| Solar-blind ultraviolet photoelectric detectors have great potential applications in military and civil fields such as national defense early warning,tail flame guidance,space exploration,security communication,fire alarm,environmental monitoring,ultraviolet radiation detection,and defogging navigation,and have received extensive attention in recent years.Gallium oxide(Ga2O3),a new ultra-wide bandgap semiconductor material with a bandgap width of 4.2-5.1 e V,has a photoresponse in the entire solar blind deep ultraviolet region(200-280 nm),and has the advantages of high atomic shift threshold energy,strong radiation resistance,and good chemical and physical stability.It is an optimal material for the preparation of solar blind ultraviolet photodetectors.Due to the shortage of traditional energy,detectors are increasingly tending to be energy-saving,efficient and miniaturized.Self-powered detectors can work by themselves without external voltage,so detectors with self-powered performance begin to emerge.Ti3C2Tx is a newly discovered graphene-like two-dimensional material with extremely high carrier mobility and excellent light transmission from deep ultraviolet to infrared spectral band.It is a transparent conductive electrode with excellent compatibility with photodetectors.Based on the high solar blind light detection efficiency of Ga2O3 and the high carrier transmission capacity of Ti3C2Tx,Schottky,phase junction and photochemical self-powered solar blind detectors are constructed to optimize and improve the solar blind photoelectric performance of the detectors.The physical mechanism of the detectors is analyzed in depth.The main results are as follows:1.Ti3C2Tx/β-Ga2O3 thin film Schottky self-powered solar blind detector.In view of the intrinsic defects of gallium oxide materials,which inevitably produce oxygen vacancies,plasma treatment is used to reduce the oxygen vacancies on the surface ofβ-Ga2O3 film to strengthen the Schottky potential barrier between Ti3C2Tx film andβ-Ga2O3film.The work function of Ti3C2Tx is large,and it is suitable to construct a Schottky solar blind detector withβ-Ga2O3.Without plasma treatment,the light-dark ratio of the detector is 4.6×103,the photoresponsiveness is 0.04 m A/W,and the response speed is 0.53 s/1.26s under the test condition of 254 nm UV light with 0 V bias and light intensity of 1000μW/cm2.The proportion of oxygen vacancies inβ-Ga2O3 films decreased from 44.5%to27.3%after treatment ofβ-Ga2O3 films with oxygen plasma.Under the same conditions,the light-dark ratio of the Ti3C2Tx/β-Ga2O3 film Schottky self-powered solar-blind detector is 2.7×104,which is 490%higher than that of the untreated one,and the photoresponsiveness is 0.26 m A/W,which is 550%higher than that of the untreated one.The light response speed was 83 ms/44 ms and 447 ms/1216 ms were accelerated.2.Ti3C2Tx/β-Ga2O3 nanocrystalline Schottky self-powered solar-blind photodetector.In view of the small specific surface area of Ga2O3 film and the existence of light reflection,which reduces the performance of the device,the vertical nanopilar structure is introduced to increase the effective light absorption area ofβ-Ga2O3.Theβ-Ga2O3nanocolumn array was prepared by hydrothermal growth of Ga OOH precursor,and the nanocolumn Schottky self-powered solar blind detector was constructed by using Ti3C2Txas the electrode.Ti3C2Tx was dispersed on the surface ofβ-Ga2O3 nanopularization,and Ag nanowires were used to connect the dispersed Ti3C2Tx into electrodes.The Ti3C2Tx/β-Ga2O3 self-powered solar blind detectors and Ag NWS-Ti3C2Tx/β-Ga2O3 self-powered solar blind detectors were constructed respectively.Compared with the Ti3C2Tx/β-Ga2O3 thin film Schottky solar blind detector,the photocurrent of Ti3C2Tx/β-Ga2O3self-powered solar blind detector reaches 200 n A under 254 nm UV light test conditions of 0 V bias and 1000μW/cm2,the photocurrent of Ti3C2Tx/β-Ga2O3 self-powered solar blind detector is increased by 199%.The light responsivity is 0.36 m A/W,which is increased by 38%.The performance of the Ag nanowire detector is further improved.Under the same test conditions,the photocurrent of the Ag NWs-Ti3C2Tx/β-Ga2O3vertical structure solar blind detector is 800%higher than that of the Ti3C2Tx/β-Ga2O3nanowire Shottky solar-blind detector at 1800n A.The light responsivity is improved by 870%to 3.5 m A/W.3.Ti3C2Tx/α/β-Ga2O3 nanocolumn Phase Junction self-powered solar blind detector.On the basis of the previous chapter,different phases of Ga2O3 nanopelms were prepared,and the phase junction structure was introduced to enhance the built-in electric field strength.The precursor of Ga OOH grown by hydrothermal method was prepared intoα-Ga2O3 after annealing.On the basis ofα-Ga2O3,α/β-Ga2O3 was prepared by rapid annealing.Ag NWs-Ti3C2Tx/α-Ga2o3 nanocrystal self-powered solar blind detector and Ag NWs-Ti3C2Tx/α/β-Ga2O3 nanocrystal phase-junction self-powered solar blind detector were constructed.The formation of the second type energy band at the phase junction interface can promote the rapid separation of photogenerated carriers.The photocurrent of the Ag NWs-Ti3C2Tx/α/β-Ga2O3 nanocolumn junction self-powered solar blind detector reaches 2.9μA,which is 1.1μA higher than that ofβ-Ga2O3 detector and2.88μA higher than that ofα-Ga2o3 detector.The responsiveness is up to 5.2 m A/W.4.Ti3C2Tx/α-Ga2O3 nanocrystalline photoelectrochemical self-powered solar blind detector.To fill the shortage ofα-Ga2O3 nanopilar detector in the previous chapter,a photochemical type photodetector is introduced.Photochemical(PEC)photodetectors are new self-powered photodetectors.Due to the special dynamic mechanism formed by solid-liquid contact between electrons and holes,directional electron movement will occur and electric current will be generated.The photochemical self-powered solar blind Ti3C2Tx/α-Ga2O3 nanocolumn detector was fabricated by drip-coating Ti3C2Tx onα-Ga2O3 nanocolumn.The photoresponsiveness of the detector to 254 nm light is 2.75m A/W at 0 V. |