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| 1 | 2-14 Investigation of the Thermonuclear 18Ne(α, p)21Na Reaction Rate via Resonant Elastic Scattering of 21Na + p显示文摘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 reaction rate of 18Ne(,p)21Na reaction, which mightbe a key breakout reaction from the hot CNO cycle to rp-process in X-ray burst and nova. Yet its reaction rate ispoorly known.Explosive hydrogen burning is thought to be the main source of energy generation and a source of nucleosynthesisin X-ray burst and nova[1;2]. For example, XRBs are characterized by a sudden increase of X-ray emission withinonly a few seconds to a total energy output of about 1040 ergs, which is observed to repeat with some regularity.The recurrence time for single bursts can range from hours to days at the typical temperature of 0.4~2 GK. Thebursts have been interpreted as being generated by thermonuclear runaway on the surface of a neutron star thataccretes H- and He-rich material from a less evolved companion star in a close binary system. As shown in Fig. 1,under its typical temperature, the hydrogen burning in X-ray burst occurs from the hot CNO cycle: | Zhang Liyong He Jianjun Xu Shiwei H.Yamaguchi S. Kubono Y.Wakabayashi Chen Size Hu Jun Ma Peng Y. Togano T. Hashimoto D. Kahl T. Teranishi Chen Ruofu Wang Hongwei Tian Wendong Guo Bing S. Hayakawa N. Iwasa T. Yamada T. Komatsubara | 2014 | IMP & HIRFL Annual Report2014，，1： | 2 |
| 2 | New low-energy RIB separator CRIB for nuclear astrophysics显示文摘 | S. Kubono Y. Yanagisawa T. Teranishi S. Kato Y. Kishida S. Michimasa Y. Ohshiro S. Shimoura K. Ue S. Watanabe N. Yamazaki | 2002 | The European Physical Journal A (-)2002，，1： | 1 |
| 3 | Measurement of the 24Mg(p, t)22Mg reaction for the states near the 21Na + p threshold显示文摘 | S. Michimasa S. Kubono S.H. Park T. Teranishi Y. Yanagisawa N. Imai Zs. Fül?p X. Liu T. Minemura C.C. Yun J.M. D’Auria K.P. Jackson | 2002 | The European Physical Journal A2002，，3： | 1 |
| 4 | Fabrication of REBa 2 Cu 3 O 7? y film by advanced TFA-MOD process显示文摘 | A. Kaneko H. Fuji R. Teranishi Y. Tokunaga J.S. Matsuda S. Asada K. Murata T. Honjo T. Izumi Y. Shiohara T. Goto A. Yoshinaka A. Yajima | 2004 | Physica C: Superconductivity and its applications2004，，： | 1 |
| 5 | Nuclear astrophysics at the east drip line显示文摘 | S. Kubono T. Teranishi M. Notani H. Yamaguchi A. Saito J. J. He Y. Wakabayashi H. Fujikawa G. Amadio H. Baba T. Fukuchi S. Shimoura S. Michimasa S. Nishimura M. Nishimura Y. Gono A. Odahara S. Kato J. Y. Moon J. H. Lee Y. K. Kwon C. S. Lee K. I. Hahn Zs. | 2006 | The European Physical Journal A2006，，1： | 1 |
| 6 | Experimental Study 18Ne(a,p)21Na of Key Astrophysical Reaction显示文摘 | Zhang Liyong He Jianjun Xu Shiwei H. Yamaguchi S. Kubono Y. Wakabayashi Chen Size Ma Peng Y. Togano T. Hashimoto D. Kahl T. Teranishi Chen Ruofu Wang Hongwei Tian Wendong Guo Bing S. Hayakawa N. Iwasa T. Yamada T. Komatsubara | 2011 | IMP & HIRFL Annual Report2011，，1： | 0 |
| 7 | 2-13 Stellar Reaction Rate of the 14O(α, p)17F显示文摘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. | Hu Jun He Jianjun 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 | 2014 | IMP & HIRFL Annual Report2014，，1： | 0 |
| 8 | 2- 8 Confirmation of Astrophysically Important 6.15 MeV, 1- State in 18Ne via Resonant Scattering of 17F+p显示文摘 | Hu Jun He Jianjun 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 | 2013 | IMP & HIRFL Annual Report2013，，1： | 0 |
| 9 | 2 - 17 Experimental Study of Key Astrophysical 18Ne(α,p) 2lNa Reaction显示文摘 | Zhang Liyong He Jianjun Xu Shiwei H. Yamaguehi S. Kubono Y. Wakabayashi Chen Size Hu Jun Ma Peng Y. Togano T. Hashimoto D. Kahl T. Teranishi Chen Ruofu Wang Hongwei TianWendong Guo Bing S. Hayakawa N. Iwasa T. Yamada T. Komatsubara | 2012 | IMP & HIRFL Annual Report2012，，1： | 0 |
| 10 | 2 - 20 Investigation for Resonant Scattering of 17F+p显示文摘 | Hu Jun He Jianjun Xu Shiwei H. Yamaguchi Ma Peng K. David Su Jun Wang Hongwei T. Nakao Y. Wakabayashi J. Y. Moon T. Teranishi H. S. Jung T. Hashimoto A. Chen D. Irvine S. Kubono | 2012 | IMP & HIRFL Annual Report2012，，1： | 0 |
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