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Title: New calculation of prompt fission neutron spectra and average prompt neutron multiplicities

Journal Article · · Nucl. Sci. Eng.; (United States)
DOI:https://doi.org/10.13182/NSE82-5· OSTI ID:7156632

On the basis of standard nuclear evaporation theory, the authors calculate the prompt fission neutron spectrum N(E) as a function of both the fissioning nucleus and its excitation energy. To simulate the initial distribution of fission-fragment excitation energy and the subsequent cooling of the fragments as neutrons are emitted, they take the distribution of fission-fragment residual nuclear temperature to be triangular in shape, extending linearly from zero to a maximum value T /SUB m/ . This maximum temperature is determined from the average energy release, the separation energy and kinetic energy of the neutron inducing fission, the total average fission-fragment kinetic energy, and the level density parameter of the Fermi gas model. The neutron energy spectrum for fixed residual nuclear temperature is integrated over this triangular distribution to obtain the neutron energy spectrum in the center-of-mass system of a given fission fragment, which is then transformed to the laboratory system. When the cross section sigma /SUB c/ for the inverse process of compound nucleus formation is assumed constant, N(E) is the sum of a four-term closed expression involving the exponential integral and the incomplete gamma function for the light fragment and an analogous result for the heavy fragment. The authors also calculate N(E) by numerical integration for an energy-dependent cross section sigma /SUB c/ that is obtained from an optical model; this shifts the peak in N(E) to somewhat lower neutron energy and changes the overall shape slightly.

Research Organization:
Los Alamos National Laboratory, Theoretical Division P.O. Box 1663, Los Alamos, New Mexico 87545
OSTI ID:
7156632
Journal Information:
Nucl. Sci. Eng.; (United States), Vol. 81:2
Country of Publication:
United States
Language:
English