Ga2O3 Schottky Avalanche Solar‐Blind Photodiode with High Responsivity and Photo‐to‐Dark Current Ratio

Abstract Solar‐blind photodetectors have attracted extensive attention due to their advantages such as ultra‐low background noise and all‐weather. In this study, the planar Ti/Ga2O3/Au Schottky avalanche photodetector (APD) is fabricated based on β‐Ga2O3 epitaxial film on the sapphire substrate grow...

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Main Authors: Shiqi Yan, Teng Jiao, Zijian Ding, Xinyu Zhou, Xingqi Ji, Xin Dong, Jiawei Zhang, Qian Xin, Aimin Song
Format: Article
Language:English
Published: Wiley-VCH 2023-11-01
Series:Advanced Electronic Materials
Subjects:
Online Access:https://doi.org/10.1002/aelm.202300297
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author Shiqi Yan
Teng Jiao
Zijian Ding
Xinyu Zhou
Xingqi Ji
Xin Dong
Jiawei Zhang
Qian Xin
Aimin Song
author_facet Shiqi Yan
Teng Jiao
Zijian Ding
Xinyu Zhou
Xingqi Ji
Xin Dong
Jiawei Zhang
Qian Xin
Aimin Song
author_sort Shiqi Yan
collection DOAJ
description Abstract Solar‐blind photodetectors have attracted extensive attention due to their advantages such as ultra‐low background noise and all‐weather. In this study, the planar Ti/Ga2O3/Au Schottky avalanche photodetector (APD) is fabricated based on β‐Ga2O3 epitaxial film on the sapphire substrate grown by metal–organic chemical vapor deposition. The Schottky APD exhibits a high responsivity of 9780.23 A W−1, an ultrahigh photo‐to‐dark current ratio of 1.88 × 107, an external quantum efficiency of 4.77 × 106%, a specific detectivity of 9.48 × 1014 Jones, with an ultrahigh gain of 1 × 106 under 254 nm light illumination at 60 V reverse bias, indicating high application potential for solar‐blind imaging. The superior photoresponse performances ascribe to the effective carrier avalanche multiplication, which contributes to the high photocurrent, and the high quality Schottky junction depletion, which leads to the low dark current.
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spelling doaj.art-8af64e18c4514a21971896a0bf1dd2602023-11-10T08:29:50ZengWiley-VCHAdvanced Electronic Materials2199-160X2023-11-01911n/an/a10.1002/aelm.202300297Ga2O3 Schottky Avalanche Solar‐Blind Photodiode with High Responsivity and Photo‐to‐Dark Current RatioShiqi Yan0Teng Jiao1Zijian Ding2Xinyu Zhou3Xingqi Ji4Xin Dong5Jiawei Zhang6Qian Xin7Aimin Song8Shandong Technology Center of Nanodevices and Integration School of Microelectronics Shandong University Jinan 250100 ChinaState Key Laboratory on Integrated Optoelectronics College of Electronic Science and Engineering Jilin University Changchun 130012 ChinaShandong Technology Center of Nanodevices and Integration School of Microelectronics Shandong University Jinan 250100 ChinaShandong Technology Center of Nanodevices and Integration School of Microelectronics Shandong University Jinan 250100 ChinaShandong Technology Center of Nanodevices and Integration School of Microelectronics Shandong University Jinan 250100 ChinaState Key Laboratory on Integrated Optoelectronics College of Electronic Science and Engineering Jilin University Changchun 130012 ChinaShandong Technology Center of Nanodevices and Integration School of Microelectronics Shandong University Jinan 250100 ChinaShandong Technology Center of Nanodevices and Integration School of Microelectronics Shandong University Jinan 250100 ChinaShandong Technology Center of Nanodevices and Integration School of Microelectronics Shandong University Jinan 250100 ChinaAbstract Solar‐blind photodetectors have attracted extensive attention due to their advantages such as ultra‐low background noise and all‐weather. In this study, the planar Ti/Ga2O3/Au Schottky avalanche photodetector (APD) is fabricated based on β‐Ga2O3 epitaxial film on the sapphire substrate grown by metal–organic chemical vapor deposition. The Schottky APD exhibits a high responsivity of 9780.23 A W−1, an ultrahigh photo‐to‐dark current ratio of 1.88 × 107, an external quantum efficiency of 4.77 × 106%, a specific detectivity of 9.48 × 1014 Jones, with an ultrahigh gain of 1 × 106 under 254 nm light illumination at 60 V reverse bias, indicating high application potential for solar‐blind imaging. The superior photoresponse performances ascribe to the effective carrier avalanche multiplication, which contributes to the high photocurrent, and the high quality Schottky junction depletion, which leads to the low dark current.https://doi.org/10.1002/aelm.202300297avalanche photodetectorsGa2O3photo‐to‐dark current ratio schottky junctionsolar‐blind photodetectors
spellingShingle Shiqi Yan
Teng Jiao
Zijian Ding
Xinyu Zhou
Xingqi Ji
Xin Dong
Jiawei Zhang
Qian Xin
Aimin Song
Ga2O3 Schottky Avalanche Solar‐Blind Photodiode with High Responsivity and Photo‐to‐Dark Current Ratio
Advanced Electronic Materials
avalanche photodetectors
Ga2O3
photo‐to‐dark current ratio 
schottky junction
solar‐blind photodetectors
title Ga2O3 Schottky Avalanche Solar‐Blind Photodiode with High Responsivity and Photo‐to‐Dark Current Ratio
title_full Ga2O3 Schottky Avalanche Solar‐Blind Photodiode with High Responsivity and Photo‐to‐Dark Current Ratio
title_fullStr Ga2O3 Schottky Avalanche Solar‐Blind Photodiode with High Responsivity and Photo‐to‐Dark Current Ratio
title_full_unstemmed Ga2O3 Schottky Avalanche Solar‐Blind Photodiode with High Responsivity and Photo‐to‐Dark Current Ratio
title_short Ga2O3 Schottky Avalanche Solar‐Blind Photodiode with High Responsivity and Photo‐to‐Dark Current Ratio
title_sort ga2o3 schottky avalanche solar blind photodiode with high responsivity and photo to dark current ratio
topic avalanche photodetectors
Ga2O3
photo‐to‐dark current ratio 
schottky junction
solar‐blind photodetectors
url https://doi.org/10.1002/aelm.202300297
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