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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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A Modern View of the Equation of State in Nuclear and Neutron Star Matter

TL;DR: In this article, the existence of possible correlations among properties of nuclear matter at saturation density with NS observables was studied and a set of different models that include several phenomenological EOSs based on Skyrme and relativistic mean field models as well as microscopic calculations based on different many-body approaches.
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Thomas–Fermi approximation for β-stable nuclear matter in the Landau Fermi-liquid theory

TL;DR: In this paper, an isentropic description of the equation of state (EOS) for β-stable nuclear matter (BSNM) is presented in a semi-classical mean-field model.
Journal ArticleDOI

Relativistic r modes and shear viscosity: regularizing the continuous spectrum

TL;DR: In this article, the authors derived and solved the perturbation equations of relativistic stars, including the stresses produced by a non-vanishing shear viscosity in the stress-energy tensor.
Journal ArticleDOI

Bounds on the moment of inertia of nonrotating neutron stars

TL;DR: In this article, upper and lower bounds on the moments of inertia of relativistic, spherical, perfect fluid neutron stars assuming that the pressure p and density ϱ are positive and that ( dp dϱ ) is positive.
Journal ArticleDOI

Plausible presence of new state in neutron stars with masses above 0.98MTOV.

TL;DR: In this article , a model-agnostic approach was proposed to investigate the sound speed of a neutron star (NS) by incorporating multi-messenger data of GW170817, PSR J0030+0451, and PSRJ0740+6620.
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