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氢键及其他非共价相互作用在确定CHNHPbI混合有机-无机卤化物钙钛矿太阳能电池半导体中八面体倾斜方面的意义。

Significance of hydrogen bonding and other noncovalent interactions in determining octahedral tilting in the CHNHPbI hybrid organic-inorganic halide perovskite solar cell semiconductor.

作者信息

Varadwaj Pradeep R, Varadwaj Arpita, Marques Helder M, Yamashita Koichi

机构信息

Department of Chemical System Engineering, School of Engineering, The University of Tokyo 7-3-1, Hongo, Bunkyo-ku, 113-8656, Japan.

CREST-JST, 7 Gobancho, Chiyoda-ku, Tokyo, 102-0076, Japan.

出版信息

Sci Rep. 2019 Jan 10;9(1):50. doi: 10.1038/s41598-018-36218-1.

DOI:10.1038/s41598-018-36218-1
PMID:30631082
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC6328624/
Abstract

The CHNHPbI (methylammonium lead triiodide) perovskite semiconductor system has been viewed as a blockbuster research material during the last five years. Because of its complicated architecture, several of its technological, physical and geometrical issues have been examined many times. Yet this has not assisted in overcoming a number of problems in the field nor in enabling the material to be marketed. For instance, these studies have not clarified the nature and type of hydrogen bonding and other noncovalent interactions involved; the origin of hysteresis; the actual role of the methylammonium cation; the nature of polarity associated with the tetragonal geometry; the unusual origin of various frontier orbital contributions to the conduction band minimum; the underlying phenomena of spin-orbit coupling that causes significant bandgap reduction; and the nature of direct-to-indirect bandgap transition features. Arising from many recent reports, it is now a common belief that the I···H-N interaction formed between the inorganic framework and the ammonium group of CHNH is the only hydrogen bonded interaction responsible for all temperature-dependent geometrical polymorphs of the system, including the most stable one that persists at low-temperatures, and the significance of all other noncovalent interactions has been overlooked. This study focussed only on the low temperature orthorhombic polymorph of CHNHPbI and CDNDPbI, where D refers deuterium. Together with QTAIM, DORI and RDG based charge density analyses, the results of density functional theory calculations with PBE with and without van der Waals corrections demonstrate that the prevailing view of hydrogen bonding in CHNHPbI is misleading as it does not alone determine the aba tilting pattern of the PbI octahedra. This study suggests that it is not only the I···H/D-N, but also the I···H/D-C hydrogen/deuterium bonding and other noncovalent interactions (viz. tetrel-, pnictogen- and lump-hole bonding interactions) that are ubiquitous in the orthorhombic CHNHPbI/CDNDPbI perovskite geometry. Their interplay determines the overall geometry of the polymorph, and are therefore responsible in part for the emergence of the functional optical properties of this material. This study also suggests that these interactions should not be regarded as the sole determinants of octahedral tilting since lattice dynamics is known to play a critical role as well, a common feature in many inorganic perovskites both in the presence and the absence of the encaged cation, as in CsPbI/WO perovskites, for example.

摘要

在过去五年中,CHNHPbI(甲基铵三碘化铅)钙钛矿半导体体系一直被视为一种重磅研究材料。由于其结构复杂,其若干技术、物理和几何问题已被多次研究。然而,这并未有助于克服该领域的一些问题,也未能使该材料得以市场化。例如,这些研究尚未阐明所涉及的氢键及其他非共价相互作用的性质和类型;滞后现象的起源;甲基铵阳离子的实际作用;与四方几何结构相关的极性的本质;各种前沿轨道对导带最小值贡献的异常起源;导致显著带隙减小的自旋 - 轨道耦合的潜在现象;以及直接带隙到间接带隙转变特征的本质。从最近的许多报道来看,现在人们普遍认为,无机骨架与CHNH的铵基团之间形成的I···H - N相互作用是导致该体系所有温度依赖性几何多晶型的唯一氢键相互作用,包括在低温下持续存在的最稳定的多晶型,而所有其他非共价相互作用的重要性被忽视了。本研究仅聚焦于CHNHPbI和CDNDPbI(其中D指氘)的低温正交多晶型。结合基于QTAIM、DORI和RDG的电荷密度分析,有无范德华校正的PBE密度泛函理论计算结果表明,CHNHPbI中关于氢键的主流观点具有误导性,因为它并不能单独决定PbI八面体的aba倾斜模式。本研究表明,在正交CHNHPbI/CDNDPbI钙钛矿几何结构中,不仅存在I···H/D - N,还存在I···H/D - C氢/氘键以及其他非共价相互作用(即碳族元素 - 、氮族元素 - 和空穴键合相互作用)。它们的相互作用决定了多晶型的整体几何结构,因此部分地决定了这种材料功能性光学性质的出现。本研究还表明,这些相互作用不应被视为八面体倾斜的唯一决定因素,因为晶格动力学也起着关键作用,这在许多无机钙钛矿中是一个共同特征,无论是否存在笼状阳离子,例如在CsPbI/WO钙钛矿中。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c7cf/6328624/3ff24af7565d/41598_2018_36218_Fig13_HTML.jpg
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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c7cf/6328624/e748f6bb562f/41598_2018_36218_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c7cf/6328624/522a8c08866c/41598_2018_36218_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c7cf/6328624/d438fa2d20f0/41598_2018_36218_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c7cf/6328624/8cae52c9ea45/41598_2018_36218_Fig6_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c7cf/6328624/507daf7c86a5/41598_2018_36218_Fig7_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c7cf/6328624/09b2da7245d5/41598_2018_36218_Fig8_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c7cf/6328624/a6479b5af3e4/41598_2018_36218_Fig9_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c7cf/6328624/8122dc162847/41598_2018_36218_Fig10_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c7cf/6328624/ad0c57fbe88d/41598_2018_36218_Fig11_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c7cf/6328624/e4a181837d56/41598_2018_36218_Fig12_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c7cf/6328624/3ff24af7565d/41598_2018_36218_Fig13_HTML.jpg

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