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 …
Evolution of shell structure in exotic nuclei
The atomic nucleus is a quantum many-body system whose constituent nucleons (protons
and neutrons) are subject to complex nucleon-nucleon interactions that include spin-and …
and neutrons) are subject to complex nucleon-nucleon interactions that include spin-and …
Ab initio predictions link the neutron skin of 208Pb to nuclear forces
Heavy atomic nuclei have an excess of neutrons over protons, which leads to the formation
of a neutron skin whose thickness is sensitive to details of the nuclear force. This links …
of a neutron skin whose thickness is sensitive to details of the nuclear force. This links …
The equation of state of hot, dense matter and neutron stars
JM Lattimer, M Prakash - Physics Reports, 2016 - Elsevier
Recent developments in the theory of pure neutron matter and experiments concerning the
symmetry energy of nuclear matter, coupled with recent measurements of high-mass …
symmetry energy of nuclear matter, coupled with recent measurements of high-mass …
[CITA][C] Model Comparison from LIGO–Virgo Data on GW170817's Binary Components and Consequences for the Merger Remnant
BP Abbott, R Abbott, TD Abbott, S Abraham… - Default …, 2020 - andrews.elsevierpure.com
Model Comparison from LIGO–Virgo Data on GW170817’s Binary Components and
Consequences for the Merger Remnant — Andrews University Research Portal Skip to main …
Consequences for the Merger Remnant — Andrews University Research Portal Skip to main …
Shape coexistence in atomic nuclei
K Heyde, JL Wood - Reviews of Modern Physics, 2011 - APS
Shape coexistence in nuclei appears to be unique in the realm of finite many-body quantum
systems. It differs from the various geometrical arrangements that sometimes occur in a …
systems. It differs from the various geometrical arrangements that sometimes occur in a …
Equation of state for dense nucleonic matter from metamodeling. I. Foundational aspects
J Margueron, R Hoffmann Casali, F Gulminelli - Physical Review C, 2018 - APS
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 …
Nonparametric inference of neutron star composition, equation of state, and maximum mass with GW170817
The detection of GW170817 in gravitational waves provides unprecedented constraints on
the equation of state (EOS) of the ultradense matter within the cores of neutron stars (NSs) …
the equation of state (EOS) of the ultradense matter within the cores of neutron stars (NSs) …
Neutron star radii and crusts: Uncertainties and unified equations of state
The uncertainties in neutron star radii and crust properties due to our limited knowledge of
the equation of state are quantitatively analyzed. We first demonstrate the importance of a …
the equation of state are quantitatively analyzed. We first demonstrate the importance of a …
Skyrme interaction and nuclear matter constraints
This paper presents a detailed assessment of the ability of the 240 Skyrme interaction
parameter sets in the literature to satisfy a series of criteria derived from macroscopic …
parameter sets in the literature to satisfy a series of criteria derived from macroscopic …