中国物理B ›› 2007, Vol. 16 ›› Issue (11): 3300-3304.doi: 10.1088/1009-1963/16/11/026

• • 上一篇    下一篇

Resonance reaction rate of 21Na(p, γ)22Mg

刘门全1, 刘晶晶1, 罗志全1, 刘宏林2   

  1. (1); (2)Institute of Theoretical Physics, China West Normal University, Nanchong 637002, China
  • 出版日期:2007-11-20 发布日期:2007-11-20
  • 基金资助:
    Project supported by the National Natural Science Foundation of China (Grant No~10347008), the Scientific Research and Fund of Sichuan Provincial Education Department of China (Grant No~2006A079) and the Science and Technological Foundation of China West

Resonance reaction rate of 21Na(p, $\gamma$)22Mg

Liu Hong-Lin(刘宏林), Liu Men-Quan(刘门全), Liu Jing-Jing(刘晶晶), and Luo Zhi-Quan(罗志全)†   

  1. Institute of Theoretical Physics, China West Normal University, Nanchong 637002, China
  • Online:2007-11-20 Published:2007-11-20
  • Supported by:
    Project supported by the National Natural Science Foundation of China (Grant No~10347008), the Scientific Research and Fund of Sichuan Provincial Education Department of China (Grant No~2006A079) and the Science and Technological Foundation of China West

PDF (PC)

545

赞

Abstract: By using the new Coulomb screening model and most recent experimental results, this paper calculates the resonance reaction rates of 21Na(p, $\gamma$)22Mg. The derived result shows that the effect of electron screening on resonant reaction is prominent in astrophysical interesting temperature range. In conjunction with the experimental results, the recommended rates of 21Na(p, $\gamma$)22Mg would increase at least 10%, which undoubtedly affect the nucleosynthesis of some heavier nuclei in a variety of astrophysical sites.

Key words: electron screening, nucleosynthesis, O–Ne nova, x-ray bursts, supernovae

中图分类号:  (Resonance reactions)

  • 25.40.Ny
25.40.Lw (Radiative capture) 26.30.-k (Nucleosynthesis in novae, supernovae, and other explosive environments) 27.30.+t (20 ≤ A ≤ 38)