Analysis of the total kinetic energy of fission fragments with the Langevin equation

M. D. Usang, F. A. Ivanyuk, C. Ishizuka, and S. Chiba
Phys. Rev. C 96, 064617 – Published 22 December 2017

Abstract

We analyzed the total kinetic energy (TKE) of fission fragments with three-dimensional Langevin calculations for a series of actinides and Fm isotopes at various excitation energies. This allowed us to establish systematic trends of TKE with Z2/A1/3 of the fissioning system and as a function of excitation energy. In the mass-energy distributions of fission fragments we see the contributions from the standard, super-long, and super-short (in the case of Fm258) fission modes. For the fission fragments mass distribution of Fm258 we obtained a single peak mass distribution. The decomposition of TKE into the prescission kinetic energy and Coulomb repulsion showed that decrease of TKE with growing excitation energy is accompanied by a decrease of prescission kinetic energy. It was also found that transport coefficients (friction and inertia tensors) calculated by a microscopic model and by macroscopic models give drastically different behaviors of TKE as a function of excitation energy. The results obtained with microscopic transport coefficients are much closer to experimental data than those calculated with macroscopic ones.

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  • Received 12 June 2017
  • Revised 11 October 2017

DOI:https://doi.org/10.1103/PhysRevC.96.064617

©2017 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

M. D. Usang1,2,*, F. A. Ivanyuk1,3, C. Ishizuka1, and S. Chiba1,4

  • 1Laboratory for Advanced Nuclear Energy, Institute of Innovative Research, Tokyo Institute of Technology, 2 chome-12-1 Ookayama, Meguro, Tokyo 152-8550, Japan
  • 2Reactor Technology Center, Technical Support Division, Malaysia Nuclear Agency, Bangi, 43000 Kajang, Selangor Darul Ehsan, Malaysia
  • 3Nuclear Theory Department, Institute for Nuclear Research, Prospect Nauki 47, 03028 Kiev, Ukraine
  • 4Theoretical Division, National Astronomical Observatory of Japan, 2 chome-21-1 Osawa, Mitaka, Tokyo 181-0015, Japan

  • *usang.m.aa@m.titech.ac.jp; mark_dennis@nm.gov.my

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Vol. 96, Iss. 6 — December 2017

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