WO2012129755A1 - Imaging array unit using ultra-violet avalanche photo diodes, application method thereof, and imaging array composed of the same - Google Patents
Imaging array unit using ultra-violet avalanche photo diodes, application method thereof, and imaging array composed of the same Download PDFInfo
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- WO2012129755A1 WO2012129755A1 PCT/CN2011/072138 CN2011072138W WO2012129755A1 WO 2012129755 A1 WO2012129755 A1 WO 2012129755A1 CN 2011072138 W CN2011072138 W CN 2011072138W WO 2012129755 A1 WO2012129755 A1 WO 2012129755A1
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- imaging array
- avalanche tube
- ultraviolet
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- array pixel
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- 238000003384 imaging method Methods 0.000 title claims abstract description 97
- 238000000034 method Methods 0.000 title claims abstract description 22
- 239000004065 semiconductor Substances 0.000 claims abstract description 39
- 239000010409 thin film Substances 0.000 claims abstract description 39
- 239000000463 material Substances 0.000 claims abstract description 34
- 239000002184 metal Substances 0.000 claims abstract description 27
- 229910002704 AlGaN Inorganic materials 0.000 claims description 28
- 238000000151 deposition Methods 0.000 claims description 15
- 238000005530 etching Methods 0.000 claims description 15
- 238000002161 passivation Methods 0.000 claims description 12
- 239000000758 substrate Substances 0.000 claims description 10
- 230000003321 amplification Effects 0.000 claims description 3
- 238000003199 nucleic acid amplification method Methods 0.000 claims description 3
- 230000007547 defect Effects 0.000 abstract description 19
- 238000000098 azimuthal photoelectron diffraction Methods 0.000 description 71
- 230000003287 optical effect Effects 0.000 description 8
- 238000001514 detection method Methods 0.000 description 5
- 238000010586 diagram Methods 0.000 description 5
- XUIMIQQOPSSXEZ-UHFFFAOYSA-N Silicon Chemical compound [Si] XUIMIQQOPSSXEZ-UHFFFAOYSA-N 0.000 description 4
- 238000002488 metal-organic chemical vapour deposition Methods 0.000 description 4
- 229910052710 silicon Inorganic materials 0.000 description 4
- 239000010703 silicon Substances 0.000 description 4
- 238000004519 manufacturing process Methods 0.000 description 3
- 239000003990 capacitor Substances 0.000 description 2
- 229910001020 Au alloy Inorganic materials 0.000 description 1
- 229910001069 Ti alloy Inorganic materials 0.000 description 1
- 238000004458 analytical method Methods 0.000 description 1
- 238000003491 array Methods 0.000 description 1
- 239000000470 constituent Substances 0.000 description 1
- 230000007423 decrease Effects 0.000 description 1
- 230000000694 effects Effects 0.000 description 1
- 230000005611 electricity Effects 0.000 description 1
- 238000005516 engineering process Methods 0.000 description 1
- 239000010408 film Substances 0.000 description 1
- 239000000203 mixture Substances 0.000 description 1
- 229910003465 moissanite Inorganic materials 0.000 description 1
- 229910052594 sapphire Inorganic materials 0.000 description 1
- 239000010980 sapphire Substances 0.000 description 1
- 229910010271 silicon carbide Inorganic materials 0.000 description 1
Classifications
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- H—ELECTRICITY
- H10—SEMICONDUCTOR DEVICES; ELECTRIC SOLID-STATE DEVICES NOT OTHERWISE PROVIDED FOR
- H10F—INORGANIC SEMICONDUCTOR DEVICES SENSITIVE TO INFRARED RADIATION, LIGHT, ELECTROMAGNETIC RADIATION OF SHORTER WAVELENGTH OR CORPUSCULAR RADIATION
- H10F39/00—Integrated devices, or assemblies of multiple devices, comprising at least one element covered by group H10F30/00, e.g. radiation detectors comprising photodiode arrays
- H10F39/80—Constructional details of image sensors
- H10F39/803—Pixels having integrated switching, control, storage or amplification elements
- H10F39/8033—Photosensitive area
-
- H—ELECTRICITY
- H10—SEMICONDUCTOR DEVICES; ELECTRIC SOLID-STATE DEVICES NOT OTHERWISE PROVIDED FOR
- H10F—INORGANIC SEMICONDUCTOR DEVICES SENSITIVE TO INFRARED RADIATION, LIGHT, ELECTROMAGNETIC RADIATION OF SHORTER WAVELENGTH OR CORPUSCULAR RADIATION
- H10F30/00—Individual radiation-sensitive semiconductor devices in which radiation controls the flow of current through the devices, e.g. photodetectors
- H10F30/20—Individual radiation-sensitive semiconductor devices in which radiation controls the flow of current through the devices, e.g. photodetectors the devices having potential barriers, e.g. phototransistors
- H10F30/21—Individual radiation-sensitive semiconductor devices in which radiation controls the flow of current through the devices, e.g. photodetectors the devices having potential barriers, e.g. phototransistors the devices being sensitive to infrared, visible or ultraviolet radiation
- H10F30/22—Individual radiation-sensitive semiconductor devices in which radiation controls the flow of current through the devices, e.g. photodetectors the devices having potential barriers, e.g. phototransistors the devices being sensitive to infrared, visible or ultraviolet radiation the devices having only one potential barrier, e.g. photodiodes
- H10F30/225—Individual radiation-sensitive semiconductor devices in which radiation controls the flow of current through the devices, e.g. photodetectors the devices having potential barriers, e.g. phototransistors the devices being sensitive to infrared, visible or ultraviolet radiation the devices having only one potential barrier, e.g. photodiodes the potential barrier working in avalanche mode, e.g. avalanche photodiodes
Definitions
- the present invention relates to an ultraviolet avalanche tube imaging array pixel, an application method thereof, and an avalanche tube imaging array.
- BACKGROUND OF THE INVENTION The detection of ultraviolet light, especially in the solar blind, has extremely important applications in space detection and military applications.
- the photon counting system in the ultraviolet band uses a photomultiplier tube (PMT), but the photomultiplier tube is bulky, fragile, high in operating voltage and expensive, so a small-sized, inexpensive solid-state ultraviolet detector is very important.
- PMT photomultiplier tube
- FIG. 1 is a graph showing the relationship between the yield of the AlGaN avalanche tube and the device area. It can be seen that if the avalanche tube area is ⁇ ⁇ ⁇ 2 , the yield is less than 1%, assuming a 1KX 1K UV is required.
- Optical avalanche tube imaging array in which the number of good quality pixels is only 10 ⁇ , and the remaining 990 pixels are bad. Such an imaging array cannot work at all, so it is difficult to use traditional avalanche tubes at the current yield.
- the structure implements an ultraviolet avalanche tube imaging array.
- the APD 100 is a typical silicon-based metal-resistance-semiconductor (MRS) [V. Saveliev, V. Golovin, Nuclear Instruments and Methods in Physics Research A 442 (2000): 223-229] Structure Avalanche
- the tube detector whose basic structure is composed of a photodiode 101, a thin film resistor 102 and a metal electrode 103, the thin film resistor 102 and the p-type semiconductor end of the photodiode 101 are in electrical contact, and then the metal layer 103 is deposited on the thin film resistor 102. It is in contact with the thin film resistor 102, and its equivalent circuit is shown in Fig. 2B.
- a negative voltage Vbias is applied to the MRS structure avalanche tube APD 100.
- the photodiode 101 When there is no light, the photodiode 101 is in a negative bias state, the diode 101 is equivalent to a capacitor, and the negative voltage Vbias is mainly distributed on the photodiode 101. If a photon reaches the diode 101, the photon is absorbed to generate electron-hole pairs, electrons and holes generate more electrons and holes in the multiplication region, and the photodiode 101 avalanches, so that the optical signal is converted into an electrical signal and amplified. The process can also be seen as a discharge process of a capacitor.
- the present invention provides an ultraviolet avalanche tube imaging array pixel, which can effectively overcome the defects of the semiconductor material itself and improve the yield.
- the invention also provides an application method of the ultraviolet avalanche tube imaging array pixel and an avalanche tube imaging array composed thereof.
- the ultraviolet avalanche tube imaging array pixel is formed by a plurality of avalanche tube detectors connected in parallel, wherein the avalanche tube detector is sequentially connected by a photodiode, a thin film resistor and a metal layer, and each of the avalanche tube detectors is photoelectrically
- the n-type semiconductor of the diode is connected to the contact electrode, and the contact electrode of each avalanche tube detector in the imaging pixel forms an electrical connection as an electrode, and each avalanche tube detector shares a complete metal layer, and the metal layer forms an ultraviolet avalanche tube.
- the other electrode of the imaging array cell is formed by a plurality of avalanche tube detectors connected in parallel, wherein the avalanche tube detector is sequentially connected by a photodiode, a thin film resistor and a metal layer, and each of the avalanche tube detectors is photoelectrically
- the n-type semiconductor of the diode is connected to the contact electrode, and the contact electrode
- the ultraviolet avalanche tube imaging array pixel comprises, in order from bottom to top, a plurality of independent photodiodes, an insulating passivation layer, and a plurality of independent thin film resistors and insulating mediums corresponding to the plurality of photodiodes.
- a layer and a metal layer wherein the passivation layer is provided with a plurality of first contact holes, so that the p-type semiconductor end of each photodiode is electrically contacted with the corresponding thin film resistor through the first contact hole, and the insulating dielectric layer is provided with a plurality of The second contact hole causes each of the thin film resistors to make electrical contact with the metal layer through the second contact hole.
- both the passivation layer and the dielectric layer are electrically insulating layers.
- the method for preparing the ultraviolet avalanche tube imaging array pixel comprises the following steps:
- the basic unit of the ultraviolet avalanche tube imaging array pixel may be the substrate 201 from the bottom up, the n-type semiconductor 202, the n-type contact electrode 203, p-type
- the semiconductor 204, the n-type and p-type semiconductors are epitaxially formed by MOCVD; then the p-type semiconductor is etched to form n rows of contact electrodes 203; the passivation layer 205 is deposited to form contact holes 206, and a thin film resistor 207 is formed.
- the metal layer 210 may be a transparent or translucent material.
- UV-APD 300 The ultraviolet avalanche tube imaging array pixel (hereinafter referred to as UV-APD 300) may be formed by a plurality of UV-APDs 200 in parallel, as shown in FIG. 3A, UV-APD 200-1, 200-2, 200-3 are Three UV-APDs 200, which are connected in parallel by a metal layer 210 and a common contact electrode 203-1, 203-2, the basic process of which is illustrated in Figure 3C:
- Step 212 forming an n-type semiconductor 202 and a p-type semiconductor 204 on the substrate 201, and epitaxially growing the semiconductor material by MOCVD;
- Step 213, etching a p-type semiconductor, forming contact electrodes 203-1 and 203-2 on the n-type semiconductor, and the contact electrodes may be connected together by a metal line as a contact electrode;
- Step 214 depositing a passivation layer 205 and etching to form a contact hole 206;
- Step 215 depositing and etching to form thin film resistors 207-1, 207-2 and 207-3;
- Step 216 depositing a dielectric layer 208 and forming a contact hole 209;
- Step 217 depositing a metal layer 210 and making electrical contact with the film resistor, and the metal layer 210 constitutes another electrode 301.
- the equivalent circuit diagram of the UV-APD 300 is shown in FIG. 3D.
- the UV-APD 300 is formed by a plurality of UV-APDs 200 connected in parallel, and the cathodes of all the UV-APDs 200 are connected together by the metal layer 210 to form an electrode, the contact electrode.
- the 203 are joined together to form another electrode.
- the UV-APD 300 thus constructed is actually composed of a plurality of UV-APD 200 units connected in parallel.
- the yield Y of GaN and AlGaN-based avalanche tubes is very low due to the high defect density of GaN and AlGaN materials.
- UV-APD 300 is composed of a suitable number of UV-APDs 200 in parallel, then UV-APD There are always a certain number of good quality UV-APD 200 in 300, so the UV-APD 300 can always detect the optical signal, so the UV avalanche tube imaging array of this structure has a pixel yield close to 100%, which can be realized.
- Ultraviolet avalanche tube imaging arrays overcome the problems caused by the high defect density of GaN and AlGaN materials themselves.
- the photodiode in the ultraviolet avalanche tube imaging array pixel is made of a m-v family and/or a ⁇ - ⁇ group semiconductor material, preferably made of at least one of GaN, AlGaN or A1N.
- the radius of the avalanche tube detector unit in the ultraviolet avalanche tube imaging array pixel is preferably from 1 to 50 ⁇ m.
- the resistance of each individual thin film resistor is from 100 ⁇ to 10 ⁇ ; the preferred material of the thin film resistor is SiC or Si x O y .
- UV-APDs 200 are bad in UV-APD 300, so when there is no light plus negative bias, these A bad avalanche has occurred in the UV-APD 200.
- I B an electrical signal on the electrode 301. This electrical signal is a dark current. We can call this current the bottom current; and those of good quality UV-APD 200 will work properly.
- the application method of the ultraviolet avalanche tube imaging array pixel is: applying a negative bias voltage to the ultraviolet avalanche tube imaging array pixel, so that the ultraviolet avalanche tube imaging array pixel works, when there is no light
- the measured photo-current of the ultraviolet avalanche tube imaging array is I B , which is used as the pixel bottom current; when there is light, those good quality UV-APD 200 undergo avalanche process to convert the optical signal into electricity.
- the signal is amplified and the pixel current of the ultraviolet avalanche tube imaging array is measured.
- Ultraviolet avalanche tube imaging array pixels operate in linear amplification mode or Geiger Mode [D. Renker, Nuclear Instruments and Methods in Physics Research A 567 (2006) 48-56].
- the applied negative bias is 10V to 100V.
- the avalanche tube imaging array is composed of a plurality of the ultraviolet avalanche tube imaging array pixels.
- the UV-APD 300 is obtained by connecting a plurality of UV-APDs 200 in parallel, the area of the UV-APD 200 can be made small, which improves the yield of the UV-APD 200 without affecting the photosensitive area of the UV-APD 300. If the UV-APD 300 is composed of a suitable number of UV-APDs 200 in parallel, there is always a certain number of good quality UV-APDs 200 in the UV-APD 300. If the defect density of GaN is 10 7 cm - 2 and the area of UV-APD200 is 5 ⁇ 5 ⁇ 2 , the yield of UV-APD200 is 13% according to the yield formula, if the UV-APD 300 is composed of 10x10 UV-APD 200 units.
- the composition, the UV-APD 200 in the pixel UV-APD 300 is of good quality, so that the UV-APD 300 can always detect the optical signal, so the purple ultraviolet avalanche tube imaging array of this structure is good.
- the rate is close to 100%, which overcomes the problems caused by the high defect density of GaN and AlGaN materials themselves.
- the UV-APD 300 is composed of 16 UV-APDs 200 in parallel. If there is always a good quality UV-APD 200 in the pixel, the UV-APD 300 is a good quality image pixel, which can The optical signal is detected and the yield is nearly 100%, and the ultraviolet avalanche tube imaging array can be realized.
- the yield of the ultraviolet avalanche tube imaging array pixel UV-APD 300 of the present invention is close to 100%, so that the avalanche tube imaging array can be fabricated by using the UV-APD 300 as an imaging unit.
- the UV-APD ARRAY 500 is an avalanche tube imaging array composed of NXN UV-APD 300.
- the imaging array UV- In the APD ARRAY 500 all the pixel units are of good quality, so the ultraviolet avalanche tube imaging array pixel UV-APD 300 of the present invention overcomes the inability to achieve ultraviolet light due to the high defect density of the GaN and AlGaN materials themselves. Avalanche tube imaging array problems.
- the novel structure proposed by the present invention can also be used to fabricate a large photosensitive area ultraviolet avalanche tube imaging array pixel. Since the defect density of the GaN and AlGaN materials themselves is relatively large, a large-area ultraviolet avalanche tube is very difficult to manufacture, but
- the UV-APD 300 is composed of a plurality of UV-APDs 200 in parallel, which can make the area of the UV-APD 200 small, improve the yield of the UV-APD 200, and is composed of a plurality of UV-APDs 200. UV-APD 300 increases the photosensitive area without affecting the yield. For example, we need to make a UV avalanche tube imaging array pixel of the size of ⁇ ⁇ ⁇ 2.
- the yield is less than 1%. If the invention is used, if the area of the UV-APD 200 is 5 ⁇ 5 ⁇ 2 ( As the process progresses, the size can be made smaller.) The yield of UV-APD 200 is about 10%, then 20-20 UV-APD 200 can be used to form UV-APD 300, so that the pixel area reaches 100 X ⁇ 2 , and its yield can be close to 100%, which is not possible with the current avalanche tube structure.
- the UV avalanche tube imaging array of the present invention is composed of 10 x 10 5 ⁇ 5 ⁇ 2 sized UV-APD 200 cells), and it can be found only when AlGaN and GaN materials are used.
- the defect density is reduced to 10 4 cm -2
- the yield of the conventional structured ultraviolet avalanche tube can be compared with the present invention. Therefore, by using the ultraviolet avalanche tube imaging array pixel structure proposed by the present invention, a large photosensitive area can be made.
- the UV avalanche tube cell avoids the problem of a drop in yield due to the large area.
- the ultraviolet avalanche tube imaging array pixel structure of the invention overcomes the problem that the defect density of the multi-defective material such as GaN, AlGaN and the like is too high, and the yield of the novel structure ultraviolet avalanche tube imaging array can be improved. Approaching and reaching 100%, using the ultraviolet avalanche tube imaging array pixel as an imaging unit, an ultraviolet avalanche tube imaging array can be fabricated.
- the ultraviolet avalanche tube imaging array pixel structure overcomes the problem of low yield of a large area avalanche tube, and the ultraviolet avalanche tube imaging array pixel can be composed of tens or hundreds of smaller basic unit structures UV-
- the APD 200 is composed, so that a large a photosensitive area of the ultraviolet avalanche tube imaging array pixel can be made, and there is no problem that the yield is lowered because the area is too large.
- FIG. 1 is a diagram showing the relationship between the yield of a conventional avalanche tube detector and the device area of a conventional AlGaN material;
- FIG. 2A is a schematic view showing the structure of a typical silicon-based MRS avalanche tube detector;
- 2B is an equivalent circuit diagram of the silicon-based MRS structure avalanche tube detector described in FIG. 1A;
- 3A is a schematic structural view of an ultraviolet avalanche tube imaging array pixel according to the present invention.
- 3B is a schematic structural diagram of a basic constituent unit in the ultraviolet avalanche tube imaging array pixel of FIG. 3A;
- 3C is a basic process of the ultraviolet avalanche tube imaging array pixel of FIG. 3A;
- 3D is an equivalent circuit diagram of the ultraviolet avalanche tube imaging array pixel of FIG. 3A;
- FIG. 4 is a schematic structural view of a specific ultraviolet avalanche tube imaging array pixel according to the present invention.
- Figure 5 is an avalanche tube imaging array of the present invention
- FIG. 6 is a graph comparing the yield of a conventional structured avalanche tube detector with an area of 50 ⁇ 50 ⁇ 2 and the yield of the ultraviolet avalanche tube imaging array of the present invention.
- DETAILED DESCRIPTION OF THE INVENTION A schematic view of an ultraviolet avalanche tube imaging array pixel of the present invention is shown in FIG. If the ultraviolet avalanche tube imaging array pixel UV-APD 300 is composed of a plurality of basic units UV-APD 200 (as shown in FIG. 3A), the radius of the UV-APD 200 may be ⁇ to 50 ⁇ . In FIG. 3A, we can form the substrate 201 from bottom to top.
- the substrate 201 can be a material such as SiC, sapphire, or silicon substrate, but requires the substrate to transmit light; the n-type semiconductor 202 and the p-type semiconductor 204, the material can be It is a material such as GaN, A1N or AlGaN.
- the n-type semiconductor 202 and the p-type semiconductor 204 can be epitaxially grown by MOCVD, and a buffer layer is also formed, thereby reducing lattice dislocations in the material and reducing the defect density; and then etching p The semiconductor is exposed to a portion of the n-type semiconductor, and then the n-type contact electrode 203 is formed.
- the electrode may be made of a material such as a Ti/Au alloy; the insulating passivation layer 205 is deposited and a contact hole 206 is formed, and the passivation layer may be made of an oxide or the like; Forming the thin film resistor 207 to make the thin film resistor 207 and the p-type semiconductor form electrical contact, the thin film resistor 207 may be made of a material such as SiC or Si x O y having a resistance value of about several hundred ⁇ ⁇ to 1 ⁇ ⁇ ; a dielectric layer 208 is deposited and a contact hole 209 is formed, the metal layer 210 and the thin film resistor 207 are in electrical contact, and 211 is a contact electrode.
- the ultraviolet avalanche tube imaging array pixel UV-APD 300 of the present invention can be composed of tens to hundreds of UV-APD 200s, and if it constitutes an ultraviolet avalanche tube imaging array pixel of the size ⁇ ⁇ ⁇ 2 , 20 X can be used. 20 UV-APD 200s with an area of 5 X 5 ⁇ m 2 are formed, and the process flow is shown in FIG. 3C.
- n-type semiconductor 202 and a p-type semiconductor 204 are formed on the substrate 201, and a semiconductor material such as GaN, A1N or AlGaN can be epitaxially grown by MOCVD;
- the p-type semiconductor 204 is etched to form a plurality of photodiode array structures having an array size of 20 X 20 and a photodiode having an area of 5 ⁇ 5 ⁇ 2 .
- a contact electrode 203 is formed on the n-type semiconductor 202, and all of the n-type contact electrodes 203 may be connected together by a metal line as an electrode of the ultraviolet avalanche photoimageable array pixel;
- the metal layer 210 is deposited and electrically contacted with all of the thin film resistors 207 through the contact holes 209, and the metal layer 210 constitutes the other electrode 211.
- a negative bias voltage Vbias is applied to the electrode 301, so that the pixel UV-APD 300 operates in linear amplification mode or Geiger Mode.
- the voltage can range from 10V to 100V.
- the operating voltage varies according to different doping concentrations and process parameters.
- I c is the size of the electrical signal read by the avalanche tube cell UV-APD 300.
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Description
说明书 紫外光雪崩管成像阵列像元、 其应用方法及雪崩管成像阵列 技术领域 本发明涉及一种紫外光雪崩管成像阵列像元、 其应用方法及雪崩管成像阵列。 背景技术 紫外光特别是日盲紫外波段的探测在空间探测以及军事方面有着极其重要的应用。目前, 紫外波段的光子计数系统 应用的是光电倍增管 (PMT), 但是光电倍增管体积大、 易碎、 工 作电压高且价格昂贵, 所以体积小、 价格便宜的固态紫外探测器就有非常重要的优势。 BACKGROUND OF THE INVENTION 1. Field of the Invention The present invention relates to an ultraviolet avalanche tube imaging array pixel, an application method thereof, and an avalanche tube imaging array. BACKGROUND OF THE INVENTION The detection of ultraviolet light, especially in the solar blind, has extremely important applications in space detection and military applications. At present, the photon counting system in the ultraviolet band uses a photomultiplier tube (PMT), but the photomultiplier tube is bulky, fragile, high in operating voltage and expensive, so a small-sized, inexpensive solid-state ultraviolet detector is very important. The advantages.
近年来随着 GaN和 AlGaN材料工艺的进步,在实验室中也出现了 GaN基和 AlGaN基材 料的紫外光雪崩管和单光子探测雪崩管 (SPAD) 的报道。 但是由于 GaN以及 AlGaN材料本 身晶格错位的原因, 材料中缺陷密度非常大 (目前报道的 GaN及 AlGaN材料的位错密度为 107cm- 2至 101Q cm-2), 特别是 AlGaN材料中随着 A1组分含量的增大 (A1含量越大, AlGaN 禁带宽度越大, 探测截止波长越短), 缺陷密度也在越大。 所以 GaN基和 AlGaN基雪崩管和 单光子探测雪崩管非常难制造, 如果 AlGaN材料的缺陷密度为 108cm- 2, 那么根据良率公式In recent years, with the advancement of GaN and AlGaN materials, reports of UV avalanche tubes and single photon detection avalanche tubes (SPAD) of GaN-based and AlGaN-based materials have also appeared in the laboratory. However, due to the lattice misalignment of GaN and AlGaN materials, the defect density in the material is very large (the reported dislocation density of GaN and AlGaN materials is 10 7 cm - 2 to 10 1 Q cm - 2 ), especially in AlGaN materials. As the content of the A1 component increases (the larger the A1 content, the larger the forbidden band width of AlGaN, the shorter the detection cutoff wavelength), the greater the defect density. Therefore, GaN-based and AlGaN-based avalanche tubes and single-photon detection avalanche tubes are very difficult to manufacture. If the defect density of AlGaN materials is 10 8 cm - 2 , then according to the yield formula
Y=( )2 [WAY KUO, FELLOW, IEEE, AND TAEHO KIM, PROCEEDINGS OF THE IEEE,Y=( ) 2 [WAY KUO, FELLOW, IEEE, AND TAEHO KIM, PROCEEDINGS OF THE IEEE,
ADAD
VOL. 87, NO. 8, AUGUST 1999】, (其中 A为器件面积, D为缺陷密度。) AlGaN雪崩管的良 率极低, 且雪崩管面积越大, 良率越低。 图 1为计算得到的 AlGaN雪崩管的良率与器件面积 的关系图, 可以看出, 若雪崩管面积为 ΙΟ Χ ΙΟμηι2, 其良率不到 1%, 假设要制造一个 1KX 1K大小的紫外光雪崩管成像阵列, 其中品质好的像元个数只有 10Κ, 其余 990Κ个像元都是 坏的, 这样的成像阵列根本不能工作, 所以以目前这样的良率, 很难用传统的雪崩管结构实 现紫外光雪崩管成像阵列。 VOL. 87, NO. 8, AUGUST 1999], (where A is the device area and D is the defect density.) The yield of the AlGaN avalanche tube is extremely low, and the larger the area of the avalanche tube, the lower the yield. Figure 1 is a graph showing the relationship between the yield of the AlGaN avalanche tube and the device area. It can be seen that if the avalanche tube area is ΙΟ ΙΟ ΙΟμηι 2 , the yield is less than 1%, assuming a 1KX 1K UV is required. Optical avalanche tube imaging array, in which the number of good quality pixels is only 10Κ, and the remaining 990 pixels are bad. Such an imaging array cannot work at all, so it is difficult to use traditional avalanche tubes at the current yield. The structure implements an ultraviolet avalanche tube imaging array.
如图 2Α所示, APD 100 是一个典型的硅基金属-电阻-半导体 (MRS ) [V.Saveliev, V.Golovin, Nuclear Instruments and Methods in Physics Research A 442 (2000): 223-229】结构雪 崩管探测器, 它的基本结构是由光电二极管 101、 薄膜电阻 102和金属电极 103构成, 薄膜 电阻 102和光电二极管 101的 p型半导体端形成电接触,然后金属层 103淀积在薄膜电阻 102 上和薄膜电阻 102接触, 其等效电路如图 2B。 工作时, 在 MRS结构雪崩管 APD 100上加负 电压 Vbias, 当无光时, 这时光电二极管 101处于负偏压状态, 二极管 101等效于一个电容, 负电压 Vbias主要分配在光电二极管 101上; 若有光子到达二极管 101,光子被吸收产生电子 空穴对, 电子和空穴在倍增区域产生更多的电子和空穴, 光电二极管 101发生雪崩, 从而光 信号转化为电信号并且被放大, 该过程也可以看是成电容的放电过程, 这时负偏压 Vbias就 有一部分电压分配到薄膜电阻 102上, 从而光电二极管 101上作用的电压降低, 雪崩被熄灭, 故薄膜电阻 102有着负反馈的作用。 一旦光电二极管 101上的电压降低, 雪崩过程被熄灭, 这时二极管 101重新充电, 电压增加, 从而能够探测下一个光信号。 As shown in FIG. 2A, the APD 100 is a typical silicon-based metal-resistance-semiconductor (MRS) [V. Saveliev, V. Golovin, Nuclear Instruments and Methods in Physics Research A 442 (2000): 223-229] Structure Avalanche The tube detector, whose basic structure is composed of a photodiode 101, a thin film resistor 102 and a metal electrode 103, the thin film resistor 102 and the p-type semiconductor end of the photodiode 101 are in electrical contact, and then the metal layer 103 is deposited on the thin film resistor 102. It is in contact with the thin film resistor 102, and its equivalent circuit is shown in Fig. 2B. In operation, a negative voltage Vbias is applied to the MRS structure avalanche tube APD 100. When there is no light, the photodiode 101 is in a negative bias state, the diode 101 is equivalent to a capacitor, and the negative voltage Vbias is mainly distributed on the photodiode 101. If a photon reaches the diode 101, the photon is absorbed to generate electron-hole pairs, electrons and holes generate more electrons and holes in the multiplication region, and the photodiode 101 avalanches, so that the optical signal is converted into an electrical signal and amplified. The process can also be seen as a discharge process of a capacitor. At this time, a part of the voltage of the negative bias voltage Vbias is distributed to the thin film resistor 102, so that the voltage applied to the photodiode 101 is lowered, and the avalanche is extinguished, so the thin film resistor 102 has a negative feedback. The role. Once the voltage on photodiode 101 decreases, the avalanche process is extinguished. At this time, the diode 101 is recharged and the voltage is increased to be able to detect the next optical signal.
前面提到由于 GaN和 AlGaN材料本身晶格错位的原因, 缺陷密度很大, GaN和 AlGaN 雪崩管很难制造, 良率极低, 其紫外光雪崩管成像阵列无法实现。 发明内容 本发明提供一种紫外光雪崩管成像阵列像元, 可以有效克服半导体材料本身的缺陷, 提 高良率。 As mentioned above, due to the lattice misalignment of GaN and AlGaN materials themselves, the defect density is very large, GaN and AlGaN avalanche tubes are difficult to manufacture, and the yield is extremely low, and the ultraviolet avalanche tube imaging array cannot be realized. SUMMARY OF THE INVENTION The present invention provides an ultraviolet avalanche tube imaging array pixel, which can effectively overcome the defects of the semiconductor material itself and improve the yield.
本发明还提供所述紫外光雪崩管成像阵列像元的应用方法及由其组成的雪崩管成像阵 列。 The invention also provides an application method of the ultraviolet avalanche tube imaging array pixel and an avalanche tube imaging array composed thereof.
所述紫外光雪崩管成像阵列像元由多个雪崩管探测器并联而成, 所述雪崩管探测器由光 电二极管、 薄膜电阻、 金属层顺序连接而成, 每个雪崩管探测器中, 光电二极管的 n型半导 体与接触电极连接,成像像元中各个雪崩管探测器的接触电极之间形成电连接作为一个电极, 各个雪崩管探测器共用一块完整的金属层, 金属层形成紫外光雪崩管成像阵列像元的另一个 电极。 The ultraviolet avalanche tube imaging array pixel is formed by a plurality of avalanche tube detectors connected in parallel, wherein the avalanche tube detector is sequentially connected by a photodiode, a thin film resistor and a metal layer, and each of the avalanche tube detectors is photoelectrically The n-type semiconductor of the diode is connected to the contact electrode, and the contact electrode of each avalanche tube detector in the imaging pixel forms an electrical connection as an electrode, and each avalanche tube detector shares a complete metal layer, and the metal layer forms an ultraviolet avalanche tube. The other electrode of the imaging array cell.
更优选的是,所述紫外光雪崩管成像阵列像元由下至上依次包括独立的多个光电二极管、 绝缘钝化层、 与多个光电二极管一一对应的独立的多个薄膜电阻、 绝缘介质层和金属层, 钝 化层中设有多个第一接触孔, 使每个光电二极管的 p型半导体端与相应的薄膜电阻通过第一 接触孔形成电接触, 绝缘介质层中设有多个第二接触孔, 使每个薄膜电阻与金属层通过第二 接触孔形成电接触。 More preferably, the ultraviolet avalanche tube imaging array pixel comprises, in order from bottom to top, a plurality of independent photodiodes, an insulating passivation layer, and a plurality of independent thin film resistors and insulating mediums corresponding to the plurality of photodiodes. a layer and a metal layer, wherein the passivation layer is provided with a plurality of first contact holes, so that the p-type semiconductor end of each photodiode is electrically contacted with the corresponding thin film resistor through the first contact hole, and the insulating dielectric layer is provided with a plurality of The second contact hole causes each of the thin film resistors to make electrical contact with the metal layer through the second contact hole.
作为公知常识, 钝化层、 介质层均为电绝缘层。 优选所述紫外光雪崩管成像阵列像元的制备方法包括如下步骤: As a common general knowledge, both the passivation layer and the dielectric layer are electrically insulating layers. Preferably, the method for preparing the ultraviolet avalanche tube imaging array pixel comprises the following steps:
( 1 ) 在衬底上依次形成 n型半导体以及 p型半导体; (1) sequentially forming an n-type semiconductor and a p-type semiconductor on the substrate;
(2)刻蚀 p型半导体, 形成多个独立的光电二极管结构, 并于刻蚀后的区域内在 n型半 导体上形成多个与光电二极管一一对应的接触电极; (2) etching the p-type semiconductor to form a plurality of independent photodiode structures, and forming a plurality of contact electrodes corresponding to the photodiodes in the n-type semiconductor in the etched region;
(3 ) 淀积钝化层并在光电二极管上方刻蚀形成第一接触孔; (3) depositing a passivation layer and etching over the photodiode to form a first contact hole;
(4)淀积并刻蚀形成薄膜电阻, 薄膜电阻通过第一接触孔与相应的光电二极管单元形成 电接触; (4) depositing and etching to form a thin film resistor, and the thin film resistor is in electrical contact with the corresponding photodiode unit through the first contact hole;
(5 ) 淀积介质层并在所有的薄膜电阻上方刻蚀形成第二接触孔; (5) depositing a dielectric layer and etching over all of the thin film resistors to form a second contact hole;
(6) 淀积金属层并通过第二接触孔与所有的薄膜电阻形成电接触。 (6) Depositing a metal layer and making electrical contact with all of the thin film resistors through the second contact hole.
如图 3B所示, 所述紫外光雪崩管成像阵列像元的基本单元(以下简称 UV-APD 200) 由 下而上可以为衬底 201, n型半导体 202, n型接触电极 203, p型半导体 204, n型和 p型半 导体采用 MOCVD的方法外延生成; 然后刻蚀 p型半导体, 再形成 n行接触电极 203; 淀积 钝化层 205, 形成接触孔 206, 并且淀积形成薄膜电阻 207使薄膜电阻 207和 p型半导体形成 电接触; 最后淀积介质层 208和形成接触孔 209, 金属层 210和薄膜电阻 207形成电接触, 211是接触电极。 其中衬底 201是透明或半透明的材料, 金属层 210可以是透明或半透明的 材料。 As shown in FIG. 3B, the basic unit of the ultraviolet avalanche tube imaging array pixel (hereinafter referred to as UV-APD 200) may be the substrate 201 from the bottom up, the n-type semiconductor 202, the n-type contact electrode 203, p-type The semiconductor 204, the n-type and p-type semiconductors are epitaxially formed by MOCVD; then the p-type semiconductor is etched to form n rows of contact electrodes 203; the passivation layer 205 is deposited to form contact holes 206, and a thin film resistor 207 is formed. Forming the thin film resistor 207 and the p-type semiconductor Electrical contact; finally, a dielectric layer 208 is deposited and a contact hole 209 is formed, the metal layer 210 and the thin film resistor 207 form an electrical contact, and 211 is a contact electrode. Where the substrate 201 is a transparent or translucent material, the metal layer 210 may be a transparent or translucent material.
所述紫外光雪崩管成像阵列像元(以下简称 UV-APD 300)可以由多个 UV-APD 200并联 形成, 如图 3A所示, UV-APD 200-1 , 200-2, 200-3是三个 UV-APD 200, 它们通过金属层 210和共同的接触电极 203-1, 203-2并联在一起, 其基本的工艺过程如图 3C所示: The ultraviolet avalanche tube imaging array pixel (hereinafter referred to as UV-APD 300) may be formed by a plurality of UV-APDs 200 in parallel, as shown in FIG. 3A, UV-APD 200-1, 200-2, 200-3 are Three UV-APDs 200, which are connected in parallel by a metal layer 210 and a common contact electrode 203-1, 203-2, the basic process of which is illustrated in Figure 3C:
步骤 212, 在衬底 201上形成 n型半导体 202以及 p型半导 204, 可以用 MOCVD的方 式外延生长半导体材料; Step 212, forming an n-type semiconductor 202 and a p-type semiconductor 204 on the substrate 201, and epitaxially growing the semiconductor material by MOCVD;
步骤 213, 刻蚀 p型半导体, 在 n型半导体上形成接触电极 203-1和 203-2, 接触电极可 以通过金属线连接在一起作为一个接触电极; Step 213, etching a p-type semiconductor, forming contact electrodes 203-1 and 203-2 on the n-type semiconductor, and the contact electrodes may be connected together by a metal line as a contact electrode;
步骤 214, 淀积钝化层 205并刻蚀形成接触孔 206; Step 214, depositing a passivation layer 205 and etching to form a contact hole 206;
步骤 215, 淀积并刻蚀形成薄膜电阻 207-1, 207-2和 207-3; Step 215, depositing and etching to form thin film resistors 207-1, 207-2 and 207-3;
步骤 216, 淀积介质层 208并形成接触孔 209; Step 216, depositing a dielectric layer 208 and forming a contact hole 209;
步骤 217, 淀积金属层 210并与薄膜电阻形成电接触, 金属层 210构成另一个电极 301。 Step 217, depositing a metal layer 210 and making electrical contact with the film resistor, and the metal layer 210 constitutes another electrode 301.
UV-APD 300的等效电路图如图 3D所示, UV-APD 300是由多个 UV-APD 200并联形成, 所有的 UV-APD 200的阴极通过金属层 210连接在一起构成一个电极, 接触电极 203连接在 一起构成另一个电极。这样构成的 UV-APD 300实际上是由多个 UV-APD 200单元并联构成。 在前面提到由于 GaN和 AlGaN材料本身缺陷密度很大,故 GaN和 AlGaN基雪崩管的良率 Y 很低, 如果 UV-APD 300由合适个数的 UV-APD 200并联构成, 则 UV-APD 300中总有一定 个数品质好的 UV-APD 200,这样 UV-APD 300总能对光信号进行探测,故这种结构的紫外光 雪崩管成像阵列像元良率接近于 100%, 能够实现紫外光雪崩管成像阵列, 克服了 GaN 和 AlGaN材料本身缺陷密度大而造成的问题。 The equivalent circuit diagram of the UV-APD 300 is shown in FIG. 3D. The UV-APD 300 is formed by a plurality of UV-APDs 200 connected in parallel, and the cathodes of all the UV-APDs 200 are connected together by the metal layer 210 to form an electrode, the contact electrode. The 203 are joined together to form another electrode. The UV-APD 300 thus constructed is actually composed of a plurality of UV-APD 200 units connected in parallel. As mentioned above, the yield Y of GaN and AlGaN-based avalanche tubes is very low due to the high defect density of GaN and AlGaN materials. If UV-APD 300 is composed of a suitable number of UV-APDs 200 in parallel, then UV-APD There are always a certain number of good quality UV-APD 200 in 300, so the UV-APD 300 can always detect the optical signal, so the UV avalanche tube imaging array of this structure has a pixel yield close to 100%, which can be realized. Ultraviolet avalanche tube imaging arrays overcome the problems caused by the high defect density of GaN and AlGaN materials themselves.
紫外光雪崩管成像阵列像元中光电二极管由 m-v族和 /或 π-νι族半导体材料制得,优选 由 GaN, AlGaN或 A1N中的至少一种制得。 The photodiode in the ultraviolet avalanche tube imaging array pixel is made of a m-v family and/or a π-νι group semiconductor material, preferably made of at least one of GaN, AlGaN or A1N.
紫外光雪崩管成像阵列像元中雪崩管探测器单元的半径优选为 1至 50μηι。 The radius of the avalanche tube detector unit in the ultraviolet avalanche tube imaging array pixel is preferably from 1 to 50 μm.
优选每个独立的薄膜电阻的阻值为 100ΚΩ至 10ΜΩ; 优选的薄膜电阻的材料为 SiC或 SixOy。 Preferably, the resistance of each individual thin film resistor is from 100 Ω to 10 Ω; the preferred material of the thin film resistor is SiC or Si x O y .
由于 GaN和 AlGaN材料本身缺陷密度很大, 故 GaN和 AlGaN基雪崩管的良率很低; 在 UV-APD 300中有些 UV-APD 200是坏的, 故在无光加负偏压时, 这些坏的 UV-APD 200就已 经发生雪崩, 这时在电极 301上就有一个电信号 IB, 这个电信号就是暗电流, 我们可以称这 个电流为背底电流; 而那些品质好的 UV-APD 200则能够正常工作。 具体操作中, 所述紫外 光雪崩管成像阵列像元的应用方法为: 在所述紫外光雪崩管成像阵列像元上加负偏压, 使紫 外光雪崩管成像阵列像元工作, 无光时, 测得紫外光雪崩管成像阵列像元电流为 IB, 将它作 为像元背底电流; 有光时, 那些品质好的 UV-APD 200发生雪崩过程从而将光信号转化为电 信号并放大, 测得紫外光雪崩管成像阵列像元电流为 , 则由光产生的倍增电流大小为 IC=IS-IB, 这就是所述紫外光雪崩管成像阵列像元得到的电信号大小。 Since the defect density of GaN and AlGaN materials is large, the yield of GaN and AlGaN-based avalanche tubes is very low; some UV-APDs 200 are bad in UV-APD 300, so when there is no light plus negative bias, these A bad avalanche has occurred in the UV-APD 200. At this time, there is an electrical signal I B on the electrode 301. This electrical signal is a dark current. We can call this current the bottom current; and those of good quality UV-APD 200 will work properly. In a specific operation, the application method of the ultraviolet avalanche tube imaging array pixel is: applying a negative bias voltage to the ultraviolet avalanche tube imaging array pixel, so that the ultraviolet avalanche tube imaging array pixel works, when there is no light The measured photo-current of the ultraviolet avalanche tube imaging array is I B , which is used as the pixel bottom current; when there is light, those good quality UV-APD 200 undergo avalanche process to convert the optical signal into electricity. The signal is amplified and the pixel current of the ultraviolet avalanche tube imaging array is measured. The magnitude of the multiplied current generated by the light is IC=IS-IB, which is the size of the electrical signal obtained by the ultraviolet avalanche tube imaging array pixel.
紫外光雪崩管成像阵列像元工作在线性放大模式或盖革模式(Geiger Mode) [D. Renker, Nuclear Instruments and Methods in Physics Research A 567 (2006) 48-56】下。 所加负偏压大小为 10V到 100V。 Ultraviolet avalanche tube imaging array pixels operate in linear amplification mode or Geiger Mode [D. Renker, Nuclear Instruments and Methods in Physics Research A 567 (2006) 48-56]. The applied negative bias is 10V to 100V.
所述雪崩管成像阵列, 由多个所述的紫外光雪崩管成像阵列像元组成。 The avalanche tube imaging array is composed of a plurality of the ultraviolet avalanche tube imaging array pixels.
由于 UV-APD 300由多个 UV-APD 200并联得到, 可以将 UV-APD 200的面积做的很小, 这样提高了 UV-APD 200的良率, 且不影响 UV-APD 300的感光面积。 如果 UV-APD 300是 由合适个数的 UV-APD200并联构成,则 UV-APD 300中总有一定个数品质好的 UV-APD 200。 如果 GaN 的缺陷密度为 107cm- 2, 且 UV-APD200 的面积为 5χ5μηι2, 则根据良率公式 UV-APD200的良率为 13%, 若 UV-APD 300 由 10x10个 UV-APD 200单元构成, 则像元 UV-APD 300中有 13个 UV-APD 200是品质好的,这样 UV-APD 300总能对光信号进行探测, 故这种结构的紫紫外光雪崩管成像阵列像元良率接近于 100%, 克服了 GaN和 AlGaN材料本 身缺陷密度大而造成的问题。 如图 4所示 UV-APD 300由 16个 UV-APD 200并联构成, 若该 像元中总有品质好的 UV-APD 200,则 UV-APD 300就是一个品质好的成像像元,它能对光信 号进行探测, 并且良率近乎达到了 100%, 可以实现紫外光雪崩管成像阵列。 Since the UV-APD 300 is obtained by connecting a plurality of UV-APDs 200 in parallel, the area of the UV-APD 200 can be made small, which improves the yield of the UV-APD 200 without affecting the photosensitive area of the UV-APD 300. If the UV-APD 300 is composed of a suitable number of UV-APDs 200 in parallel, there is always a certain number of good quality UV-APDs 200 in the UV-APD 300. If the defect density of GaN is 10 7 cm - 2 and the area of UV-APD200 is 5χ5μηι 2 , the yield of UV-APD200 is 13% according to the yield formula, if the UV-APD 300 is composed of 10x10 UV-APD 200 units. The composition, the UV-APD 200 in the pixel UV-APD 300 is of good quality, so that the UV-APD 300 can always detect the optical signal, so the purple ultraviolet avalanche tube imaging array of this structure is good. The rate is close to 100%, which overcomes the problems caused by the high defect density of GaN and AlGaN materials themselves. As shown in FIG. 4, the UV-APD 300 is composed of 16 UV-APDs 200 in parallel. If there is always a good quality UV-APD 200 in the pixel, the UV-APD 300 is a good quality image pixel, which can The optical signal is detected and the yield is nearly 100%, and the ultraviolet avalanche tube imaging array can be realized.
由前面分析得到, 本发明紫外光雪崩管成像阵列像元 UV-APD 300的良率接近于 100%, 所以利用 UV-APD 300作为成像单元, 可以制成雪崩管成像阵列。 如图 5所示, UV-APD ARRAY 500是由 NXN个 UV-APD 300组成的雪崩管成像阵列,在上面提到由于像元 UV-APD 300的良率接近于 100%, 所以成像阵列 UV-APD ARRAY 500中, 所有的像素单元都是品质 好的, 因此本发明所述紫外光雪崩管成像阵列像元 UV-APD 300克服了由于 GaN和 AlGaN 材料本身缺陷密度大而造成的无法实现紫外光雪崩管成像阵列的问题。 As a result of the foregoing analysis, the yield of the ultraviolet avalanche tube imaging array pixel UV-APD 300 of the present invention is close to 100%, so that the avalanche tube imaging array can be fabricated by using the UV-APD 300 as an imaging unit. As shown in FIG. 5, the UV-APD ARRAY 500 is an avalanche tube imaging array composed of NXN UV-APD 300. It is mentioned above that since the yield of the pixel UV-APD 300 is close to 100%, the imaging array UV- In the APD ARRAY 500, all the pixel units are of good quality, so the ultraviolet avalanche tube imaging array pixel UV-APD 300 of the present invention overcomes the inability to achieve ultraviolet light due to the high defect density of the GaN and AlGaN materials themselves. Avalanche tube imaging array problems.
同时本发明提出的新型结构也可以用来制造大感光面积紫外光雪崩管成像阵列像元, 由 于 GaN和 AlGaN材料本身的缺陷密度比较大, 故大面积的紫外光雪崩管非常难制造成功, 但本发明中 UV-APD 300是由多个 UV-APD 200并联构成, 可以将 UV-APD 200的面积做的 很小, 提高了 UV-APD 200的良率, 同时由多个 UV-APD 200构成 UV-APD 300, 使感光面积 增大且不影响良率。 比如我们需要制成 ΙΟΟ Χ ΙΟΟμηι2大小的紫外光雪崩管成像阵列像元, 若 用传统的结构, 其良率不到 1%, 如果采用本发明, 若 UV-APD 200的面积为 5χ5μηι2 (随着 工艺的进步, 尺寸可以做的更小), 则 UV-APD 200的良率是 10%左右, 那么可以用 20x20 个 UV-APD 200构成 UV-APD 300,使像元面积到达 100 X ΙΟΟμηι2,且其良率可以接近于 100%, 这是目前的雪崩管结构无法达到的。 假若材料技术的发展使得 AlGaN和 GaN等材料的缺陷 密度减小, 那么制造同样 50 Χ 50μηι2大小的紫外光雪崩管成像阵列像元, 传统结构的良率与 本发明紫外光雪崩管成像阵列像元的良率随缺陷密度的关系如图 6所示 (图中本发明紫外光 雪崩管成像阵列像元由 10x10个 5χ5μηι2大小的 UV-APD 200单元构成), 可以发现只有当 AlGaN和 GaN材料的缺陷密度减小到 104cm- 2时, 传统结构的紫外光雪崩管的良率才能与本 发明相比拟。 所以利用本发明提出的紫外光雪崩管成像阵列像元结构, 可以制成大感光面积 的紫外光雪崩管像元, 且避免了由于面积较大而导致良率下降的问题。 At the same time, the novel structure proposed by the present invention can also be used to fabricate a large photosensitive area ultraviolet avalanche tube imaging array pixel. Since the defect density of the GaN and AlGaN materials themselves is relatively large, a large-area ultraviolet avalanche tube is very difficult to manufacture, but In the present invention, the UV-APD 300 is composed of a plurality of UV-APDs 200 in parallel, which can make the area of the UV-APD 200 small, improve the yield of the UV-APD 200, and is composed of a plurality of UV-APDs 200. UV-APD 300 increases the photosensitive area without affecting the yield. For example, we need to make a UV avalanche tube imaging array pixel of the size of ΙΟΟ ΙΟΟ ημηι 2. If the conventional structure is used, the yield is less than 1%. If the invention is used, if the area of the UV-APD 200 is 5χ5μηι 2 ( As the process progresses, the size can be made smaller.) The yield of UV-APD 200 is about 10%, then 20-20 UV-APD 200 can be used to form UV-APD 300, so that the pixel area reaches 100 X ΙΟΟμηι 2 , and its yield can be close to 100%, which is not possible with the current avalanche tube structure. If the development of material technology causes the defect density of materials such as AlGaN and GaN to be reduced, then the same 50 Χ 50μηι 2 size ultraviolet avalanche tube imaging array pixel, the yield of the conventional structure and the ultraviolet avalanche tube imaging array image of the present invention are produced. The relationship between the yield of the element and the defect density is shown in Fig. 6 (the UV avalanche tube imaging array of the present invention is composed of 10 x 10 5 χ 5 μη 2 sized UV-APD 200 cells), and it can be found only when AlGaN and GaN materials are used. When the defect density is reduced to 10 4 cm -2 , the yield of the conventional structured ultraviolet avalanche tube can be compared with the present invention. Therefore, by using the ultraviolet avalanche tube imaging array pixel structure proposed by the present invention, a large photosensitive area can be made. The UV avalanche tube cell avoids the problem of a drop in yield due to the large area.
本发明的有效效果为: The effective effects of the present invention are:
本发明所述紫外光雪崩管成像阵列像元结构克服了 GaN, AlGaN等多缺陷材料本身缺陷 密度大而造成的良率过低的问题, 该新型结构紫外光雪崩管成像阵列像元良率可以接近并达 到 100%,利用该紫外光雪崩管成像阵列像元作为成像单元,可以制成紫外光雪崩管成像阵列。 本发明中紫外光雪崩管成像阵列像元结构克服了大面积雪崩管良率过低的问题, 该紫外 光雪崩管成像阵列像元可以由几十或者数百个较小的基本单元结构 UV-APD 200组成, 所以 可以制成大感光面积的紫外光雪崩管成像阵列像元,且没有因为面积过大而良率降低的问题。 附图说明 图 1为现有技术中 AlGaN材料传统结构雪崩管探测器良率与器件面积的关系; 图 2A为典型的硅基 MRS结构雪崩管探测器结构示意图; The ultraviolet avalanche tube imaging array pixel structure of the invention overcomes the problem that the defect density of the multi-defective material such as GaN, AlGaN and the like is too high, and the yield of the novel structure ultraviolet avalanche tube imaging array can be improved. Approaching and reaching 100%, using the ultraviolet avalanche tube imaging array pixel as an imaging unit, an ultraviolet avalanche tube imaging array can be fabricated. In the present invention, the ultraviolet avalanche tube imaging array pixel structure overcomes the problem of low yield of a large area avalanche tube, and the ultraviolet avalanche tube imaging array pixel can be composed of tens or hundreds of smaller basic unit structures UV- The APD 200 is composed, so that a large a photosensitive area of the ultraviolet avalanche tube imaging array pixel can be made, and there is no problem that the yield is lowered because the area is too large. BRIEF DESCRIPTION OF THE DRAWINGS FIG. 1 is a diagram showing the relationship between the yield of a conventional avalanche tube detector and the device area of a conventional AlGaN material; FIG. 2A is a schematic view showing the structure of a typical silicon-based MRS avalanche tube detector;
图 2B为图 1A中描述的硅基 MRS结构雪崩管探测器的等效电路图; 2B is an equivalent circuit diagram of the silicon-based MRS structure avalanche tube detector described in FIG. 1A;
图 3A为本发明一种紫外光雪崩管成像阵列像元的结构示意图; 3A is a schematic structural view of an ultraviolet avalanche tube imaging array pixel according to the present invention;
图 3B为图 3A中紫外光雪崩管成像阵列像元中的基本组成单元结构示意图; 3B is a schematic structural diagram of a basic constituent unit in the ultraviolet avalanche tube imaging array pixel of FIG. 3A;
图 3C为图 3A中紫外光雪崩管成像阵列像元的基本工艺过程; 3C is a basic process of the ultraviolet avalanche tube imaging array pixel of FIG. 3A;
图 3D为图 3A中紫外光雪崩管成像阵列像元的等效电路图; 3D is an equivalent circuit diagram of the ultraviolet avalanche tube imaging array pixel of FIG. 3A;
图 4为本发明一种具体的紫外光雪崩管成像阵列像元的结构示意图; 4 is a schematic structural view of a specific ultraviolet avalanche tube imaging array pixel according to the present invention;
图 5为本发明一种雪崩管成像阵列; Figure 5 is an avalanche tube imaging array of the present invention;
图 6为面积为 50 Χ 50μηι2的传统结构雪崩管探测器良率与本发明紫外光雪崩管成像阵列 像元的良率对比图。 具体实施方式 如图 3Α所示是本发明所述紫外光雪崩管成像阵列像元的一个示意图。 若所述紫外光雪崩管成像阵列像元 UV-APD 300由多个基本单元 UV-APD 200 (如图 3Β) 并联构成, UV-APD 200的半径可以为 Ιμηι到 50μηι。 在图 3Β中, 我们可以由下而上形成 衬底 201, 衬底 201可以是 SiC、 蓝宝石以及硅衬底等材料, 但要求衬底透光; n型半导体 202和 p型半导体 204, 材料可以是 GaN, A1N和 AlGaN等材料, 可以采用 MOCVD的方 式外延生长 n型半导体 202和 p型半导体 204, 其中也有缓冲层, 从而降低材料中的晶格位 错, 减小缺陷密度; 然后刻蚀 p型半导体露出部分 n型半导体, 再形成 n型接触电极 203, 电极可以采用 Ti/Au合金等材料; 淀积绝缘钝化层 205并且形成接触孔 206, 钝化层可以用 氧化物等材料; 淀积形成薄膜电阻 207使薄膜电阻 207和 p型半导体形成电接触, 薄膜电阻 207可以采用 SiC或 SixOy等材料, 其电阻值约为几百 ΚΩ到 1ΜΩ; 淀积介质层 208和形成 接触孔 209, 金属层 210和薄膜电阻 207形成电接触, 211是接触电极。 Figure 6 is a graph comparing the yield of a conventional structured avalanche tube detector with an area of 50 Χ 50 μηι 2 and the yield of the ultraviolet avalanche tube imaging array of the present invention. DETAILED DESCRIPTION OF THE INVENTION A schematic view of an ultraviolet avalanche tube imaging array pixel of the present invention is shown in FIG. If the ultraviolet avalanche tube imaging array pixel UV-APD 300 is composed of a plurality of basic units UV-APD 200 (as shown in FIG. 3A), the radius of the UV-APD 200 may be Ιμηι to 50μηι. In FIG. 3A, we can form the substrate 201 from bottom to top. The substrate 201 can be a material such as SiC, sapphire, or silicon substrate, but requires the substrate to transmit light; the n-type semiconductor 202 and the p-type semiconductor 204, the material can be It is a material such as GaN, A1N or AlGaN. The n-type semiconductor 202 and the p-type semiconductor 204 can be epitaxially grown by MOCVD, and a buffer layer is also formed, thereby reducing lattice dislocations in the material and reducing the defect density; and then etching p The semiconductor is exposed to a portion of the n-type semiconductor, and then the n-type contact electrode 203 is formed. The electrode may be made of a material such as a Ti/Au alloy; the insulating passivation layer 205 is deposited and a contact hole 206 is formed, and the passivation layer may be made of an oxide or the like; Forming the thin film resistor 207 to make the thin film resistor 207 and the p-type semiconductor form electrical contact, the thin film resistor 207 may be made of a material such as SiC or Si x O y having a resistance value of about several hundred Ω Ω to 1 Μ Ω; a dielectric layer 208 is deposited and a contact hole 209 is formed, the metal layer 210 and the thin film resistor 207 are in electrical contact, and 211 is a contact electrode.
本发明紫外光雪崩管成像阵列像元 UV-APD 300可以由数十个到数百个 UV-APD 200构 成, 若构成 ΙΟΟ Χ ΙΟΟμηι2大小的紫外光雪崩管成像阵列像元, 可以用 20 X 20个面积为 5 X 5μηι2大小的 UV-APD 200构成, 其工艺流程如图 3C所示。 The ultraviolet avalanche tube imaging array pixel UV-APD 300 of the present invention can be composed of tens to hundreds of UV-APD 200s, and if it constitutes an ultraviolet avalanche tube imaging array pixel of the size ΙΟΟ ΙΟΟ ΙΟΟμηι 2 , 20 X can be used. 20 UV-APD 200s with an area of 5 X 5 μm 2 are formed, and the process flow is shown in FIG. 3C.
简单的工艺流程为: The simple process flow is:
在衬底 201上形成 n型半导体 202以及 p型半导 204, 可以用 MOCVD的方式外延生长 GaN, A1N和 AlGaN等半导体材料; An n-type semiconductor 202 and a p-type semiconductor 204 are formed on the substrate 201, and a semiconductor material such as GaN, A1N or AlGaN can be epitaxially grown by MOCVD;
刻蚀 p型半导体 204, 形成多个光电二极管阵列结构, 阵列大小为 20 X 20, 光电二极管 的面积为 5 Χ 5μηι2。 The p-type semiconductor 204 is etched to form a plurality of photodiode array structures having an array size of 20 X 20 and a photodiode having an area of 5 Χ 5 μηι 2 .
然后在 η型半导体 202上形成接触电极 203, 所有的 η型接触电极 203可以通过金属线 连接在一起作为紫外光雪崩光成像阵列像元的一个电极; Then, a contact electrode 203 is formed on the n-type semiconductor 202, and all of the n-type contact electrodes 203 may be connected together by a metal line as an electrode of the ultraviolet avalanche photoimageable array pixel;
淀积绝缘钝化层 205并在光电二极管单元上方刻蚀形成接触孔 206; Depositing an insulating passivation layer 205 and etching over the photodiode unit to form a contact hole 206;
淀积并刻蚀形成 20 X 20个薄膜电阻 207, 薄膜电阻通过接触孔与相应的光电二极管单元 形成电接触; Depositing and etching to form 20 X 20 thin film resistors 207, and the thin film resistors make electrical contact with the corresponding photodiode cells through the contact holes;
淀积介质层 208并在所有的薄膜电阻 207上方刻蚀形成接触孔 209; Depositing dielectric layer 208 and etching over all of the thin film resistors 207 to form contact holes 209;
淀积金属层 210并通过接触孔 209与所有的薄膜电阻 207形成电接触, 金属层 210构成 另一个电极 211。 The metal layer 210 is deposited and electrically contacted with all of the thin film resistors 207 through the contact holes 209, and the metal layer 210 constitutes the other electrode 211.
前面诉述 100 X ΙΟΟμηι2大小紫外光雪崩管成像阵列像元 UV-APD 300在具体操作时, 电 极 301上加上负偏压 Vbias, 使像元 UV-APD 300工作在线性放大模式或者 Geiger Mode下, 其电压大小可以为 10V至 100V, 根据不同的掺杂浓度以及工艺参数, 其工作电压亦不同。 无光时, 在电极 301上测得像元 UV-APD 300的电流大小为 IB, 这是紫外光雪崩管成像阵列 像元 UV-APD 300的背底电流; 有光时, 在电极 301上测得雪崩管的电流为 Is, 则由光信号 转化成的电流的大小为: The foregoing describes a 100 X ΙΟΟμηι 2 size ultraviolet avalanche tube imaging array pixel UV-APD 300. In specific operation, a negative bias voltage Vbias is applied to the electrode 301, so that the pixel UV-APD 300 operates in linear amplification mode or Geiger Mode. The voltage can range from 10V to 100V. The operating voltage varies according to different doping concentrations and process parameters. When there is no light, the current of the pixel UV-APD 300 measured on the electrode 301 is I B , which is the background current of the ultraviolet avalanche tube imaging array pixel UV-APD 300; when there is light, on the electrode 301 When the current of the avalanche tube is measured as I s , the magnitude of the current converted by the optical signal is:
IC=IS-IB IC=IS-IB
即 Ic为雪崩管像元 UV-APD 300读出的电信号的大小。 That is, I c is the size of the electrical signal read by the avalanche tube cell UV-APD 300.
Claims
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