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Statistical Hauser-Feshbach theory with width-fluctuation correction including direct reaction channels for neutron-induced reactions at low energies

Journal Article · · Physical Review C
 [1];  [2];  [3];  [3]
  1. Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
  2. International Atomic Energy Agency, Vienna (Austria)
  3. CEA, DAM, DIF, Arpajon (France)
Here, a model to calculate particle-induced reaction cross sections with statistical Hauser-Feshbach theory including direct reactions is given. The energy average of the scattering matrix from the coupled-channels optical model is diagonalized by the transformation proposed by Engelbrecht and Weidenmüller [C. A. Engelbrecht and H. A. Weidenmüller, Phys. Rev. C 8, 859 (1973)]. The ensemble average of S -matrix elements in the diagonalized channel space is approximated by a model of Moldauer [P. A. Moldauer, Phys. Rev. C 12, 744 (1975)] using the newly parametrized channel degree-of-freedom νa to better describe the Gaussian orthogonal ensemble (GOE) reference calculations. The Moldauer approximation is confirmed by a Monte Carlo study using a randomly generated S matrix, as well as the GOE threefold integration formula. Lastly, the method proposed is applied to the 238U(n,n') cross-section calculation in the fast-energy range, showing an enhancement in the inelastic scattering cross sections.
Research Organization:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Sponsoring Organization:
USDOE; USDOE National Nuclear Security Administration (NNSA)
Grant/Contract Number:
AC52-06NA25396
OSTI ID:
1457256
Alternate ID(s):
OSTI ID: 1267546
Report Number(s):
LA-UR--15-26433
Journal Information:
Physical Review C, Journal Name: Physical Review C Journal Issue: 1 Vol. 94; ISSN PRVCAN; ISSN 2469-9985
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English

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Cited By (12)

Inter-comparison of Hauser-Feshbach model codes toward better actinide evaluations journal January 2017
Reverse engineering nuclear properties from rare earth abundances in the r process journal February 2017
Neutron- γ competition for β -delayed neutron emission journal December 2016
Neutron inelastic scattering on 54Fe journal October 2018
The Origin of r -process Elements in the Milky Way journal March 2018
β -delayed Fission in r -process Nucleosynthesis journal December 2018
Actinide Production in the Neutron-rich Ejecta of a Neutron Star Merger journal December 2018
Actinide-rich and Actinide-poor r -process-enhanced Metal-poor Stars Do Not Require Separate r -process Progenitors journal August 2019
Gamma Rays from Kilonova: A Potential Probe of r -process Nucleosynthesis journal February 2020
Reverse engineering nuclear properties from rare earth abundances in the $r$ process text January 2016
Actinide-rich and Actinide-poor $r$-Process Enhanced Metal-Poor Stars do not Require Separate $r$-Process Progenitors text January 2019
Gamma-rays from kilonova: a potential probe of r-process nucleosynthesis text January 2019

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