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JAEA-Conf 2011-002 - 日本原子力研究開発機構

JAEA-Conf 2011-002 - 日本原子力研究開発機構

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<strong>JAEA</strong>-<strong>Conf</strong> <strong>2011</strong>-<strong>002</strong><br />

Table 1 Comparison between ENDF/B-VII and UDV/TAGS [5] of mean - and -ray energies<br />

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Figure 1 Comparison of the FP decay-heat calculations of the -ray component of Pu-239<br />

before and after the introducing UDV/TAGS data (taken from A.Algora et al.[1])<br />

3. Evaluation<br />

3.1 Pandemonium Problem Revisited<br />

The cause of the pandemonium-problem lies in the difficulty in detecting all of the large<br />

number of -rays emitted following a -decay, and a lot of -rays, even though they were<br />

detected, cannot find their correct positions in the complex decay scheme. They are called<br />

the unplaced gammas. Therefore, nuclides having a lot of unplaced gammas are surely<br />

influenced by the pandemonium-problem. In the case of short-lived nuclides, the highest<br />

known levels of their daughter nuclides tend to be much lower than their Q-values in the<br />

decay schemes now available, which are constructed on the basis of the current<br />

high-resolution -ray data. In the case of JENDL, for most of the short-lived FP nuclides<br />

where the highest known levels in their daughter nuclides is much lower than 0.7Q, the<br />

gross theory of beta decay was introduced and this treatment lead to a good agreement<br />

between the calculations and the measurements [2]. When the -feeding to a single<br />

particular level is very large, these nuclides tend to be free from the pandemonium-problem

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