Author:
He Chuangye,Dang Yongle,Liu Fulong,Fu Guangyong,Wu Di,Shen Yangping,Han Zhiyu,Fan Qiwen,Guo Bing,Wang Naiyan
Abstract
The (p, γ) resonance is a good way to produce monoenergetic γ rays. It becomes an important tool for studying photonuclear reactions. In this work, 13C(p, γ)14N resonance is studied to produce 9.17 MeV γ ray using the 2 × 1.7 MV tandem accelerator at CIAE. The flux of 9.17 MeV γ was determined to be 2.3 × 105/s. 197Au photoneutron cross section was measured to be 45.4 ± 6.9 mb under the irradiation of 13C(p, γ)14N resonance γ -source. The value is close to the previous results. It certificates that we have developed an experimental method for photonuclear reaction study.
Reference27 articles.
1. IAEA, Handbook on photonuclear data for applications: Cross-Sections and spectra (International Atomic Energy Agency, Vienna, 2000) IAEA Report No. 1178.
2. Nuclear astrophysics
3. The p-process in supernovae
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