Lj. Burcham et Ie. Wachs, VIBRATIONAL ANALYSIS OF THE 2 NONEQUIVALENT, TETRAHEDRAL TUNGSTATE (WO4) UNITS IN CE-2(WO4)(3) AND LA-2(WO4)(3), SPECT ACT A, 54(10), 1998, pp. 1355-1368
Citations number
47
Categorie Soggetti
Spectroscopy
Journal title
SPECTROCHIMICA ACTA PART A-MOLECULAR AND BIOMOLECULAR SPECTROSCOPY
The infrared and Raman spectra of Ce-2(WO4)(3) and La-2(WO4)(3), which
are complicated by the superposition of bands from two non-equivalent
WO4 units, have been successfully assigned above 300 cm(-1) according
to T-d point group symmetry. Individual assignment of the two types o
f tungstate units, (WO4)-O-I (C-2 site symmetry) and (WO4)-O-II (C-1 s
ite symmetry), relies on comparison with the spectra of tetrahedral re
ference tungstates of Na2WO4, CaWO4, and MgWO4, and on the differences
between (WO4)-O-I and (WO4)-O-II known from the crystal structure. No
rmal coordinate analysis indicates that the force constants for (WO4)-
O-I and (WO4)-O-II roughly correlate with the amount of deviation from
ideal T-d point symmetry, (WO4)-O-I being similar to CaWO4 (both mild
ly distorted tetrahedrons), while (WO4)-O-II is closer to MgWO4 (both
highly distorted tetrahedrons). Non-ideality is also indicated by the
calculated potential energy distribution (PED), which shows a substant
ial degree of vibrational interaction between bonds-especially in the
less symmetric (WO4)-O-II unit. Frequency differences between IR and R
aman bands that originate from the same T-d point group modes are attr
ibuted mainly to factor group splitting (i.e. Raman active gerade and
IR active ungerade factor group modes). However, the LO-TO polarizatio
n mixing and surface modes that generate the observed vibrational freq
uencies in powders may also contribute to these frequency differences,
since the magnitude of these effects may not be the same in Raman as
in IR. Finally, it is likely that other rare earth tungstates of stoic
hiometry Ln(2)(WO4)(3), where Ln = La similar to Dy, have similar vibr
ational spectra due to their similar structures. (C) 1998 Elsevier Sci
ence B.V. All rights reserved.