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 W proceeds via electron capture into the intermediate autoionizing states of the Tm-like ion W followed by the radiative decay to singly-excited bound states. In particular, energy levels, radiative transition probabilities, and autoionization rates for [Cd], [Cd], [Cd], and [Cd] (, , ) states in Tm-like tungsten (W) 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] () and nonautoionizing doubly-excited [Cd], [Cd], [Cd], [Cd], and [Cd] states. Also, contributions from the autoionizing doubly-excited [Cd], [Cd], [Cd], and [Cd] states (with 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 W ion properties useful for a variety of applications, including for fusion applications.
- Received 21 January 2012
DOI:https://doi.org/10.1103/PhysRevA.85.032507
©2012 American Physical Society