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Hot neutron stars with microscopic equations of state

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arxiv 1907.03120 v1 pith:DDGYNVV2 submitted 2019-07-06 nucl-th astro-ph.HEastro-ph.SR

Jia-Jing Lu , Zeng-Hua Li , G. F. Burgio , H.-J Schulze This is my paper · ORCID
classification nucl-thastro-ph.HEastro-ph.SR
keywords equationsstatetemperatureneutronpropertiesstarsaccurateanalyze
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We study the properties of hot beta-stable nuclear matter using equations of state derived within the Brueckner-Hartree-Fock approach at finite temperature including consistent three-body forces. Simple and accurate parametrizations of the finite-temperature equations of state are provided. The properties of hot neutron stars are then investigated within this framework, in particular the temperature dependence of the maximum mass. We find very small temperature effects and analyze the interplay of the different contributions.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Supernova Remnants with Mirror Dark Matter and Hyperons

    hep-ph 2024-12 conditional novelty 6.0 of 10

    Mirror dark matter inside proto-neutron stars reduces maximum mass, radius, and tidal deformability while heating the remnant and raising the speed of sound.

  2. Setting nonperturbative uncertainties on finite-temperature properties of neutron matter

    nucl-th 2019-08 conditional novelty 6.0 of 10

    First-principles finite-temperature neutron matter calculations are combined into an uncertainty band covering interaction, many-body, and thermodynamic uncertainties.

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