Advanced Search
ZENG Sheng, LI Zhi-hong, LIAN Gang, WANG You-bao, SU Jun, YAN Sheng-quan, WANG Bao-xiang, GUO Bing, BAI Xi-xiang, LIU Wei-ping. Production of 13N Secondary Beam[J]. Atomic Energy Science and Technology, 2007, 41(5): 513-516. DOI: 10.7538/yzk.2007.41.05.0513
Citation: ZENG Sheng, LI Zhi-hong, LIAN Gang, WANG You-bao, SU Jun, YAN Sheng-quan, WANG Bao-xiang, GUO Bing, BAI Xi-xiang, LIU Wei-ping. Production of 13N Secondary Beam[J]. Atomic Energy Science and Technology, 2007, 41(5): 513-516. DOI: 10.7538/yzk.2007.41.05.0513
shu
    Graphical Abstract
    • Abstract
  • A 13N secondary beam to be used in the study of nuclear astrophysics was produced by the 2H(12C,13N)n reaction using the secondary beam line of the HI-13 tandem accelerator at Beijing. The energy of the 13N secondary beam is （70.2±0.7） MeV, with a purity of 91 % and the intensity of about 10 s－1•pnA-1 after collimation. The beam can be used for the study of transfer reaction in inverse kinematics.
    • FullText(HTML)
  • loading
    • References (8)
    • Related Articles

Catalog

    Turn off MathJax
    Article Contents

    /

    DownLoad:  Full-Size Img  PowerPoint
    Return
    Return