Journal ArticleDOI
The Ground state of matter at high densities: Equation of state and stellar models
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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.read more
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Computation of Neutron Star Structure Using Modern Equation of State
Gholam Hossein Bordbar,M. Hayati +1 more
TL;DR: In this paper, the authors used the modern equations of state derived from microscopic calculations to calculate the structure of a neutron star and obtained a minimum mass about 0.1 and a maximum mass between 1.47 and 1.98.
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Birth events, masses and the maximum mass of Compact Stars
TL;DR: In this paper, the authors give an overview of the problem of neutron star mass distribution, the issue of the maximum mass as inferred from the existing sample and the new gravitational wave events, and the connection with the formation events.
Journal ArticleDOI
Hyperons and quarks in proto-neutron stars
J. Roark,Xingfu Du,C. Constantinou,Veronica Dexheimer,Andrew W. Steiner,Andrew W. Steiner,Jirina Stone,Jirina Stone +7 more
TL;DR: In this article, the authors studied the impact of the composition of the cores of proto-neutron stars on the stellar structure, using the DSH model and the Chiral Mean Field (CMF) model.
Journal ArticleDOI
Dynamical constraints on some orbital and physical properties of the WD0137-349A/B binary system
TL;DR: In this article, the WD0137-349 binary system consisting of a white dwarf and a brown dwarf in a close circular orbit of about 116 min is considered and the most likely values for i are those that prevent such an anomalous behavior of Q, i.e. those for which the third Kepler law is an adequate modeling of the orbital period.
Journal ArticleDOI
Equation of State for Nucleonic and Hyperonic Neutron Stars with Mass and Radius Constraints
TL;DR: In this article, a new equation of state for the nucleonic and hyperonic inner core of neutron stars is obtained from a new parametrization of the FSU2 relativistic mean field functional that satisfies these latest astrophysical constraints and reproduces the properties of nuclear matter and finite nuclei while fulfilling the restrictions on high-density matter deduced from heavy-ion collisions.
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