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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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Hybrid Stars

Ashok Goyal
TL;DR: In this paper, the effect of quark and nuclear matter mixed phase on mass radius relationship of neutron stars employing recent models from two classes of EOS's and discuss their implications.

NMMA: A nuclear-physics and multi-messenger astrophysics framework to analyze binary neutron star mergers

TL;DR: In this paper , the authors developed the NMMA (Nuclear-physics and multi-messenger Astrophysics) framework, which allows incorporating of nuclear-physysics constraints at low densities as well as X-ray and radio observations of isolated neutron stars.
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Neutron stars and nuclei in the modified relativistic Hartree approximation

TL;DR: In this paper, the authors examined the properties of neutron-rich matter and finite nuclei in the modified relativistic Hartree approximation for several values of the renormalization parameter, μ, around the standard choice of μ equal to the nucleon mass M.
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Pygmies, Giants, and Skins

TL;DR: In this article, the authors focus on the EOS of cold baryonic matter with special emphasis on its impact on the structure, dynamics, and composition of neutron stars, and discuss how laboratory experiments on neutron skins as well as on Pygmy and Giant resonances can help us elucidate the structure of these fascinating objects.
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Hadron-quark phase transition: the QCD phase diagram and stellar conversion

TL;DR: In this paper, different extensions of the Nambu-Jona-Lasinio model are used to investigate a possible hadron-quark phase transition at zero temperature and to build the corresponding binodal sections.
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