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000836738 0247_ $$2doi$$a10.1103/PhysRevB.96.054107
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000836738 245__ $$aThermally assisted ordering in Mott insulators
000836738 260__ $$aWoodbury, NY$$bInst.$$c2017
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000836738 520__ $$aLandau theory describes phase transitions as the competition between energy and entropy: The ordered phase has lower energy, while the disordered phase has larger entropy. When heating the system, ordering is reduced entropically until it vanishes at the critical temperature. This picture implicitly assumes that the energy difference between the ordered and disordered phases does not change with temperature. We show that for orbital ordering in the Mott insulator KCuF3, this assumption fails qualitatively: entropy plays a negligible role, while thermal expansion energetically stabilizes the orbitally ordered phase to such an extent that no phase transition is observed. To understand this strong dependence on the lattice constant, we need to take into account the Born-Mayer repulsion between the ions. It is the latter, and not the Jahn-Teller elastic energy, which determines the magnitude of the distortion. This effect will be seen in all materials where the distortion expected from the Jahn-Teller mechanism is so large that the ions would touch. Our mechanism explains not only the absence of a phase transition in KCuF3, but even suggests the possibility of an inverted transition in closed-shell systems, where the ordered phase emerges only at high temperatures.
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000836738 536__ $$0G:(DE-Juel1)jiff41_20091101$$aMultiplet effects in strongly correlated materials (jiff41_20091101)$$cjiff41_20091101$$fMultiplet effects in strongly correlated materials$$x2
000836738 536__ $$0G:(DE-Juel1)jiff46_20101101$$aOrder-disorder transitions in strongly correlated systems (jiff46_20101101)$$cjiff46_20101101$$fOrder-disorder transitions in strongly correlated systems$$x3
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000836738 7001_ $$0P:(DE-Juel1)130881$$aPavarini, Eva$$b1
000836738 7001_ $$0P:(DE-Juel1)130763$$aKoch, Erik$$b2$$eCorresponding author
000836738 773__ $$0PERI:(DE-600)2844160-6$$a10.1103/PhysRevB.96.054107$$p054107$$tPhysical review / B$$v96$$x0163-1829$$y2017
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