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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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Accretion effects on compact members of binary stars

TL;DR: In this paper, the authors explore the change in the period of axial rotation and in the radius of a magnetized compact star in a binary system, induced by the accretion on it of mass with angular momentum from the surface of its non-compact companion.
Journal ArticleDOI

Superdense stars containing strange baryons

Yu. L. Vartanyan
- 17 Mar 2010 - 
TL;DR: A review dedicated to the centenary of V. A. Ambartsumyan and G. S. Sahakyan's work on superdense stars containing strange quarks is presented in this paper.
Posted Content

Constraints on the skewness coefficient of symmetric nuclear matter

Bao-Jun Cai, +1 more
TL;DR: In this paper, the authors show that both the pressure of symmetric nuclear matter at supra-saturation densities and the maximum mass of neutron stars are sensitive to the skewness coefficient.
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Neutron spin polarization in strong magnetic fields

TL;DR: In this paper, the effects of strong magnetic fields on the inner crust of neutron stars were investigated after taking into account the anomalous magnetic moments of nucleons, and the energy spectra and wave functions for protons and neutrons in a uniform magnetic field were provided.
Journal ArticleDOI

Breaking of universal relationships of axial <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>w</mml:mi><mml:mi>I</mml:mi></mml:math> modes in hybrid stars: Rapid and slow hadron-quark conversion scenarios

- 25 Aug 2022 - 
TL;DR: In this article , the authors focus on quadrupolar purely spacetime $wI$ modes of oscillating compact objects described using a wide range of hybrid equations of state able to include several theoretical possibilities of exotic matter in the inner core of such stars.
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