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Fabrication And Performance Study Of Mixed Phase (InxGa1-x)2O3 Thin Film Solar-blind Photodetector

Posted on:2024-01-15Degree:MasterType:Thesis
Country:ChinaCandidate:K QiFull Text:PDF
GTID:2568307109483374Subject:Condensed matter physics
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In recent years,with the deep understanding of the solar-blind ultraviolet band(200-280 nm),its applicability has gradually received attention,including in the military and civil fields such as flame warning,missile detection,medical analysis,digital imaging,etc.This also leads to the vigorous development of solar-blind ultraviolet band photodetector.The working mechanism of a solar-blind ultraviolet photodetector(PD)is to convert the light signal into an electrical signal for qualitative or quantitative monitoring.Ultrawide band gap semiconductors are considered to be the preferred materials for the preparation of solar-blind PD.The ultrawide band gap corresponds to the absorption edge located in the solar-blind ultraviolet band,which can avoid interference caused by absorption signals from other bands.Among them,gallium oxide has~4.9 eV ultra-wide band gap,many crystal structures,large dielectric constant,high breakdown field strength,excellent chemical and thermal stability,and is one of the ideal materials for the preparation of the solar-blind PD.Due to the fact that ternary compounds can improve the stability of materials,increase their versatility,and extend their service life,the(InxGa1-x)2O3(0<x<1)mixed-phase film similar to MgxZn1-xO and AlxGa1-xN ternary compound semiconductors was prepared,and then the Metal-Semiconductor-Metal(MSM)structured photoconductive solar-blind photodetector was prepared based on this film.To further improve the performance,annealing and lattice mismatch reduction were performed.The specific research contents are as follows:(1)(InxGa1-x)2O3 thin film preparation and characterization:In this paper,chemical vapor deposition(CVD)was used to fabricate(InxGa1-x)2O3 thin films on a quartz substrate,argon(Ar)as the carrier gas,oxygen(O2)as reaction gas at 1080℃.The morphology,composition,structure,optical properties,and electrical properties of(InxGa1-x)2O3 thin films were analyzed.The results show that(InxGa1-x)2O3 mixed-phase films with different Ga:In atomic ratios have been prepared.In addition,the(InxGa1-x)2O3 mixed-phase films at all ratios are in ohmic contact with the golden interdigital electrodes.The high-quality,different proportions(InxGa1-x)2O3 mixed-phase thin films prepared in this chapter lay a good foundation for subsequent device preparation and further optimization.(2)(InxGa1-x)2O3 mixed-phase thin film solar-blind ultraviolet photodetector construction and optimization:Preparation of MSM structure ultraviolet photodetector based on different Ga:In atom ratio(InxGa1-x)2O3 mixed-phase thin film.Comparisons show that the optimum device dark current is as low as 10-12A,due to the grain boundary between In2O3 and Ga2O3capturing electrons to form barriers that impede electron transport.In order to improve the performance of(InxGa1-x)2O3 mixed-phase film PD,post-annealing was studied.The device responsiveness is 1000 times higher than that of the unannealed device,but the recovery time is longer due to the higher oxygen vacancy concentration in the(InxGa1-x)2O3 mixed-phase film after air annealing.(3)Preparation and performance test of solar-blind ultraviolet photodetector based on the(InxGa1-x)2O3 mixed-phase film grow on sapphire substrate:We substituted quartz substrate for c-Al2O3 substrate with a smaller lattice mismatch,and found that Ga2O3 in the film grows along the(-201)orientation,which greatly improves the quality of the film.The samples with the higher In2O3 content in the precursor also grow In2O3 micron lines.Optimal performance(InxGa1-x)2O3 mixed film(In:6.27 at%)photodetector shows an ultralow dark current of0.2 p A and a large I254 nm/Idark up to 4.27×106,with a prominent responsivity(1 A/W,254 nm)and a remarkable detectivity(4.62×1014 Jones)under 10 V bias.And it also shows a high internal gain(488.83%)and faster response(response time:2.81 s;recovery time:0.26 s).All properties are significantly better than those of devices on quartz substrates,which is attributed to the greatly improved film growth quality after reducing the lattice mismatch on the substrates.In summary,it can be seen that(InxGa1-x)2O3 material has great potential and research value in the field of ultraviolet photodetection.
Keywords/Search Tags:Ga2O3, Mixed-phase (InxGa1-x)2O3, In2O3, Solar-blind ultraviolet photodetector, Heterojunction
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