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氧诱导板钛矿型二氧化钛粉末中近红外发射增强:与金红石型和锐钛矿型二氧化钛粉末的比较

Oxygen induced enhancement of NIR emission in brookite TiO powders: comparison with rutile and anatase TiO powders.

作者信息

Vequizo Junie Jhon M, Kamimura Sunao, Ohno Teruhisa, Yamakata Akira

机构信息

Graduate School of Engineering, Toyota Technological Institute, 2-12-1 Hisakata, Tempaku, Nagoya 468-8511, Japan.

出版信息

Phys Chem Chem Phys. 2018 Jan 31;20(5):3241-3248. doi: 10.1039/c7cp06975h.

Abstract

Brookite TiO attracts considerable attention in photocatalysis owing to its superior performance in several photocatalytic reactions. In this work, we investigated the behavior of charge carriers in brookite, rutile, and anatase TiO by using photoluminescence (PL) and transient absorption (TA) spectroscopies. PL measurements revealed that brookite TiO exhibits a visible and a NIR emission at ∼520 nm and ∼860 nm, respectively. Addition of methanol vapor quenched both the visible and NIR emissions by the hole-consuming reaction of methanol. However, exposure to O shows curious behaviors: the visible emission was quenched but the NIR emission was enhanced. These results can be accounted for by the enhancement of upward band bending resulting in the effective separation of electrons and holes into the bulk and the surface, respectively. Furthermore, the shallowly trapped electrons, which are responsible for visible PL, are consumed by O; hence, the visible emission is quenched. However, in the case of NIR emission, the deeply trapped electrons are responsible and they are mainly located at the surface defects. The O adsorption promotes the hole accumulation at the surface and then assists the recombination of these deeply trapped electrons, resulting in the enhancement of the NIR emission. We also found that the lifetime of NIR emission (τ = 43 ± 0 ns and τ = 589 ± 1 ns) was much longer than that of visible emission (τ = 15 ± 0 ns and τ = 23 ± 0 ns), since the mobility of these deeply trapped electrons to encounter with holes is lower than that of the shallowly trapped electrons. However, even for this slow NIR emission, the actual lifetime of the deeply trapped electrons estimated by TA (1.5 ± 0.0 μs and 17 ± 0 μs) was one or two orders of magnitude longer, confirming that non-radiative recombination is dominant and it is much slower than radiative recombination: TAS and PL provide detailed information on the radiative and non-radiative recombination processes. The PL of anatase and rutile TiO powders was also measured and the difference from brookite TiO was discussed.

摘要

板钛矿TiO₂由于在几种光催化反应中表现出优异性能,在光催化领域引起了广泛关注。在本工作中,我们通过光致发光(PL)和瞬态吸收(TA)光谱研究了板钛矿、金红石和锐钛矿TiO₂中电荷载流子的行为。PL测量表明,板钛矿TiO₂分别在约520 nm和约860 nm处表现出可见光和近红外发射。添加甲醇蒸汽通过甲醇的空穴消耗反应猝灭了可见光和近红外发射。然而,暴露于O₂表现出奇特的行为:可见光发射被猝灭,但近红外发射增强。这些结果可以通过向上能带弯曲的增强来解释,这导致电子和空穴分别有效地分离到体相和表面。此外,负责可见光PL的浅捕获电子被O₂消耗;因此,可见光发射被猝灭。然而,在近红外发射的情况下,深捕获电子起作用,它们主要位于表面缺陷处。O₂吸附促进了表面空穴的积累,然后协助这些深捕获电子的复合,导致近红外发射增强。我们还发现近红外发射的寿命(τ = 43 ± 0 ns和τ = 589 ± 1 ns)比可见光发射的寿命(τ = 15 ± 0 ns和τ = 23 ± 0 ns)长得多,因为这些深捕获电子与空穴相遇的迁移率低于浅捕获电子。然而,即使对于这种缓慢的近红外发射,通过TA估计的深捕获电子的实际寿命(1.5 ± 0.0 μs和17 ± 0 μs)长一个或两个数量级,证实了非辐射复合占主导,并且比辐射复合慢得多:TAS和PL提供了关于辐射和非辐射复合过程的详细信息。还测量了锐钛矿和金红石TiO₂粉末的PL,并讨论了与板钛矿TiO₂的差异。

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