The microscopic origin of the spin Hamiltonian (SH) parameters for
Ni2+(3d8) ions in a trigonal
type I symmetry (C3v,D3d,D3) crystal field (CF) is studied. In addition to the spin–orbit (SO) interaction,
we consider also the spin–spin (SS) and spin–other-orbit (SOO) interactions.
The relative importance of the four (SO, SS, SOO, and combined SO–SS–SOO)
contributions to the SH parameters is investigated using the CFA/MSH package and
the complete diagonalization method (CDM). The SO mechanism is dominant
for all CF parameter (CFP) ranges studied, except where the contributions
DSO to the zero-field splitting
(ZFS) parameter D
change sign. For the trigonal CFP,
due to the other three mechanisms exceeds
DSO. Although
|DSOO| is quite small,
the combined |DSO−SOO|
is appreciable. The SO-based perturbation theory (PT) works generally well for the
g-factors:
and
, while it fails for D
in the vicinity of vc
and for large
and v>0. The high percentage
discrepancy ratio δD = 2020% for
vc indicates unreliability
of DSO (in PT). Applications
to Ni2+ ions at trigonal
symmetry sites in LiNbO3, α-LiIO3, and
Al2O3, are
provided. The theoretical SH parameters are in good agreement with the experimental data. The low symmetry
(C3) effects induced
by the angle φ
are tentatively studied, but appear to be quite small.