Abstract
In the
Ln1-xAxMnO3
pseudoperovskites in which Ln is a lanthanide and A an alkaline-earth atom, an
intrinsic colossal magnetoresistance (CMR) occurs in an O-orthorhombic phase
near an O′-orthorhombic/O-orthorhombic phase boundary. For a fixed
ratio Mn(IV)/Mn = 0·3, the transition through the O phase
from localised-electron behaviour and orbital ordering in the O′ phase
to itinerant-electron behaviour in an R-rhombohedral phase occurs with
increasing geometric tolerance factor t ≡
⟨A-O⟩/√2⟨Mn-O⟩, where ⟨A-O⟩ and
⟨Mn-O⟩ are mean equilibrium bond lengths. The CMR occurs in the
temperature interval Tc ≤ T <
Ts where there is a segregation, via cooperative oxygen
displacements, into a Mn(IV)-rich ferromagnetic phase imbedded in a
paramagnetic phase. The volume of the ferromagnetic, more conductive clusters
increases from below to beyond a percolation threshold in response, above
Tc, to an applied magnetic field and, below
Tc, to a Weiss molecular field. In the O phase, the
magnetic transition at Tc decreases on the exchange of
18O/16O and increases under
hydrostatic pressure. Charge and orbital ordering below a
Tco ≤ Tc is found in
compositions with x ≈ ⅛ or
x ≈ ½. With x ≈
½, the charge-ordered phase CE is tetragonal and antiferromagnetic. An
applied magnetic field stabilises the ferromagnetic, conductive phase relative
to the insulator phase CE to give a second type of intrinsic CMR. For
x ≈ 0·3, there is no static charge and orbital
ordering; but for smaller t, strong electron-lattice
coupling gives a ‘bad metal’ behaviour below
Tc indicative of a dynamic phase segregation as in a
traveling charge-density wave. In
La1-xCaxMnO3
with ½ ≤ x ≤ ⅞, segregation of the
CE x = 0·5 phase and the all-Mn(IV)
x = 1 phase has been reported to take the form of
a static charge-density wave. The origins of this complex behaviour are
discussed.
Subject
General Physics and Astronomy
Cited by
92 articles.
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