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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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Pasta properties of the neutron star within effective relativistic mean-field model

TL;DR: In this article , the properties of pasta structures and their influence on the neutron star observables employing the effective relativistic mean-based (E-RMF) model were investigated.
Journal ArticleDOI

Computing Differentially Rotating Neutron Stars Obeying Realistic Equations of State by Using Hartle’s Perturbation Method

TL;DR: In this paper, the Hartle's perturbation method was used to compute models of differentially rotating neutron stars obeying realistic equations of state, where terms up to third order in the angular velocity were kept.
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Bayesian inference of neutron-star observables based on effective nuclear interactions

TL;DR: In this paper , the authors studied the constraints on the parameters of the nuclear matter equation of state (EOS) from adopted astrophysical observables using a Bayesian approach, and obtained a robust constraint on nuclear matter EOS, and meanwhile, understand the model dependence of the results.
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Constraining nuclear matter parameters from correlation systematics: a mean-field perspective

TL;DR: In this paper, the lower order nuclear matter parameters such as the binding energy per nucleon, incompressibility and symmetry energy coefficients are found to be constrained in narrow limits through their strong ties with selective properties of finite nuclei.
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SGRs/AXPs as Rotation-Powered Neutron Stars

TL;DR: In this paper, it was shown that nine soft gamma repeaters and anomalous X-ray Pulsars (AXPs) of the twenty three known sources can be described as rotation-powered canonical pulsars.
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