Compound nucleus formation probability PCN determined within the dynamical cluster-decay model for various “hot” fusion reactions

Arshdeep Kaur, Sahila Chopra, and Raj K. Gupta
Phys. Rev. C 90, 024619 – Published 26 August 2014

Abstract

The compound nucleus (CN) fusion/formation probability PCN is defined and its detailed variations with the CN excitation energy E*, center-of-mass energy Ec.m., fissility parameter χ, CN mass number ACN, and Coulomb interaction parameter Z1Z2 are studied for the first time within the dynamical cluster-decay model (DCM). The model is a nonstatistical description of the decay of a CN to all possible processes. The (total) fusion cross section σfusion is the sum of the CN and noncompound nucleus (nCN) decay cross sections, each calculated as the dynamical fragmentation process. The CN cross section σCN is constituted of evaporation residues and fusion-fission, including intermediate-mass fragments, each calculated for all contributing decay fragments (A1, A2) in terms of their formation and barrier penetration probabilities P0 and P. The nCN cross section σnCN is determined as the quasi-fission (qf) process, where P0=1 and P is calculated for the entrance-channel nuclei. The DCM, with effects of deformations and orientations of nuclei included in it, is used to study the PCN for about a dozen “hot” fusion reactions forming a CN of mass number A100 to superheavy nuclei and for various different nuclear interaction potentials. Interesting results are that PCN=1 for complete fusion, but PCN<1 or PCN1 due to the nCN contribution, depending strongly on different parameters of the entrance-channel reaction but found to be independent of the nuclear interaction potentials used.

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  • Received 12 April 2014
  • Revised 3 July 2014

DOI:https://doi.org/10.1103/PhysRevC.90.024619

©2014 American Physical Society

Authors & Affiliations

Arshdeep Kaur, Sahila Chopra, and Raj K. Gupta

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

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Issue

Vol. 90, Iss. 2 — August 2014

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