Effects of microscopic transport coefficients on fission observables calculated by the Langevin equation

M. D. Usang, F. A. Ivanyuk, C. Ishizuka, and S. Chiba
Phys. Rev. C 94, 044602 – Published 7 October 2016

Abstract

Nuclear fission is treated by using the Langevin dynamical description with macroscopic and microscopic transport coefficients (mass and friction tensors), and it is elucidated how the microscopic (shell and pairing) effects in the transport coefficients, especially their dependence on temperature, affects various fission observables. We found that the microscopic transport coefficients, calculated by linear response theory, change drastically as a function of temperature: in general, the friction increases with growing temperature while the mass tensor decreases. This temperature dependence brings a noticeable change in the mass distribution and kinetic energies of fission fragments from nuclei around U236 at an excitation energy of 20 MeV. The prescission kinetic energy decreases from 25 MeV at low temperature to about 2.5 MeV at high temperature. In contrast, the Coulomb kinetic energy increases as the temperature increases. Interpolating the microscopic transport coefficients among the various temperatures enabled our Langevin equation to use the microscopic transport coefficients at a deformation-dependent local temperature of the dynamical evolution. This allowed us to compare directly the fission observables of both macroscopic and microscopic calculations, and we found almost identical results under the conditions considered in this work.

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  • Received 3 June 2016
  • Revised 8 August 2016

DOI:https://doi.org/10.1103/PhysRevC.94.044602

©2016 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

M. D. Usang*

  • Tokyo Institute of Technology, Tokyo, Japan and Malaysian Nuclear Agency, Bangi, Malaysia

F. A. Ivanyuk

  • Tokyo Institute of Technology, Tokyo, Japan and Institute for Nuclear Research, Kiev, Ukraine

C. Ishizuka

  • Tokyo Institute of Technology, Tokyo, Japan

S. Chiba

  • Tokyo Institute of Technology, Tokyo, Japan and National Astronomical Observatory of Japan, Tokyo, Japan

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

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Vol. 94, Iss. 4 — October 2016

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