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

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3.3.4. Results and discussion<br />

The results <strong>of</strong> <strong>the</strong> normal spline fit are given in<br />

Annex 3.3.2, while <strong>the</strong> results <strong>of</strong> <strong>the</strong> spline fit with<br />

symmetric reflection are given in Annex 3.3.3. Both<br />

are compared with <strong>the</strong> evaluated experimental data<br />

(Figs 3.3.2–3.3.5).<br />

Total yields under <strong>the</strong> light and heavy mass<br />

peaks, as well as v – , were calculated in order to check<br />

<strong>the</strong> correctness <strong>of</strong> <strong>the</strong> spline fit curve. The<br />

borderline between <strong>the</strong> light and heavy mass peaks<br />

was taken at mass 124, which was calculated from<br />

<strong>the</strong> mass number <strong>of</strong> 252 Cf and v – = 3.7661<br />

(Table 3.3.2). As shown by <strong>the</strong> normal spline fit, <strong>the</strong><br />

integral yield under <strong>the</strong> heavy mass peak is in good<br />

agreement with 100%, while <strong>the</strong> total yield under<br />

<strong>the</strong> light mass peak is in similar agreement within an<br />

uncertainty <strong>of</strong> 1.3%, and v – is in agreement with <strong>the</strong><br />

internationally recommended value <strong>of</strong> 3.7661 within<br />

an uncertainty <strong>of</strong> 2.93%. Similarly, <strong>for</strong> <strong>the</strong><br />

symmetric fit <strong>the</strong> integral yield under <strong>the</strong> light and<br />

heavy mass peak is in agreement with 100% within<br />

an uncertainty <strong>of</strong> 1.0%, and v – is in agreement with<br />

<strong>the</strong> internationally recommended value <strong>of</strong> 3.7661<br />

within an uncertainty <strong>of</strong> 1.86%.<br />

A comparison between <strong>the</strong> results <strong>of</strong> fits with<br />

and without symmetric reflection is shown in<br />

Fig. 3.3.6. These data are in very good agreement,<br />

but <strong>the</strong>re are some differences in <strong>the</strong> peak regions.<br />

The light mass peak without symmetric reflection is<br />

narrower than <strong>the</strong> equivalent peak with symmetric<br />

reflection, and <strong>the</strong> situation is <strong>the</strong> reverse <strong>for</strong> <strong>the</strong><br />

heavy mass peak. Also, <strong>the</strong> right hand side <strong>of</strong> <strong>the</strong><br />

light peak is narrower <strong>for</strong> <strong>the</strong> normal fit than <strong>for</strong> <strong>the</strong><br />

symmetric fit, but <strong>the</strong> left hand side <strong>of</strong> <strong>the</strong> heavy<br />

mass peak is <strong>the</strong> opposite (see Figs 3.3.1 and 3.3.8).<br />

c 2 is 1.551 <strong>for</strong> <strong>the</strong> normal fit and 1.795 <strong>for</strong> symmetric<br />

fit, indicating that <strong>the</strong> mass distribution is not<br />

completely symmetric around <strong>the</strong> reflection point.<br />

The fits to <strong>the</strong> results imply that <strong>the</strong>re is a<br />

systematic trend towards <strong>the</strong> light fragment peak<br />

being higher and narrower and <strong>the</strong> area under <strong>the</strong><br />

peak being slightly smaller. Individual experimental<br />

data by different authors also exhibit <strong>the</strong> same<br />

92<br />

FIG. 3.3.6. Comparison <strong>of</strong> regular and symmetric spline fit:<br />

mass distribution.<br />

FIG. 3.3.7. Comparison <strong>of</strong> regular and symmetric spline fit:<br />

light mass peak.<br />

trend. Table 3.3.3 shows some <strong>of</strong> <strong>the</strong> results from<br />

different authors, who measured a wide range <strong>of</strong><br />

fission products so that integrals <strong>of</strong> <strong>the</strong> yields under<br />

<strong>the</strong> peaks can be calculated more reliably. These<br />

integral data are given in <strong>the</strong> papers by Li Ze et al.<br />

and Chen et al., and were calculated <strong>for</strong> Schmitt et<br />

al. and Fraser et al. by using <strong>the</strong>ir original data<br />

without any adjustments. The yields under <strong>the</strong> light<br />

mass peak are smaller than those under <strong>the</strong> heavy<br />

mass peak in all four cases. Comparing <strong>the</strong> light and<br />

heavy mass peak yields <strong>of</strong> Li Ze et al. and Schmitt et<br />

al. (Figs 3.3.9 and 3.3.10), <strong>the</strong> light peak can be seen<br />

to be narrower than <strong>the</strong> heavy peak — this<br />

TABLE 3.3.2. REDUCED c 2 , TOTAL YIELD AND v – FROM FITTED DATA<br />

Fit mode Reduced c 2<br />

Total yield<br />

Light peak Heavy peak Total<br />

Normal 1.551 98.76 99.77 198.52 3.8764<br />

Symmetric 1.795 98.98 98.96 197.95 3.6962<br />

v –

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