A site preference of niobium atom in Rb(2-x)La(2)Ti(3-x)Nh(x)O(10) (0.0 les
s than or equal to x less than or equal to 1.0) and RbLa2-xCaxTi2-xNb1+xO10
(0.0 less than or equal to x less than or equal to 2.0), which are the sol
id-solutions between Rb2La2Ti3O10 and RbCa2Nb3O10, has been investigated by
Raman spectroscopy. The Raman spectra of Rb2-xLa2Ti3-xNbxO10 (0.0 less tha
n or equal to x less than or equal to 1.0) gave an evidence that niobium at
oms substituted for titanium atoms preferably occupy the highly distorted o
uter octahedral sites rather than the central ones in triple-octahedral per
ovskite layers. In contrast, the Raman spectra of RbLa2-xCaxTi2-xNb1+xO10 (
0.0 less than or equal to x less than or equal to 2.0) showed no clear info
rmation for the cationic arrangement in perovskite slabs. This difference i
ndicated that a site preference of niobium atoms is observed only when the
linear Rb-O-Ti linkage can be replaced by much stronger terminal Nb-O bond
with double bond character. From comparison with the Raman spectroscopic be
havior of CsLa(2-x)A'xTi2-xNb1+xO10 (A' = Ca and Ba; 0.0 less than or equal
to x less than or equal to 2.0), it is also proposed that a local differen
ce in arrangement of interlayer atoms causes a significantly different soli
d acidity and photocatalytic activity of the layered perovskite oxides, des
pite their crystallographically similar structures.