Study of proton resonances in 18Ne via resonant elastic scattering of 17F+p and its astrophysical implication

被引:5
|
作者
He JianJun [1 ]
Hu Jun [1 ,2 ]
Xu ShiWei [1 ]
Chen ZhiQiang [1 ]
Zhang XueYing [1 ]
Wang JianSong [1 ]
Yu XiangQing [1 ]
Zhang LiYong [1 ,2 ]
Li Long [1 ,2 ]
Yang YanYun [1 ,2 ]
Ma Peng [1 ,2 ]
Zhang XueHeng [1 ]
Hu ZhengGuo [1 ]
Guo ZhongYan [1 ]
Xu Xing [1 ,2 ]
Yuan XiaoHua [1 ]
Lu Wan [1 ,2 ]
Yu YuHong [1 ]
Zang YongDong [1 ,2 ]
Tang ShuWen [1 ,2 ]
Ye RuiPing [1 ,2 ]
Chen JinDa [1 ,2 ]
Jin ShiLun [1 ,2 ]
Du ChengMing [1 ,2 ]
Wang ShiTao [1 ,2 ]
Ma JunBing [1 ,2 ]
Liu LongXiang [1 ,2 ]
Bai Zhen [1 ,2 ]
Lei XiangGuo [1 ]
Sun ZhiYu [1 ]
Zhang YuHu [1 ]
Zhou XiaoHong [1 ]
Xu HuShan [1 ]
Su Jun [3 ]
Li ErTao [3 ]
Wang HongWei [4 ]
Tian WenDong [4 ]
Li XiangQing [5 ,6 ]
机构
[1] Chinese Acad Sci, IMP, Lanzhou 730000, Peoples R China
[2] Chinese Acad Sci, Grad Univ, Beijing 100049, Peoples R China
[3] CIAE, Beijing 102413, Peoples R China
[4] Chinese Acad Sci, Shanghai Inst Appl Phys SINAP, Shanghai 201800, Peoples R China
[5] Peking Univ, Sch Phys, Beijing 100871, Peoples R China
[6] Peking Univ, State Key Lab Nucl Phys & Technol, Beijing 100871, Peoples R China
基金
中国国家自然科学基金;
关键词
resonant reaction; reaction rate; explosive burning; accreting binary systems; SHORT-LIVED NUCLEI; STELLAR REACTIONS; RP-PROCESS;
D O I
10.1007/s11433-011-4407-9
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The proton resonant properties in Ne-18, which determine the reaction rate of the key stellar O-14(alpha,p)F-17 reaction, have been studied by using a technique of proton resonant elastic scattering of F-17+p. A 4.22 MeV/nucleon F-17 radioactive ion (RI) beam was produced via a projectile-fragmentation reaction, and separated by a Radioactive Ion Beam Line in Lanzhou (RIBLL). By bombarding a thick (CH2)(n) target, the energy spectra of the recoiled protons were measured by two Delta E-E silicon telescopes at the center-of-mass scattering angles of theta(c.m.)approximate to 175 degrees +/- 5 degrees, theta(c.m.)approximate to 152 degrees +/- 8 degrees, respectively. Several proton resonances in Ne-18 were observed clearly. A further R-matrix analysis of the experimental data is under way to determine the resonant parameters. The present work reports the preliminary results briefly.
引用
收藏
页码:S32 / S36
页数:5
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