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物理学   3篇
  2011年   3篇
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L&#;  LinHui  Ye  YanLin  Jiang  DongXing  Hua  Hui  Zheng  Tao  Li  ZhiHuan  Ge  YuCheng  Li  XiangQing  Lou  JianLing  Cao  ZhongXin  Song  YuShou  Xiao  Jun  Li  QiTe  Qiao  Rui  You  HaiBo  Chen  RuiJiu  Xu  HuShan  Wang  JianSong  Guo  ZhongYan  Zhang  XueYing  Li  Chen  Hu  ZhengGuo  Chen  RuoFu  Wang  Meng  Xu  ZhiGuo  Yue  Ke  Tang  Bin  Zang  YongDong  Zhang  XueHeng  Yao  XiangWu  Chen  JinDa  Bai  Zhen 《中国科学:物理学 力学 天文学(英文版)》2011,54(1):136-140

Knockout reaction experiment was carried out by using the 6He beams at 61.2 MeV/u impinging on a CH2 target. The α core fragments at forward angles were detected in coincidence with the recoiled protons at larger angles. From this exclusive measurement the valence nucleon knockout mechanism and the core knockout mechanism can be distinguished by the relation between the polar angles of the core fragments and the recoiled protons, respectively. It is demonstrated that the core knockout mechanism may result in some strong contamination to the real invariant mass spectrum.

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2.
The proton resonant properties in 18Ne, which determine the reaction rate of the key stellar 14O(α,p)17F reaction, have been studied by using a technique of proton resonant elastic scattering of 17F+p. A 4.22 MeV/nucleon 17F 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 ΔE-E silicon telescopes at the center-of-...  相似文献   
3.
He  JianJun  Hu  Jun  Xu  ShiWei  Chen  ZhiQiang  Zhang  XueYing  Wang  JianSong  Yu  XiangQing  Zhang  LiYong  Li  Long  Yang  YanYun  Ma  Peng  Zhang  XueHeng  Hu  ZhengGuo  Guo  ZhongYan  Xu  Xing  Yuan  XiaoHua  Lu  Wan  Yu  YuHong  Zang  YongDong  Tang  ShuWen  Ye  RuiPing  Chen  JinDa  Jin  ShiLun  Du  ChengMing  Wang  ShiTao  Ma  JunBing  Liu  LongXiang  Bai  Zhen  Lei  XiangGuo  Sun  ZhiYu  Zhang  YuHu  Zhou  XiaoHong  Xu  HuShan  Su  Jun  Li  ErTao  Wang  HongWei  Tian  WenDong  Li  XiangQing 《中国科学:物理学 力学 天文学(英文版)》2011,54(1):32-36
The proton resonant properties in 18Ne, which determine the reaction rate of the key stellar 14O(α,p)17F reaction, have been studied by using a technique of proton resonant elastic scattering of 17F+p. A 4.22 MeV/nucleon 17F 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 ΔE-E silicon telescopes at the center-of-mass scattering angles of θ c.m.≈175°±5°, θ c.m.≈152°±8°, respectively. Several proton resonances in 18Ne 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.  相似文献   
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