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The Ground state of matter at high densities: Equation of state and stellar models

Gordon Baym, +2 more
- 01 Jan 1971 - 
- Vol. 170, pp 299-317
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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.

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New equations of state constrained by nuclear physics, observations, and QCD calculations of high-density nuclear matter

TL;DR: In this paper, an effective mass parametrization was proposed for core-collapse supernova and neutron star merger simulations. But the parameter range of the energy-density functional underlying the equation of state is constrained by chiral effective field theory results at nuclear densities as well as by functional renormalization group computations at high densities based on QCD.
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Neutron stars, β -stable ring-diagram equation of state, and Brown-Rho scaling

TL;DR: In this article, the authors used the ring-diagram equation of state (EOS) obtained from realistic low-momentum interactions to calculate the neutron star properties, such as mass, radius, and moment of inertia.
Journal ArticleDOI

Effects of nuclear symmetry energy and equation of state on neutron star properties

TL;DR: In this paper, the effects of nuclear symmetry energy on the mass-radius relation and tidal deformability of neutron stars, considering the self-consistency of the equation of state (EOS), were investigated.
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Constraints on the maximum mass of neutron stars with a quark core from GW170817 and NICER PSR J0030+0451 data

TL;DR: In this article, the authors performed a Bayesian analysis of the maximum mass of a binary neutron star with a quark core, incorporating the observational data from tidal deformability of the GW170817 binary Neutron Star merger as detected by LIGO/Virgo and the mass and radius of PSR J0030+0451.
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