期刊文献+

中国锦屏地下实验室缪子辐射环境蒙特卡罗方法模拟 被引量:1

Monte Carlo simulation of muon radiation environment in China Jinping Underground Laboratory
下载PDF
导出
摘要 用蒙特卡罗方法对中国锦屏地下实验室(CJPL)的缪子辐射本底进行了模拟。在对宇宙线缪子进行模拟时,依据海平面缪子流强Gaisser公式建立模型,并利用MUSIC程序,模拟了CJPL实验室的剩余缪子归一化能谱,进一步利用FLUKA程序模拟得到了缪致光子、中子的产额和平均能量。结果表明:剩余缪子的平均能量369GeV,通量3.17×10-6 m-2·s-1,次级光子总的注量率约1.57×10-4 m-2·s-1,次级中子总的注量率约8.37×10-7 m-2·s-1。通过与世界上其他地下实验室本底水平的对比,表明CJPL的缪子辐射环境低于世界上大多数地下实验室。 Muon radiation background of China Jinping Underground Laboratory(CJPL) was simulated by Monte Carlo method.According to the Gaisser formula and the MUSIC soft,the model of cosmic ray muons was established.Then the yield and the average energy of muon-induced photons and muon-induced neutrons were simulated by FLUKA.With the single-energy approximation,the contribution to the radiation background of shielding structure by secondary photons and neutrons was evaluated.The estimation results show that the average energy of residual muons is 369 GeV and the flux is 3.17×10^-6 m^-2·s^-1.The fluence rate of secondary photons is about 1.57×10^-4 m-2·s-1,and the fluence rate of secondary neutrons is about 8.37×10^-7 m^-2·s^-1.The muon radiation background of CJPL is lower than those of most other underground laboratories in the world.
出处 《强激光与粒子束》 EI CAS CSCD 北大核心 2012年第12期3015-3018,共4页 High Power Laser and Particle Beams
基金 国家自然科学基金项目(11175099 11035002 11075091 11105081)
关键词 宇宙线 缪子 辐射本底 蒙特卡罗方法 cosmic ray muon radiation background Monte Carlo method
  • 相关文献

参考文献12

  • 1程建平,吴世勇,岳骞,申满斌.国际地下实验室发展综述[J].物理,2011,40(3):149-154. 被引量:27
  • 2Li L, Yue Q’ Tang C,et al. A Monte Carlo study for the shielding of gamma backgrounds induced by radionuclides for CDEX[J]. ChinesePhysics C ,20X1, 35(3): 282-287.
  • 3Breier R,Povinec P P. Simulation of background characteristics of low-level gamma-ray spectrometers using Monte Carlo method[J]. Ap-plied Radiation and Isotopes , 2010,68(7/8) : 1231-1235.
  • 4阿尔科费尔.宇宙线人门[M].北京:科学出版社,1987:155-159.
  • 5Beringer J,Arguin J F,Barnett R M, et al. Review of particle physics[J]. Phys Rev D .2012,86:010001.
  • 6Kudryavtsev V A. Muon simulation codes MUSIC and MU SUN for underground physics[J]. Computer Physics Communications , 2009,180: 339-346.
  • 7Antonioli P, Ghetti C, Korolkova E V,et al. A three-dimensional code for muon propagation through the rock: MUSIC[J]. AstroparticlePhysics,1997,7(4): 357-368.
  • 8Gaisser T K. Cosmic rays and particle physics [M]. London: Cambridge University Press, 1990.
  • 9Bettini A. Underground laboratories[J]. Nuclear Instruments and Methods in Physics Research A , 2011, 626/627 : S64-S68.
  • 10Carson M J,Davies J C, Daw E, et al. Neutron background in large-scale xenon detectors for dark matter searches[J], AstroparticlePhysics, 2004,21(6): 667-687.

二级参考文献14

  • 1美国杜赛尔实验室网站:http://www.dusel.org.
  • 2加拿大斯诺实验室网站:http://www.srlo.phy.queensu.ca.
  • 3日本神冈实验室网站:http://www-sk.icrr.u-tokyo.ac.jp/index-e.html.
  • 4韩国襄阳实验室网站dmrc.snu.ac.kr.
  • 5意大利格兰萨索实验室网站www.1ngs.infn.it.
  • 6法国摩丹实验室网站www-lsm.in2p3.fr.
  • 7英国伯毕实验室网站www.hep.shef.ac.uk/research/dm/boulby/info.php.
  • 8西班牙坎弗兰克实验室网站www.1sc-canfranc.es.
  • 9俄罗斯伯克山实验室网站www.inr.troitsk.ru/eng/ebno.ht-ml.
  • 10二滩水电开发有限责任公司网站http://www.ehdc.com.cn/.

共引文献26

引证文献1

二级引证文献6

相关作者

内容加载中请稍等...

相关机构

内容加载中请稍等...

相关主题

内容加载中请稍等...

浏览历史

内容加载中请稍等...
;
使用帮助 返回顶部