1982
DOI: 10.1103/physrevc.25.524
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Beta decay properties using a statistical model

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Cited by 12 publications
(12 citation statements)
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“…Benchmarking of the CINDER-10 calculations contributing to ENDF/B-VI showed good agreement with measuredν d data [139]. However, application of the ENDF/B-VI temporal fits showed that the mean delayed neutron emission time following a fission event was lower by a factor of 2 to 3 than that predicted by functions fit to measurements.…”
Section: Delayed Neutronsmentioning
confidence: 65%
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“…Benchmarking of the CINDER-10 calculations contributing to ENDF/B-VI showed good agreement with measuredν d data [139]. However, application of the ENDF/B-VI temporal fits showed that the mean delayed neutron emission time following a fission event was lower by a factor of 2 to 3 than that predicted by functions fit to measurements.…”
Section: Delayed Neutronsmentioning
confidence: 65%
“…Most precursor spectra were modeled using either the BETA code of Mann, Dunn and Schenter [139] or an evaporation spectrum. Detailed fine-binned spectra were accumulated for the six temporal groups by assigning contributions of each precursor to neighboring temporal groups while enforcing maximum likelihood to total spectra.…”
Section: Delayed Neutronsmentioning
confidence: 99%
“…The statistical theory has been applied to calculate the decay probabilities of the excited states in the past [4][5][6][7][8]. However, due to the lack of detailed nuclear-structure calculations and approximations made for the neutron and γ -ray penetration probabilities, these studies only reproduce the general trend of the experimental data.…”
Section: B Neutron Emission From Excited Statesmentioning
confidence: 99%
“…(2). The ENDF/B-VI evaluation for 80 Ga is based on experimental data [26][27][28] in the energy range 100 keV-1.05 MeV, and the BETA code [8] was employed to extrapolate the spectrum outside the range [3]. Because our calculations consider all the possible transitions between the excited states in the daughter and granddaughter nuclei, the details of the complicated structure in the experimental spectra, which cannot be reproduced by an evaporation or Maxwellian spectrum [29], are present in our results.…”
Section: A Structure In Neutron Spectramentioning
confidence: 99%
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