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[会议论文] 作者：G.L.Zhang,X.X.Xu,F.Yang,S.Kubono,H.Yamaguchi,S.Hayakawa,D.N.Binh,
来源：第十四届全国核物理大会暨第十届会员代表大会 年份：2010
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Study of Proton Resonances in ~(22)Mg by Resonant Elastic Scattering of ~(21)Na+p and Its Astrophysi
[期刊论文] 作者：S.Kubono,T.Teranishi,M.Notani,H.Baba,S.Nishimura,J.Y.Moon,M.Nishimura,S.Michimasa,H.Iwasaki,Y.Yanagisawa,
来源：原子核物理评论 年份：2004
Proton resonant states in 22Mg have been investigated by the resonant elastic scattering of 21Na+p. The 21Na beam with a mean energy of 4.00 MeV/u was separated...
Study of Proton Resonances in ~(22)Mg by Resonant Elastic Scattering of ~(21)Na+p and Its Astrophysi
[期刊论文] 作者：HEJian-jun，S.Kubono，T.Teranishi，M.Notani，H.Baba，S.Nishimura，J.Y.Moon，M.Nishimura，S.Michimasa，H.Iwasaki,
来源：原子核物理评论 年份：2009
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STUDY OF ASTROPHYSICALLY IMPORTANT STATES IN 26Si WITH THE p(27Si,26Si*)d REACTION AND THE p(25Al,p)
[会议论文] 作者：H.Yamaguchi,N.Iwasa,S.Hayakawa,A.A.Chen,S.Michimasa,T.Teranishi,Y.Kurihawa,Y.Wakabayashi,H.Schatz,S.Kubono,
来源：The 10th International Conference on Nucleus-Nucleus Collisi 年份：2009
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[期刊论文] 作者：Jun,Wang Hongwei,T.Nakao,Y.Wakabayashi,J.Y.Moon,T.Teranishi,H.S.Jung,T.Hashimoto,A.Chen,D.Irvine,S.Kubono,
来源：IMP & HIRFL Annual Report 年份：2012
X-ray bursts[1]are probably an important source for the production of proton-rich nuclei via the high temperature rp-process[2],and the 14 O(α,p)17F reaction i...
BARE NUCLEUS S(E)FACTOR FOR THE BORON BURNING 11B(p,α)8Be AND 10B(p,α)7Be REACTIONS THROUGH THE INDI
[会议论文] 作者：L.Lamia,M.Gulino,G.Kiss,V.Kroha,S.Kubono,M.La Cognata,ChengBo Li,A.Mukhamedzhanov,R.G.Pizzone,QunGang,
来源：The 10th International Conference on Nucleus-Nucleus Collisi 年份：2009
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Measurement of ~2H(~(12)N, ~(13)O)n Angular Distribution and Determination of Astrophysical ~(12)N(p
[期刊论文] 作者：Yin-lu,BAI Xi-xiang,CHEN Yong-shou,LIU Wei-ping,H.Yamaguchi,D.N.Binh,T.Hashimoto,S.Hayakawa,D.Kahl,S.Kubono,
来源：Annual Report of China Institute of Atomic Energy 年份：2012
The evolution of massive stars with very low-metallicities depends critically on the amount of CNO nuclides which they produce. The 12N(p, γ)13O reaction is an...
BARE NUCLEUS S(E)FACTOR FOR THE BORON BURNING 11B(p,α)8Be AND 10B(p,α)7Be REACTIONS THROUGH THE INDI
[会议论文] 作者：L.Lamia[1]M.Gulino[1]G.Kiss[2]V.Kroha[3]S.Kubono[4]M.LaCognata[1]ChengBoLi[5]A.Mukhamedzhanov[6]R.G.Pizzone,
来源：The 10th International Conference on Nucleus-Nucleus Collisi 年份：2009
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[期刊论文] 作者：张立勇,He Jianjun,Xu Shiwei,H.Yamaguchi,S.Kubono,Y.Wakabayashi,Chen Size,Hu Jun,Ma Peng,Y.Togano,T.Hashimoto,
来源：IMP & HIRFL Annual Report 年份：2012
A nuclear astrophysics experiment was performed at CRIB(CNS low-energy Radioactive-Ion Beam separator)on Mar.2011.The goal of this experiment is to study the re...
[期刊论文] 作者：郭冰,苏俊,李志宏,王友宝,颜胜权,李云居,舒能川,韩银录,白希祥,陈永寿,柳卫平,H.Yamaguchi,D.N.Binh,T.Hashimoto,S.Hayakwa,D.Kahl,S.Kubono,,
来源：中国原子能科学研究院年报 年份：2012
大质量贫金属恒星的演化与其产生的CNO核数目紧密相关,快速αp俘获过程是产生CNO种子核的重要过程之一,它可改变大质量恒星的命运。12N(p,γ)13O反应是快速αp过程中的一个重...
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