The absorption and emission spectra of the cubic elpasolite Cs2NaTmCl6
in the near infrared range from 4100 cm(-1) to 8600 cm(-1) have been
reported previously. The absorption transitions involve the H-3(6) gro
und state, the F-3(4) and H-3(5) excited free ion electronic states, w
hereas the emission excitations involve the initial H-3(4), H-3(5) and
F-3(4) terms. For the first time, we report explicit calculation for
the vibronic intensities associated with the emission H-3(4)(Gamma(i))
--> F-3(4)(Gamma(1)). We have chosen this transition so that to illus
trate the effect of the inclusion of several relativistic terms in the
electronic hamiltonian for the system. Throughout the course of the p
resent work, we examine the role played by the various order of approx
imations in the calculated relative vibronic intensity calculation. We
shall show that these results are unexpected and the most important f
eatures of the spectra can be explained reasonably well using a few pa
rameters model for this system. Extensions of the current model are gi
ven in detail in the text.