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
JAEA-Conf 2011-002 - 日本原子力研究開発機構
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in this work was confirmed.<br />
(2) 153 Eu<br />
The preliminary neutron capture cross sections of 153 Eu were obtained in the neutron energy<br />
region from 0.03 eV to 4 keV as shown in Fig. 5. Widder measured the capture cross sections in the<br />
region from 0.01 to 10 eV, using a reactor with a fast chopper [6]. The results of Widder are larger than<br />
the present results by about 20 % in the thermal energy region. On the other hand, the evaluated values<br />
of JENDL-4.0 show good agreement with the present ones below 1 eV. In the energy range from 100<br />
eV to 4 keV, the present data agree well with the experimental data by Konks et al.[7] and Moxon et<br />
al.[8], while the discrepancy between the evaluated values of JENDL-4.0 and the present results<br />
ranges from 5 to 40 %. An undesirable structure is clearly observed around 0.6 eV. There is a<br />
possibility that the correction for 151 Eu as an isotopic impurity was not completely made.<br />
5. Conclusion<br />
The preliminary neutron capture cross sections of 151 Eu and 153 Eu have been measured from<br />
0.03 eV to the keV region with a pair of C6D6 detectors by the TOF method. As for 151 Eu, the present<br />
data agree well with the previous experimental data and the evaluated values of JENDL-4.0. Therefore,<br />
the validity of the weighting function derived in this work was confirmed. As for 153 Eu, the results of<br />
Widder are larger than the presents by about 20 % at the thermal energy. The evaluated values of<br />
JENDL-4.0 are in good agreement with the present ones except the energy region from 100 eV to 4<br />
keV.<br />
Acknowledgement<br />
The authors would like to express their thanks to the linac staff of the KURRI for making it<br />
possible to operate the accelerator steadily. They would also like to express their thanks to Dr. Takumi<br />
Kubota for cooperation on calculation with the EGS5, and to Prof. Samyol Lee and Mr. Naoya Abe for<br />
their helpful discussions.<br />
Counts / 25keV / γ-ray<br />
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<strong>JAEA</strong>-<strong>Conf</strong> <strong>2011</strong>-<strong>002</strong><br />
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γ-ray Energy (MeV)<br />
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Fig. 2. Simulated response function of a pair of C6D6 liquid scintillators