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胶体Ag2S纳米晶体异常激子吸收与发射的起源:超快光物理与太阳能电池

Origin of Unusual Excitonic Absorption and Emission from Colloidal Ag2S Nanocrystals: Ultrafast Photophysics and Solar Cell.

作者信息

Mir Wasim J, Swarnkar Abhishek, Sharma Rituraj, Katti Aditya, Adarsh K V, Nag Angshuman

机构信息

Department of Chemistry, Indian Institute of Science Education and Research (IISER) , Pune 411008, India.

Department of Physics, Indian Institute of Science Education and Research , Bhopal 462023, India.

出版信息

J Phys Chem Lett. 2015 Oct 1;6(19):3915-22. doi: 10.1021/acs.jpclett.5b01692. Epub 2015 Sep 17.

Abstract

Colloidal Ag2S nanocrystals (NCs) typically do not exhibit sharp excitonic absorption and emission. We first elucidate the reason behind this problem by preparing Ag2S NCs from nearly monodisperse CdS NCs employing cation exchange reaction. It was found that the defect-related midgap transitions overlap with excitonic transition, blurring the absorption spectrum. On the basis of this observation, we prepared nearly defect-free Ag2S NCs using molecular precursors. These defect-free Ag2S NCs exhibit sharp excitonic absorption, emission (quantum yield 20%) in near-infrared (853 nm) region, and improved performance of Ag2S quantum-dot-sensitized solar cells (QDSSCs). Samples with lower defects exhibit photoconversion efficiencies >1% and open circuit voltage of ∼0.3 V, which are better compared with prior reports of Ag2S QDSSCs. Femtosecond transient absorption shows pump-probe two-photon absorption above 630 nm and slow-decaying excited state absorption below 600 nm. Concomitantly, open-aperture z-scan shows strong two-photon absorption at 532 nm (coefficient 55 ± 3 cm/GW).

摘要

胶体硫化银纳米晶体(NCs)通常不会表现出尖锐的激子吸收和发射。我们首先通过利用阳离子交换反应从近乎单分散的硫化镉纳米晶体制备硫化银纳米晶体来阐明这一问题背后的原因。研究发现,与缺陷相关的带隙中跃迁与激子跃迁重叠,使吸收光谱变得模糊。基于这一观察结果,我们使用分子前驱体制备了近乎无缺陷的硫化银纳米晶体。这些无缺陷的硫化银纳米晶体在近红外(853 nm)区域表现出尖锐的激子吸收、发射(量子产率20%),并提高了硫化银量子点敏化太阳能电池(QDSSCs)的性能。缺陷较少的样品表现出大于1%的光转换效率和约0.3 V的开路电压,与之前关于硫化银量子点敏化太阳能电池的报道相比更好。飞秒瞬态吸收表明,在630 nm以上存在泵浦-探测双光子吸收,在600 nm以下存在缓慢衰减的激发态吸收。同时,开孔z扫描显示在532 nm处有强烈的双光子吸收(系数55±3 cm/GW)。

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