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2- 8 Confirmation of Astrophysically Important 6.15 MeV, 1- State in 18Ne via Resonant Scattering of 17F+p
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作者 Hu Jun He Jianjun +14 位作者 Xu Shiwei H. Yamaguchi Ma Peng D. Kahl Su Jun Wang Hongwei t. nakao Y. Wakabayashi J. Y. Moon t. teranishi H. S. Jung t. Hashimoto A. Chen D.Irvines S. Kubono 《IMP & HIRFL Annual Report》 2013年第1期43-44,共2页
关键词 英语 阅读 理解 物理研究
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2-13 Stellar Reaction Rate of the 14O(α, p)17F
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作者 Hu Jun He Jianjun +14 位作者 Xu Shiwei H. Yamaguchi Ma Peng D. Kahl Su Jun Wang Hongwei t. nakao Y. Wakabayashi J. Y. Moon t. teranishi H. S. Jung t. Hashimoto A. Chen D. Irvine S. Kubono 《IMP & HIRFL Annual Report》 2014年第1期45-46,共2页
Proton resonant states in 18Ne have been investigated by the resonant scattering of 17F+p with a 17F beambombarding a thick H2 gas target. Several resonances have been observed. In particular, the astrophysically cruc... Proton resonant states in 18Ne have been investigated by the resonant scattering of 17F+p with a 17F beambombarding a thick H2 gas target. Several resonances have been observed. In particular, the astrophysically crucialstate 6.15 MeV was observed as a spin-parity assignment of 1?? with high statistics. The groove-like structureobserved in this work is completely different with previous peak one[1]. The confirmation of 1?? on a firm groundclarified this significant discrepancy. In addition, a new state was observed at Ex = 6.85 MeV with a tentativespin assignment of 0, which could be the mirror state of 6.88 MeV, 0?? in 18O, or a bandhead state (0+) of thesix-particle four-hole (6p-4h) band[2,3]. The resonant parameters have been determined by an R-matrix analysis ofthe excitation functions. 展开更多
关键词 STELLAR REACTION RATE
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Confirmation/Observation of Hindered E2 Strengths in ^(16,18)C
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作者 H. J. Ong N. Imai +20 位作者 D. Suzuki H. Iwasaki H. Sakurai t. Onishi M. Suzuki S. Ota S. takeuchi t. nakao Y. togano Y. Kondo N. Aoi H. Baba B. Shawn Y. Ichikawa M. Ishihara t. Kubo K. Kurita t. Motobayashi t. Nakamura t. Okumura Y. Yanagisawa 《原子核物理评论》 CAS CSCD 北大核心 2009年第S1期70-74,共5页
The lifetime of the first excited 2+ state in 18C was measured using an upgraded recoil shadow method to determine the electric quadrupole transition. The measured mean lifetime is 18.9±0.9(stat)±4.4(syst)ps... The lifetime of the first excited 2+ state in 18C was measured using an upgraded recoil shadow method to determine the electric quadrupole transition. The measured mean lifetime is 18.9±0.9(stat)±4.4(syst)ps,which corresponds to a B(E2; 2+1→0+gs) value of (4.3± 0.2±1.0) e2fm4,or about 1.5 Weisskopf units. The mean lifetime of the first 2+ state in 16C was remeasured to be about 18 ps,about four times shorter than the value reported previously. This discrepancy was explained by incorporating the γ-ray angular distribution measured in this work into the previous measurement. The observed transition strengths in 16,18C are hindered compared to the empirical transition strengths,indicating that the anomalous hindrance observed in 16C persists in 18C. 展开更多
关键词 NEUTRON-RICH NUCLEI LIFETIME measurement B(E2)
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~1H(^(17)F,α)^(14)O反应截面测量
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作者 贾宝路 胡钧 +17 位作者 何建军 许世伟 H.Yamaguchi D.Kahl 马朋 苏俊 王宏伟 t.nakao Y.Wakabayashi t.teranishi K.I.Hahn J.Y.Moon H.S.Jung t.Hashimoto A.A.Chen D.Irvine C.S.Lee S.Kubono 《原子核物理评论》 CAS CSCD 北大核心 2019年第1期37-42,共6页
^(14)O(α, p)^(17)F是天体X射线暴中重要的突破反应。本工作通过厚靶方法测量其逆反应~1H(^(17)F,α)^(14)O的反应截面来研究这一关键反应。本实验工作是在日本东京大学原子核科学研究中心(CNS)的低能次级束流线(CRIB)上完成的,后续的... ^(14)O(α, p)^(17)F是天体X射线暴中重要的突破反应。本工作通过厚靶方法测量其逆反应~1H(^(17)F,α)^(14)O的反应截面来研究这一关键反应。本实验工作是在日本东京大学原子核科学研究中心(CNS)的低能次级束流线(CRIB)上完成的,后续的扣除本底实验是在兰州放射性束流线(RIBLL1)上完成的。CRIB实验是通过~2H(^(16)O,n)^(17)F转移反应产生^(17)F次级束,经过CRIB分离提纯之后,利用该次级束轰击氢气靶。在氢气靶后布置了三套望远镜探测器系统,用以探测不同实验角度的反冲α粒子,在数据处理的过程中经过动力学重构后得到了~1H(^(17)F,α)^(14)O反应在质心系能区E_(c.m.)=2.7~3.4 MeV的反应截面。实验结果在3 MeV以上的高能区与前人的薄靶实验数据是一致的,在低能区本工作获得了新的实验数据,倾向于支持干涉相消的理论预言结果。 展开更多
关键词 X射线暴 厚靶方法 放射性核束 反应截面 激发函数
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