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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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Axisymmetric toroidal modes of general relativistic magnetized neutron star models

TL;DR: In this article, the axisymmetric toroidal modes of magnetized neutron stars with a solid crust were calculated in the general relativistic Cowling approximation, assuming that the interior of the star is threaded by a poloidal magnetic field, which is continuous at the surface with an outside dipole field.
Journal ArticleDOI

Hadron-Quark Crossover and Hot Neutron Stars at Birth

TL;DR: In this article, a new isentropic equation of state (EOS) at finite temperature "CRover" was constructed on the basis of the hadron-quark crossover at high density.
Journal ArticleDOI

Quark Stars as inner engines for Gamma Ray Bursts

TL;DR: In this article, a model for Gamma ray bursts inner engine based on quark stars is presented, which is capable of reproducing crucial features of gamma ray bursts, such as the episodic activity of the engine (multiple and random shell emission) and the two distinct categories of the bursts (two regimes are isolated in the model with two distinct regimes of the burst duration).
Journal ArticleDOI

The structure of cold neutron star with a quark core within the MIT and NJL models

TL;DR: In this article, the authors used two models for describing EOS of quark matter, namely, the NJL and MIT bag models, and employed three approaches in this work to compute the equation of state of these parts of neutron star to evaluate its structure properties.
Journal ArticleDOI

Chiral Restoration of Nucleons in Neutron Star Matter: Studies Based on a Parity Doublet Model

TL;DR: In this article , a model of linear realization of chiral symmetry with the nucleon parity doublet structure that permits the chiral invariant mass, m 0, for positive and negative parity nucleons, was considered.
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