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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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Extreme relativistic model for neutron stars and pulsars

TL;DR: In this paper, it was shown that for pulsationally stable configurations the surface to central density ratio is greater than 0.30, the maximum values for surface and central redshifts are 0.85 and 3.40 respectively in the extreme case, and the maximum mass and size are respectively 4.8M and 20.1 km.
Journal ArticleDOI

Properties of static limit and rotating equilibrium sequences of compact stars: Systematic correlations and constraints

TL;DR: In this article, the properties of nonrotating and rapidly rotating configurations of compact stars (CS) by employing a representative set of equations of state (EOSs) were investigated.
Journal ArticleDOI

Variational Method for Infinite Nuclear Matter with Noncentral Forces

TL;DR: In this article, an effective theory is proposed by introducing a density-dependent modification of the noncentral part of the energy expression to suppress the long tails of noncentral distribution functions.
Journal ArticleDOI

Slowly rotating neutron stars and hadronic stars in the chiral SU(3) quark mean-field model

TL;DR: In this paper, the equations of state for neutron matter, strange and nonstrange hadronic matter in the chiral SU(3) quark mean-field model are applied in the study of slowly rotating neutron stars and hadronic stars.
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