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飞秒极紫外吸收揭示的CHNHPbI中特定载流子的热声子瓶颈效应

Carrier-Specific Hot Phonon Bottleneck in CHNHPbI Revealed by Femtosecond XUV Absorption.

作者信息

Verkamp Max, Leveillee Joshua, Sharma Aastha, Lin Ming-Fu, Schleife André, Vura-Weis Josh

机构信息

Department of Chemistry, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, United States.

Department of Materials Science and Engineering, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, United States.

出版信息

J Am Chem Soc. 2021 Dec 8;143(48):20176-20182. doi: 10.1021/jacs.1c07817. Epub 2021 Nov 23.

Abstract

Femtosecond carrier cooling in the organohalide perovskite semiconductor CHNHPbI is measured using extreme ultraviolet (XUV) and optical transient absorption spectroscopy. XUV absorption between 44 and 58 eV measures transitions from the I 4d core to the valence and conduction bands and gives distinct signals for hole and electron dynamics. The core-to-valence-band signal directly maps the photoexcited hole distribution and provides a quantitative measurement of the hole temperature. The combination of XUV and optical probes reveals that upon excitation at 400 nm, the initial hole distribution is 3.5 times hotter than the electron distribution. At an initial carrier density of 1.4 × 10 cm both carriers are subject to a hot phonon bottleneck, but at 4.2 × 10 cm the holes cool to less than 1000 K within 400 fs. This result places significant constraints on the use of organohalide perovskites in hot-carrier photovoltaics.

摘要

利用极紫外(XUV)和光学瞬态吸收光谱法测量了有机卤化物钙钛矿半导体CHNHPbI中的飞秒载流子冷却。44至58电子伏特之间的XUV吸收测量了从I 4d芯能级到价带和导带的跃迁,并给出了空穴和电子动力学的独特信号。芯能级到价带的信号直接映射了光激发空穴分布,并提供了空穴温度的定量测量。XUV和光学探针的结合表明,在400纳米激发时,初始空穴分布比电子分布热3.5倍。在初始载流子密度为1.4×10厘米时,两种载流子都受到热声子瓶颈的影响,但在4.2×10厘米时,空穴在400飞秒内冷却到低于1000 K。这一结果对有机卤化物钙钛矿在热载流子光伏中的应用施加了重大限制。

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