Optical and magneto-optical data from the perovskite itinerant ferromagnet
SrRuO3 are presented and compared to fully relativistic, local spin-density
approximation band-structure calculations. We find that the basic features
of the optical data are well described by the ferromagnetic band calculati
on. To test recent predictions that the ferromagnetic transition in SrRuO3
is driven by long-wavelength longitudinal spin fluctuations, we track the t
emperature dependence of the O(2p) --> Ru(4d) interband transition which we
observe in the magneto-optic conductivity. The absence of significant chan
ges in the energy of this transition suggests that the ferromagnetic order
is destroyed largely through transverse, not longitudinal, fluctuations of
the ferromagnetic moment. We discuss the implications of these observations
for the electronic structure of the ruthenium perovskites. [S0163-1829(99)
51134-X].