Abstract
A microscopic nuclear equation of state compatible with all current astrophysical constraints constructed within the Brueckner-Hartree-Fock formalism is presented and extended in a consistent way to finite temperature. The effects of finite temperature on the properties of neutron stars are studied in detail and a universal relation regarding stellar stability is proposed.
- Received 6 May 2022
- Accepted 20 July 2022
DOI:https://doi.org/10.1103/PhysRevC.106.025801
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