Neutron stars and the nuclear equation of state

GF Burgio, HJ Schulze, I Vidaña, JB Wei - Progress in Particle and Nuclear …, 2021 - Elsevier
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 …

Evolution of shell structure in exotic nuclei

T Otsuka, A Gade, O Sorlin, T Suzuki, Y Utsuno - Reviews of modern physics, 2020 - APS
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 …

Ab initio predictions link the neutron skin of 208Pb to nuclear forces

B Hu, W Jiang, T Miyagi, Z Sun, A Ekström, C Forssén… - Nature Physics, 2022 - nature.com
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 …

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 …

[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 …

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 …

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 …

Nonparametric inference of neutron star composition, equation of state, and maximum mass with GW170817

R Essick, P Landry, DE Holz - Physical Review D, 2020 - APS
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) …

Neutron star radii and crusts: Uncertainties and unified equations of state

M Fortin, C Providência, AR Raduta, F Gulminelli… - Physical Review C, 2016 - APS
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 …

Skyrme interaction and nuclear matter constraints

M Dutra, O Lourenço, JS Sá Martins, A Delfino… - Physical Review C …, 2012 - APS
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 …