JIN Sun-jun, WANG You-bao, SU Jun, YAN Sheng-quan, LI Yun-ju, GUO Bing, LI Zhi-hong, ZENG Sheng, LIAN Gang, BAI Xi-xiang, LIU Wei-ping, YAMAGUCHI Hidetoshi, KUBONO Shigeru, HU Jun, D. Kahl, JUNG Hyo-soon, MOON Jung-young, TERANISHI Takashi, WANG Hong-wei, ISHIYAMA Hironobu, IWASA Naohito, KOMATSUBARA Tetsuro, LI Er-tao, ZHANG Jian. Production and Utilization of 22Na Secondary Beam[J]. Atomic Energy Science and Technology, 2014, 48(12): 2182-2186. DOI: 10.7538/yzk.2014.48.12.2182
Citation: JIN Sun-jun, WANG You-bao, SU Jun, YAN Sheng-quan, LI Yun-ju, GUO Bing, LI Zhi-hong, ZENG Sheng, LIAN Gang, BAI Xi-xiang, LIU Wei-ping, YAMAGUCHI Hidetoshi, KUBONO Shigeru, HU Jun, D. Kahl, JUNG Hyo-soon, MOON Jung-young, TERANISHI Takashi, WANG Hong-wei, ISHIYAMA Hironobu, IWASA Naohito, KOMATSUBARA Tetsuro, LI Er-tao, ZHANG Jian. Production and Utilization of 22Na Secondary Beam[J]. Atomic Energy Science and Technology, 2014, 48(12): 2182-2186. DOI: 10.7538/yzk.2014.48.12.2182
  • The 22Na secondary beam was produced via the 1H(22Ne, 22Na)n reaction at the CNS Radioactive Ion Beam separator (CRIB) in University of Tokyo. After the separation and purification with the electric-magnetic system of the separator, a high-quality 22Na secondary beam was delivered with energy of (78.3±1.0) MeV, intensity of about 2.5×105 s-1 and purity better than 90%. The 22Na secondary beam has been used for the study of the resonant scattering of 22Na+α, which is related to the neon extraordinary problem in nuclear astrophysics.
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