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Observing dynamic and static Rashba effects in a thin layer of 3D hybrid perovskite nanocrystals using transient absorption spectroscopy

机译:使用瞬态吸收光谱观察3D杂交钙钛矿纳米晶体薄层中的动态和静态Rashba效应

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The dynamic and static Rashba effects in hybrid methylammonium (MA) lead halide perovskites have recently been theoretically predicted. However, only the static effect was experimentally confirmed so far. Here, we report on the dynamic (sub-picosecond/picosecond timescale) and static (nanosecond/microsecond timescale) Rashba effects observed in a fully encapsulated layer with various thicknesses (ranging from ~40 nm to ~100 nm) of ~20-nm-sized 3D MAPbBrsub3/sub nanocrystals (NCs) using transient absorption (TA) spectroscopy. The effect appears as a splitting of the corresponding peaks in TA spectra. We argue that the physical reason for the Rashba effect to be observed is fundamentally determined by configurational entropy loss in NCs possessing a strong spin asymmetry. Specifically, owing to an enhanced flexibility of the NC lattice, a built-in electric field initially induced by an ultrashort (100 fs) pumping pulse through the photo-Dember effect and subsequently developed due to dynamic charge separation throughout NCs is able to initiate the order–disorder transition associated with the MA cation reorientations, the process that efficiently breaks structural inversion symmetry and hence induces the Rashba spin–orbit interaction. The dynamic Rashba effect is found to be strongly dependent on photoexcited carrier density (pumping power), whereas it weakens sharply upon increasing the NC layer thickness up to ~80 nm due to the NC stacking effect. The integrated intensities of the corresponding spin-split subbands demonstrate a photon-helicity-dependent asymmetry, thus proving the Rashba-type spin-splitting. The magnitudes of the Rashba and Fr?hlich polaron effects and the methods of controlling the dynamic Rashba effect are discussed.
机译:最近已经理论上预测了杂交甲基铵(MA)铅卤化物钙酸盐中的动态和静态RASHBA效应。但是,到目前为止只有静态效果实验证实。在这里,我们报告动态(亚皮秒/皮秒秒尺度)和静态(纳秒/微秒时间尺度)RASHBA效应,在一个完全封装的层中观察到的,其各种厚度(范围为约40nm至100nm),为20nm使用瞬态吸收(TA)光谱 - 为3D MAPBBR 3 纳米晶体(NCS)。效果显示为TA光谱中相应峰的分裂。我们认为要观察到的RASHBA效果的物理原因基本上通过具有强大旋转不对称的NCS中的配置熵损失基本确定。具体地,由于NC格的增强性,由于在整个NCS整个NCS的动态电荷分离而最初由超短(100FS)泵浦脉冲引起的内置电场并随后开发了能够启动与MA阳离子重构相关的令紊乱转变,该过程有效地破坏结构反转对称性,因此诱导Rashba旋转轨道交互。发现动态RASHBA效应强烈依赖于光屏蔽载波密度(泵送电源),而由于NC堆叠效果增加了最高〜80nm的NC层厚度,它在增加NC层厚度时急剧削弱。相应的自旋分流子带的综合强度证明了光子螺旋依赖性的不对称性,从而证明RASHBA型旋转分裂。讨论了Rashba和Fr的大小Δhlichpolaron效应和控制动态Rashba效果的方法。

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