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Chin. Phys. B, 2009, Vol. 18(9): 4049-    DOI: 10.1088/1674-1056/18/9/072
GEOPHYSICS, ASTRONOMY, AND ASTROPHYSICS Prev  

Analytical solutions for the slow neutron capture process of heavy element nucleosynthesis

Wu Kai-Su(吴开谡)
Beijing University of Chemical Technology, Beijing 100029, China
Abstract  In this paper, the network equation for the slow neutron capture process (s-process) of heavy element nucleosynthesis is investigated. Dividing the s-process network reaction chains into two standard forms and using the technique of matrix decomposition, a group of analytical solutions for the network equation are obtained. With the analytical solutions, a calculation for heavy element abundance of the solar system is carried out and the results are in good agreement with the astrophysical measurements.
Keywords:  s-process      network equation      analytical solution      element abundance  
Received:  16 January 2009      Revised:  24 February 2009      Accepted manuscript online: 
PACS:  25.55.-e (3H-, 3He-, and 4He-induced reactions)  
  25.10.+s (Nuclear reactions involving few-nucleon systems)  
  26.35.+c (Big Bang nucleosynthesis)  
  27.20.+n (6 ≤ A ≤ 19)  
  27.30.+t (20 ≤ A ≤ 38)  
  97.10.Cv (Stellar structure, interiors, evolution, nucleosynthesis, ages)  
Fund: Project supported by the National Natural Science Foundation of China (Grant No 10447141 ) and the Youth Foundation of Beijing University of Chemical Technology, China (Grant No QN0622).

Cite this article: 

Wu Kai-Su(吴开谡) Analytical solutions for the slow neutron capture process of heavy element nucleosynthesis 2009 Chin. Phys. B 18 4049

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