Optoelectronic properties of facile synthesized orthorhombic cesium lead bromide (CsPbBr3)
Autor: | Prasenjit Maji, Sachindranath Das, Priyabrata Sadhukhan |
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Rok vydání: | 2020 |
Předmět: |
010302 applied physics
Photocurrent Materials science Rietveld refinement business.industry Schottky barrier Condensed Matter Physics 01 natural sciences Atomic and Molecular Physics and Optics Electronic Optical and Magnetic Materials Responsivity Nanocrystal 0103 physical sciences Optoelectronics Orthorhombic crystal system Grain boundary Crystallite Electrical and Electronic Engineering business |
Zdroj: | Journal of Materials Science: Materials in Electronics. 31:17100-17109 |
ISSN: | 1573-482X 0957-4522 |
Popis: | CsPbBr3 has been synthesized via a wet chemical technique instead of colloidal hot injection route. Crystalline structure and chemical composition of the material have been assured by Rietveld refinement and energy dispersive X-ray spectroscopy. Photoresponse capability of CsPbBr3 nanocrystal in cubic phase has been already explored. Here, intrinsic optoelectronic properties of orthorhombic CsPbBr3 have been investigated in detail. A prototype photodetector has been fabricated on a transparent conducting oxide-coated glass by using silver as the other electrode material. The photo-responsibility of CsPbBr3 arises due to the combined effect of electron–hole pair generation and trapping within material and recombination. The non-linearity of I–V characteristics clearly reveals the formation of well-established Schottky contact at perovskite–ITO junction. Responsivity of the detector increases from 1.4 to 1.73 mA W−1 after enhancing the irradiance from 25 to 100 mW cm−2 at 8 V bias voltages. Linear dynamic range has been accounted to study the linear photosensitivity of the device. In order to investigate the stability and reversibility, photocurrent has been measured under ON/OFF condition of frequency 20 s. The quantitative contribution of polycrystalline grain and grain boundary to charge mobilization has been evaluated by fitting the Cole–Cole plot under different solar intensities. |
Databáze: | OpenAIRE |
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