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Two dimensional thin film surface layer structure of the promising new photo-catalyst InVO_4 for water molecule decomposition with water molecules adsorbed on the surface

机译:有前景的新型光催化剂InVO_4的二维薄膜表面层结构,用于水分子分解并吸附在表面上

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A photo-catalyst able to enhance the decomposition of water molecules (hydrolysis) and able to work in the frequency range of visible light (or a wider wavelength region) is highly desirable for solar energy storing. However, to date, most of the photo-catalyst can work only in the ultra violet (UV) region (< 420 nm). The electron affinity - that can be identified as the conduction band bottom (CBB) - of the most of the photo-catalysts consists of d orbitals of transition metals (e.g. Zr, Ta, Nb, Ti), while the ionization potential ― represented by the valence band top (VBT) ― is represented by the 2p states of the oxygen atoms. Given this scenario, one could intuitively infer that a way to activate the catalyst in the longer wavelength region would be to lower the bottom of the 3d conduction band in order to make it closer to the redox level of H~+/H~2. A previous work by Z. Zou et al. indicated that InTaO_4 and InNbO_4 have a catalytic activity in the visible region up to 500nm. This has encouraged us to inspect V-based catalysts in order to get a better insight in this class of systems. The results coming from experiments have shown that, indeed, InVO_4 has a photo-catalytic activity responsible for the observed hydrogen evolution in the visible range (> 600 nm)as shown in Figure. 1 and this provided a basis for a theoretical inspection of the related electronic structure. In this paper, we report the results of our first principles calculations on the structural properties of InVO_4 and surface relaxation processes induced by the absorption of H_2O. This study is a necessary step and a valid testing ground in view of the extension of the approach to the analysis of the excitation spectrum of the catalyst surface in presence of H_2O molecules.
机译:对于太阳能存储,非常需要能够增强水分子的分解(水解)并且能够在可见光的频率范围(或更宽的波长范围)内工作的光催化剂。但是,到目前为止,大多数光催化剂只能在紫外线(<420 nm)区域中工作。大多数光催化剂的电子亲合势能(可以识别为导带底(CBB))由过渡金属的d个轨道(例如Zr,Ta,Nb,Ti)组成,而电离势以价带顶(VBT)由氧原子的2p态表示。在这种情况下,可以直观地推断出在较长波长区域内激活催化剂的一种方法是降低3d导带的底部,以使其更接近H〜+ / H〜2的氧化还原水平。 Z. Zou等人的先前工作。指出InTaO_4和InNbO_4在高达500nm的可见光区具有催化活性。这鼓励我们检查基于V的催化剂,以便对此类系统有更好的了解。来自实验的结果表明,实际上,InVO_4具有光催化活性,这是在可见光范围(> 600 nm)中观察到的氢逸出的原因,如图所示。参照图1,这为相关电子结构的理论检查提供了基础。在本文中,我们报告了有关InVO_4的结构性质和H_2O吸收引起的表面弛豫过程的第一性原理计算结果。鉴于将方法扩展到存在H_2O分子时催化剂表面的激发光谱的分析,这项研究是必要的步骤和有效的试验依据。

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