A. Barshalom et al., A NEW APPROACH TO INCLUDING DOUBLY-EXCITED LEVELS IN THE COLLISIONAL RADIATIVE MODEL, Journal of quantitative spectroscopy & radiative transfer, 54(1-2), 1995, pp. 35-42
A severe limitation on the application of the collisional radiative mo
del is the need to include an exceedingly high number of relevant doub
ly excited and inner shell excited levels. The direct inclusion of all
these levels is simply impractical. In a previous theory we have incl
uded doubly excited configurations as effective levels assuming statis
tical distribution of the populations within these configurations. In
the present work we develop a new approach which minimizes even furthe
r the amount of effective levels, and leading, paradoxically, to weake
r statistical assumptions. It is shown that the outer Rydberg orbital
of the doubly excited configuration resembles a continuum electron, an
d is only weakly coupled to the internal core. This fact allows the ap
plication of the Factorization Interpolation method, reducing the cros
s-sections of the various collisional radiative processes to one elect
ron multipole transitions between core states only. The radial integra
ls include the outer orbital and the summation over all the involved c
ontinuum orbitals. It is also shown that the assumption of a statistic
al distribution can be extended to groups of states with neighboring R
ydberg orbitals. Each group then contains effective levels characteriz
ed by the core state designation and therefore has the same dimension
as the original core. A convergence procedure is described that involv
es reducing the number of Rydberg orbitals within a group. It is shown
that a small number of groups is sufficient for convergence, reducing
drastically the number of effective levels in the model. The simple e
xample of the Ne-like ion is discussed. The many thousands of relevant
doubly excited states are reduced in this case to the 37 levels of th
e core multiplied by the small number of groups. This reduction is eve
n more striking in more complex ions and in cases where the core is fa
r from closed shell configurations.