Prediction for the synthesis cross sections of new moscovium isotopes in fusion-evaporation reactions
Abstract
In the framework of the dinuclear system model, the synthesis mechanism of the superheavy nuclides with atomic number Z=112, 114, 115 in the reactions of projectiles 40,48Ca bombarding on targets 238U, 242Pu, and 243Am at a wide incident energies (excitation energy from 0-100 MeV) have been investigated systematically. Based on the available experimental excitation functions, the dependence of calculated synthesis cross sections on collision orientations has been studied thoroughly. The TKEs of these collisions with the fixed collision orientation show its orientation dependence which can be used to predict the tendency of kinetic energy diffusion. The TKEs are dependent on incident energies which have been discussed. The method of Coulomb barrier distribution function has been applied in our calculations which could treat all of the collision orientations from the tip-tip to side-side approximately. The calculations of excitation functions of 48Ca + 238U, 48Ca + 242Pu, and 48Ca + 243Am have a nice agreement with the available experimental data. The isospin effect of projectiles on production cross sections of moscovium isotopes and the influence of entrance channel effect on the synthesis cross sections of superheavy nuclei have been discussed. The synthesis cross section of new moscovium isotopes 278-286Mc have been predicted as large as hundreds pb, in the fusion-evaporation reactions of 35,37Cl + 248Cf, 38,40Ar + 247Bk, 39,41K + 247Cm, 40,42,44,46Ca + 238Am, 45Sc + 242Pu, and 46,48,50Ti + 243Np, 51V + 238U at the excitation energy interval of 0-100 MeV.
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