NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = X.R.Zhang Found 9 matches. 2024ZH08 Phys.Rev. C 109, 024606 (2024) L.-L.Zhou, J.-J.Cai, L.-Q.Li, Z.-L.Wang, R.Zhu, X.-Y.Zhang, X.-R.Zhang, L.Zhu, G.Zhang, F.-Sh.Zhang Fusion enhancement in the collisions with ^{44}Ca beams and the production of neutron-deficient ^{245-250}Lr isotopes
doi: 10.1103/PhysRevC.109.024606
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 ^{232}Th(^{204}Hg, X), E(cm)=678.1 MeV; ^{249}Bk(^{238}U, X), E(cm)=823.4 MeV; ^{248}Cm(^{238}U, X), E(cm)=824.9 MeV; calculated σ in fusion evaporation (FE) reactions and multinucleon transfer (MNT) reactions.
doi: 10.1142/S0218301323300023
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 ^{197}Au + ^{232}Th NUCLEAR REACTIONS ^{232}Th(^{197}Au, X)^{258}Es/^{259}Es/^{260}Es/^{261}Es/^{262}Es/^{260}Fm/^{261}Fm/^{262}Fm/^{263}Fm/^{261}Md/^{262}Md/^{263}Md/^{264}Md/^{265}Md/^{261}No/^{263}No/^{264}No/^{265}No/^{266}No/^{267}No/^{263}Lr/^{265}Lr/^{267}Lr/^{268}Lr/^{264}Rf/^{266}Rf/^{268}Rf/^{269}Rf/^{270}Rf/^{264}Db/^{265}Db/^{269}Db/^{271}Db/^{267}Sg/^{268}Sg/^{270}Sg/^{272}Sg/^{273}Sg, E(cm)=690.69;^{232}Th(^{197}Au, X)^{243}U/^{244}U/^{245}U/^{246}U/^{247}U/^{248}U/^{249}U/^{246}Np/^{247}Np/^{248}Np/^{249}Np/^{250}Np/^{251}Np/^{252}Np/^{248}Pu/^{249}Pu/^{250}Pu/^{251}Pu/^{252}Pu/^{253}Pu/^{254}Pu/^{248}Am/^{249}Am/^{250}Am/^{251}Am/^{252}Am/^{253}Am/^{254}Am/^{255}Am/^{256}Am/^{252}Cm/^{253}Cm/^{254}Cm/^{255}Cm/^{256}Cm/^{257}Cm/^{258}Cm/^{252}Bk/^{254}Bk/^{255}Bk/^{256}Bk/^{257}Bk/^{258}Bk/^{259}Bk/^{257}Cf/^{258}Cf/^{259}Cf/^{260}Cf/^{261}Cf/^{258}Es/^{259}Es/^{260}Es/^{261}Es/^{262}Es, E(cm)=756.47 MeV; calculated production σ. ^{232}Th(^{197}Au, X), E=690.7, 723.6, 756.5 MeV;^{232}Th(^{186}W, X), E=681, 2 MeV;^{232}Th(^{238}U, 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. ^{232}Th(^{197}Au, X), E=690.7, 723.6, 756.5, 789.4 MeV; interaction time as a function of the impact parameter. ^{249}Cf(^{136}Xe, 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
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 ^{248}Cm(^{136}Xe, X)^{229}Pu/^{230}Pu/^{231}Pu/^{232}Pu/^{233}Pu/^{234}Pu/^{235}Pu/^{236}Pu/^{237}Pu/^{238}Pu/^{239}Pu/^{240}Pu/^{241}Pu/^{242}Pu/^{243}Pu/^{244}Pu/^{245}Pu/^{246}Pu/^{247}Pu/^{248}Pu/^{249}Pu/^{250}Pu/^{251}Pu/^{252}Pu/^{253}Pu/^{254}Pu/^{233}Am/^{234}Am/^{235}Am/^{236}Am/^{237}Am/^{238}Am/^{239}Am/^{240}Am/^{241}Am/^{242}Am/^{243}Am/^{244}Am/^{245}Am/^{246}Am/^{247}Am/^{248}Am/^{249}Am/^{250}Am/^{251}Am/^{252}Am/^{253}Am/^{254}Am/^{255}Am/^{235}Cm/^{236}Cm/^{237}Cm/^{238}Cm/^{239}Cm/^{240}Cm/^{241}Cm/^{242}Cm/^{243}Cm/^{244}Cm/^{245}Cm/^{246}Cm/^{247}Cm/^{248}Cm/^{249}Cm/^{250}Cm/^{251}Cm/^{252}Cm/^{253}Cm/^{254}Cm/^{255}Cm/^{256}Cm/^{257}Cm/^{258}Cm/^{238}Bk/^{239}Bk/^{240}Bk/^{241}Bk/^{242}Bk/^{243}Bk/^{244}Bk/^{245}Bk/^{246}Bk/^{247}Bk/^{248}Bk/^{249}Bk/^{250}Bk/^{251}Bk/^{252}Bk/^{253}Bk/^{254}Bk/^{255}Bk/^{256}Bk/^{257}Bk/^{258}Bk/^{259}Bk/^{260}Bk/^{240}Cf/^{241}Cf/^{242}Cf/^{243}Cf/^{244}Cf/^{245}Cf/^{246}Cf/^{247}Cf/^{248}Cf/^{249}Cf/^{250}Cf/^{251}Cf/^{252}Cf/^{253}Cf/^{254}Cf/^{255}Cf/^{256}Cf/^{257}Cf/^{258}Cf/^{259}Cf/^{260}Cf/^{261}Cf/^{243}Es/^{244}Es/^{245}Es/^{246}Es/^{247}Es/^{248}Es/^{249}Es/^{250}Es/^{251}Es/^{252}Es/^{253}Es/^{254}Es/^{255}Es/^{256}Es/^{257}Es/^{258}Es/^{259}Es/^{260}Es/^{261}Es/^{262}Es , E(cm)=533 MeV; ^{249}Cf(^{136}Xe, X)^{229}Pu/^{230}Pu/^{231}Pu/^{232}Pu/^{233}Pu/^{234}Pu/^{235}Pu/^{236}Pu/^{237}Pu/^{238}Pu/^{239}Pu/^{240}Pu/^{241}Pu/^{242}Pu/^{243}Pu/^{244}Pu/^{245}Pu/^{246}Pu/^{247}Pu/^{248}Pu/^{249}Pu/^{250}Pu/^{251}Pu/^{252}Pu/^{253}Pu/^{230}Am/^{231}Am/^{232}Am/^{233}Am/^{234}Am/^{235}Am/^{236}Am/^{237}Am/^{238}Am/^{239}Am/^{240}Am/^{241}Am/^{242}Am/^{243}Am/^{244}Am/^{245}Am/^{246}Am/^{247}Am/^{248}Am/^{249}Am/^{250}Am/^{251}Am/^{252}Am/^{253}Am/^{254}Am/^{255}Am/^{233}Cm/^{234}Cm/^{235}Cm/^{236}Cm/^{237}Cm/^{238}Cm/^{239}Cm/^{240}Cm/^{241}Cm/^{242}Cm/^{243}Cm/^{244}Cm/^{245}Cm/^{246}Cm/^{247}Cm/^{248}Cm/^{249}Cm/^{250}Cm/^{251}Cm/^{252}Cm/^{253}Cm/^{254}Cm/^{255}Cm/^{256}Cm/^{257}Cm/^{258}Cm/^{236}Bk/^{237}Bk/^{238}Bk/^{239}Bk/^{240}Bk/^{241}Bk/^{242}Bk/^{243}Bk/^{244}Bk/^{245}Bk/^{246}Bk/^{247}Bk/^{248}Bk/^{249}Bk/^{250}Bk/^{251}Bk/^{252}Bk/^{253}Bk/^{254}Bk/^{255}Bk/^{256}Bk/^{257}Bk/^{258}Bk/^{259}Bk/^{260}Bk/^{237}Cf/^{238}Cf/^{239}Cf/^{240}Cf/^{241}Cf/^{242}Cf/^{243}Cf/^{244}Cf/^{245}Cf/^{246}Cf/^{247}Cf/^{248}Cf/^{249}Cf/^{250}Cf/^{251}Cf/^{252}Cf/^{253}Cf/^{254}Cf/^{255}Cf/^{256}Cf/^{257}Cf/^{258}Cf/^{259}Cf/^{260}Cf/^{261}Cf/^{240}Es/^{241}Es/^{242}Es/^{243}Es/^{244}Es/^{245}Es/^{246}Es/^{247}Es/^{248}Es/^{249}Es/^{250}Es/^{251}Es/^{252}Es/^{253}Es/^{254}Es/^{255}Es/^{256}Es/^{257}Es/^{258}Es/^{259}Es/^{260}Es, E(cm)=526 MeV; ^{238}U(^{92}Kr, X)/^{229}Np/^{230}Np/^{231}Np/^{232}Np/^{233}Np/^{234}Np/^{235}Np/^{236}Np/^{237}Np/^{238}Np/^{239}Np/^{240}Np/^{241}Np/^{242}Np/^{243}Np/^{244}Np/^{234}Pu/^{235}Pu/^{236}Pu/^{237}Pu/^{238}Pu/^{239}Pu/^{240}Pu/^{241}Pu/^{242}Pu/^{243}Pu/^{244}Pu/^{245}Pu/^{246}Pu/^{247}Pu/^{238}Am/^{239}Am/^{240}Am/^{241}Am/^{242}Am/^{243}Am/^{244}Am/^{245}Am/^{246}Am/^{247}Am/^{248}Am/^{249}Am/^{250}Am/^{251}Am/^{252}Am/^{242}Cm/^{243}Cm/^{244}Cm/^{245}Cm/^{246}Cm/^{247}Cm/^{248}Cm/^{249}Cm/^{250}Cm/^{251}Cm/^{252}Cm/^{253}Cm/^{254}Cm/^{255}Cm/^{256}Cm/^{242}Bk/^{243}Bk/^{244}Bk/^{245}Bk/^{246}Bk/^{247}Bk/^{248}Bk/^{249}Bk/^{250}Bk/^{251}Bk/^{252}Bk/^{253}Bk/^{254}Bk/^{242}Cf/^{243}Cf/^{244}Cf/^{245}Cf/^{246}Cf/^{247}Cf/^{248}Cf/^{249}Cf/^{250}Cf/^{251}Cf/^{252}Cf/^{253}Cf/^{254}Cf/^{255}Cf/^{256}Cf, E(cm)=357 MeV; ^{238}U(^{132}Sn, X), ^{230}Np/^{231}Np/^{232}Np/^{233}Np/^{234}Np/^{235}Np/^{236}Np/^{237}Np/^{238}Np/^{239}Np/^{240}Np/^{241}Np/^{242}Np/^{243}Np/^{244}Np/^{245}Np/^{246}Np/^{247}Np/^{248}Np/^{249}Np/^{250}Np/^{251}Np/^{252}Np/^{253}Np/^{254}Np/^{255}Np/^{232}Pu/^{233}Pu/^{234}Pu/^{235}Pu/^{236}Pu/^{237}Pu/^{238}Pu/^{239}Pu/^{240}Pu/^{241}Pu/^{242}Pu/^{243}Pu/^{244}Pu/^{245}Pu/^{246}Pu/^{247}Pu/^{248}Pu/^{249}Pu/^{250}Pu/^{251}Pu/^{252}Pu/^{253}Pu/^{254}Pu/^{255}Pu/^{256}Pu/^{257}Pu/^{236}Am/^{237}Am/^{238}Am/^{239}Am/^{240}Am/^{241}Am/^{242}Am/^{243}Am/^{244}Am/^{245}Am/^{246}Am/^{247}Am/^{248}Am/^{249}Am/^{250}Am/^{251}Am/^{252}Am/^{253}Am/^{254}Am/^{255}Am/^{256}Am/^{257}Am/^{235}Cm/^{236}Cm/^{237}Cm/^{238}Cm/^{239}Cm/^{240}Cm/^{241}Cm/^{242}Cm/^{243}Cm/^{244}Cm/^{245}Cm/^{246}Cm/^{247}Cm/^{248}Cm/^{249}Cm/^{250}Cm/^{251}Cm/^{252}Cm/^{253}Cm/^{254}Cm/^{255}Cm/^{256}Cm/^{257}Cm/^{258}Cm/^{259}Cm/^{260}Cm/^{261}Cm/^{242}Bk/^{243}Bk/^{244}Bk/^{245}Bk/^{246}Bk/^{247}Bk/^{248}Bk/^{249}Bk/^{250}Bk/^{251}Bk/^{252}Bk/^{253}Bk/^{254}Bk/^{255}Bk/^{256}Bk/^{257}Bk/^{258}Bk/^{259}Bk/^{260}Bk/^{261}Bk/^{262}Bk/^{244}Cf/^{245}Cf/^{246}Cf/^{247}Cf/^{248}Cf/^{249}Cf/^{250}Cf/^{251}Cf/^{252}Cf/^{253}Cf/^{254}Cf/^{255}Cf/^{256}Cf/^{257}Cm/^{258}Cm/^{259}Cm/^{260}Cm/^{261}Cm/^{262}Cm/^{263}Cm/^{264}Cm, E(cm)=478, 521, 564 MeV; ^{238}U(^{144}Xe, X), ^{236}Np/^{237}Np/^{238}Np/^{239}Np/^{240}Np/^{241}Np/^{242}Np/^{243}Np/^{244}Np//^{245}Np/^{246}Np/^{247}Np/^{248}Np/^{249}Np/^{250}Np/^{235}Pu/^{236}Pu/^{237}Pu/^{238}Pu/^{239}Pu/^{240}Pu/^{241}Pu/^{242}Pu/^{243}Pu/^{244}Pu/^{245}Pu/^{246}Pu/^{247}Pu/^{248}Pu/^{249}Pu/^{250}Pu/^{251}Pu/^{252}Pu/^{240}Am/^{241}Am/^{242}Am/^{243}Am/^{244}Am/^{245}Am/^{246}Am/^{247}Am/^{248}Am/^{249}Am/^{250}Am/^{251}Am/^{252}Am/^{253}Am/^{254}Am/^{243}Cm/^{244}Cm/^{245}Cm/^{246}Cm/^{247}Cm/^{248}Cm/^{249}Cm/^{250}Cm/^{251}Cm/^{252}Cm/^{253}Cm/^{254}Cm/^{255}Cm/^{241}Bk/^{242}Bk/^{243}Bk/^{244}Bk/^{245}Bk/^{246}Bk/^{247}Bk/^{248}Bk/^{249}Bk/^{250}Bk/^{251}Bk/^{252}Bk/^{253}Bk/^{254}Bk/^{255}Bk/^{265}Bk/^{246}Cf/^{247}Cf/^{248}Cf/^{249}Cf/^{250}Cf/^{251}Cf/^{252}Cf/^{253}Cf/^{254}Cf/^{255}Cf/^{256}Cf/^{257}Cm/^{258}Cm/^{259}Cm/^{260}Cm/^{261}Cm/^{262}Cm, 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
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 ^{248}Cm(^{86}Kr, X)^{235}Am/^{236}Am/^{237}Am/^{238}Am/^{239}Am/^{240}Am/^{241}Am/^{242}Am/^{243}Am/^{244}Am/^{245}Am/^{246}Am/^{247}Am/^{248}Am/^{249}Am/^{250}Am/^{235}Cm/^{236}Cm/^{237}Cm/^{238}Cm/^{239}Cm/^{240}Cm/^{241}Cm/^{242}Cm/^{243}Cm/^{244}Cm/^{245}Cm/^{246}Cm/^{247}Cm/^{248}Cm/^{249}Cm/^{250}Cm/^{251}Cm/^{252}Cm/^{238}Bk/^{239}Bk/^{240}Bk/^{241}Bk/^{242}Bk/^{243}Bk/^{244}Bk/^{245}Bk/^{246}Bk/^{247}Bk/^{248}Bk/^{249}Bk/^{250}Bk/^{251}Bk/^{252}Bk/^{253}Bk/^{240}Cf/^{241}Cf/^{242}Cf/^{243}Cf/^{244}Cf/^{245}Cf/^{246}Cf/^{247}Cf/^{248}Cf/^{249}Cf/^{250}Cf/^{251}Cf/^{252}Cf/^{253}Cf/^{254}Cf/^{255}Cf/^{242}Es/^{243}Es/^{244}Es/^{245}Es/^{246}Es/^{247}Es/^{248}Es/^{249}Es/^{250}Es/^{251}Es/^{252}Es/^{253}Es/^{254}Es/^{255}Es/^{256}Es/^{245}Fm/^{246}Fm/^{247}Fm/^{248}Fm/^{249}Fm/^{250}Fm/^{251}Fm/^{252}Fm/^{253}Fm/^{254}Fm/^{255}Fm/^{256}Fm/^{257}Fm , E(cm)=386 MeV; calculated capture probability, isotopic production σ, σ dependence on angular momentum of ^{251}Es and ^{254}Fm reaction products. ^{249}Cf(^{112}Sn, X)^{230}Bk/^{231}Bk/^{232}Bk/^{233}Bk/^{234}Bk/^{235}Bk/^{236}Bk/^{237}Bk/^{238}Bk/^{239}Bk/^{240}Bk/^{241}Bk/^{242}Bk/^{243}Bk/^{244}Bk/^{245}Bk/^{246}Bk/^{247}Bk/^{248}Bk/^{249}Bk/^{250}Bk/^{231}Cf/^{232}Cf/^{233}Cf/^{234}Cf/^{235}Cf/^{236}Cf/^{237}Cf/^{238}Cf/^{239}Cf/^{240}Cf/^{241}Cf/^{242}Cf/^{243}Cf/^{244}Cf/^{245}Cf/^{246}Cf/^{247}Cf/^{248}Cf/^{249}Cf/^{250}Cf/^{239}Es/^{240}Es/^{241}Es/^{242}Es/^{243}Es/^{244}Es/^{245}Es/^{246}Es/^{247}Es/^{248}Es/^{249}Es/^{250}Es/^{240}Fm/^{241}Fm/^{242}Fm/^{243}Fm/^{244}Fm/^{245}Fm/^{246}Fm/^{247}Fm/^{248}Fm/^{249}Fm/^{250}Fm/^{251}Fm/^{252}Fm/^{253}Fm/^{254}Fm/^{255}Fm, E=475 MeV; ^{249}Cf(^{124}Sn, X)^{238}Bk/^{239}Bk/^{240}Bk/^{241}Bk/^{242}Bk/^{243}Bk/^{244}Bk/^{245}Bk/^{246}Bk/^{247}Bk/^{248}Bk/^{249}Bk/^{250}Bk/^{251}Bk/^{252}Bk/^{253}Bk/^{254}Bk/^{255}Bk/^{256}Bk/^{237}Cf/^{238}Cf/^{239}Cf/^{240}Cf/^{241}Cf/^{242}Cf/^{243}Cf/^{244}Cf/^{245}Cf/^{246}Cf/^{247}Cf/^{248}Cf/^{249}Cf/^{250}Cf/^{251}Cf/^{252}Cf/^{253}Cf/^{254}Cf/^{255}Cf/^{256}Cf/^{239}Es/^{240}Es/^{241}Es/^{242}Es/^{243}Es/^{244}Es/^{245}Es/^{246}Es/^{247}Es/^{248}Es/^{249}Es/^{250}Es/^{251}Es/^{252}Es/^{253}Es/^{254}Es/^{255}Es/^{256}Es/^{257}Es/^{258}Es/^{259}Es/^{260}Es/^{240}Fm/^{241}Fm/^{242}Fm/^{243}Fm/^{244}Fm/^{245}Fm/^{246}Fm/^{247}Fm/^{248}Fm/^{249}Fm/^{250}Fm/^{251}Fm/^{252}Fm/^{253}Fm/^{254}Fm/^{255}Fm/^{256}Fm/^{257}Fm/^{258}Fm/^{259}Fm/^{260}Fm/^{261}Fm/^{262}Fm, E=468 MeV; ^{249}Cf(^{132}Sn, X)^{239}Bk/^{240}Bk/^{241}Bk/^{242}Bk/^{243}Bk/^{244}Bk/^{245}Bk/^{246}Bk/^{247}Bk/^{248}Bk/^{249}Bk/^{250}Bk/^{251}Bk/^{252}Bk/^{253}Bk/^{254}Bk/^{255}Bk/^{256}Bk/^{257}Bk/^{258}Bk/^{259}Bk/^{242}Cf/^{243}Cf/^{244}Cf/^{245}Cf/^{246}Cf/^{247}Cf/^{248}Cf/^{249}Cf/^{250}Cf/^{251}Cf/^{252}Cf/^{253}Cf/^{254}Cf/^{255}Cf/^{256}Cf/^{257}Cf/^{258}Cf/^{259}Cf/^{260}Cf/^{261}Cf/^{244}Es/^{245}Es/^{246}Es/^{247}Es/^{248}Es/^{249}Es/^{250}Es/^{251}Es/^{252}Es/^{253}Es/^{254}Es/^{255}Es/^{256}Es/^{257}Es/^{258}Es/^{259}Es/^{260}Es/^{261}Es/^{247}Fm/^{248}Fm/^{249}Fm/^{250}Fm/^{251}Fm/^{252}Fm/^{253}Fm/^{254}Fm/^{255}Fm/^{256}Fm/^{257}Fm/^{258}Fm/^{259}Fm/^{260}Fm/^{261}Fm/^{262}Fm/^{263}Fm/^{264}Fm/^{265}Fm/^{250}Md/^{251}Md/^{252}Md/^{253}Md/^{254}Md/^{255}Md/^{256}Md/^{257}Md/^{258}Md/^{259}Md/^{260}Md/^{261}Md/^{262}Md/^{263}Md/^{264}Md/^{265}Md/^{266}Md/^{253}No/^{254}No/^{255}No/^{256}No/^{257}No/^{258}No/^{259}No/^{260}No/^{261}No/^{262}No/^{263}No/^{264}No/^{265}No/^{266}No/^{267}No/^{268}No, 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
2022ZH54 J.Phys.(London) G49, 095104 (2022) X.-r.Zhang, G.Zhang, J.-j.Li, Z.Liu, Y.-x.Yang, F.-s.Zhang Production mechanism and prediction cross sections of unknown neutron-rich ^{263-265, 267-269}Lr isotopes in multinucleon transfer reactions based on the dinuclear system model NUCLEAR REACTIONS ^{235}U(^{40}Ar, X), E(cm)=184.6 MeV; ^{249}Bk(^{130}Te, X)^{263}Lr/^{264}Lr/^{265}Lr/^{267}Lr/^{268}Lr/^{269}Lr, E(cm)=526.7 MeV; analyzed available data; calculated production σ.
doi: 10.1088/1361-6471/ac81df
2021ZH16 Phys.Rev. C 103, 024608 (2021) X.-R.Zhang, G.Zhang, J.-J.Li, S.H.Cheng, Z.Liu, F.-S.Zhang Effects of nucleus orientation on transfer process and production of unknown neutron-rich isotopes with Z = 62-75 in ^{204}Hg + ^{232}Th based on the dinuclear system model NUCLEAR REACTIONS ^{166}Er(^{86}Kr, X), E(cm)=464 MeV; calculated mass and charge distributions of total kinetic energy (TKE) of the primary binary fragments. ^{232}Th(^{204}Hg, X)^{168}Sm/^{169}Sm/^{170}Eu/^{171}Eu/^{172}Eu/^{172}Gd/^{173}Gd/^{174}Gd/^{175}Gd/^{175}Tb/^{176}Tb/^{177}Tb/^{177}Dy/^{178}Dy/^{179}Dy/^{180}Dy/^{179}Ho/^{180}Ho/^{181}Ho/^{182}Ho/^{181}Er/^{182}Er/^{183}Er/^{184}Er/^{185}Er/^{182}Tm/^{183}Tm/^{184}Tm/^{185}Tm/^{186}Tm/^{187}Tm/^{186}Yb/^{187}Yb/^{188}Yb/^{189}Yb/^{190}Yb/^{189}Lu/^{190}Lu/^{191}Lu/^{192}Lu/^{193}Lu/^{191}Hf/^{192}Hf/^{193}Hf/^{194}Hf/^{195}Hf/^{195}Ta/^{196}Ta/^{197}Ta/^{198}W/^{199}W/^{200}Re/^{201}Re/^{202}Re, E(cm)=678.1 MeV; calculated potential energies for the tip-to-tip and side-to-side configurations, production σ. Dinuclear system (DNS) model. Comparison with available experimental data.
doi: 10.1103/PhysRevC.103.024608
2020ZH28 Phys.Rev. C 102, 024617 (2020) G.Zhang, J.-J.Li, X.-R.Zhang, B.Li, C.A.T.Sokhna, C.Wang, Z.Liu, F.-S.Zhang Role of the quasifission yields in the multinucleon transfer reactions of ^{136}Xe + ^{208}Pb NUCLEAR REACTIONS ^{208}Pb(^{136}Xe, X), (^{136}Xe, F), E(cm)=526 MeV; calculated mass distributions with and without the quasifission yields, σ(A) as function of the angular momentum, production σ of Hg, Pb, and Po isotopes contributed from quasifission yields, quasifission yields and excitation energies of ^{202}Hg and ^{208}Hg, isotopic distribution σ(Z) of Hg, Pb and Po isotopes. Dinuclear system (DNS) model. Comparison with experimental data.
doi: 10.1103/PhysRevC.102.024617
2019XU06 Chin.Phys.C 43, 064105 (2019) X.-X.Xu, G.Zhang, J.-J.Li, B.Li, C.A.T.Sokhna, X.-R.Zhang, X.-X.Yang, S.-H.Cheng, Y.-H.Zhang, Z.-S.Ge, C.Li, Z.Liu, F.-S.Zhang Production of exotic neutron-deficient isotopes near N, Z = 50 in multinucleon transfer reactions NUCLEAR REACTIONS ^{124}Sn(^{40}Ca, X), E=128.5 MeV; ^{112}Sn(^{48}Ca, X), (^{40}Ca, X), (^{58}Ni, X), (^{106}Cd, X), E(cm)=280 MeV; ^{112}Sn(^{106}Cd, X)^{101}Sb/^{112}Sb/^{103}Te/^{106}I/^{107}I, E(cm)=300, 500, 780 MeV; calculated production σ. Comparison with experimental data.
doi: 10.1088/1674-1137/43/6/064105
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