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Properties of rapidly rotating hot neutron stars within Brueckner theory
Abstract
We study the properties of hot rapidly rotating neutron stars using various equations of state based on the Brueckner-Hartree-Fock approach at finite temperature. The temperature dependence of gravitational mass, equatorial radius, Kepler frequency, moment of inertia are analysed in detail and universal relations are examined.
Versions
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BibTeX
@misc{liu2026properties,
title = {{Properties of rapidly rotating hot neutron stars within Brueckner theory}},
author = {Hong-Ming Liu and Bo-Xiu Zhou and Zeng-Hua Li and Jin-Biao Wei and H. -J. Schulze},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2610.01577},
eprint = {2610.01577},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2610.01577},
}
RIS
TY - UNPB
TI - Properties of rapidly rotating hot neutron stars within Brueckner theory
AU - Hong-Ming Liu
AU - Bo-Xiu Zhou
AU - Zeng-Hua Li
AU - Jin-Biao Wei
AU - H. -J. Schulze
PY - 2026
DA - 2026/10/01
PB - arXiv
DO - 10.48550/arxiv.2610.01577
UR - https://arxiv.org/abs/2610.01577
AB - We study the properties of hot rapidly rotating neutron stars using various equations of state based on the Brueckner-Hartree-Fock approach at finite temperature. The temperature dependence of gravitational mass, equatorial radius, Kepler frequency, moment of inertia are analysed in detail and universal relations are examined.
ER -