In this contribution we discuss several new complete EoS for supernova, whose detailed composition is important for the neutrino dynamics. We focus on one important distinction for various EoS - the density dependence of symmetry energy E'(sym), and its interesting correlation with the radii of neutron star, as well as properties of neutron distribution in neutron rich nuclei
The role of the nuclear equation of state (EOS) in producing prompt supernova explosions is examined...
Documentos apresentados no âmbito do reconhecimento de graus e diplomas estrangeirosEquation of stat...
A better understanding of the density dependence of the nuclear equation of state (EOS) of isospin a...
International audienceWe give an overview about equations of state (EOS) which are currently availab...
We present a review of a broad selection of nuclear matter equations of state (EOSs) applicable in c...
We construct a new equation of state (EOS) for numerical simulations of core-collapse supernovae and...
International audienceThe equation of state (EoS) of hot and dense matter is a fundamental input to ...
To be published in Physical Review CThe nuclear mean-field potentials obtained in the Hartree-Fock m...
Context. An equation of state (EoS) of dense nuclear matter is a prerequisite for studies of the str...
International audienceWe review the equation of state (EoS) models covering a large range of tempera...
We derive a new equation of state (EoS) for neutron stars (NS) from the outer crust to the core base...
Using a meta model for nuclear Equation of State (EOS) with its parameters constrained by astrophysi...
We calculate total masses and radii of neutron stars (NS) for pure neutron matter and nuclear matter...
International audienceA review is given of various theoretical approaches for the equation of state ...
The role of the nuclear equation of state (EOS) in producing prompt supernova explosions is examined...
Documentos apresentados no âmbito do reconhecimento de graus e diplomas estrangeirosEquation of stat...
A better understanding of the density dependence of the nuclear equation of state (EOS) of isospin a...
International audienceWe give an overview about equations of state (EOS) which are currently availab...
We present a review of a broad selection of nuclear matter equations of state (EOSs) applicable in c...
We construct a new equation of state (EOS) for numerical simulations of core-collapse supernovae and...
International audienceThe equation of state (EoS) of hot and dense matter is a fundamental input to ...
To be published in Physical Review CThe nuclear mean-field potentials obtained in the Hartree-Fock m...
Context. An equation of state (EoS) of dense nuclear matter is a prerequisite for studies of the str...
International audienceWe review the equation of state (EoS) models covering a large range of tempera...
We derive a new equation of state (EoS) for neutron stars (NS) from the outer crust to the core base...
Using a meta model for nuclear Equation of State (EOS) with its parameters constrained by astrophysi...
We calculate total masses and radii of neutron stars (NS) for pure neutron matter and nuclear matter...
International audienceA review is given of various theoretical approaches for the equation of state ...
The role of the nuclear equation of state (EOS) in producing prompt supernova explosions is examined...
Documentos apresentados no âmbito do reconhecimento de graus e diplomas estrangeirosEquation of stat...
A better understanding of the density dependence of the nuclear equation of state (EOS) of isospin a...
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