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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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The effects of strong magnetic fields on neutron star structure: lowest order constrained variational calculations

TL;DR: In this paper, the effects of strong magnetic fields on the large-scale properties of neutron and protoneutron stars were investigated using the lowest order constrained variational approach at zero and finite temperatures, and employing AV18 potential.
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A starquake model for the Vela pulsar

TL;DR: In this paper, it was shown that the FMI of the Vela pulsar is inconsistent with the starquake mechanism for glitch generation in various neutron star (NS) models, based upon the parametrized equations of state (EOSs) of dense nuclear matter.
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Massive relativistic compact stars from SU(3) symmetric quark models

TL;DR: In this paper , a set of hyperonic equations of state (EoS) was constructed by assuming SU(3) symmetry within the baryon octet and by using a covariant density functional (CDF) theory approach.
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Vacuum polarization effects in hyperon-rich dense matter?a nonperturbative treatment

TL;DR: In this article, the authors derived the equation of state (EOS) for electrically charged neutral dense matter using the quantum hadrodynamics (QHD) model in a nonperturbative manner.
Journal ArticleDOI

Neutron matter, symmetry energy and neutron stars

TL;DR: In this paper, the nuclear symmetry energy, the energy cost of creating an isospin asymmetry, and its connection to the structure of neutron stars are discussed, combining these advances with recent observations of neutron star masses and radii gives insight into the equation of state of neutron-rich matter near and above the saturation density.
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