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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Isothermal vs. isentropic description of protoneutron stars in the Brueckner-Bethe-Goldstone theory
G. F. Burgio,H.-J. Schulze +1 more
TL;DR: In this article, the structure of hadronic protoneutron stars within the finite-temperature Brueckner-Bethe-Goldstone theoretical approach was studied, and it was shown that particle populations and equation of state are very similar.
Journal ArticleDOI
From nuclear reactions to compact stars: a unified approach
TL;DR: In this paper, an equation of state for symmetric and asymmetric nuclear matter was constructed using the density-dependent M3Y effective interaction and extended for isospin asymmetric nuclei.
Journal ArticleDOI
Influence of the nuclear matter equation of state on the r-mode instability using the finite-range simple effective interaction
TL;DR: In this article, the amplitude of the r-mode at saturation was calculated using the data of particular neutron stars from the considerations of "spin equilibrium" and "thermal equilibrium", and the upper limit of the saturation amplitude was found to lie in the range 10^{-8}-10^{-6], in agreement with the predictions of earlier work.
Journal ArticleDOI
Key factor for determining relation between radius and tidal deformability of neutron stars: Slope of symmetry energy *
Nai-Bo Zhang,Bin Qi,S. Y. Wang +2 more
TL;DR: In this paper, the relationship between the radius of a massive neutron star and its deformability was investigated using an isospin-dependent parameterized equation of state (EOS).
Posted ContentDOI
The Equation of State of Nuclear Matter : from Finite Nuclei to Neutron Stars
G. F. Burgio,Isaac Vidaña +1 more
TL;DR: In this article, the authors investigate possible correlations between neutron star observables and properties of atomic nuclei and explore how the tidal deformability of a 1.4 solar mass neutron star, and the neutron skin thickness of ${48}$Ca and ${208}$Pb are related to stellar radius and the stiffness of the symmetry energy.
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