Synthesis of the Z=122 superheavy nucleus via Fe58- and Ni64-induced reactions using the dynamical cluster-decay model

Sahila Chopra, Hemdeep, and Raj K. Gupta
Phys. Rev. C 95, 044603 – Published 4 April 2017

Abstract

Within the framework of the dynamical cluster-decay model (DCM), we have studied the nuclear system with Z=122 and mass number A = 306 formed via two “hot” fusion reactions Fe58+Cm248 and Ni64+Pu242. The up-to-date measured data are available only for the first reaction, and for fusion-fission cross section σff and quasifission cross section σqf, only at one compound nucleus (CN) excitation energy E*=33MeV. In this study, we have included the deformation effects up to quadrupole deformations β2i and with “optimum” orientations θiopt. for coplanar (Φ=00) configurations. The only parameter of the model is the neck-length parameter ΔR whose value, for the nuclear proximity potential used here, remains within its range of validity (2fm). Using the best fitted ΔR's to the observed data for σff, calculated for mass region A/2±20, and σqf for the incoming channel of Fe-induced reaction at E*=33MeV, we have extended the DCM calculations to the other Ni-induced reaction, and to E*'s in the energy range 25–68 MeV. The interesting result is that the predicted evaporation residue cross section σER for 1–4 neutrons is largest for 4n decay at E*=45MeV, having the value σERσ4n105 pb for both reactions, and that the ΔR's for the three processes (ER, ff, and qf) are different, i.e., they belong to different time scales where ff occurs first, then qf and the ER at the end. Other results of interest are the predictions of the magic N=82Xe136 fragment in the ff region of mass A/2±20, and the doubly magic Pb208 in the qf region, in near close agreement with observed data (the observed fission fragment is of mass 132, instead of the predicted mass 136). The role of the weakly bound neutron-rich intermediate mass fragments and of the nucleus in the neighborhood of deformed magic Z = 108 are also indicated in the DCM calculations, which need experimental verification. For the predicted σER, the largest value of CN fusion probability PCN=0.2, and its survival probability against fission Psurv0. Further experiments are called for.

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  • Received 12 September 2016
  • Revised 14 February 2017

DOI:https://doi.org/10.1103/PhysRevC.95.044603

©2017 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

Sahila Chopra, Hemdeep, and Raj K. Gupta

  • Department of Physics, Panjab University, Chandigarh 160014, India

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Issue

Vol. 95, Iss. 4 — April 2017

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