[3]姜炳,王小鹤,韩建龙,等. TMSR白光中子源能量分辨率函数的模拟研究[J].原子能科学技术, 2021,55(8):1508-1515. DOI:10.7538/yzk.2020.youxian.0594.
[4]Jiang B, Han J, Jiang W, et al. Monte-Carlo calculations of the energy resolution function with Geant4 for analyzing the neutron capture cross section of 232Th measured at CSNS Back-n[J]. Nuclear Instruments and Methods in Physics Research Section A, 2021, 1013: 165677. DOI: 10.1016/j.nima.2021.165677.
[5]Jiang B, Han J, Ren J, et al. Measurement of 232Th (n,gamma) cross section at the CSNS Back-n facility in the unresolved resonance region from 4 keV to 100 keV. Chinese Physics B, 2022, 31(6): 060101. DOI:10.1088/1674-1056/ac5394.
[6]Tian B B,Jiang B, Jing H T, et al. Monte Carlo simulation study of a novel neutron resonance radiography method for oxygen identification in oxides and composite materials. Journal of Instrumentation, 2024, 19(09): T09002.
[7]张江林,姜炳,陈永浩,等.基于中国散裂中子源反角白光中子束线的天然锂中子全截面测量.物理学报, 2022, 71(5): 052901.
[8]Wang J, Ren J, Jiang W, ......,Bing Jiang, et al. Determination of the 232Th (n, γ) cross section from 10 to 200 keV at the Back-n facility at CSNS[J]. The European Physical Journal A, 2023, 59(10): 224.
[9]胡继峰,王小鹤,姜炳,等.基于TMSR-PNS装置0.008~0.1 eV能区Th的全截面测量[J].原子能科学技术,2022,56(01):61-67.
[10]王小鹤,胡继峰,韩建龙,......,姜炳,等. TMSR白光中子源关键核数据实验进展[J].原子核物理评论,2020,37(04):908-912.
[11]王小鹤,胡继峰,刘龙祥,......,姜炳,等. TMSR白光中子源本底屏蔽设计[J].原子核物理评论,2020,37(03):777-783.
[12]黄泽棋,谭志新,李 强,......,姜炳,等.中国散裂中子源伴生质子束实验平台及其应用[J].现代应用物理,2024,15(04):40409-40409.
[13]李鑫祥,刘龙祥,蒋伟,......,姜炳,等.脉冲高度权重技术测量197Au中子俘获截面[J].核技术,2020,43(08):90-98.
[14]Li X X, Liu L X, Jiang W, ......,Jiang B, et al.[J]. New experimental measurement of Er-nat (n, γ) cross sections between 1 and 100 eV. Physical Review C, 2021, 104(5): 054302.
[15]Li X X, Liu L X, Jiang W,......,Jiang B, et al. Measurements of the 107Ag neutron capture cross sections with pulse height weighting technique at the CSNS Back-n facility[J]. Chinese Physics B, 2022, 31(3): 038204.
[16]Xinrong Hu, Gongtao Fan, Wei Jiang, ......,Bing Jiang, et al. Measurements of the 197Au(n, γ) cross section up to 100 keV at the CSNS Back-n facility. Nuclear Science and Techniques, 2021, 32(9): 1-10.
[17]Xinrong Hu, Longxiang Liu, Wei Jiang, ......,Bing Jiang, et al.New experimental measurement of natSe(n, γ)cross section between 1 eV to 1 keV at the CSNS Back-n facility[J].Chinese Physics B,2022,31(08):12-19.
[18]Li X X, Liu L X, Jiang W,......,Bing Jiang, et al. Experimental determination of the neutron resonance peak of Er 162 at 67.8 eV[J]. Physical Review C, 2022, 106(6): 065804.
[19]Yang G, An Z, Jiang W,......,Bing Jiang, et al. Measurement of the neutron capture cross sections of rhenium up to stellar s-and r-process temperatures at the China Spallation Neutron Source Back-n facility[J]. Physical Review Research, 2024, 6(1): 013225.
[20]An Z, Qiu W, Jiang W,......,Bing Jiang, et al. Measurement of the 181 Ta (n, γ) cross sections up to stellar s-process temperatures at the CSNS Back-n[J]. Scientific Reports, 2023, 13(1): 12657.
[21]Li X, An Z, Jiang W, ......,Bing Jiang,et al. Measurement of the Pr 141 (n, γ) cross section up to stellar s-process temperatures at the China Spallation Neutron Source Back-n facility[J]. Physical Review C, 2023, 108(3): 035802.
[22]Yang G L, An Z D, Jiang W,......,Bing Jiang, et al. Measurement of Br (n, γ) cross sections up to stellar s-process temperatures at the CSNS Back-n[J]. Nuclear Science and Techniques, 2023, 34(11): 180.
[23]Li X, An Z, Jiang W, ......,Bing Jiang, et al. Measurement of the nat Eu (n, γ) cross section up to 500 keV at the CSNS Back-n facility, and the stellar 151, 153 Eu (n, γ) cross section at s-process temperatures[J]. The European Physical Journal A, 2022, 58(12): 251.
招生要求