Author:
Tang Jingyu,Liu Rong,Zhang Guohui,Ruan Xichao,Wu Xiaoguang,An Qi,Bai Jiangbo,Bao Jie,Bao Yu,Cao Ping,Chen Haolei,Chen Qiping,Chen Yonghao,Chen Zhen,Cui Zengqi,Fan Ruirui,Feng Changqing,Gan Lin,Gao Keqing,Gao Xiaolong,Gu Minhao,Han Changcai,Han Zijie,He Guozhu,He Yongcheng,Hong Yang,Hu Yiwei,Huang Hanxiong,Huang Xiru,Jiang Haoyu,Jiang Wei,Jiang Zhijie,Jing Hantao,Kang Ling,Li Bo,Li Chao,Li Jiawen,Li Qiang,Li Xiao,Li Yang,Liu Jie,Liu Minliang,Liu Shubin,Liu Xingyan,Long Ze,Luan Guangyuan,Ning Changjun,Niu Mengchen,Qi Binbin,Ren Jie,Ren Zhizhou,Song Zhaohui,Sun Kang,Sun Zhijia,Tan Zhixin,Tang Xinyi,Tian Binbin,Wang Lijiao,Wang Pengcheng,Wang Zhaohui,Wen Jie,Wen Zhongwei,Wu Xuan,Xie Likun,Yang Xiaoyun,Yang Yiwei,Yi Han,Yu Li,Yu Tao,Yu Yongji,Zhang Linhao,Zhang Qiwei,Zhang Xianpeng,Zhang Yuliang,Zhang Zhiyong,Zhou Luping,Zhou Zhihao,Zhu Kejun,(The Back-n Collaboration)
Abstract
Abstract
The Back-n white neutron source (known as Back-n) is based on back-streaming neutrons from the spallation target at the China Spallation Neutron Source (CSNS). With its excellent beam properties, e.g., a neutron flux of approximately 1.8×107 n/cm2/s at 55 m from the spallation target, energy range spanning from 0.5 eV to 200 MeV, and time-of-flight resolution of a few per thousand, along with the equipped physical spectrometers, Back-n is considered to be among the best facilities in the world for carrying out nuclear data measurements. Since its completion and commencement of operation in May 2018, five types of cross-section measurements concerning neutron capture cross-sections, fission cross-sections, total cross-sections, light charged particle emissions, in-beam gamma spectra, and more than forty nuclides have been measured. This article presents an overview of the experimental setup and result analysis on the neutron-induced cross-section measurements and gamma spectroscopy at Back-n in the initial years.
Funder
National Key Research and Development Program
National Natural Science Foundation of China
Subject
Astronomy and Astrophysics,Instrumentation,Nuclear and High Energy Physics