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Dense nuclear matter equation of state from heavy-ion collisions
The nuclear equation of state (EOS) is at the center of numerous theoretical and
experimental efforts in nuclear physics. With advances in microscopic theories for nuclear …
experimental efforts in nuclear physics. With advances in microscopic theories for nuclear …
Neutron stars and the nuclear equation of state
We review the current status and recent progress of microscopic many-body approaches
and phenomenological models, which are employed to construct the equation of state of …
and phenomenological models, which are employed to construct the equation of state of …
Equations of state for supernovae and compact stars
A review is given of various theoretical approaches for the equation of state (EoS) of dense
matter, relevant for the description of core-collapse supernovae, compact stars, and compact …
matter, relevant for the description of core-collapse supernovae, compact stars, and compact …
Nuclear ground-state masses and deformations: FRDM (2012)
We tabulate the atomic mass excesses and binding energies, ground-state shell-plus-
pairing corrections, ground-state microscopic corrections, and nuclear ground-state …
pairing corrections, ground-state microscopic corrections, and nuclear ground-state …
Equation of state for dense nucleonic matter from metamodeling. I. Foundational aspects
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 …
around the saturation density of symmetric nuclear matter, is proposed and parameterized in …
Nuclear equation of state from ground and collective excited state properties of nuclei
This contribution reviews the present status on the available constraints to the nuclear
equation of state (EoS) around saturation density from nuclear structure calculations on …
equation of state (EoS) around saturation density from nuclear structure calculations on …
The nuclear equation of state and neutron star masses
Neutron stars are valuable laboratories for the study of dense matter. Recent observations
have uncovered both massive and low-mass neutron stars and have also set constraints on …
have uncovered both massive and low-mass neutron stars and have also set constraints on …
Relativistic mean-field hadronic models under nuclear matter constraints
Background: The microscopic composition and properties of infinite hadronic matter at a
wide range of densities and temperatures have been subjects of intense investigation for …
wide range of densities and temperatures have been subjects of intense investigation for …
The nuclear symmetry energy
The nuclear symmetry energy characterizes the variation of the binding energy as the
neutron to proton ratio of a nuclear system is varied. This is one of the most important …
neutron to proton ratio of a nuclear system is varied. This is one of the most important …
Constraints on the symmetry energy and neutron skins from experiments and theory
The symmetry energy contribution to the nuclear equation of state impacts various
phenomena in nuclear astrophysics, nuclear structure, and nuclear reactions. Its …
phenomena in nuclear astrophysics, nuclear structure, and nuclear reactions. Its …