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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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