Orbital-order phase transition in Pr1−xCaxMnO3 probed by photovoltaics

B. Kressdorf, T. Meyer, M. Ten Brink, C. Seick, S. Melles, N. Ottinger, T. Titze, H. Meer, A. Weisser, J. Hoffmann, S. Mathias, H. Ulrichs, D. Steil, M. Seibt, P. Blöchl, C. Jooss
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引用次数: 2

Abstract

A new phase diagram of $Pr_{1-x}Ca_xMnO_3$ for x $\le$ 0.3 is derived that suggests a necessary revaluation of the phase diagram of other manganites in that doping region. Rather than an orbital ordered phase reaching up to high temperatures 850 K for x=0.1 and 950 K for x=0, we propose a loss of spontaneous order already near room temperature. Above this temperature, the phase is characterized by a finite orbital polarization and octahedral tilt pattern. The tilt pattern couples to the Jahn-Teller distortion and thus induces a remaining orbital order, which persists up to high temperatures, where the tilt order is lost as well. This explains the experimental observation of orbital order up to high temperatures. Anomalies at a temperature 220-260 K have been observed in epitaxial thin films of doping x=0.1 for photovoltaic effect, electric transport, magnetisation, optical and ultrafast transient pump probe studies. The onset of the polaron photovoltaic effect and the increase of the hot polaron relaxation time below $T_{OO}$ suggest a change in the orbital order. Finite-temperature simulations based on a tight-binding model with carefully adjusted parameters from first-principles calculations exhibit an orbital-order phase transition at $T_{OO} \approx$ 300 K for x=0.1. This is consistent with the experimental observation of a change in temperature dependent lattice parameter for bulk samples of the same doping at 300 K for x=0.1 and 350 K for x=0, typical for a second order phase transition.
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Pr1−xCaxMnO3的轨道序相变
得到了x $\le$ 0.3的新相图$Pr_{1-x}Ca_xMnO_3$,这表明有必要对该掺杂区域内其他锰的相图进行重新评估。而不是轨道有序相达到高温850 K, x=0.1和950 K, x=0,我们提出自发有序的损失已经接近室温。在此温度以上,相位的特征是有限轨道极化和八面体倾斜模式。倾斜模式与扬-泰勒扭曲耦合,从而引起剩余的轨道顺序,这种顺序一直持续到高温,在高温下倾斜顺序也会丢失。这解释了在高温下轨道有序的实验观察。在220-260 K温度下,掺杂x=0.1的外延薄膜在光伏效应、电输运、磁化、光学和超快瞬态泵探针研究中发现了异常现象。极化子光伏效应的发生和热极化子弛豫时间在$T_{OO}$以下的增加表明轨道顺序发生了变化。基于紧密结合模型的有限温度模拟,通过第一原理计算仔细调整参数,显示出在$T_{OO} \approx$ 300 K时x=0.1的轨道阶相变。这与实验观察到的相同掺杂的大块样品在300 K时(x=0.1)和350 K时(x=0)的晶格参数随温度变化的变化是一致的,这是典型的二级相变。
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