CN117673188A - Self-driven solar blind ultraviolet detector based on asymmetric Schottky barrier - Google Patents

Self-driven solar blind ultraviolet detector based on asymmetric Schottky barrier Download PDF

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CN117673188A
CN117673188A CN202311653005.XA CN202311653005A CN117673188A CN 117673188 A CN117673188 A CN 117673188A CN 202311653005 A CN202311653005 A CN 202311653005A CN 117673188 A CN117673188 A CN 117673188A
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layer
self
ultraviolet detector
solar blind
blind ultraviolet
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杨国锋
谷燕
王博翔
陈华志
叶炳杰
谢峰
钱维莹
张向阳
张秀梅
刘玉申
陈国庆
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Jiangnan University
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    • 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
    • H01L31/08Semiconductor 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
    • H01L31/10Semiconductor 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 characterised by potential barriers, e.g. phototransistors
    • H01L31/101Devices sensitive to infrared, visible or ultraviolet radiation
    • H01L31/102Devices sensitive to infrared, visible or ultraviolet radiation characterised by only one potential barrier
    • H01L31/108Devices sensitive to infrared, visible or ultraviolet radiation characterised by only one potential barrier the potential barrier being of the Schottky type
    • H01L31/1085Devices sensitive to infrared, visible or ultraviolet radiation characterised by only one potential barrier the potential barrier being of the Schottky type the devices being of the Metal-Semiconductor-Metal [MSM] Schottky barrier type
    • 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
    • H01L31/0304Inorganic materials including, apart from doping materials or other impurities, only AIIIBV compounds
    • H01L31/03046Inorganic materials including, apart from doping materials or other impurities, only AIIIBV compounds including ternary or quaternary compounds, e.g. GaAlAs, InGaAs, InGaAsP
    • H01L31/03048Inorganic materials including, apart from doping materials or other impurities, only AIIIBV compounds including ternary or quaternary compounds, e.g. GaAlAs, InGaAs, InGaAsP comprising a nitride compounds, e.g. InGaN
    • 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
    • H01L31/18Processes or apparatus specially adapted for the manufacture or treatment of these devices or of parts thereof
    • H01L31/184Processes or apparatus specially adapted for the manufacture or treatment of these devices or of parts thereof the active layers comprising only AIIIBV compounds, e.g. GaAs, InP
    • H01L31/1844Processes or apparatus specially adapted for the manufacture or treatment of these devices or of parts thereof the active layers comprising only AIIIBV compounds, e.g. GaAs, InP comprising ternary or quaternary compounds, e.g. Ga Al As, In Ga As P
    • H01L31/1848Processes or apparatus specially adapted for the manufacture or treatment of these devices or of parts thereof the active layers comprising only AIIIBV compounds, e.g. GaAs, InP comprising ternary or quaternary compounds, e.g. Ga Al As, In Ga As P comprising nitride compounds, e.g. InGaN, InGaAlN
    • 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
    • H01L31/18Processes or apparatus specially adapted for the manufacture or treatment of these devices or of parts thereof
    • H01L31/184Processes or apparatus specially adapted for the manufacture or treatment of these devices or of parts thereof the active layers comprising only AIIIBV compounds, e.g. GaAs, InP
    • H01L31/1852Processes or apparatus specially adapted for the manufacture or treatment of these devices or of parts thereof the active layers comprising only AIIIBV compounds, e.g. GaAs, InP comprising a growth substrate not being an AIIIBV compound
    • YGENERAL TAGGING OF NEW TECHNOLOGICAL DEVELOPMENTS; GENERAL TAGGING OF CROSS-SECTIONAL TECHNOLOGIES SPANNING OVER SEVERAL SECTIONS OF THE IPC; TECHNICAL SUBJECTS COVERED BY FORMER USPC CROSS-REFERENCE ART COLLECTIONS [XRACs] AND DIGESTS
    • Y02TECHNOLOGIES OR APPLICATIONS FOR MITIGATION OR ADAPTATION AGAINST CLIMATE CHANGE
    • Y02PCLIMATE CHANGE MITIGATION TECHNOLOGIES IN THE PRODUCTION OR PROCESSING OF GOODS
    • Y02P70/00Climate change mitigation technologies in the production process for final industrial or consumer products
    • Y02P70/50Manufacturing or production processes characterised by the final manufactured product

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Abstract

The invention discloses a self-driven solar blind ultraviolet detector based on an asymmetric Schottky barrier, and belongs to the technical field of semiconductor device manufacturing. The ultraviolet detector comprises the following components in sequence from bottom to top: substrate layer, alN buffer layer, al 0.65 Ga 0.35 N layer, al 0.4 Ga 0.6 N active layer, al 0.55 Ga 0.45 An N barrier layer and a metal electrode layer. The invention uses the electrode and Al on one side only 0.4 Ga 0.6 Inserting Al between N active layers 0.55 Ga 0.45 The N barrier layer forms an asymmetric MSM structure, and different barrier heights are utilized to induce energy bands to bend, so that asymmetric energy bands are formed, separation and transportation of photogenerated carriers are obviously promoted, the problem of high power consumption of the detector with the symmetric MSM structure is solved, and the self-driving characteristic is realized. Formation ofIs an asymmetric heterostructure of (2) enhancing Al 0.4 Ga 0.6 The polarization field of the N layers is further increased, so that the generation of photocurrent is increased, and the responsiveness under 0V is greatly improved. In addition, the screw dislocation density of the epitaxial structure manufactured by the invention is lower, so that the device obtains ultra-low dark current, and the sensitivity of the device is improved.

Description

Self-driven solar blind ultraviolet detector based on asymmetric Schottky barrier
Technical Field
The invention relates to a self-driven solar blind ultraviolet detector based on an asymmetric Schottky barrier, and belongs to the technical field of semiconductor device manufacturing.
Background
To accommodate the rapid development of modern electronic information, optoelectronic devices are gradually evolving towards "miniaturization" and "integration". Therefore, developing a high-sensitivity, low-energy-consumption and high-response-speed ultraviolet detector is a core of future development in the field. Furthermore, the construction of a self-driven ultraviolet photoelectric detector which can work continuously and does not need an external power supply has become an important research point in the field of photoelectric detection. From the application point of view, the self-driven ultraviolet detector has the special advantages of low energy consumption, energy conservation, environmental protection, small device size, suitability for use under extreme conditions and the like, and is very popular in the fields of forest fire prevention, submarine petroleum leakage monitoring and the like.
Wide band gap semiconductor material Al x Ga 1-x N has adjustable band gap, intrinsic solar blind property, high temperature resistance and excellent chemical and physical stability. In addition, al x Ga 1-x The polarization characteristic of N helps to form a highly conductive two-dimensional electron gas (2 DEG) at the heterojunction interface, thereby improving device performance. In view of these significant advantages, alGaN has become an ideal material for developing high performance ultraviolet detectors. So far, most AlGaN-based ultraviolet detectors adopt an MSM structure due to the advantages of simple and controllable manufacturing process, strong plane integration capability, low noise, high detection rate and the like. Whereas conventional MSM structures use the same metal/semiconductor schottky contact to form symmetric electrodes, resulting in mirror symmetry of the schottky barrier formed across the metal/semiconductor contact. In this case, the photo-generated electrons/holes in the AlGaN semiconductor layer have no preferential drift direction. In other words, although these symmetrical AlGaN-based MSM structure uv detectors have achieved very high photodetection performance, they mostly require an external bias voltage to drive operation, facilitating the separation and transport of photogenerated electron-hole pairs. These external power sources not only add to the complexity of the circuit design and processing costs of the ultraviolet detection system, but also limit their use in particular environments and conditions.
In order to realize self-driving of the ultraviolet detector with the AlGaN-based MSM structure, namely, the ultraviolet detector can be driven to work under zero bias voltage, the common practice is to design an asymmetric structure and obtain an asymmetric Schottky barrier. While it is common practice to implement an asymmetric schottky barrier to deposit different metal contacts at both ends of the device, including using different metal materials and changing the contact area of the metal electrodes. However, the method is unfavorable for flexibility and wear resistance of the device, has the defects of high cost, limited work function difference of Schottky metal and the like, prevents further improvement of asymmetric Schottky barrier and further improvement of device performance, and mainly has low response and detection rate at zero bias because the photocurrent of the device at zero bias voltage is smaller.
Disclosure of Invention
In order to solve the problems of high energy consumption and low sensitivity of the existing AlGaN-based MSM structure ultraviolet detector, the invention provides a self-driven solar blind ultraviolet detector based on an asymmetric Schottky barrier, which is formed by a metal electrode at one sideWith Al 0.4 Ga 0.6 Inserting Al between N active layers 0.55 Ga 0.45 An N barrier layer for forming asymmetric Al with polarization effect 0.55 Ga 0.45 N/Al 0.4 Ga 0.6 N/Al 0.65 Ga 0.35 N heterostructure builds an asymmetric MSM structure, thereby realizing a self-driven AlGaN-based MSM solar blind ultraviolet detector, and because Al with polarization enhancement effect is designed 0.55 Ga 0.45 N/Al 0.4 Ga 0.6 N/Al 0.65 Ga 0.55 N epitaxial structure with enhanced absorption layer Al by controlling polarization 0.4 Ga 0.6 The built-in electric field in N causes interface charge due to polarization effect in the heterostructure, and a strong built-in electric field exists in the AlGaN absorption layer, so that separation of photo-generated electron-hole pairs is promoted, generation of photocurrent is further increased, and responsiveness and detection rate in zero bias are greatly improved.
A self-driven solar blind ultraviolet detector based on an asymmetric schottky barrier, comprising, in order from bottom to top: the substrate layer, the AlN buffer layer, the heterostructure layer and the metal electrode layer; wherein, heterostructure layer includes three high aluminium component layers: al (Al) 0.65 Ga 0.35 N buffer layer, al 0.4 Ga 0.6 N active layer and Al 0.55 Ga 0.45 An N barrier layer; and one side electrode of the self-driven solar blind ultraviolet detector is composed of three layers of Al in a high-aluminum component layer 0.55 Ga 0.45 The N barrier layer and the metal electrode layer, and the other electrode is composed of only the metal electrode layer.
Optionally, the two side electrodes of the self-driven solar blind ultraviolet detector are interdigital electrodes, and the metal electrode layer on one side electrode and Al in the three high-aluminum component layers 0.4 Ga 0.6 The N active layer forms Schottky contact, the metal electrode layer on the other side electrode and Al in the three high-aluminum component layers 0.55 Ga 0.45 The N barrier layer forms a schottky contact.
Alternatively, the interdigital electrodes on two sides are symmetrically arranged, the interdigital width is 25+/-5 μm, the interdigital length is 500 μm, and the interval between adjacent interdigital is 10+/-5 μm.
Optionally, al in the three high-aluminum component layers 0.65 Ga 0.35 The thickness of the N layer is 1.5 mu m, al 0.4 Ga 0.6 The thickness of the N active layer is 300nm, al 0.55 Ga 0.45 The N barrier layer thickness was 50nm.
Optionally, the AlN buffer layer has a thickness of 2 μm.
Optionally, the material of the metal electrode layer is Ni/Au composite metal.
Optionally, the substrate layer material is sapphire.
The application provides a preparation method of a self-driven solar blind ultraviolet detector based on an asymmetric Schottky barrier, which comprises the following steps of:
step 1: growing an AlN buffer layer on the substrate layer;
step 2: to be undoped Al 0.65 Ga 0.35 N is deposited on the AlN buffer layer to form Al 0.65 Ga 0.35 An N buffer layer;
step 3: al (Al) 0.65 Ga 0.35 After the growth of the N layer, at the Al 0.65 Ga 0.35 Deposition of undoped Al on N buffer layer 0.4 Ga 0.6 N, form Al 0.4 Ga 0.6 An N active layer;
step 4: al (Al) 0.4 Ga 0.6 After the growth of the N layer, at the Al 0.4 Ga 0.6 Deposition of undoped Al on N active layer 0.55 Ga 0.45 N, form Al 0.55 Ga 0.45 N barrier layer simultaneously forming Al with polarization enhancement effect 0.55 Ga 0.45 N/Al 0.4 Ga 0.6 N/Al 0.65 Ga 0.35 An N heterostructure;
step 5: for the Al 0.55 Ga 0.45 Performing mesa isolation etching on the N barrier layer to form the asymmetric heterostructure;
step 6: and depositing a symmetrical interdigital metal electrode layer to form a Schottky electrode.
Optionally, the device epitaxial heterostructure grown on the substrate layer adopts a Metal Organic Chemical Vapor Deposition (MOCVD) method.
Optionally, the step 5 uses inductively coupled plasma and BCl 3 /Cl 2 And carrying out mesa etching by using gas.
The invention has the beneficial effects that:
(1) The AlGaN-based solar blind ultraviolet detector with the asymmetric heterostructure utilizes asymmetric polarization enhanced Al under one side electrode 0.55 Ga 0.45 N/Al 0.4 Ga 0.6 N/Al 0.65 Ga 0.35 The N heterostructure forms different barrier heights at two Schottky contact positions to induce energy band bending, so that an asymmetric energy band structure is formed, an internal potential difference exists between two electrodes, a built-in electric field is provided for photo-generated carriers, carrier separation and transportation are obviously promoted, photocurrent can be generated even if a device is not provided with bias voltage, self-driven detection is realized, and the defect of high energy consumption of the ultraviolet detector with the traditional MSM structure is overcome.
(2) The invention constructs three layers of high aluminum component layers and utilizes Al with polarization enhancement effect 0.55 Ga 0.45 N/Al 0.4 Ga 0.6 N/Al 0.65 Ga 0.55 The N epitaxial structure enhances the built-in electric field of the absorption layer by controlling polarization, and the interface charge is caused by the polarization effect in the heterostructure, so that a strong built-in electric field exists in the AlGaN absorption layer, thereby promoting the separation of photo-generated electron-hole pairs and further increasing the generation of photocurrent. Compared with the existing self-driven MSM ultraviolet photoelectric detector, the responsivity and the detection rate of the self-driven MSM ultraviolet photoelectric detector are greatly improved when the self-driven MSM ultraviolet photoelectric detector is in zero bias.
(3) The self-driven solar blind ultraviolet detector of the invention enables the screw dislocation density of the epitaxial structure to be lower and to be about 2.45 multiplied by 10 through the AlN/sapphire substrate 8 cm -2 The leakage channel is reduced, the device has ultra-low dark current, and the sensitivity of the device is improved.
Drawings
In order to more clearly illustrate the technical solutions of the embodiments of the present invention, the drawings required for the description of the embodiments will be briefly described below, and it is apparent that the drawings in the following description are only some embodiments of the present invention, and other drawings may be obtained according to these drawings without inventive effort for a person skilled in the art.
Fig. 1 is a schematic layer structure diagram of a self-driven solar blind ultraviolet detector based on an asymmetric schottky barrier.
FIG. 2 is a graph showing the I-V curve characteristics of the device of the present invention under-10 to 10V bias at room temperature without illumination and with illumination at 280 nm.
Fig. 3 is a graph of photocurrent response and spectral response of an ultraviolet detector of the present invention without a bias voltage (0V).
Fig. 4 is a structural comparison diagram of an ultraviolet detector a with an asymmetric MSM structure and a comparison device B of the present invention.
FIG. 5 is a graph of the spectral response of an asymmetric MSM structured UV detector of the present invention at 0V versus a control device symmetric MSM structured UV detector.
Detailed Description
For the purpose of making the objects, technical solutions and advantages of the present invention more apparent, the embodiments of the present invention will be described in further detail with reference to the accompanying drawings.
Embodiment one:
the present embodiment provides a self-driven solar blind ultraviolet detector based on an asymmetric schottky barrier, referring to fig. 1, the ultraviolet detector sequentially includes, from top to bottom: the substrate layer, the AlN buffer layer, the heterostructure layer and the metal electrode layer; wherein, heterostructure layer includes three high aluminium composition layers: al (Al) 0.65 Ga 0.35 N buffer layer, al 0.4 Ga 0.6 N active layer and Al 0.55 Ga 0.45 An N barrier layer; and one side electrode of the self-driven solar blind ultraviolet detector is composed of three layers of Al in high-aluminum component layers 0.55 Ga 0.45 The N barrier layer and the metal electrode layer, and the other electrode is composed of only the metal electrode layer.
The two side electrodes are interdigital electrodes, and the metal electrode layer on one side electrode and Al in the three high-aluminum component layers 0.4 Ga 0.6 N-activeThe layers form Schottky contact, and the metal electrode layer on the other side electrode and Al in the three high-aluminum component layers 0.55 Ga 0.45 The N barrier layer forms a schottky contact.
The application considers screw dislocation which is one of main defects in AlGaN materials, adopts an AlN/sapphire substrate, greatly reduces the screw dislocation density of an epitaxial structure, and improves the sensitivity of the device. In the AlN/sapphire substrate, the substrate layer is a sapphire substrate, the thickness of the AlN buffer layer is 2 mu m, and Al 0.65 Ga 0.35 The N buffer layer was not doped to a thickness of 1.5 μm, followed by 300nm thick Al 0.4 Ga 0.6 N active layer and 50nm thick Al 0.55 Ga 0.45 The N barrier layer forms a heterostructure. The material of the metal electrode layer is Ni/Au composite metal.
Using a cell with BCl 3 /Cl 2 Mesa etching is carried out by gas inductively coupled plasma to remove the residual Al 0.55 Ga 0.45 An N barrier layer of Al 0.55 Ga 0.45 N mesa, al of mesa structure 0.55 Ga 0.45 The N width was 25. Mu.m. Thus, the constitution is based on Al 0.55 Ga 0.45 N/Al 0.4 Ga 0.6 N/Al 0.65 Ga 0.55 An asymmetric heterostructure of N.
The interdigital electrodes on two sides of the ultraviolet detector are symmetrically arranged, the interdigital width is 25+/-5 mu m, the interdigital length is 500 mu m, and the distance between adjacent interdigital is 10+/-5 mu m.
Example two
The embodiment provides a preparation method of a self-driven solar blind ultraviolet detector based on an asymmetric schottky barrier, which is used for preparing the self-driven solar blind ultraviolet detector with the asymmetric heterostructure provided in the first embodiment, and the preparation method grows a device epitaxial heterostructure on a sapphire substrate through Metal Organic Chemical Vapor Deposition (MOCVD), and comprises the following steps:
step 1: growing an AlN buffer layer on the substrate layer;
step 2: to be undoped Al 0.65 Ga 0.35 The N layer is deposited on the AlN buffer layer;
step 3: al (Al) 0.65 Ga 0.35 After the growth of the N layer, at the Al 0.65 Ga 0.35 Deposition of undoped Al on the N layer 0.4 Ga 0.6 N, form Al 0.4 Ga 0.6 An N active layer;
step 4: al (Al) 0.4 Ga 0.6 After the growth of the N layer, at the Al 0.4 Ga 0.6 Deposition of undoped Al on the N layer 0.55 Ga 0.45 N, form Al 0.55 Ga 0.45 An N barrier layer forming Al 0.55 Ga 0.45 N/Al 0.4 Ga 0.6 N/Al 0.65 Ga 0.55 An N heterostructure;
step 5: using inductively coupled plasma with BCl 3 /Cl 2 Gas to Al 0.55 Ga 0.45 Performing mesa isolation etching on the N barrier layer to form asymmetric Al 0.55 Ga 0.45 N/Al 0.4 Ga 0.6 N/Al 0.65 Ga 0.55 An N heterostructure;
step 6: after mesa isolation etch, a standard Ni/Au (50/150 nm) schottky metal stack is deposited.
In order to further illustrate the beneficial effects that the self-driven solar blind ultraviolet detector with the asymmetric Schottky barrier can achieve, a series of experiments are carried out, and the experimental results are shown in figures 2-5.
FIG. 2 shows the I-V curves of the UV detector of the present invention under dark conditions and under illumination with 280nm monochromatic light, respectively. Dark current measured at room temperature is less than 1.0X10 at bias voltage ranging from-10V to 10V -11 A, at a bias voltage of 5V, can be as low as 1.8X10 -13 A. Photocurrent at bias voltage of 5V was 2.8x10 -9 A. Therefore, the test result shows that the self-driven solar blind ultraviolet detector device provided by the application has ideal light-dark current ratio of about 1.6X10 4
FIG. 3 shows the photocurrent response curve and the calibrated spectral response curve of the self-driven solar blind ultraviolet detector in the unbiased state. It can be seen that the device takes a photocurrent maximum at 280nm, is significantly cut off at 285nm at wavelength, and is compatible with Al 0.4 Ga 0.6 The forbidden bandwidth of the N absorption layer is consistent. In addition, at 0V, the responsivity of the self-driven solar blind ultraviolet detector device is 0.04A/W, and the detection rate is 3.1X10 12 Jones, achieves the self-driven function. This is due to the asymmetric heterostructure with polarization enhancement effect forming an asymmetric MSM device, whereby the different barrier heights provide an asymmetric energy band and enhance Al due to its polarization effect 0.4 Ga 0.6 Built-in electric field of the N active layer.
To highlight the application of the self-driven solar blind ultraviolet detector, the metal electrode layer on one side electrode and the Al in three high-aluminum component layers are provided 0.4 Ga 0.6 The N active layer forms Schottky contact, the metal electrode layer on the other side electrode and Al in the three high-aluminum component layers 0.55 Ga 0.45 The N barrier layer forms the beneficial effect brought by schottky contact, and the embodiment also prepares a symmetrical structure device B, and compares the self-driven solar blind ultraviolet detector provided by the application, and the symmetrical structure device B is different from the device of the application in that electrodes on two sides of the symmetrical structure device B are both identical to Al 0.55 Ga 0.45 The N barrier layer forms a schottky contact, see fig. 4.
Fig. 5 shows the comparison result of the light response curve of the self-driven solar blind ultraviolet detector device a and the symmetrical structure device B provided by the application at 0V, and the comparison result can obviously show that the response spectrum of the self-driven solar blind ultraviolet detector device a provided by the application has obvious response broad peaks at 250-280 nm, namely obvious response broad peaks to solar blind ultraviolet rays, but the light response curve of the device B at 0V has no obvious response peak.
In summary, the ultraviolet detector of the invention can realize self-driving characteristics, low dark current and higher zero bias responsivity. Therefore, the structural design makes up the defect of high power consumption of the horizontal symmetrical MSM structural device, and the responsiveness is greatly improved.
Some steps in the embodiments of the present invention may be implemented by using software, and the corresponding software program may be stored in a readable storage medium, such as an optical disc or a hard disk.
The foregoing description of the preferred embodiments of the invention is not intended to limit the invention to the precise form disclosed, and any such modifications, equivalents, and alternatives falling within the spirit and scope of the invention are intended to be included within the scope of the invention.

Claims (10)

1. The utility model provides a self-driven solar blind ultraviolet detector based on asymmetric schottky barrier which characterized in that, self-driven solar blind ultraviolet detector from down includes in proper order: the substrate layer, the AlN buffer layer, the heterostructure layer and the metal electrode layer; wherein, heterostructure layer includes three high aluminium component layers: al (Al) 0.65 Ga 0.35 N buffer layer, al 0.4 Ga 0.6 N active layer and Al 0.55 Ga 0.45 An N barrier layer; and one side electrode of the self-driven solar blind ultraviolet detector is composed of three layers of Al in a high-aluminum component layer 0.55 Ga 0.45 The N barrier layer and the metal electrode layer, and the other electrode is composed of only the metal electrode layer.
2. The self-driven solar blind ultraviolet detector according to claim 1, wherein the two side electrodes of the self-driven solar blind ultraviolet detector are interdigital electrodes, and the metal electrode layer on one side electrode and the Al in the three high-aluminum component layers 0.4 Ga 0.6 The N active layer forms Schottky contact, the metal electrode layer on the other side electrode and Al in the three high-aluminum component layers 0.55 Ga 0.45 The N barrier layer forms a schottky contact.
3. The self-driven solar blind ultraviolet detector according to claim 2, wherein the interdigital electrodes on both sides are symmetrically arranged, the interdigital width is 25±5 μm, the interdigital length is 500 μm, and the interval between adjacent interdigital is 10±5 μm.
4. The self-driven solar blind ultraviolet detector according to claim 1, wherein Al in the three high-alumina component layers 0.65 Ga 0.35 The thickness of the N layer is 1.5 mu m, al 0.4 Ga 0.6 The N active layer thickness is 300nm,Al 0.55 Ga 0.45 the N barrier layer thickness was 50nm.
5. The self-driven solar blind ultraviolet detector according to claim 1, wherein the AlN buffer layer has a thickness of 2 μm.
6. The self-driven solar blind ultraviolet detector according to claim 1, wherein the material of the metal electrode layer is Ni/Au complex metal.
7. The self-driven solar blind ultraviolet detector of claim 1 wherein the substrate layer material is sapphire.
8. The preparation method of the self-driven solar blind ultraviolet detector based on the asymmetric Schottky barrier is characterized by comprising the following steps of:
step 1: growing an AlN buffer layer on the substrate layer;
step 2: to be undoped Al 0.65 Ga 0.35 N is deposited on the AlN buffer layer to form Al 0.65 Ga 0.35 An N buffer layer;
step 3: al (Al) 0.65 Ga 0.35 After the growth of the N layer, at the Al 0.65 Ga 0.35 Deposition of undoped Al on N buffer layer 0.4 Ga 0.6 N, form Al 0.4 Ga 0.6 An N active layer;
step 4: al (Al) 0.4 Ga 0.6 After the growth of the N layer, at the Al 0.4 Ga 0.6 Deposition of undoped Al on N active layer 0.55 Ga 0.45 N, form Al 0.55 Ga 0.45 N barrier layer simultaneously forming Al with polarization enhancement effect 0.55 Ga 0.45 N/Al 0.4 Ga 0.6 N/Al 0.65 Ga 0.35 An N heterostructure;
step 5: for the Al 0.55 Ga 0.45 The N barrier layer is subjected to mesa isolation etching to formForming the asymmetric heterostructure;
step 6: and depositing a symmetrical interdigital metal electrode layer to form a Schottky electrode.
9. The method of claim 8, wherein growing the device epitaxial heterostructure on the substrate layer employs a metal organic chemical vapor deposition MOCVD process.
10. The method of claim 8, wherein said step 5 employs inductively coupled plasma with BCl 3 /Cl 2 And carrying out mesa etching by using gas.
CN202311653005.XA 2023-12-05 2023-12-05 Self-driven solar blind ultraviolet detector based on asymmetric Schottky barrier Pending CN117673188A (en)

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