Microscopic nuclear equation of state at finite temperature and stellar stability
Hong-Ming Liu, Jing Zhang, Zeng-Hua Li, Jin-Biao Wei, G. F. Burgio, H.-J. Schulze
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.
Topics & Concepts
PhysicsFormalism (music)Neutron starEquation of stateNuclear astrophysicsNuclear matterStability (learning theory)StarsNuclear physicsQuantum electrodynamicsQuantum mechanicsAstrophysicsNucleonArtMusicalVisual artsComputer scienceMachine learningPulsars and Gravitational Waves ResearchHigh-pressure geophysics and materialsNuclear physics research studies