Physics
Scientific paper
Oct 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...80..321g&link_type=abstract
Solar Physics, vol. 80, Oct. 1982, p. 321-331.
Physics
Electron Transitions, Far Ultraviolet Radiation, Ions, Silicon, Solar Spectra, Energy Levels, Transition Probabilities, Wave Equations
Scientific paper
Extensive CI calculations are presented of energy levels, wavelengths, oscillator strengths, line strengths, transitions probabilities, lifetimes, and branching ratios for transitions between the 2lnl-prime (n = 2, 3; l-prime less than or equal to l) states for Si XI. The calculations show that including the nonfine structure relativistic corrections in the Hamiltonian can change the transition probabilities drastically in particular for transitions between the 2l3l-prime (l-prime greater than or equal to l) states. This is a consequence of the very small energy separations between the 2l3l-prime states; a small change in the energy level of each state in the transition can result in quite a large change in the transition energy. For this reason, for transitions between the 2l3l-prime states a set of radial functions which gives a representation of the energy levels to better than 100/cm (0.005 AU) is sought.
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