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NSR database version of April 26, 2024.

Search: Author = Y.M.Kim

Found 8 matches.

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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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2020KI06      Phys.Rev. C 101, 064614 (2020)

M.Kim, S.Jeon, Y.-M.Kim, Y.Kim, C.-H.Lee

Extended parity doublet model with a new transport code

NUCLEAR REACTIONS ¹⁹⁷Au(¹⁹⁷Au, X), E=100, 400 MeV/nucleon; calculated radial density profile, Pauli blocking factor, transverse flow, rapidity and momentum distributions, neutron and proton effective masses and densities, and proton directed flow using extended parity doublet model with a new transport code DaeJeon Boltzmann-Uehling-Uhlenbeck (DJBUU). Comparison with experimental data from FOPI collaboration. Dynamical properties of heavy-ion collisions and box calculations of collisions and blocking.

doi: 10.1103/PhysRevC.101.064614
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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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2020KI14      Int.J.Mod.Phys. E29, 2030007 (2020)

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

Neutron star equations of state and their applications

NUCLEAR STRUCTURE ^16,28O, ^40,48,60Ca, ⁹⁰Zr, ¹³²Sn, ²⁰⁸Pb; calculated binding energies, charge radii and neutron skin from five selected Skyrme type models.

doi: 10.1142/S0218301320300076
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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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2018KI19      Phys.Rev. C 98, 065805 (2018)

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

Tidal deformability of neutron stars with realistic nuclear energy density functionals

doi: 10.1103/PhysRevC.98.065805
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2017KI05      Phys.Rev. C 96, 015201 (2017)

Y.-M.Kim, C.-H.Lee, D.Teaney, I.Zahed

Direct photon elliptic flow at energies available at the BNL Relativistic Heavy Ion Collider and the CERN Large Hadron Collider

doi: 10.1103/PhysRevC.96.015201
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2011LE44      J.Korean Phys.Soc. 59, 2118s (2011)

C.-H.Lee, H.-S.Cho, Y.M.Kim, H.-Y.Park

Kaon Condensation in Neutron Stars and Related Astrophysical Issues

doi: 10.3938/jkps.59.2118
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