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 …
Self-consistent methods for structure and production of heavy and superheavy nuclei
GG Adamian, NV Antonenko, H Lenske… - The European Physical …, 2021 - Springer
Self-consistent methods for the structure of heavy and superheavy nuclei are reviewed. The
construction and application of energy-density functionals are discussed. The relationship …
construction and application of energy-density functionals are discussed. The relationship …
Constraints on the curvature of nuclear symmetry energy from recent astronomical data within the KIDS framework
H Gil, P Papakonstantinou, CH Hyun - International Journal of …, 2022 - World Scientific
In this paper, we investigate the density dependence of the nuclear symmetry energy S (ρ) in
the KIDS (Korea-IBS-Daegu-SKKU) framework for the nuclear equation of state (EoS) and …
the KIDS (Korea-IBS-Daegu-SKKU) framework for the nuclear equation of state (EoS) and …
Constraining the density dependence of the symmetry energy with nuclear data and astronomical observations in the Korea-IBS-Daegu-SKKU framework
H Gil, YM Kim, P Papakonstantinou, CH Hyun - Physical Review C, 2021 - APS
Background: The properties of very neutron rich nuclear systems are largely determined by
the density dependence of the nuclear symmetry energy. The Korea-IBS-Daegu-SKKU …
the density dependence of the nuclear symmetry energy. The Korea-IBS-Daegu-SKKU …
Bayesian inference of neutron-star observables based on effective nuclear interactions
Based on the Skyrme-Hartree-Fock model (SHF) as well as its extension [the Korea-IBS-
Daegu-SKKU (KIDS) model] and the relativistic mean-field (RMF) model, we have studied …
Daegu-SKKU (KIDS) model] and the relativistic mean-field (RMF) model, we have studied …
Bayesian inference of finite-nuclei observables based on the KIDS model
Bayesian analyses on both isoscalar and isovector nuclear interaction parameters are
carried out based on the Korea-IBS-Daegu-SKKU (KIDS) model under the constraints of …
carried out based on the Korea-IBS-Daegu-SKKU (KIDS) model under the constraints of …
Energy-density modeling of strongly interacting matter: Atomic nuclei and dense stars
P Papakonstantinou, CH Hyun - Symmetry, 2023 - mdpi.com
We seek a simple but physically motivated model of strongly interacting matter applicable in
atomic nuclei and the dense matter in the core of neutron stars. For densities below and …
atomic nuclei and the dense matter in the core of neutron stars. For densities below and …
[HTML][HTML] Quasielastic charged-current neutrino-nucleus scattering with nonrelativistic nuclear energy density functionals
KS Kim, H Gil, CH Hyun - Physics Letters B, 2022 - Elsevier
Charged-current neutrino-nucleus scattering is studied in the quasielastic region with the
KIDS (Korea-IBS-Daegu-SKKU) nuclear energy density functional. We focus on the …
KIDS (Korea-IBS-Daegu-SKKU) nuclear energy density functional. We focus on the …
Probing hadron-quark transition through binary neutron star merger
LJ Guo, WC Yang, YL Ma, YL Wu - arxiv preprint arxiv:2308.01770, 2023 - arxiv.org
The cores of massive neutron stars provide a unique environment for the dense nuclear
matter in the universe. The global properties of a neutron star and gravitational waves …
matter in the universe. The global properties of a neutron star and gravitational waves …
Analysis of nuclear structure in a converging power expansion scheme
Background: In the framework of the newly developed generalized energy density functional
(EDF) called KIDS, the nuclear equation of state (EoS) is expressed as an expansion in …
(EDF) called KIDS, the nuclear equation of state (EoS) is expressed as an expansion in …