Journal ArticleDOI
The Ground state of matter at high densities: Equation of state and stellar models
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This article is published in The Astrophysical Journal.The article was published on 1971-01-01. It has received 1314 citations till now. The article focuses on the topics: Ground state & Equation of state.read more
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Proceedings ArticleDOI
Applicability of Relativistic Point-Coupling Models to Neutron Star Physics
TL;DR: In this paper, the relativistic point-coupling models with the zero-range contact interaction are used to establish nuclear equation of state (EoS) and investigate neutron star properties.
Journal ArticleDOI
Unified neutron star EOSs and neutron star structures in RMF models
TL;DR: In this paper , the Thomas-Fermi approximation of the EOSs and microscopic structures of neutron star matter in a vast density range with n b ≈ 10−10-2 fm−3, where various covariant density functionals are adopted, i.e., those with nonlinear self couplings (NL3, PK1, TM1, GM1, MTVTC) and density-dependent coupling (DD-LZ1, DDME-X, PKDD, DD-ME2, DD2, TW99).
Journal ArticleDOI
Neutron Star Physics and EOS
TL;DR: In this paper, it was shown that measurements of the masses and radii of neutron stars can constrain the nuclear matter symmetry energy, which controls the neutron star matter pressure and the interior composition and will influence the interpretation of nuclear experiments.
Journal ArticleDOI
Hadron-Quark phase transition in the context of GW190814
TL;DR: In this article, the properties of the neutron stars were calculated for the hadronic matter within the density-dependent relativistic mean-field model (DD-RMF), and the phase transition to the quark matter was studied and the hybrid star matter properties were systematically calculated using the Vector-Enhanced Bag model (vBag).
Journal ArticleDOI
Proton branch of modified urca process in strong magnetic field and superfluidity of neutron star cores
TL;DR: In this article, the effects of strong magnetic field and superfluidity on the proton branch of the modified URCA process were investigated simultaneously, and it was shown that strong magnetic fields enhanced the neutrino emissivities compared to the case in zero magnetic field, and the superfluidity reduced the emissivity significantly.
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