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Fission Product Yield Data for the Transmutation of Minor Actinide ...

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activities were recorded with a proportional counter<br />

<strong>for</strong> b emissions and with a NaI scintillator <strong>for</strong> g rays.<br />

The efficiency <strong>of</strong> <strong>the</strong> g ray detector was determined<br />

experimentally. Ei<strong>the</strong>r <strong>the</strong> predetermined g ray<br />

efficiency curve was used or <strong>the</strong> efficiency <strong>of</strong> <strong>the</strong><br />

g ray and b particle detectors was determined<br />

directly via <strong>the</strong> measured fission product. The total<br />

uncertainties <strong>of</strong> <strong>the</strong> data are 3–15% and include<br />

contributions from detector calibration and chemical<br />

yield, fission rate and peak area determinations.<br />

The data were taken from Table 1 <strong>of</strong> <strong>the</strong> paper<br />

(no corresponding EXFOR entry exists) and agree<br />

reasonably well with <strong>the</strong> data <strong>of</strong> Li Ze et al. [3.3.8],<br />

although <strong>the</strong>re are fewer values in <strong>the</strong> valley range.<br />

Chain yields are too large <strong>for</strong> A = 113, 134 and 135, as<br />

deduced from 113g Ag, 134 Te and 135 I, respectively. These<br />

nuclides are far from <strong>the</strong> stable nuclides <strong>of</strong> <strong>the</strong><br />

respective chains (i.e. by 2–3 charges). The adjustment<br />

factors from <strong>the</strong> literature are relatively large (when<br />

calculated using ENDF/B-VI data <strong>the</strong>y are even<br />

larger), <strong>the</strong> resulting yields are unreliable, and <strong>the</strong>ir<br />

uncertainties are increased by 10% <strong>for</strong> mass chains<br />

113 and 135, and by 13% <strong>for</strong> mass chain 134. Also, <strong>the</strong><br />

uncertainty <strong>for</strong> 99 Mo was increased from 3.5% to 5%.<br />

3.3.2.8. Fraser et al. [3.3.10]<br />

Fragment mass distributions <strong>of</strong> pre- and postneutron<br />

emission were measured by <strong>the</strong> double<br />

time <strong>of</strong> flight method, with a source intensity <strong>of</strong> 0.6–<br />

3 × 10 5 fissions/min. The flight paths were 144.3 and<br />

146.2 cm, time resolution was 1.35 ns, and data were<br />

adjusted <strong>for</strong> mass resolution.<br />

The mass yields are given <strong>for</strong> each mass<br />

number in <strong>the</strong> range 80–168, which represents a<br />

reasonably complete coverage <strong>of</strong> <strong>the</strong> mass distribution,<br />

but <strong>the</strong> measurement statistics are poor due<br />

to <strong>the</strong> weak source and <strong>the</strong> long flight distance.<br />

Fur<strong>the</strong>rmore, <strong>the</strong>re may have been some problems<br />

with <strong>the</strong> energy and mass calibration because <strong>the</strong><br />

light mass peak is narrower and <strong>the</strong> heavy mass<br />

peak is systematically shifted to <strong>the</strong> right (Fig. 3.3.1)<br />

when compared with o<strong>the</strong>r studies (e.g. Li Ze et al.,<br />

and Schmitt et al.). The data were eventually<br />

discarded in <strong>the</strong> evaluation.<br />

3.3.2.9. Adopted data<br />

All adopted and adjusted experimental data<br />

are given in Annex 3.3.1 and shown in Figs 3.3.2–<br />

3.3.5. Seven sets <strong>of</strong> data altoge<strong>the</strong>r are in agreement<br />

within <strong>the</strong> assigned uncertainties, except <strong>for</strong> a few<br />

specific data points.<br />

90<br />

FIG. 3.3.1. Comparison <strong>of</strong> data <strong>of</strong> Li Ze, Fraser and<br />

Schmitt.<br />

FIG. 3.3.2. Mass distribution from 252 Cf spontaneous<br />

fission.<br />

FIG. 3.3.3. Mass distribution from 252 Cf spontaneous<br />

fission.<br />

3.3.3. Processing <strong>of</strong> evaluated experimental data<br />

3.3.3.1. <strong>Data</strong> at mass numbers 99 and 140<br />

The yields <strong>for</strong> mass numbers 99 (Nervik<br />

[3.3.6]) and 140 (Blachot et al. [3.3.5] and Flynn et<br />

al. [3.3.7]) were used as monitors in <strong>the</strong> relative<br />

measurements. These data have to be renormalized

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