiently describe the quantum state of highly degenerate system.
format Preprint
id arxiv_https___arxiv_org_abs_2412_02990
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle General Relativistic Hartree-Fock Calculations for Neutron Star
Onishi, Naoki
General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
Nuclear Theory
We investigate the global structures of neutron stars within the framework of general relativity, treating the entire star as a quantum-degenerate system. Rather than relying on the Tolman-Oppenheimer-Volkoff (TOV) equation, we solve the Einstein-Cartan (EC) field equations self-consistently, incorporating the energy-momentum tensor contributions from neutrons. Neutron wave functions are obtained by solving the Dirac equation in a curved spacetime with both torsion and curvature effects. Given that neutron stars contain about 10^57 particles, we adopt a scaled h-bar approach to efficiently describe the quantum state of highly degenerate system.
title General Relativistic Hartree-Fock Calculations for Neutron Star
topic General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
Nuclear Theory
url https://arxiv.org/abs/2412.02990