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This study delves into the isoelectronic systematization of line strength factors, deduced and parametrized from measured data. Dirac Equation calculations for singlet-triplet mixing levels provide valuable insights, which are further explored through MCDHF calculations and resonance transitions analysis. Challenges and exceptions within the data availability are discussed, emphasizing the need for improved experimental methods.
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ISOELECTRONIC SYSTEMATIZATION Line Strength Factor: Sifmi mf i | r/ao | f 2 Deduced from measured data: Sif = [ if (Å) / 1265.38]3giBif/ i (ns) Parametrized: Z 2 SifSH + b/(Z-C) ; SH = 3n2 (n2-1) gi / 4
Singlet-Triplet Mixing nsnp levels RES INT
sp 1 and 2 free parameters: Wolfe, PR 41, 443 (1932) (spin-other-orbit) King & VanVleck, PR 56, 464 (1939) (spin dep. radial wave fctn.)
Alkaline-earthlike sequences
Radioactive 5670
All applications to here are n = 0 resonance transitions: Alkali-metallike ns – np Alkaline-earthlike ns2 – nsnp Are these data-based semiempirical methods also applicable to other types of transitions? Yes, but there are no data! Lifetime data exist, but branching fraction data are essentially non-existent for multiply charged ions Exceptions:
Differential Lifetime Measurements
Determination of branching fractions: Requires intensity calibration of detection apparatus as a function of wavelength Standard lamps: continuum radiation fixed in laboratory beam light Doppler shifted Line standards available in Visible, but not UV Need in-beam ions with known intensity ratios
S II : (Å) 907, 911, 913 1053, 1056 1167, 1173