NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = M.H.Mun Found 11 matches. 2023MU15 Eur.Phys.J. A 59, 149 (2023) M.-H.Mun, I.J.Shin, W.-G.Paeng, M.Harada, Y.Kim Nuclear structure in parity doublet model
doi: 10.1140/epja/s10050-023-01064-x
2023ZH15 Phys.Rev. C 107, L041303 (2023) K.Y.Zhang, P.Papakonstantinou, M.-H.Mun, Y.Kim, H.Yan, X.-X.Sun Collapse of the N=28 shell closure in the newly discovered 39Na nucleus and the development of deformed halos towards the neutron dripline NUCLEAR STRUCTURE 39Na; calculated S(n), single-neutron levels, J, π, quadrupole deformation, rms radius. 31,33,35,37,39,41Na; calculated neutron density distributions. Pointed that 39Na could be single nucleus with the coexistence of several exotic structures, including the quenched N=28 shell closure, Borromean structure, deformed halo, and between the core and the halo. Discussed the microscopic mechanisms behind the shape decoupling phenomenon and the development of halos towards dripline. Deformed relativistic Hartree-Bogoliubov theory in continuum.
doi: 10.1103/PhysRevC.107.L041303
2023ZH35 Phys.Lett. B 844, 138112 (2023) K.Y.Zhang, S.Q.Yang, J.L.An, S.S.Zhang, P.Papakonstantinou, M.-H.Mun, Y.Kim, H.Yan Missed prediction of the neutron halo in 37Mg NUCLEAR STRUCTURE 35,36,37Mg; calculated neutron density distributions, single-neutron energies, occupation probabilities using a microscopic and self-consistent way using the deformed relativistic Hartree-Bogoliubov theory in continuum; deduced the deformed p-wave halo characteristics of 37Mg.
doi: 10.1016/j.physletb.2023.138112
2022CH07 Phys.Rev. C 105, 024306 (2022) Y.-B.Choi, C.-H.Lee, M.-H.Mun, Y.Kim Bubble nuclei with shape coexistence in even-even isotopes of Hf to Hg NUCLEAR STRUCTURE 152,154,156,158,160,162,164,166,168,170,172,174,176,178,180,182,184,186,188,190,192,194,196,198,200,202,204,206,208,210,212,214,216,218,220,222,224,226,228,230,232,234,236,238,240,242,244,246,248,250,252,254,256Hf, 156,158,160,162,164,166,168,170,172,174,176,178,180,182,184,186,188,190,192,194,196,198,200,202,204,206,208,210,212,214,216,218,220,222,224,226,228,230,232,234,236,238,240,242,244,246,248,250,252,254,256,258W, 162,164,166,168,170,172,174,176,178,180,182,184,186,188,190,192,194,196,198,200,202,204,206,208,210,212,214,216,218,220,222,224,226,228,230,232,234,236,238,240,242,244,246,248,250,252,254,256,258,260Os, 170,172,174,176,178,180,182,184,186,188,190,192,194,196,198,200,202,204,206,208,210,212,214,216,218,220,222,224,226,228,230,232,234,236,238,240,242,244,246,248,250,252,254,256,258,260,262Pt, 172,174,176,178,180,182,184,186,188,190,192,194,196,198,200,202,204,206,208,210,212,214,216,218,220,222,224,226,228,230,232,234,236,238,240,242,244,246,248,250,252,254,256,258,260,262,264Hg; calculated quadrupole deformation parameters. 256Hf, 258W, 260Os, 256W; calculated neutron, proton and total nuclear densities. 196,208Os; calculated single-particle energy levels, J, π. 198,200,256Hf; calculated proton single-particle levels around the Fermi surface. Discussed the bubble structure and shape coexistence. Calculations based on deformed relativistic Hartree-Bogoliubov theory in continuum (DRHBc) and relativistic continuum Hartree-Bogoliubov (RCHB) theory with spherical symmetry. Comparison with experimenatal values.
doi: 10.1103/PhysRevC.105.024306
2022KI10 Phys.Rev. C 105, 034340 (2022) S.Kim, M.-H.Mun, M.K.Cheoun, E.Ha Shape coexistence and neutron skin thickness of Pb isotopes by the deformed relativistic Hartree-Bogoliubov theory in continuum NUCLEAR STRUCTURE 178,180,182,184,186,188,190,192,194,196,198,200,202,204,206,208,210,212,214Pb; calculated neutron pairing gaps. 172,174,176,178,180,182,184,186,188,190,192,194,196,198,200,202,204,206,208,210,212,214,216,218,220,222,224,226,228,230,232,234,236,238,240,242,244,246,248,250,252,254,256,258,260,262,264,266,268,270,272,274,276,278,260,282,284,286,288,290,292,294,296,298,300,302Pb; calculated deformation parameter by the minimum of the total binding energy. 182,184,186,188,208Pb; calculated neutron single-particle energies for various shape coexistence cases - oblate, spherical, prolate. 180,182,184,186,188,190,192,194,196,198,200,202,204,206,208,210,212,214,216,218Pb; calculated total binding energy dependence on the deformation.266,268,278Pb; calculated neutron single-particle states occupation probabilities. 260,262,264,266,268,270,272,274,276,278,260,282,284,286,288,290,292,294,296,298,300,302,304Pb; calculated S(2n), Fermi energies, deformation parameters. 208Pb; calculated proton and netron density distributions. 174,176,178,180,182,184,186,188,190,192,194,196,198,200,202,204,206,208,210,212,214,216,218,220,222,224,226,228,230,232,234,236,238,240,242,244,246,248,250,252,254,256,258,260,262,264,266Pb; calculated proton and neutron radii, neutron skin thickness. Deformed relativistic Hartree-Bogoliubov theory in continuum (DRHBc). Comparison to available experimental data.
doi: 10.1103/PhysRevC.105.034340
2020MU05 Phys.Rev. C 101, 044602 (2020) M.-H.Mun, K.Kwak, G.G.Adamian, N.V.Antonenko Possible production of neutron-rich No isotopes NUCLEAR REACTIONS 248,249,250,251Cf, 254Es(36S, X), (40Ar, X), (48Ca, X), (50Ti, X), 258No/259No/260No/261No/262No/263No/264No/265No/266No, E(cm)=150-230 MeV; 249,250,251Cf, (48Ca, X), Q=48-70 MeV; 254Es(36S, X), (40Ar, X), (48Ca, X), (50Ti, X), Q=30-55 MeV; calculated production σ(E) in zero-neutron and one-neutron evaporation channels. Comparison of production yields of No and Md isotopes. Dinuclear system (DNS) model.
doi: 10.1103/PhysRevC.101.044602
2019MU09 Phys.Rev. C 99, 054627 (2019) M.-H.Mun, K.Kwak, G.G.Adamian, N.V.Antonenko Possible production of neutron-rich Md isotopes in multinucleon transfer reactions with Cf and Es targets NUCLEAR REACTIONS 254Es(14C, X)258Md/259Md/260Md/261Md/262Md, E(cm)=60-80 MeV; 254Es(18O, X)258Md/259Md/260Md/261Md/262Md, E(cm)=80-95 MeV; 254Es(22Ne, X)258Md/259Md/260Md/261Md/262Md, E(cm)=100-120 MeV; 254Es(26Mg, X)258Md/259Md/260Md/261Md/262Md, E(cm)=115-140 MeV; 254Es(30Si, X)258Md/259Md/260Md/261Md/262Md, E(cm)=130-160 MeV; 254Es(36S, X)258Md/259Md/260Md/261Md/262Md, E(cm)=155-165 MeV; 254Es(40Ar, X)258Md/259Md/260Md/261Md/262Md/263Md/264Md/265Md, E(cm)=170-210 MeV; 254Es(40Ar, X)258Md/259Md/260Md/261Md/262Md/263Md, E(cm)=210-230 MeV; 249Cf(48Ca, X)258Md/259Md/260Md/261Md/262Md, E(cm)=200-210 MeV; 250Cf(48Ca, X)258Md/259Md/260Md/261Md/262Md/263Md, E(cm)=200-210 MeV; 251Cf(48Ca, X)258Md/259Md/260Md/261Md/262Md/263Md/264Md, E(cm)=195-212.5 MeV; 252Cf(48Ca, X)258Md/259Md/260Md/261Md/262Md/263Md/264Md/265Md, E(cm)=195-212.5 MeV; calculated total capture σ(E), maximal production σ(E) for zero- and one-neutron evaporation channels of multinucleon transfer reactions. Dinuclear system (DNS) model.
doi: 10.1103/PhysRevC.99.054627
2016MU17 Eur.Phys.J. A 52, 363 (2016) M.-Hw.Mun, G.G.Adamian, N.V.Antonenko, Y.-O.Lee Possibilities of production of neutron-rich Md isotopes in multi-nucleon transfer reactions NUCLEAR REACTIONS 238U(48Ca, x)259,260,261,262,263Md, E(cm)=191-197 MeV;242,244Pu(48Ca, x)259,260,261,262,263Md, E(cm)=191-201 MeV;245,246,248Cm(48Ca, x)259,260,261,262,263Md, E(cm)=197-205 MeV; calculated σ.
doi: 10.1140/epja/i2016-16363-y
2015MU05 Phys.Rev. C 91, 054610 (2015) M.-H.Mun, G.G.Adamian, N.V.Antonenko, Y.Oh, Y.Kim Toward neutron-rich nuclei via transfer reactions with stable and radioactive beams NUCLEAR REACTIONS 160Gd, 164Dy, 170Er, 176Yb, 180Hf, 186W, 192Os, 204Hg, 208Pb, 232Th(48Ca, X)52Ca/54Ca/56Ca/58Ca, E(cm)=150-225 MeV; 64,66,68,70,72,74,76,78Ni, 86,88,90,92,94Kr(160Gd, X)166Gd/168Gd/170Gd/172Gd/174Gd, E(cm)=145-260 MeV; 48Ca, 50Ti, 54Cr, 58Fe, 64,66,68,70,72,74,76,78Ni, 70Zn, 76Ge, 82Se, 86,88,90,92,94Kr(164Dy, X)170Dy/172Dy/174Dy/176Dy/178Dy, E(cm)=150-260 MeV; 48Ca, 50Ti, 54Cr, 58Fe, 64,66,68,70,72,74,76,78Ni, 70Zn, 76Ge, 82Se, 86,88,90,92,94Kr(170Er, X)176Er/178Er/180Er/182Er/184Er, E(cm)=150-270 MeV; 48Ca, 50Ti, 54Cr, 58Fe, 64,66,68,70,72,74,76,78Ni, 70Zn, 76Ge, 82Se, 86,88,90,92,94Kr(176Yb, X)182Yb/184Yb/186Yb/188Yb/190Yb, E(cm)=160-270 MeV; 64,66,68,70,72,74,76,78Ni(180Hf, X)186Hf/188Hf/190Hf/192Hf/194Hf, E(cm)=190-230 MeV; 48Ca, 50Ti, 54Cr, 58Fe, 64,66,68,70,72,74,76,78Ni, 70Zn, 76Ge, 82Se(186W, X)192W/194W/196W/198W/200W, E(cm)=170-270 MeV; 48Ca, 50Ti, 54Cr, 58Fe, 64,66,68,70,72,74,76,78Ni, 70Zn, 76Ge, 82Se(192Os, X)196Os/198Os/200Os/202Os/204Os, E(cm)=165-270 MeV; 48Ca, 66,68,70,72,74,76,78Ni(204Hg, X)210Hg/212Hg/214Hg/216Hg, E(cm)=192-255 MeV; 48Ca, 66,68,70,72,74,76,78Ni(208Pb, X)214Pb/216Pb/218Pb/220Pb, E(cm)=200-268 MeV; 48Ca, 66,68,70,72,74,76,78Ni(232Th, X)238Th/240Th/242Th/244Th, E(cm)=199-261 MeV; calculated σ(E) for production of neutron-rich nuclei close to the neutron drip line in multi-nucleon transfer reactions. Dinuclear system (DNS) approach with synthesis through nucleon transfers and decay into two fragments.
doi: 10.1103/PhysRevC.91.054610
2014MU02 Phys.Rev. C 89, 034622 (2014) M.-H.Mun, G.G.Adamian, N.V.Antonenko, Y.Oh, Y.Kim Production cross section of neutron-rich isotopes with radioactive and stable beams NUCLEAR REACTIONS 48Ca, 70Zn, 86Kr, 88Sr(144Xe, X)148Xe/150Xe/152Xe, E(cm)=130-240 MeV; 48Ca(134Te, X), (136Te, X)136Te/138Te/140Te/142Te, E(cm)=120-170 MeV; 68,70Zn(142Xe, X), (144Xe, X)82Zn/84Zn/86Zn, E(cm)=160-195 MeV; 48Ca(134Te, X), (136Te, X)52Ca/54Ca/56Ca/58Ca/60Ca, E(cm)=125-165 MeV; 198Pt(48Ca, X), (50Ti, X), (54Cr, X), (58Fe, X), (64Ni, X), (70Zn, X), (76Ge, X)202Pt/204Pt/206Pt, E(cm)=170-270 MeV; 198Pt(48Ca, X)202Pt/203Pt/204Pt/205Pt/206Pt, E(cm)=170-220 MeV; 198Pt(64Ni, X), (66Ni, X), (68Ni, X), (70Ni, X), (72Ni, X)202Pt/204Pt/206Pt/208Pt/210Pt, E(cm)=215-260 MeV; calculated production σ for neutron-rich isotopes close to the neutron drip line using stable and radioactive beams. Diffusive multinucleon transfer reaction model.
doi: 10.1103/PhysRevC.89.034622
2011KI25 J.Korean Phys.Soc. 59, 1023s (2011) H.Il.Kim, D.H.Kim, Y.-O.Lee, M.Mun Nuclear Data Evaluations for Silicon Isotopes Induced by Proton, Deuteron and Alpha NUCLEAR REACTIONS 28,29,30Si(p, p'), (d, d'), (α, α'), E=0-200 MeV; calculated, evaluated σ; 28Si(p, p), E=5.93, 17.7, 28.4, 40.2, 51.9, 65, 80, 100, 179 MeV;29Si(p, p), E=10, 40, 80 MeV;30Si(p, p), E=40.8, 180 MeV;28Si(d, d), E=7, 11, 13, 17.9, 29.5, 52, 56 MeV;29Si(d, d), E=10, 12.3 MeV;30Si(d, d), E=10, 11.8, 12.3, 17 MeV;28Si(α, α'), E=5.96, 27, 40, 104, 120, 166 MeV;29Si(α, α'), E=26.3, 28, 41 MeV;30Si(α, α'), E=26.6, 27, 41 MeV; calculated, evaluated σ(θ). TALYS code. Calculations compared to data.
doi: 10.3938/jkps.59.1023
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