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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Sensitivity of the Moment of Inertia of Neutron Stars to the Equation of State of Neutron-Rich Matter
TL;DR: In this paper, the sensitivity of the stellar moment of inertia to the neutron-star matter equation of state is examined using accurately calibrated relativistic mean-field models, and it is shown that constraining the density dependence of the symmetry energy -through, for example, the measurement of the neutron skin thickness in {sup 208}Pb - will place no significant bound on either the transition pressure or the crustal moment of gravity.
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Astrophysical Constraints on Dense Matter in Neutron Stars
TL;DR: In this paper, the current status of constraints from various methods and the prospects for future improvements are reviewed, as well as a review of the current state of the art and the future improvements.
Journal ArticleDOI
Semi-classical equation of state and specific-heat expressions with proton shell corrections for the inner crust of a neutron star
TL;DR: In this article, an approach to the inner crust of neutron stars based on Skyrme-type forces is presented, where the energy is calculated by the TETF (temperature-dependent extended Thomas-Fermi) method, with proton shell corrections added self-consistently by the Strutinsky-integral method.
Journal ArticleDOI
Relativistic Feynman-Metropolis-Teller theory for white dwarfs in general relativity
TL;DR: In this paper, the relativistic Thomas-Fermi model within the Feynman-Metropolis-Teller theory for compressed atoms is applied to the study of general relatievistic white dwarf equilibrium configurations.
Journal ArticleDOI
A new equation of state for neutron star matter with nuclei in the crust and hyperons in the core
TL;DR: In this paper, the chiral quark-meson coupling model within relativistic Hartree-Fock approximation is adopted for uniform nuclear matter and the coupling constants are determined so as to reproduce the experimental data of atomic nuclei and hypernuclei.
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