【24h】

Production of selected cosmogenic radionuclides by muons 1. Fast muons

机译:用μ子生产选定的宇宙放射性核素1.快速μ子

获取原文
获取原文并翻译 | 示例
           

摘要

To investigate muon-induced nuclear reactions leading to the production of radionuclides, targets made of C-9H_(12), SiO_2, Al_2O_3, Al, S, CaCO_3, Fe, Ni, Cu, Gd, Yb and Tl were irradiated with 100 and 190 GeV muons in the NA54 experimental setup at CERN. The radionuclide concentrations were measured with accelerator mass spectrometry and γ-spectroscopy. Results are presented for the corresponding partial formation cross-sections. Several of the long-lived and short-lived radionuclides studied are also produced by fast cosmic ray muons in the atmosphere and at depths underground. Because of their importance to earth sciences investigations, calculations of the depth dependence of production rates by fast cosmic ray muons have been made.
机译:为了研究介子引起的导致放射性核素产生的核反应,对C-9H_(12),SiO_2,Al_2O_3,Al,S,CaCO_3,Fe,Ni,Cu,Gd,Yb和Tl制成的靶进行了辐照在CERN的NA54实验装置中有190 GeV介子。放射性核素浓度通过加速器质谱和γ光谱法测量。给出了对应的部分地层横截面的结果。研究的几种长寿命和短寿命放射性核素也是由大气中和地下深处的快速宇宙射线μ子产生的。由于它们对地球科学研究的重要性,因此已经对快速宇宙射线μ子对生产率的深度依赖性进行了计算。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号