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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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Magnetized color flavor locked state and compact stars

TL;DR: In this article, the stability of the color flavor locked phase in the presence of a strong magnetic field was investigated within the phenomenological MIT bag model, taking into account the variation of the strange quark mass, the baryon density, the magnetic field, as well as the bag and gap parameters.
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Neutron star cooling and GW170817 constraint within quark-meson coupling models

TL;DR: In this article, five different versions of the quark-meson coupling (QMC) model were used to compute astrophysical quantities related to the GW170817 event and to neutron star cooling process.
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Stability valley for strange dwarfs

TL;DR: In this article, the stability of superdense stars with a small self-confining core (M ≥ 0.02 m) and an extended crust consisting of atomic nuclei and degenerate electron gas was studied.
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Phase transition from a4He plasma to stable8Be matter

TL;DR: In this article, it was shown that a4He quantum fluid will undergo a phase transition to stable 8Be matter at densitiesρ ≈ 2×109109g/cm3.
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Nuclear Matter and Neutron Stars from Relativistic Brueckner–Hartree–Fock Theory

TL;DR: In this paper , the RBHF theory in the full Dirac space was investigated and the saturation properties of symmetric and asymmetric nuclear matter were systematically investigated based on the realistic Bonn nucleon-nucleon potentials.
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