| Ultraviolet(UV)detectors have attracted much attention because of their wide application in military and civilian fields.According to different detection wavebands,UV detectors can be divided into visible-blind UV detectors and solar-blind UV detectors.Ga2O3 is a wide bandgap semiconductor material widely used in the solar-blind UV detection field.However,the bandgap of undoped Ga2O3 is too large(the common structure is about 4.9 e V),which makes Ga2O3 detectors difficult to detect the whole solar-blind UV region and easy to cause signal loss.(InxGa1-x)2O3is a ternary wide bandgap semiconductor material obtained by In element doping Ga2O3.With the increase of In content,the bandgap of(InxGa1-x)2O3 can be adjusted continuously from 3.7 e V-4.9 e V,which effectively solves the problem faced by Ga2O3.However,at present,the application of In doping in the field of Ga2O3 solar-blind UV detection is far from extensive,partly due to the insufficient research on material preparation,the controversial mechanism of In doping on the photoelectric performance of detectors,and the lack of design and performance research of heterojunction self-powered detectors.Based on the above problems,the main research contents of this dissertation are as follows:(InxGa1-x)2O3 films were prepared on sapphire substrates by magnetron sputtering.The effects of sputtering pressure and annealing temperature on the structural and optical properties of(InxGa1-x)2O3 films were investigated.As the sputtering pressure increased,the VO concentration decreased and the sputtering particle energy reduced,leading to the grain size of(InxGa1-x)2O3 films increasing first and then nearly invariant and then decreasing.The decrease of VO concentration also leads to the increase of optical bandgaps and the ratio of intensity with a green light to blue light emission.After annealing treatment,(InxGa1-x)2O3 films grown at room temperature were transformed from an amorphous structure to a polycrystalline structure.The increment of annealing temperature increased the particle size of the films,but they also produced non-(2?01)-oriented particles,leading to the poor preferred orientation.The increase of the annealing temperature also decreased the In content and the compressive stress,which caused the increase of the optical bandgaps.(InxGa1-x)2O3 films grown at high temperature were polycrystalline structures.The increment of annealing temperature increased the grain size of(InxGa1-x)2O3 films.But if the annealing temperature was too high,the grain size decreased,or the homogeneity deteriorated.Considering the grain size and uniformity of the(InxGa1-x)2O3 films grown at high temperature,800°C is the best annealing temperature.The effects of In content on the structural and optical properties of(InxGa1-x)2O3films were investigated.With the increase of In content,the crystal structure of(InxGa1-x)2O3 films was gradually transformed from a monoclinic phase to a mix-phase in which the bixbyite phase and the monoclinic phase coexisted until a bixbyite phase was formed.Due to the differences in the substitutional impurities,the increase of In content led to the decrease of the grain size of monoclinic structure(InxGa1-x)2O3 films,and the increase of the grain size of bixbyite phase(InxGa1-x)2O3 films.The optical bandgaps of(InxGa1-x)2O3 films decreased linearly with the increase of In content.MSM structure detectors based on(InxGa1-x)2O3 films were fabricated.The influence of In content on photoelectric performance of(InxGa1-x)2O3 film detectors was discussed.It was found that monoclinic(InxGa1-x)2O3 film detectors had excellent solar-blind UV detection performance,and In doping could regulate the responsivity of monoclinic(InxGa1-x)2O3 film detectors by changing the grain size.The(In0.23Ga0.77)2O3/(In0.67Ga0.33)2O3 heterojunction self-powered solar-blind UV detector was fabricated by adjusting the energy band structure of(InxGa1-x)2O3films with In element.At zero bias,the responsivity of the detector was 5.78 m A/W,and the detectivity was 1.69×1011 cm Hz1/2 W-1,which had excellent self-powered detection performance.The(In0.23Ga0.77)2O3/(In0.67Ga0.33)2O3 heterojunction detector also had excellent solar-blind UV spectral selectivity due to the inhibition effect of the high carrier concentration of the(In0.67Ga0.33)2O3 film on the internal electric field width.This detector provided a new idea for the design of self-powered solar-blind UV detectors based on(InxGa1-x)2O3 heterojunction.In addition,the influence of the thickness of the Au electrodes and(In0.23Ga0.77)2O3 films on the responsivity of the heterojunction detectors was also investigated.The optimal thickness of the Au electrodes and the(In0.23Ga0.77)2O3 films was determined as 12.9 nm and 350 nm.The FTO/(In0.23Ga0.77)2O3/Spiro-Me OTAD organic-inorganic hybrid hetero-junction self-powered visible-blind UV detector was fabricated by the synergistic effect of(In0.23Ga0.77)2O3 and Spiro-Me OTAD films.The detector had excellent photoelectric detection performance from 200 nm to 400 nm.At zero bias,the responsivity of the detector was 0.63 m A/W,and the detectivity was 5.4×1010 cm Hz1/2 W-1.There was a double built-in electric field in the(In0.23Ga0.77)2O3 film,which promoted the separation and transmission of photogenerated electron-hole pairs,resulting in a fast response speed of the detector.The response time was only0.02 s.Moreover,the rejection ratio(R400/R450)of this detector was 125,indicating this detector had excellent UV-visible spectral selectivity.Finally,the resolution of solar-blind UV and non-solar-blind UV wavebands was successfully realized by using the“UV filtering”function of FTO,which provided a new idea for the design of wide-response self-powered visible-blind detectors with waveband resolution. |