Dielectronic recombination of Er-like tungsten

U. I. Safronova and A. S. Safronova
Phys. Rev. A 85, 032507 – Published 5 March 2012

Abstract

Theoretical studies of dielectronic recombination, a very important process for both atomic and plasma physics, are carried out for low-ionized Er-like W. The dielectronic recombination (DR) of the Er-like ion W6+ proceeds via electron capture into the intermediate autoionizing states of the Tm-like ion W5+ followed by the radiative decay to singly-excited bound states. In particular, energy levels, radiative transition probabilities, and autoionization rates for [Cd]4f145p55lnl, [Cd]4f145p56lnl, [Cd]4f135p65lnl, and [Cd]4f135p66lnl (l=d,f,g, l=s,p,d,f,g, n=57) states in Tm-like tungsten (W5+) are calculated using the relativistic many-body perturbation theory and relativistic all-order single-double method as well as the Hartree-Fock-relativistic method (cowan code). Branching ratios relative to the first threshold and intensity factors are calculated for satellite lines. DR rate coefficients are determined for the singly-excited [Cd]4f145p6nl (n=57) and nonautoionizing doubly-excited [Cd]4f145p55d2, [Cd]4f135p65d2, [Cd]4f135p66s2, [Cd]4f135p65d6s, and [Cd]4f135p65d6p states. Also, contributions from the autoionizing doubly-excited [Cd]4f145p55lnl, [Cd]4f145p56lnl, [Cd]4f135p65lnl, and [Cd]4f135p66lnl states (with n up to 100), which are very important for calculating total DR rates, are estimated. Synthetic dielectronic satellite spectra from Tm-like W are simulated in a broad spectral range from 140 to 1200 Å. These relativistic calculations provide recommended values critically evaluated for their accuracy for a number of W5+ ion properties useful for a variety of applications, including for fusion applications.

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  • Received 21 January 2012

DOI:https://doi.org/10.1103/PhysRevA.85.032507

©2012 American Physical Society

Authors & Affiliations

U. I. Safronova and A. S. Safronova

  • Physics Department, University of Nevada, Reno, Nevada 89557, USA

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Vol. 85, Iss. 3 — March 2012

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