Study on the Reaction Rate of Key Reaction $\bf ^{12}$C($\bm\upalpha$,~$\bm\upgamma$)$\bf ^{16}$O in Astrophysics Base on Shanghai Laser Electron $\bm\upgamma$ Source

  • The MeV photon beam will be produced by Shanghai Laser Electron γ Source which is being proposed. Based on it, a series of nuclear astrophysics experiments can be carried on and the reaction rates of these reactions can be determined accurately. In this paper, the reaction rates of the key reaction 12C(α,γ)16O are calculated according to experiments data and theoretical results, and the mean value and statistical error of these calculated rates are evaluated. The new set of parameters of reaction rate formula are obtained though fitting above results. The reaction rate and its error at T9=0.2 in which 12C(α,γ)16O occurred are extracted, and the screening effects of reaction rate are discussed.
  • 加载中
  • [1] . Burbidge E et al. Rev. Mod. Phys., 1958, C29: 547-6502. Caughlan G. R et al. At. Data Nucl. Data Tables, 1988,40: 283-2983. Buchmann L. Astrophys. J., 1996, 468: L127-L1304. Angulo C et al. Nucl. Phys., 1999, A656: 3-1835. Kunz R et al. Astrophys. J., 2002, 567: 643-6506. Fowler A et al. Ann. Rev. Astron. Astrophys., 1967, 5:525-5707. Braizinha B et al. Nucl. Phys., 2001, A689: 369c-372c8. Brune R et al. Phys. Rev. Lett., 1999, 83: 4025-40289. Brune R et al. Nucl. Phys., 2001, A688: 263c-266c10. Hammer J et al. Nucl. Phys., 2005, A752: 514c-521c11. Hammer J et al. Nucl. Phys., 2005, A758: 363c-366c12. Ouellet J et al. Phys. Rev., 1996, C54: 1982-199813. Kunz R et al. Phys. Rev. Lett., 2001, 86: 3244-324714. Liolios T. Phys. Rev., 2001, C63: 045801:1-7
  • 加载中

Get Citation
XU Yi, XU Wang, MA Yu-Gang, CAI Xiang-Zhou, CHEN Jin-Gen, GU Jia-Hui, GUO Wei, PAN Qiang-Yan, SHEN Wen-Qing, WANG Cheng-Bin, WANG Hong-Wei, XU Jia-Qiang and YUAN Ren-Yong. Study on the Reaction Rate of Key Reaction $\bf ^{12}$C($\bm\upalpha$,~$\bm\upgamma$)$\bf ^{16}$O in Astrophysics Base on Shanghai Laser Electron $\bm\upgamma$ Source[J]. Chinese Physics C, 2006, 30(S2): 252-254.
XU Yi, XU Wang, MA Yu-Gang, CAI Xiang-Zhou, CHEN Jin-Gen, GU Jia-Hui, GUO Wei, PAN Qiang-Yan, SHEN Wen-Qing, WANG Cheng-Bin, WANG Hong-Wei, XU Jia-Qiang and YUAN Ren-Yong. Study on the Reaction Rate of Key Reaction $\bf ^{12}$C($\bm\upalpha$,~$\bm\upgamma$)$\bf ^{16}$O in Astrophysics Base on Shanghai Laser Electron $\bm\upgamma$ Source[J]. Chinese Physics C, 2006, 30(S2): 252-254. shu
Milestone
Received: 2006-10-18
Revised: 1900-01-01
Article Metric

Article Views(3285)
PDF Downloads(603)
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 on the Reaction Rate of Key Reaction $\bf ^{12}$C($\bm\upalpha$,~$\bm\upgamma$)$\bf ^{16}$O in Astrophysics Base on Shanghai Laser Electron $\bm\upgamma$ Source

    Corresponding author: XU Yi,
  • Shanghai Institute of Applied Physics, CAS, Shanghai 201800, China

Abstract: The MeV photon beam will be produced by Shanghai Laser Electron γ Source which is being proposed. Based on it, a series of nuclear astrophysics experiments can be carried on and the reaction rates of these reactions can be determined accurately. In this paper, the reaction rates of the key reaction 12C(α,γ)16O are calculated according to experiments data and theoretical results, and the mean value and statistical error of these calculated rates are evaluated. The new set of parameters of reaction rate formula are obtained though fitting above results. The reaction rate and its error at T9=0.2 in which 12C(α,γ)16O occurred are extracted, and the screening effects of reaction rate are discussed.

    HTML

Reference (1)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return