Monte Carlo approach to sequential γ-ray emission from fission fragments

S. Lemaire, P. Talou, T. Kawano, M. B. Chadwick, and D. G. Madland
Phys. Rev. C 73, 014602 – Published 19 January 2006

Abstract

A Monte Carlo simulation of the fission fragment statistical decay based on a sequential neutron followed by γ-ray emission is proposed. The γ-ray energy spectrum is calculated as a function of the mass of the fission fragments and integrated over the whole mass distribution. The prompt γ-ray multiplicity distribution, both the average number of emitted γ rays and the average γ-ray energy as a function of the mass of the fission fragments [respectively, N¯γ(A) and ɛγ(A)], are also assessed. The γ-γ correlations emitted from both light and heavy fragments are calculated as well as correlations between γ-ray energies. Results are reported for the neutron-induced fission of U235 (at 0.53 MeV neutron energy) and for the spontaneous fission of Cf252.

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  • Received 7 July 2005

DOI:https://doi.org/10.1103/PhysRevC.73.014602

©2006 American Physical Society

Authors & Affiliations

S. Lemaire1,*, P. Talou1, T. Kawano1, M. B. Chadwick2, and D. G. Madland1

  • 1Theoretical Division, Nuclear Physics Group, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
  • 2PADNWP, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA

  • *Electronic address: lemaire@lanl.gov

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Vol. 73, Iss. 1 — January 2006

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