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Program - Brookhaven National Laboratory

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Session LE Evaluated Nuclear Data Libraries<br />

Wednesday March 6, 2013<br />

Room: Central Park West at 3:30 PM<br />

LE 1 3:30 PM<br />

Development of JENDL Decay and Fission Yield Data Libraries<br />

Jun-ichi Katakura<br />

Nagaoka University of Technology<br />

The decay and fission yield data of fission products have been developed for decay heat calculation as<br />

JENDL (Japanese Evaluated Nuclear Data Library) family as JENDL/FPD-2011 and JENDL/FPY-2011.<br />

The data in the previous decay data file, JENDL FP Decay Data File 2000, have been updated based<br />

on the ENSDF (Evaluated Nuclear Structure Data File) data file. Newly measured decay energy values<br />

by TAGS (Total Absorption Gamma-ray Spectroscopy) method have been incorporated into the file. The<br />

fission yield data have been updated from the data in the JENDL-4 library. The main change came from<br />

the change of decay chains adopted in the decay data file. The number of nuclides are kept consistent<br />

between the decay data file and the fission yield file. The decay heat calculations were performed using the<br />

both updated data and compared with some measured decay heat data. The uncertainty analyses were<br />

also performed and have given the uncertainties. The components of the uncertainties were also identified<br />

from the uncertainty analyses. Similar uncertainty analyses were applied to the calculations using the<br />

ENDF and JEFF files. Their comparison with those of the JENDL library was also shown.<br />

LE 2 4:00 PM<br />

Table of E0 Electronic Factors for Conversion Electron Probabilities<br />

T. Kibédi<br />

Department of Nuclear Physics, Research School of Physics and Engineering, The Australian <strong>National</strong><br />

University, Canberra, ACT 0200, Australia<br />

G. Gosselin, V. Meot, M. Pascal,<br />

CEA, Serv. Phys. Nucl., Dept. Phys. Theor. & Appl, F-91680 Bruyeres Le Chatel, France<br />

A.E. Stuchbery<br />

Department of Nuclear Physics, Research School of Physics and Engineering, The Australian <strong>National</strong><br />

University, Canberra, ACT 0200, Australia<br />

The accurate knowledge of conversion coefficients is essential to evaluate total electromagnetic transition<br />

rates and to normalize decay schemes. The new theoretical conversion coefficient tables [1,2,3] represent a<br />

major improvement in terms of accuracy and coverage for elements between Z = 5 and 126. On the other<br />

hand, there is no universal table available yet for electric monopole (E0) transitions connecting states with<br />

the same spin–parity. In this paper we report on the tabulation of Ω(E0) electronic factors for electron<br />

conversion in Z = 2 to Z = 96 elements and all possible s 1/2 and p 1/2 atomic shells. The calculations<br />

have been carried out with a modified version [4] of the relativistic Hartree–Fock–Slater method developed<br />

by Pauli and Raff [5]. The data tables presented here cover transition energies from 1 keV up to 6000<br />

keV, similar to our recent ICC tabulations. In contrast to the internal conversion coefficients, the Ω(E0)<br />

electronic factors, can not be directly determined experimentally. Instead, the ratios of Ω(E0) values,<br />

which are proportional to the ratios of the corresponding conversion electron intensities, can be compared<br />

to theoretical ratios. A list of 80 experimental Ω(E0) ratios are presented in the first time for transitions in<br />

180

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