Solution-Processed Tin-Antimony Quaternary Chalcohalides for Self-Powered Broadband Photodetectors

IF 6 3区 工程技术 Q2 ENERGY & FUELS
Solar RRL Pub Date : 2024-10-30 DOI:10.1002/solr.202400633
Debjit Manna, Krishnaiah Mokurala, G. Krishnamurthy Grandhi, Basheer Al-Anesi, Noolu Srinivasa Manikanta Viswanath, Vipinraj Sugathan, Amit Tewari, Ceylan Doyranli, Paola Vivo
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Abstract

The mixed-metal quaternary chalcohalides of group IV and V elements are a promising class of low-toxicity perovskite-inspired materials with tunable bandgaps and desirable defect tolerance. Sn2SbS2I3 is known for its broadband absorption, low exciton binding energy, ambient stability, and solution processability in thin films. However, its use in optoelectronic devices has so far been only limited to solar cells. In this work, the first self-powered photodetectors based on Sn2SbS2I3 thin films, sandwiched in an n–i–p device configuration are reported. The insertion of an interlayer at the hole-transport layer/gold top-electrode interface reduces the dark current and improves the device performance. The high external quantum efficiency of the devices in the range of 350−900 nm hints to a broadband spectral photoresponsivity. The devices indeed exhibit promising photodetection properties, namely a photoresponsivity of 0.33 A W−1, a specific detectivity of 1.55 × 1012 Jones, and photoresponse/decay times of 0.52 and 0.45 s at zero bias voltage. These results, combined with the excellent operational stability of the photodetectors, encourage the exploration of a wide range of practical light-sensing applications for quaternary chalcohalides and stimulate device and material engineering to further enhance photodetection across the UV-Visible-NIR spectrum.

Abstract Image

第 IV 族和第 V 族元素的混合金属季卤化物是一类很有前途的低毒性过氧化物启发材料,具有可调带隙和理想的缺陷容限。Sn2SbS2I3 因其宽带吸收、低激子结合能、环境稳定性和薄膜的溶液加工性而闻名。然而,迄今为止,它在光电设备中的应用还仅限于太阳能电池。在这项研究中,首次报道了基于 Sn2SbS2I3 薄膜的自供电光电探测器,它采用 ni-p 器件配置夹层。在空穴传输层/金顶电极界面插入中间层可降低暗电流并提高器件性能。器件在 350-900 纳米范围内的高外部量子效率暗示了宽光谱光致发光性。该器件确实表现出良好的光探测特性,即光致共振率为 0.33 A W-1,比探测率为 1.55 × 1012 Jones,零偏置电压下的光致响应/衰减时间分别为 0.52 秒和 0.45 秒。这些结果与光电探测器出色的工作稳定性相结合,鼓励人们探索四元卤化物在光传感方面的广泛实际应用,并激励器件和材料工程进一步增强紫外-可见-近红外光谱的光电探测能力。
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来源期刊
Solar RRL
Solar RRL Physics and Astronomy-Atomic and Molecular Physics, and Optics
CiteScore
12.10
自引率
6.30%
发文量
460
期刊介绍: Solar RRL, formerly known as Rapid Research Letters, has evolved to embrace a broader and more encompassing format. We publish Research Articles and Reviews covering all facets of solar energy conversion. This includes, but is not limited to, photovoltaics and solar cells (both established and emerging systems), as well as the development, characterization, and optimization of materials and devices. Additionally, we cover topics such as photovoltaic modules and systems, their installation and deployment, photocatalysis, solar fuels, photothermal and photoelectrochemical solar energy conversion, energy distribution, grid issues, and other relevant aspects. Join us in exploring the latest advancements in solar energy conversion research.
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