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Figure 6. FP target configuration<br />

a) Plate Type for I-129 b) Rod Type for I-129<br />

Table 3 shows the results of evaluations. The higher transmutation rate for both 99 Tc and 129 I are<br />

achieved in Type B than Type A. The loading amount of 129 I for Type B is reduced by 30% compared<br />

to that of Type A. However, there is not much difference between two types in terms of the total<br />

amount of the transmuted 129 I. In addition, the pin power peaking is kept within an acceptable range in<br />

both types.<br />

Table 3. Performance of FP Targets in the HYPER System<br />

Target<br />

configuration<br />

Type A<br />

Initial loading<br />

(kg)<br />

Transmuted<br />

(kg/yr)<br />

Transmutation<br />

rate(%/yr)<br />

99<br />

Tc 901.8 54.2 6.01<br />

129<br />

I 129.72 13.12 10.09<br />

Pin power<br />

peaking<br />

1.211<br />

Type B<br />

99<br />

Tc 901.8 57.8 6.41<br />

129<br />

I 93.8 13 13.90<br />

1.232<br />

As mentioned before, the support ratio of the HYPER is expected to be about ~5. In terms of<br />

material balance, the HYPER system is desired to have the support ratio for 99 Tc and 129 I similar to that<br />

of TRU. The optimised configuration Type B can transmute 57.8 kg, 13 kg of 99 Tc and 129 I,<br />

respectively. In general, LWR (1.0 GWth) produces about 8.826 kg of 99 Tc and 2.721 kg of 129 I a year.<br />

The HYPER system itself generates about 7.9 kg and 2.3 kg of 99 Tc and 129 I due to the TRU<br />

transmutation. As results, the net support ratios of the HYPER are estimated to be 5.7 and 4.0 for 99 Tc<br />

and 129 I, respectively. The fission product support ratios are very close to that of TRU in the HYPER<br />

system.<br />

6. Safety factor evaluation<br />

As mentioned, the localised thermal flux increases the pin power peaking of TRU assemblies.<br />

The target configuration is optimised to minimise such an impact. Figures 7 and 8 represent the<br />

neutron energy spectrum for the target configuration of Type A and B. The energy spectrum for the<br />

485

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