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Journal ArticleDOI

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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Bayesian inference of the dense-matter equation of state encapsulating a first-order hadron-quark phase transition from observables of canonical neutron stars

TL;DR: In this article, the posterior probability distribution functions (PDFs) and correlations of nine parameters characterizing the EOS of dense neutron-rich matter encapsulating a first-order hadron-quark phase transition from the radius data of canonical NSs reported by LIGO/VIRGO, NICER, and Chandra Collaborations.
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Attributes of a rotating neutron star with a hyperon core

TL;DR: In this article, the authors studied the effect of rotation on the global properties of a rotating compact star with a hyperon core in an effective chiral model with varying nucleon effective masses within a mean field approach.
Journal ArticleDOI

Magnetars versus Radio Pulsars: MHD Stability in Newborn Highly Magnetized Neutron Stars

TL;DR: In this paper, the stability/establishment of dipolar magnetostatic equilibrium configurations in new-born neutron stars (NSs) in dependence on the rotational velocity and on the initial angle between rotation and magnetic axis was studied.
Journal ArticleDOI

The Equation of State of Nuclear Matter: From Finite Nuclei to Neutron Stars

G. Fiorella Burgio, +1 more
- 08 Jul 2020 - 
TL;DR: In this article, the authors examined a large set of nuclear equations of state based on phenomenological models (Skyrme, NLWM, DDM) and ab initio theoretical methods (BBG, Dirac-Brueckner, Variational, Quantum Monte Carlo).
Journal ArticleDOI

Symmetry energy, neutron skin, and neutron star radius from chiral effective field theory interactions

TL;DR: In this article, the authors discuss neutron matter calculations based on chiral eective eld theory interactions and their predictions for the symmetry energy, the neutron skin of 208 Pb, and for the radius of neutron stars.
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