Temperature-dependent photoluminescence of lead-free cesium tin halide perovskite microplates

Tin halide perovskites recently have attracted extensive research attention due to their similar electronic and band structures but non-toxicity compared with their lead analogues. In this work, we prepare high-quality CsSn X 3 ( X = Br, I) microplates with lateral sizes of around 1–4 μm by chemical...

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Veröffentlicht in:Chinese physics B 2023-11, Vol.32 (11), p.117802-137
Hauptverfasser: Tan, Jiayu, Zhou, Yixuan, Lu, De, Feng, Xukun, Liu, Yuqi, Zhang, Mengen, Lu, Fangzhengyi, Huang, Yuanyuan, Xu, Xinlong
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container_end_page 137
container_issue 11
container_start_page 117802
container_title Chinese physics B
container_volume 32
creator Tan, Jiayu
Zhou, Yixuan
Lu, De
Feng, Xukun
Liu, Yuqi
Zhang, Mengen
Lu, Fangzhengyi
Huang, Yuanyuan
Xu, Xinlong
description Tin halide perovskites recently have attracted extensive research attention due to their similar electronic and band structures but non-toxicity compared with their lead analogues. In this work, we prepare high-quality CsSn X 3 ( X = Br, I) microplates with lateral sizes of around 1–4 μm by chemical vapor deposition and investigate their low-temperature photoluminescence (PL) properties. A remarkable splitting of PL peaks of the CsSnBr 3 microplate is observed at low temperatures. Besides the possible structural phase transition at below 70 K, the multi-peak fittings using Gauss functions and the power-dependent saturation phenomenon suggest that the PL could also be influenced by the conversion from the emission of bound excitons into free excitons. With the increase of temperature, the peak position shows a blueshift tendency for CsSnI 3 , which is governed by thermal expansion. However, the peak position of the CsSnBr 3 microplate exhibits a transition from redshift to blueshift at ∼160 K. The full width at half maximum of CsSn X 3 broadens with increasing temperature, and the fitting results imply that longitudinal optical phonons dominate the electron–phonon coupling and the coupling strength is much more robust in CsSnBr 3 than in CsSnI 3 . The PL intensity of CsSn X 3 microplates is suppressed due to the enhanced non-radiative relaxation and exciton dissociation competing with radiative recombination. According to the Arrhenius law, the exciton binding energy of CsSnBr 3 is ∼38.4 meV, slightly smaller than that of CsSnI 3 .
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In this work, we prepare high-quality CsSn X 3 ( X = Br, I) microplates with lateral sizes of around 1–4 μm by chemical vapor deposition and investigate their low-temperature photoluminescence (PL) properties. A remarkable splitting of PL peaks of the CsSnBr 3 microplate is observed at low temperatures. Besides the possible structural phase transition at below 70 K, the multi-peak fittings using Gauss functions and the power-dependent saturation phenomenon suggest that the PL could also be influenced by the conversion from the emission of bound excitons into free excitons. With the increase of temperature, the peak position shows a blueshift tendency for CsSnI 3 , which is governed by thermal expansion. However, the peak position of the CsSnBr 3 microplate exhibits a transition from redshift to blueshift at ∼160 K. The full width at half maximum of CsSn X 3 broadens with increasing temperature, and the fitting results imply that longitudinal optical phonons dominate the electron–phonon coupling and the coupling strength is much more robust in CsSnBr 3 than in CsSnI 3 . The PL intensity of CsSn X 3 microplates is suppressed due to the enhanced non-radiative relaxation and exciton dissociation competing with radiative recombination. 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Phys. B</addtitle><description>Tin halide perovskites recently have attracted extensive research attention due to their similar electronic and band structures but non-toxicity compared with their lead analogues. In this work, we prepare high-quality CsSn X 3 ( X = Br, I) microplates with lateral sizes of around 1–4 μm by chemical vapor deposition and investigate their low-temperature photoluminescence (PL) properties. A remarkable splitting of PL peaks of the CsSnBr 3 microplate is observed at low temperatures. Besides the possible structural phase transition at below 70 K, the multi-peak fittings using Gauss functions and the power-dependent saturation phenomenon suggest that the PL could also be influenced by the conversion from the emission of bound excitons into free excitons. With the increase of temperature, the peak position shows a blueshift tendency for CsSnI 3 , which is governed by thermal expansion. However, the peak position of the CsSnBr 3 microplate exhibits a transition from redshift to blueshift at ∼160 K. The full width at half maximum of CsSn X 3 broadens with increasing temperature, and the fitting results imply that longitudinal optical phonons dominate the electron–phonon coupling and the coupling strength is much more robust in CsSnBr 3 than in CsSnI 3 . The PL intensity of CsSn X 3 microplates is suppressed due to the enhanced non-radiative relaxation and exciton dissociation competing with radiative recombination. 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Phys. B</addtitle><date>2023-11-01</date><risdate>2023</risdate><volume>32</volume><issue>11</issue><spage>117802</spage><epage>137</epage><pages>117802-137</pages><issn>1674-1056</issn><eissn>2058-3834</eissn><abstract>Tin halide perovskites recently have attracted extensive research attention due to their similar electronic and band structures but non-toxicity compared with their lead analogues. In this work, we prepare high-quality CsSn X 3 ( X = Br, I) microplates with lateral sizes of around 1–4 μm by chemical vapor deposition and investigate their low-temperature photoluminescence (PL) properties. A remarkable splitting of PL peaks of the CsSnBr 3 microplate is observed at low temperatures. Besides the possible structural phase transition at below 70 K, the multi-peak fittings using Gauss functions and the power-dependent saturation phenomenon suggest that the PL could also be influenced by the conversion from the emission of bound excitons into free excitons. With the increase of temperature, the peak position shows a blueshift tendency for CsSnI 3 , which is governed by thermal expansion. However, the peak position of the CsSnBr 3 microplate exhibits a transition from redshift to blueshift at ∼160 K. The full width at half maximum of CsSn X 3 broadens with increasing temperature, and the fitting results imply that longitudinal optical phonons dominate the electron–phonon coupling and the coupling strength is much more robust in CsSnBr 3 than in CsSnI 3 . The PL intensity of CsSn X 3 microplates is suppressed due to the enhanced non-radiative relaxation and exciton dissociation competing with radiative recombination. According to the Arrhenius law, the exciton binding energy of CsSnBr 3 is ∼38.4 meV, slightly smaller than that of CsSnI 3 .</abstract><pub>Chinese Physical Society and IOP Publishing Ltd</pub><doi>10.1088/1674-1056/ad028e</doi><tpages>8</tpages></addata></record>
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subjects cesium tin halide perovskite
chemical vapor deposition
microplate
temperature-dependent photoluminescence
title Temperature-dependent photoluminescence of lead-free cesium tin halide perovskite microplates
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