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In-beam gamma rays of CSNS Back-n characterized by black resonance filter

  • Jin-Cheng Wang,
  • Jie Ren,
  • Wei Jiang,
  • Xi-Chao Ruan,
  • Ying-Yi Liu,
  • Hao-Lan Yang,
  • Kuo-Zhi Xu,
  • Xin-Yi Pan,
  • Qi Sun,
  • Jie Bao,
  • Han-Xiong Huang,
  • Hao-Fan Bai,
  • Jiang-Bo Bai,
  • Ping Cao,
  • Qi-Ping Chen,
  • Yong-Hao Chen,
  • Wen-Hao Duan,
  • An-Chuan Fan,
  • Rui-Rui Fan,
  • Chang-Qing Feng,
  • Min-Hao Gu,
  • Chang-Cai Han,
  • Zi-Jie Han,
  • Guo-Zhu He,
  • Yong-Cheng He,
  • Yang Hong,
  • Yi-Wei Hu,
  • Zhi-Jie Jiang,
  • Ling Kang,
  • Chang-Lin Lan,
  • Bo Li,
  • Feng Li,
  • Qiang Li,
  • Xiao Li,
  • Yang Li,
  • Jie Liu,
  • Rong Liu,
  • Shu-Bin Liu,
  • Yi-Na Liu,
  • Guang-Yuan Luan,
  • Chang-Jun Ning,
  • Yi-Jia Qiu,
  • Wen-Kai Ren,
  • Zhi-Zhou Ren,
  • Zhao-Hui Song,
  • Kang Sun,
  • Zhi-Xin Tan,
  • Jing-Yu Tang,
  • Sheng-Da Tang,
  • Li-Jiao Wang,
  • Peng-Cheng Wang,
  • Zhao-Hui Wang,
  • Zhong-Wei Wen,
  • Xiao-Guang Wu,
  • Xuan Wu,
  • Ze-Peng Wu,
  • Cong Xia,
  • Li-Kun Xie,
  • Han Yi,
  • Tao Yu,
  • Yong-Ji Yu,
  • Guo-Hui Zhang,
  • Hang-Chang Zhang,
  • Qi-Wei Zhang,
  • Xian-Peng Zhang,
  • Yu-Liang Zhang,
  • Zhi-Yong Zhang,
  • Mao-Yuan Zhao,
  • Zhi-Hao Zhou,
  • Ke-Jun Zhu,
  • Chong Zou

摘要

The back-streaming white-neutron beamline (Back-n) of the China Spallation Neutron Source is an essential neutron-research platform built for the study of nuclear data, neutron physics, and neutron applications. Many types of cross-sectional neutron-reaction measurements have been performed at Back-n since early 2018. These measurements have shown that a significant number of gamma rays can be transmitted to the experimental stations of Back-n along with the neutron beam. These gamma rays, commonly referred to as in-beam gamma rays, can induce a non-negligible experimental background in neutron-reaction measurements. Studying the characteristics of in-beam gamma rays is important for understanding the experimental background. However, measuring in-beam gamma rays is challenging because most gamma-ray detectors are sensitive to neutrons; thus, discriminating between neutron-induced signals and those from in-beam gamma rays is difficult. In this study, we propose the use of the black resonance filter method and a \(\hbox {CeBr}_{3}\) CeBr 3 scintillation detector to measure the characteristics of the in-beam gamma rays of Back-n. Four types of black resonance filters, 181Ta, 59Co, natAg, and natCd, were used in this measurement. The time-of-flight (TOF) technique was used to select the detector signals remaining in the absorption region of the TOF spectra, which were mainly induced by in-beam gamma rays. The energy distribution and flux of the in-beam gamma rays of Back-n were determined by analyzing the deposited energy spectra of the \(\hbox {CeBr}_{3}\) CeBr 3 scintillation detector and using Monte Carlo simulations. Based on the results of this study, the background contributions from in-beam gamma rays in neutron-reaction measurements at Back-n can be reasonably evaluated, which is beneficial for enhancing both the experimental methodology and data analysis.