首站-论文投稿智能助手
典型文献
Gamma ray multiplicity of a 240Pu solid sphere simulated by JMCT
文献摘要:
Determining the mass of plutonium metal is an important research objective in the field of nuclear material accounting and control.Based on the 3D neutron and photon transport code JMCT(Jointed Monte Carlo Trans-port),the gamma ray multiplicity of 240Pu was simulated in this study,and the average number of gamma rays leaking from 240Pu solid spheres with different masses was also obtained.The simulation results show that there is a one-to-one correspondence between the average number of gamma rays and the mass of 240Pu solid spheres in the range of 0.50-3.00 kg.This result provides a basis for using the average number of gamma rays to account for the mass of 240Pu.
文献关键词:
作者姓名:
Huan-Huan Ding;Fan Gao;Chang-Bing Lu;Rui Li;Chen-Guang Li;Zhao-Hong Mo;Dun-Fu Shi;Ming Su;De-Shan Zhao;Mao-Bing Shuai;Zhong-Hua Xiong;Bin-Yuan Xia;Yun Bai
作者机构:
Institute of Materials,China Academy of Engineering Physics,Mianyang 621908,China;The 93147th Unit of PLA,Mianyang 621000,China;CAEP Software Center for High Performance Numerical Simulation,Beijing 100088,China;Institute of Applied Physics and Computational Mathematics,Beijing 100088,China
引用格式:
[1]Huan-Huan Ding;Fan Gao;Chang-Bing Lu;Rui Li;Chen-Guang Li;Zhao-Hong Mo;Dun-Fu Shi;Ming Su;De-Shan Zhao;Mao-Bing Shuai;Zhong-Hua Xiong;Bin-Yuan Xia;Yun Bai-.Gamma ray multiplicity of a 240Pu solid sphere simulated by JMCT)[J].核技术(英文版),2022(05):8-15
A类:
Jointed
B类:
Gamma,multiplicity,240Pu,solid,simulated,by,JMCT,Determining,plutonium,metal,important,research,objective,field,nuclear,material,accounting,control,Based,neutron,photon,transport,code,Monte,Carlo,Trans,gamma,was,this,study,average,number,rays,leaking,from,spheres,different,masses,also,obtained,simulation,results,show,that,there,one,correspondence,between,range,This,provides,basis,using
AB值:
0.504122
相似文献
Effectiveness of coal mine dust control:A new technique for preparation and efficacy of self-adaptive microcapsule suppressant
Bo Ren;Liang Yuan;Gang Zhou;Shuailong Li;Qunzhi Meng;Kai Wang;Bingyou Jiang;Guofeng Yu-School of Emergency Management and Safety Engineering,China University of Mining and Technology-Beijing,Beijing 100083,China;State Key Laboratory of Deep Coal Mining&Environment Protection,Huainan Mining Group Co.,LTD.,Huainan 232001,China;Key Laboratory of Industrial Dust Control and Occupational Health,Ministry of Education,Anhui University of Science and Technology,Huainan 232001,China;College of Safety and Environmental Engineering,Shandong University of Science and Technology,Qingdao 266590,China;Department of Civil and Environmental Engineering,University of Alberta,Edmonton T6G 2R3,Canada
Metabolomic and elemental profiling of blood serum in bladder cancer
Krzysztof Ossoliński;Tomasz Ruman;Valérie Copié;Brian P.Tripet;Leonardo B.Nogueira;Katiane O.P.C.Nogueira;Artur Ko?odziej;Aneta P?aza-Altamer;Anna Ossolińska;Tadeusz Ossoliński;Joanna Nizio?-Department of Urology,John Paul Ⅱ Hospital,36-100,Kolbuszowa,Poland;Rzeszów University of Technology,Faculty of Chemistry,35-959,Rzeszów,Poland;The Department of Chemistry and Biochemistry,Montana State University,Bozeman,MT,59717,USA;Department of Geology,Federal University of Ouro Preto,35400-000,Ouro Preto,Brazil;Department of Biological Sciences,Federal University of Ouro Preto,35400-000,Ouro Preto,Brazil;Doctoral School of Engineering and Technical Sciences at the Rzeszów University of Technology,35-959,Rzeszów,Poland
Prospective study on observations of γ-ray sources in the Galaxy using the HADAR experiment
Xiangli Qian;Huiying Sun;Tianlu Chen;Danzengluobu;Youliang Feng;Qi Gao;Quanbu Gou;Yiqing Guo;Hongbo Hu;Mingming Kang;Haijin Li;Cheng Liu;Maoyuan Liu;Wei Liu;Bingqiang Qiao;Xu Wang;Zhen Wang;Guangguang Xin;Yuhua Yao;Qiang Yuan;Yi Zhang-School of Intelligent Engineering,Shandong Management University,Jinan 250357,China;The Key Laboratory of Cosmic Rays(Tibet University),Ministry of Education,Lhasa 850000,China;Key Laboratory of Particle Astrophysics,Institute of High Energy Physics,Chinese Academy of Sciences,Beijing 100049,China;University of Chinese Academy of Sciences,19 A Yuquan Road,Shijingshan District,Beijing 100049,China;College of Physics,Sichuan University,Chengdu 610064,China;Tsung-Dao Lee Institute,Shanghai Jiao Tong University,Shanghai 200240,China;School of Physics and Technology,Wuhan University,Wuhan 430072,China;Key Laboratory of Dark Matter and Space Astronomy,Purple Mountain Observatory,Chinese Academy of Sciences,Nanjing 210008,China
机标中图分类号,由域田数据科技根据网络公开资料自动分析生成,仅供学习研究参考。