Late Time Emission of Prompt Fission Gamma Rays
arXiv:1607.00337 · doi:10.1103/PhysRevC.94.064613
Abstract
The emission of prompt fission rays within a few nanoseconds to a few microseconds following the scission point is studied in the Hauser-Feshbach formalism applied to the deexcitation of primary excited fission fragments. Neutron and -ray evaporations from fully accelerated fission fragments are calculated in competition at each stage of the decay, and the role of isomers in the fission products, before -decay, is analyzed. The time evolution of the average total -ray energy, average total -ray multiplicity, and fragment-specific -ray spectra, is presented in the case of neutron-induced fission reactions of U and Pu, as well as spontaneous fission of Cf. The production of specific isomeric states is calculated and compared to available experimental data. About 7% of all prompt fission rays are predicted to be emitted between 10 nsec and 5 sec following fission, in the case of U and Pu reactions, and up to 3% in the case of Cf spontaneous fission. The cumulative average total -ray energy increases by 2 to 5% in the same time interval. Finally, those results are shown to be robust against significant changes in the model input parameters.
arXiv comment11 pages, 14 figures
References in corpus (1)
Cited by in corpus (10)
- Review on the progress in nuclear fission
- Theory of Nuclear Fission
- Fission Fragment Decay Simulations with the CGMF Code
- Correlated Prompt Fission Data in Transport Simulations
- Hauser-Feshbach fission fragment de-excitation with calculated macroscopic-microscopic mass yields
- Improved modeling of photon observables with FREYA
- High resolution measurement of tagged two-neutron energy and angle correlations in Cf-252(sf)
- Energy dependence of the prompt -ray emission from the -induced fission of and
- Event-by-Event Multiplicity Correlations in Cf(sf)
- Consideration of memory of spin and parity in the fissioning compound nucleus by applying the Hauser-Feshbach fission fragment decay model to photonuclear reactions