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Chinese Physics, 2007, Vol. 16(11): 3300-3304    DOI: 10.1088/1009-1963/16/11/026
NUCLEAR PHYSICS Prev   Next  

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)
Institute of Theoretical Physics, China West Normal University, Nanchong 637002, China
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.
Keywords:  electron screening      nucleosynthesis      O–Ne nova      x-ray bursts      supernovae  
Accepted manuscript online: 
PACS:  25.40.Ny (Resonance reactions)  
  25.40.Lw (Radiative capture)  
  26.30.-k (Nucleosynthesis in novae, supernovae, and other explosive environments)  
  27.30.+t (20 ≤ A ≤ 38)  
Fund: 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

Cite this article: 

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) Resonance reaction rate of 21Na(p, $\gamma$)22Mg 2007 Chinese Physics 16 3300

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