CN109449219A - Based on β-Ga2O3The solar blind ultraviolet detector of monocrystalline grade thin slice - Google Patents

Based on β-Ga2O3The solar blind ultraviolet detector of monocrystalline grade thin slice Download PDF

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Publication number
CN109449219A
CN109449219A CN201811096590.7A CN201811096590A CN109449219A CN 109449219 A CN109449219 A CN 109449219A CN 201811096590 A CN201811096590 A CN 201811096590A CN 109449219 A CN109449219 A CN 109449219A
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monocrystalline
thin slice
solar blind
ultraviolet detector
blind ultraviolet
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郭道友
黄亚磊
李培刚
唐为华
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Beijing Gallium Science And Technology Co Ltd
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Beijing Gallium Science And Technology Co Ltd
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    • H01LSEMICONDUCTOR DEVICES NOT COVERED BY CLASS H10
    • H01L31/00Semiconductor devices sensitive to infrared radiation, light, electromagnetic radiation of shorter wavelength or corpuscular radiation and specially adapted either for the conversion of the energy of such radiation into electrical energy or for the control of electrical energy by such radiation; Processes or apparatus specially adapted for the manufacture or treatment thereof or of parts thereof; Details thereof
    • H01L31/08Semiconductor devices sensitive to infrared radiation, light, electromagnetic radiation of shorter wavelength or corpuscular radiation and specially adapted either for the conversion of the energy of such radiation into electrical energy or for the control of electrical energy by such radiation; Processes or apparatus specially adapted for the manufacture or treatment thereof or of parts thereof; Details thereof in which radiation controls flow of current through the device, e.g. photoresistors
    • H01L31/09Devices sensitive to infrared, visible or ultraviolet radiation
    • HELECTRICITY
    • H01ELECTRIC ELEMENTS
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    • H01L31/00Semiconductor devices sensitive to infrared radiation, light, electromagnetic radiation of shorter wavelength or corpuscular radiation and specially adapted either for the conversion of the energy of such radiation into electrical energy or for the control of electrical energy by such radiation; Processes or apparatus specially adapted for the manufacture or treatment thereof or of parts thereof; Details thereof
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    • H01L31/0224Electrodes
    • HELECTRICITY
    • H01ELECTRIC ELEMENTS
    • H01LSEMICONDUCTOR DEVICES NOT COVERED BY CLASS H10
    • H01L31/00Semiconductor devices sensitive to infrared radiation, light, electromagnetic radiation of shorter wavelength or corpuscular radiation and specially adapted either for the conversion of the energy of such radiation into electrical energy or for the control of electrical energy by such radiation; Processes or apparatus specially adapted for the manufacture or treatment thereof or of parts thereof; Details thereof
    • H01L31/0248Semiconductor devices sensitive to infrared radiation, light, electromagnetic radiation of shorter wavelength or corpuscular radiation and specially adapted either for the conversion of the energy of such radiation into electrical energy or for the control of electrical energy by such radiation; Processes or apparatus specially adapted for the manufacture or treatment thereof or of parts thereof; Details thereof characterised by their semiconductor bodies
    • H01L31/0256Semiconductor devices sensitive to infrared radiation, light, electromagnetic radiation of shorter wavelength or corpuscular radiation and specially adapted either for the conversion of the energy of such radiation into electrical energy or for the control of electrical energy by such radiation; Processes or apparatus specially adapted for the manufacture or treatment thereof or of parts thereof; Details thereof characterised by their semiconductor bodies characterised by the material
    • H01L31/0264Inorganic materials
    • H01L31/032Inorganic materials including, apart from doping materials or other impurities, only compounds not provided for in groups H01L31/0272 - H01L31/0312
    • HELECTRICITY
    • H01ELECTRIC ELEMENTS
    • H01LSEMICONDUCTOR DEVICES NOT COVERED BY CLASS H10
    • H01L31/00Semiconductor devices sensitive to infrared radiation, light, electromagnetic radiation of shorter wavelength or corpuscular radiation and specially adapted either for the conversion of the energy of such radiation into electrical energy or for the control of electrical energy by such radiation; Processes or apparatus specially adapted for the manufacture or treatment thereof or of parts thereof; Details thereof
    • H01L31/0248Semiconductor devices sensitive to infrared radiation, light, electromagnetic radiation of shorter wavelength or corpuscular radiation and specially adapted either for the conversion of the energy of such radiation into electrical energy or for the control of electrical energy by such radiation; Processes or apparatus specially adapted for the manufacture or treatment thereof or of parts thereof; Details thereof characterised by their semiconductor bodies
    • H01L31/036Semiconductor devices sensitive to infrared radiation, light, electromagnetic radiation of shorter wavelength or corpuscular radiation and specially adapted either for the conversion of the energy of such radiation into electrical energy or for the control of electrical energy by such radiation; Processes or apparatus specially adapted for the manufacture or treatment thereof or of parts thereof; Details thereof characterised by their semiconductor bodies characterised by their crystalline structure or particular orientation of the crystalline planes
    • H01L31/0392Semiconductor devices sensitive to infrared radiation, light, electromagnetic radiation of shorter wavelength or corpuscular radiation and specially adapted either for the conversion of the energy of such radiation into electrical energy or for the control of electrical energy by such radiation; Processes or apparatus specially adapted for the manufacture or treatment thereof or of parts thereof; Details thereof characterised by their semiconductor bodies characterised by their crystalline structure or particular orientation of the crystalline planes including thin films deposited on metallic or insulating substrates ; characterised by specific substrate materials or substrate features or by the presence of intermediate layers, e.g. barrier layers, on the substrate
    • HELECTRICITY
    • H01ELECTRIC ELEMENTS
    • H01LSEMICONDUCTOR DEVICES NOT COVERED BY CLASS H10
    • H01L31/00Semiconductor devices sensitive to infrared radiation, light, electromagnetic radiation of shorter wavelength or corpuscular radiation and specially adapted either for the conversion of the energy of such radiation into electrical energy or for the control of electrical energy by such radiation; Processes or apparatus specially adapted for the manufacture or treatment thereof or of parts thereof; Details thereof
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Abstract

The present invention provides a kind of based on β-Ga2O3The solar blind ultraviolet detector of monocrystalline grade thin slice, by β-Ga2O3Monocrystalline grade thin slice and electrode constitute Ohmic contact, and light absorbing layer is the β-Ga of monocrystalline2O3Mm band, the electrode are that one of titanium, gold, silver, platinum or multiple material are constituted.The present invention also proposes described based on β-Ga2O3The preparation method and application of the solar blind ultraviolet detector of monocrystalline grade thin slice.The invention proposes one kind to be based on β-Ga2O3The solar blind ultraviolet detector of monocrystalline grade thin slice, the detector have the characteristics that Ohmic contact and compared with high-responsivities.The method that the present invention is by mechanically pulling off obtains β-Ga2O3Lamella grows Ti/Au electrode using magnetically controlled sputter method, and to form solar blind ultraviolet detector, device obtained has many advantages, such as high Light To Dark Ratio, fast response time.

Description

Based on β-Ga2O3The solar blind ultraviolet detector of monocrystalline grade thin slice
Technical field
The invention belongs to optical technical fields, and in particular to one kind is based on β-Ga2O3Solar blind ultraviolet detector.
Background technique
Due to the absorption of ozone layer, the deep ultraviolet light that wavelength is 200-280nm, the light of the wave band there's almost no in earth's surface Referred to as solar blind UV, and it is referred to as day blind ultraviolet detection for the signal detection of the wave band.Due to not by sunlight background Influence, solar blind ultraviolet light signal detectivity is high, and accuracy rate is high, it is military and in terms of have it is extensive Using Ultraviolet Communication especially day, blind Ultraviolet Communication just like had become the highest priority of various countries' military affairs contest.In addition to blind in day Except application in Ultraviolet Communication, there are also the applications of other aspects for solar blind UV electric explorer, such as national defence early warning and tracking, life The science of life, the detection of high-voltage line corona, ozone layer, detection of gas and analysis, flame sensing etc..
Ultraviolet detector currently on the market is vacuum ultraviolet detector part, compares it, the solid-state based on semiconductor material Ultraviolet detector is increasingly becoming scientific research people since weight is small, low in energy consumption, quantum efficiency is high, is convenient for the features such as integrated in recent years The research hotspot of member.The forbidden bandwidth of solar blind ultraviolet detector core semiconductor material is often greater than 4.4eV, studies ratio at present More material concentrates on AlGaN, ZnMgO and diamond.But AlGaN is since its film needs very high temperature to grow and is difficult to outer Prolong film forming, ZnMgO is difficult to remain above the band gap of 4.5eV under the structure of mono-crystlling fibre zinc ore, and diamond has fixed The band gap of 5.5eV, corresponding wavelength 225nm only occupy the sub-fraction of day blind ultraviolet wavelength.And β-Ga2O3Forbidden bandwidth be about 4.9eV, corresponding wavelength 253nm, and be easy to and Al2O3And In2O3It forms continuous solid solution and realizes its covering completely in day-old chick Lid, is a kind of oxide semiconductor candidate material for being very suitable for preparing solar blind UV electric explorer.And grope to be easy to make β-Ga standby, best in quality2O3Solar blind ultraviolet detector technology is completely new challenge and opportunity that field of semiconductor materials faces.
Summary of the invention
Place in view of the shortcomings of the prior art, the purpose of the present invention is to provide a kind of formation Ohmic contact, can visit Survey day-old chick ultraviolet light based on β-Ga2O3The solar blind ultraviolet detector of monocrystalline grade thin slice.
Another object of the present invention is that proposition is described based on β-Ga2O3The solar blind ultraviolet detector of monocrystalline grade thin slice Preparation method.
Third object of the present invention is to propose the application of the solar blind ultraviolet detector.
Realize the technical solution of above-mentioned purpose of the present invention are as follows:
One kind being based on β-Ga2O3The solar blind ultraviolet detector of monocrystalline grade thin slice, by β-Ga2O3Monocrystalline grade thin slice Ohmic contact is constituted with electrode, light absorbing layer is the β-Ga of monocrystalline2O3Mm band, the electrode are one of titanium, gold, silver, platinum Or multiple material is constituted.
Wherein, the β-Ga2O3The width range of monocrystalline grade thin slice be 0.5~10mm, thickness range be 0.02~ 0.2mm。
Wherein, the electrode is strip shaped electric poles, and the width range of electrode is 0.05~0.5mm, thickness range is 25~ 230nm。
A preferred technical solution of the present invention is that the electrode is that titanium coating and gold metal layer are constituted;It is highly preferred that The thickness range of titanium coating is 5~30nm, and the thickness range of gold metal layer is 20~200nm.
It is of the present invention to be based on β-Ga2O3The preparation method of the solar blind ultraviolet detector of monocrystalline grade thin slice, including step It is rapid:
(1) use mechanical stripping method, the β-Ga for floating zone method being grown with adhesive tape2O3Monocrystalline carries out bonding removing, transfer Onto substrate, maintains adhesive tape to be sticked on substrate and remove adhesive tape after 10~50h;
(2) β-Ga obtained by organic solvent cleaning step (1)2O3Lamella, it is dry;
(3) β-Ga for obtaining step (2)2O3The mask plate shielding of lamella hollow out, is prepared using magnetically controlled sputter method Electrode.
Substrate need to be insulating materials.A kind of optimal technical scheme is provided herein are as follows:
The substrate is one of glass slide, glass plate, sapphire, and controlling between adhesive tape and substrate does not have bubble.Glue Between band and glass slide cannot there are bubbles, otherwise cannot get complete β-Ga2O3Lamella.
A preferred technical solution of the present invention is, in step (1), after adhesive tape glues on substrate, to adhesive tape position Apply 10~1500g/cm2Pressure, maintain 10~50h.
For example, the one side of adhesive tape is horizontally arranged upward, a weight is set on adhesive tape, weight range is 10~ 200g keeps horizontal.
Wherein, in step (2), the organic solvent be one of acetone, ethyl alcohol, ethylene glycol, n-hexane or a variety of, clearly The mode washed are as follows: infiltrate the β-Ga with organic solvent2O3Lamella 5~15 minutes.
It is highly preferred that successively sputtering titanium coating and gold metal layer in step (3), titanium coating and gold metal layer are obtained Constitute the strip shaped electric poles of (Au/Ti), sputtering technology condition are as follows: back end vacuum range is 1 × 10-5~5 × 10-4Pa, underlayer temperature For room temperature, operating air pressure range is 0.1~1.0Pa, and sputtering power range is 20~80W.
Optionally, in sputtering technology, work atmosphere is Ar gas.The sputtering time of titanium coating and gold metal layer depends on gold Belong to the thickness of layer, for example, Ti layers of sputtering time is 5~60s, Au layers of sputtering time is 20~200s.
The application of solar blind ultraviolet detector of the present invention, which is characterized in that the day for detecting 200-280nm wavelength is blind Ultraviolet light.
The beneficial effects of the present invention are:
The invention proposes one kind to be based on β-Ga2O3The solar blind ultraviolet detector of monocrystalline grade thin slice, the detector have Ohmic contact and the characteristics of compared with high-responsivity.This detector technology is β-Ga2O3The application of solar blind UV electric explorer provides reason By and technical support.
The method that the present invention is by mechanically pulling off obtains β-Ga2O3Lamella, using magnetically controlled sputter method growth Ti/Au electricity Pole, to form solar blind ultraviolet detector, which has the characteristics that high Light To Dark Ratio, fast response time.β-Ga in the present invention2O3It is thin The preparation of lamella uses mechanical stripping method, and passes through commercialized magnetron sputtering depositing Ti/Au metal layer and β-Ga2O3It is formed Ohmic contact.Preparation method is easy to operate, at low cost, reproducible, before following photoelectric field centainly has huge application Scape.
Detailed description of the invention
Fig. 1 is the β-Ga made from the method for the present invention2O3Grade thin slice solar blind ultraviolet detector structural schematic diagram;
Fig. 2 is I-V curve figure under dark situations;
Fig. 3 is the β-Ga made from the method for the present invention2O3Grade thin slice solar blind ultraviolet detector is at dark and 254nm I-V curve comparison diagram;
Fig. 4 is the β-Ga made from the method for the present invention2O3Grade thin slice solar blind ultraviolet detector is in 15V bias and light intensity For 400 μ W/cm2254nm illumination under I-t curve (3 circulation);
Fig. 5 is the β-Ga made from the method for the present invention2O3Grade thin slice solar blind ultraviolet detector is in 15V bias and light intensity For 400 μ W/cm2254nm illumination under I-t curve magnification figure and the response time fitting.
Specific embodiment
The following examples are used to illustrate the present invention, but are not intended to limit the scope of the present invention..
In embodiment, β-Ga used2O3Monocrystalline is floating zone method preparation.
Unless otherwise specified, means used in the examples are this field conventional technology.
Embodiment 1
Using mechanical stripping method, the β-Ga for being prepared floating zone method using adhesive tape2O3Monocrystalline carries out bonding removing, will glue There is β-Ga2O3Lamellose adhesive tape adheres on clean glass slide, between adhesive tape and glass slide cannot there are bubbles, in glue after gluing A weight, about 50g or so are set on band, keep glass slide horizontal.
After placing for 24 hours at room temperature, adhesive tape is gently torn with tweezers, has just obtained β-Ga2O3Lamella.Pass through microexamination It is found that β-the Ga2O3Lamella length and width about 2 × 5mm, thickness 0.1mm.
It, can be with acetone to β-Ga to remove the included offset printing of adhesive tape2O3The net glass slide of lamella is cleaned, still Operation is centainly careful, and slightly infiltration a moment (5 minutes), places dry in a vacuum drying oven later.
By the β-Ga of above-mentioned preparation2O3The mask plate shielding of lamella hollow out, using the successive splash-proofing sputtering metal of magnetically controlled sputter method Ti layers (thickness about 30nm) and Au layers (thickness about 70nm), obtain the translucent Au/Ti electrode of strip of a wide 0.2mm.Sputtering Process conditions are as follows: back end vacuum is 1 × 10-4Pa, underlayer temperature are room temperature, and work atmosphere is Ar gas, and operating air pressure is 1.0Pa, the sputtering time that 45W, Ti layers of sputtering power are 1min, and Au layers of sputtering time is 3min.
β-Ga can be prepared by above-mentioned experimentation2O3Solar blind ultraviolet detector, structure are as shown in Figure 1.The β- Ga2O3/ solar blind ultraviolet detector shows obvious ohmic contact characteristic under dark situations, as shown in Figure 2;This detector Under 254nm ultraviolet light, it is still shown as Ohmic contact, as shown in Figure 3.β-the Ga2O3Solar blind ultraviolet detector has Europe The characteristics of nurse contact and higher responsiveness.It is 400 μ W/cm that Fig. 4, which gives in 15V bias and light intensity,2254nm illumination under lead to It crosses continuous lamp and turns on light and close the I-t curve that measures, 3 I-t circulations are repeated in we, which shows good repeatability.? Under dark situations, the dark current of the detector is~1.8 × 10-9A, when light intensity is 400 μ W/cm2254nm ultraviolet light Afterwards, electric current is rapidly increased to~2.8 × 10-7A, Light To Dark Ratio Iphoto/Idark≈156.By being further fitted, we learn this Detector is 400 μ W/cm in 15V bias and light intensity2254nm illumination under rising response time τ r and die-away time τ d difference For 0.64s and 0.16s, as shown in Figure 5.
Embodiment 2
Using mechanical stripping method, the β-Ga for being prepared floating zone method using adhesive tape2O3Monocrystalline carries out bonding removing, will glue There is β-Ga2O3Lamellose adhesive tape adheres on clean glass slide, between adhesive tape and glass slide cannot there are bubbles, in glue after gluing A weight, about 50g or so are set on band, keep glass slide horizontal.
After placing for 24 hours at room temperature, adhesive tape is gently torn with tweezers, has just obtained β-Ga2O3Lamella.Pass through microexamination It is found that β-the Ga2O3Lamella length and width about 1 × 5mm, thickness 0.15mm.
It, can be with acetone to β-Ga to remove the included offset printing of adhesive tape2O3The net glass slide of lamella is cleaned, still Operation is centainly careful, and slightly infiltration a moment (10 minutes), places dry in a vacuum drying oven later.
By the β-Ga of above-mentioned preparation2O3The mask plate shielding of lamella hollow out, using the successive splash-proofing sputtering metal of magnetically controlled sputter method Ti layers (thickness about 30nm) and Au layers (thickness about 100nm), obtain the translucent Au/Ti electrode of strip of a wide 0.3mm.Sputtering Process conditions are as follows: back end vacuum is 1 × 10-4Pa, underlayer temperature are room temperature, and work atmosphere is Ar gas, and operating air pressure is 1.0Pa, the sputtering time that 45W, Ti layers of sputtering power are 1min, and Au layers of sputtering time is 4min.
Embodiment 3
Using mechanical stripping method, the β-Ga for being prepared floating zone method using adhesive tape2O3Monocrystalline carries out bonding removing, will glue There is β-Ga2O3Lamellose adhesive tape adheres on clean glass slide, between adhesive tape and glass slide cannot there are bubbles, in glue after gluing A weight, about 50g or so are set on band, keep glass slide horizontal.
After placing for 24 hours at room temperature, adhesive tape is gently torn with tweezers, has just obtained β-Ga2O3Lamella.Pass through microexamination It is found that β-the Ga2O3Lamella length and width about 2 × 2mm, thickness 0.2mm.
It, can be with acetone to β-Ga to remove the included offset printing of adhesive tape2O3The net glass slide of lamella is cleaned, still Operation is centainly careful, and slightly infiltration a moment (5 minutes), places dry in a vacuum drying oven later.
By the β-Ga of above-mentioned preparation2O3The mask plate shielding of lamella hollow out, using the successive splash-proofing sputtering metal of magnetically controlled sputter method Ti layers (thickness about 20nm) and Au layers (thickness about 50nm), obtain the translucent Au/Ti electrode of strip of a wide 0.3mm.Sputtering Process conditions are as follows: back end vacuum is 1 × 10-4Pa, underlayer temperature are room temperature, and work atmosphere is Ar gas, and operating air pressure is 1.0Pa, the sputtering time that 45W, Ti layers of sputtering power are 40s, and Au layers of sputtering time is 2min.
Embodiment that is disclosed above or requiring can be produced in the range of being no more than existing disclosed laboratory facilities or Implement.All products and/or method described in the preferred embodiment of the present invention expressly refer to that those do not violate the present invention Concept, scope and spirit can be used for the product and/or experimental method and following step.To in the technique All changes and improvement of technological means, belong to concept, the scope and spirit that the claims in the present invention define.

Claims (10)

1. one kind is based on β-Ga2O3The solar blind ultraviolet detector of monocrystalline grade thin slice, which is characterized in that by β-Ga2O3Monocrystalline milli Meter level thin slice and electrode constitute Ohmic contact, and light absorbing layer is the β-Ga of monocrystalline2O3Mm band, the electrode are titanium, gold, silver, platinum One of or multiple material constitute.
2. according to claim 1 be based on β-Ga2O3The solar blind ultraviolet detector of monocrystalline grade thin slice, which is characterized in that β-the Ga2O3The width range of monocrystalline grade thin slice is 0.5~10mm, and thickness range is 0.02~0.2mm.
3. according to claim 1 be based on β-Ga2O3The solar blind ultraviolet detector of monocrystalline grade thin slice, which is characterized in that The electrode is strip shaped electric poles, and the width range of electrode is 0.05~0.5mm, and thickness range is 25~230nm.
4. described in any item according to claim 1~3 be based on β-Ga2O3The solar blind ultraviolet detector of monocrystalline grade thin slice, It is characterized in that, the electrode is that titanium coating and gold metal layer are constituted;Preferably, the thickness range of titanium coating is 5~30nm, The thickness range of gold metal layer is 20~200nm.
5. being based on β-Ga described in any one of Claims 1 to 42O3The preparation side of the solar blind ultraviolet detector of monocrystalline grade thin slice Method characterized by comprising
(1) use mechanical stripping method, the β-Ga for floating zone method being grown with adhesive tape2O3Monocrystalline carries out bonding removing, is transferred to base On piece maintains adhesive tape to be sticked on substrate and removes adhesive tape after 10~50h;
(2) β-Ga obtained by organic solvent cleaning step (1)2O3Lamella, it is dry;
(3) β-Ga for obtaining step (2)2O3The mask plate shielding of lamella hollow out prepares electricity using magnetically controlled sputter method Pole.
6. preparation method according to claim 5, which is characterized in that the substrate is glass slide, in glass plate, sapphire One kind, controlling between adhesive tape and substrate does not have bubble.
7. preparation method according to claim 5, which is characterized in that in step (1), after adhesive tape glues on substrate, to Adhesive tape position applies 10~1500g/cm2Pressure, maintain 10~50h.
8. preparation method according to claim 5, which is characterized in that in step (2), the organic solvent is acetone, second One of alcohol, ethylene glycol, n-hexane are a variety of, the mode of cleaning are as follows: infiltrate the β-Ga with organic solvent2O3Lamella 5~ 15 minutes.
9. preparation method according to claim 5, which is characterized in that in step (3), successively sputter titanium coating and Jin Jin Belong to layer, obtain the strip shaped electric poles that titanium coating and gold metal layer are constituted, sputtering technology condition are as follows: back end vacuum range is 1 × 10-5 ~5 × 10-4Pa, underlayer temperature are room temperature, and operating air pressure range is 0.1~1.0Pa, and sputtering power range is 20~80W.
10. the application of any one of Claims 1 to 4 solar blind ultraviolet detector, which is characterized in that for detecting 200- The solar blind UV of 280nm wavelength.
CN201811096590.7A 2018-09-19 2018-09-19 Based on β-Ga2O3The solar blind ultraviolet detector of monocrystalline grade thin slice Pending CN109449219A (en)

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CN110061089A (en) * 2019-03-18 2019-07-26 北京镓族科技有限公司 The method that sapphire miscut substrate optimizes the growth of gallium oxide film and solar blind ultraviolet detector performance
CN110061089B (en) * 2019-03-18 2022-06-07 北京铭镓半导体有限公司 Method for optimizing gallium oxide film growth and solar blind ultraviolet detector performance by sapphire beveled substrate
CN109980053A (en) * 2019-03-27 2019-07-05 深圳市思坦科技有限公司 A kind of electrode preparation method and light emitting diode
CN110676352A (en) * 2019-09-22 2020-01-10 太原理工大学 Sn doped beta-Ga2O3Film and preparation method of solar blind ultraviolet detector thereof
CN111463299A (en) * 2020-04-17 2020-07-28 中国科学院半导体研究所 Direct detector based on gallium oxide solar blind ultraviolet polarized light and polarization imaging device
CN113380906A (en) * 2021-05-26 2021-09-10 浙江大学 Transparent ultraviolet photoelectric detector based on metal-semiconductor-metal structure
CN114597281A (en) * 2022-02-26 2022-06-07 太原理工大学 Doped with beta-Ga2O3And preparation method of ultraviolet detector of P-type diamond
CN114597281B (en) * 2022-02-26 2024-01-30 太原理工大学 beta-Ga doped 2 O 3 And method for preparing ultraviolet detector of P-type diamond

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