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NSR database version of April 26, 2024.

Search: Author = H.Gil

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2023GI09      Phys.Rev. C 108, 044316 (2023)

H.Gil, N.Hinohara, C.H.Hyun, K.Yoshida

Nuclear mass table in density functional approach inspired by neutron-star observations

doi: 10.1103/PhysRevC.108.044316
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2022GI02      Int.J.Mod.Phys. E31, 2250013 (2022)

H.Gil, P.Papakonstantinou, C.H.Hyun

Constraints on the curvature of nuclear symmetry energy from recent astronomical data within the KIDS framework

NUCLEAR STRUCTURE ²⁰⁸Pb; calculated neutron skin thickness; deduced no correlation at all with the neutron star radii. The KIDS (Korea-IBS-Daegu-SKKU) framework for the nuclear equation of state (EoS) and energy-density functional (EDF).

doi: 10.1142/S0218301322500136
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2022GI03      Phys.Rev. C 105, 024607 (2022)

H.Gil, C.H.Hyun, K.Kim

Inclusive electron scattering in the quasielastic region with the Korea-IBS-Daegu-SKKU density functional

NUCLEAR REACTIONS ¹²C, ⁵⁶Fe, ¹⁹⁷Au(e^-, e^-'), E=2.02 GeV; ⁴⁰Ca(e^-, e^-'), E=330, 375, 628 MeV; ²⁰⁸Pb(e^-, e^-'), E=310, 354, 485 MeV; calculated σ(θ), longitudinal and transverse σ. Calculations in the frame of KIDS (Korea-IBS-Daegu-SKKU) density functional model. Comparison to experimental data.

doi: 10.1103/PhysRevC.105.024607
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2022HU11      Phys.Rev. C 106, 035802 (2022)

P.T.P.Hutauruk, H.Gil, S.-il.Nam, C.H.Hyun

Effect of nucleon effective mass and symmetry energy on the neutrino mean free path in a neutron star

doi: 10.1103/PhysRevC.106.035802
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2021GI05      Phys.Rev. C 103, 034330 (2021)

H.Gil, Y.-M.Kim, P.Papakonstantinou, C.H.Hyun

Constraining the density dependence of the symmetry energy with nuclear data and astronomical observations in the Korea-IBS-Daegu-SKKU framework

NUCLEAR STRUCTURE ¹⁶O, ^40,48Ca, ⁹⁰Zr, ¹³²Sn, ²⁰⁸Pb, ²¹⁸U; calculated binding energies, S(2n). Z=20, N=20-48; Z=50, N=52-116; calculated S(2n). O, Ca, Ni, Zr, Sn, Pb; calculated position of the neutron drip line and for the neutron skin thickness of selected nuclei based on the six equations of state (EoSs). ²⁶O, ⁷⁰Ca; nuclei predicted as close to the neutron drip line. Korea-IBS-Daegu-SKKU (KIDS) framework for the nuclear equation of state (EoS) and energy density functional (EDF).

doi: 10.1103/PhysRevC.103.034330
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2021GI15      Phys.Rev. C 104, 044613 (2021)

H.Gil, C.H.Hyun, K.Kim

Quasielastic electron scattering with the KIDS nuclear energy density functional

NUCLEAR REACTIONS ¹⁶O, ⁴⁰Ca, ²⁰⁸Pb(e, e'p), E=300-2500 MeV; calculated σ(E) with parallel and perpendicular kinematics, fourth response functions and left-right asymmetry for ¹⁶O, spectroscopic factors for ⁴⁰Ca and ²⁰⁸Pb. ¹⁶O, ⁴⁰Ca, ²⁰⁸Pb; calculated charge and neutron density profiles; investigated isoscalar and isovector effective masses of the nucleon in nuclear medium, and ground state properties of spherical nuclei. KIDS (Korea-IBS-Daegu-SKKU) density functional model using KIDS0, KIDS0-m^*99 KIDS-m^*77 interactions, with wave functions of the nucleon in target nuclei obtained from nonrelativistic Hartree-Fock equation. Comparison with results from SLy4 interaction, and with experimental data from NIKHEF, Saclay and JLab facilities.

doi: 10.1103/PhysRevC.104.044613
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2020KI09      Eur.Phys.J. A 56, 157 (2020)

Y.-M.Kim, K.Kwak, C.H.Hyun, Ha.Gil, C.-H.Lee

Neutron star equation of state and tidal deformability with nuclear energy density functionals

doi: 10.1140/epja/s10050-020-00164-2
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2019GI12      Phys.Rev. C 99, 064319 (2019)

H.Gil, P.Papakonstantinou, C.H.Hyun, Y.Oh

From homogeneous matter to finite nuclei: Role of the effective mass

NUCLEAR STRUCTURE ^16,28O, ^{40,42,44,46,48,50,52,54,56,58,60}Ca, ⁹⁰Zr, ^{100,102,104,106,108,110,112,114,116,118,120,122,124,126,128,130,132}Sn, ²⁰⁸Pb, ²¹⁸U; calculated binding energy per nucleon, charge radii and neutron-skin thickness for ^16,28O, ^40,48,60Ca, ⁹⁰Zr, ¹³²Sn, ²⁰⁸Pb, ²¹⁸U, and energies of occupied proton levels in ²⁰⁸Pb using microscopic Skyrme type energy density functional (EDF) generated from a immutable equation of state (EoS). Comparison with experimental values, and with other theoretical predictions.

doi: 10.1103/PhysRevC.99.064319
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2019GI13      Phys.Rev. C 100, 014312 (2019)

H.Gil, Y.-M.Kim, C.H.Hyun, P.Papakonstantinou, Y.Oh

Analysis of nuclear structure in a converging power expansion scheme

NUCLEAR STRUCTURE ^16,28O, ^40,48,60Ca, ⁹⁰Zr, ¹³²Sn, ²⁰⁸Pb; calculated binding energies per nucleon, charge radii, and neutron skin thickness using generalized energy density functional model (KIDS EDF) to parametrized nuclear equation of state (EoS). Comparison with experimental values.

doi: 10.1103/PhysRevC.100.014312
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2017GI05      Acta Phys.Pol. B48, 305 (2017)

H.Gil, P.Papakonstantinou, C.H.Hyun, T.-S.Park, Y.Oh

Nuclear Energy Density Functional for KIDS

NUCLEAR STRUCTURE ^16,28O, ^40,60Ca; calculated energy per p article, mass excess, charge radius vs k-parameter of the radius using density functional theory. Masses compared with AME-2012 values.

doi: 10.5506/APhysPolB.48.305
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