NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = Y.Lim Found 19 matches. 2024LI22 Phys.Rev. C 109, 035801 (2024) Symmetry energy and neutron star properties constrained by chiral effective field theory calculations
doi: 10.1103/PhysRevC.109.035801
2023XA01 Phys.Rev. C 108, 064310 (2023) Realistic evaluation of the Coulomb potential in spherical nuclei and a test of the traditional approach
doi: 10.1103/PhysRevC.108.064310
2021LI15 Phys.Rev. C 103, 025807 (2021) Proton pairing in neutron stars from chiral effective field theory
doi: 10.1103/PhysRevC.103.025807
2021LI48 Phys.Rev. C 104, L032802 (2021) Y.Lim, A.Bhattacharya, J.W.Holt, D.Pati Radius and equation of state constraints from massive neutron stars and GW190814
doi: 10.1103/PhysRevC.104.L032802
2021WH01 Phys.Rev.Lett. 127, 182502 (2021) T.R.Whitehead, Y.Lim, J.W.Holt Global Microscopic Description of Nucleon-Nucleus Scattering with Quantified Uncertainties NUCLEAR REACTIONS 14N, 16O, 34S, 56Fe, 90Zr, 121Sb, 138Ba, 182W, 208Pb(n, n), E<75 MeV; 16O, 27Al, 48Ti, 60Ni, 80Se, 120Sn, 182W, 194Pt, 206Pb(p, p), E<135 MeV; analyzed available data; deduced s(θ), optical potentials from a set of five nuclear forces from chiral effective field theory for 1800 target nuclei.
doi: 10.1103/PhysRevLett.127.182502
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
2020WH01 Phys.Rev. C 101, 064613 (2020) T.R.Whitehead, Y.Lim, J.W.Holt Neutron elastic scattering on calcium isotopes from chiral nuclear optical potentials NUCLEAR STRUCTURE 40,48Ca; calculated matter density distributions using mean-field theory with the Skyrme Skχ450 effective interaction constrained by chiral effective field theory. NUCLEAR REACTIONS 40,48Ca(n, n), E=3.2, 30, 85 MeV; calculated real, imaginary, and spin-orbit terms of the microscopic chiral optical potential. 40Ca(n, n), E=3.2, 5.3, 6.52, 11.9, 16.9, 21.7, 25.5, 30, 40, 65, 85, 107.5, 155, 185 MeV; 48Ca(n, n), E=7.97, 11.9, 16.9 MeV; calculated differential σ(E, θ). 48Ca(polarized n, n), E=11.9, 16.9 MeV; calculated vector analyzing powers Ay(E, θ). Calculated used the chiral optical potential, and Koning-Delaroche phenomenological optical potential. 40,48Ca(n, x), E=10-200 MeV; calculated total σ(E) using the chiral optical potential. Comparison with experimental data. Improved microscopic optical potential based on nuclear two- and three-body interactions from chiral effective field theory.
doi: 10.1103/PhysRevC.101.064613
2019LI43 Phys.Rev. C 100, 035802 (2019) Predicting the moment of inertia of pulsar J0737-3039A from Bayesian modeling of the nuclear equation of state
doi: 10.1103/PhysRevC.100.035802
2019LI53 Eur.Phys.J. A 55, 209 (2019) Bayesian modeling of the nuclear equation of state for neutron star tidal deformabilities and GW170817
doi: 10.1140/epja/i2019-12917-9
2019WH01 Phys.Rev. C 100, 014601 (2019) T.R.Whitehead, Y.Lim, J.W.Holt Proton elastic scattering on calcium isotopes from chiral nuclear optical potentials NUCLEAR REACTIONS 40Ca(p, p), E=2.35, 35, 100 MeV; calculated real, imaginary, and spin-orbit terms of the microscopic optical potential from chiral EFT, and from fits to the Koning-Delaroche (KD) form. 40,42,44,48Ca; calculated nucleon density distributions in mean field theory using the Skyrme Skχ450 effective interaction. 40Ca(p, p), E=2.35, 25, 35, 45, 55, 65, 80, 135, 160 MeV; 42,44,48Ca(p, p), E=25, 35, 45 MeV; 40,42,44,48Ca(p, X), E=20-50 MeV; calculated differential elastic σ(θ, E), and total reaction σ(E) using microscopic optical potentials calculated from chiral effective field theory, and from the chiral optical potential by the Koning-Delaroche (KD) phenomenological imaginary part, and using the reaction code TALYS. Comparison with experimental data.
doi: 10.1103/PhysRevC.100.014601
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
2018LI39 Phys.Rev.Lett. 121, 062701 (2018) Neutron Star Tidal Deformabilities Constrained by Nuclear Theory and Experiment
doi: 10.1103/PhysRevLett.121.062701
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
2018XI02 At.Data Nucl.Data Tables 121-122, 1 (2018) X.W.Xia, Y.Lim, P.W.Zhao, H.Z.Liang, X.Y.Qu, Y.Chen, H.Liu, L.F.Zhang, S.Q.Zhang, Y.Kim, J.Meng The limits of the nuclear landscape explored by the relativistic continuum Hartree-Bogoliubov theory NUCLEAR STRUCTURE Z=8-120; calculated ground-state properties using the spherical relativistic continuum Hartree-Bogoliubov (RCHB) theory with the relativistic density functional PC-PK1.
doi: 10.1016/j.adt.2017.09.001
2017LI09 Phys.Rev. C 95, 034311 (2017) Nuclear energy density functional and the nuclear α decay RADIOACTIVITY 271Sg, 270,272Bh, 275Hs, 274,275,276Mt, 279Ds, 278,279,280Rg, 283,285Cn, 282,283,284Nh, 286,287,288,289Fl, 287,288Mc, 290,291,292,293Lv, 294Og(α); calculated half-lives for α decay using the Skyrme SLy4 and Gogny D1S models as nonrelativistic models and the relativistic mean-field DD-ME2 model, and using experimental Q(α) values, half-lives compared with experimental values. 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 for α decay using the Skyrme SLy4 and Gogny D1S models as nonrelativistic models and the relativistic mean-field DD-ME2 model, and Q(α) values calculated from liquid-drop model (LDM) and from a local formula. Nuclear energy density functional formalism applied to α decay, using a Skyrme-type force model to obtain the nuclear potential of the α particle as a functional of proton and neutron density profiles of the daughter nucleus obtained from non-relativistic Skyrme SLy4, Gogny D1S, and relativistic mean-field DD-ME2 models.
doi: 10.1103/PhysRevC.95.034311
2017LI20 Phys.Rev. C 95, 065805 (2017) Structure of neutron star crusts from new Skyrme effective interactions constrained by chiral effective field theory
doi: 10.1103/PhysRevC.95.065805
2016LI04 Phys.Rev. C 93, 014314 (2016) Proton radioactivity in relativistic continuum Hartree-Bogoliubov theory RADIOACTIVITY 109I, 112,113Cs, 144,145,146,146m,147,147mTm, 150,150m,151,151mLu, 155,156,156m,157Ta, 159m,160,161,161mRe, 164m,165m,166,166m,167,167mIr, 170,170m,171,171mAu, 176,177,177mTl, 185Bi(p); calculated half-lives, nonoccupation probabilities u2 of corresponding orbitals in the daughter nuclei. Wentzel-Kramers-Brillouin (WKB) method for half-lives, with continuum effect treated by using relativistic continuum Hartree-Bogoliubov theory with energy density functional PC-PK1. Comparison with experimental half-lives.
doi: 10.1103/PhysRevC.93.014314
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
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