Production and utilization of 22Na secondary beam

Sun Jun Jin, You Bao Wang, Jun Su, Sheng Quan Yan, Yun Ju Li, Bing Guo, Zhi Hong Li, Sheng Zeng, Gang Lian, Xi Xiang Bai, Wei Ping Liu, Hidetoshi Yamaguchi, Shigeru Kubono, Jun Hu, D. Kahl, Hyo Soon Jung, Jung Young Moon, Takashi Teranishi, Hong Wei Wang, Hironobu IshiyamaNaohito Iwasa, Tetsuro Komatsubara, Er Tao Li, Jian Zhang

研究成果: ジャーナルへの寄稿記事

抄録

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.

元の言語英語
ページ(範囲)2182-2186
ページ数5
ジャーナルYuanzineng Kexue Jishu/Atomic Energy Science and Technology
48
発行部数12
DOI
出版物ステータス出版済み - 12 20 2014

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Separators
Astrophysics
Neon
Ion beams
Purification
Scattering

All Science Journal Classification (ASJC) codes

  • Nuclear Energy and Engineering

これを引用

Jin, S. J., Wang, Y. B., Su, J., Yan, S. Q., Li, Y. J., Guo, B., ... Zhang, J. (2014). Production and utilization of 22Na secondary beam. Yuanzineng Kexue Jishu/Atomic Energy Science and Technology, 48(12), 2182-2186. https://doi.org/10.7538/yzk.2014.48.12.2182

Production and utilization of 22Na secondary beam. / 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; Kahl, D.; Jung, Hyo Soon; Moon, Jung Young; Teranishi, Takashi; Wang, Hong Wei; Ishiyama, Hironobu; Iwasa, Naohito; Komatsubara, Tetsuro; Li, Er Tao; Zhang, Jian.

:: Yuanzineng Kexue Jishu/Atomic Energy Science and Technology, 巻 48, 番号 12, 20.12.2014, p. 2182-2186.

研究成果: ジャーナルへの寄稿記事

Jin, SJ, Wang, YB, Su, J, Yan, SQ, Li, YJ, Guo, B, Li, ZH, Zeng, S, Lian, G, Bai, XX, Liu, WP, Yamaguchi, H, Kubono, S, Hu, J, Kahl, D, Jung, HS, Moon, JY, Teranishi, T, Wang, HW, Ishiyama, H, Iwasa, N, Komatsubara, T, Li, ET & Zhang, J 2014, 'Production and utilization of 22Na secondary beam', Yuanzineng Kexue Jishu/Atomic Energy Science and Technology, 巻. 48, 番号 12, pp. 2182-2186. https://doi.org/10.7538/yzk.2014.48.12.2182
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 ; Kahl, D. ; 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. :: Yuanzineng Kexue Jishu/Atomic Energy Science and Technology. 2014 ; 巻 48, 番号 12. pp. 2182-2186.
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abstract = "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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T1 - Production and utilization of 22Na secondary beam

AU - Jin, Sun Jun

AU - Wang, You Bao

AU - Su, Jun

AU - Yan, Sheng Quan

AU - Li, Yun Ju

AU - Guo, Bing

AU - Li, Zhi Hong

AU - Zeng, Sheng

AU - Lian, Gang

AU - Bai, Xi Xiang

AU - Liu, Wei Ping

AU - Yamaguchi, Hidetoshi

AU - Kubono, Shigeru

AU - Hu, Jun

AU - Kahl, D.

AU - Jung, Hyo Soon

AU - Moon, Jung Young

AU - Teranishi, Takashi

AU - Wang, Hong Wei

AU - Ishiyama, Hironobu

AU - Iwasa, Naohito

AU - Komatsubara, Tetsuro

AU - Li, Er Tao

AU - Zhang, Jian

PY - 2014/12/20

Y1 - 2014/12/20

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