Solution techniques allow the preparation of La1-yMn1-yO3 at low temperatur
es. However, the as-prepared compounds show thermodynamically induced vacan
cies on both cationic sites. The transport and magnetic properties strongly
depend on both bulk and surface defects. In order to separate these effect
s, we have studied La1-yMn1-yO3 compositions by varying the vacancy content
y and the grain size. The electronic structure of these phases has been in
vestigated by means of the X-ray absorption spectroscopy at the Mn K-edge.
XAS experiments have been carried out on the La1-yMn1-yO3 system as compare
d with the La1-xCaxMnO3 reference series. For both series, the absorption e
dge and the unit cell volume vary linearly with the formal Mn(IV) content,
resulting from a direct correlation between the hole count in Mn 3d states
and the concentration of doping or of cationic vacancies in the perovskite
phase. However, in the La1-yMn1-yO3 system, a deviation from this linearity
occurs for vacancy contents above 30% of Mn(IV). This corresponds to a lim
it of solubility of the cationic vacancy in the bulk. Larger hole contents
(up to 40%) may still be measured, but XANES spectra indicate that the exce
ss holes are then trapped onto Mn sites, probably located at the surface. D
espite this localization, transport measurements indicate a transition from
an insulating to a metallic behavior in the low-temperature ferromagnetic
regime beyond the critical concentration of 30% of Mn(IV). (C) 2000 Elsevie
r Science B.V. All rights reserved.