Prompt γ-ray production in neutron-induced fission of 239Pu

被引:40
|
作者
Ullmann, J. L. [1 ]
Bond, E. M. [1 ]
Bredeweg, T. A. [1 ]
Couture, A. [1 ]
Haight, R. C. [1 ]
Jandel, M. [1 ]
Kawano, T. [1 ]
Lee, H. Y. [1 ]
O'Donnell, J. M. [1 ]
Hayes, A. C. [1 ]
Stetcu, I. [1 ]
Taddeucci, T. N. [1 ]
Talou, P. [1 ]
Vieira, D. J. [1 ]
Wilhelmy, J. B. [1 ]
Becker, J. A. [2 ]
Chyzh, A. [2 ]
Gostic, J. [2 ]
Henderson, R. [2 ]
Kwan, E. [2 ]
Wu, C. Y. [2 ]
机构
[1] Los Alamos Natl Lab, Los Alamos, NM 87544 USA
[2] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA
来源
PHYSICAL REVIEW C | 2013年 / 87卷 / 04期
关键词
NUCLEAR-DATA; DANCE; CF-252;
D O I
10.1103/PhysRevC.87.044607
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
Background: The prompt gamma-ray spectrum from fission is important for understanding the physics of nuclear fission, and also in applications involving fission. Relatively few measurements of the prompt gamma spectrum from Pu-239(n, f) have been published. Purpose: This experiment measured the multiplicity, individual gamma energy spectrum, and total gamma energy spectrum of prompt fission gamma rays from Pu-239(n, f) in the neutron energy range from thermal to 30 keV, to test models of fission and to provide information for applications. Method: Gamma rays from neutron-induced fission of Pu-239 were measured using the DANCE gamma-ray calorimeter. Fission events were tagged by detecting fission products in a parallel-plate avalanche counter in the center of DANCE. The measurements were corrected for detector response using a GEANT4 model of DANCE. A detailed analysis for the gamma rays from the 1(+) resonance complex at 10.93 eV is presented. Results: A six-parameter analytical parametrization of the fission gamma-ray spectrum was obtained. A Monte Carlo Hauser-Feshbach calculation provided good general agreement with the data, but some differences remain to be resolved. Conclusions: An analytic parametrization can be made of the gamma-ray multiplicity, energy distribution, and total-energy distribution for the prompt gamma rays following neutron-induced fission of Pu-239. This parametrization may be useful for applications. Modern Monte Carlo Hauser-Feshbach calculations can do a good job of calculating the fission gamma-ray emission spectrum, although some details remain to be understood. DOI: 10.1103/PhysRevC.87.044607
引用
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页数:7
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