C. Mendoza et al., Atomic data from the IRON Project - XXXIII. Radiative rates for the intercombination transitions in the carbon isoelectronic sequence, ASTR AST SS, 135(1), 1999, pp. 159-169
Radiative decay rates are computed with the atomic structure code SUPERSTRU
CTURE for the 2s2p(3) S-5(2)o - 2s(2)2p(2) P-3(1), P-3(2) and D-1(2) interc
ombination transitions of the carbon isoelectronic sequence (6 less than or
equal to Z less than or equal to 28). Contributions from configuration int
eraction and relativistic corrections are carefully studied, in particular
the spin-spin interaction that is shown to be of considerable importance fo
r low Z. By extensive comparisons with other theoretical datasets and measu
rements of the S-5(2)o radiative lifetime and the B = A(S-5(2)o - P-3(2))/A
(S-5(2)o - P-3(1)) branching ratio, rye are able to assign accuracy ratings
to the present transition probabilities. The transitions to the ground ter
m are believed to be accurate to better than 10% whereas the smaller A-valu
es belonging to transitions to the D-1(2) are not expected to be accurate t
o more than 20%.