Journal ArticleDOI
Relativistic mean-field theory with non-linear σ and ω terms for neutron stars and supernovae
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In this article, the properties of dense matter in neutron stars and supernovae in the relativistic mean field (RMF) theory with non-linear σ and ω terms were studied.About:
This article is published in Nuclear Physics.The article was published on 1995-01-16. It has received 77 citations till now. The article focuses on the topics: Neutron star & Nuclear matter.read more
Citations
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Journal ArticleDOI
Relativistic equation of state of nuclear matter for supernova and neutron star
TL;DR: In this article, the relativistic mean field (RMF) theory was used to construct the EOS of homogeneous nuclear matter, where heavy nuclei are formed together with free nucleon gas.
Journal ArticleDOI
Postbounce Evolution of Core-Collapse Supernovae: Long-Term Effects of the Equation of State
TL;DR: In this paper, the authors study the evolution of a supernova core from the beginning of the gravitational collapse of a 15 M☉ star up to 1 s after core bounce and compare two sets of EOS, namely, those by Lattimer and Swesty (LS-EOS) and by Shen et al. (SH-Eos).
Journal ArticleDOI
Hyperons and massive neutron stars: The role of hyperon potentials
TL;DR: In this paper, the influence of the hyperon potentials on the stiffness of the hadronic equation of state (EoS) was systematically investigated and it was shown that the maximum mass of purely nucleonic stars is very sensitive to the effective nucleon mass but only very little to the compression modulus.
Journal ArticleDOI
Equation of state for dense nucleonic matter from metamodeling. I. Foundational aspects
Jérôme Margueron,Jérôme Margueron,Rudiney Hoffmann Casali,Rudiney Hoffmann Casali,Francesca Gulminelli +4 more
TL;DR: In this article, a metamodeling for the nucleonic equation of state (EOS), inspired from a Taylor expansion around the saturation density of symmetric nuclear matter, is proposed and parameterized in terms of the empirical parameters.
Journal ArticleDOI
Dynamics and neutrino signal of black hole formation in nonrotating failed supernovae. I. Equation of state dependence
TL;DR: In this paper, the neutrino signal from the gravitational collapse of a nonrotating massive star of 40 M is studied and the influence of realistic equations of state (EOSs) for dense matter is explored.
References
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Book ChapterDOI
The Relativistic Nuclear Many-Body Problem
Brian D. Serot,John Dirk Walecka +1 more
TL;DR: These lectures are based on a book "The RELATIVISTIC NUCLEAR MANY-BODY PROBLEM" written with Brian Serot which will appear as volume 16 of the series Advances in Nuclear Physics edited by J. W. Negele and E. Vogt.
Journal ArticleDOI
A theory of highly condensed matter
TL;DR: In this article, a model relativistic, many-body, quantum field theory composed of a baryon field, a neutral scalar meson field coupled to the scalar density ψ ψ, and a neutral vector meson fields coupled with the conserved Baryon current i Ψ γλψ is developed.
Book
Black Holes, White Dwarfs and Neutron Stars: The Physics of Compact Objects
TL;DR: In this paper, the Equilibrium and Stability of Fluid Configurations of Neutron Star Models: Masses and Radii, Pulsars, Supermassive Stars and Black Holes.
Journal ArticleDOI
Measurements of Interaction Cross-Sections and Nuclear Radii in the Light p Shell Region
Isao Tanihata,Hideki Hamagaki,Osamu Hashimoto,Y. Shida,N. Yoshikawa,K. Sugimoto,O. Yamakawa,T. Kobayashi,N. Takahashi +8 more
TL;DR: The nucleus of the known Li isotopes showed a remarkably large radius suggesting a large deformation or a long tail in the matter distribution, and was observed for the first time.
Journal ArticleDOI
A Generalized equation of state for hot, dense matter
TL;DR: In this paper, an equation of state for hot, dense matter is presented in a form that is sufficiently rapid to use directly in hydrodynamical simulations, for example, in stellar collapse calculations.
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