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NSR database version of May 10, 2024.

Search: Author = C.C.Guo

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2023DU05      Eur.Phys.J. A 59, 93 (2023)

H.-X.Duan, F.Zhang, J.Su, L.Zhu, C.-C.Guo

Studying sub-saturation density symmetry energy with different nuclear thermometers

NUCLEAR REACTIONS U(155Gd, X), E not given; 197Au(197Au, X), E=35 MeV/nucleon; analyzed available data; deduced the relation between nuclear temperatures and symmetry energy using the IQMD model.

doi: 10.1140/epja/s10050-023-01008-5
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2020ZH22      Int.J.Mod.Phys. E29, 2030004 (2020)

L.Zhu, C.Li, C.-C.Guo, J.Su, P.W.Wen, G.Zhang, F.-S.Zhang

Theoretical progress on production of isotopes in the multinucleon transfer process

NUCLEAR REACTIONS 238U(64Ni, X), E(cm)=307.5 MeV; 208Pb(124Xe, X), E(cm)=50 MeV; 186W(160Gd, X), E=503 MeV; calculated transfer σ for production of neutron-rich transuranium nuclei.

doi: 10.1142/S0218301320300040
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2019GU08      Phys.Rev. C 99, 044607 (2019)

C.-C.Guo, Y.-G.Ma, Z.-D.An, B.-S.Huang

Influence of α-clustering configurations in 16O + 197Au collisions at Fermi energy

NUCLEAR REACTIONS 197Au(16O, X), E=40 MeV/nucleon; calculated contour plots of nucleon density, directed flow and flow parameters of free protons as function of rapidity with the chain and a tetrahedron α configurations of 16O projectile, and transverse momentum dependence of flow parameters. 197Au(12C, X), (14N, X), (36Ar, X), E=30, 35, 40 MeV/nucleon; calculated charge multiplicity distributions. Extended quantum molecular dynamics model (ImQMD). Comparison with available experimental data. Relevance to α-clustering configurations in light nuclei.

doi: 10.1103/PhysRevC.99.044607
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2019ZH13      Phys.Lett. B 791, 20 (2019)

L.Zhu, C.Li, J.Su, C.-C.Guo, W.Hua

Advantages of the multinucleon transfer reactions based on 238U target for producing neutron-rich isotopes around N=126

NUCLEAR REACTIONS 238U(186W, X), (160Gd, X), E(cm)=660, 475 MeV; analyzed available data; deduced mechanism of multinucleon transfer (MNT) reactions for producing neutron-rich heavy nuclei around N=126 using dinuclear system (DNS) model and isospin-dependent quantum molecular dynamics (IQMD) model.

doi: 10.1016/j.physletb.2019.02.015
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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
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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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2018ZH17      Phys.Rev. C 97, 044614 (2018)

L.Zhu, P.-W.Wen, C.-J.Lin, X.-J.Bao, J.Su, C.Li, C.-C.Guo

Shell effects in a multinucleon transfer process

NUCLEAR REACTIONS 198Pt(136Xe, X), E(cm)=643, 420 MeV; 208Pb(136Xe, X), E(cm)=450, 526 MeV; 186W(136Xe, X), E(cm)=408 MeV; 186W(150Nd, X), E(cm)=451 MeV; calculated potential energy surfaces, total kinetic energy losses (TKEL), and production σ with and without shell corrections using dinuclear system (DNS) model; deduced shell effects on producing trans-target nuclei. Comparison with experimental values.

doi: 10.1103/PhysRevC.97.044614
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2018ZH39      Phys.Rev. C 98, 034609 (2018)

L.Zhu, J.Su, P.-W.Wen, C.-C.Guo, C.Li

Multinucleon transfer process in the reaction 160Gd + 186W

NUCLEAR REACTIONS 186W(160Gd, X), E(cm)=430, 450, 503, 550 MeV; calculated potential energy surface as a function of mass asymmetry and β2 deformation, σ(E) for production of primary products as function of mass number, TKEL and β2, N/Z distribution of primary products, and production σ(E) of Os and Np isotopes, 202Os, 201Re, 240Np, 241U, and isotopes of Z=60-100, N=90-150. Dinuclear system (DNS) model with GEMINI code for multinucleon transfer (MNT) process.

doi: 10.1103/PhysRevC.98.034609
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2017GU22      Chin.Phys.Lett. 34, 092101 (2017)

C.-C.Guo, W.-B.He, Y.-G.Ma

Collective Flows of 16O+16O Collisions with α-Clustering Configurations

NUCLEAR REACTIONS 16O(16O, X), E=40-60 MeV/nucleon; calculated flow parameters. An extended quantum molecular dynamics model, four α-clustering (linear chain, kite, square and tetrahedron) configurations.

doi: 10.1088/0256-307X/34/9/092101
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