Neutron capture cross section of 169Tm measured at the CSNS Back-n facility in the energy region from 30 keV to 300 keV

Author:

Ren JieORCID,ruan xichao,Jiang Wei,Bao Jie,wang jincheng,Zhang Qiwei,Luan Guangyuan,Huang Hanxiong,Nie YangBo,Ge Zhigang,An Qi 安琪,Bai Huaiyong,Bao Yu,Cao PingORCID,Chen Haolei,Chen Qiping,Chen Yonghao,Chen Yukai,Chen Zhen,Cui Zengqi,Fan Rui-Rui,Feng Changqing,Gao Keqing,Gu Minhao,Han Changcai,Han Zijie,He Guozhu,He Yongcheng,Hong Yang,Huang Weiling,Huang Xiru,Ji Xiaolu,Ji Xuyang,Jiang Haoyu,Jiang Zhijie,Jing Hantao,Kang Ling,Kang Mingtao,Li Bo,Li Chao,Li Jiawen,Li Lun,Li Qiang,Li Xiao,Li Yang,Liu RongORCID,Liu Shubin,Liu Xingyan,Mu Qili,Ning Changjun,Qi Binbin,Ren Zhizhou,Song Yinpeng,Song Zhaohui,Sun Hong 孙虹,Sun Kang,Sun Xiaoyang,Sun Zhijia,Tan Zhixin,Tang Hongqing,Tang JingyuORCID,Tang Xinyi,Tian Binbin,Wang Lijiao,Wang Pengcheng,Wang Qi,Wang TaofengORCID,Wang Zhaohui,Wen Jie,Wen Zhongwei,Wu QingbiaoORCID,Wu Xiao-Guang 吴晓光,wu xi,Xie Likun,Yang Yiwei,Yi Han,Yu Li,Yu Tao,Yu Yongji,Zhang Guo-Hui 张国辉ORCID,Zhang Linhao,Zhang Xian-Peng,Zhang Yuliang,Zhang ZhiyongORCID,Zhao Yu-Bin,Zhou Luping,Zhou Zuying,Zhu Danyang,Zhu KejunORCID,Zhu Peng

Abstract

Abstract The capture cross sections of the 169Tm(n, γ) reaction were measured at the back streaming white neutron beam line (Back-n) of the China Spallation Neutron Source (CSNS) using four C6D6 liquid scintillation detectors. To obtain accurate cross sections, the background subtraction, normalization, and correction were carefully taken into consideration in the data analysis. For the resonance at 3.9 eV, the R-matrix code SAMMY was used to determine the resonance parameters with internally normalization method. While the average capture cross sections of 169Tm in the energy range between 30 keV and 300 keV were extracted relative to the 197Au(n, γ) reaction. The measured cross sections of the 169Tm(n, γ) reaction were reported in logarithmically equidistant energy bins with 20 bins per energy decade with a total uncertainty of 5.4%-7.0% in this paper, and described in terms of average resonance parameters by means of a Hauser-Feshbach calculation with fluctuations. Both of the point-wise cross sections and the averge resonance parameters showed fair agreement with the evaluated values of ENDF/B-VIII.0 library in the energy region studied.

Funder

National Natural Science Foundation of China

National Key Research and Development Program of China

Publisher

IOP Publishing

Subject

Astronomy and Astrophysics,Instrumentation,Nuclear and High Energy Physics

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