Study of Astrophysical Nuclear Reaction on Beijing Secondary Beam Line GIRAFFE

Get Citation
LIU Wei-Ping, BAI Xi-Xiang, WANG You-Bao, LI Zhi-Hong, LIAN Gang, LI Zhi-Chang, GUO Gang, JIANG Li-Yang, LU Shao-Jun, FU Chang-Bo and CHEN Yong-Shou. Study of Astrophysical Nuclear Reaction on Beijing Secondary Beam Line GIRAFFE[J]. Chinese Physics C, 2000, 24(S1): 6-8.
LIU Wei-Ping, BAI Xi-Xiang, WANG You-Bao, LI Zhi-Hong, LIAN Gang, LI Zhi-Chang, GUO Gang, JIANG Li-Yang, LU Shao-Jun, FU Chang-Bo and CHEN Yong-Shou. Study of Astrophysical Nuclear Reaction on Beijing Secondary Beam Line GIRAFFE[J]. Chinese Physics C, 2000, 24(S1): 6-8. shu
Milestone
Received: 1900-01-01
Revised: 1900-01-01
Article Metric

Article Views(2903)
PDF Downloads(561)
Cited by(0)
Policy on re-use
To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.
通讯作者: 陈斌, bchen63@163.com
  • 1. 

    沈阳化工大学材料科学与工程学院 沈阳 110142

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Email This Article

Title:
Email:

Study of Astrophysical Nuclear Reaction on Beijing Secondary Beam Line GIRAFFE

    Corresponding author: LIU Wei-Ping,
  • China Institute of Atomic Energy,Beijing 102413,China

Abstract: The 11C(p,γ)12N reaction is one of the key processes in hot pp chains.We have carried out a measurement of 11C(d,n)12N reaction.The 11C beam was produced with the secondary beam facility GIRAFFE.The angular distribution was measured and used to deduce ANC through DWBA analysis.We are performinga microscopic study to get the astrophysical S-factor of 11C(p,γ)12N reaction from ANC square constant of 3.5±1.5.This result implies that the direct contribution to (p,γ) reaction is not negligible.

    HTML

Reference (1)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return