NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = L.G.Cao Found 41 matches. 2024SU01 Phys.Rev. C 109, 014321 (2024) Sh.Sun, L.-G.Cao, F.-Sh.Zhang, H.Sagawa, G.Colo Microscopic study of M1 resonances in Sn isotopes
doi: 10.1103/PhysRevC.109.014321
2024SU06 Eur.Phys.J. A 60, (2024) Sh.Sun, R.-Q.Yu, L.-G.Cao, Ch.-L.Zhang, F.-Sh.Zhang Application of relativistic continuum random phase approximation to giant dipole resonance of 208Pb and 132Sn NUCLEAR STRUCTURE 132Sn, 208Pb; calculated the properties of isovector giant dipole resonances (IVGDR) using the relativistic continuum random phase approximation (RCRPA).
doi: 10.1140/epja/s10050-024-01288-5
2023CH06 Chin.Phys.C 47, 024102 (2023) S.-H.Cheng, J.Wen, L.-G.Cao, F.-S.Zhang Neutron skin thickness of 90Zr and symmetry energy constrained by charge exchange spin-dipole excitations NUCLEAR REACTIONS 90Zr(p, n), (n, p), E<50 MeV; analyzed available data. 90Zr; deduced charge exchange spin-dipole (SD) excitations using the Skyrme Hartee-Fock plus proton-neutron random phase approximation with SAMi-J interactions, neutron skin thickness.
doi: 10.1088/1674-1137/aca38e
2022AN05 Phys.Rev. C 105, 014325 (2022) R.An, X.Jiang, L.-G.Cao, F.-S.Zhang Odd-even staggering and shell effects of charge radii for nuclei with even Z from 36 to 38 and from 52 to 62 NUCLEAR STRUCTURE 72,73,74,75,76,77,78,79,80,81,82,83,84,85,86,87,88,89,90,91,92,93,94,95,96,97,98,99,100,101,102Kr, 74,75,76,77,78,79,80,81,82,83,84,85,86,87,88,89,90,91,92,93,94,95,96,97,98,99,100,101,102,103,104Sr, 110,111,112,113,114,115,116,117,118,119,120,121,122,123,124,125,126,127,128,129,130,131,132,133,134,135,136,137,138,139,140,141,142,143,144,145,146,147,148,149,150Te, 110,111,112,113,114,115,116,117,118,119,120,121,122,123,124,125,126,127,128,129,130,131,132,133,134,135,136,137,138,139,140,141,142,143,144,145,146,147,148,149,150,151,152,153,154,155,156Xe, 116,117,118,119,120,121,122,123,124,125,126,127,128,129,130,131,132,133,134,135,136,137,138,139,140,141,142,143,144,145,146,147,148,149,150,151,152,153,154,155,156,157,158,159,160,161,162Ba, 126,127,128,129,130,131,132,133,134,135,136,137,138,139,140,141,142,143,144,145,146,147,148,149,150,151,152,153,154,155,156,157,158Ce, 126,127,128,129,130,131,132,133,134,135,136,137,138,139,140,141,142,143,144,145,146,147,148,149,150,151,152,153,154,155,156,157,158,159,160Nd, 130,131,132,133,134,135,136,137,138,139,140,141,142,143,144,145,146,147,148,149,150,151,152,153,154,155,156,157,158,159,160,161,162,163,164,165Sm; calculated charge radii and odd-even staggering (OES) effects by the relativistic mean field (RMF-BCS) and the modified RMF(BCS)* approaches; deduced no significant influence of neutron-proton short-range correlations (np-SRCs) for some nuclei due to the strong coupling between different levels around Fermi surface. Comparison with available experimental data.
doi: 10.1103/PhysRevC.105.014325
2022AN16 Chin.Phys.C 46, 064101 (2022) R.An, X.Jiang, L.-G.Cao, F.-S.Zhang Evolution of nuclear charge radii in copper and indium isotopes NUCLEAR STRUCTURE 57,58,59,60,61,62,63,64,65,66,67,68,69,70,71,72,73,74,75,76,77,78,79,80,81Cu, 99,100,101,102,103,104,105,106,107,108,109,110,111,112,113,114,115,116,117,118,119,120,121,122,123,124,125,126,127,128,129,130,131,132,133,134,135,136,137,138,139In; calculated rms charge radii using the relativistic mean field (RMF) model with NL3, PK1 and NL3* parameter sets. Comparison with experimental data.
doi: 10.1088/1674-1137/ac501a
2021LI26 Chin.Phys.C 45, 044105 (2021) L.Liu, S.Liu, S.-S.Zhang, L.-G.Cao Isovector giant dipole resonances in proton-rich Ar and Ca isotopes NUCLEAR STRUCTURE 30,32,34Ar, 32,34,36Ca; analyzed available data; calculated energy levels, J, π, proton and neutron density distributions using Skyrme HF+BCS and HF+BCSR approximation with the SLy5 parameter set. QRPA strength distributions, proton and neutron transition densities for the PDR states and GDR states.
doi: 10.1088/1674-1137/abdfbc
2021LI27 Chin.Phys.C 45, 044110 (2021) L.Liu, S.Liu, S.-S.Zhang, L.-G.Cao Systematic study of two-proton radioactivity within a Gamow-like model RADIOACTIVITY 6Be, 12O, 16Ne, 19Mg, 45Fe, 48Ni, 54Zn, 67Kr(2p), 22Si, 26S, 34Ca, 36Sc, 38,39Ti, 40V, 42Cr, 47Co, 49Ni, 56Ga, 58,59,60Ge, 61As, 10N, 28Cl, 32K, 57Ga, 60,62As, 52Cu(2p); calculated T1/2. Comparison with available data.
doi: 10.1088/1674-1137/abe10f
2021SU19 Chin.Phys.C 45, 094101 (2021) S.Sun, S.-S.Zhang, Z.-H.Zhang, L.-G.Cao Effect of pairing correlation on low-lying quadrupole states in Sn isotopes NUCLEAR STRUCTURE 102,104,106,108,110,112,114,116,118,120,122,124,126,128,130,132,134Sn; calculated neutron pairing gaps, 2+ states energies, B(E2) in the framework of fully self-consistent Hartree-Fock+BCS plus QRPA.
doi: 10.1088/1674-1137/ac0b39
2021WE03 Chin.Phys.C 45, 014105 (2021) P.-W.Wen, S.-S.Zhang, L.G.Cao, F.-S.Zhang Fully self-consistent calculation of β-decay half-lives within Skyrme energy density functional RADIOACTIVITY 22,24O, 34,42Si, 52Ca, 68,78Ni, 82Ge, 102Sr, 104,110Zr, 132Sn, 150Ce(β-); calculated T1/2 using Skyrme HF plus charge-exchange RPA approach with SGII, LNS, SKX, and SAMi interactions. Comparison with experimental data.
doi: 10.1088/1674-1137/abc1d1
2019CA22 Phys.Rev. C 100, 054324 (2019) L.-G.Cao, S.-S.Zhang, H.Sagawa Quenching factor of Gamow-Teller and spin dipole giant resonances NUCLEAR STRUCTURE 48Ca, 90Zr, 132Sn, 208Pb; calculated Gamow-Teller (GT) and spin-dipole (SD) strength distributions, and sum rules of GT-, SD-, and SD+ resonances using self-consistent Hartree-Fock plus random phase approximation (RPA) method, with Skyrme forces SAMi and SAMi-T with and tensor interactions. Comparison with available experimental data.
doi: 10.1103/PhysRevC.100.054324
2017LV02 Chin.Phys.Lett. 34, 082101 (2017) H.Lv, S.-S.Zhang, Z.-H.Zhang, Y.-Q.Wu, L.-G.Cao Pygmy and Giant dipole Resonances in Proton-Rich Nuclei 17, 18Ne* NUCLEAR STRUCTURE 17,18Ne; calculated particle density, total binding energies, neutron and proton Fermi energies, rms and charge radii, response functions, dipole strengths. Skyrme Hartree-Fock with the Bardeen-Cooper-Schrieffer approximation to take into account the pairing correlation.
doi: 10.1088/0256-307x/34/8/082101
2016RO25 Phys.Rev. C 94, 044313 (2016) X.Roca-Maza, L.-G.Cao, G.Colo, H.Sagawa Fully self-consistent study of charge-exchange resonances and the impact on the symmetry energy parameters NUCLEAR STRUCTURE 90Zr, 208Pb; calculated energy of the IAS and strength for 90Zr, single-particle proton levels in 208Pb, energy of the IAS as a function of neutron skin in 208Pb, energy difference between the anti-analog giant dipole resonance (AGDR) and the isobaric analog state; deduced correlations between the neutron-skin thickness and either the symmetry energy at saturation density or the corresponding slope parameter. HF+RPA calculations with the exchange term of the two-body Coulomb interaction treated exactly without Slater approximation, and the two-parameters spin-orbit interaction is treated in a consistent way within the energy density functional theory using several SAMi-J interactions. Comparison with available experimental information.
doi: 10.1103/PhysRevC.94.044313
2016ZH15 Phys.Rev. C 93, 044329 (2016) S.S.Zhang, L.G.Cao, U.Lombardo, P.Schuck Medium polarization in asymmetric nuclear matter
doi: 10.1103/PhysRevC.93.044329
2015CA20 Phys.Rev. C 92, 034308 (2015) L.-G.Cao, X.Roca-Maza, G.Colo, H.Sagawa Constraints on the neutron skin and symmetry energy from the anti-analog giant dipole resonance in 208Pb NUCLEAR STRUCTURE 208Pb; calculated neutron skin thickness, energies of anti-analog giant dipole resonance (AGDR), isobaric analog state (IAS) and isovector giant dipole resonance (IVGDR). Droplet model, and fully self-consistent Hartree-Fock (HF) plus charge-exchange random phase approximation (RPA) framework. Comparison with experimental data.
doi: 10.1103/PhysRevC.92.034308
2014CA07 Phys.Rev. C 89, 044314 (2014) L.-G.Cao, G.Colo, H.Sagawa, P.F.Bortignon Properties of single-particle states in a fully self-consistent particle-vibration coupling approach NUCLEAR STRUCTURE 40Ca, 208Pb; calculated levels, J, π, B(Eλ), energies of neutron single-particle states, spectroscopic factors, effective neutron mass around Fermi surface. Fully self-consistent particle-vibration coupling (PVC) approach within the framework of Skyrme energy density functional theory with SLy5 and T44 parameter sets, and random phase approximation for phonons. Comparison with experimental data.
doi: 10.1103/PhysRevC.89.044314
2014WE02 Phys.Rev. C 89, 044311 (2014) P.Wen, L.-G.Cao, J.Margueron, H.Sagawa Spin-isospin response in finite nuclei from an extended Skyrme interaction NUCLEAR STRUCTURE 48Ca, 90Zr, 208Pb; calculated centroid energies of low and high energy peaks of Gamow-Teller (GT) response functions, RPA response function and energies of GT and magnetic dipole excitations with and without spin-density dependent terms. Fully self-consistent Hartree-Fock (HF) plus random phase approximation (RPA) with Skyrme interaction with spin and spin-isospin densities. Comparison with experimental data.
doi: 10.1103/PhysRevC.89.044311
2013KH08 Phys.Rev. C 87, 064311 (2013) E.Khan, N.Paar, D.Vretenar, L.-G.Cao, H.Sagawa, G.Colo Incompressibility of finite fermionic systems: Stable and exotic atomic nuclei NUCLEAR STRUCTURE Z=50, A=94-168; Z=82, A=170-262; calculated nuclear incompressibility using microscopic Skyrme-CHFB method, the Skyrme-QRPA, and the relativistic QRPA. 110,114,118,122,126,130,134,138,142,146Sn, 200,204,208,212,216,220,224,228,232,236Pb; calculated isoscalar monopole response, nuclear compressibility using the relativistic QRPA with the DD-ME2 functional and the QRPA with the functional SLy5.
doi: 10.1103/PhysRevC.87.064311
2013RO08 Phys.Rev. C 87, 034301 (2013) X.Roca-Maza, M.Brenna, B.K.Agrawal, P.F.Bortignon, G.Colo, L.-G.Cao, N.Paar, D.Vretenar Giant quadrupole resonances in 208Pb, the nuclear symmetry energy, and the neutron skin thickness NUCLEAR STRUCTURE 208Pb; calculated strength functions, neutron and proton transition densities, excitation energies of isoscalar and isovector giant quadrupole resonance (ISGQR and IVGQR), neutron skin thickness, symmetry energy. Macroscopic approach based on quantal harmonic oscillator model, and microscopic approach based on nonrelativistic and covariant energy density functionals (EDF) within the RPA. Comparison with experimental data.
doi: 10.1103/PhysRevC.87.034301
2013YA23 Chin.Phys.C 37, 124102 (2013) Collective multipole excitations of exotic nuclei in relativistic continuum random phase approximation NUCLEAR STRUCTURE 34,40,48,60Ca, 16,28O, 100,132Sn; calculated isoscalar and isovector collective multipole excitations, strength functions. Comparison with available data.
doi: 10.1088/1674-1137/37/12/124102
2012CA33 Prog.Theor.Phys.(Kyoto), Suppl. 196, 322 (2012) Effect of Tensor Force on the Multipole Resonances of Finite Nuclei NUCLEAR STRUCTURE 208Pb; analyzed available data; deduced the necessity to include the tensor component of the Skyrme force in mean field theory.
doi: 10.1143/PTPS.196.322
2012CA38 Phys.Rev. C 86, 054313 (2012) Microscopic study of the isoscalar giant monopole resonance in Cd, Sn, and Pb isotopes NUCLEAR STRUCTURE 106,110,112,114,116Cd, 112,114,116,118,120,122,124Sn, 204,206,208Pb; calculated isoscalar giant monopole resonance (ISGMR) strength distributions, centroids, scaling, constrained and peak energies using the self-consistent Skyrme Hartree-Fock+BCS and quasiparticle random phase approximation (QRPA). Comparison with experimental data.
doi: 10.1103/PhysRevC.86.054313
2011CA07 Phys.Rev. C 83, 034324 (2011) Effects of tensor correlations on low-lying collective states in finite nuclei NUCLEAR STRUCTURE 208Pb; calculated levels, J, π, B(M1), B(E2), B(E3), p-h matrix elements. 40Ca; calculated levels, J, π, B(E3), p-h matrix elements. Fully self-consistent random phase approximation with Skyrme interactions including tensor correlations.
doi: 10.1103/PhysRevC.83.034324
2011DO12 Phys.Rev. C 84, 014303 (2011) J.M.Dong, W.Zuo, J.Z.Gu, Y.Z.Wang, L.G.Cao, X.Z.Zhang Effects of tensor interaction on pseudospin energy splitting and shell correction NUCLEAR STRUCTURE 106,108,110,112,114,116,118,120,122,124,126,128,130,132,134Sn; calculated proton and neutron pseudospin orbit splittings. 132Sn, 298Fl; calculated neutron and proton shell correction energies, single particle spectra. Skyrme-Hartree-Fock approach with the SLy5+TF and T31+TF parameter sets combined with the BCS method.
doi: 10.1103/PhysRevC.84.014303
2010CA11 Phys.Rev. C 81, 041301 (2010) A.Carbone, G.Colo, A.Bracco, L.-G.Cao, P.F.Bortignon, F.Camera, O.Wieland Constraints on the symmetry energy and neutron skins from pygmy resonances in 68Ni and 132Sn NUCLEAR STRUCTURE 68Ni, 132Sn, 208Pb; calculated dipole strength function, neutron symmetry energy, neutron skin radius, and EWSR from pygmy dipole resonances using random-phase approximation (RPA). Comparison with experimental data.
doi: 10.1103/PhysRevC.81.041301
2010CA13 Phys.Rev. C 81, 044302 (2010) Spin and spin-isospin instabilities and Landau parameters of Skyrme interactions with tensor correlations
doi: 10.1103/PhysRevC.81.044302
2010YA20 Phys.Rev. C 82, 054305 (2010) D.Yang, L.-G.Cao, Y.Tian, Z.-Y.Ma Importance of self-consistency in relativistic continuum random-phase approximation calculations NUCLEAR STRUCTURE 40Ca, 132Sn, 208Pb; calculated inverse energy-weighted moments and strength distributions of isoscalar giant-monopole resonances (ISGMR), isovector giant-monopole resonances (IVGMR), isoscalar giant-quadrupole resonances (ISGQR), isovector giant-quadrupole resonances (IVGQR) using relativistic continuum random phase approximation (RCRPA) method.
doi: 10.1103/PhysRevC.82.054305
2010ZH10 Phys.Rev. C 81, 044313 (2010) S.S.Zhang, L.G.Cao, U.Lombardo, E.G.Zhao, S.G.Zhou Isospin-dependent pairing interaction from nuclear matter calculations
doi: 10.1103/PhysRevC.81.044313
2009CA32 Phys.Rev. C 80, 064304 (2009) L.-G.Cao, G.Colo, H.Sagawa, P.F.Bortignon, L.Sciacchitano Effects of the tensor force on the multipole response in finite nuclei NUCLEAR STRUCTURE 40,48Ca, 208Pb; calculated isoscalar quadrupole (2+), isoscalar octupole (3-), and isoscalar and isovector magnetic-dipole (1+) strength functions using self-consistent random phase approximation (RPA) model with Skyrme interactions. Comparison with experimental data.
doi: 10.1103/PhysRevC.80.064304
2009CA34 Chin.Phys.C 33, Supplement 1, 33 (2009) L.-G.Cao, U.Lombardo, P.Schuck Superfluid nuclear matter in BCS theory and beyond
doi: 10.1088/1674-1137/33/S1/011
2009YA02 Chin.Phys.Lett. 26, 022101 (2009) Isoscalar Giant Monopole Resonance in Relativistic Continuum Random Phase Approximation NUCLEAR STRUCTURE 120Sn, 208Pb; calculated Isoscalar Giant Monopole resonance strength in the framework of relativistic continuum random phase approximation.
doi: 10.1088/0256-307X/26/2/022101
2008CA10 Chin.Phys.Lett. 25, 1625 (2008) Symmetry Energy and Isovector Giant Dipole Resonance in Finite Nuclei NUCLEAR STRUCTURE 90Zr, 132Sn, 144Sm, 208Pb; calculated IVGDR energies as a function of symmetry energy using relativistic mean field theory.
doi: 10.1088/0256-307X/25/5/028
2006CA04 Phys.Rev. C 73, 014313 (2006) L.G.Cao, U.Lombardo, C.W.Shen, N.Van Giai From Brueckner approach to Skyrme-type energy density functional NUCLEAR STRUCTURE 16O, 40,48Ca, 56,78Ni, 90Zr, 100,132Sn, 208Pb; calculated radii, binding energies, spin-orbit potentials, particle densities. Skyrme-type energy density functional.
doi: 10.1103/PhysRevC.73.014313
2006CA34 Phys.Rev.C 74, 064301 (2006) Screening effects in superfluid nuclear and neutron matter within Brueckner theory
doi: 10.1103/PhysRevC.74.064301
2006MA82 Int.J.Mod.Phys. E15, 1347 (2006) Z.-Yu.Ma, B.-Q.Chen, J.Liang, L.-G.Cao Giant resonances and asymmetry energy NUCLEAR STRUCTURE 70,72,74,76,78,80,82,84,86,88,90,92,94,96Ni; calculated GDR energies. 132Sn, 208Pb; calculated asymmetry energy, giant resonance strength. Relativistic quasiparticle RPA.
doi: 10.1142/S0218301306004934
2005ZU03 Phys.Rev. C 72, 014005 (2005) W.Zuo, L.G.Cao, B.A.Li, U.Lombardo, C.W.Shen Isospin splitting of the nucleon mean field
doi: 10.1103/PhysRevC.72.014005
2004CA17 Chin.Phys.Lett. 21, 810 (2004) Isoscalar Giant Resonances of 120Sn in the Quasiparticle Relativistic Random Phase Approximation NUCLEAR STRUCTURE 120Sn; calculated giant resonance response functions. Quasiparticle relativistic RPA.
doi: 10.1088/0256-307X/21/5/013
2004CA44 Eur.Phys.J. A 22, 189 (2004) Effect of resonant continuum on pairing correlations in the relativistic approach NUCLEAR STRUCTURE 68,70,72,74,76,78,80,82,84,86,88,90,92,94,96,98Ni; calculated pairing energies, binding energies, two-neutron separation energies, radii. Relativistic approach, role of resonant continuum discussed.
doi: 10.1140/epja/i2004-10029-5
2003CA33 Chin.Phys.Lett. 20, 1459 (2003) Isovector Giant Dipole Resonance of Stable Nuclei in a Consistent Relativistic Random-phase Approximation NUCLEAR STRUCTURE 40Ca, 90Zr, 116Sn, 208Pb; A=10-250; calculated isovector GDR energies. Relativistic RPA, comparisons with data.
doi: 10.1088/0256-307X/20/9/314
2003MA71 Nucl.Phys. A722, 491c (2003) Z.Ma, L.-G.Cao, Nguyen Van Giai, P.Ring Giant resonances of stable and exotic nuclei in relativistic RPA NUCLEAR STRUCTURE 208Pb, 32,34,40,48,60,70Ca; calculated giant resonance response functions. A=10-240; calculated isovector GDR energies. Relativistic RPA approach.
doi: 10.1016/S0375-9474(03)01414-3
2002MA27 Nucl.Phys. A703, 222 (2002) Z.-Y.Ma, A.Wandelt, V.G.Nguyen, D.Vretenar, P.Ring, L.-G.Cao Collective Multipole Excitations in a Microscopic Relativistic Approach NUCLEAR STRUCTURE 16O, 40,48Ca, 90Zr, 208Pb; calculated giant resonance strength distributions. 208Pb; calculated transitions B(Eλ). Relativistic RPA, comparisons with data.
doi: 10.1016/S0375-9474(01)01598-6
2001RI17 Nucl.Phys. A694, 249 (2001) P.Ring, Z.-Y.Ma, V.G.Nguyen, D.Vretenar, A.Wandelt, L.-G.Cao The Time-Dependent Relativistic Mean-Field Theory and the Random Phase Approximation NUCLEAR STRUCTURE 116Sn; calculated isoscalar giant monopole resonance strength distribution. Relativistic RPA, time-dependent relativistic mean field theory.
doi: 10.1016/S0375-9474(01)00986-1
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