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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Nuclear constraints on properties of neutron star crusts
TL;DR: In this paper, the transition density and pressure at the inner edge separating the liquid core from the solid crust of neutron stars are systematically studied using a modified Gogny (MDI) and 47 popular Skyrme interactions within well established dynamical and thermodynamical methods.
Journal ArticleDOI
Crystallization of the inner crust of a neutron star and the influence of shell effects
TL;DR: In this article, the effect of the different nuclear ingredients with their associated uncertainties separately: the nuclear equation of state, the surface properties in the presence of a uniform gas of dripped neutrons, and the proton shell effects arising from the ion single-particle structure.
Journal ArticleDOI
Nuclear superfluidity and cooling time of neutron stars
TL;DR: In this article, the nuclear superfluidity affects the thermal response of the inner crust of a neutron star in the case of a rapid cooling process, and two pairing scenarios are proposed: one corresponding to the BCS approximation and the other to many-body techniques including polarisation effects.
Journal ArticleDOI
Hadron matter in neutron stars in view of gravitational wave observations.
TL;DR: In this paper, the authors highlight a few physical properties of neutron stars and their theoretical treatment inasmuch as they can be useful for nuclear and particle physicists concerned with matter at finite density (and newly, temperature).
Journal ArticleDOI
Ruling out the supersoft high-density symmetry energy from the discovery of PSR J0740+6620 with mass $2.14^{+0.10}_{-0.09}M_\odot$
Ying Zhou,Lie-Wen Chen +1 more
TL;DR: In this paper, the authors show that the symmetry energy cannot supersoft so that it becomes negative at suprasaturation densities in neutron stars (NSs) and thus may make the NS have a pure neutron matter core, which is in contrast to the fact that using the mass $2.04 M_\odot$ of PSR J0348+0432 as the NS maximum mass cannot rule out the supersoft high-density $E_{\rm sym}(n)$.
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