Sc V
 
Data files [20]
  • Hyperfine Parameters
  • Isotope Shift
 
[20] A. Irimia and C. Froese Fischer, Method: MCHF (ab initio), 2003
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.