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^(12)C+^(12)C fusion reaction at astrophysical energies using HOPG target
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作者 Shuo Wang Yun-Zhen li +44 位作者 Long-Hui Ru Xin-Yu Wang Ning-Tao Zhang Yi-Hua Fan Yu-Cheng Feng Bing-Shui Gao Hao Huang Tao-Yu Jiao Hao Jian kuo-ang li Jia-Qing li li-Bin li Xiao-Bin li Chen-Gui Lu En-Qiang liu Bing-Feng Lv Hong-Yi Ma Hooi-Jin Ong Fu-Shuai Shi liang-Ting Sun Xiao-Dong Tang Yu Tang Bing Wang Hou-Qing Wang Yao Yang Yu-Han Zhai Jin-Long Zhang Bo Zhang Peng Zhang Zhi-Chao Zhang Xiao-Dong Xu Wei-Ping lin Chun Wen De-Hao Xie Zhi-Yong Zhang Xiao Fang Hong-Yi Wu Tao Tian Jun-Rui Ma Cheng-lin Hao Yu-Na Yang Yu-Yang Yu Xue liu Yun-Long Lu Si-Tao Zhu 《Nuclear Science and Techniques》 2025年第8期190-198,共9页
Highly oriented pyrolytic graphite (HOPG) is frequently adopted as the reaction target in12C+12C fusion reaction experiments owing to its superior purity.In this study,we investigate the reaction yield dependence on t... Highly oriented pyrolytic graphite (HOPG) is frequently adopted as the reaction target in12C+12C fusion reaction experiments owing to its superior purity.In this study,we investigate the reaction yield dependence on the accumulated beam dose on HOPG target using a novel detection system consisting of a time-projection chamber and silicon array.The reaction yields are significantly reduced under intense beam bombardment owing to radiation damage to the HOPG surface.The α_(0) and p_(0,1) yields decrease by 51.5% and 25%,respectively,when the ^(12)C^(2+) beam dose accumulates at 5 C.Using the novel detection system and HOPG target,the α0yield is determined to be 2.68_(-1.69)^(+4.69)×10^(-17/12) C after correcting for the yield loss due to radiation damage.Our result represents the highest sensitivity achieved to date in direct measurements of ^(12)C(12C,α_(0))^(20)Ne. 展开更多
关键词 Massive star Fusion reaction Projection chamber Low background
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Development of a low-background neutron detector array 被引量:5
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作者 Yu-Tian li Wei-Ping lin +14 位作者 Bing-Shui Gao Han Chen Hao Huang Yu Huang Tao-Yu Jiao kuo-ang li Xiao-Dong Tang Xin-Yu Wang Xiao Fang Han-Xiong Huang Jie Ren Long-Hui Ru Xi-Chao Ruan Ning-Tao Zhang Zhi-Chao Zhang 《Nuclear Science and Techniques》 SCIE EI CAS CSCD 2022年第4期10-18,共9页
A low-background neutron detector array was developed to measure the cross section of the ^(13)C(a,n)^(16)O reaction,which is the neutron source for the s-process in AGB stars,in the Gamow window(E_(c.m.)=190±40 ... A low-background neutron detector array was developed to measure the cross section of the ^(13)C(a,n)^(16)O reaction,which is the neutron source for the s-process in AGB stars,in the Gamow window(E_(c.m.)=190±40 keV)at the China Jinping Underground Laboratory(CJPL).The detector array consists of 24^(3)He proportional counters embedded in a polyethylene cube.Owing to the deep underground location and a borated polyethylene shield around the detector array,a low background of 4.5(2)/h was achieved.The ^(51)V(p,n)^(51)Cr reaction was used to determine the neutron detection efficiency of the array for neutrons with energies E_(n)<1 MeV.Geant4 simulations are shown to effectively reproduce the experimental results.They were used to extrapolate the detection efficiency to higher energies for neutrons emitted in the ^(13)C(α,n)^(16)O reaction.The theoretical angular distributions of the ^(13)C(α,n)^(16)O reaction were shown to be important in the estimation of the uncertainties of the detection efficiency. 展开更多
关键词 Underground laboratory Neutron detector Low background ^(3)He Counter
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