Data files [16] |
Energy Levels and Lifetimes
|
Transition Rates
|
LS Convergence Trends
|
View or save the original data (.lsj file)
|
Hyperfine Parameters
|
Isotope Shift
|
[16] C. Froese Fischer, Method: MCHF (ab initio), Aug. 2002 |
Important Notice:
The total energies are from spectrum calculations within
a correlation model. Since different models are used for different
spectra, differences of total energies between different
spectra do not yield valid data. |
Disclaimer:
In the Breit-Pauli approximation when there is significant
term mixing, the velocity form of the transition operator has neglected some
relativistic corrections and hence, unlike the length form, is not correct in
that some terms of order \alpha^2 have been omitted. The two values are included
in the .lsj files for information only and have significance when term
mixing is small and the transition is spin-allowed. |