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Orbital tomography: Molecular band maps, momentum maps and the imaging of real space orbitals of adsorbed molecules

机译:轨道层析成像:分子能带图,动量图和被吸附分子的真实空间轨道成像

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The frontier orbitals of molecules are the prime determinants of their chemical, optical and electronic properties. Arguably, the most direct method of addressing the (filled) frontier orbitals is ultra-violet photoemission spectroscopy (UPS). Although UPS is a mature technique from the early 1970s on, the angular distribution of the photoemitted electrons was thought to be too complex to be analysed quantitatively. Recently angle resolved UPS (ARUPS) work on conjugated molecules both, in ordered thick films and chemisorbed monolayers, has shown that the angular (momentum) distribution of the photocurrent from orbital emissions can be simply understood. The approach, based on the assumption of a plane wave final state is becoming known as orbital tomography. Here we will demonstrate, with selected examples of pentacene (5A) and sexiphenyl (6P), the potential of orbital tomography. First it will be shown how the full angular distribution of the photocurrent (momentum map) from a specific orbital is related to the real space orbital by a Fourier transform. Examples of the reconstruction of 5A orbitals will be given and the procedure for recovering the lost phase information will be outlined. We then move to examples of sexiphenyl where we interrogate the original band maps of thick sexiphenyl in the light of our understanding of orbital tomography that has developed since then. With comparison to theoretical simulations of the molecular band maps, the molecular conformation and orientation will be concluded. New results for the sexiphenyl monolayer on Al(1 1 0) will then be presented. From the band maps it will be concluded that the molecule is planarised and adopts a tilted geometry. Finally the momentum maps down to HOMO-11 will be analysed and real space orbitals reconstructed. (C) 2015 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY license.
机译:分子的边界轨道是其化学,光学和电子性质的主要决定因素。可以说,解决(填充的)前沿轨道最直接的方法是紫外光发射光谱法(UPS)。尽管UPS是从1970年代初期开始的一项成熟技术,但人们认为光发射电子的角度分布过于复杂,无法进行定量分析。最近,角度分辨UPS(ARUPS)在有序厚膜和化学吸附的单层膜上对共轭分子都进行了研究,结果表明,可以很容易地理解来自轨道发射的光电流的角(动量)分布。这种基于平面波最终状态的假设的方法被称为轨道层析成像。在这里,我们将通过并五苯(5A)和六苯(6P)的选定例子来证明轨道层析成像的潜力。首先,将通过傅立叶变换示出来自特定轨道的光电流(动量图)的整个角分布如何与实际空间轨道相关。将给出重建5A轨道的示例,并概述恢复丢失相位信息的过程。然后,我们移至六联苯的例子,根据我们对自那时以来形成的轨道层析成像技术的了解,我们在其中询问了厚六联苯的原始谱带图。与分子带图的理论模拟相比较,将得出分子构象和取向。然后将介绍Al(1 1 0)上六苯基单层的新结果。从能带图可以得出结论,分子被平面化并采用倾斜的几何形状。最后,将分析直到HOMO-11的动量图,并重建实际空间轨道。 (C)2015作者。由Elsevier B.V.发布。这是CC BY许可下的开放获取文章。

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