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Chin. Phys., 2003, Vol. 12(10): 1140-1142    DOI: 10.1088/1009-1963/12/10/015
PHYSICS OF GASES, PLASMAS, AND ELECTRIC DISCHARGES Prev   Next  

The dielectronic recombination process in laser-produced Au plasmas

Jiao Rong-Zhena, Cheng Xin-Lub, Yang Xiang-Dongb
a College of Natural Science, Beijing University of Posts and Telecommunication, Beijing 100876, China; b Institute of Atomic and Molecular Physics, Sichuan University, Chengdu 610065, China
Abstract  The calculations of the rate coefficients for dielectronic recombination (DR) along the NiI isoelectronic sequence in the ground state Au^{51+} through Cu-like 3d^9nln′f (n,n′=4,5,6) inner-shell excited configurations are performed using the spin-orbit-split array (SOSA) model. Resonant and nonresonant radiative stabilizing transitions and decays to autoionizing levels followed by radiative cascades are included. Collisional transitions following electron capture are neglected. The trend of the DR rate coefficients and the ratio of dielectronic satellite lines intensities with the change of the electron temperature are discussed.
Keywords:  dielectronic recombination      autoionization coefficients      spin-orbit-split array  
Received:  01 April 2003      Revised:  31 May 2003      Published:  16 March 2005
PACS:  34.80.Lx (Recombination, attachment, and positronium formation)  
  33.80.Eh (Autoionization, photoionization, and photodetachment)  
  52.38.-r (Laser-plasma interactions)  
  52.25.Jm (Ionization of plasmas)  
  33.15.Bh (General molecular conformation and symmetry; stereochemistry)  
  34.70.+e (Charge transfer)  
  52.20.Hv (Atomic, molecular, ion, and heavy-particle collisions)  
Fund: Project supported by the Doctoral Program Foundation of Institution of Higher Education of China (Grant No JW1902) and the Key Laboratory Foundation of National Defence Science and Technology of China (Grant No SC0303).

Cite this article: 

Jiao Rong-Zhen, Cheng Xin-Lu, Yang Xiang-Dong The dielectronic recombination process in laser-produced Au plasmas 2003 Chin. Phys. 12 1140

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