W0281
The Use of Crenel Functions in the Description of Aperiodic
Perovskite-like
A1+xBX3
Oxides and Sulfides. Olivier Gourdona Michel
Evain,b and Vaclav
Petricekc,
aDept. of Chemistry, Iowa State Univ., Ames, Iowa
50011-3111, bLaboratoire de Chimie des Solides, I.M.N., UMR C6502
CNRS - Univ. de Nantes, 2 rue de la Houssinière, BP 32229, 44322 Nantes
Cedex 3, France, cInstitute of Physics, Academy of Sciences of the
Czech Republic, Na Slovance 2, 182 21 Praha 8, Czech Republic.
In the A1+xBX3 (A = Sr, Ba,
etc., B = Co, Ni, Ti etc. and X= O or S) hexagonal perovskite-like family
can be described as intergrowth compounds with two chain subsystems: a
[BX3] chain subsystem with various successions of face sharing
octahedra and trigonal prisms (for the oxides) and an [A] chain
subsystem.
Through single crystal X-ray structure determinations using
superspace group formalism, crenel functions, and occasionally non-harmonic
development of the Debye-Waller factor, we show that all
AxMX3 hexagonal perovskite oxides and
sulfides can be uniquely described. Indeed, all phases have R-3m(00_)0s as a
common superspace group. Moreover, the use of crenel functions is demonstrated
to be a key factor for the resolution of these aperiodic structures. The models
developed using those crenel functions revealed interesting unforeseen features
for NiII and CoII in the oxides that is their instability
in the center of the trigonal prism, and showed the particularity of the sulfur
structures, bringing to light new original [MS6] units as
called (PO) units for prism-octahedron, that is, units exactly intermediate
between trigonal prisms and octahedra. In addition, the displacive modulations,
almost exclusively along the chain axis in the oxides, have large out of the
chain axis components in the sulfides. Both differences impose different crenel
arrangements and lead to different potential twinnings.