NSR Query Results
Output year order : Descending NSR database version of May 8, 2024. Search: Author = C.H.Hyun Found 43 matches. 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
2022CH39 Eur.Phys.J. A 58, 161 (2022) S.Choi, E.Hiyama, C.H.Hyun, M.-K.Cheoun Effects of many-body interactions in hypernuclei with Korea-IBS-Daegu-SKKU functionals NUCLEAR STRUCTURE 16O, 28Si, 32S, 40Ca, 51V, 89Y, 139La, 208Pb, Sn; analyzed available data; calculated properties of Λ hyperon in Λ-hypernuclei using an effective nuclear density functional theory which is based on the low-energy effective field theory.
doi: 10.1140/epja/s10050-022-00817-4
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
2022GI03 Phys.Rev. C 105, 024607 (2022) 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
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
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
2021GI15 Phys.Rev. C 104, 044613 (2021) 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
2020AN03 Phys.Rev. C 101, 054001 (2020) S.-I.Ando, Y.-H.Song, C.H.Hyun Neutrino-deuteron reactions at solar neutrino energies in pionless effective field theory with dibaryon fields NUCLEAR REACTIONS 2H(ν, np), (ν-bar, e+2n), (ν-bar, np), (ν, e-2p), E=2-20 MeV, solar neutrino energies; calculated σ(E), and S-wave contribution to the σ(E) using pionless effective field theory with dibaryon fields (dEFT). Comparison with other theoretical prediction.
doi: 10.1103/PhysRevC.101.054001
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
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
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, 40,42,44,46,48,50,52,54,56,58,60Ca, 90Zr, 100,102,104,106,108,110,112,114,116,118,120,122,124,126,128,130,132Sn, 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
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
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
2018PA03 Phys.Rev. C 97, 014312 (2018) P.Papakonstantinou, T.-S.Park, Y.Lim, C.H.Hyun Density dependence of the nuclear energy-density functional
doi: 10.1103/PhysRevC.97.014312
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
2017SO10 Phys.Rev. C 96, 014001 (2017) Y.-H.Song, S.-I.Ando, C.H.Hyun Spin-polarization observables of deuteron photodisintegration at low energies in pionless effective-field theory NUCLEAR REACTIONS 2H(γ, np), (polarized γ, np), E=2-30 MeV; calculated unpolarized total σ(E) for deuteron photodisintegration, ratio of the unpolarized differential σ(θ) and total σ, polarized differential σ(θ, E), tensor analyzing powers T20(θ, E) and T22(θ, E), induced neutron polarization. Pionless effective field theory up to next-to-next-to-leading order (NNLO), and with dibaryon fields. Comparison with experimental data from High Intensity Gamma-Ray Source facility at Duke University.
doi: 10.1103/PhysRevC.96.014001
2016SH26 Phys.Rev. C 94, 024320 (2016) Nuclear isospin asymmetry in α decay of heavy nuclei RADIOACTIVITY 270Db, 271Sg, 270,272,274Bh, 275Hs, 274,275,276,278Mt, 279Ds, 278,279,280,282Rg, 285Cn, 282,283,284,286Nh, 286,287,288,289Fl, 287,288,290Mc, 290,291,292,293Lv, 293,294,295,296,297,298Ts, 293,294,295,296,297,298Og, 293,294,295,296,297,298119, 299,300,301,302,303,304120, 301,302,303,304,305,306121, 302,303,304,305,306,307122(α); calculated half-lives using various phenomenological models of the nuclear potential for the α particle and Wentzel-Kramers-Brillouin (WKB) approximation: square-well potential, Woods-Saxon potential modified by including an isospin asymmetry term, energy density functional approach using Skyrme force model, and modified Viola and Seaborg formula to include isospin asymmetry effect. Comparison with available experimental results.
doi: 10.1103/PhysRevC.94.024320
2014LI23 Phys.Rev. C 89, 055804 (2014) Y.Lim, K.Kwak, C.H.Hyun, C.-H.Lee Kaon condensation in neutron stars with Skyrme-Hartree-Fock models
doi: 10.1103/PhysRevC.89.055804
2013SH40 Phys.Rev. C 88, 035501 (2013) J.W.Shin, C.H.Hyun, S.-I.Ando, S.W.Hong Polarization of the neutron induced by hadronic weak interactions in the photodisintegration of the deuteron NUCLEAR REACTIONS 2H(γ, n)p, E=2-15 MeV; calculated polarization observables of neutrons in photodisintegration of deuteron. Pionless field effect theory. Implication on the understanding of hadronic weak interactions.
doi: 10.1103/PhysRevC.88.035501
2012AN09 Phys.Rev. C 86, 024002 (2012) Effective range corrections from effective field theory with dibaryon fields and perturbative pions
doi: 10.1103/PhysRevC.86.024002
2011AN16 Phys.Rev. C 83, 064002 (2011) S.-I.Ando, Y.-H.Song, C.H.Hyun, K.Kubodera Spin polarization in γd → (n-pol)p at low energies with a pionless effective field theory NUCLEAR REACTIONS 2H(γ, n), E<30 MeV; calculated spin up/down differential cross sections, neutron polarization as function of incident energy and angle, σ(E, θ). Pionless effective field theory with dibaryon fields (dEFT) framework. Comparison with experimental data.
doi: 10.1103/PhysRevC.83.064002
2011HY02 J.Korean Phys.Soc. 59, 2114s (2011) Kaon Condensation in the Neutron Star with a Quark-Meson Coupling Model
doi: 10.3938/jkps.59.2114
2011RY06 Phys.Rev. C 84, 035809 (2011) Hyperons and nuclear symmetry energy in neutron star matter
doi: 10.1103/PhysRevC.84.035809
2011RY07 J.Korean Phys.Soc. 59, 1521s (2011) Theoretical Calculation of the Anomalous Magnetic Moments of Baryons in Heavy Ion Collision
doi: 10.3938/jkps.59.1521
2010AN16 Nucl.Phys. A844, 165c (2010) Hadronic weak interaction in the two-nucleon system with effective field theories
doi: 10.1016/j.nuclphysa.2010.05.029
2010SH10 Phys.Rev. C 81, 055501 (2010) Parity-violating polarization in np → dγ with a pionless effective field theory
doi: 10.1103/PhysRevC.81.055501
2008DE18 Phys.Rev. C 77, 064002 (2008) B.Desplanques, C.H.Hyun, S.Ando, C.-P.Liu Parity-violating nucleon-nucleon interaction from different approaches NUCLEAR REACTIONS p(polarized p, p), p(polarized n, γ)E=13.6, 45, 221 MeV; calculated spectral functions, dependence of total potential energy on charge and radius, PV asymmetries. Effective field theory. Comparison with covariant approach.
doi: 10.1103/PhysRevC.77.064002
2007AN32 Phys.Rev. C 76, 064001 (2007) S.Ando, J.W.Shin, C.H.Hyun, S.-W.Hong Low energy proton-proton scattering in effective field theory NUCLEAR REACTIONS p(p, X), E not given; calculated scattering amplitudes using pionless effective field theory.
doi: 10.1103/PhysRevC.76.064001
2007HY01 Eur.Phys.J. A 32, 513 (2007) C.H.Hyun, S.Ando, B.Desplanques Two-pion-exchange parity-violating potential and np → dγ
doi: 10.1140/epja/i2006-10426-8
2007RY05 Phys.Rev. C 75, 055804 (2007) C.Y.Ryu, C.H.Hyun, S.W.Hong, B.T.Kim Kaon condensation and composition of neutron star matter in a modified quark-meson coupling model
doi: 10.1103/PhysRevC.75.055804
2006AN16 Phys.Rev. C 74, 025809 (2006) S.Ando, R.H.Cyburt, S.W.Hong, C.H.Hyun Radiative neutron capture on a proton at big-bang nucleosynthesis energies NUCLEAR REACTIONS 1H(n, γ), E(cm) ≈ 0-1 MeV; 2H(γ, n), E(cm) ≈ 0-1 MeV; calculated total σ. 2H(polarized γ, n), E ≈ 0-1 MeV; calculate analyzing power.
doi: 10.1103/PhysRevC.74.025809
2006LI29 Phys.Rev. C 73, 065501 (2006) C.-P.Liu, C.H.Hyun, B.Desplanques Parity nonconservation in elastic p(pol)p scattering NUCLEAR REACTIONS 1H(polarized p, p), E=13.6, 45, 221 MeV; analyzed parity-nonconserving asymmetry, weak coupling constants.
doi: 10.1103/PhysRevC.73.065501
2005AN16 Phys.Rev. C 72, 014008 (2005) Effective field theory of the deuteron with dibaryon fields NUCLEAR REACTIONS 2H(e, e), E not given; calculated form factors. 1H(n, γ), E=0-1 MeV; calculated δ, magnetic dipole contributions. Pionless effective field theory, comparison with data.
doi: 10.1103/PhysRevC.72.014008
2005HY01 Eur.Phys.J. A 24, 129 (2005) C.H.Hyun, S.J.Lee, J.Haidenbauer, S.W.Hong Parity-nonconserving observables in thermal neutron capture on a proton NUCLEAR REACTIONS 1H(n, γ), (polarized n, γ), E ≈ threshold; calculated parity-nonconserving polarization observables. Several models compared.
doi: 10.1140/epja/i2004-10131-8
2005HY02 Eur.Phys.J. A 24, Supplement 2, 179 (2005) C.H.Hyun, C.-P.Liu, B.Desplanques Parity violating asymmetry in γ + d → n + p at low energy NUCLEAR REACTIONS 2H(polarized γ, np), E=2-12 MeV; calculated parity-violating asymmetry.
doi: 10.1140/epjad/s2005-04-045-7
2005LE09 Eur.Phys.J. A 24, Supplement 2, 105 (2005) H.-J.Lee, C.H.Hyun, C.-H.Lee, H.-C.Kim Strangeness-conserving effective weak chiral Lagrangian
doi: 10.1140/epjad/s2005-04-024-0
2005RY01 Eur.Phys.J. A 24, 149 (2005) C.Y.Ryu, C.H.Hyun, S.W.Hong, B.K.Jennings Hadron masses in medium and neutron star properties
doi: 10.1140/epja/i2004-10133-6
2005RY05 Phys.Rev. C 72, 045206 (2005) C.Y.Ryu, C.H.Hyun, J.Y.Lee, S.W.Hong Effective mass and decay of Θ+ in nuclear matter by using the quark-meson coupling models
doi: 10.1103/PhysRevC.72.045206
2004LI44 Phys.Rev. C 69, 065502 (2004) C.-P.Liu, C.H.Hyun, B.Desplanques Parity nonconservation in the photodisintegration of the deuteron at low energy NUCLEAR REACTIONS 2H(polarized γ, np), E ≈ threshold; calculated σ, parity-nonconserving asymmetry, vector-meson exchange contributions.
doi: 10.1103/PhysRevC.69.065502
2003HY01 Phys.Lett. 552B, 41 (2003) The anapole moment of the deuteron with the Argonne v18 nucleon-nucleon interaction model NUCLEAR STRUCTURE 2H; calculated anapole moment. Comparison with previous results.
doi: 10.1016/S0370-2693(02)03107-6
2003HY04 Nucl.Phys. A718, 709c (2003) Effects of Meson Mass Reduction on the Properties of Neutron Star Matter
doi: 10.1016/S0375-9474(03)00896-0
2003LI49 Phys.Rev. C 68, 045501 (2003) C.-P.Liu, C.H.Hyun, B.Desplanques Deuteron anapole moment with heavy mesons NUCLEAR STRUCTURE 2H; calculated anapole moment, meson exchange contributions.
doi: 10.1103/PhysRevC.68.045501
2000HY01 Phys.Lett. 473B, 6 (2000) A Higher-Order Calculation of np Scattering in Cut-Off Effective Field Theory NUCLEAR REACTIONS 1H(n, X), E(cm)=70-280 MeV; calculated phase shifts; deduced two-pion exchange contributions, related features.
doi: 10.1016/S0370-2693(99)01487-2
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