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Search: Author = N.Tang

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2023LI17      Int.J.Mod.Phys. E32, 2330002 (2023)

J.-J.Li, N.Tang, Y.-H.Zhang, M.-H.Zhang, C.Wang, X.-R.Zhang, L.Zhu, F.-S.Zhang

Progress on production cross-sections of unknown nuclei in fusion evaporation reactions and multinucleon transfer reactions

NUCLEAR REACTIONS 232Th(204Hg, X), E(cm)=678.1 MeV; 249Bk(238U, X), E(cm)=823.4 MeV; 248Cm(238U, X), E(cm)=824.9 MeV; calculated σ in fusion evaporation (FE) reactions and multinucleon transfer (MNT) reactions.

doi: 10.1142/S0218301323300023
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2023TA03      Phys.Rev. C 107, 014603 (2023)

N.Tang, B.Li, J.-J.Li, F.-S.Zhang

Production of 61Ca, 63Sc, 65Ti, 68, 69V, 71Cr, 77Fe and 79Co in projectile fragmentation with radioactive ion beams at 1A GeV

NUCLEAR REACTIONS 9Be(69Cu, X)37Ar/38Ar/39Ar/40Ar/41Ar/42Ar/43Ar/44Ar/39K/40K/41K/42K/43K/44K/45K/46K/41Ca/42Ca/43Ca/44Ca/45Ca/46Ca/47Ca/43Sc/44Sc/45Sc/46Sc/47Sc/48Sc/49Sc/50Sc/45Ti/46Ti/47Ti/48Ti/49Ti/50Ti/51Ti/52Ti/48V/49V/50V/51V/52V/53V/54V/55V/50Cr/51Cr/52Cr/53Cr/54Cr/55Cr/56Cr/57Cr/53Mn/54Mn/55Mn/56Mn/57Mn/58Mn/59Mn, E=98.1 MeV/nucleon; calculated isotopes production σ. 9Be(81Ga, X)48Ca/49Ca/50Ca/51Ca/52Ca/53Ca/54Ca/55Ca/56Ca/49Sc/50Sc/51Sc/52Sc/53Sc/54Sc/55Sc/56Sc/57Sc/58Sc/59Sc/60Sc/52Ti/53Ti/54Ti/55Ti/56Ti/57Ti/58Ti/59Ti/60Ti/61Ti/62Ti/63Ti/56V/57V/58V/59V/60V/61V/62V/63V/64V/65V/56Cr/57Cr/58Cr/59Cr/60Cr/61Cr/62Cr/63Cr/64Cr/65Cr/66Cr/67Cr/59Mn/60Mn/61Mn/62Mn/63Mn/64Mn/65Mn/66Mn/67Mn/68Mn/69Mn/62Fe/63Fe/64Fe/65Fe/66Fe/67Fe/68Fe/69Fe/70Fe/71Fe/72Fe/64Co/65Co/66Co/67Co/68Co/69Co/70Co/71Co/72Co/73Co, E=1 GeV/nucleon; 9Be(84Ga, X)48Ca/49Ca/50Ca/51Ca/52Ca/53Ca/54Ca/55Ca/56Ca/57Ca/58Ca/59Ca/60Ca/51Sc/52Sc/53Sc/54Sc/55Sc/56Sc/57Sc/58Sc/59Sc/60Sc/61Sc/53Ti/54Ti/55Ti/56Ti/57Ti/58Ti/59Ti/60Ti/61Ti/62Ti/63Ti/64Ti/57V/58V/59V/60V/61V/62V/63V/64V/65V/66V/58Cr/59Cr/60Cr/61Cr/62Cr/63Cr/64Cr/65Cr/66Cr/67Cr/68Cr/69Cr/60Mn/61Mn/62Mn/63Mn/64Mn/65Mn/66Mn/67Mn/68Mn/69Mn/70Mn/71Mn/72Mn/64Fe/65Fe/66Fe/67Fe/68Fe/69Fe/70Fe/71Fe/72Fe/73Fe/74Fe/75Fe/66Co/67Co/68Co/69Co/70Co/71Co/72Co/73Co/74Co/75Co/76Co/77Co, E=1 GeV/nucleon; 9Be(86Ga, X)48Ca/49Ca/50Ca/51Ca/52Ca/53Ca/54Ca/55Ca/56Ca/57Ca/58Ca/59Ca/60Ca/61Ca/51Sc/52Sc/53Sc/54Sc/55Sc/56Sc/57Sc/58Sc/59Sc/60Sc/61Sc/62Sc/63Sc/54Ti/55Ti/56Ti/57Ti/58Ti/59Ti/60Ti/61Ti/62Ti/63Ti/64Ti/65Ti/57V/58V/59V/60V/61V/62V/63V/64V/65V/66V/67V/68V/69V/59Cr/60Cr/61Cr/62Cr/63Cr/64Cr/65Cr/66Cr/67Cr/68Cr/69Cr/70Cr/71Cr/62Mn/63Mn/64Mn/65Mn/66Mn/67Mn/68Mn/69Mn/70Mn/71Mn/72Mn/73Mn/74Mn/75Mn/65Fe/66Fe/67Fe/68Fe/69Fe/70Fe/71Fe/72Fe/73Fe/74Fe/75Fe/76Fe/77Fe/67Co/68Co/69Co/70Co/71Co/72Co/73Co/74Co/75Co/76Co/77Co/78Co/79Co, E=1 GeV/nucleon; calculated isotopes production σ. Isospin-dependent Boltzmann-Langevin equation (IBLE) model. Comparison of model predictions with experimental data for 9Be(69Cu, X) reaction.

doi: 10.1103/PhysRevC.107.014603
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2023ZH09      Phys.Rev. C 107, 024604 (2023)

Y.-H.Zhang, J.-J.Li, N.Tang, X.-R.Zhang, Z.Liu, F.-S.Zhang

Production cross sections of new neutron-rich isotopes with Z=92-106 in the multinucleon transfer reaction 197Au + 232Th

NUCLEAR REACTIONS 232Th(197Au, X)258Es/259Es/260Es/261Es/262Es/260Fm/261Fm/262Fm/263Fm/261Md/262Md/263Md/264Md/265Md/261No/263No/264No/265No/266No/267No/263Lr/265Lr/267Lr/268Lr/264Rf/266Rf/268Rf/269Rf/270Rf/264Db/265Db/269Db/271Db/267Sg/268Sg/270Sg/272Sg/273Sg, E(cm)=690.69;232Th(197Au, X)243U/244U/245U/246U/247U/248U/249U/246Np/247Np/248Np/249Np/250Np/251Np/252Np/248Pu/249Pu/250Pu/251Pu/252Pu/253Pu/254Pu/248Am/249Am/250Am/251Am/252Am/253Am/254Am/255Am/256Am/252Cm/253Cm/254Cm/255Cm/256Cm/257Cm/258Cm/252Bk/254Bk/255Bk/256Bk/257Bk/258Bk/259Bk/257Cf/258Cf/259Cf/260Cf/261Cf/258Es/259Es/260Es/261Es/262Es, E(cm)=756.47 MeV; calculated production σ. 232Th(197Au, X), E=690.7, 723.6, 756.5 MeV;232Th(186W, X), E=681, 2 MeV;232Th(238U, X), E=823.8; calculated final isotopic production σ for U, Np, Pu, Am, Cm, Bk, Cf, Es, Fm, Md, No, Lr, Rf, Db and Sg isotopes, calculated driving potentials, potential energy surfaces. 232Th(197Au, X), E=690.7, 723.6, 756.5, 789.4 MeV; interaction time as a function of the impact parameter. 249Cf(136Xe, X), E(cm)=567 MeV; calculated final production σ for Pu, Am, Cm, Bk, Cf, Es isotopes. Calculations performed within the framework of dinuclear system (DNS) model with a decay model GEMINI++. Comparison to experimental data.

doi: 10.1103/PhysRevC.107.024604
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2022LI39      Phys.Rev. C 106, 014606 (2022)

J.-J.Li, N.Tang, Y.-H.Zhang, X.-R.Zhang, G.Zhang, F.-S.Zhang

Theoretical study on the production of neutron-rich transuranium nuclei with radioactive beams in multinucleon transfer reactions

NUCLEAR REACTIONS 248Cm(136Xe, X)229Pu/230Pu/231Pu/232Pu/233Pu/234Pu/235Pu/236Pu/237Pu/238Pu/239Pu/240Pu/241Pu/242Pu/243Pu/244Pu/245Pu/246Pu/247Pu/248Pu/249Pu/250Pu/251Pu/252Pu/253Pu/254Pu/233Am/234Am/235Am/236Am/237Am/238Am/239Am/240Am/241Am/242Am/243Am/244Am/245Am/246Am/247Am/248Am/249Am/250Am/251Am/252Am/253Am/254Am/255Am/235Cm/236Cm/237Cm/238Cm/239Cm/240Cm/241Cm/242Cm/243Cm/244Cm/245Cm/246Cm/247Cm/248Cm/249Cm/250Cm/251Cm/252Cm/253Cm/254Cm/255Cm/256Cm/257Cm/258Cm/238Bk/239Bk/240Bk/241Bk/242Bk/243Bk/244Bk/245Bk/246Bk/247Bk/248Bk/249Bk/250Bk/251Bk/252Bk/253Bk/254Bk/255Bk/256Bk/257Bk/258Bk/259Bk/260Bk/240Cf/241Cf/242Cf/243Cf/244Cf/245Cf/246Cf/247Cf/248Cf/249Cf/250Cf/251Cf/252Cf/253Cf/254Cf/255Cf/256Cf/257Cf/258Cf/259Cf/260Cf/261Cf/243Es/244Es/245Es/246Es/247Es/248Es/249Es/250Es/251Es/252Es/253Es/254Es/255Es/256Es/257Es/258Es/259Es/260Es/261Es/262Es , E(cm)=533 MeV; 249Cf(136Xe, X)229Pu/230Pu/231Pu/232Pu/233Pu/234Pu/235Pu/236Pu/237Pu/238Pu/239Pu/240Pu/241Pu/242Pu/243Pu/244Pu/245Pu/246Pu/247Pu/248Pu/249Pu/250Pu/251Pu/252Pu/253Pu/230Am/231Am/232Am/233Am/234Am/235Am/236Am/237Am/238Am/239Am/240Am/241Am/242Am/243Am/244Am/245Am/246Am/247Am/248Am/249Am/250Am/251Am/252Am/253Am/254Am/255Am/233Cm/234Cm/235Cm/236Cm/237Cm/238Cm/239Cm/240Cm/241Cm/242Cm/243Cm/244Cm/245Cm/246Cm/247Cm/248Cm/249Cm/250Cm/251Cm/252Cm/253Cm/254Cm/255Cm/256Cm/257Cm/258Cm/236Bk/237Bk/238Bk/239Bk/240Bk/241Bk/242Bk/243Bk/244Bk/245Bk/246Bk/247Bk/248Bk/249Bk/250Bk/251Bk/252Bk/253Bk/254Bk/255Bk/256Bk/257Bk/258Bk/259Bk/260Bk/237Cf/238Cf/239Cf/240Cf/241Cf/242Cf/243Cf/244Cf/245Cf/246Cf/247Cf/248Cf/249Cf/250Cf/251Cf/252Cf/253Cf/254Cf/255Cf/256Cf/257Cf/258Cf/259Cf/260Cf/261Cf/240Es/241Es/242Es/243Es/244Es/245Es/246Es/247Es/248Es/249Es/250Es/251Es/252Es/253Es/254Es/255Es/256Es/257Es/258Es/259Es/260Es, E(cm)=526 MeV; 238U(92Kr, X)/229Np/230Np/231Np/232Np/233Np/234Np/235Np/236Np/237Np/238Np/239Np/240Np/241Np/242Np/243Np/244Np/234Pu/235Pu/236Pu/237Pu/238Pu/239Pu/240Pu/241Pu/242Pu/243Pu/244Pu/245Pu/246Pu/247Pu/238Am/239Am/240Am/241Am/242Am/243Am/244Am/245Am/246Am/247Am/248Am/249Am/250Am/251Am/252Am/242Cm/243Cm/244Cm/245Cm/246Cm/247Cm/248Cm/249Cm/250Cm/251Cm/252Cm/253Cm/254Cm/255Cm/256Cm/242Bk/243Bk/244Bk/245Bk/246Bk/247Bk/248Bk/249Bk/250Bk/251Bk/252Bk/253Bk/254Bk/242Cf/243Cf/244Cf/245Cf/246Cf/247Cf/248Cf/249Cf/250Cf/251Cf/252Cf/253Cf/254Cf/255Cf/256Cf, E(cm)=357 MeV; 238U(132Sn, X), 230Np/231Np/232Np/233Np/234Np/235Np/236Np/237Np/238Np/239Np/240Np/241Np/242Np/243Np/244Np/245Np/246Np/247Np/248Np/249Np/250Np/251Np/252Np/253Np/254Np/255Np/232Pu/233Pu/234Pu/235Pu/236Pu/237Pu/238Pu/239Pu/240Pu/241Pu/242Pu/243Pu/244Pu/245Pu/246Pu/247Pu/248Pu/249Pu/250Pu/251Pu/252Pu/253Pu/254Pu/255Pu/256Pu/257Pu/236Am/237Am/238Am/239Am/240Am/241Am/242Am/243Am/244Am/245Am/246Am/247Am/248Am/249Am/250Am/251Am/252Am/253Am/254Am/255Am/256Am/257Am/235Cm/236Cm/237Cm/238Cm/239Cm/240Cm/241Cm/242Cm/243Cm/244Cm/245Cm/246Cm/247Cm/248Cm/249Cm/250Cm/251Cm/252Cm/253Cm/254Cm/255Cm/256Cm/257Cm/258Cm/259Cm/260Cm/261Cm/242Bk/243Bk/244Bk/245Bk/246Bk/247Bk/248Bk/249Bk/250Bk/251Bk/252Bk/253Bk/254Bk/255Bk/256Bk/257Bk/258Bk/259Bk/260Bk/261Bk/262Bk/244Cf/245Cf/246Cf/247Cf/248Cf/249Cf/250Cf/251Cf/252Cf/253Cf/254Cf/255Cf/256Cf/257Cm/258Cm/259Cm/260Cm/261Cm/262Cm/263Cm/264Cm, E(cm)=478, 521, 564 MeV; 238U(144Xe, X), 236Np/237Np/238Np/239Np/240Np/241Np/242Np/243Np/244Np//245Np/246Np/247Np/248Np/249Np/250Np/235Pu/236Pu/237Pu/238Pu/239Pu/240Pu/241Pu/242Pu/243Pu/244Pu/245Pu/246Pu/247Pu/248Pu/249Pu/250Pu/251Pu/252Pu/240Am/241Am/242Am/243Am/244Am/245Am/246Am/247Am/248Am/249Am/250Am/251Am/252Am/253Am/254Am/243Cm/244Cm/245Cm/246Cm/247Cm/248Cm/249Cm/250Cm/251Cm/252Cm/253Cm/254Cm/255Cm/241Bk/242Bk/243Bk/244Bk/245Bk/246Bk/247Bk/248Bk/249Bk/250Bk/251Bk/252Bk/253Bk/254Bk/255Bk/265Bk/246Cf/247Cf/248Cf/249Cf/250Cf/251Cf/252Cf/253Cf/254Cf/255Cf/256Cf/257Cm/258Cm/259Cm/260Cm/261Cm/262Cm, E(cm)=511 MeV; calculated σ of the isotopes production, driving potential during the transfer of nucleons. Dinuclear system model (DNS) calculations performed with GEMINI++ code. Comparison to experimental data.

doi: 10.1103/PhysRevC.106.014606
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2022TA17      Phys.Rev. C 106, 034601 (2022)

N.Tang, X.-R.Zhang, J.-J.Li, P.-W.Wen, F.-S.Zhang

Production of unknown neutron-rich isotopes with Z=99-102 in multinucleon transfer reactions near the Coulomb barrier

NUCLEAR REACTIONS 248Cm(86Kr, X)235Am/236Am/237Am/238Am/239Am/240Am/241Am/242Am/243Am/244Am/245Am/246Am/247Am/248Am/249Am/250Am/235Cm/236Cm/237Cm/238Cm/239Cm/240Cm/241Cm/242Cm/243Cm/244Cm/245Cm/246Cm/247Cm/248Cm/249Cm/250Cm/251Cm/252Cm/238Bk/239Bk/240Bk/241Bk/242Bk/243Bk/244Bk/245Bk/246Bk/247Bk/248Bk/249Bk/250Bk/251Bk/252Bk/253Bk/240Cf/241Cf/242Cf/243Cf/244Cf/245Cf/246Cf/247Cf/248Cf/249Cf/250Cf/251Cf/252Cf/253Cf/254Cf/255Cf/242Es/243Es/244Es/245Es/246Es/247Es/248Es/249Es/250Es/251Es/252Es/253Es/254Es/255Es/256Es/245Fm/246Fm/247Fm/248Fm/249Fm/250Fm/251Fm/252Fm/253Fm/254Fm/255Fm/256Fm/257Fm , E(cm)=386 MeV; calculated capture probability, isotopic production σ, σ dependence on angular momentum of 251Es and 254Fm reaction products. 249Cf(112Sn, X)230Bk/231Bk/232Bk/233Bk/234Bk/235Bk/236Bk/237Bk/238Bk/239Bk/240Bk/241Bk/242Bk/243Bk/244Bk/245Bk/246Bk/247Bk/248Bk/249Bk/250Bk/231Cf/232Cf/233Cf/234Cf/235Cf/236Cf/237Cf/238Cf/239Cf/240Cf/241Cf/242Cf/243Cf/244Cf/245Cf/246Cf/247Cf/248Cf/249Cf/250Cf/239Es/240Es/241Es/242Es/243Es/244Es/245Es/246Es/247Es/248Es/249Es/250Es/240Fm/241Fm/242Fm/243Fm/244Fm/245Fm/246Fm/247Fm/248Fm/249Fm/250Fm/251Fm/252Fm/253Fm/254Fm/255Fm, E=475 MeV; 249Cf(124Sn, X)238Bk/239Bk/240Bk/241Bk/242Bk/243Bk/244Bk/245Bk/246Bk/247Bk/248Bk/249Bk/250Bk/251Bk/252Bk/253Bk/254Bk/255Bk/256Bk/237Cf/238Cf/239Cf/240Cf/241Cf/242Cf/243Cf/244Cf/245Cf/246Cf/247Cf/248Cf/249Cf/250Cf/251Cf/252Cf/253Cf/254Cf/255Cf/256Cf/239Es/240Es/241Es/242Es/243Es/244Es/245Es/246Es/247Es/248Es/249Es/250Es/251Es/252Es/253Es/254Es/255Es/256Es/257Es/258Es/259Es/260Es/240Fm/241Fm/242Fm/243Fm/244Fm/245Fm/246Fm/247Fm/248Fm/249Fm/250Fm/251Fm/252Fm/253Fm/254Fm/255Fm/256Fm/257Fm/258Fm/259Fm/260Fm/261Fm/262Fm, E=468 MeV; 249Cf(132Sn, X)239Bk/240Bk/241Bk/242Bk/243Bk/244Bk/245Bk/246Bk/247Bk/248Bk/249Bk/250Bk/251Bk/252Bk/253Bk/254Bk/255Bk/256Bk/257Bk/258Bk/259Bk/242Cf/243Cf/244Cf/245Cf/246Cf/247Cf/248Cf/249Cf/250Cf/251Cf/252Cf/253Cf/254Cf/255Cf/256Cf/257Cf/258Cf/259Cf/260Cf/261Cf/244Es/245Es/246Es/247Es/248Es/249Es/250Es/251Es/252Es/253Es/254Es/255Es/256Es/257Es/258Es/259Es/260Es/261Es/247Fm/248Fm/249Fm/250Fm/251Fm/252Fm/253Fm/254Fm/255Fm/256Fm/257Fm/258Fm/259Fm/260Fm/261Fm/262Fm/263Fm/264Fm/265Fm/250Md/251Md/252Md/253Md/254Md/255Md/256Md/257Md/258Md/259Md/260Md/261Md/262Md/263Md/264Md/265Md/266Md/253No/254No/255No/256No/257No/258No/259No/260No/261No/262No/263No/264No/265No/266No/267No/268No, E=463 MeV; calculated isotope production σ, driving potential. Theoretical framework of a hybrid model combining the dinuclear system model and the GRAZING model. Comparison to experimental data.

doi: 10.1103/PhysRevC.106.034601
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