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• W2078100827 abstract "Energy levels, radiative transition probabilities, and autoionization rates for 1s22s22p53l′nl,1s22s2p63l′nl(n=3–7,l⩽n-1) and 1s22s22p54l′nl,1s22s2p64l′nl(n=4–6,l⩽n-1) states in Na-like tungsten (W63+) are calculated. Cowan’s relativistic Hartree–Fock method, the relativistic multiconfiguration method implemented in the Hebrew University Lawrence Livermore Atomic Code, and the relativistic many-body perturbation theory method, are used. Autoionizing levels above the threshold 1s22s22p6 are considered. It is found that configuration mixing [3sns+3pnp+3dnd],[3snp+3pns+3pnd+3dnp] plays an important role for all atomic characteristics. Also strong mixing between states with 2s and 2p holes (1s22s22p53l1nl2+1s22s2p63l3nl4) occurs. Branching ratios relative to the first threshold and intensity factors are calculated for satellite lines, and dielectronic recombination (DR) rate coefficients are determined for the excited 1s22s22p6nl(n=3–7,l⩽n-1) states. It is shown that the contribution of the highly excited states is very important for calculation of total DR rates. Contributions from the autoionizing states 1s22s22p53l′nl,1s22s2p63l′nl(n⩾8) and 1s22s22p54l′nl,1s22s2p64l′nl(n⩾7) to the DR rate coefficients are estimated by extrapolation of all atomic parameters. The orbital angular momentum (l) distribution of the rate coefficients shows a peak at l=2. The total DR rate coefficient is derived as a function of electron temperature. The dielectronic satellite spectra of W63+ are important for L-shell diagnostics of very high-temperature laboratory plasmas such as future ITER fusion plasmas." @default.
• W2078100827 created "2016-06-24" @default.
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• W2078100827 date "2009-11-01" @default.
• W2078100827 modified "2023-09-23" @default.
• W2078100827 title "Excitation energies, radiative and autoionization rates, dielectronic satellite lines, and dielectronic recombination rates for excited states of Na-like W from Ne-like W" @default.
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• W2078100827 doi "https://doi.org/10.1016/j.adt.2009.04.001" @default.
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