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NSR database version of May 10, 2024.

Search: Author = T.Ganesh

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2022DA17      Phys.Rev. C 106, 064603 (2022)

P.S.Damodara Gupta, N.Sowmya, H.C.Manjunatha, L.Seenappa, T.Ganesh

Quasifission barrier of heavy ion fusion reactions leading to the formation of the superheavy nucleus 302120

NUCLEAR REACTIONS 251Cf(56Ti, 3n)304120, E*=36 MeV; 251Cf(57Ti, 4n)304120, E*=47 MeV; 251Cf(58Ti, 5n)304120, E*=60 MeV; 249Bk(58V, 3n)304120, E*=37 MeV; 249Bk(59V, 4n)304120, E*=47 MeV; 249Bk(60V, 5n)304120, E*=59 MeV; 248Cm(59Cr, 3n)304120, E *=36 MeV; 248Cm(60Cr, 4n)304120, E*=46 MeV; 248Cm(61Cr, 5n)304120, E*=57 MeV; 248Cf(45Sc, 3n)290119, E*=39 MeV; 247Bk(50Ti, 3n)294119, E*=36 MeV; 242Cm(51V, 3n)290119, E*=38 MeV; 242Am(54Cr, 3n)293119, E*=37 MeV; calculated evaporation residue σ. 237Th(65Zn, X), 218Po(84Kr, X), E not given; calculated nucleus-nucleus interaction potential from the fusion which leads to 302120 production. 252Cf(50Ti, X), E(cm)=223 MeV; 249Bk(53V, X), E(cm)=229 MeV; 248Cm(54Cr, X), E(cm)=236 MeV; 244Pu(58Fe, X), E(cm)=249 MeV; 239Pa(63Cu, X), E(cm)=260 MeV; 232Th(70Zn, X), E(cm)=281 MeV; 222Rn(80Se, X), E(cm)=309 MeV; 228Ra(74Ge, X), E(cm)=240 MeV; 238U(64Ni, X), E(cm)=267 MeV; calculated quasifission barrier, evaporation residue σ, entrance channel parameters. Investigated the influence of the projectile-target orientation and angular momentum on quasifission barriers. Dinuclear system (DNS) model. Comparison to other theoretical estimations.

doi: 10.1103/PhysRevC.106.064603
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