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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
Citations: PlumX Metrics

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
Citations: PlumX Metrics