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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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Moment of inertia of neutron star crust in alternative and modified theories of gravity

TL;DR: In this paper, the authors calculate the ratio of the crustal to the total moment of inertia of neutron stars in the scalar-tensor theory of gravity and the nonperturbative gravity model.
Journal ArticleDOI

Periodic box Fermi hypernetted chain calculations of neutron star crustal matter

TL;DR: In this paper, the authors extended the periodic box Fermi hypernetted chain method to include longitudinal-isospin dependence of the correlations, making feasible a study of asymmetric crustal matter.
Journal ArticleDOI

The Equation of state of dense skyrmion matter

T.S. Walhout
- 17 Dec 1990 - 
TL;DR: In this article, a face-centered cubic lattice of skyrmions is used to construct the equation of state for dense neutron matter, and the implications for neutron star structure are discussed, and comparisons are made with previous calculations.
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Static and rotating neutron stars fulfilling all fundamental interactions

TL;DR: In this paper, the key ingredients of a new neutron star model fulfilling global, but not local, charge neutrality are described by what are called the Einstein-Maxwell-Thomas-Fermi equations, which account for the strong, weak, electromagnetic, and gravitational interactions, as well as thermodynamical equilibrium, within the framework of general relativity and relativistic nuclear mean field theory.
Journal ArticleDOI

Rosat observations of the vela pulsar

TL;DR: In this article, the ROSAT HRI was used to monitor X-ray emission from the Vela pulsar, and it was found to be 12% pulsed with one broad and two narrow peaks.
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