NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = Z.H.Wu Found 4 matches. 2023WU05 Nucl.Phys. A1036, 122671 (2023) Z.-H.Wu, H.-B.Fu, T.Zhong, D.Huang, D.-D.Hu, X.-G.Wu α0(980)-meson twist-2 distribution amplitude within the QCD sum rules and investigation of D → α0(980)(→ ηπ)e+ ve
doi: 10.1016/j.nuclphysa.2023.122671
2019CH53 J.Radioanal.Nucl.Chem. 322, 1605 (2019) Y.Chen, S.-H.Huang, R.i-X.Hu, Y.-G.Zhao, L.-L.Li, J.-J.Zhou, C.Li, J.-L.Zhang, Z.-H.Wu Age determination for uranium standard samples by 231Pa/235U radiochronometer
doi: 10.1007/s10967-019-06922-x
2018LI33 Phys.Rev. C 98, 014618 (2018) F.Li, L.Zhu, Z.-H.Wu, X.-B.Yu, J.Su, C.-C.Guo Predictions for the synthesis of superheavy elements Z=119 and 120 NUCLEAR REACTIONS 238U, 242,244Pu, 243Am, 245,248Cm, 249Bk, 249Cf(48Ca, 3n), (48Ca, 4n), (48Ca, 5n), E*=25-60 MeV; calculated evaporation residue σ(E), and compared with available experimental data. 252Es(40Ca, 3n), E(cm)=204.08 MeV; 252Es(42Ca, 3n), E(cm)=203.00 MeV; 249Cf(45Sc, 3n), E(cm)=211.09 MeV; 255Es(40Ca, 4n), E(cm)=207.02 MeV; 254Es(40Ca, 3n), E(cm)=203.60 MeV; 247Bk(47Ti, 3n), E(cm)=219.19 MeV; 248Bk(46Ti, 3n), E(cm)=217.76 MeV; 242Cm(51V, 2n), E(cm)=225.86 MeV; 248Cf(45Sc, 2n), E(cm)=209.29 MeV; 241Am(52Cr, 2n), E(cm)=231.94 MeV; 252Es(44Ca, 3n), E(cm)=204.27 MeV; 253Es(43Ca, 3n), E(cm)=202.49 MeV; 254Es(42Ca, 3n), E(cm)=201.65 MeV; 251Cf(45Sc, 3n), E(cm)=210.03 MeV; 249Bk(47Ti, 3n), E(cm)=217.18 MeV; 248Bk(48Ti, 3n), E(cm)=219.47 MeV; 245Cm(51V, 3n), E(cm)=229.29 MeV; 247Bk(49Ti, 3n), E(cm)=222.17 MeV; 246Cm(50V, 3n), E(cm)=225.70 MeV; 244Cm(51V, 2n), E(cm)=224.00 MeV; 255Es(42Ca, 4n), E(cm)=205.95 MeV; 243Am(53Cr, 3n), E(cm)=236.20 MeV; 254Es(43Ca, 4n), E(cm)=206.90 MeV; 253Es(44Ca, 4n), E(cm)=210.94 MeV; 243Am(52Cr, 2n), E(cm)=229.49 MeV; 254Es(44Ca, 3n), E(cm)=201.64 MeV; 255Es(43Ca, 3n), E(cm)=201.49 MeV; 255Es(44Ca, 4n), E(cm)=207.59 MeV; 252Es(46Ca, 3n), E(cm)=206.00 MeV; 248Bk(50Ti, 3n), E(cm)=222.48 MeV; 247Cm(51V, 3n), E(cm)=226.83 MeV; 254Cf(45Sc, 4n), E(cm)=211.93 MeV; 249Bk(49Ti, 3n), E(cm)=218.88 MeV; 254Es(46Ca, 3n), E(cm)=203.64 MeV; 255Es(46Ca, 4n), E(cm)=210.13 MeV; 252Es(48Ca, 3n), E(cm)=208.42 MeV; 255Es(46Ca, 3n), E(cm)=204.13; 254Es(48Ca, 3n), E(cm)=205.96 MeV; 255Es(48Ca, 4n), E(cm)=212.72 MeV; 242Cm(50Cr, 2n), E(cm)=234.22 MeV; 249Cf(46Ti, 3n), E(cm)=222.89 MeV; 248Cf(46Ti, 2n), E(cm)=219.12 MeV; 257Fm(40Ca, 5n), E(cm)=222.66 MeV; 257Fm(40Ca, 4n), E(cm)=211.66 MeV; 257Fm(40Ca, 3n), E(cm)=205.66 MeV; 251Cf(46Ti, 3n), E(cm)=220.39 MeV; 252Es(45Sc, 3n), E(cm)=214.17 MeV; 250Cf(46Sc, 2n), E(cm)=218.88 MeV; 247Bk(50V, 3n), E(cm)=231.13 MeV; 244Cm(52Cr, 2n), E(cm)=234.88 MeV; 245Cm(52Cr, 3n), E(cm)=240.80 MeV; 243Cm(53Cr, 2n), E(cm)=236.02 MeV; 247Cm(50Cr, 3n), E(cm)=235.12 MeV; 257Fm(42Ca, 3n), E(cm)=205.29 MeV; 254Es(45Sc, 3n), E(cm)=213.40 MeV; 257Fm(43Ca, 4n), E(cm)=210.97 MeV; 257Fm(44Ca, 3n), E(cm)=205.27 MeV; 257Fm(46Ca, 3n), E(cm)=207.84 MeV; 250Cm(53Cr, 3n), E(cm)=234.59 MeV; 257Fm(48Ca, 3n), E(cm)=211.07 MeV; calculated production σ for Z=119 and 120 superheavy isotopes. Dinuclear system (DNS) model.
doi: 10.1103/PhysRevC.98.014618
2018WU06 Phys.Rev. C 97, 064609 (2018) Z.-H.Wu, L.Zhu, F.Li, X.-B.Yu, J.Su, C.-C.Guo Synthesis of neutron-rich superheavy nuclei with radioactive beams within the dinuclear system model NUCLEAR REACTIONS 242,244Pu, 243Am, 245,248,250Cm, 249Bk, 250,251Cf(48Ca, 2n), (48Ca, 3n), (48Ca, 4n), (48Ca, 5n), E*=25-60 MeV; 234Th(42S, 2n), (42S, 3n), (42S, 4n), (42S, 5n), E*=20-65 MeV; 234Th, 244Pu(46Ar, 2n), (46Ar, 3n), (46Ar, 4n), (46Ar, 5n), E*=20-65 MeV; 234Th, 238U, 248Cm, 255Es(44Cl, 2n), (44Cl, 3n), (44Cl, 4n), (44Cl, 5n), E*=20-65 MeV; 228Ra(45Cl, 2n), (45Cl, 3n), (45Cl, 4n), (45Cl, 5n), E*=20-65 MeV; 244Pu, 248Cm(43Cl, 2n), (43Cl, 3n), (43Cl, 4n), (43Cl, 5n), E*=20-65 MeV; 244Pu, 254Cf, 255Es(41S, 2n), (41S, 3n), (41S, 4n), (41S, 5n), E*=20-65 MeV; 257Fm(42Ar, 2n), (42Ar, 3n), (42Ar, 4n), (42Ar, 5n), E*=20-65 MeV; 260Md(38Cl, 2n), (38Cl, 3n), (38Cl, 4n), (38Cl, 5n), E*=20-65 MeV; calculated evaporation residue σ. 228Ra(45Cl, 2n), E*=36.0 MeV; 228Ra(46Cl, 3n), E*=46.0 MeV; 226Ra(47Cl, 2n), E*=36.0 MeV; 234Th(42S, 4n), E*=43.0 MeV; 228Ra(46Ar, 2n), E*=34.0 MeV; 234Th(43S, 5n), E*=51.0 MeV; 234Th(42S, 3n), E*=41.0 MeV; 234Th(43S, 4n), E*=46.0 MeV; 234Th(44S, 5n), E*=59.0 MeV; 234Th(44Cl, 2n), E*=37.0 MeV; 234Th(45Cl, 3n), E*=44.0 MeV; 228Ra(50K, 2n), E*=36.0 MeV; 234Th(46Ar, 2n), E*=34.0 MeV; 238U(43S, 3n), E*=41.0 MeV; 238U(42S, 2n), E*=37.0 MeV; 238U(44Cl, 3n), E*=38.0 MeV; 238U(43Cl, 2n), E*=36.0 MeV; 238U(43S, 3n), E*=41.0 MeV; 234Th(47K, 2n), E*=33.0 MeV; 244Pu(41S, 3n), E*=38.0 MeV; 244Pu(42S, 4n), E*=42.0 MeV; 238U(46Ar, 2n), E*=33.0 MeV; 244Pu(43Cl, 4n), E*=44.0 MeV; 242Pu(44Cl, 3n), E*=37.0 MeV; 244Pu(42Cl, 3n), E*=38.0 MeV; 244Pu(46Ar, 4n), E*=38.0 MeV; 244Pu(45Ar, 3n), E*=44.0 MeV; 242Pu(46Ar, 2n), E*=33.0 MeV; 248Cm(43Cl, 4n), E*=38.0 MeV; 250Cm(42Cl, 5n), E*=43.0 MeV; 248Cm(44Cl, 5n), E*=43.0 MeV; 248Cm(44Cl, 4n), E*=38.0 MeV; 250Cm(42Cl, 4n), E*=39.0 MeV; 250Cm(43Cl, 5n), E*=45.0 MeV; 254Cf(41S, 5n), E*=40.0 MeV; 253Cf(42S, 5n), E*=40.0 MeV; 250Cm(44Ar, 4n), E*=37.0 MeV; 255Es(41S, 5n), E*=40.0 MeV; 254Cf(42Cl, 5n), E*=40.0 MeV; 253Cf(43Cl, 5n), E*=39.0 MeV; 255Es(41S, 4n), E*=37.0 MeV; 253Cf(43Cl, 4n), E*=36.0 MeV; 254Cf(42Cl, 4n), E*=37.0 MeV; 250Cm(48Ca, 4n), E*=35.0 MeV; 248Cm(48Ca, 2n), E*=31.0 MeV; 250Cm(46Ca, 2n), E*=35.0 MeV; 255Es(44Cl, 5n), E*=40.0 MeV; 254Cf(44Ar, 4n), E*=36.0 MeV; 257Fm(41S, 4n), E*=37.0 MeV; 250Cm(48Ca, 3n), E*=31.0 MeV; 255Es(44Cl, 4n), E*=36.0 MeV; 253Cf(46Ar, 4n), E*=34.0 MeV; 254Cf(46Ar, 5n), E*=41.0 MeV; 250Cf(48Ca, 3n), E*=34.0 MeV; 250Cm(49Ti, 4n), E*=42.0 MeV; 252Cf(46Ca, 3n), E*=36.0 MeV; 260Md(38Cl, 3n), E*=41.0 MeV; 260Md(39Cl, 4n), E*=42.0 MeV; 257Fm(42Ar, 4n), E*=41.0 MeV; 251Cf(48Ca, 3n), E*=30.0 MeV; 252Cf(48Ca, 4n), E*=38.0 MeV; 250Cm(49Ti, 3n), E*=34.0 MeV; 257Fm(42Ar, 3n), E*=33.0 MeV; 257Fm(43Ar, 4n), E*=38.0 MeV; 260Md(39Cl, 3n), E*=37.0 MeV; 244Pu(43Cl, n), E*=40.0 MeV; 238Cm(48Ca, 2np), E*=41.0 MeV; 254Cf(41S, 5n), E*=40.0 MeV; 248Cm(48Ca, 2nα), E*=46.0 MeV; 248Cm(43Cl, 4n), E*=38.0 MeV; 242Pu(48Ca, 2np), E*=35.0 MeV; 248Cm(44Cl, 4n), E*=38.0 MeV; 242Pu(48Ca, np), E*=40.0 MeV; 244Pu(48Ca, 3np), E*=45.0 MeV; 255Es(41S, 5n), E*=40.0 MeV; 245Cm(48Ca, np), E*=32.0 MeV; 249Bk(48Ca, 2nα), E*=37.0 MeV; 255Es(41S, 4n), E*=37.0 MeV; 248Cm(48Ca, 3np), E*=44.0 MeV; 249Bk(48Ca, nα), E*=32.0 MeV; calculated evaporation residue σ, and optimal incident beam energies. 48Ca(238U, 2n), (238U, 3n), (238U, 4n), E(cm)=184.13-214.13 MeV; calculated evaporation residue σ, potential energy surface, driving potential, survival and complete fusion probabilities, and capture σ. Dinuclear system model. 271Db, 272,273Sg, 276Bh, 278Hs, 279Mt, 282Ds, 283Rg, 286Cn, 287,288Nh, 290Fl, 291,292Mc, 294,295Lv, 295,296Og; calculated evaporation residue σ, and optimal incident beam energies for various reactions. Comparison with available experimental data. Relevance to synthesis of neutron-rich superheavy nuclei using radioactive ion beams, such as those at ATLAS-ANL.
doi: 10.1103/PhysRevC.97.064609
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