Skyrme forces and decay of the Rf*104266 nucleus synthesized via different incoming channels

Niyti, Aman Deep, Rajesh Kharab, Sahila Chopra, and Raj K. Gupta
Phys. Rev. C 95, 034602 – Published 7 March 2017

Abstract

The excitation functions for the production of Rf262, Rf261, and Rf260 isotopes via 4n-, 5n-, and 6n-decay channels from the Rf*266 compound nucleus are studied within the dynamical cluster-decay model (DCM), including deformations β2i and so-called hot-optimum orientations θi which support symmetric fission, in agreement with experiments. The data are available for O18+Cm248 and Ne22+Pu244 reactions, respectively, at the energy ranges of Elab=88.2 to 101.3 and 109.0 to 124.8 MeV. For the nuclear interaction potentials, we use the Skyrme energy density functional (SEDF) based on semiclassical extended Thomas Fermi (ETF) approach, which means an extension of the earlier study of excitation functions of Rf*266 formed in O18+Cm248 reaction, based on the DCM using the pocket formula for nuclear proximity potential, showing interaction dependence. The Skyrme forces used here are the old SIII and SIV and new GSkI and KDE0(v1) given for both normal and isospin-rich nuclei, with densities added in frozen density approximation. Interestingly, the DCM gives an excellent fit to the measured data on fusion evaporation residue (ER) for both the incoming channels (O18+Cm248 and Ne22+Pu244) at the energy range Elab=88.2 to 124.8 MeV, independent of the entrance channel and Skyrme force used. The possible fusion-fission (ff) and quasifission (qf) mass regions of fragments on DCM are also predicted. The DCM with Skyrme forces is further used to look for all the possible target-projectile (t-p) combinations forming the cold compound nucleus (CN) Rf*266 at the CN excitation energy of Elab for hot compact configurations. The fusion evaporation residue cross sections, for the proposed new reactions in synthesizing the CN Rf*266, are also estimated for the future experiments, and role of mass asymmetry of nuclei is indicated.

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  • Received 21 January 2017
  • Revised 14 February 2017

DOI:https://doi.org/10.1103/PhysRevC.95.034602

©2017 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

Niyti1, Aman Deep1, Rajesh Kharab1, Sahila Chopra2, and Raj K. Gupta2

  • 1Department of Physics, Kurukshetra University, Kurukshetra 136119, India
  • 2Department of Physics, Panjab University, Chandigarh 160014, India

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Issue

Vol. 95, Iss. 3 — March 2017

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