TW202218178A - Nitride semiconductor ultraviolet light emitting element - Google Patents
Nitride semiconductor ultraviolet light emitting element Download PDFInfo
- Publication number
- TW202218178A TW202218178A TW110126567A TW110126567A TW202218178A TW 202218178 A TW202218178 A TW 202218178A TW 110126567 A TW110126567 A TW 110126567A TW 110126567 A TW110126567 A TW 110126567A TW 202218178 A TW202218178 A TW 202218178A
- Authority
- TW
- Taiwan
- Prior art keywords
- layer
- type
- region
- algan
- aln
- Prior art date
Links
- 239000004065 semiconductor Substances 0.000 title claims abstract description 216
- 150000004767 nitrides Chemical class 0.000 title claims abstract description 97
- 229910002704 AlGaN Inorganic materials 0.000 claims abstract description 332
- 239000000203 mixture Substances 0.000 claims abstract description 144
- 230000004888 barrier function Effects 0.000 claims description 307
- 239000000758 substrate Substances 0.000 claims description 51
- 229910052594 sapphire Inorganic materials 0.000 claims description 41
- 239000010980 sapphire Substances 0.000 claims description 41
- 239000000463 material Substances 0.000 claims description 24
- WGPCGCOKHWGKJJ-UHFFFAOYSA-N sulfanylidenezinc Chemical group [Zn]=S WGPCGCOKHWGKJJ-UHFFFAOYSA-N 0.000 claims description 3
- 210000000746 body region Anatomy 0.000 abstract description 19
- 229910052984 zinc sulfide Inorganic materials 0.000 abstract 1
- 239000010410 layer Substances 0.000 description 886
- 238000005253 cladding Methods 0.000 description 162
- 239000013078 crystal Substances 0.000 description 51
- 238000001228 spectrum Methods 0.000 description 50
- 239000010408 film Substances 0.000 description 49
- 239000000969 carrier Substances 0.000 description 45
- 229910052782 aluminium Inorganic materials 0.000 description 30
- 229910052733 gallium Inorganic materials 0.000 description 30
- 239000012535 impurity Substances 0.000 description 25
- 238000000034 method Methods 0.000 description 20
- 238000005259 measurement Methods 0.000 description 19
- 230000007423 decrease Effects 0.000 description 15
- 239000007789 gas Substances 0.000 description 13
- 238000004020 luminiscence type Methods 0.000 description 13
- 238000004519 manufacturing process Methods 0.000 description 13
- 230000000694 effects Effects 0.000 description 12
- 230000015572 biosynthetic process Effects 0.000 description 11
- 230000004807 localization Effects 0.000 description 11
- 230000006798 recombination Effects 0.000 description 11
- 238000012546 transfer Methods 0.000 description 10
- 238000004458 analytical method Methods 0.000 description 9
- 238000010586 diagram Methods 0.000 description 9
- 238000010894 electron beam technology Methods 0.000 description 9
- 229910021478 group 5 element Inorganic materials 0.000 description 8
- 238000005215 recombination Methods 0.000 description 8
- 238000005204 segregation Methods 0.000 description 7
- 238000000731 high angular annular dark-field scanning transmission electron microscopy Methods 0.000 description 6
- 238000002513 implantation Methods 0.000 description 6
- 229910052950 sphalerite Inorganic materials 0.000 description 6
- 239000012159 carrier gas Substances 0.000 description 5
- 238000009792 diffusion process Methods 0.000 description 5
- 238000002149 energy-dispersive X-ray emission spectroscopy Methods 0.000 description 5
- 239000002994 raw material Substances 0.000 description 5
- 238000005001 rutherford backscattering spectroscopy Methods 0.000 description 5
- 238000000354 decomposition reaction Methods 0.000 description 4
- 238000005530 etching Methods 0.000 description 4
- 229910052751 metal Inorganic materials 0.000 description 4
- 239000002184 metal Substances 0.000 description 4
- 230000000737 periodic effect Effects 0.000 description 4
- 238000002360 preparation method Methods 0.000 description 4
- 239000011347 resin Substances 0.000 description 4
- 229920005989 resin Polymers 0.000 description 4
- 238000004088 simulation Methods 0.000 description 4
- 239000000126 substance Substances 0.000 description 4
- 230000001629 suppression Effects 0.000 description 4
- 238000001947 vapour-phase growth Methods 0.000 description 4
- 238000000151 deposition Methods 0.000 description 3
- 229910052738 indium Inorganic materials 0.000 description 3
- 238000010884 ion-beam technique Methods 0.000 description 3
- 150000002736 metal compounds Chemical class 0.000 description 3
- 229910052757 nitrogen Inorganic materials 0.000 description 3
- 238000001878 scanning electron micrograph Methods 0.000 description 3
- 238000012360 testing method Methods 0.000 description 3
- 239000010409 thin film Substances 0.000 description 3
- IJGRMHOSHXDMSA-UHFFFAOYSA-N Atomic nitrogen Chemical compound N#N IJGRMHOSHXDMSA-UHFFFAOYSA-N 0.000 description 2
- 229910052796 boron Inorganic materials 0.000 description 2
- 230000008859 change Effects 0.000 description 2
- 230000003247 decreasing effect Effects 0.000 description 2
- 230000007547 defect Effects 0.000 description 2
- 238000010438 heat treatment Methods 0.000 description 2
- 230000006872 improvement Effects 0.000 description 2
- 150000002902 organometallic compounds Chemical class 0.000 description 2
- 238000012545 processing Methods 0.000 description 2
- 230000001737 promoting effect Effects 0.000 description 2
- 238000000851 scanning transmission electron micrograph Methods 0.000 description 2
- XCZXGTMEAKBVPV-UHFFFAOYSA-N trimethylgallium Chemical compound C[Ga](C)C XCZXGTMEAKBVPV-UHFFFAOYSA-N 0.000 description 2
- QGZKDVFQNNGYKY-UHFFFAOYSA-N Ammonia Chemical compound N QGZKDVFQNNGYKY-UHFFFAOYSA-N 0.000 description 1
- ZOKXTWBITQBERF-UHFFFAOYSA-N Molybdenum Chemical compound [Mo] ZOKXTWBITQBERF-UHFFFAOYSA-N 0.000 description 1
- 238000000137 annealing Methods 0.000 description 1
- 229910052785 arsenic Inorganic materials 0.000 description 1
- RQNWIZPPADIBDY-UHFFFAOYSA-N arsenic atom Chemical compound [As] RQNWIZPPADIBDY-UHFFFAOYSA-N 0.000 description 1
- 238000004140 cleaning Methods 0.000 description 1
- 239000011247 coating layer Substances 0.000 description 1
- 238000005566 electron beam evaporation Methods 0.000 description 1
- 238000000295 emission spectrum Methods 0.000 description 1
- 230000001747 exhibiting effect Effects 0.000 description 1
- 238000000605 extraction Methods 0.000 description 1
- 238000012423 maintenance Methods 0.000 description 1
- 230000005012 migration Effects 0.000 description 1
- 238000013508 migration Methods 0.000 description 1
- 238000012986 modification Methods 0.000 description 1
- 230000004048 modification Effects 0.000 description 1
- 229910052750 molybdenum Inorganic materials 0.000 description 1
- 239000011733 molybdenum Substances 0.000 description 1
- 230000002093 peripheral effect Effects 0.000 description 1
- 238000001020 plasma etching Methods 0.000 description 1
- -1 polysiloxane Polymers 0.000 description 1
- 229920001296 polysiloxane Polymers 0.000 description 1
- 230000035755 proliferation Effects 0.000 description 1
- 230000001681 protective effect Effects 0.000 description 1
- 230000009467 reduction Effects 0.000 description 1
- 230000004044 response Effects 0.000 description 1
- 125000006850 spacer group Chemical group 0.000 description 1
- 230000000087 stabilizing effect Effects 0.000 description 1
- 238000013517 stratification Methods 0.000 description 1
- 230000007704 transition Effects 0.000 description 1
- JLTRXTDYQLMHGR-UHFFFAOYSA-N trimethylaluminium Chemical compound C[Al](C)C JLTRXTDYQLMHGR-UHFFFAOYSA-N 0.000 description 1
- 238000007740 vapor deposition Methods 0.000 description 1
Images
Classifications
-
- H—ELECTRICITY
- H01—ELECTRIC ELEMENTS
- H01L—SEMICONDUCTOR DEVICES NOT COVERED BY CLASS H10
- H01L33/00—Semiconductor devices having potential barriers specially adapted for light emission; Processes or apparatus specially adapted for the manufacture or treatment thereof or of parts thereof; Details thereof
- H01L33/02—Semiconductor devices having potential barriers specially adapted for light emission; Processes or apparatus specially adapted for the manufacture or treatment thereof or of parts thereof; Details thereof characterised by the semiconductor bodies
- H01L33/16—Semiconductor devices having potential barriers specially adapted for light emission; Processes or apparatus specially adapted for the manufacture or treatment thereof or of parts thereof; Details thereof characterised by the semiconductor bodies with a particular crystal structure or orientation, e.g. polycrystalline, amorphous or porous
- H01L33/18—Semiconductor devices having potential barriers specially adapted for light emission; Processes or apparatus specially adapted for the manufacture or treatment thereof or of parts thereof; Details thereof characterised by the semiconductor bodies with a particular crystal structure or orientation, e.g. polycrystalline, amorphous or porous within the light emitting region
-
- H—ELECTRICITY
- H01—ELECTRIC ELEMENTS
- H01L—SEMICONDUCTOR DEVICES NOT COVERED BY CLASS H10
- H01L33/00—Semiconductor devices having potential barriers specially adapted for light emission; Processes or apparatus specially adapted for the manufacture or treatment thereof or of parts thereof; Details thereof
- H01L33/02—Semiconductor devices having potential barriers specially adapted for light emission; Processes or apparatus specially adapted for the manufacture or treatment thereof or of parts thereof; Details thereof characterised by the semiconductor bodies
- H01L33/20—Semiconductor devices having potential barriers specially adapted for light emission; Processes or apparatus specially adapted for the manufacture or treatment thereof or of parts thereof; Details thereof characterised by the semiconductor bodies with a particular shape, e.g. curved or truncated substrate
- H01L33/22—Roughened surfaces, e.g. at the interface between epitaxial layers
-
- H—ELECTRICITY
- H01—ELECTRIC ELEMENTS
- H01L—SEMICONDUCTOR DEVICES NOT COVERED BY CLASS H10
- H01L33/00—Semiconductor devices having potential barriers specially adapted for light emission; Processes or apparatus specially adapted for the manufacture or treatment thereof or of parts thereof; Details thereof
- H01L33/02—Semiconductor devices having potential barriers specially adapted for light emission; Processes or apparatus specially adapted for the manufacture or treatment thereof or of parts thereof; Details thereof characterised by the semiconductor bodies
- H01L33/26—Materials of the light emitting region
- H01L33/30—Materials of the light emitting region containing only elements of Group III and Group V of the Periodic Table
- H01L33/32—Materials of the light emitting region containing only elements of Group III and Group V of the Periodic Table containing nitrogen
Landscapes
- Engineering & Computer Science (AREA)
- Manufacturing & Machinery (AREA)
- Computer Hardware Design (AREA)
- Microelectronics & Electronic Packaging (AREA)
- Power Engineering (AREA)
- Led Devices (AREA)
Abstract
Description
本發明係有關具備閃鋅礦構造之AlGaN系半導體所成n型層、活性層、及p型層,層積於上下方向之發光元件構造部而成之氮化物半導體紫外線發光元件。The present invention relates to a nitride semiconductor ultraviolet light emitting element formed of an AlGaN-based semiconductor having a sphalerite structure, an n-type layer, an active layer, and a p-type layer, which are laminated on a light-emitting element structure portion in the vertical direction.
一般而言,多數存在氮化物半導體發光元件係於藍寶石等之基板上,經由磊晶成長,形成複數之氮化物半導體層所成發光元件構造者。氮化物半導體層係以一般式Al 1-x-yGa xIn yN(0≦x≦1,0≦y≦1,0≦x+y≦1)加以表示。 Generally speaking, there are many nitride semiconductor light-emitting elements that are formed by epitaxial growth on a substrate such as sapphire to form a plurality of nitride semiconductor layers to form a light-emitting element structure. The nitride semiconductor layer is represented by the general formula Al 1-xy Ga x In y N (0≦x≦1,0≦y≦1,0≦x+y≦1).
發光二極體之發光元件構造係於n型氮化物半導體層與p型氮化物半導體層之2個包覆層之間,具有挾持有經由氮化物半導體層所成活性層之雙異質構造。活性層為AlGaN系半導體之時,經由調整AlN莫耳分率(亦稱為Al組成比),將能帶隙能量,調整在將GaN與AlN所取得能帶隙能量(約3.4eV與約6.2eV)各別成為下限及上限之範圍內,得發光波長約200nm至約365nm之紫外線發光元件。具體而言,藉由自p型氮化物半導體層朝向n型氮化物半導體層,流動順方向電流,於活性層,產生載體(電子及電洞)之再結合所成對應上述能帶隙能量之發光。將該順方向電流從外部供給之故,於p型氮化物半導體層上,設置p電極,於n型氮化物半導體層上,設置n電極。The light-emitting element structure of the light-emitting diode is between the two cladding layers of the n-type nitride semiconductor layer and the p-type nitride semiconductor layer, and has a double-heterostructure in which an active layer formed through the nitride semiconductor layer is sandwiched. When the active layer is an AlGaN-based semiconductor, by adjusting the AlN molar ratio (also called the Al composition ratio), the bandgap energy is adjusted to the bandgap energy obtained by combining GaN and AlN (about 3.4eV and about 6.2eV). eV) is within the range of the lower limit and the upper limit, respectively, and an ultraviolet light emitting element with an emission wavelength of about 200 nm to about 365 nm can be obtained. Specifically, by flowing a forward current from the p-type nitride semiconductor layer toward the n-type nitride semiconductor layer, in the active layer, the recombination of carriers (electrons and holes) is generated, which corresponds to the above-mentioned energy band gap energy. glow. Since the forward current is supplied from the outside, a p-electrode is provided on the p-type nitride semiconductor layer, and an n-electrode is provided on the n-type nitride semiconductor layer.
活性層為AlGaN系半導體之時,挾有活性層之n型氮化物半導體層與p型氮化物半導體層係以較活性層高AlN莫耳分率之AlGaN系半導體加以構成。但是,高AlN莫耳分率之p型氮化物半導體層係難以形成與p電極良好之歐姆接觸之故,於p型氮化物半導體層之最上層,一般進行形成可與低AlN莫耳分率之p型AlGaN系半導體(具體而言p-GaN)所成p電極良好歐姆接觸之p型連接層。此p型連接層係AlN莫耳分率較構成活性層之AlGaN系半導體為小之故,從活性層朝向p型氮化物半導體層側射出之紫外線係在該p型連接層被吸收,無法有效取出至元件外部。為此,活性層為AlGaN系半導體之一般之紫外線發光二極體係採用圖22模式性顯示元件構造,可將自活性層朝向n型氮化物半導體層側射出之紫外線,有效取出至元件外部(例如參照下述之專利文獻1及2等)。When the active layer is an AlGaN-based semiconductor, the n-type nitride semiconductor layer and the p-type nitride semiconductor layer sandwiching the active layer are composed of an AlGaN-based semiconductor having a higher molar fraction of AlN than the active layer. However, since it is difficult to form a good ohmic contact with the p-electrode in a p-type nitride semiconductor layer with a high AlN molar ratio, it is generally formed on the uppermost layer of the p-type nitride semiconductor layer, which is compatible with a low AlN molar ratio. The p-type connection layer with good ohmic contact to the p-electrode is made of p-type AlGaN-based semiconductor (specifically, p-GaN). The p-type junction layer is made of AlN with a smaller molar fraction than the AlGaN-based semiconductor constituting the active layer, and the ultraviolet rays emitted from the active layer toward the p-type nitride semiconductor layer are absorbed in the p-type junction layer and cannot be effectively Take out to the outside of the element. For this reason, the general ultraviolet light-emitting diode system in which the active layer is an AlGaN-based semiconductor adopts the schematic display device structure shown in Fig. 22, and the ultraviolet light emitted from the active layer toward the n-type nitride semiconductor layer side can be effectively extracted to the outside of the device (for example, Refer to the following
如圖22所示,一般之紫外線發光二極體係於藍寶石基板等之基板100上,堆積AlGaN系半導體層101(例如,AlN層)形成之模板102上,順序堆積n型AlGaN系半導體層103、活性層104、p型AlGaN系半導體層105、及、p型連接層106,將活性層104與p型AlGaN系半導體層105與p型連接層106之一部分,直至露出n型AlGaN系半導體層103進行蝕刻除去,於n型AlGaN系半導體層103之露出面,將n電極107,在於p型連接層106之表面,各別形成p電極108而構成。As shown in FIG. 22, a general ultraviolet light emitting diode system is deposited on a
又,為提高活性層內之載子再結合所成發光效率(內部量子效率),實施將活性層成為多重量子井構造,於活性層上,設置電子阻障層等。In addition, in order to improve the luminous efficiency (internal quantum efficiency) formed by the recombination of carriers in the active layer, the active layer is formed into a multiple quantum well structure, and an electron barrier layer is provided on the active layer.
另一方面,有報告顯示於以n型AlGaN系半導體層構成之包覆層內,產生Ga偏析(伴隨Ga之質量移動之偏析)造成之組成調製,對於包覆層表面在向斜方向延伸之局部,形成AlN莫耳分率低之層狀領域(例如,參照下述之專利文獻3、非專利文獻1、2等)。局部AlN莫耳分率低之AlGaN系半導體層係能帶隙能量亦局部變小之故,於專利文獻3中,有報告顯示該包覆層內之載子則易於局部存在化於層狀領域,可對於活性層提供低阻抗之電流路徑,可達成紫外線發光二極體之發光效率的提升。層狀領域之上述特徵係在從圖23所示以往之氮化物半導體紫外線發光元件之n型包覆層至電子阻障層之半導體層之高角度環形暗場(HAADF)-STEM像中亦被確認。HAADF-STEM像係可得得比例於原子量之對比,重元素係被明亮顯示。因此,AlN莫耳分率低之領域係相對地被明亮顯示。HAADF-STEM像係較通常之STEM像(明視野像),更適於AlN莫耳分率之差之觀察。
[先前技術文獻]
[專利文獻]
On the other hand, it has been reported that in the cladding layer composed of the n-type AlGaN-based semiconductor layer, the composition modulation caused by Ga segregation (segregation accompanying the mass shift of Ga) occurs, and the surface of the cladding layer extends in the syncline direction. Partially, a layered area with a low AlN molar ratio is formed (for example, refer to the following
[專利文獻1]國際公開第2014/178288號公報 [專利文獻2]國際公開第2016/157518號公報 [專利文獻3]國際公開第2019/159265號公報 [非專利文獻] [Patent Document 1] International Publication No. 2014/178288 [Patent Document 2] International Publication No. 2016/157518 [Patent Document 3] International Publication No. 2019/159265 [Non-patent literature]
[非專利文獻1]Y. Nagasawa, et al., "Comparison of Al xGa 1−xN multiple quantum wells designed for 265 and 285nm deep-ultraviolet LEDs grown on AlN templates having macrosteps", Applied Physics Express 12, 064009 (2019) [非專利文獻2]K. Kojima, et al., "Carrier localization structure combined with current micropaths in AlGaN quantum wells grown on an AlN template with macrosteps", Applied Physics letter 114, 011102 (2019) [Non-Patent Literature 1] Y. Nagasawa, et al., "Comparison of Al x Ga 1−x N multiple quantum wells designed for 265 and 285nm deep-ultraviolet LEDs grown on AlN templates having macrosteps", Applied Physics Express 12, 064009 (2019) [Non-Patent Literature 2] K. Kojima, et al., "Carrier localization structure combined with current micropaths in AlGaN quantum wells grown on an AlN template with macrosteps", Applied Physics letter 114, 011102 (2019)
[發明欲解決之課題][The problem to be solved by the invention]
以AlGaN系半導體構成之紫外線發光元件係於藍寶石基板等之基板上,例如經由有機金屬化合物氣相成長(MOVPE)法等之周知之磊晶成長法加以製作。但是,生產紫外線發光元件之時,紫外線發光元件之特性(發光波長、插座效率、順方向偏壓等之特性)係接受結晶成長裝置之漂移之影響而變動之故,不一定容易以安定之產率加以生產。The ultraviolet light-emitting element made of AlGaN-based semiconductor is fabricated on a substrate such as a sapphire substrate, for example, by a well-known epitaxial growth method such as an organometallic compound vapor deposition (MOVPE) method. However, when producing an ultraviolet light emitting element, the characteristics of the ultraviolet light emitting element (emission wavelength, socket efficiency, forward bias, etc.) are affected by the drift of the crystal growth device, so stable production is not necessarily easy. rate to be produced.
結晶成長裝置之漂移係承載盤或處理室之壁等之附著物之原因,起因於改變結晶成長部位之實效溫度等而產生。為此,為抑制漂移,以往係檢討成長履歷,雖然有經驗者經由微妙改變設定溫度或原料氣體之組成,或固定一定期間之成長歷程,清掃等之維護亦在一定期間同樣加以實施等之努力,但仍難以完全排除漂移。The drift of the crystal growth device is caused by the attachment of the carrier plate or the wall of the processing chamber, etc., which is caused by changing the effective temperature of the crystal growth site. For this reason, in order to suppress drift, the growth history has been reviewed in the past. Although experienced persons have made efforts such as subtly changing the set temperature or the composition of the raw material gas, or fixing the growth history for a certain period of time, maintenance such as cleaning is also carried out for a certain period of time. , but it is still difficult to completely rule out drift.
本發明係有鑑於上述之問題點而成,該目的係提供可進行起因於結晶成長裝置之漂移等之舟性變動之被抑制之安定生產之氮化物半導體紫外線發光元件。 [為解決課題之手段] The present invention has been made in view of the above-mentioned problems, and an object thereof is to provide a nitride semiconductor ultraviolet light emitting device that can perform stable production with suppressed boating fluctuations due to drift of a crystal growth apparatus. [Means for solving problems]
本發明係為達成上述目的,提供具備閃鋅礦構造之AlGaN系半導體所成n型層、活性層、及p型層層積於上下方向之發光元件構造部而成之氮化物半導體紫外線發光元件中, 前述n型層係以n型AlGaN系半導體所構成, 配置於前述n型層與前述p型層之間之前述活性層,則具有包含AlGaN系半導體所構成之1層以上之阱層的量子井構造, 前述p型層係以p型AlGaN系半導體所構成, 前述n型層與前述活性層與前述p型層內之各半導體層則具有形成平行於(0001)面之多段狀之平台之表面的磊晶成長層, 前述活性層內之各半導體層係各別具有對於連結前述多段狀之平台之鄰接之平台間之(0001)面傾斜之傾斜領域、和前述傾斜領域以外之平台領域, 前述n型層具有在前述n型層內一樣地分散存在之局部AlN莫耳分率為低之層狀領域,和前述層狀領域以外之n型本體領域, 與前述n型層之上表面正交之第1平面上之前述層狀領域之各延伸方向,具有對於前述n型層之前述上面與前述第1平面之交線而言傾斜之部分, 整數n為5、6、7、或8, 於前述層狀領域內,存在包含AlGaN組成比成為整數比之Al nGa 12-nN 12之n型AlGaN領域的Ga富化n型領域, 於前述n型本體領域內,存在包含AlGaN組成比成為整數比之Al n+1Ga 11-nN 12之n型AlGaN領域,局部地AlN莫耳分率為高的Al富化n型領域, 前述n型層之平均性AlN莫耳分率Xna成為、(n+0.5)/12<Xna<(n+1)/12之範圍內, 於前述阱層之前述傾斜領域內,存在AlN莫耳分率局部地較前述阱層之前述平台領域之AlN莫耳分率為低之Ga富化阱領域為第1特徵之氮化物半導體紫外線發光元件。 In order to achieve the above object, the present invention provides a nitride semiconductor ultraviolet light-emitting element in which an n-type layer, an active layer, and a p-type layer formed of an AlGaN-based semiconductor having a sphalerite structure are stacked on a light-emitting element structure portion in the vertical direction. Among them, the n-type layer is composed of an n-type AlGaN-based semiconductor, and the active layer disposed between the n-type layer and the p-type layer has a well layer including one or more well layers composed of an AlGaN-based semiconductor. In the quantum well structure, the p-type layer is composed of p-type AlGaN-based semiconductor, the n-type layer, the active layer, and each semiconductor layer in the p-type layer have a multi-segment platform parallel to the (0001) plane. On the surface of the epitaxial growth layer, each semiconductor layer in the active layer has an inclined region that is inclined with respect to the (0001) plane between adjacent platforms connecting the multi-segmented platforms, and a platform region other than the aforementioned inclined region. , the aforementioned n-type layer has a layered domain with a low molar fraction of local AlN equally dispersed in the aforementioned n-type layer, and an n-type bulk domain other than the aforementioned layered domain, and the upper surface of the aforementioned n-type layer. Each extending direction of the layered region on the orthogonal first plane has a portion inclined with respect to the intersection of the upper surface of the n-type layer and the first plane, and the integer n is 5, 6, 7, or 8. In the aforementioned layered domain, there is a Ga - enriched n -type domain including an n-type AlGaN domain where the composition ratio of AlGaN is an integer ratio of AlnGa12 -nN12, and in the aforementioned n-type bulk domain, there is an AlGaN domain The composition ratio becomes the n-type AlGaN region of the integer ratio of Al n+1 Ga 11-n N 12 , the Al-rich n-type region with a high AlN molar fraction locally, the average AlN molar fraction of the aforementioned n-type layer In the range of (n+0.5)/12<Xna<(n+1)/12, in the range of the ratio Xna, in the inclination region of the well layer, the AlN molar ratio is locally higher than the plateau of the well layer. The AlN molar fraction of the field is low in the Ga-enriched well field, which is the nitride semiconductor ultraviolet light emitting device of the first feature.
然而,AlGaN系半導體雖以一般式Al
1-xGa
xN (0≦x≦1)加以表示,令能帶隙能量在可取得GaN與AlN之能帶隙能量,各別成為下限及上限之範圍內,可微量含有B或In等之3族元素或P等之5族元素等之不純物。又,GaN系半導體雖為基本上以Ga與N構成之氮化物半導體,亦可微量含有Al、B或In等之3族元素或P等之5族元素等之不純物。又,AlN系半導體雖為基本上以Al與N構成之氮化物半導體,亦可微量含有Ga、B或In等之3族元素或P等之5族元素等之不純物。因此,本發明中,GaN系半導體及AlN系半導體係各別為AlGaN系半導體之一部分。
However, although the AlGaN-based semiconductor is represented by the general formula Al 1-x Ga x N (0≦x≦1), the energy of the bandgap in which the bandgap energy of GaN and AlN can be obtained is the lower limit and the upper limit, respectively. Within the range, impurities such as
更且,n型或p型AlGaN系半導體係作為供體或受體不純物,摻雜Si或Mg等之AlGaN系半導體。本發明中,未明記p型及n型之AlGaN系半導體係意味未摻雜之AlGaN系半導體,但即使未摻雜,可含有不可避免混入程度之微量之供體或受體不純物。又,第1平面係非在前述n型層之製造過程中,與具體形成之露出面或其他之半導體層之邊界面,為將前述n型層內平行延伸於上下方向之假想平面。更且,於本說明書中,AlGaN系半導體層、GaN系半導體層及AlN系半導體層係各別以AlGaN系半導體、GaN系半導體及AlN系半導體加以構成之半導體層。Furthermore, an n-type or p-type AlGaN-based semiconductor is an AlGaN-based semiconductor doped with Si or Mg as a donor or acceptor impurity. In the present invention, p-type and n-type AlGaN-based semiconductors that are not specified means undoped AlGaN-based semiconductors, but even undoped, they may contain trace amounts of donor or acceptor impurities to an unavoidable degree. In addition, the first plane is an imaginary plane extending parallel to the up-down direction in the n-type layer, which is not a boundary interface with an exposed surface or other semiconductor layers specifically formed during the manufacturing process of the n-type layer. Furthermore, in this specification, the AlGaN-based semiconductor layer, the GaN-based semiconductor layer, and the AlN-based semiconductor layer are semiconductor layers each composed of an AlGaN-based semiconductor, a GaN-based semiconductor, and an AlN-based semiconductor.
根據上述第1特徵之氮化物半導體紫外線發光元件時,如以下之說明,利用各別形成於n型層內之Ga富化n型領域與Al富化n型領域之後述之AlGaN組成比為整數比之準安定AlGaN,抑制起因於結晶成長裝置之漂移等之特性變動,可期待安定生產具有所期望發光特性之氮化物半導體紫外線發光元件。In the nitride semiconductor ultraviolet light emitting device according to the first feature, as described below, the AlGaN composition ratio described later using the Ga-rich n-type region and the Al-rich n-type region formed in the n-type layer, respectively, is an integer. Compared with quasi-stable AlGaN, it is possible to suppress fluctuations in characteristics due to drift of the crystal growth device, and it can be expected to stably produce nitride semiconductor ultraviolet light-emitting elements with desired light-emitting properties.
首先,對於AlGaN組成比為特定之整數比所表示之「準安定AlGaN」加以說明。First, "quasi-stable AlGaN" in which the composition ratio of AlGaN is represented by a specific integer ratio will be described.
通常,AlGaN等之三元混晶係隨機混合3族元素(Al和Ga)之結晶狀態,近似「隨機不均勻(random nonuniformity)」加以說明。但是,Al之共有結合半徑與Ga之共有結合半徑不同之故,於結晶構造中,Al與Ga之原子排列之對稱性高者,一般而言成為安定之構造。Usually, the crystalline state of the ternary mixed crystal system such as AlGaN is randomly mixed with
閃鋅礦構造之AlGaN系半導體係存在有無對稱性之隨機排列與安定之對稱排列之2種排列。在此,以一定之比率,顯現對稱排列成為支配之狀態。後述之AlGaN組成比(Al與Ga與N之組成比)以特定之整數比所表示之「準安定AlGaN」中,發現Al與Ga之週期性之對稱排列構造。The AlGaN-based semiconductor system of the sphalerite structure has two kinds of arrangement: random arrangement with or without symmetry and stable symmetrical arrangement. Here, at a certain ratio, it appears that the symmetrical arrangement becomes the dominant state. In "quasi-stable AlGaN" in which the composition ratio of AlGaN (the composition ratio of Al to Ga to N) described later is represented by a specific integer ratio, a periodic symmetrical arrangement structure of Al and Ga is found.
該週期性對稱排列構造中,對於結晶成長面僅些微增加Ga供給量,由於對稱性高之故,成為能量上若干安定之混晶莫耳分率,可防止易於質量移動(mass transfer)之Ga,極端增加場所之增殖。即,經由利用形成於n型層內之Ga富化n型領域之「準安定AlGaN」之性質,作為AlGaN系半導體,即使產生起因於結晶成長裝置之漂移等之混晶莫耳分率之變動,如後所述仍可局部抑制對於活性層提供低阻抗之電流路徑之層狀領域之混晶莫耳分率之變動。此結果,可實現從n型層至活性層內之安定之載子供給,抑制裝置特性之變動的結果,可期待安定生產發揮所期望特性之氮化物半導體紫外線發光元件。In this periodic symmetrical arrangement structure, the supply amount of Ga is only slightly increased for the crystal growth plane, and due to the high symmetry, it becomes a mixed crystal molar ratio with stable energy, which can prevent Ga that is prone to mass transfer. , extremely increases the proliferation of places. That is, by utilizing the properties of "quasi-stable AlGaN" in the Ga-enriched n-type region formed in the n-type layer, as an AlGaN-based semiconductor, even if the fluctuation of the mixed crystal molar ratio occurs due to drift of the crystal growth device, etc. , as will be described later, the variation of the mixed crystal molar ratio in the layered region that provides a low-impedance current path to the active layer can still be locally suppressed. As a result, stable carrier supply from the n-type layer to the active layer can be achieved, and fluctuations in device characteristics can be suppressed, and stable production of nitride semiconductor ultraviolet light-emitting elements exhibiting desired characteristics can be expected.
接著,對於Al與Ga在(0001)面內成為週期性之對稱排列之AlGaN組成比加以說明。Next, the composition ratio of AlGaN in which Al and Ga are periodically symmetrically arranged in the (0001) plane will be described.
於圖1,於AlGaN之c軸方向顯示1單元晶胞(2單原子層)之模式圖。於圖1中,白圈係顯示3族元素之原子(Al、Ga)所在之位置,黑圈係顯示5族元素之原子(N)所在之位置。In FIG. 1, a schematic diagram of 1 unit cell (2 single atomic layers) is shown in the c-axis direction of AlGaN. In FIG. 1 , the white circles show the positions of the atoms (Al, Ga) of the
於圖1中,以六角形所示之3族元素之位置面(A3面、B3面),及5族元素之位置面(A5面、B5面)係皆平行於(0001)面。A3面與A5面(總稱為A面)之各位置中,於六角形之各頂點存在6個位置,於六角形之中心,存在1個位置。對於B3面與B5面(總稱為B面)亦相同,於圖1中,僅圖示存在於B面之六角形內之3個位置。A面之各位置係重疊於c軸方向,B面之各位置係重疊於c軸方向。但是,B5面之1個位置之原子(N)係位於B5面之上側之A3面之3個位置之原子(Al、Ga)、和位於B5面之下側之B3面之1個位置之原子(Al、Ga)形成4配位結合,B3面之1個位置之原子(Al、Ga)係位於B3面之上側之B5面之1個位置之原子(N)、和位於B3面之下側之A5面之3個位置之原子(N)形成4配位結合之故,如圖1所示,A面之各位置係不與B面之各位置在c軸方向重疊。In FIG. 1 , the position planes (A3 and B3 planes) of the
圖2係作為將A面之各位置與B面之各位置之間之位置關係,從c軸方向所視平面圖加以圖示者。A面及B面,六角形之6個各頂點係經由鄰接之其他之2個六角形被共有,中心之位置係與其他之六角形未共有之故,於1個之六角形內,實質性存在3原子分之位置。因此,每1單元晶胞,3族元素之原子(Al、Ga)之位置則存在6個,5族元素之原子(N)之位置則存在6個。因此,作為除了GaN與AlN以整數比表示之AlGaN組成比,存在以下之5個情形。
1)Al
1Ga
5N
6、
2)Al
2Ga
4N
6(=Al
1Ga
2N
3)、
3)Al
3Ga
3N
6(=Al
1Ga
1N
2)、
4)Al
4Ga
2N
6(=Al
2Ga
1N
3)、
5)Al
5Ga
1N
6。
FIG. 2 is a plan view showing the positional relationship between the positions of the A surface and the B surface, as viewed from the c-axis direction. On the A and B sides, each of the six vertices of the hexagon is shared by the other two adjacent hexagons, and the position of the center is not shared with the other hexagons, so within one hexagon, substantially There are 3 atomic positions. Therefore, there are 6 positions of atoms (Al, Ga) of
於圖3,模式性顯示上述5個組合之3族元素之A3面與B3面。Ga為以黑圈,Al為以白圈顯示。In FIG. 3, the A3 surface and the B3 surface of the
圖3(A)所示Al 1Ga 5N 6之時,於A3面之6個頂點位置與B3面之6個頂點位置與1個中心位置,位有Ga,於A3面之1個中心位置,位有Al。 In the case of Al 1 Ga 5 N 6 shown in Fig. 3(A), Ga is located at the 6 apex positions of the A3 face and 6 apex positions and 1 central position of the B3 face, and Ga is located at 1 central position of the A3 face. , the bits have Al.
圖3(B)所示Al 1Ga 2N 3之時,於A3面及B3面之3個頂點位置與1個中心位置,位有Ga,於A3面及B3面之3個頂點位置,位有Al。 In the case of Al 1 Ga 2 N 3 shown in Fig. 3(B), Ga is located at the three vertex positions and one center position of the A3 plane and B3 plane, and the three vertex positions of the A3 plane and the B3 plane are located at the position of Ga. There is Al.
圖3(C)所示Al 1Ga 1N 2之時,於A3面之3個頂點位置與1個中心位置與B3面之3個頂點位置,位有Ga,於A3面之3個頂點位置與B3面之3個頂點位置與1個之中心位置,位有Al。 In the case of Al 1 Ga 1 N 2 shown in Fig. 3(C), there are Ga at the three vertex positions and one central position of the A3 face and three vertex positions of the B3 face, and the positions of the three vertexes of the A3 face are Al is located at the three vertex positions and one center position of the B3 face.
圖3(D)所示Al 2Ga 1N 3之時,於A3面及B3面之3個頂點位置,位有Ga,於A3面及B3面之3個頂點位置與1個中心位置,位有Al。此係相等於替換圖3(B)所示Al 1Ga 2N 3之時之Al與Ga之位置。 In the case of Al 2 Ga 1 N 3 shown in Fig. 3(D), Ga is located at the three vertex positions of the A3 and B3 surfaces, and Ga is located at the three vertex positions and one center position of the A3 and B3 surfaces. There is Al. This is equivalent to the positions of Al and Ga when replacing Al 1 Ga 2 N 3 shown in FIG. 3(B).
圖3(E)所示Al 5Ga 1N 6之時,於A3面之1個中心位置,位有Ga,於A3面之6個頂點位置與B3面之6個頂點位置與1個中心位置,位有Al。此係相等於替換圖3(A)所示Al 1Ga 5N 6之時之Al與Ga之位置。 In the case of Al 5 Ga 1 N 6 shown in Fig. 3(E), Ga is located at one central position of the A3 plane, and there are 6 vertex positions of the A3 plane and 6 vertex positions and 1 central position of the B3 plane. , the bits have Al. This is equivalent to the positions of Al and Ga when replacing Al 1 Ga 5 N 6 shown in FIG. 3(A).
於圖3(A)~(E)之各圖,可知假想於六角形之6個之頂點之任1個中心移動之其他六角形時,與於A3面之6個頂點位置,位有Al或Ga,以及於A3面之3個頂點位置與1個之中心位置,位有Al或Ga等效,於A3面之1個之中心位置,位有Al或Ga係與於A3面之3個頂點位置,位有Al或Ga等效。有關於B3面亦相同。又,於圖3(A)、(C)及(E)之各圖,替換A3面與B3面亦可。In Figure 3(A)~(E), it can be seen that when other hexagons are imagined to move at any one center of the 6 vertices of the hexagon, the positions of the 6 vertices on the A3 plane have Al or Ga, and at the center position of the 3 vertices of the A3 face, there are Al or Ga equivalent, and at the central position of the A3 face, there are Al or Ga and the 3 vertices of the A3 face. Position, bit has Al or Ga equivalent. The same is true for the B3 side. In addition, in each figure of FIG.3(A), (C) and (E), you may replace A3 surface and B3 surface.
圖3(A)~(E)之各圖中,不論是A3面與B3面之任一者,Al與Ga之原子排列係維持對稱性。又,即使移動六角形之中心,Al與Ga之原子排列係維持對稱性。In each of FIGS. 3(A) to (E), the atomic arrangement of Al and Ga maintains symmetry regardless of whether it is the A3 plane or the B3 plane. Also, even if the center of the hexagon is shifted, the atomic arrangement of Al and Ga maintains symmetry.
更且,於圖3(A)~(E)之A3面與B3面,六角形之位置面重覆配置成蜂巢狀時,在平行於(0001)面之方向,例如於[11-20]方向、[10-10]方向,觀看各位置時,出現Al與Ga則週期性重覆就位,或Al與Ga之任一方連續就位之狀態。因此,皆成為週期性對稱性之原子排列。Moreover, in the A3 plane and the B3 plane of Fig. 3(A)~(E), when the hexagonal position plane is repeatedly arranged in a honeycomb shape, in the direction parallel to the (0001) plane, for example in [11-20] Direction, [10-10] direction, when viewing each position, Al and Ga are periodically repeated in place, or either Al or Ga is continuously in place. Therefore, they are all atomic arrangements of periodic symmetry.
在此,將對應於上述1)~5)之AlGaN組成比之AlN莫耳分率x1(x1=1/6,1/3,1/2,2/3,5/6)之Al x1Ga 1-x1N,為了說明之方便,稱為「第1之準安定AlGaN」。第1之準安定AlGaN係Al與Ga之原子排列成為週期性之對稱排列,成為能量上安定之AlGaN。 Here, the AlN molar ratio x1 (x1=1/6, 1/3, 1/2, 2/3, 5/6) corresponding to the AlGaN composition ratios of the above 1) to 5) is set to Al x1 Ga 1-x1 N is referred to as "the first quasi-stable AlGaN" for the convenience of description. The first quasi-stable AlGaN system is that the atomic arrangement of Al and Ga becomes a periodic symmetrical arrangement, resulting in an energetically stable AlGaN.
接著,將圖1所示六角形所示位置面擴張於2單元晶胞(4單原子層)時,3族元素之位置面(A3面、B3面)與5族元素之位置面(A5面、B5面)則各別存在2個,每2單元晶胞,3族元素之原子(Al、Ga)之位置則存在12個,5族元素之原子(N)之位置則存在12個。因此,作為除了GaN與AlN以整數比表示之AlGaN組成比,除了上述1)~5)之AlGaN組成比以外,存在以下之6個組合。
6)Al
1Ga
11N
12(=GaN+Al
1Ga
5N
6)、
7)Al
3Ga
9N
12(=Al
1Ga
3N
4=Al
1Ga
5N
6+Al
1Ga
2N
3)、
8)Al
5Ga
7N
12(=Al
1Ga
2N
3+Al
1Ga
1N
2)、
9)Al
7Ga
5N
12(=Al
1Ga
1N
2+Al
2Ga
1N
3)、
10)Al
9Ga
3N
12(=Al
3Ga
1N
4=Al
2Ga
1N
3+Al
5Ga
1N
6)、
11)Al
11Ga
1N
12(=Al
5Ga
1N
6+AlN)。
Next, when the positional planes shown in the hexagon shown in FIG. 1 are expanded to a 2-unit unit cell (4 monoatomic layers), the positional planes of
但是,此等6)~11)之6個之AlGaN組成比係組合位於該前後之第1之準安定AlGaN、GaN及AlN內之2個之AlGaN組成比而成之故,c軸方向之對稱性混亂之可能性高之故,雖較第1之準安定AlGaN安定度下降,但A3面及B3面內之Al與Ga之原子排列之對稱性係與第1之準安定AlGaN相同,較隨機非對稱排列狀態之AlGaN安定度為高。在此,將對應於上述6)~11)之AlGaN組成比之AlN莫耳分率x2(x2=1/12,1/4,5/12,7/12,3/4,11/12)之Al x2Ga 1-x2N,為了說明之方便,稱為「第2之準安定AlGaN」。經由以上,第1及第2之準安定AlGaN係成為較結晶構造中之Al與Ga之原子排列之對稱性安定之構造。以下,將第1及第2之準安定AlGaN,總稱為「準安定AlGaN」。 However, the six AlGaN composition ratios of 6) to 11) are formed by combining the first quasi-stable AlGaN, GaN, and AlN in the first and subsequent AlGaN composition ratios, so the symmetry in the c-axis direction Although the stability of AlGaN is higher than that of the first quasi-stable AlGaN, the symmetry of the atomic arrangement of Al and Ga in the A3 plane and the B3 plane is the same as that of the first quasi-stable AlGaN, which is more random. The stability of AlGaN in the asymmetric alignment state is high. Here, the AlN molar ratio x2 (x2=1/12, 1/4, 5/12, 7/12, 3/4, 11/12) corresponding to the AlGaN composition ratios in 6) to 11) above The Alx2Ga1 -x2N is referred to as "the second quasi-stable AlGaN" for the convenience of description. From the above, the first and second quasi-stable AlGaN systems have a more stable structure than the symmetry of the atomic arrangement of Al and Ga in the crystal structure. Hereinafter, the first and second quasi-stable AlGaN are collectively referred to as "quasi-stable AlGaN".
在此,上述1)~11)之11種之準安定AlGaN之整數比所表示之AlGaN組成比係使用整數n(n=1~11)一般化時,表示為Al nGa 12-nN 12,AlN莫耳分率係成為n/12。整數n為偶數之1)~5)係第1之準安定AlGaN,整數n為奇數之6)~11)為第2之準安定AlGaN。然而,Al nGa 12-nN 12之AlN莫耳分率係欲貿數表記之時雖成為n/12,但以百分率表記之時,於小數點以下會產生尾數。因此,以下中,為了說明上之方便,以分數表示之1/12、2/12(=1/6)、4/12(=1/3)、5/12、7/12、8/12(=2/3)、10/12(=5/6)、11/12之8個AlN莫耳分率係近似表記為8.3%、16.7%、33.3%、41.7%、58.3%、66.7%、83.3%、91.7%。 Here, the AlGaN composition ratio represented by the integer ratio of the 11 kinds of quasi-stable AlGaN of the above 1) to 11) is expressed as Al n Ga 12-n N 12 when the integer n (n=1 to 11) is used to generalize , the AlN molar ratio becomes n/12. The integer n is the even number of 1) to 5) is the first quasi-stable AlGaN, and the integer n is the odd number of 6) to 11) is the second quasi-stable AlGaN. However, the AlN molar ratio of AlnGa12 - nN12 is n / 12 when expressed as a trade number, but when expressed as a percentage, a mantissa will be generated below the decimal point. Therefore, in the following, for the convenience of description, 1/12, 2/12 (=1/6), 4/12 (=1/3), 5/12, 7/12, 8/12 expressed in fractions (=2/3), 10/12 (=5/6), 11/12 8 AlN molar ratios are approximately expressed as 8.3%, 16.7%, 33.3%, 41.7%, 58.3%, 66.7%, 83.3%, 91.7%.
要將AlGaN維持一定之結晶品質加以成長,需以1000℃以上之高溫進行結晶成長。但是,Ga係於結晶表面之位置,原子到達後,在1000℃以上想定為亂動。另一方面,Al係與Ga不同,易於吸附於表面,進入位置之後之行動,雖多少會有移動,但被強力限制。To grow AlGaN with a certain crystal quality, crystal growth needs to be performed at a high temperature of 1000°C or higher. However, Ga is located at the position of the crystal surface, and after the atoms arrive, it is assumed to be disturbed at 1000°C or higher. On the other hand, Al-based, unlike Ga, is easily adsorbed to the surface, and the movement after entering the position is somewhat moved, but is strongly restricted.
因此,即使為準安定AlGaN,上述1)之Al 1Ga 5N 6、上述6)之Al 1Ga 11N 12、及、上述7)之Al 1Ga 3N 4係AlN莫耳分率皆為25%以下,Ga之組成比為高之故,1000℃附近之成長溫度中,Ga之移動則激烈,原子排列之對稱性則混亂,Al與Ga之原子排列係接近隨機狀態,上述之安定度則較其他之準安定AlGaN下降。 Therefore, even if it is quasi-stable AlGaN, the molar ratio of Al 1 Ga 5 N 6 in the above 1), Al 1 Ga 11 N 12 in the above 6), and Al 1 Ga 3 N 4 series AlN in the above 7) is all Below 25%, because the composition ratio of Ga is high, at the growth temperature around 1000°C, the movement of Ga is intense, the symmetry of the atomic arrangement is disordered, the atomic arrangement of Al and Ga is close to a random state, and the above-mentioned stability It is lower than other quasi-stable AlGaN.
接著,對於「Ga富化n型領域」與「Al富化n型領域」加以說明。上述第1特徵之氮化物半導體紫外線發光元件中,n型層與活性層與p型層內之各半導體層則具有形成平行於(0001)面之多段狀之平台之表面的磊晶成長層之故,於n型層內,易於質量移動之Ga係移動在n型本體領域之平台上,集中於鄰接之平台間之邊界領域,形成較n型本體領域AlN莫耳分率低之領域。該邊界領域則伴隨n型層之n型AlGaN層之磊晶成長,對於(0001)面朝向斜上方延伸,局部AlN莫耳分率低之層狀領域則於n型層內一樣分散而形成。Next, the "Ga-enriched n-type region" and the "Al-enriched n-type region" will be described. In the nitride semiconductor ultraviolet light emitting device of the above-mentioned first feature, each semiconductor layer in the n-type layer, the active layer, and the p-type layer has an epitaxial growth layer formed on the surface of the multi-segment platform parallel to the (0001) plane. Therefore, in the n-type layer, Ga, which is easy to mass transfer, moves on the platform of the n-type body region, and is concentrated in the boundary region between adjacent platforms, forming a region with a lower molar ratio than the AlN region of the n-type body region. The boundary region is accompanied by the epitaxial growth of the n-type AlGaN layer in the n-type layer, and extends obliquely upward for the (0001) plane, and the layered region with local low AlN molar ratio is formed in the same manner as dispersed in the n-type layer.
在此,伴隨從n型本體領域至層狀領域內之Ga之質量移動,層狀領域內之AlN莫耳分率則下降,對層狀領域內之Ga之質量移動量(以後,亦稱Ga供給量)充分為大時,於層狀領域內,形成包含AlGaN組成比為Al nGa 12-nN 12之n型準安定AlGaN之Ga富化n型領域。前述準安定AlGaN之AlN莫耳分率係接近較n型層之平均性AlN莫耳分率Xna為低之AlN莫耳分率(n/12),於Ga富化n型領域內,藉由存在AlGaN組成比為Al nGa 12-nN 12之準安定AlGaN,對於Ga富化n型領域內之Ga供給量之變動,及平均性之AlN莫耳分率Xna之變動則於該準安定AlGaN被吸收。即,於Ga富化n型領域內,增加Ga供給量,或AlN莫耳分率Xna下降時,準安定AlGaN則增加,減少Ga供給量,或AlN莫耳分率Xna上昇時,準安定AlGaN則減少,就結果而言,抑制Ga富化n型領域內之AlN莫耳分率之變動。 Here, with the mass shift of Ga from the n-type bulk domain to the layered domain, the AlN molar ratio in the layered domain decreases, and the mass shift amount of Ga in the layered domain (hereinafter, also referred to as Ga When the supply amount) is sufficiently large, a Ga - rich n -type region including n-type quasi-stable AlGaN whose composition ratio of AlGaN is AlnGa12 -nN12 is formed in the layered region. The AlN molar ratio of the aforementioned quasi-stable AlGaN is close to the AlN molar ratio (n/12) which is lower than the average AlN molar ratio Xna of the n-type layer. In the Ga-enriched n-type region, by There is a quasi-stable AlGaN whose AlGaN composition ratio is AlnGa12 -nN12, and the fluctuation of Ga supply in the Ga - enriched n -type region and the fluctuation of the average AlN molar ratio Xna are in this quasi-stable AlGaN is absorbed. That is, in the Ga-enriched n-type region, when the supply amount of Ga increases or the AlN molar ratio Xna decreases, the quasi-stable AlGaN increases and the Ga supply amount decreases, or when the AlN molar ratio Xna increases, the quasi-stable AlGaN increases is reduced, and as a result, the variation in the molar ratio of AlN in the Ga-enriched n-type region is suppressed.
來自阱層之發光透過n型層在外部被取出之一般之實施形態中,Ga富化n型領域內之AlN莫耳分率通常較,形成於阱層之傾斜領域內之Ga富化阱領域之AlN莫耳分率,設定高達8.3%以上,較佳為16%以上。因此,經由抑制起因於結晶成長裝置之漂移等之Ga供給量之變動所造成Ga富化n型領域內之AlN莫耳分率之大幅下降,可抑制來自阱層之發光於Ga富化阱領域被吸收,使發光效率下降。In the general embodiment where the light emission from the well layer is extracted externally through the n-type layer, the AlN molar ratio in the Ga-enriched n-type region is generally higher than that in the Ga-enriched well region formed in the inclined region of the well layer. The molar ratio of AlN is set as high as 8.3% or more, preferably 16% or more. Therefore, by suppressing a significant drop in the molar ratio of AlN in the Ga-rich n-type region due to fluctuations in the Ga supply amount due to drift of the crystal growth device, it is possible to suppress light emission from the well layer in the Ga-rich well region absorbed, reducing the luminous efficiency.
另一方砷,n型層內之n型本體領域中,經由對層狀領域內質量移動Ga,在鄰接於n型本體領域內之層狀領域之端緣部或該附近(以下,匯總兩者單純稱為「端緣部」),形成AlN莫耳分率則較n型本體領域內之平均性AlN莫耳分率為高之Al富化n型領域。在此,對應於對Ga富化n型領域內之Ga供給量之增加或AlN莫耳分率Xna之上昇,Al富化n型領域之AlN莫耳分率則增加。在此,Ga富化n型領域係形成於與n型層內之n型本體領域比較為窄之層狀領域之故,或對層狀領域內之Ga之質量移動係從挾持該層狀領域之兩側之n型本體領域產生之故以n型層之平均性之AlN莫耳分率Xna為基準,對於對層狀領域內之Ga之質量移動量之Ga富化n型領域內之AlN莫耳分率之下降程度係較Al富化n型領域內之AlN莫耳分率之增加程度為大。On the other hand, arsenic, in the n-type bulk domain within the n-type layer, is adjacent to or near the edge of the layered domain within the n-type bulk domain by mass shifting Ga to the layered domain (hereinafter, the two are summarized). Simply referred to as "edge portion"), an Al-rich n-type domain with a higher AlN molar ratio than the average AlN molar ratio in the n-type bulk domain is formed. Here, the AlN molar ratio in the Al-rich n-type region increases in response to an increase in the Ga supply amount in the Ga-enriched n-type region or an increase in the AlN molar ratio Xna. Here, the Ga-enriched n-type domain is formed in a layered domain that is narrower than the n-type body domain in the n-type layer, or the mass transfer of Ga in the layered domain is caused by holding the layered domain. The reason why the n-type bulk domains on both sides are generated is based on the average AlN molar ratio Xna of the n-type layer, and the AlN in the n-type domain is enriched by Ga for the mass shift amount of Ga in the layered domain. The decrease in molar ratio is greater than the increase in AlN molar ratio in the Al-rich n-type domain.
因此,n型層之平均性之AlN莫耳分率Xna係成為(n+0.5)/12<Xna<(n+1)/12之適切範圍內時,對層狀領域內之Ga供給量充分為大,於Ga富化n型領域內,形成AlGaN組成比為Al nGa 12-nN 12之準安定AlGaN之同時,對於Al富化n型領域內,形成AlGaN組成比為Al n+1Ga 11-nN 12之準安定AlGaN。於Al富化n型領域內,藉由存在AlGaN組成比為Al n+1Ga 11-nN 12之準安定AlGaN,對於Ga富化n型領域內之Ga供給量之變動,及平均性之AlN莫耳分率Xna之變動則在存在於Al富化n型領域內之該準安定AlGaN中亦被吸收。即,在鄰接於n型本體領域內之層狀領域之Al富化n型領域內,存在能量上安定之準安定AlGaN,抑制從n型本體領域經由Al富化n型領域之層狀領域內之過剩之Ga之質量移動,,而可抑制上述Ga供給量之變動所造成Ga富化n型領域內之AlN莫耳分率之大幅之下降。 Therefore, when the average AlN molar fraction Xna of the n-type layer is within an appropriate range of (n+0.5)/12<Xna<(n+1)/12, the supply amount of Ga in the layered region is sufficient. In the Ga - enriched n -type region, while forming quasi-stable AlGaN with a composition ratio of AlnGa12 -nN12, in the Al-enriched n-type region, an AlGaN with a composition ratio of Aln +1 is formed. Quasi-stable AlGaN of Ga 11-n N 12 . In the Al-enriched n-type region, due to the presence of quasi-stable AlGaN with a composition ratio of Aln +1 Ga 11-n N 12 , the variation of the Ga supply in the Ga-enriched n-type region and the average Variations in the AlN molar fraction Xna are also absorbed in the quasi-stable AlGaN existing in the Al-rich n-type region. That is, in the Al-rich n-type region adjacent to the layered region in the n-type body region, there is an energetically stable quasi-stable AlGaN, which suppresses the transition from the n-type body region through the Al-rich n-type region in the layered region. The mass of the excess Ga is shifted, and the above-mentioned fluctuations in the supply of Ga can be suppressed from the sharp drop in the molar ratio of AlN in the Ga-enriched n-type region.
在此,如上所述,於n型層中,局部AlN莫耳分率低之層狀領域係載子易於局部存在化,可對於活性層提供低阻抗之電流路徑。又,於活性層中,存在於阱層之傾斜領域內之局部AlN莫耳分率低之Ga富化阱領域中,載子易於局部存在化,阱層之傾斜領域係位於n型層之層狀領域之延長上之故,可藉由層狀領域,對於阱層之Ga富化阱領域,有效率提供載子。因此,藉由於層狀領域之Ga富化n型領域內,形成AlGaN組成比為Al nGa 12-nN 12之準安定AlGaN,於n型本體領域之Al富化n型領域內,形成AlGaN組成比為Al n+1Ga 11-nN 12之準安定AlGaN,作為Ga富化n型領域與Al富化n型領域之間之AlN莫耳分率差,安定確保12分1(約8.33%),可更安定實現上述載子之局部存在化所成之低阻抗之電流路徑之提供。就結果而言,可達成氮化物半導體紫外線發光元件之特性變動之抑制。 Here, as described above, in the n-type layer, a layered domain with a low AlN molar ratio is localized easily, and a low-impedance current path can be provided to the active layer. Also, in the active layer, in the Ga-rich well region with a low AlN molar ratio that exists locally in the inclined region of the well layer, the carriers are easily localized, and the inclined region of the well layer is located in the layer of the n-type layer. Because of the extension of the state domain, carriers can be efficiently supplied to the Ga-enriched well domain of the well layer through the layer domain. Therefore, by forming a quasi-stable AlGaN with AlGaN composition ratio of AlnGa12- nN12 in the Ga - enriched n -type region of the layered region, and forming AlGaN in the Al-enriched n-type region of the n-type body region Quasi-stable AlGaN with a composition ratio of Al n+1 Ga 11-n N 12 , as the AlN molar ratio difference between the Ga-rich n-type region and the Al-rich n-type region, the stability is guaranteed to be 12 minutes 1 (about 8.33 %), which can more stably realize the provision of a low-impedance current path formed by the localization of the above-mentioned carriers. As a result, suppression of characteristic variation of the nitride semiconductor ultraviolet light emitting element can be achieved.
惟,於AlGaN之結晶成長中,通常可混合存在獲得隨機非對稱排列之狀態、和規則對稱排列之狀態之故,n型層之平均性之AlN莫耳分率Xna則非上述適切之範圍內,成為n/12≦Xna≦(n+0.5)/12之範圍內,Ga供給量過度增加時,於Ga富化n型領域內,形成AlGaN組成比為Al nGa 12-nN 12之準安定AlGaN的同時,可形成AlN莫耳分率較n/12為低之隨機非對稱排列之非準安定AlGaN。更且,AlN莫耳分率Xna係成為n/12≦Xna≦(n+0.5)/12之範圍內,Ga供給量非充分為大時,於Al富化n型領域內,不形成AlGaN組成比為Al n+1Ga 11-nN 12之準安定AlGaN,伴隨Ga供給量之變動,Al富化n型領域內之AlN莫耳分率亦會變動。 However, in the crystal growth of AlGaN, the state of random asymmetric arrangement and the state of regular symmetric arrangement are usually mixed, and the average AlN molar ratio Xna of the n-type layer is not within the above appropriate range. , in the range of n/12≦Xna≦(n+0.5)/12, when the supply of Ga is excessively increased, in the Ga - enriched n -type region, the composition ratio of AlGaN is formed as AlnGa12 -nN12 While stabilizing AlGaN, non-quasi-stable AlGaN with random asymmetric arrangement of AlN molar ratio lower than n/12 can be formed. Furthermore, when the AlN molar fraction Xna is in the range of n/12≦Xna≦(n+0.5)/12, and the Ga supply amount is not sufficiently large, no AlGaN composition is formed in the Al-rich n-type region. For the quasi-stable AlGaN whose ratio is Al n+1 Ga 11 -n N 12 , the molar ratio of AlN in the Al-enriched n-type region also fluctuates with the fluctuation of the Ga supply.
因此,n型層之平均性之AlN莫耳分率Xna係成為n/12≦Xna≦(n+0.5)/12之範圍內時,相較於成為(n+0.5)/12<Xna<(n+1)/12之範圍內,Ga富化n型領域與Al富化n型領域之間之AlN莫耳分率差不會成為安定之12分之1(約8.33%),易於變動之故,對層狀領域內之載子之局部存在化之程度則下降,會產生載子從層狀領域向n型本體領域擴展之情形。更且,形成AlN莫耳分率較n/12為低之隨機非對稱排列之非準安定AlGaN時,來自阱層之發光則於Ga富化阱領域被吸收,使發光效率下降。就結果而言,有無法充分達成氮化物半導體紫外線發光元件之特性變動之抑制之可能性。Therefore, when the average AlN molar fraction Xna of the n-type layer is within the range of n/12≦Xna≦(n+0.5)/12, compared with (n+0.5)/12<Xna<( Within the range of n+1)/12, the difference in AlN molar ratio between the Ga-enriched n-type domain and the Al-enriched n-type domain will not become 1/12 of the stability (about 8.33%), and it is easy to fluctuate. Therefore, the degree of localization of carriers in the layered domain is reduced, and a situation in which the carriers expand from the layered domain to the n-type bulk domain occurs. Furthermore, when the random asymmetric arrangement of non-quasi-stable AlGaN with AlN molar ratio lower than n/12 is formed, the luminescence from the well layer is absorbed in the Ga-rich well region, resulting in a decrease in luminous efficiency. As a result, there is a possibility that the suppression of characteristic variation of the nitride semiconductor ultraviolet light emitting element cannot be sufficiently achieved.
更且`。上述第1特徵之氮化物半導體紫外線發光元件係前述n型層之平均性AlN莫耳分率Xna為(n+0.9)/12以下為佳。More and `. In the nitride semiconductor ultraviolet light emitting element of the above-mentioned first feature, the average AlN molar fraction Xna of the n-type layer is preferably (n+0.9)/12 or less.
根據上述適切實施形態時,於層狀領域之Ga富化n型領域內,可更安定形成AlGaN組成比為Al nGa 12-nN 12之準安定AlGaN,於n型本體領域之Al富化n型領域內,可更安定形成AlGaN組成比為Al n+1Ga 11-nN 12之準安定AlGaN。 According to the above-mentioned suitable embodiment, in the Ga - enriched n -type region in the layered region, quasi-stable AlGaN with a composition ratio of AlnGa12 -nN12 can be more stably formed, and the Al-rich region in the n-type body region can be formed more stably In the n-type field, quasi-stable AlGaN with the AlGaN composition ratio of Aln + 1Ga11 - nN12 can be formed more stably.
更且,本發明係除了上述第1特徵,提供前述p型層係具有作為前述p型層內之最下層,形成於前述1層以上之阱層之最上層之上面側的電子阻障層, 前述電子阻障層係各別具有對於連結前述多段狀之平台之鄰接之平台間之(0001)面傾斜之傾斜領域、和前述傾斜領域以外之平台領域, 整數m為8、9或10, 於前述電子阻障層之前述傾斜領域內,存在包含AlGaN組成比成為整數比之Al mGa 12-mN 12之p型AlGaN領域,局部地AlN莫耳分率為低的Ga富化EB領域, 前述電子阻障層之平均性AlN莫耳分率Xea成為(m+0.24)/12≦Xea<(m+1)/12之範圍內之第2特徵之氮化物半導體紫外線發光元件。 Furthermore, the present invention provides that the p-type layer has, as the lowermost layer in the p-type layer, an electron barrier layer formed on the upper surface side of the uppermost layer of the one or more well layers, in addition to the above-mentioned first feature, The electron barrier layer respectively has an inclined region that is inclined to the (0001) plane between the adjacent platforms connecting the multi-segmented platforms, and a platform region other than the aforementioned inclined region. The integer m is 8, 9 or 10. In the aforementioned inclined region of the aforementioned electron barrier layer, there is a p-type AlGaN region including AlmGa12 - mN12 whose composition ratio of AlGaN is an integer ratio, a Ga-enriched EB region with a low AlN molar fraction locally, The nitride semiconductor ultraviolet light emitting element of the second feature is the average AlN molar fraction Xea of the electron barrier layer in the range of (m+0.24)/12≦Xea<(m+1)/12.
在此,對於在電子阻障層之傾斜領域內,未形成Ga富化EB領域時之課題加以說明。Here, the problem when the Ga-enriched EB region is not formed in the inclined region of the electron barrier layer will be described.
為了達成阱層內之載子(電子及電洞)之再結合所造成發光效率之提升,需有效率進行對阱層內之從n型層側之載子(電子)之植入、和從p型層側之載子(電洞)之植入之兩者。一般而言,為了提高從n型層側向阱層內之載子(電子)之植入効率,較n型包覆層或量子阻障層之AlN莫耳分率高之通常80%以上之AlN莫耳分率之電子阻障層,則設於活性層最靠p型層之阱層之p型層側。In order to achieve the improvement of luminous efficiency caused by the recombination of carriers (electrons and holes) in the well layer, it is necessary to efficiently perform implantation of carriers (electrons) from the n-type layer side in the well layer, and from Both of the implantation of carriers (holes) on the p-type layer side. Generally speaking, in order to improve the implantation efficiency of carriers (electrons) from the n-type layer to the well layer, the molar ratio of AlN is usually 80% higher than that of the n-type cladding layer or the quantum barrier layer. The electron barrier layer of AlN molar ratio is arranged on the p-type layer side of the active layer which is closest to the well layer of the p-type layer.
於電子阻障層內,與阱層相同,為形成平行於(0001)面之多段狀之平台,形成對於連結鄰接之平台間之(0001)面傾斜之傾斜領域。但是,一般而言,電子阻障層之AlN莫耳分率極高之故,在n型包覆層及阱層內所產生之Ga之偏析所造成組成調製,則在電子阻障層內難以產生,電子阻障層內之AlN莫耳分率係在傾斜領域與平台領域之間,難以產生差異。作為一例,圖23所示以往之氮化物半導體紫外線發光元件之HAADF-STEM中,雖可確認在n型包覆層及阱層內產生Ga之偏析所造成組成調製,於n型包覆層之層狀領域及阱層之傾斜領域中,產生AlN莫耳分率之下降,但無法確認在電子阻障層內,產生Ga之偏析所造成組成調製,於電子阻障層之傾斜領域中,產生AlN莫耳分率之下降。In the electron barrier layer, like the well layer, a multi-stage terrace parallel to the (0001) plane is formed, and an inclined region inclined with respect to the (0001) plane connecting adjacent terraces is formed. However, in general, since the molar fraction of AlN in the electron barrier layer is extremely high, the composition modulation caused by the segregation of Ga generated in the n-type cladding layer and the well layer is difficult to achieve in the electron barrier layer. Therefore, the molar ratio of AlN in the electron barrier layer is difficult to produce difference between the inclined domain and the plateau domain. As an example, in the HAADF-STEM of the conventional nitride semiconductor ultraviolet light-emitting device shown in FIG. 23, although it was confirmed that the composition modulation caused by the segregation of Ga in the n-type cladding layer and the well layer was generated, in the n-type cladding layer In the layered region and the inclined region of the well layer, the molar ratio of AlN decreases, but it cannot be confirmed that the composition modulation caused by the segregation of Ga in the electron barrier layer occurs. In the inclined region of the electron barrier layer, the A drop in AlN molar ratio.
更且。阱層及電子阻障層之該傾斜領域之膜厚係伴隨向階梯流動成長之平台邊緣之側面之橫方向成長,阱層及電子阻障層之各上面之平台則對各下面之平台向橫方向移動之故,較傾斜領域以外之平台領域之膜厚為厚。And more. The film thickness of the sloping area of the well layer and the electron barrier layer is accompanied by the lateral growth of the side of the edge of the platform where the step flow grows. Because of the direction movement, the film thickness is thicker than that of the platform area other than the inclined area.
形成於電子阻障層內之傾斜領域中,不產生Ga之偏析所造成組成調製,不產生如阱層局部之AlN莫耳分率之下降之情形,以及膜厚較平台領域為厚之情形,會成為從p型層側向阱層內之載子(電洞)之有效植入之阻礙因素。此部分,使用圖4,模式性加以說明。In the inclined region formed in the electron barrier layer, the composition modulation caused by the segregation of Ga does not occur, the situation such as the drop of the molar ratio of AlN locally in the well layer, and the situation where the film thickness is thicker than that of the plateau region, do not occur. It will become an obstacle to the effective implantation of carriers (holes) from the p-type layer to the well layer. This section will be explained schematically using FIG. 4 .
於p電極與n電極間,施加順向偏壓時,如模式性顯示於圖4,雖從p型連接層(p-GaN)向電子阻障層(EB)內,植入電洞(h+),如上所述,於電子阻障層內,傾斜領域之AlN莫耳分率係未局部地下降,不激發載子(電洞)之局部存在化,相反地,傾斜領域之膜厚為厚,電阻為高,阻礙電洞之通過之故,植入於電子阻障層內之電洞係從平台領域到達阱層內之平台領域。另一方面,電子(e-)係從n型包覆層側經由層狀領域,到達阱層(QW)內之傾斜領域。電子與電洞為在阱層之傾斜領域內之局部存在中心(圖中,以☆(星形)圖示)進行發光再結合,到達阱層內之平台領域之電洞,則需擴散到達傾斜領域。但是,電洞之擴散長度係較電子為短,擴散到達傾斜領域之電洞之量則有限,到達阱層之平台領域之電洞係一部分在平台領域擴散中,在點缺陷之Al空洞等之非發光再結合中心(圖中,以●(黑圓)圖示)捕獲,進行非發光再結合之故,有內部量子效率下降之問題。When a forward bias is applied between the p-electrode and the n-electrode, as shown schematically in Figure 4, although holes (h+) are implanted from the p-type junction layer (p-GaN) to the electron barrier layer (EB) ), as described above, in the electron barrier layer, the AlN molar ratio in the inclined region does not decrease locally, and does not stimulate the local existence of carriers (holes), on the contrary, the film thickness of the inclined region is thick , the resistance is high, which hinders the passage of holes. The holes implanted in the electron barrier layer reach the platform area in the well layer from the platform area. On the other hand, electrons (e-) pass through the layered region from the n-type cladding layer side and reach the inclined region in the well layer (QW). Electrons and holes are localized centers in the inclined field of the well layer (in the figure, represented by ☆ (star)) to emit light and recombine, and the holes that reach the platform field in the well layer need to diffuse to reach the inclined area. field. However, the diffusion length of holes is shorter than that of electrons, and the amount of holes that diffuse to the inclined domain is limited. The holes that reach the platform domain of the well layer are partly diffused in the platform domain, and the holes such as Al holes of point defects are diffused in the platform domain. Since the non-luminescent recombination center (in the figure, shown by ● (black circle)) is trapped and the non-luminescent recombination is performed, there is a problem that the internal quantum efficiency decreases.
更且,尖峰發光波長約285nm以上之氮化物半導體紫外線發光元件中,與約不足285nm之情形比較,構成阱層之AlGaN系半導體之AlN莫耳分率為低之故,相對成為點缺陷之Al空洞變少,到達阱層內之平台領域之電洞係在較傾斜領域AlN莫耳分率高之平台領域內,發光再結合,會有產生以較傾斜領域之短波長之發光的問題。具體而言,於發光光譜中,產生不同波長之2個發光尖峰未合成於1個尖峰而成分離顯現之雙尖峰發光,成為產率下降之要素。In addition, in the nitride semiconductor ultraviolet light-emitting element with a peak emission wavelength of about 285 nm or more, compared with the case of less than about 285 nm, the AlGaN-based semiconductor constituting the well layer has a lower molar fraction of AlN than Al, which is a point defect. There are fewer holes, and the holes reaching the plateau region in the well layer are located in the plateau region with a higher AlN molar ratio than the inclined region, and the luminescence recombines, resulting in a problem of emitting light with a shorter wavelength than the oblique region. Specifically, in the emission spectrum, two emission peaks with different wavelengths are generated, and the two emission peaks of different wavelengths are not synthesized into a single peak, and the double-peak emission appears separately, which is a factor for decreasing the yield.
因此,根據上述第2特徵特徵之氮化物半導體紫外線發光元件時,於電子阻障層之傾斜領域內,存在AlN莫耳分率局部性低之Ga富化EB領域,在Ga富化EB領域內,可產生載子(電洞)之局部存在化之故,如模示性示於圖5,植入於電子阻障層(EB)內之電洞(h+)係亦直接植入傾斜領域IA內。然後,直接植入於電子阻障層之傾斜領域IA內,不擴散平台領域TA內,到達阱層(QW)之傾斜領域IA內之發光再結合之局部存在中心(圖中以☆(星型)圖示)之電洞量則大幅增加。此結果,直接植入於電子阻障層之傾斜領域內,不擴散平台領域內,到達發光再結合之局部存在中心之阱層之傾斜領域內之電洞量則大幅增加,可抑制於電子阻障層之傾斜領域內未形成Ga富化EB領域時所產生內部量子效率之下降、及雙發光尖峰之產生。然而,圖5中之●(黑圓)係與圖4相同,顯示非發光再結合中心。Therefore, in the nitride semiconductor ultraviolet light emitting device according to the second characteristic feature, in the inclined region of the electron barrier layer, there is a Ga-rich EB region where the AlN molar fraction is locally low, and in the Ga-rich EB region , can generate the localized existence of carriers (holes), as shown schematically in Figure 5, the holes (h+) implanted in the electron barrier layer (EB) are also directly implanted in the inclined area IA Inside. Then, it is directly implanted in the inclined area IA of the electronic barrier layer, in the non-diffusion platform area TA, and reaches the local existence center of the luminescence recombination in the inclined area IA of the well layer (QW) (in the figure marked with ☆ (star-shaped). ) as shown in the figure) increases significantly. As a result, directly implanted in the inclined area of the electron barrier layer, in the non-diffusion platform area, the amount of holes in the inclined area of the well layer that reaches the localized center of the light-emitting recombination is greatly increased, which can suppress the electron resistance. The decrease of the internal quantum efficiency and the generation of double emission peaks are caused when the Ga-enriched EB region is not formed in the inclined region of the barrier layer. However, the ● (black circle) in FIG. 5 is the same as in FIG. 4, showing the non-luminescent recombination center.
根據上述第2特徵之氮化物半導體紫外線發光元件時,利用形成於電子阻障層內之Ga富化EB領域之AlGaN組成比為整數比之準安定AlGaN,與於n型層內之Ga富化n型領域,形成AlGaN組成比為整數比之準安定AlGaN之時相同,抑制起因於結晶成長裝置之漂移等之特性變動,可期待安定生產具有所期望發光特性之氮化物半導體紫外線發光元件。In the nitride semiconductor ultraviolet light emitting device according to the second feature, the quasi-stable AlGaN whose composition ratio of the Ga-rich EB region formed in the electron barrier layer is an integer ratio and the Ga-rich AlGaN in the n-type layer are used. In the n-type field, it is the same when forming quasi-stable AlGaN whose composition ratio of AlGaN is an integer ratio, suppressing characteristic variation due to drift of the crystal growth device, and stably producing nitride semiconductor ultraviolet light-emitting elements with desired light-emitting properties.
更且,根據上述第2特徵之氮化物半導體紫外線發光元件時,電子阻障層之平均性之AlN莫耳分率Xea成為(m+0.24)/12≦Xea<(m+1)/12之範圍內之故,對應於形成於Ga富化EB領域之Al mGa 12-mN 12(m=8~10)之AlGaN組成比,於電子阻障層內,使平台領域與Ga富化EB領域間之AlN莫耳分率差確保在約2%以上,調整平台領域之AlN莫耳分率之設定範圍。因此,p型層內之載子(電洞)在電子阻障層內包含較平台領域能帶隙能量小之平台領域之Ga富化EB領域之傾斜領域內,更安定地局部存在化,可於電子阻障層內,電流係優先安定流入Ga富化EB領域,達到氮化物半導體紫外線發光元件之特性變動之抑制。 Furthermore, in the nitride semiconductor ultraviolet light-emitting device according to the second feature, the average AlN molar fraction Xea of the electron barrier layer is the relationship between (m+0.24)/12≦Xea<(m+1)/12 Therefore, the AlGaN composition ratio of AlmGa12- mN12 ( m =8~10) formed in the Ga - rich EB field corresponds to the AlGaN composition ratio in the electron barrier layer, so that the plateau field and the Ga-rich EB are formed in the electronic barrier layer. The difference in AlN molar ratio between the fields is ensured to be more than about 2%, and the setting range of the AlN molar ratio in the platform field is adjusted. Therefore, the carriers (holes) in the p-type layer are more stably localized in the inclined domain of the Ga-enriched EB domain of the platform domain including the band gap energy of the platform domain in the electron barrier layer, which can be more stable and localized. In the electronic barrier layer, the current flows preferentially and stably into the Ga-enriched EB region, so as to suppress the characteristic variation of the nitride semiconductor ultraviolet light emitting device.
更且,本發明係除了上述第2特徵之外,於前述電子阻障層之前述平台領域內,存在局部性AlN莫耳分率為高的Al富化EB領域, 整數m為8或9之時,前述Al富化EB領域係包含AlGaN組成比成為整數比之Al m+1Ga 11-mN 12之p型AlGaN領域,前述電子阻障層之平均性AlN莫耳分率Xea在(m+0.5)/12<Xea<(m+1)/12之範圍內為第3特徵。 Furthermore, in addition to the above-mentioned second feature, in the present invention, there is an Al-enriched EB domain with a local high AlN molar fraction in the above-mentioned plateau domain of the above-mentioned electron barrier layer, and the integer m is 8 or 9. When the above-mentioned Al-enriched EB domain is a p-type AlGaN domain including Alm + 1Ga11 - mN12 whose composition ratio is an integer ratio, the average AlN molar fraction Xea of the above-mentioned electron barrier layer is in (m The third characteristic is within the range of +0.5)/12<Xea<(m+1)/12.
根據上述第3特徵之氮化物半導體紫外線發光元件時,利用各別形成於電子阻障層內之Ga富化EB領域與Al富化EB領域之AlGaN組成比為整數比之準安定AlGaN,與於n型層內之Ga富化n型領域與Al富化n型領域,各別形成AlGaN組成比為整數比之準安定AlGaN之時相同,抑制起因於結晶成長裝置之漂移等之特性變動,可期待安定生產具有所期望發光特性之氮化物半導體紫外線發光元件。In the nitride semiconductor ultraviolet light emitting device according to the third feature, the quasi-stable AlGaN in which the composition ratio of the AlGaN of the Ga-rich EB domain and the Al-rich EB domain formed in the electron barrier layer is an integer ratio is used, and the The Ga-enriched n-type region and the Al-enriched n-type region in the n-type layer are the same as when the quasi-stable AlGaN whose composition ratio of AlGaN is an integer ratio is formed, and the characteristic variation caused by the drift of the crystal growth device can be suppressed. The stable production of nitride semiconductor ultraviolet light-emitting elements with desired light-emitting properties is expected.
更且,上述第2或第3特徵之氮化物半導體紫外線發光元件係前述電子阻障層之平均性AlN莫耳分率Xea為(m+0.9)/12以下為佳。Furthermore, in the nitride semiconductor ultraviolet light emitting device of the second or third feature, the average AlN molar fraction Xea of the electron barrier layer is preferably (m+0.9)/12 or less.
根據上述適切實施形態時,上述第2或第3特徵之氮化物半導體紫外線發光元件中,於電子阻障層之傾斜領域之Ga富化EB領域域內,可更安定形成AlGaN組成比為Al mGa 12-mN 12之準安定AlGaN,於上述第3特徵之氮化物半導體紫外線發光元件中,於電子阻障層之平台領域之Al富化n型領域內,可更安定形成AlGaN組成比為Al m+1Ga 11-mN 12之準安定AlGaN。 According to the above-mentioned suitable embodiment, in the nitride semiconductor ultraviolet light emitting element of the second or third feature, in the Ga-rich EB region of the inclined region of the electron barrier layer, AlGaN can be more stably formed with a composition ratio of Alm The quasi-stable AlGaN of Ga 12-m N 12 , in the nitride semiconductor ultraviolet light-emitting element of the third feature, can be more stably formed in the Al-rich n-type region of the plateau region of the electron barrier layer, and the composition ratio is: Quasi-stable AlGaN of Al m+1 Ga 11-m N 12 .
更且,本發明係提供具備閃鋅礦構造之AlGaN系半導體所成n型層、活性層、及p型層,層積於上下方向之發光元件構造部的氮化物半導體紫外線發光元件 前述n型層係以n型AlGaN系半導體所構成, 配置於前述n型層與前述p型層之間之前述活性層,則具有包含AlGaN系半導體所構成之1層以上之阱層的量子井構造, 前述p型層係以p型AlGaN系半導體所構成, 前述n型層與前述活性層與前述p型層內之各半導體層則具有形成平行於(0001)面之多段狀之平台之表面的磊晶成長層, 前述活性層內之各半導體層及前述電子阻障層係各別具有對於連結前述多段狀之平台之鄰接之平台間之(0001)面傾斜之傾斜領域、和前述傾斜領域以外之平台領域, 前述n型層具有在前述n型層內一樣地分散存在之局部性AlN莫耳分率為低之層狀領域,和前述層狀領域以外之n型本體領域, 與前述n型層之上表面正交之第1平面上之前述層狀領域之各延伸方向,具有對於前述n型層之前述上面與前述第1平面之交線而言傾斜之部分, 前述p型層係具有作為前述p型層內之最下層,形成於前述1層以上之阱層之最上層之上面側的電子阻障層, 整數m為8或9, 於前述電子阻障層之前述傾斜領域內,存在包含AlGaN組成比成為整數比之Al mGa 12-mN 12之p型AlGaN領域,局部地AlN莫耳分率為低的Ga富化EB領域, 於前述電子阻障層之前述平台領域內,存在包含AlGaN組成比成為整數比之Al m+1Ga 11-mN 12之p型AlGaN領域,局部地AlN莫耳分率為高的Al富化EB領域, 前述電子阻障層之平均性AlN莫耳分率Xea成為(m+0.5)/12<Xea<(m+1)/12之範圍囲內, 於前述阱層之前述傾斜領域內,存在AlN莫耳分率局部性較前述阱層之前述平台領域之AlN莫耳分率為低之Ga富化阱領域為第4特徵之氮化物半導體紫外線發光元件。 Furthermore, the present invention provides a nitride semiconductor ultraviolet light-emitting element comprising an n-type layer, an active layer, and a p-type layer of an AlGaN-based semiconductor having a zinc blende structure, which are laminated on the light-emitting element structure portion in the vertical direction. The layer is composed of an n-type AlGaN-based semiconductor, and the active layer disposed between the n-type layer and the p-type layer has a quantum well structure including one or more well layers composed of the AlGaN-based semiconductor, and the above-mentioned The p-type layer is made of p-type AlGaN-based semiconductor, the n-type layer, the active layer, and the semiconductor layers in the p-type layer have epitaxial surfaces that form a multi-segment platform parallel to the (0001) plane. The growth layer, the semiconductor layers in the active layer and the electron barrier layer respectively have inclined regions that are inclined with respect to the (0001) plane between adjacent platforms connecting the multi-segment platforms, and platforms other than the inclined regions. The above-mentioned n-type layer has a localized AlN layered domain with a low molar fraction distributed uniformly in the above-mentioned n-type layer, and an n-type bulk domain other than the above-mentioned layered domain, and the above-mentioned n-type layer. Each extending direction of the layered region on a first plane orthogonal to the upper surface has a portion inclined with respect to the intersection of the upper surface of the n-type layer and the first plane, and the p-type layer has as the The lowermost layer in the p-type layer, the electron barrier layer formed on the upper surface side of the uppermost layer of the above-mentioned one or more well layers, the integer m is 8 or 9, and in the above-mentioned inclined area of the above-mentioned electron barrier layer, there are The p-type AlGaN region where the AlGaN composition ratio is an integer ratio of AlmGa12 - mN12 , the Ga-rich EB region where the AlN molar fraction is locally low, and the plateau region of the electron barrier layer, exist The p-type AlGaN domain including Alm + 1Ga11 - mN12 whose AlGaN composition ratio is an integer ratio, the Al-rich EB domain having a high AlN molar fraction locally, and the average AlN molar ratio of the aforementioned electron barrier layer The ear fraction Xea is within the range of (m+0.5)/12<Xea<(m+1)/12, and in the above-mentioned inclined region of the above-mentioned well layer, there is a higher locality of AlN molar rate than that of the above-mentioned well layer. The Ga-enriched well region with a low AlN molar fraction in the platform region is the nitride semiconductor ultraviolet light emitting device of the fourth feature.
根據上述第4特徵特徵之氮化物半導體紫外線發光元件時,與上述第2特徵之氮化物半導體紫外線發光元件相同,於電子阻障層之傾斜領域內,存在AlN莫耳分率局部性低之Ga富化EB領域,在Ga富化EB領域內,可產生載子(電洞)之局部存在化之故,植入於電子阻障層內之電洞係亦可直接植入傾斜領域內。此結果,直接植入於電子阻障層之傾斜領域內,不擴散平台領域內,到達發光再結合之局部存在中心之阱層之傾斜領域內之電洞量則大幅增加,可抑制於電子阻障層之傾斜領域內未形成Ga富化EB領域時所產生內部量子效率之下降、及雙發光尖峰之產生。According to the nitride semiconductor ultraviolet light emitting element according to the fourth feature, as in the nitride semiconductor ultraviolet light emitting element according to the second feature, in the slanted region of the electron barrier layer, there is Ga, which is locally low in AlN molar fraction. In the enriched EB field, in the Ga-enriched EB field, the localized existence of carriers (holes) can be generated, and the holes implanted in the electron barrier layer can also be directly implanted in the inclined field. As a result, directly implanted in the inclined area of the electron barrier layer, in the non-diffusion platform area, the amount of holes in the inclined area of the well layer that reaches the localized center of the light-emitting recombination is greatly increased, which can suppress the electron resistance. The decrease of the internal quantum efficiency and the generation of double emission peaks are caused when the Ga-enriched EB region is not formed in the inclined region of the barrier layer.
更且,根據上述第4特徵之氮化物半導體紫外線發光元件時,於電子阻障層內,經由對傾斜領域質量移動Ga,於傾斜領域內,形成Ga富化EB領域的同時,在鄰接於平台領域內化傾斜領域之端緣部,形成AlN莫耳分率較平台領域內之平均性AlN莫耳分率為高之Al富化EB領域。然後,利用各別形成於電子阻障層內之Ga富化EB領域與Al富化EB領域之AlGaN組成比為整數比之準安定AlGaN,於上述第1特徵之氮化物半導體紫外線發光元件中,與n型層內之Ga富化n型領域與Al富化n型領域,各別形成AlGaN組成比為整數比之準安定AlGaN之時相同,抑制起因於結晶成長裝置之漂移等之特性變動,可期待安定生產具有所期望發光特性之氮化物半導體紫外線發光元件。Furthermore, in the nitride semiconductor ultraviolet light emitting element according to the fourth feature, in the electron barrier layer, Ga-enriched EB regions are formed in the inclined regions by mass-shifting Ga to the inclined regions, and at the same time adjacent to the terraces. The edge of the sloping field is internalized to form an Al-rich EB field with a higher AlN molar ratio than the average AlN molar ratio in the plateau field. Then, using the quasi-stable AlGaN whose composition ratio of the Ga-rich EB domain and the Al-rich EB domain respectively formed in the electron barrier layer is an integer ratio, in the nitride semiconductor ultraviolet light emitting element of the above-mentioned first feature, In the same way as when the Ga-enriched n-type region and the Al-enriched n-type region in the n-type layer are respectively formed into quasi-stable AlGaN whose composition ratio is an integer ratio, it is possible to suppress characteristic variation due to drift of the crystal growth device, etc. Stable production of nitride semiconductor ultraviolet light-emitting elements with desired light-emitting properties can be expected.
更且,根據上述第4特徵之氮化物半導體紫外線發光元件時,電子阻障層之平均性之AlN莫耳分率Xea成為(m+0.5)/12<Xea<(m+1)/12之適切範圍內之故,對傾斜領域內之Ga供給量充分為大時,於Ga富化EB領域內,形成AlGaN組成比為Al mGa 12-mN 12之準安定AlGaN之同時,對於Al富化EB領域內,形成AlGaN組成比為Al n+1Ga 11-nN 12之準安定AlGaN。於Al富化EB領域內,藉由存在AlGaN組成比為Al m+1Ga 11-mN 12之準安定AlGaN,對於Ga富化EB領域內之Ga供給量之變動,及平均性之AlN莫耳分率Xea之變動則在存在於Al富化EB領域內之該準安定AlGaN中亦被吸收。即,藉由在鄰接於電子阻障層內之傾斜領域之Al富化EB領域內,存在能量上安定之準安定AlGaN,可抑制從平台領域經由Al富化EB領域之傾斜領域內之過剩之Ga之質量移動,而抑制Ga供給量之變動所造成Ga富化EB領域內之AlN莫耳分率之大幅之下降。 Furthermore, in the nitride semiconductor ultraviolet light emitting device according to the fourth feature, the average AlN molar fraction Xea of the electron barrier layer is the equation of (m+0.5)/12<Xea<(m+1)/12 Therefore, within the appropriate range, when the supply amount of Ga in the inclined region is sufficiently large, in the Ga-rich EB region, quasi-stable AlGaN with a composition ratio of AlmGa12 - mN12 is formed, while the Al-rich AlGaN is formed. In the chemical EB field, quasi-stable AlGaN with a composition ratio of Aln + 1Ga11 - nN12 is formed. In the field of Al-enriched EB, due to the presence of quasi-stable AlGaN with a composition ratio of Alm +1 Ga 11-m N 12 , the variation of Ga supply in the field of Ga-enriched EB, and the average AlN molar The variation in ear fraction Xea is also absorbed in the quasi-stable AlGaN present in the Al-rich EB domain. That is, by the presence of energy-stable quasi-stable AlGaN in the Al-rich EB region adjacent to the slanted region in the electron barrier layer, excess in the slanted region from the plateau region via the Al-rich EB region can be suppressed. The mass shift of Ga suppresses the significant drop in the molar ratio of AlN in the Ga-enriched EB area caused by the change in the supply amount of Ga.
更且,上述第4特徵之氮化物半導體紫外線發光元件係前述電子阻障層之平均性AlN莫耳分率Xea為(m+0.9)/12以下為佳。Furthermore, in the nitride semiconductor ultraviolet light emitting device of the fourth feature, the average AlN molar fraction Xea of the electron barrier layer is preferably (m+0.9)/12 or less.
根據上述適切實施形態時,於電子阻障層之傾斜領域之Ga富化EB領域內,可更安定形成AlGaN組成比為Al mGa 12-mN 12之準安定AlGaN,於鄰接於平台領域之傾斜領域之端緣部之Al富化EB領域內,可更安定形成AlGaN組成比為Al m+1Ga 11-mN 12之準安定AlGaN。 According to the above-mentioned suitable embodiment, in the Ga-enriched EB region of the inclined region of the electron barrier layer, quasi-stable AlGaN with a composition ratio of AlmGa12 - mN12 can be formed more stably in the region adjacent to the plateau region. In the Al-enriched EB region at the edge of the inclined region, quasi-stable AlGaN with the AlGaN composition ratio of Alm + 1Ga11 - mN12 can be formed more stably.
更且,本發明係除了上述第4特徵,提供整數n為5、6、7、或8中, 於前述層狀領域內,存在包含AlGaN組成比成為整數比之Al nGa 12-nN 12之n型AlGaN領域的Ga富化n型領域, 前述n型層之平均性AlN莫耳分率Xna成為(n+0.24) /12<Xna<(n+1)/12之範圍內之第5特徵之氮化物半導體紫外線發光元件。 Furthermore, in addition to the above-mentioned fourth feature, the present invention provides that when the integer n is 5, 6, 7, or 8, in the aforementioned layered region, there is AlnGa12 - nN12 including AlGaN whose composition ratio is an integer ratio. In the Ga-enriched n-type region of the n-type AlGaN region, the average AlN molar fraction Xna of the n-type layer is the fifth in the range of (n+0.24)/12<Xna<(n+1)/12 Characteristic nitride semiconductor ultraviolet light-emitting element.
根據上述第5特徵之氮化物半導體紫外線發光元件時,伴隨從n型本體領域至層狀領域內之Ga之質量移動,層狀領域內之AlN莫耳分率則下降,對層狀領域內之Ga之質量移動量充分為大時,於層狀領域內,形成包含AlGaN組成比為Al nGa 12-nN 12之n型AlGaN領域之Ga富化n型領域。前述準安定AlGaN之AlN莫耳分率係接近較n型層之平均性AlN莫耳分率Xna為低之AlN莫耳分率(n/12),於Ga富化n型領域內,藉由存在AlGaN組成比為Al nGa 12-nN 12之準安定AlGaN,對於Ga富化n型領域內之Ga供給量之變動,及平均性之AlN莫耳分率Xna之變動則於該準安定AlGaN被吸收。即,於Ga富化n型領域內,增加Ga供給量,或AlN莫耳分率Xna下降時,準安定AlGaN則增加,減少Ga供給量,或AlN莫耳分率Xna上昇時,準安定AlGaN則減少,就結果而言,抑制Ga富化n型領域內之AlN莫耳分率之變動。 According to the nitride semiconductor ultraviolet light-emitting element according to the fifth feature, as the mass of Ga moves from the n-type bulk region to the layered region, the molar ratio of AlN in the layered region decreases. When the mass shift amount of Ga is sufficiently large, a Ga - enriched n-type region including an n -type AlGaN region with AlGaN composition ratio of AlnGa12 -nN12 is formed in the layered region. The AlN molar ratio of the aforementioned quasi-stable AlGaN is close to the AlN molar ratio (n/12) which is lower than the average AlN molar ratio Xna of the n-type layer. In the Ga-enriched n-type region, by There is a quasi-stable AlGaN whose AlGaN composition ratio is AlnGa12 -nN12, and the fluctuation of Ga supply in the Ga - enriched n -type region and the fluctuation of the average AlN molar ratio Xna are in this quasi-stable AlGaN is absorbed. That is, in the Ga-enriched n-type region, when the supply amount of Ga increases or the AlN molar ratio Xna decreases, the quasi-stable AlGaN increases and the Ga supply amount decreases, or when the AlN molar ratio Xna increases, the quasi-stable AlGaN increases is reduced, and as a result, the variation in the molar ratio of AlN in the Ga-enriched n-type region is suppressed.
更且,根據上述第5特徵之氮化物半導體紫外線發光元件時,n型層之平均性之AlN莫耳分率Xna成為(n+0.24)/12<Xna<(n+1)/12之範圍內之故,對應於形成於Ga富化n型領域之Al nGa 12-nN 12(n=5~8)之AlGaN組成比,於n型層內,使層狀領域與n型本體領域間之AlN莫耳分率差確保在約2%以上,調整n型本體領域之AlN莫耳分率之設定範圍。因此,n型層內之載子(電子)係於n型層內,在包含較n型本體領域能帶隙能量小之Ga富化n型領域之層狀領域內,更安定地局部存在化,可於n型層內,電流係可優先安定流入Ga富化n型領域,達到氮化物半導體紫外線發光元件之特性變動之抑制。 Furthermore, in the nitride semiconductor ultraviolet light emitting device according to the fifth feature, the average AlN molar fraction Xna of the n-type layer is in the range of (n+0.24)/12<Xna<(n+1)/12 Therefore, corresponding to the AlGaN composition ratio of AlnGa12- nN12 ( n =5~8) formed in the Ga - enriched n-type region, in the n-type layer, the layered region and the n-type bulk region are formed. The difference in AlN molar ratio between them is ensured to be more than about 2%, and the setting range of the AlN molar ratio in the n-type body area is adjusted. Therefore, the carriers (electrons) in the n-type layer are localized in the n-type layer more stably and locally in the layered domain including the Ga-enriched n-type domain with a smaller energy bandgap energy than the n-type bulk domain. In the n-type layer, the current system can preferentially and stably flow into the Ga-enriched n-type region, so as to suppress the characteristic variation of the nitride semiconductor ultraviolet light-emitting element.
更且,本發明係除了上述第1乃至第5特徵,提供前述活性層係具有包含2層以上之前述阱層之多重量子井構造,於2層之前述阱層間,存在以AlGaN系半導體構成之阻障層為第6特徵之氮化物半導體紫外線發光元件。Furthermore, the present invention provides, in addition to the above-mentioned first to fifth features, that the active layer has a multiple quantum well structure including two or more of the well layers, and between the two well layers, there is a structure composed of an AlGaN-based semiconductor. The barrier layer is the nitride semiconductor ultraviolet light emitting element of the sixth feature.
根據上述第6特徵之氮化物半導體紫外線發光元件,活性層則成為多重量子井構造,阱層則較僅1層之時,可期待發光效率之提升。According to the nitride semiconductor ultraviolet light emitting device of the sixth feature, the active layer has a multiple quantum well structure, and the well layer can be expected to improve the luminous efficiency compared to the case of only one layer.
更且,於上述第6特徵之氮化物半導體紫外線發光元件中,前述阻障層係以AlGaN系半導體所構成,各別具有對於連結前述多段狀之平台之鄰接之平台間之(0001)面傾斜之傾斜領域、和前述傾斜領域以外之平台領域,於前述阻障層之前述傾斜領域內,存在AlN莫耳分率局部地較前述阻障層之前述平台領域之AlN莫耳分率為低之Ga富化阻障領域為佳。Furthermore, in the nitride semiconductor ultraviolet light emitting device of the sixth feature, the barrier layer is formed of an AlGaN-based semiconductor, and each has a (0001) plane inclination with respect to the adjacent terraces connecting the multi-segment terraces. In the inclined area of the barrier layer, and the plateau area other than the inclined area, the AlN molar ratio in the inclined area of the barrier layer is locally lower than the AlN molar rate in the plateau area of the barrier layer. Ga enrichment barrier field is better.
經由上述之適切之實施形態,於阻障層中,與n型層之Ga富化n型領域及阱層之Ga富化阱領域同樣地,於Ga富化阻障領域中,可產生載子之局部存在化。因此,於從n型層朝向在阱層發光集中之鄰接之平台間之傾斜領域內之Ga富化阱領域之供給載子(電子)之時,可經由n型層之Ga富化n型領域與阻障層之Ga富化阻障領域,有效率地加以進行。Through the above-mentioned appropriate embodiments, in the barrier layer, similarly to the Ga-enriched n-type region of the n-type layer and the Ga-enriched well region of the well layer, carriers can be generated in the Ga-enriched barrier region localized existence. Therefore, when supplying carriers (electrons) from the n-type layer to the Ga-enriched well region in the inclined region between the adjacent terraces of the well layer emission concentration, the Ga-enriched n-type region of the n-type layer can be passed through. The Ga-enriched barrier area of the barrier layer is efficiently performed.
於上述第6特徵之氮化物半導體紫外線發光元件之上述適切實施形態中, 整數j為6、7、8、9或10, 前述Ga富化阻障領域係包含AlGaN組成比成為整數比之Al jGa 12-jN 12之AlGaN領域,前述阻障層之平均性AlN莫耳分率Xba成為(j+0.24)/12≦Xba<(j+1)/12之範圍內為更佳。 In the above-mentioned suitable embodiment of the nitride semiconductor ultraviolet light emitting device of the above-mentioned sixth feature, the integer j is 6, 7, 8, 9 or 10, and the Ga-enriched barrier region includes Alj whose composition ratio of AlGaN becomes an integer ratio. In the AlGaN field of Ga 12-j N 12 , it is more preferable that the average AlN molar fraction Xba of the barrier layer is in the range of (j+0.24)/12≦Xba<(j+1)/12.
經由上述適切實施形態,抑制起因於結晶成長裝置之漂移等之混晶莫耳分率之變動,於阻障層內,產生載子之局部存在化之傾斜領域,則以對應於整數j之AlN莫耳分率安定地加以形成。By the above-mentioned suitable embodiment, the variation of the mixed crystal molar ratio caused by the drift of the crystal growth device, etc. is suppressed, and in the barrier layer, the inclined region of the localization of the carrier is generated, and the AlN corresponding to the integer j is used. The mole fraction is formed stably.
更且,上述第1至第6之任一特徵之氮化物半導體紫外線發光元件係更具備包含藍寶石基板之基材部,前述藍寶石基板係對於(0001)面而言,具有僅傾斜特定之角度之主面,於該主面之上方,形成前述發光元件構造部,至少從前述藍寶石基板之前述主面至前述活性層之表面之各半導體層係具有形成平行於(0001)面之多段狀之平台之表面的磊晶成長層為佳。Furthermore, the nitride semiconductor ultraviolet light emitting element of any one of the first to sixth features further includes a base portion including a sapphire substrate, and the sapphire substrate is inclined only by a specific angle with respect to the (0001) plane. The main surface, above the main surface, the light-emitting element structure portion is formed, at least each semiconductor layer from the main surface of the sapphire substrate to the surface of the active layer has a multi-segment platform parallel to the (0001) plane. The epitaxial growth layer on the surface is better.
經由上述適切之實施形態,可使用具有偏角之藍寶石基板,於從藍寶石基板之主面至活性層之表面之各層之表面,以表現出多段狀之平台之方式,進行磊晶成長,實現上述各特徵之氮化物半導體紫外線發光元件。Through the above-mentioned suitable embodiments, a sapphire substrate with an off-angle can be used to perform epitaxial growth on the surface of each layer from the main surface of the sapphire substrate to the surface of the active layer in the form of a multi-segment platform to achieve the above Nitride semiconductor ultraviolet light-emitting element of each characteristic.
於上述第1至第6之任一特徵之氮化物半導體紫外線發光元件中, 整數k為3、4、5、6、或7,且對於整數n而言,k≦n-1, 前述Ga富化阱領域係包含AlGaN組成比成為整數比之Al kGa 12-kN 12之AlGaN領域為更佳。 In the nitride semiconductor ultraviolet light emitting device according to any one of the first to sixth features, the integer k is 3, 4, 5, 6, or 7, and for the integer n, k≦n−1, and the aforementioned Ga-rich The chemical well region is preferably an AlGaN region including AlkGa12 - kN12 in which the composition ratio of AlGaN is an integer ratio.
經由上述適切實施形態,抑制起因於結晶成長裝置之漂移等之混晶莫耳分率之變動,於阱層內,產生載子之局部存在化之傾斜領域,則以對應於尖峰發光波長之目標值所決定之整數k之AlN莫耳分率安定地加以形成。 [發明效果] By the above-mentioned suitable embodiment, the variation of the mixed crystal molar ratio caused by the drift of the crystal growth device, etc. is suppressed, and in the well layer, the inclined region of the localization of the carrier is generated, and the target corresponding to the peak emission wavelength is made. The AlN molar ratio of the integer k determined by the value is stably formed. [Inventive effect]
根據上述仕一特徵之氮化物半導體紫外線發光元件時,可安定提供抑制起因於結晶成長裝置之漂移等之特性變動之具有所期望發光特性之氮化物半導體紫外線發光元件。According to the nitride semiconductor ultraviolet light emitting element according to the above-mentioned feature, it is possible to stably provide a nitride semiconductor ultraviolet light emitting element having desired light emitting characteristics and suppressing characteristic variation due to drift or the like of the crystal growth device.
關於本發明之實施形態之氮化物半導體紫外線發光元件(以下,單純略稱為「發光元件」),根據圖面加以說明。然而,以下說明所使用之圖面之模式圖中,為了容易理解說明,強調主要部分,模式性顯示本發明內容之故,各部之尺寸不見得與實際之元件有相同尺寸。以下、本實施形態中,發光元件假定為發光二極體之情形加以說明。The nitride semiconductor ultraviolet light-emitting element (hereinafter, simply abbreviated as "light-emitting element") according to the embodiment of the present invention will be described with reference to the drawings. However, in the schematic drawings of the drawings used in the following description, in order to facilitate the understanding of the description, the main parts are emphasized and the content of the present invention is schematically shown, and the dimensions of each part are not necessarily the same as the actual components. Hereinafter, in this embodiment, the light-emitting element will be described as a light-emitting diode.
[第1實施形態]
<發光元件之元件構造>
如圖6所示,第1實施形態之發光元件1係具備包含藍寶石基板11之基材部10、和複數之AlGaN系半導體層21~24、包含p電極26及n電極27之發光元件構造部20。發光元件1係將發光元件構造部20側(圖6之圖中上側)朝向安裝用之基台(副固定座等)加以安裝(覆晶安裝)者,光取出方向係基材部10側(圖6之圖中下側)。然而,本說明書中,為了說明上之方便,將垂直於藍寶石基板11之主面11a(或基材部10及各AlGaN系半導體層21~24之上面)之方向稱之為「上下方向」(或「縱方向」),令從基材部10朝向發光元件構造部20之方向為上方向、其相反者為下方向。又,令平行於上下方向之平面稱之為「第1平面」。更且,將平行於藍寶石基板11之主面11a(或基材部10及各AlGaN系半導體層21~24之上面)之平面稱之為「第2平面」,將平行於該第2平面之方向稱為「橫方向」。
[1st Embodiment]
<Element structure of light-emitting element>
As shown in FIG. 6 , the light-emitting
基材部10係具備藍寶石基板11、和直接形成於藍寶石基板11之主面11a上之AlN層12而構成。藍寶石基板11係主面11a對於(0001)面以一定之範圍內(例如0度至6度程度)之角度(偏角)傾斜,於主面11a上表現出多段狀之平台之微傾斜基板。The
AlN層12係以從藍寶石基板11之主面磊晶成長之AlN結晶加以構成,此AlN結晶係對於藍寶石基板11之主面11a而言,具有磊晶之結晶方位關係。具體而言,例如為使藍寶石基板11之C軸方向(<0001>方向)與AlN結晶之C軸方向一致,成長AlN結晶。然而,構成AlN層12之AlN結晶係可包含微量之Ga或其他之不純物,亦可為AlN系半導體層。本實施形態中,作為AlN層12之膜厚,假設為2μm~3μm程度。然而,基材部10之構造及使用之基板等係非限定於上述構成。例如,於AlN層12與AlGaN系半導體層21之間,具備AlN莫耳分率為該AlGaN系半導體層21之AlN莫耳分率以上之AlGaN系半導體層亦可。The
發光元件構造部20之AlGaN系半導體層21~24係具備從基材部10側順序地,依n型包覆層21(n型層)、活性層22、電子阻障層23(p型層)、p型連接層24(p型層)之順序磊晶成長加以層積之構造。The AlGaN-based semiconductor layers 21 to 24 of the light-emitting
本實施形態中,從藍寶石基板11之主面11a順序磊晶成長之基材部10之AlN層12、及發光元件構造部20之n型包覆層21和活性層22內之各半導體層與電子阻障層23係具有由來於藍寶石基板11之主面11a之形成平行於(0001)面之多段狀之平台之表面。然而,對於p型層之p型連接層24,於電子阻障層23上,經由磊晶成長而形成之故,雖可形成同樣之多段狀之平台,但亦可不具有形成同樣之多段狀之平台之表面。In the present embodiment, the
然而,如圖6所示,發光元件構造部20之內、活性層22、電子阻障層23、及p型連接層24係層積於n型包覆層21之上面之第2領域R2上之部分則經由蝕刻等加以除去,形成於、n型包覆層21之上面之第1領域R1上。然後,n型包覆層21之上面係露出於排除第1領域R1之第2領域R2中。n型包覆層21之上面係如圖6模式性顯示,在第1領域R1與第2領域R2間,有高度不同之情形,此時n型包覆層21之上面係於第1領域R1與第2領域R2中,個別加以規定。However, as shown in FIG. 6 , the
n型包覆層21係以n型AlGaN系半導體加以構成,於n型包覆層21內,在n型包覆層21內,一樣分散存在局部性AlN莫耳分率低之層狀領域21a。層狀領域21a係在先前技術之欄之上述所述,能帶隙能量局部地變小之故,載子易於局部存在化,作為低阻抗之電流路徑工作。該層狀領域21a中,如上所述,支配存在包含AlGaN組成比成為整數比之Al
nGa
12-nN
12之n型AlGaN領域(即,AlN莫耳分率為12分之n(n/12)之n型之準安定AlGaN)的Ga富化n型領域。惟,本實施形態中,整數n為5、6、7、或8。即,含於Ga富化n型領域之n型之準安定AlGaN係Al
5Ga
7N
12和Al
1Ga
1N
2和Al
7Ga
5N
12和Al
2Ga
1N
3之4種類,AlN莫耳分率係各別為41.7%(12分之5)、50%(2分之1)、58.3%(12分之7)、66.7%(3分之2)。圖6中,模示性顯示作為於層狀領域21a內,支配存在Ga富化n型領域之一例,層狀領域21a所有成為Ga富化n型領域之情形。令n型包覆層21內之層狀領域21a以外之領域,稱之為n型本體領域21b。
The n-
雖在圖6未圖示,包含Ga富化n型領域之層狀領域21a內係,經由從n型本體領域21b之Ga之質量移動加以形成之故,於n型本體領域21b中,尤其於挾持層狀領域21a之兩側之端緣部,形成局部性AlN莫耳分率高之Al富化n型領域。更且,本實施形態中,於Al富化n型領域,存在AlGaN組成比成為整數比之Al
n+1Ga
11-nN
12之n型AlGaN領域(即,AlN莫耳分率為12分之(n+1)之n型之準安定AlGaN)。即,存在於Al富化n型領域之n型之準安定AlGaN之AlN莫耳分率係較存在於Ga富化n型領域之n型之準安定AlGaN之AlN莫耳分率高12分之1(約8.3%)。以下之中,為了簡潔說明,令存在於Ga富化n型領域內之AlGaN組成比成為整數比之Al
nGa
12-nN
12之準安定AlGaN之n型AlGaN領域,在方便上稱之為「第1準安定n型領域」,令存在於Al富化n型領域內之AlGaN組成比成為整數比之Al
n+1Ga
11-nN
12之準安定AlGaN之n型AlGaN領域,在方便上稱之為「第2準安定n型領域」。
Although not shown in FIG. 6, the inner system of the
本實施形態中,n型包覆層21之平均性AlN莫耳分率Xna係調整成為(n+0.5)/12<Xna<(n+1)/12之第1適切範圍內,更佳為調整成為(n+0.5)/12<Xna≦(n+0.9) /12之第2之適切範圍內。In the present embodiment, the average AlN molar fraction Xna of the n-
n型包覆層21之平均性AlN莫耳分率Xna係如後述,於n型包覆層21之成膜時,作為AlN莫耳分率之目標值加以使用。又,平均性AlN莫耳分率Xna係在形成於n型包覆層21之成膜時之多段狀之平台及連絡該平台間之邊界領域各別複數含於橫方向之寬廣範圍內,例如可經由拉塞福背向散射(RBS)分析法所成n型包覆層21內之Al與Ga之組成分析加以測定。RBS分析法中,例如雖將He
2+離子束(束徑:2.2mm)以加速電壓2.3MeV,從試料之n型包覆層21之上面側垂直照射,但垂直方向之測定範圍大到300nm程度之故,分析對象之膜厚需較300nm為大。因此,對於膜厚不足300nm之n型包覆層21以外之半導體層而言、平均性AlN莫耳分率係經由後述之能量分散型X線分光法(剖面TEM-EDX),或CL(陰極射線發光)法,求得分為複數之領域加以測定之AlN莫耳分率之平均值。
The average AlN molar fraction Xna of the n-
如上所述,對於從n型本體領域21b向層狀領域21a內之Ga之質量移動量而言之Ga富化n型領域內之AlN莫耳分率之下降程度(令平均性AlN莫耳分率Xna作為基準)係較Al富化n型領域內之AlN莫耳分率之增加程度為大。因此,如模式性顯示於圖7之左側部分,經由令AlN莫耳分率Xna設定成較Ga富化n型領域內之第1準安定n型領域之AlN莫耳分率(Xn0=n/12)與Al富化n型領域之第2準安定n型領域之AlN莫耳分率(Xn1=(n+1)/12)之平均值((n+0.5)/12)為高,對應Ga之質量移動量,於Ga富化n型領域內與Al富化n型領域內,可各別安定形成AlN莫耳分率僅不同12分之1之2種類之準安定n型領域。在此,如模式性顯示於圖7之右側部分,經由令AlN莫耳分率Xna設定成較上述平均值((n+0.5)/12)為低,Ga之質量移動量過度增加之時,於層狀領域21a內,形成AlN莫耳分率Xn0(=n/12)之第1準安定n型領域之外,可更形成AlN莫耳分率低之非準安定AlGaN。更且,Ga之質量移動量不充分之時,Al富化n型領域內之AlN莫耳分率係無法達到第2準安定n型領域之AlN莫耳分率Xn1(=(n+1)/12)。As described above, with respect to the mass shift amount of Ga from the n-
排除Al富化n型領域之n型本體領域21b之平均性AlN莫耳分率係與n型包覆層21之平均性AlN莫耳分率Xna略同。因此,支配存在AlN莫耳分率為n/12之第1準安定n型領域之Ga富化n型領域之AlN莫耳分率與n型本體領域21b之平均性AlN莫耳分率之差係成為1/24(約4.17%)以上之故,可安定發揮載子之局部存在化之效果。The average AlN molar ratio of the n-
經由將Ga富化n型領域與Al富化n型領域各別以安定度高之第1及第2準安定n型領域構成,可抑制起因於結晶成長裝置之漂移等之混晶莫耳分率之變動,於n型包覆層21內,產生載子之局部存在化之Ga富化n型領域,則以對應於使用之第1準安定n型領域之AlN莫耳分率安定地加以形成。此結果,於n型包覆層21內,電流係優先安定流入Ga富化n型領域,更可達成發光元件1之特性變動之抑制。By forming the Ga-enriched n-type region and the Al-enriched n-type region with the first and second quasi-stable n-type regions with high stability, respectively, it is possible to suppress the mixed crystal molar ratio due to drift of the crystal growth device. In the n-
本實施形態中,作為n型包覆層21之膜厚,雖與一般氮化物半導體紫外線發光元件所採用之膜厚相同,設想為1μm~2μm,但該膜厚係亦可為2μm~4μm程度。In the present embodiment, the film thickness of the n-
n型包覆層21之層狀領域21a係於圖6中,1個層則以2重線模式性顯示,複數層則向上下方向遠離存在。又,以平行於上下方向之1個之第1平面(例如,圖6所示剖面),層狀領域21a之至少一部分之延伸方向則對於橫方向(第1平面與第2平面之交線之延伸方向)而言成為傾斜。層狀領域21a之上述特徵係在圖23所示以往之氮化物半導體紫外線發光元件之n型包覆層之HAADF-STEM像中亦被確認。The
然而,圖6所示第1平面上,層狀領域21a之各層雖以模式性平行之線(2重線)以圖示,該延伸方向與橫方向所成傾斜角係在各層狀領域21a間,並非一定相同,在相同層狀領域21a內,會由於位置而有所變化之故,第1平面上之層狀領域21a係非一定限定為延伸成直線狀。又,該傾斜角係經由第1平面之朝向而變化。因此,層狀領域21a之一部分則於第1平面上,可與其他之層狀領域21a交叉,或,可從其他之層狀領域21a分歧。However, on the first plane shown in FIG. 6, although each layer of the layered
又,層狀領域21a係於圖6中之第1平面上,雖各別以1條之線(2重線)顯示,垂直於該第1平面之方向中,平行或傾斜延伸於第2平面,具有2次元之擴展。因此,複數之層狀領域21a係在n型包覆層21內之複數之第2平面上,存在成條紋狀。In addition, the
層狀領域21a係如上所述,於n型包覆層21內,局部性AlN莫耳分率低之領域。即,層狀領域21a之AlN莫耳分率則相對於n型本體領域21b之AlN莫耳分率為低。又,於層狀領域21a與n型本體領域21b之邊界附近,兩領域之AlN莫耳分率澌進地連續之時,兩領域間之邊界則無法明確規定。The
n型包覆層21內之層狀領域21a之AlN莫耳分率係即,Ga富化n型領域內之第1準安定n型領域之AlN莫耳分率(n/12)、更具體而言,令整數n成為5、6、7或8之任一者,如後所述,對應於阱層220內之AlN莫耳分率加以設定,阱層220內之AlN莫耳分率係對應於尖峰發光波長之目標值加以設定。The AlN molar ratio of the layered
活性層22係具備交互層積以AlGaN系半導體或GaN系半導體所構成之2層以上之阱層220、和以AlGaN系半導體或AlN系半導體所構成之1層以上之阻障層221的多重量子井構造。於最下層之阱層220與n型包覆層21之間,無需一定設置阻障層221。又,本實施形態中,作為較佳實施形態,於最上層之阱層220與電子阻障層23之間,雖未設置阻障層221,作為較佳實施形態,設置較阻障層221為薄之膜AlN莫耳分率高之AlGaN層或AlN層亦可。The
電子阻障層23係以p型AlGaN系半導體所構成。p型連接層24係以p型AlGaN系半導體或p型GaN系半導體所構成。p型連接層24係典型地以p-GaN所構成。The
於圖8,模式顯示活性層22之阱層220及阻障層221之層積構造(多重量子井構造)之一例。圖8中,例示阱層220為3層,阻障層221為2層之情形。最上層之阱層220係位於電子阻障層23與上側之阻障層221之間,中間之阱層220係位於上側與下側之阻障層221之間,最下層之阱層220係位於下側之阻障層221與n型包覆層21之間。In FIG. 8, an example of the laminated structure (multiple quantum well structure) of the
圖8所示阱層220、阻障層221及電子阻障層23之平台T成長成多段狀之構造係如上述非專利文獻1及2所揭示,為公知之構造。於各層中,鄰接於橫方向之平台T間係如上述,形成對於(0001)面傾斜之傾斜領域IA。令傾斜領域IA以外之上下被平台T挾持之領域,稱之為平台領域TA。本實施形態中,1個平台T之深度(鄰接之傾斜領域IA間之距離)係設想為數10nm~數100nm。因此,於傾斜領域IA內表現出階梯狀之(0001)面係與多段狀之平台T之平台面區分。The structure in which the
如圖8模式性顯示,於電子阻障層23中,於傾斜領域IA內,形成較平台領域TA,AlN莫耳分率為低之Ga富化EB領域23a。阱層220以AlGaN系半導體所構成,AlN莫耳分率不為0%之時,於阱層220之各層中,於傾斜領域IA內,形成較平台領域TA,AlN莫耳分率為低之第Ga富化阱領域220a。阻障層221以AlGaN系半導體所構成,AlN莫耳分率不為100%之時,於阱層221之各層中,與電子阻障層23及阱層220同樣,於傾斜領域IA內,形成較平台領域TA,AlN莫耳分率為低之Ga富化阻障領域221a。於電子阻障層23、阱層220、及阻障層221之各層,經由從平台領域TA至傾斜領域IA之Ga之質量移動,於各別傾斜領域IA內,形成局部性AlN莫耳分率為低之Ga富化EB領域23a、Ga富化阱領域220a、及Ga富化阻障領域221a。As schematically shown in FIG. 8 , in the
即,n型包覆層21中,於局部性AlN莫耳分率低之層狀領域21a,載子易於局部存在化,活性層22中,於存在於阱層220之傾斜領域IA內之局部性AlN莫耳分率低之Ga富化阱領域220a,於存在阻障層221之傾斜領域IA內之局部性AlN莫耳分率低之Ga富化阻障領域221a中,各別載子易於部存在化,電子阻障層23中,於存在於傾斜領域IA內之局部性AlN莫耳分率低之Ga富化EB領域23a中,載子則載於局部存在化。因此,從n型包覆層21側係隔著層狀領域21a,從電子阻障層23側係隔著Ga富化EB領域23a,對於阱層220之Ga富化阱領域220a,可各別有效率供給載子,成為可達成阱層220內之載子(電子及電洞)之再結合所成發光效率之提升的元件構造。That is, in the n-
更且,圖8中雖未圖示,作為較佳實施形態,於電子阻障層23中,於鄰接於傾斜領域IA之平台領域TA之端緣部,令電子阻障層23之平均性AlN莫耳分率Xea作為基準,形成局部性AlN莫耳分率為高之Al富化EB領域。Moreover, although not shown in FIG. 8, as a preferred embodiment, in the
更且,圖8中雖未圖示,作為較佳實施形態,阻障層221以AlGaN系半導體構成,AlN莫耳分率非100%之時,於阻障層221之各層中,與電子阻障層23相同,於鄰接於傾斜領域IA之平台領域TA之端緣部,令阻障層221之平均性AlN莫耳分率Xba作為基準,形成局部性AlN莫耳分率為高之Al富化阻障領域。Furthermore, although not shown in FIG. 8 , as a preferred embodiment, the
電子阻障層23及阻障層221之平均性AlN莫耳分率Xea及Xba係如後述,於電子阻障層23及阻障層221之各成膜時,作為AlN莫耳分率之目標值加以使用。The average AlN molar fractions Xea and Xba of the
本實施形態中,電子阻障層23之膜厚係包含平台領域TA及傾斜領域IA,例如設定在15nm~30nm之範圍內(最佳值為約20nm)。阱層220之膜厚係包含平台領域TA及傾斜領域IA,例如在1.5單元晶胞~7單元晶胞之範圍內,對應於發光元件1之尖峰發光波長之目標值加以設定。又,阻障層221之膜厚係包含平台領域TA及傾斜領域IA,例如在6nm~8nm之範圍內加以設定。In this embodiment, the film thickness of the
阱層220係以AlGaN系半導體加以構成,AlN莫耳分率非0%之時,阱層220之Ga富化阱領域220a之AlN莫耳分率係對應於發光元件1之尖峰發光波長之目標值加以設定。作為較佳之實施形態,於阱層220之Ga富化阱領域220a中,形成AlGaN組成比為整數比之Al
kGa
12-kN
12之準安定AlGaN所成準安定阱領域。惟,整數k係3、4、5、6或7,對應尖峰發光波長之目標值加以決定。即,存在於Ga富化阱領域220a之準安定阱領域係Al
1Ga
3N
4、Al
1Ga
2N
3、Al
5Ga
7N
12、Al
1Ga
1N
2、Al
7Ga
5N
12之5種類,AlN莫耳分率係各別為25%(4分之1)、33.3%(3分之1)、41.7%(12分之5)、50%(2分之1)、58.3%(12分之7)。然而,作為一實施形態,雖於Ga富化阱領域220a內支配存在準安定阱領域為佳,於Ga富化阱領域220a內,包含AlN莫耳分率成為準安定阱領域與阱層220之平台領域TA之各AlN莫耳分率之中間之AlN莫耳分率的領域亦可,於相關之情形下,於阱層220之傾斜領域IA內,產生載子之局部存在化。
The
作為上述較佳之一實施形態,經由將Ga富化阱領域220a以安定度高之準安定阱領域構成,伴隨將n型包覆層21內之Ga富化n型領域與Al富化n型領域各別以安定度高之第1及第2準安定n型領域構成所成效果,起因於結晶成長裝置之漂移等之混晶莫耳分率之變動在阱層220內亦被抑制,於阱層220內,產生載子之局部存在化之Ga富化阱領域220a,則以對應於使用之準安定阱領域之AlN莫耳分率安定地加以形成。此結果,於阱層220內,電流係優先安定流入Ga富化阱領域,更可達成發光元件1之特性變動之抑制。As a preferred embodiment of the above, the Ga-enriched
阱層220係以GaN系半導體加以構成,AlN莫耳分率為0%之時,鄰接於阱層220之阻障層、電子阻障層23、及n型包覆層21之AlN莫耳分率及阱層220之膜厚係對應於發光元件1之尖峰發光波長之目標值加以設定。The
圖9、圖10及圖11係對於阱層220及阻障層221以AlGaN構成之量子井構造模型而言,圖表化將阱層之膜厚在3ML(單原子層)~14ML(1.5單元晶胞~7單元晶胞)或4ML~14ML(2單元晶胞~7單元晶胞)之範圍內變化所得之發光波長之模擬結果(相當於尖峰發光波長)者。作為上記模擬之條件,圖9中,將阱層220之Ga富化阱領域220a之AlN莫耳分率,成為準安定阱領域之AlN莫耳分率之50%(2分之1),圖10中,將阱層220之Ga富化阱領域220a之AlN莫耳分率,成為準安定阱領域之AlN莫耳分率41.7%(12分之5),圖11中,將阱層220之Ga富化阱領域220a之AlN莫耳分率,成為準安定阱領域之AlN莫耳分率33.3%(3分之1),於圖9~圖11之各別中,阻障層221之Ga富化阻障領域221a之AlN莫耳分率係成為66.7%(3分之2)、75%(4分之3)、及、83.3%(6分之5)之3種。圖9~圖11所示模擬結果中,阱層220之紫外線發光設想在傾斜領域IA顯著發生。為此,阱層220之膜厚條件係滿足於該傾斜領域IA是為重要。FIGS. 9 , 10 and 11 are for the quantum well structure model in which the
經由圖9~圖11,可知阱層220之膜厚為3ML~14ML之範圍內時,阱層220之膜厚愈小,對於阱層220之量子封閉效果愈大,發光波長則短波長化,更且,阻障層221之AlN莫耳分率愈大,對於阱層220之膜厚之變化而言之發光波長之變化程度則愈大。又,如圖9,Ga富化阱領域220a之AlN莫耳分率為50%時,於阱層220之膜厚及阻障層221之AlN莫耳分率之上述範圍內,可知發光波長在概略246nm~295nm之範圍變化。如圖10,Ga富化阱領域220a之AlN莫耳分率為41.7%時,於阱層220之膜厚及阻障層221之AlN莫耳分率之上述範圍內,可知發光波長在概略249nm~311nm之範圍變化。如圖11,Ga富化阱領域220a之AlN莫耳分率為33.3%時,於阱層220之膜厚及阻障層221之AlN莫耳分率之上述範圍內,可知發光波長在概略261nm~328nm之範圍變化。更且,將阻障層221以AlN(AlN莫耳分率=100%)構成時,可將發光波長更加擴張。From FIGS. 9 to 11 , it can be seen that when the film thickness of the
經由圖9~圖11,於阱層220之Ga富化阱領域220a,形成AlGaN組成比為Al
1Ga
1N
2或Al
5Ga
7N
12或Al
1Ga
2N
3之準安定阱領域,對應於該準安定阱領域之AlN莫耳分率,令阱層220之膜厚調整於3ML~14ML之範圍內,及,令阻障層221之Ga富化阻障領域221a之AlN莫耳分率調整於66.7%~100%之範圍內經由各別調整,可使尖峰發光波長,設定於246nm~328nm之範圍內。
9 to 11, in the Ga-enriched
圖12阱層為GaN,對於阻障層以AlGaN或AlN構成之量子井構造模型而言,對於阻障層之AlN莫耳分率為66.7%(AlGaN)、與100%(AlN)之2種情形,圖表化將阱層之膜厚在4ML~10ML之範圍內變化所得之發光波長之模擬結果(相當於尖峰發光波長)者。經由圖12,於該範圍內,可知發光波長在概略270nm~325nm之範圍變化。因此,阱層即使GaN(AlN莫耳分率=0%)所構成之時,令阱層220厚調整於4ML~10ML之範圍內,及,令阻障層221之Ga富化阻障領域221a之AlN莫耳分率調整於66.7%~100%之範圍內,可使尖峰發光波長,設定於270nm~325nm之範圍內。Figure 12 The well layer is GaN. For the quantum well structure model in which the barrier layer is composed of AlGaN or AlN, the molar ratio of AlN to the barrier layer is 66.7% (AlGaN) and 100% (AlN). In this case, the simulation results of the emission wavelength (equivalent to the peak emission wavelength) obtained by changing the film thickness of the well layer in the range of 4ML to 10ML are graphed. From FIG. 12 , within this range, it can be seen that the emission wavelength changes in a range of approximately 270 nm to 325 nm. Therefore, even when the well layer is composed of GaN (AlN molar ratio = 0%), the thickness of the
經由圖12,尖峰發光波長之目標值在270nm~325nm之範圍內時,作為形成於阱層220之Ga富化阱領域220a之準安定阱領域之AlGaN組成比,除了圖9~圖11所示Al
1Ga
1N
2、Al
5Ga
7N
12、及、Al
1Ga
2N
3以外,可選擇Al
1Ga
3N
4(AlN莫耳分率為25%(4分之1))、或、Al
1Ga
5N
6(AlN莫耳分率為16.7%(6分之1))。此時,令準安定阱領域之AlN莫耳分率從33.3%以8.33%(12分之1)程度下降之故,阻障層221之AlN莫耳分率,亦在適合於尖峰發光波長之目標值之範圍內,可設定較66.7%為低,例如可設定於58.3%或50%。
Through FIG. 12 , when the target value of the peak emission wavelength is in the range of 270 nm to 325 nm, as the composition ratio of AlGaN in the quasi-stable well region formed in the Ga-enriched
更且,如圖9~圖11,準安定阱領域之AlGaN組成比,除了為Al
1Ga
1N
2、Al
5Ga
7N
12、及、Al
1Ga
2N
3以外,成為Al
7Ga
5N
12之時,對應AlN莫耳分率僅高約8.33%,尖峰發光波長則短長波長化。因此,尖峰發光波長之目標值例如較250nm為短之時,作為形成於Ga富化阱領域220a之準安定阱領域之AlGaN組成比,亦可設定為Al
7Ga
5N
12(AlN莫耳分率為58.3%(7分之12))。
Furthermore, as shown in FIGS. 9 to 11 , the composition ratio of AlGaN in the quasi-stable well region is Al 7 Ga 5 except for Al 1 Ga 1 N 2 , Al 5 Ga 7 N 12 , and Al 1 Ga 2 N 3 . At N 12 , the corresponding AlN molar ratio is only about 8.33% higher, and the peak emission wavelength is shortened to a longer wavelength. Therefore, when the target value of the peak emission wavelength is, for example, shorter than 250 nm, the composition ratio of AlGaN in the quasi-stable well region formed in the Ga-
又,阱層220以AlGaN系半導體所構成,AlN莫耳分率不為0%之時,阱層220之平均性AlN莫耳分率Xwa係作為一例,於Ga富化阱領域220a形成AlN莫耳分率Xw0之準安定阱領域之時,概略調整於Xw0+2%~Xw0+3%之範圍為佳。經由該較佳實施形態,阱層220之準安定阱領域與平台領域TA之AlN莫耳分率差係成為可抑制起因於傾斜領域IA與平台領域TA之AlN莫耳分率差之雙發光尖峰之產生之4%以下。然而,阱層220之平台領域之AlN莫耳分率Xwa係即使超出Xw0+2%~Xw0+3%之範圍外,只僅於阱層220之傾斜領域IA內,形成局部性AlN莫耳分率低之Ga富化阱領域220a時,可令對應於尖峰發光波長之目標值之該Ga富化阱領域220a內之AlN莫耳分率為Xw1%,設定在Xw1+2%~Xw1+3%之範圍內之任意值。In addition, the
阱層220之平均性AlN莫耳分率Xwa係如後述,於阱層220之成膜時,作為AlN莫耳分率之目標值加以使用。The average AlN molar ratio Xwa of the
n型包覆層21之層狀領域21a之AlN莫耳分率係較阱層220之Ga富化阱領域220a之AlN莫耳分率,設定成8.3%以上,較佳為16%以上,設定在高水準。The AlN molar ratio of the layered
作為較佳一實施形態,於阱層220之Ga富化阱領域220a內,支配存在AlGaN組成比為整數比之Al
kGa
12-kN
12(k=3~7)之準安定阱領域,於n型包覆層21內之層狀領域21a內,支配存在AlGaN組成比成為整數比之Al
nGa
12-nN
12(n=5~8)之第1準安定n型領域之時,準安定阱領域之AlGaN組成比與第1準安定n型領域之AlGaN組成比之間之可能組合係成為n≧k+1之組合中,成為可滿足上述條件(層狀領域21a與Ga富化阱領域220a之AlN莫耳分率差為8.3%以上)之組合。因此,上述較佳之一實施形態中,整數k與整數n之可能組合係成為(k=3~4:n=5~8)、(k=5:n=6~8)、(k=6:n=7~8)、(k=7:n=8)。
As a preferred embodiment, in the Ga-enriched
阻障層221之Ga富化阻障領域221a之AlN莫耳分率係如上所述,對應於發光元件1之尖峰發光波長之目標值,伴隨阱層220之Ga富化阱領域220a之AlN莫耳分率及阱層220之膜厚,例如調整在50%~100%之範圍內。更且,作為較佳之實施形態,阻障層221以AlGaN系半導體(排除AlN系半導體)所構成之時,於阻障層221之Ga富化阻障領域221a,形成AlGaN組成比為整數比之Al
jGa
12-jN
12之準安定AlGaN所成準安定阻障領域。惟,整數j係6、7、8、9或10,對應尖峰發光波長之目標值加以決定。即,存在於Ga富化阻障領域221a內之準安定阻障領域係Al
1Ga
1N
2、Al
7Ga
5N
12、Al
2Ga
1N
3、Al
3Ga
1N
4、Al
5Ga
1N
6之5種類,AlN莫耳分率係各別為50%(2分之1)、58.3%(12分之7)、66.7%(3分之2)、75%(4分之3)、83.3%(6分之5)。
The AlN molar ratio of the Ga-enriched
又,阻障層221以AlGaN系半導體(排除AlN系半導體)所構成之時,阻障層221之平台領域TA之AlN莫耳分率係大概在51%~90%之範圍內,較Ga富化阻障領域221a之AlN莫耳分率,設定成1%以上,較佳為2%以上,更佳為4%以上,設定在高水準。為了充分確保Ga富化阻障領域221a之載子之局部存在化効果,雖令阻障層221內之Ga富化阻障領域221a與平台領域TA之AlN莫耳分率差成為4~5%以上為佳、但1~2%程度下,以可期待載子之局部存在化效果。In addition, when the
於阻障層221之Ga富化阻障領域221a內,形成上述AlGaN組成比(Al
jGa
12-jN
12,j=6~10),AlN莫耳分率為Xb0(=j/12)之準安定阻障領域之時,阻障層221之平均性AlN莫耳分率Xba係調整在成為(j+0.24)/12≦Xba<(j+1)/12之範圍內為佳。阻障層221之平台領域TA之平均性AlN莫耳分率(未形成Al富化阻障領域之時,排除Al富化阻障領域)係與阻障層221之平均性AlN莫耳分率Xba略同。因此,作為阻障層221之Ga富化阻障領域221a與平台領域TA之AlN莫耳分率差,可確保在約2%以上。更佳係經由AlN莫耳分率Xba之上述調整範圍之上限之(j+1)/12下降至(j+0.9)/12,更安定於Ga富化阻障領域221a形成AlGaN組成比為Al
jGa
12-jN
12之準安定阻障領域。
In the Ga-enriched
更且,阻障層221之平均性AlN莫耳分率Xba係調整成為(j+0.5)/12<Xba<(j+1)/12之第1之適切範圍內,更佳為調整成為(j+0.5)/12<Xba≦(j+0.9)/12之第2之適切範圍內為佳。由此,於Ga富化阻障領域221a內,抑制形成較AlN莫耳分率為Xb0(=j/12)之準安定阻障領域AlN莫耳分率為低之非準安定AlGaN,更安定確保傾斜領域IA之阱層220與阻障層221間之特定AlN莫耳分率差。Furthermore, the average AlN molar fraction Xba of the
然而,阻障層221之平均性AlN莫耳分率Xba係即使超出成為(j+0.24)/12≦Xba<(j+1)/12範圍,只要於阻障層221之傾斜領域IA內形成可載子之局部存在化之Ga富化阻障領域221a,在大概51%~90%之範圍內,可取得對應於阱層220之Ga富化阱領域220a內之AlN莫耳分率之任意值。However, even if the average AlN molar fraction Xba of the
作為上述較佳之一實施形態,經由將Ga富化阻障領域221a以安定度高之準安定阱領域構成,伴隨將n型包覆層21內之Ga富化n型領域與Al富化n型領域各別以安定度高之第1及第2準安定n型領域構成所成效果,起因於結晶成長裝置之漂移等之混晶莫耳分率之變動在阻障層221內亦被抑制,於阻障層221內,產生載子之局部存在化之Ga富化阻障領域221a,則以對應於使用之準安定阻障領域之AlN莫耳分率安定地加以形成。此結果,於阻障層221內,電流係優先安定流入Ga富化阻障領域,更可達成發光元件1之特性變動之抑制。As a preferred embodiment of the above, the Ga-enriched
電子阻障層23之平台領域TA之AlN莫耳分率係大概在69%~90%之範圍內,較阱層220之AlN莫耳分率,設定成20%以上,較佳為25%以上,更佳為30%以上,設定在高水準。更且,電子阻障層23之Ga富化EB領域23a之AlN莫耳分率係較阱層220之Ga富化阱領域220a之AlN莫耳分率,設定成20%以上,較佳為25%以上,更佳為30%以上,設定在高水準。The molar ratio of AlN in the platform area TA of the
作為較佳一實施形態,於阱層220之Ga富化阱領域220a內,對應尖峰發光波長之目標值,與支配存在AlGaN組成比為整數比之Al
kGa
12-kN
12(k=3~7)之準安定阱領域相同,於電子阻障層23之Ga富化EB領域23a內,支配存在AlN莫耳分率較準安定阱領域之AlN莫耳分率高20%以上,AlGaN組成比成為整數比之Al
mGa
12-mN
12之p型之準安定AlGaN所構成之第1準安定EB領域。惟,整數m為8、9或10。即,存在於Ga富化EB領域23a內之第1準安定EB領域係Al
2Ga
1N
3、Al
3Ga
1N
4、Al
5Ga
1N
6之3種類,AlN莫耳分率係各別為66.7%(3分之2)、75%(4分之3)、83.3%(6分之5)。
As a preferred embodiment, in the Ga-enriched
此時,準安定阱領域之AlGaN組成比(Al
kGa
12-kN
12,k=3~7)與第1準安定EB領域之AlGaN組成比(Al
mGa
12-mN
12,m=8~10)之間之組合係於成為m>k+2之組合中,成為滿足上述條件(Ga富化EB領域23a與Ga富化阱領域220a之AlN莫耳分率差為20%以上)之組合。因此,上述較佳之一實施形態中,整數k與整數m之可能組合之內,(k=6,m=8)、(k=7,m=9)、及び(k=7,m=8)係未滿足上述條件而排除。
At this time, the composition ratio of AlGaN in the quasi-stable well region (Al k Ga 12-k N 12 , k=3~7) and the composition ratio of AlGaN in the first quasi-stable EB region (Al m Ga 12-m N 12 , m= The combination between 8 and 10) is in the combination of m>k+2, which satisfies the above conditions (the difference in AlN molar ratio between the Ga-enriched
電子阻障層23之平台領域TA之AlN莫耳分率係大概在69%~90%之範圍內,較Ga富化EB領域23a之AlN莫耳分率,設定成1%以上,較佳為2%以上,更佳為4%以上,設定在高水準。為了充分確保Ga富化EB領域23a之載子之局部存在化効果,雖令電子阻障層23內之Ga富化EB領域23a與平台領域TA之AlN莫耳分率差成為4~5%以上為佳、但1~2%程度下,以可期待載子之局部存在化效果。The molar ratio of AlN in the platform area TA of the
作為較佳之一實施形態,於電子阻障層23之Ga富化EB領域23a內,形成上述AlGaN組成比(Al
mGa
12-mN
12,m=8~10),AlN莫耳分率為Xe0(=m/12)之第1準安定EB領域之時,電子阻障層23之平均性AlN莫耳分率Xea係調整在成為(m+0.24)/12≦Xea<(m+1)/12之範圍內為佳。電子阻障層23之平台領域TA之平均性AlN莫耳分率(形成Al富化EB領域之時,排除Al富化EB領域)係與電子阻障層23之平均性AlN莫耳分率Xea略同。由此,作為電子阻障層23之Ga富化EB領域23a與平台領域TA之AlN莫耳分率差,可確保在約2%以上。更佳係經由AlN莫耳分率Xea之上述調整範圍之上限之(m+1)/12下降至(m+0.9)/12,更安定於Ga富化EB領域23a內,形成AlGaN組成比為Al
mGa
12-mN
12之第1準安定EB領域。
As a preferred embodiment, the above-mentioned AlGaN composition ratio (AlmGa12 -mN12 , m =8~10) is formed in the Ga-enriched
然而,電子阻障層23之平均性AlN莫耳分率Xea係即使超出成為(m+0.24)/12≦Xea<(m+1)/12範圍,只要於電子阻障層23之傾斜領域IA內形成可載子之局部存在化之Ga富化EB領域23a,在大概69%~90%之範圍內,可取得對應於阱層220之Ga富化阱領域220a內之AlN莫耳分率之任意值。However, even if the average AlN molar fraction Xea of the
作為上述較佳之一實施形態,經由將Ga富化EB領域23a以安定度高之第1準安定EB領域構成,伴隨將n型包覆層21內之Ga富化n型領域與Al富化n型領域各別以安定度高之第1及第2準安定n型領域加以構成所成效果,起因於結晶成長裝置之漂移等之混晶莫耳分率之變動在電子阻障層23內亦被抑制,於電子阻障層23內,產生載子之局部存在化之Ga富化EB領域23a,則以對應於使用之第1準安定EB領域之AlN莫耳分率安定地加以形成。此結果,於電子阻障層23內,電流係優先安定流入Ga富化EB領域23a,更可達成發光元件1之特性變動之抑制。As a preferred embodiment of the above, the Ga-enriched
p電極26係例如以Ni/Au等之多層金屬膜所構成,形成於p型連接層24之上面。n電極27係例如以Ti/Al/Ti/Au等之多層金屬膜所構成,形成於n型包覆層21之第2領域R2內之露出面上之一部分之領域。然而,p電極26及n電極27係非限定於上述之多層金屬膜,構成各電極之金屬、層積數、層積順序等之電極構造係可適當變更。於圖13,顯示從p電極26與n電極27之發光元件1之上側所視之形狀之一例。於圖13中,存在於p電極26與n電極27之間之線BL係顯示第1領域R1與第2領域R2之邊界線,與活性層22、電子阻障層23、及、p型連接層24之外周側壁面一致。The p-
本實施形態中,如圖13所示,第1領域R1及p電極26之平面所視形狀係作為一例,雖採用梳形形狀者,第1領域R1及p電極26之平面所視形狀及配置等係非限定於圖13之例示。In the present embodiment, as shown in FIG. 13 , the shapes of the first region R1 and the p-
於p電極26與n電極27間,施加順方向偏壓時,從p電極26朝向活性層22供給電洞,從n電極27朝向活性層22供給電子,供給之各個電洞及電子則到達活性層22再結合而發光。又,由此,於p電極26與n電極27間,流動順方向電流。When a forward bias is applied between the
<發光元件之製造方法>
接著,說明對於圖6所例示之發光裝置1之製造方法之一例。
<Manufacturing method of light-emitting element>
Next, an example of a method of manufacturing the light-emitting
首先,經由有機金屬化合物氣相成長(MOVPE)法,將含於基材部10之AlN層12及含於發光元件構造部20之氮化物半導體層21~24於藍寶石基板11上,順序磊晶成長而層積。此時,於n型包覆層21中,作為供體不純物,例如摻雜Si,於電子阻障層23、及、p型連接層24作為受體不純物,例如摻雜Mg。First, the
本實施形態中,至少於AlN層12、n型包覆層21及活性層22(阱層220、阻障層221)、及電子阻障層23之各表面,為表現出平行於(0001)面之多段狀之平台,藍寶石基板11係主面11a對於(0001)面以一定之範圍內(例如0度至6度程度)之角度(偏角)傾斜,於主面11a上使用表現出多段狀之平台之微傾斜基板。In this embodiment, at least the surfaces of the
作為相關磊晶成長之條件,除了上述之微傾斜基板之(0001)藍寶石基板11之使用,例如可列舉例如易於表現出多段狀之平台之成長速度(具體而言,例如經由適切設定成長溫度、原料氣體或載流氣體之供給量或流速等之諸條件,達成該成長速度)等。然而,此等之諸條件係經由成膜裝置之種類或構造而不同獲得之故,於成膜裝置,實際製作幾個試料,特定此等之條件即可。As the conditions for the related epitaxial growth, in addition to the use of the (0001)
作為n型包覆層21之成長條件,於成長開始之後,在形成於AlN層12之上面之多段狀之平台間之階差部(傾斜領域),經由Ga之質量移動,形成層狀領域21a之成長開始點,接著,伴隨n型包覆層21之磊晶成長,層狀領域21a則伴隨Ga之質量移動,可以經由偏析朝向斜上方成長之方式,選擇成長溫度、成長壓力、及、供體不純物濃度。As a growth condition of the n-
具體而言,作為成長溫度,在Ga之質量移動易於產生之1050℃以上,可調製良好n型AlGaN之1150℃以下為佳。又,成長溫度超過1170℃之成長溫度時,Ga之質量移動會過剩,即使第1之準安定AlGaN,AlN莫耳分率易於隨機變動之故,難以安定形成AlN莫耳分率為41.7%~75%之n型之準安定AlGaN之第1及第2之準安定n型領域之故,並不喜好。作為成長壓力,75Torr以下作為良好之AlGaN之成長條件為佳,作為成膜裝置之控制界限,現實上10Torr以上為佳。供體不純物濃度係1×10 18~5×10 18cm -3程度為佳。然而,上述成長溫度及成長壓力等係一例而已,對應於使用之成膜裝置特定適切最佳之條件即可。 Specifically, the growth temperature is preferably 1050°C or higher, where mass shift of Ga is likely to occur, and 1150°C or lower, where n-type AlGaN can be well prepared. In addition, when the growth temperature exceeds the growth temperature of 1170°C, the mass transfer of Ga will be excessive. Even if the first quasi-stable AlGaN, the AlN molar rate is easy to fluctuate randomly, so it is difficult to stably form AlN with a molar rate of 41.7%~ 75% of the n-type quasi-stable AlGaN is the first and second quasi-stable n-type field, so I don't like it. As a growth pressure, 75 Torr or less is preferable as a good growth condition for AlGaN, and as a control limit of a film-forming apparatus, 10 Torr or more is actually preferable. The concentration of impurities in the donor is preferably about 1×10 18 to 5×10 18 cm -3 . However, the above-mentioned growth temperature, growth pressure, etc. are only examples, and the conditions may be suitable and optimal according to the specific film-forming apparatus to be used.
有機金屬化合物氣相成長法所使用之原料氣體(三甲基鋁(TMA)氣體、三甲基鎵(TMG)氣體、氨氣)或載流氣體之供給量及流速係將n型包覆層21之平均之AlN莫耳分率Xna作為目標值加以設定。The supply amount and flow rate of the raw material gas (trimethylaluminum (TMA) gas, trimethylgallium (TMG) gas, ammonia gas) or carrier gas used in the organometallic compound vapor phase growth The average AlN molar ratio Xna of 21 was set as a target value.
n型包覆層21之平均性AlN莫耳分率Xna係存在於Ga富化n型領域內之第1準安定n型領域之AlGaN組成比為整數比之Al
nGa
12-nN
12(n=5~8)之時,設定在(n+0.5)/12<Xna<(n+1)/12之第1之適切範圍內,更佳為設定在(n+0.5)/12<Xna≦(n+0.9)/12之第2之適切範圍內。
The average AlN molar fraction Xna of the n-
本實施形態中,為得到上述適切之Ga之質量移動之成長條件,係對應於上述第1或第2之適切範圍內之AlN莫耳分率Xna,於Ga富化n型領域內,安定形成AlGaN組成比成為整數比之Al nGa 12-nN 12之第1準安定n型領域,於Al富化n型領域內,安定形成AlGaN組成比成為整數比之Al n+1Ga 11-nN 12之第2準安定n型領域而加以調整。然而,AlN莫耳分率Xna在上述第2之適切範圍內時,於Ga富化n型領域及Al富化n型領域內,更易於安定形成上述AlGaN組成比之第1及第2準安定n型領域。 In this embodiment, in order to obtain the above-mentioned suitable growth conditions for mass transfer of Ga, the AlN molar ratio Xna within the above-mentioned first or second suitable range is stably formed in the Ga-enriched n-type region. The AlGaN composition ratio becomes the first quasi-stable n -type region of AlnGa12 -nN12 in the integer ratio, and in the Al-rich n -type region, the AlGaN composition ratio becomes the integer ratio of Aln + 1Ga11 -n . Adjusted for the second quasi-stable n-type region of N12. However, when the AlN molar fraction Xna is within the above-mentioned second appropriate range, in the Ga-enriched n-type region and the Al-enriched n-type region, the first and second quasi-stable AlGaN composition ratios can more easily be formed stably. n-type field.
於層狀領域21a內,安定存在AlGaN組成比為整數比之Al
nGa
12-nN
12(n=5~8)之第1準安定n型領域,第1準安定n型領域之AlN莫耳分率(n/12)與n型本體領域21b之平均之AlN莫耳分率(≒Xna)之差係如上所述,安定確保在約1/24(約4.17%)以上之故,n型包覆層21內之載子係局部存在化於較n型本體領域21b能帶隙能量小之層狀領域21a內。
In the
然而,供體不純物濃度係對於n型包覆層21之膜厚,無需一定均勻控制於上下方向。例如,n型包覆層21內之特定之薄膜厚部分之不純物濃度則較上述設定濃度為低,例如可為控制於不足1×10
18cm
-3,更較為1×10
17cm
-3以下之低不純物濃度層。作為該低不純物濃度層之膜厚,較0nm為大200nm以下程度為佳,10nm以上100nm以下程度則更佳,更甚者為20nm以上50nm以下程度。又,該低不純物濃度層之供體不純物濃度係較上述設定濃度低即可,未摻雜層(0cm
-3)亦可含於一部分。更且,該低不純物濃度層之一部分或全部係存在於從n型包覆層21之上面向下方側100nm以內之深度之上層域為佳。
However, the concentration of the donor impurity depends on the thickness of the n-
就上述要領中,形成具有層狀領域21a與n型本體領域21b之n型包覆層21時,於n型包覆層21之上面全面,接著,經由有機金屬化合物氣相成長(MOVPE)法等之公知之磊晶成長法,形成活性層22(阱層220、阻障層221)、電子阻障層23、及p型連接層24等。In the above-mentioned method, when forming the n-
電子阻障層23之受體不純物濃度係作為一例,1.0×10
16~1.0×10
18cm
-3程度為佳,p型連接層24之受體不純物濃度係作為一例,1.0×10
18~1.0×10
20cm
-3程度為佳。然而,受體不純物濃度係對於電子阻障層23及p型連接層24之各膜厚而言,無需一定均勻控制於上下方向。
The acceptor impurity concentration of the
活性層22形成中,以與n型包覆層21同樣之要領,在易於表現出上述之多段狀之平台的成長條件下,將阱層220之平均性AlN莫耳分率Xwa作為目標值,成長阱層220,更且,將阻障層221之平均性AlN莫耳分率Xba作為目標值,成長阻障層221。In the formation of the
阱層220之平均性AlN莫耳分率Xwa係於Ga富化阱領域220a形成AlN莫耳分率Xw0之準安定阱領域之時,概略設定成Xw0+2%~Xw0+3%之範圍內。The average AlN mole fraction Xwa of the
更且,阻障層221之平均性AlN莫耳分率Xba係於Ga富化阻障領域221a內形成AlN莫耳分率Xb0之準安定阻障領域之時,設定在Xb0+2%≦Xba<Xb0+8.33%之範圍內。Furthermore, the average AlN mol fraction Xba of the
於電子阻障層23之形成中,以與n型包覆層21同樣之要領,在易於表現出上述之多段狀之平台的成長條件下,將電子阻障層23之平均之AlN莫耳分率Xea作為目標值,成長電子阻障層23。In the formation of the
電子阻障層23之平均性AlN莫耳分率Xea係於電子阻障層23之Ga富化EB領域23a內,形成AlN莫耳分率Xe0之第1準安定EB領域之時,設定在Xe0+2%≦Xea< Xe0+8.33%之範圍內。The average AlN mole fraction Xea of the
本實施形態中,活性層22(阱層220、阻障層221)、電子阻障層23、及、p型連接層之長溫度係令n型包覆層21之成長溫度為T1,令活性層22之成長溫度為T2,令電子阻障層23之成長溫度為T3,令p型連接層之成長溫度為T4之時,於些述較佳溫度範圍內(1050℃~1170℃),滿足以下式(1)及(2)所示關係為佳。
T3≧T2 (1)
T3>T1>T4 (2)
In this embodiment, the long temperature of the active layer 22 (the
更且,上述式(1)之關係係電子阻障層23之第1Ga富化領域23a內之第1準安定EB領域之AlN莫耳分率為83.3%或75%之時,成為下述式(1A)為佳,第1準安定EB領域之AlN莫耳分率為66.7%之時,成為下述式(1B)為佳。此係第1準安定EB領域之AlN莫耳分率變高時,為促進Ga之質量移動,需更高溫之成長溫度之緣故。
T3≧T2+50℃ (1A)
T2+50℃>T3≧T2 (1B)
Furthermore, the relationship of the above formula (1) is the following formula when the AlN molar ratio of the first quasi-stable EB region in the first Ga-enriched
更且,電子阻障層23之成長溫度T3係第1準安定EB領域之AlN莫耳分率為83.3%時,1150℃以上為佳,第1準安定EB領域之AlN莫耳分率為75%或66.7%之時,1100℃以上為佳,更且較1100℃之高溫則更佳。然而,上述各溫度僅為一例而已,例如增加氮原料氣體之流量。使成長速度下降,可使上述1150℃及1100℃,各別減低至1100℃及1050℃。Furthermore, when the growth temperature T3 of the
然而,將電子阻障層23之成長溫度T3從活性層22之成長溫度T2上昇之時,於該成長溫度之遷移過程中,在該下方之位置之阱層220內,產生GaN之分解,起因於該GaN之分解,有惡化發光元件1之特性之可能性。因此,為抑制該GaN之分解,於最上層之阱層220與電子阻障層23之間,為了防止上述GaN之分解,以較阻障層221為薄之膜(例如3nm以下,較佳為2nm以下),形成較阻障層221及電子阻障層23,AlN莫耳分率高之AlGaN層或AlN層為佳。However, when the growth temperature T3 of the
作為為促進電子阻障層23之Ga之質量移動之成長溫度以外之成長條件之一例,成長溫度T3為1150℃之時,令原料氣體之流量比(V/III)為5000~6000,令成長速度成為約150nm/h為佳。As an example of growth conditions other than the growth temperature for promoting the mass transfer of Ga in the
將滿足n型包覆層21、活性層22(阱層220、阻障層221)、電子阻障層23、及、p型連接層之成長溫度T1~T4之上述式(1A)及(2)之一例,示於如下。
T1=T2=1080℃、T3=1150℃、T4=980℃
The above formulas (1A) and (2) will satisfy the growth temperatures T1 to T4 of the n-
上述成長溫度T1~T4之一例係可對於以下所示n型包覆層21之層狀領域21a內之第1準安定n型領域之AlN莫耳分率Xn0、阱層220之Ga富化阱領域220a內之準安定阱領域之AlN莫耳分率Xw0、阻障層221之Ga富化阻障領域221a內之準安定阻障領域之AlN莫耳分率Xb0、及、電子阻障層23之Ga富化EB領域23a內之第1準安定EB領域之AlN莫耳分率Xe0加以適用。
Xn0=41.7%、50%、58.3%、66.7%
Xw0=0%、25%、33.3%、41.7%、50%、58.3%
Xb0=50%、58.3%、66.7%、75%、83.3%
Xe0=66.7%、75%、83.3%
One example of the above-mentioned growth temperatures T1 to T4 is that the AlN molar fraction Xn0 in the first quasi-stable n-type region in the layered
就上述要領中,於n型包覆層21之上面之全面,形成活性層22(阱層220、阻障層221)、電子阻障層23、及p型連接層24等時,接著,經由反應性離子蝕刻等之周知之蝕刻法,將氮化物半導體層21~24之第2領域R2,選擇性蝕刻至露出n型包覆層21之上面,露出n型包覆層21之上面之第2領域R2部分。然後,經由電子束蒸鍍法等之公知之成膜法,於未蝕刻之第1領域R1內之p型連接層24上,形成p電極26的同時,於蝕刻之第1領域R2內之n型包覆層21上,形成n電極27。然而,於p電極26及n電極27之一方或雙方之形成後,經由RTA(瞬間熱退火)等之公知之熱處理方法,進行熱處理亦可。In the above method, when the active layer 22 (the
然而,發光元件1係作為一例,於副固定座等之基台,覆晶安裝之後,在經由聚矽氧樹脂或非晶質氟樹脂等之特定之樹脂(例如透鏡形狀之樹脂)所封閉之狀態下加以使用。However, the light-emitting
以上述要領所製作之發光元件1之AlGaN系半導體層21~24之剖面構造係製作p第2領域R2之蝕刻及電極26與n電極27之形成前之試料,將具有垂直(或略垂直)於該資料之上面之剖面之試料片,以聚焦離子束(FIB)加工,經由該試料片之HAADF-STEM像進行觀察。The cross-sectional structure of the AlGaN-based semiconductor layers 21 to 24 of the light-emitting
更且,AlGaN系半導體層21~24中之特定之半導體層內之組成分析,係可使用上述試料片,以能量分散型X線分光法(剖面TEM-EDX)或CL(陰極射線發光)法進行。對於剖面TEM-EDX所成之組成分析,雖省略說明,本案發明人之先行申請(PCT/JP2020/023050、PCT/JP2020/024828、PCT/JP2020/026558、PCT/JP2020/031620)之說明書中,有詳細之說明。Furthermore, the composition analysis in a specific semiconductor layer among the AlGaN-based semiconductor layers 21 to 24 can be performed by energy dispersive X-ray spectroscopy (cross-sectional TEM-EDX) or CL (cathode ray luminescence) method using the above-mentioned sample pieces. conduct. Although the description of the composition analysis by the cross-section TEM-EDX is omitted, in the descriptions of the prior applications (PCT/JP2020/023050, PCT/JP2020/024828, PCT/JP2020/026558, PCT/JP2020/031620) of the present inventor, There are detailed instructions.
<n型包覆層之組成分析結果>
接著,說明將n型包覆層21內之層狀領域21a與n型本體領域21b之AlN莫耳分率之測定,以CL(陰極射線發光)法加以進行之結果。
<Results of composition analysis of n-type cladding layer>
Next, the results of measuring the AlN molar fraction in the layered
為n型包覆層21之組成分析用製作2種類之試料,將具有從各試料垂直(或略垂直)於n型包覆層21之上面之剖面之試料片,以聚焦離子束(FIB)加工,製作測定用之2個之試料片A及B。For the composition analysis of the n-
試料片A之試料係根據上述之n型包覆層21等之製作要領,於從上述之藍寶石基板11與AlN層12所成基材部10上,順序堆積n型包覆層21、和較n型包覆層21為高AlN莫耳分率之AlGaN層、和試料表面保護用之AlGaN層、和保護用樹脂膜加以製作。然而,於該試料之製作中,使用主面對於(0001)面具有偏角之藍寶石基板11,於AlN層12之表面,使用表現出多段狀之平台之基材部10。然而,該試料之製作中,n型包覆層21之膜厚係成為3.1μm,令n型包覆層21之平均性AlN莫耳分率Xna(目標值)為63%。AlN莫耳分率Xna之RBS分析法所成測定值亦為63%。更且,又,使供體不純物濃度約成為3×10
18cm
-3,控制供體不純物(Si)之注入量。
The sample of the sample piece A is formed by sequentially depositing the n-
試料片B之試料係根據上述之n型包覆層21等之製作要領,於從上述之藍寶石基板11與AlN層12所成基材部10上,順序堆積n型包覆層21、和活性層22、和較n型包覆層21為高AlN莫耳分率之AlGaN層、和試料表面保護用之AlGaN層、和保護用樹脂膜加以製作。然而,於該試料之製作中,使用主面對於(0001)面具有偏角之藍寶石基板11,於AlN層12之表面,使用表現出多段狀之平台之基材部10。然而,於該試料之製作中,n型包覆層21之膜厚係約為2.6μm,對於下側之膜厚約1μm,令n型包覆層21之平均性之AlN莫耳分率Xna(目標值)為55%,對於上側之膜厚約1.6μm,令n型包覆層21之平均性之AlN莫耳分率Xna(目標值)為43%。AlN莫耳分率Xna之RBS分析法所成測定值,下側亦為55%,上側亦為43%。更且,上側及下側,皆使供體不純物濃度約成為3×10
18cm
-3,控制供體不純物(Si)之注入量。
The sample of the sample piece B is formed by sequentially depositing the n-
圖14係顯示包含上述試料片A之測定剖面上之n型包覆層21之主要部分之掃描型電子顯微鏡(SEM)像。圖15係顯示包含上述試料片B之測定剖面上之n型包覆層21之主要部分之SEM像。FIG. 14 shows a scanning electron microscope (SEM) image of the main part of the n-
試料片A之測定範圍(測定用所照射之電子射束之入射點之範圍)係於X方向(平行於第2平面之橫方向)與Y方向(與第2平面正交之縱方向),各別為6.25μm與3.2μm,成為121網目×60網目之格子狀設定電子光束之入射點。網目間隔係X方向為約52nm,Y方向為約53nm。試料片B之測定範圍係於X方向與Y方向,各別為6.25μm與4.6μm,成為125網目與93網目之格子狀設定電子光束之入射點。網目間隔係X方向及Y方向皆為50nm。然而,圖14所示試料片A之測定剖面上之主要部分係顯示上述測定範圍(6.25μm×3.2μm)之一部分之正方領域(3.2μm×3.2μm)。又,圖15所示試料片B之測定剖面上之主要部分係顯示上述測定範圍(6.25μm×4.6μm)之一部分之正方領域(3.25μm×3.25μm)。The measurement range of the sample A (the range of the incident point of the electron beam irradiated for the measurement) is in the X direction (the horizontal direction parallel to the second plane) and the Y direction (the vertical direction perpendicular to the second plane), They are 6.25 μm and 3.2 μm, respectively, and the incident points of the electron beams are set in a grid pattern of 121 meshes×60 meshes. The mesh spacer is about 52 nm in the X direction and about 53 nm in the Y direction. The measurement range of the sample piece B was 6.25 μm and 4.6 μm in the X direction and the Y direction, respectively, and the incident points of the electron beams were set in a grid pattern of 125 meshes and 93 meshes. The mesh spacing is 50 nm in both the X direction and the Y direction. However, the main part on the measurement cross section of the sample piece A shown in FIG. 14 shows a square area (3.2 μm×3.2 μm) of a part of the above-mentioned measurement range (6.25 μm×3.2 μm). In addition, the main part on the measurement cross section of the sample piece B shown in FIG. 15 shows the square area (3.25 μm×3.25 μm) of a part of the above-mentioned measurement range (6.25 μm×4.6 μm).
記載於圖14及圖15所示試料片A與試料片B之各測定範圍中之Y值(Y座標)係表示從各測定範圍之上端計數之網目數,各圖之上端為Y=0。圖14中,Y=3與Y=58係各別相當於n型包覆層21之上端與下端。圖15中,Y=7與Y=58係各別相當於n型包覆層21之上端與下端。The Y value (Y coordinate) in each measurement range of the sample pieces A and B shown in FIGS. 14 and 15 represents the number of meshes counted from the upper end of each measurement range, and Y=0 at the upper end of each graph. In FIG. 14, Y=3 and Y=58 correspond to the upper end and the lower end of the n-
於試料片A與試料片B之各測定範圍內之格子狀之電子束之入射點,將光束徑50nm(直徑)之電子束,各照射1次,測定各入射點之CL光譜。The electron beam with a beam diameter of 50 nm (diameter) was irradiated once at the incident point of the grid-shaped electron beam in each measurement range of the sample piece A and the sample piece B, and the CL spectrum of each incident point was measured.
圖16係顯示各別試料片A之Y=7、Y=15、Y=30、Y=43、Y=56之5個Y座標中,對於掃描於X方向所得121個CL光譜,以下述要領導出之第1CL光譜(實線)與第2CL光譜(虛線)。5個Y座標之第1及第2CL光譜係於縱軸方向偏移各別之原點,在相同圖表上,可相互識別地加以表示。圖16之縱軸係顯示發光強度(任意單位),更且,一部分之Y座標(Y=30,43,56)之發光強度係成為2倍使之易於辨識。圖16之橫軸係顯示波長(nm)。Fig. 16 shows that among the five Y coordinates of Y=7, Y=15, Y=30, Y=43, and Y=56 of each sample A, for the 121 CL spectra obtained by scanning in the X direction, the following requirements are used. The 1st CL spectrum (solid line) and the 2nd CL spectrum (dashed line) are shown. The first and second CL spectra of the five Y-coordinates are shifted from their respective origins in the vertical axis direction, and are shown on the same graph so as to be recognizable from each other. The vertical axis of FIG. 16 shows the luminous intensity (arbitrary unit), and the luminous intensity of a part of the Y-coordinates (Y=30, 43, 56) is doubled for easy identification. The horizontal axis of FIG. 16 shows wavelength (nm).
示於圖16之各Y座標之第1CL光譜係從相同Y座標之CL光譜中,將發光強度之尖峰向較平均性AlN莫耳分率Xna(63%)長波長側之相同波長附近偏移之CL光譜,抽出6~7點以上,平均算出抽出之CL光譜。又,示於圖16之各Y座標之第2CL光譜係從相同Y座標之CL光譜中,將發光強度之尖峰向較平均性AlN莫耳分率Xna(63%)短波長側之相同波長附近偏移之CL光譜,抽出6~7點以上,平均算出抽出之CL光譜。The first CL spectrum of each Y-coordinate shown in FIG. 16 is a CL spectrum of the same Y-coordinate, and the peak of the luminous intensity is shifted to the vicinity of the same wavelength on the longer wavelength side than the average AlN molar ratio Xna (63%). CL spectrum, extract more than 6~7 points, and calculate the extracted CL spectrum on average. In addition, the second CL spectrum of each Y coordinate shown in FIG. 16 is from the CL spectrum of the same Y coordinate, and the peak of the luminous intensity is shifted to the vicinity of the same wavelength on the shorter wavelength side than the average AlN molar ratio Xna (63%). For the shifted CL spectrum, extract more than 6 to 7 points, and average the extracted CL spectrum.
圖17係顯示各別試料片B之下側部分之Y=42、Y=45、Y=50、Y=55之4個Y座標中,對於掃描於X方向所得125個CL光譜,以下述要領導出之第3CL光譜(實線)與第4CL光譜(虛線)。4個Y座標之第3及第4CL光譜係於縱軸方向偏移各別之原點,在相同圖表上,可相互識別地加以表示。圖17之縱軸係顯示發光強度(任意單位)。圖17之橫軸係顯示波長(nm)。Fig. 17 shows that among the four Y coordinates of Y=42, Y=45, Y=50, and Y=55 of the lower portion of each sample piece B, for 125 CL spectra obtained by scanning in the X direction, the following equations are used. The 3rd CL spectrum (solid line) and the 4th CL spectrum (dashed line) are shown. The 3rd and 4th CL spectra of the four Y-coordinates are shifted from their respective origins in the vertical axis direction, and are shown on the same graph so as to be recognizable from each other. The vertical axis of FIG. 17 shows the luminous intensity (arbitrary unit). The horizontal axis of FIG. 17 shows wavelength (nm).
示於圖17之各Y座標之第3CL光譜係從相同Y座標之CL光譜中,將發光強度之尖峰向較平均性AlN莫耳分率Xna(55%)長波長側之相同波長附近偏移之CL光譜,抽出6~7點以上,平均算出抽出之CL光譜。又,示於圖17之各Y座標之第4CL光譜係從相同Y座標之CL光譜中,將發光強度之尖峰向較平均性AlN莫耳分率Xna(55%)短波長側之相同波長附近偏移之CL光譜,抽出6~7點以上,平均算出抽出之CL光譜。The 3rd CL spectrum of each Y coordinate shown in Fig. 17 is a CL spectrum of the same Y coordinate, and the peak of the luminous intensity is shifted to the vicinity of the same wavelength on the longer wavelength side than the average AlN molar ratio Xna (55%). CL spectrum, extract more than 6~7 points, and calculate the extracted CL spectrum on average. In addition, the 4th CL spectrum of each Y coordinate shown in FIG. 17 is from the CL spectrum of the same Y coordinate, and the peak of the luminous intensity is shifted to the vicinity of the same wavelength on the shorter wavelength side than the average AlN molar ratio Xna (55%). For the shifted CL spectrum, extract more than 6 to 7 points, and average the extracted CL spectrum.
圖18係顯示各別試料片B之上側部分之Y=10、Y=15、Y=20、Y=27、Y=35之5個Y座標中,對於掃描於X方向所得125個CL光譜,以下述要領導出之第5CL光譜(實線)與第6CL光譜(虛線)。5個Y座標之第5及第6CL光譜係於縱軸方向偏移各別之原點,在相同圖表上,可相互識別地加以表示。圖18之縱軸係顯示發光強度(任意單位)。圖18之橫軸係顯示波長(nm)。18 shows that among the five Y coordinates of Y=10, Y=15, Y=20, Y=27, and Y=35 of the upper portion of each sample piece B, for 125 CL spectra obtained by scanning in the X direction, The 5th CL spectrum (solid line) and the 6th CL spectrum (dashed line) are shown below. The fifth and sixth CL spectra of the five Y-coordinates are shifted from their respective origins in the vertical axis direction, and are shown on the same graph so as to be recognizable from each other. The vertical axis of FIG. 18 shows the luminous intensity (arbitrary unit). The horizontal axis of FIG. 18 shows wavelength (nm).
示於圖18之各Y座標之第5CL光譜係從相同Y座標之CL光譜中,將發光強度之尖峰向較平均性AlN莫耳分率Xna(43%)長波長側之相同波長附近偏移之CL光譜,抽出6~7點以上,平均算出抽出之CL光譜。又,示於圖18之各Y座標之第6CL光譜係從相同Y座標之CL光譜中,將發光強度之尖峰向較平均性AlN莫耳分率Xna(43%)短波長側之相同波長附近偏移之CL光譜,抽出6~7點以上,平均算出抽出之CL光譜。The 5th CL spectrum of each Y coordinate shown in FIG. 18 is a CL spectrum of the same Y coordinate, and the peak of the luminous intensity is shifted to the vicinity of the same wavelength on the longer wavelength side than the average AlN molar ratio Xna (43%). CL spectrum, extract more than 6~7 points, and calculate the extracted CL spectrum on average. In addition, the sixth CL spectrum of each Y coordinate shown in FIG. 18 is from the CL spectrum of the same Y coordinate, and the peak of the luminous intensity is shifted to the vicinity of the same wavelength on the shorter wavelength side than the average AlN molar ratio Xna (43%). For the shifted CL spectrum, extract more than 6 to 7 points, and average the extracted CL spectrum.
電子束之射束徑為50nm(直徑),垂直於層狀領域21a之延伸方向之剖面的寬度為平均約20nm程度之故,於1個入射點之電子束之照射範圍內,存在層狀領域21a之Ga富化n型領域之時,於鄰接於層狀領域21a之n型本體領域21b之端緣部,存在Al富化n型領域。The beam diameter of the electron beam is 50 nm (diameter), and the width of the cross-section perpendicular to the extending direction of the layered
因此,偏移於較平均性AlN莫耳分率Xna長波長側之第1、第3、及第5CL光譜係於電子束之照射範圍內,存在Ga富化n型領域之CL光譜,該發光強度之尖峰係位於對應於Ga富化n型領域內之AlN莫耳分率之波長附近。更且,於束徑50nm之該照射範圍內,存在Al富化n型領域之故,於Al富化n型領域內之AlN莫耳分率之波長附近,有存在發光強度之第2之尖峰之情形。Therefore, the 1st, 3rd, and 5th CL spectra shifted to the longer wavelength side of the more average AlN molar fraction Xna are in the irradiation range of the electron beam, and there is a CL spectrum in the Ga-enriched n-type region, which emits light. The intensity peaks are located near wavelengths corresponding to the molar ratio of AlN in the Ga-rich n-type domain. Furthermore, in this irradiation range with a beam diameter of 50 nm, since there is an Al-rich n-type region, there is a second peak of luminous intensity near the wavelength of the AlN molar ratio in the Al-rich n-type region. situation.
又,偏移於較平均性AlN莫耳分率Xna短波長側之第2、第4、及第6CL光譜係於電子束之照射範圍內,不存在Ga富化n型領域,存在Al富化n型領域之CL光譜,該發光強度之尖峰係位於對應於Al富化n型領域內之AlN莫耳分率之波長附近。In addition, the second, fourth, and sixth CL spectra shifted to the shorter wavelength side of the more average AlN molar fraction Xna are within the irradiation range of the electron beam, and there is no Ga-enriched n-type region, but Al-enriched. In the CL spectrum of the n-type domain, the peak of the luminescence intensity is located near the wavelength corresponding to the molar ratio of AlN in the Al-enriched n-type domain.
試料片A之n型包覆層21之平均性AlN莫耳分率Xna(=63%)係調整於整數n為7之時之成為(n+0.5)/ 12<Xna<(n+1)/12之第1之適切範圍內,及(n+0.5)/12 <Xna≦(n+0.9)/12之第2之適切範圍內。然後,於層狀領域21a之Ga富化n型領域中,存在AlGaN組成比為Al
7Ga
5N
12之第1準安定n型領域(AlN莫耳分率係58.3%,換算成波長時為約266nm),於n型本體領域21b之Al富化n型領域,存在AlGaN組成比為Al
2Ga
1N
3之第2準安定n型領域(AlN莫耳分率係66.7%,換算成波長為約253nm)。
The average AlN molar ratio Xna (=63%) of the n-
示於圖16之5個Y座標(Y=7,15,30,43,56)之第1CL光譜之發光強度之尖峰係在約264nm~約267nm之範圍內,皆位於約266nm附近,可知於各Y座標中,於層狀領域21a之Ga富化n型領域內,存在AlGaN組成比為整數比之Al
7Ga
5N
12之第1準安定n型領域。更且。示於圖16之上述5個Y座標之第2CL光譜之發光強度之尖峰係在約252nm~約255nm之範圍內,皆位於約253nm附近,可知於各Y座標中,於n型本體領域21b之Al富化n型領域內,存在AlGaN組成比為整數比之Al
2Ga
1N
3之第2準安定n型領域。
The peaks of the luminescence intensity of the first CL spectrum of the five Y-coordinates (Y=7, 15, 30, 43, 56) shown in Fig. 16 are in the range of about 264 nm to about 267 nm, all located near 266 nm, which can be seen from In each Y coordinate, in the Ga - enriched n-type region of the
試料片B之n型包覆層21之膜厚約1μm之下側部分之平均性AlN莫耳分率Xna(=55%)係調整於整數n為6之時之成為(n+0.5)/12<Xna<(n+1)/12之第1之適切範圍內,及(n+0.5)/12<Xna≦(n+0.9)/12之第2之適切範圍內。因此,於層狀領域21a之Ga富化n型領域中,存在AlGaN組成比為Al
1Ga
1N
2之第1準安定n型領域(AlN莫耳分率係50%,換算成波長時為約279nm),於n型本體領域21b之Al富化n型領域,存在AlGaN組成比為Al
7Ga
5N
12之第2準安定n型領域(AlN莫耳分率係58.3%,換算成波長為約266nm)。
The average AlN molar fraction Xna (=55%) of the lower portion of the n-
示於圖17之4個Y座標(Y=42,45,50,55)之第3CL光譜之發光強度之尖峰係在約276nm~約279nm之範圍內,皆位於約279nm附近,可知於各Y座標中,於層狀領域21a之Ga富化n型領域內,存在AlGaN組成比為整數比之Al
1Ga
1N
2之第1準安定n型領域。更且。示於圖17之上述4個Y座標之第4CL光譜之發光強度之尖峰係在約265nm~約267nm之範圍內,皆位於約266nm附近,可知於各Y座標中,於n型本體領域21b之Al富化n型領域內,存在AlGaN組成比為整數比之Al
7Ga
5N
12之第2準安定n型領域。
The peaks of the luminescence intensity of the 3rd CL spectrum of the 4 Y coordinates (Y=42, 45, 50, 55) shown in Fig. 17 are in the range of about 276 nm to about 279 nm, and they are all located near about 279 nm. It can be seen that each Y In the coordinates, in the Ga-rich n-type region of the layered
試料片B之n型包覆層21之膜厚約1.6μm之上側部分之平均性AlN莫耳分率Xna(=43%)係未調整於整數n為5之時之成為(n+0.5)/12<Xna<(n+1)/12之第1之適切範圍內,及(n+0.5)/12<Xna≦(n+0.9)/12之第2之適切範圍內,調整於n/12<Xna<(n+0.5)/12之範圍內。為此,於層狀領域21a之Ga富化n型領域中,雖存在AlGaN組成比為Al
5Ga
7N
12之第1準安定n型領域(AlN莫耳分率係41.7%,換算成波長時為約293nm),於n型本體領域21b之Al富化n型領域,存在AlGaN組成比為Al
1Ga
1N
2之第2準安定n型領域(AlN莫耳分率係50%,換算成波長為約279nm)之可能性為低。
The average AlN molar fraction Xna (=43%) of the upper portion of the n-
示於圖18之5個Y座標(Y=10,15,20,27,35)之第5CL光譜之發光強度之尖峰係在約291nm~約293nm之範圍內,皆位於約293nm附近,可知於各Y座標中,於層狀領域21a之Ga富化n型領域內,存在AlGaN組成比為整數比之Al
5Ga
7N
12之第1準安定n型領域。更且。示於圖18之上述5個Y座標之第2CL光譜之發光強度之尖峰係在約283nm~約285nm之範圍內,於5個之所有Y座標中,位於較約279nm高波長側,於各Y座標中,於n型本體領域21b之Al富化n型領域內,不支配存在AlGaN組成比為整數比之Al
1Ga
1N
2之第2準安定n型領域。此係相當模示性顯示圖7之右側部分之情形。
The peaks of the luminescence intensity of the 5th CL spectrum of the five Y-coordinates (Y=10, 15, 20, 27, 35) shown in Fig. 18 are in the range of about 291 nm to about 293 nm, and they are all located near 293 nm, which can be seen from In each Y coordinate, in the Ga - enriched n-type region of the
如以上所述,試料片A(整數n=7、Xna=63%)及試料片B之下側部分(整數n=6、Xna=55%)係皆調整於平均性AlN莫耳分率Xna成為(n+0.5)/12<Xna<(n+1)/12之第1之適切範圍內,及成為(n+0.5)/12<Xna≦(n+0.9)/12之第2之適切範圍內,於層狀領域21a之Ga富化n型領域與n型本體領域21b之Al富化n型領域內,存在AlGaN組成比成為整數比之Al
nGa
12-nN
12與Al
n+1Ga
11-nN
12之第1及第2準安定n型領域,而具備第1實施形態之發光元件1之元件構造。
As described above, both the sample piece A (integer n=7, Xna=63%) and the lower part of the sample piece B (integer n=6, Xna=55%) are adjusted to the average AlN molar ratio Xna It is within the first suitable range of (n+0.5)/12<Xna<(n+1)/12, and the second suitable range of (n+0.5)/12<Xna≦(n+0.9)/12 Within the range, in the Ga - enriched n -type region of the
另一方面,試料片B之上側部分(整數n=5、Xna=43%)係未調整於平均性AlN莫耳分率Xna成為(n+0.5)/12<Xna<(n+1)/12之第1之適切範圍內,及成為(n+0.5)/12<Xna≦(n+0.9)/12之第2之適切範圍內,其結果,在於n型本體領域21b之Al富化n型領域內,不支配存在AlGaN組成比為整數比之Al
n+1Ga
11-nN
12之第2準安定n型領域之部分,與第1實施形態之發光元件1之元件構造不同。
On the other hand, the upper portion of the sample piece B (integer n=5, Xna=43%) was not adjusted to the average AlN molar ratio Xna so that (n+0.5)/12<Xna<(n+1)/ Within the first appropriate range of 12, and within the second appropriate range of (n+0.5)/12<Xna≦(n+0.9)/12, the result is that the Al in the n-
[第2實施形態]
第1實施形態之發光元件1中,作為較佳一實施形態,說明於電子阻障層23之Ga富化EB領域23a內,支配存在AlN莫耳分率較準安定阱領域之AlN莫耳分率高20%以上,AlGaN組成比為整數比之Al
mGa
12-mN
12(m=8~10)之p型之準安定AlGaN所成第1準安定EB領域,電子阻障層23之平均性之AlN莫耳分率Xea係調整於成為(m+0.24)/12≦Xea< (m+1)/12之範圍內之情形。更且,作為較佳實施形態,說明於電子阻障層23中,於鄰接於傾斜領域IA之平台領域TA之端緣部,令電子阻障層23之平均性AlN莫耳分率Xea作為基準,形成局部性AlN莫耳分率為高之Al富化EB領域之情形。
[Second Embodiment] In the light-emitting
第2實施形態之發光元件1中,作為較佳一實施形態,說明於電子阻障層23之Ga富化EB領域23a內,支配存在AlN莫耳分率較準安定阱領域之AlN莫耳分率高20%以上,AlGaN組成比為整數比之Al
mGa
12-mN
12之p型之準安定AlGaN所成第1準安定EB領域的同時,於電子阻障層23之Al富化EB領域內,支配存在AlGaN組成比為整數比之Al
m+1Ga
11-mN
12之p型之準安定AlGaN所成第2準安定EB領域。此時,電子阻障層23之平均性之AlN莫耳分率Xea之調整範圍係較上述第1實施形態所說明之範圍為窄,AlN莫耳分率Xea係調整成為(m+0.5)/12<Xea<(m+1)/12之第1之適切範圍內,更佳為調整成為(m+0.5)/12<Xea≦ (m+0.9)/12之第2之適切範圍內。惟,整數m為8或9。
In the light-emitting
因此、第2實施形態中,於發光裝置1之製造方法中,以第1實施形態所說明之要領,經由MOVPE法,於藍寶石基板11上成膜至活性層22後,令電子阻障層23,以原料氣體或載流氣體之供給量及流速、AlN莫耳分率Xea作為目標值加以設定進行成膜。對於電子阻障層23之成長溫度,基本上如第1實施形態所說明,AlN莫耳分率Xea設定成較第1實施形態為高之故,依需要,在第1實施形態所例示之溫度範圍內進行調整即可。Therefore, in the second embodiment, in the method for manufacturing the light-emitting
整數m為10之時,於Ga富化EB領域23a內,AlGaN組成比成為Al
5Ga
1N
6之p型之準安定AlGaN雖作為第1準安定EB領域安定存在,於Al富化EB領域內,難以安定支配存在AlGaN組成比為Al
11Ga
1N
12之p型之準安定AlGaN。其理由係AlGaN組成比為Al
11Ga
1N
12之時,AlN莫耳分率極高至91.7%(12分之11),易於移動之Ga在進入對稱排列之位置前,量多之Al則隨機進入位置,Al與Ga之原子排列有很高的可能性不能成為對稱排列,Al與Ga之原子排列係接近隨機之狀態,作為準安定AlGaN之安定度會下降之緣故。
When the integer m is 10, in the Ga-enriched
整數m為8或9之故,準安定阱領域之AlGaN組成比(Al kGa 12-kN 12(k=3~7))與第1準安定EB領域(Al mGa 12-mN 12)之AlGaN組成比之間之組合係相當於第1實施形態所說明之m>k+2之條件時,與k=7之組合係不會成為適切之組合。 Since the integer m is 8 or 9, the composition ratio of AlGaN in the quasi-stable well region (Al k Ga 12-k N 12 (k=3~7)) and the first quasi-stable EB region (Al m Ga 12-m N 12 When the combination of the AlGaN composition ratios of ) corresponds to the condition of m>k+2 described in the first embodiment, the combination with k=7 is not an appropriate combination.
第2實施形態中,雖從準安定阱領域之AlGaN組成比,排除Al
7Ga
5N
12(AlN莫耳分率=58.3%),以準安定阱領域之AlGaN組成比(Al
kGa
12-kN
12(k=3~6))與n型包覆層21內之層狀領域21a內之第1準安定n型領域之AlGaN組成比為整數比之Al
nGa
12-nN
12(n=5~8)間之第1實施形態加以說明之關係(n≧k+1)係直接維持。
In the second embodiment, Al 7 Ga 5 N 12 (AlN molar ratio = 58.3%) is excluded from the AlGaN composition ratio in the quasi-stable well region, and the AlGaN composition ratio in the quasi-stable well region (Al k Ga 12- k N 12 (k=3~6)) and the AlGaN composition ratio of the first quasi-stable n-type region in the layered
本第2實施形態中,經由將Ga富化EB領域23a與Al富化EB領域各別以安定度高之第1及第2準安定EB領域構成,可更抑制起因於結晶成長裝置之漂移等之混晶莫耳分率之變動,於電子阻障層23,產生載子之局部存在化之Ga富化EB領域23a,對應於使用之第1準安定EB領域之AlN莫耳分率安定地加以形成。此結果,於電子阻障層23內,電流係優先安定流入Ga富化EB領域23a,更可達成發光元件1之特性變動之抑制。In the second embodiment, by forming the Ga-
第2實施形態之發光元件1之基材部10、及發光元件構造部20之AlGaN系半導體層21~24、p電極26、n電極27係除了於電子阻障層23之Al富化EB領域內支配存在第2準安定EB領域之部分,及調整成電子阻障層23之平均性之AlN莫耳分率Xea成為(m+0.5)/12<Xea<(m+1)/12之第1之適切範圍內,更佳係成為(m+0.5)/12<Xea≦ (m+0.9)/12之第2之適切範圍內之部分之外,與第1實施形態之發光元件1之基材部10、及發光元件構造部20之AlGaN系半導體層21~24、p電極26、n電極27相同之故,省略重覆之說明。The
[第3實施形態]
第3實施形態之發光元件1中,與第2實施形態之發光元件1相同,說明於電子阻障層23之Ga富化EB領域23a內,支配存在AlN莫耳分率較準安定阱領域之AlN莫耳分率高20%以上,AlGaN組成比為整數比之Al
mGa
12-mN
12之p型之準安定AlGaN所成第1準安定EB領域的同時,於電子阻障層23之Al富化EB領域內,支配存在AlGaN組成比為整數比之Al
m+1Ga
11-mN
12之p型之準安定AlGaN所成第2準安定EB領域。更且,電子阻障層23之平均性之AlN莫耳分率Xea之調整範圍係較上述第1實施形態所說明之範圍為窄,AlN莫耳分率Xea係調整成為(m+0.5)/12<Xea<(m+1)/12之第1之適切範圍內,更佳為調整成為(m+0.5)/12<Xea≦ (m+0.9)/12之第2之適切範圍內。惟,整數m為8或9。
[Third Embodiment] In the light-emitting
因此、第3實施形態中,於發光裝置1之製造方法中,以第1實施形態所說明之要領,經由MOVPE法,於藍寶石基板11上成膜至活性層22後,令電子阻障層23,以原料氣體或載流氣體之供給量及流速、AlN莫耳分率Xea作為目標值加以設定進行成膜。對於電子阻障層23之成長溫度,基本上如第1實施形態所說明,AlN莫耳分率Xea設定成較第1實施形態為高之故,依需要,在第1實施形態所例示之溫度範圍內進行調整即可。Therefore, in the third embodiment, in the method of manufacturing the light-emitting
更且,如第2實施形態所說明,準安定阱領域之AlGaN組成比(Al
kGa
12-kN
12(k=3~7))與第1準安定EB領域(Al
mGa
12-mN
12)之AlGaN組成比之間之組合係整數m為8或9之故,與k=7之組合係不會成為適切之組合。更且,雖從準安定阱領域之AlGaN組成比,排除Al
7Ga
5N
12(AlN莫耳分率=58.3%),以準安定阱領域之AlGaN組成比(Al
kGa
12-kN
12(k=3~6))與n型包覆層21內之層狀領域21a內之第1準安定n型領域之AlGaN組成比為整數比之Al
nGa
12-nN
12(n=5~8)間之第1實施形態加以說明之關係(n≧k+1)係直接維持。
Furthermore, as described in the second embodiment, the composition ratio of AlGaN in the quasi-stable well region (Al k Ga 12-k N 12 (k=3~7)) and the first quasi-stable EB region (Al m Ga 12-m Since the combination between the AlGaN composition ratios of N 12 ) is an integer m of 8 or 9, the combination with k=7 cannot be an appropriate combination. Furthermore, although Al 7 Ga 5 N 12 (AlN molar ratio=58.3%) was excluded from the AlGaN composition ratio in the quasi-stable well region, the AlGaN composition ratio in the quasi-stable well region (Al k Ga 12-k N 12 (k=3~6)) and the AlGaN composition ratio of the first quasi-stable n-type region in the layered
第3實施形態之發光元件1中,與第1及第2實施形態之發光元件1相同,n型包覆層21係以n型AlGaN系半導體加以構成,於n型包覆層21內,在n型包覆層21內,一樣分散存在局部性AlN莫耳分率低之層狀領域21a。因此,層狀領域21a係在先前技術之欄之上述所述,能帶隙能量局部地變小之故,載子易於局部存在化,作為低阻抗之電流路徑工作。In the light-emitting
但是,第3實施形態之發光元件1中,與第1及第2實施形態之發光元件1不同,無需於層狀領域21a之Ga富化n型領域內,存在AlGaN組成比成為整數比之Al
nGa
12-nN
12(n=5~8)之第1準安定n型領域,於n型本體領域21b之Al富化n型領域內,存在AlGaN組成比成為整數比之Al
n+1Ga
11-nN
12之第2準安定n型領域,及於n型本體領域21b,形成Al富化n型領域。但是,作為較佳之一實施形態之於層狀領域21a之Ga富化n型領域內,可存在AlGaN組成比成為整數比之Al
nGa
12-nN
12(n=5~8)之第1準安定n型領域,及/或可於n型本體領域21b,形成Al富化n型領域。
However, in the light-emitting
於層狀領域21a之Ga富化n型領域內,存在AlGaN組成比為整數比之Al
nGa
12-nN
12(n=5~8)之第1準安定n型領域之時,n型包覆層21之平均性之AlN莫耳分率Xna係在成為(n+0.24)/12<Xna<(n+1)/12之範圍內為佳。
In the Ga-enriched n-type region of the layered
即,第3實施形態之發光元件1中,與第1及第2實施形態之發光元件1相同,載子之局部存在化係各別易於產生在n型包覆層21之層狀領域21a、阱層220之Ga富化阱領域220a、阻障層221之Ga富化阻障領域221a及電子阻障層23之Ga富化EB領域23a。That is, in the light-emitting
另一方面,關於起因於結晶成長裝置之漂移等之發光元件1之特性變動,係於第1實施形態之發光元件1中,經由將n型包覆層21內之Ga富化n型領域與Al富化n型領域各別以安定度高之第1及第2準安定n型領域加以構成,主要於n型包覆層21內,對於強化混晶莫耳分率之變動抑制,第3實施形態之發光元件1中,經由將電子阻障層23內之Ga富化EB領域23a與Al富化EB領域各別以安定度高之第1及第2準安定EB領域加以構成,主要於電子阻障層23內,強化混晶莫耳分率之變動抑制。然而,第2實施形態之發光元件1中,於n型包覆層21內及電子阻障層23內之雙方,強化混晶莫耳分率之變動抑制。On the other hand, with regard to the variation in characteristics of the light-emitting
第3實施形態之發光元件1之基材部10、及發光元件構造部20之AlGaN系半導體層21~24、p電極26、n電極27係除了調整成在於n型包覆層21之n型本體領域21b之Al富化n型領域內,支配存在AlGaN組成比成為整數比之Al
n+1Ga
11-nN
12之第2準安定n型領域之部分,及於電子阻障層23之Al富化EB領域內,支配存在第2準安定EB領域之部分,及電子阻障層23之平均性之AlN莫耳分率Xea成為(m+0.5)/12<Xea<(m+1)/12之第1之適切範圍內,更佳係成為(m+0.5)/12<Xea≦(m+0.9)/12之第2之適切範圍內之部分之外,與第1實施形態之發光元件1之基材部10、及發光元件構造部20之AlGaN系半導體層21~24、p電極26、n電極27相同之故,省略重覆之說明。
The
[第4實施形態]
第1至第3實施形態之發光元件1中,構成發光元件構造部20之p型層係電子阻障層23與p型連接層24之2層,但第4實施形態之發光元件2中,p型層係於電子阻障層23與p型連接層24間,具有以1層以上之p型AlGaN系半導體構成之p型包覆層25。
[4th Embodiment]
In the light-emitting
因此,第4實施形態中,如圖19所示,發光元件構造部20之AlGaN系半導體層21~25係具備從基材部10側順序地,依n型包覆層21(n型層)、活性層22、電子阻障層23(p型層)、p型包覆層25(p型層)及p型連接層24(p型層)之順序磊晶成長加以層積之構造。Therefore, in the fourth embodiment, as shown in FIG. 19 , the AlGaN-based semiconductor layers 21 to 25 of the light-emitting
第4實施形態之發光元件2之基材部10、及發光元件構造部20之AlGaN系半導體層21~24、p電極26、n電極27係與第1至第3實施形態之任一之發光元件1之基材部10、及發光元件構造部20之AlGaN系半導體層21~24、p電極26、n電極27相同之故,省略重覆之說明。The
p型包覆層25係與藍寶石基板11之主面11a順序磊晶成長之基材部10之AlN層12、及發光元件構造部20之n型包覆層21和活性層22內之各半導體層與電子阻障層23相同,具有由來於藍寶石基板11之主面11a之形成平行於(0001)面之多段狀之平台之表面。The p-
於圖20,模式顯示活性層22之阱層220及阻障層221之層積構造(多重量子井構造)之一例。圖20中,於第1實施形態中,於使用圖8說明之層積構造之電子阻障層23上,形成p型包覆層25。In FIG. 20, an example of the laminated structure (multiple quantum well structure) of the
於p型包覆層25中,鄰接於橫方向之平台T間係如上述,形成對於(0001)面傾斜之傾斜領域IA。令傾斜領域IA以外之上下被平台T挾持之領域,稱之為平台領域TA。p型包覆層25之膜厚係包含平台領域TA及傾斜領域IA,例如調整在20nm~200nm之範圍內。In the p-
如圖20模式性顯示,於p型包覆層25中,經由從平台領域TA向傾斜領域IA之Ga之質量移動,於傾斜領域IA內,形成較平台領域TA,AlN莫耳分率為低之第3Ga富化領域25a。As schematically shown in FIG. 20 , in the p-
p型包覆層25之平台領域TA之AlN莫耳分率係51%以上,設定在不足電子阻障層23之平台領域TA之AlN莫耳分率之範圍內。更且,p型包覆層25之Ga富化p型領域25a之AlN莫耳分率係設定成不足電子阻障層23之Ga富化EB領域23a之AlN莫耳分率。The AlN molar ratio of the terrace area TA of the p-
更且,p型包覆層25之平台領域TA之AlN莫耳分率係於上述範圍中,較Ga富化p型領域25a之AlN莫耳分率,設定成1%以上,較佳為2%以上,更佳為4%以上,設定在高水準。為了充分確保Ga富化p型領域25a之載子之局部存在化効果,雖令p型包覆層25內之第2Ga富化領域25a與平台領域TA之AlN莫耳分率差成為4~5%以上為佳、但1~2%程度下,以可期待載子之局部存在化效果。Moreover, the AlN molar ratio of the plateau region TA of the p-
作為較佳一實施形態,於電子阻障層23之Ga富化EB領域23a內,與支配存在AlN莫耳分率較準安定阱領域之AlN莫耳分率高20%以上,AlGaN組成比成為整數比之Al
mGa
12-mN
12 ,AlN莫耳分率為Xe0(=m/12)之p型之準安定AlGaN所構成之第1準安定EB領域相同,於p型包覆層25之Ga富化p型領域25a內,支配存在AlGaN組成比成為整數比之Al
iGa
12-iN
12,AlN莫耳分率為Xp0(=i/12),且不足電子阻障層23之第1準安定EB領域之AlN莫耳分率Xe0之p型之準安定AlGaN所構成之第1準安定p型領域。電子阻障層23與第1實施形態之發光元件1之電子阻障層23相同之時、整數m係8、9、或10,與第2或第3實施形態之發光元件1之電子阻障層23相同之時,整數m係8或9。整數i為6、7或8,且滿足i<m。因此,整數m為8之時,整數i係6或7。
As a preferred embodiment, in the Ga-enriched
更且,作為較佳之一實施形態,於p型包覆層25之Ga富化p型領域25a,形成上述AlGaN組成比(Al
iGa
12-iN
12,i=6~8),AlN莫耳分率為Xp0(=i/12)之第1準安定p型領域之時,p型包覆層25之平均性AlN莫耳分率Xpa係調整在成為(i+0.24)/12≦Xpa<(i+1)/12之範圍內為佳。p型包覆層25之平台領域TA之平均性AlN莫耳分率(形成後述Al富化p型領域之時,排除Al富化p型領域)係與p型包覆層25之平均性AlN莫耳分率Xpa略同。因此,作為p型包覆層25之Ga富化p型領域25a與平台領域TA之AlN莫耳分率差,可確保在約2%以上。然而,p型包覆層25之平均性AlN莫耳分率Xpa係即使超出成為(i+0.24)/12≦Xpa< (i+1)/12範圍,只要於p型包覆層25之傾斜領域IA內形成可載子之局部存在化之Ga富化p型領域25a,在大概51%~75%之範圍內,可取得對應於電子阻障層23之Ga富化EB領域23a內之AlN莫耳分率Xe0之任意值。
Furthermore, as a preferred embodiment, in the Ga-enriched p-
接著,對於p型包覆層25之成長方法簡單加以說明。於p型包覆層25形成中,以與第1實施形態所說明之n型包覆層21及電子阻障層23同樣之要領,在易於表現出上述之多段狀之平台的成長條件下,將p型包覆層25之AlN莫耳分率Xpa作為目標值,成長p型包覆層25。Next, a method of growing the p-
p型包覆層25之平均性AlN莫耳分率Xpa係於p型包覆層25之Ga富化p型領域25a內,形成AlN莫耳分率Xp0之第1準安定p型領域之時,設定在成為Xp0+2%≦ Xpa<Xp0+8.33%之範圍內。The average AlN molar fraction Xpa of the p-
第4實施形態中,令p型包覆層25之成長溫度為T5之時,電子阻障層23之成長溫度T3與p型連接層之成長溫度T4之間之關係係例如於1050℃~1170℃之範圍內,滿足以下式(3)所示關係為佳。
T3>T5>T4 (3)
In the fourth embodiment, when the growth temperature of the p-
更且,p型包覆層25之成長溫度T5係第1準安定p型領域之AlN莫耳分率Xp0為66.7%時,1100℃以上為佳,第1準安定p型領域之AlN莫耳分率Xp0為58.3%或50%之時,1050℃以上為佳。Furthermore, when the growth temperature T5 of the p-
作為為促進p型包覆層25之Ga之質量移動之成長溫度以外之成長條件之一例,成長溫度T5為1080℃之時,令原料氣體之流量比(V/III)為1000~6000,令成長速度成為約100nm/h為佳。As an example of growth conditions other than the growth temperature for promoting the mass transfer of Ga of the p-
將滿足n型包覆層21、活性層22(阱層220、阻障層221)、電子阻障層23、p型連接層24、及p型包覆層25之成長溫度T1~T5之上述式(1A)、(2)及(3)之一例,示於如下。
T1=T2=1080℃、T3=1150℃、T4=980℃、T5=1080℃
The above-mentioned growth temperatures T1 to T5 of the n-
上述成長溫度T5之一例係適用於以下所示p型包覆層25之Ga富化p型領域25a內之第1準安定p型領域之AlN莫耳分率Xp0。
Xp0=50%、58.3%、66.7%
An example of the above-mentioned growth temperature T5 is applied to the AlN molar fraction Xp0 of the first quasi-stable p-type region in the Ga-enriched p-
p型包覆層25之受體不純物濃度係作為一例,1.0×10
16~1.0×10
18cm
-3程度為佳。然而,受體不純物濃度係對於p型包覆層25之膜厚,無需一定均勻控制於上下方向。
As an example, the acceptor impurity concentration of the p-
更且,作為p型包覆層25之較佳實施形態,於p型包覆層25中,於鄰接於傾斜領域IA之平台領域TA之端緣部,令p型包覆層25之平均性AlN莫耳分率Xpa作為基準,形成局部性AlN莫耳分率為高之Al富化p型領域亦可。Furthermore, as a preferred embodiment of the p-
更且,作為p型包覆層25之較佳一實施形態,於p型包覆層25之平台領域TA,形成Al富化p型領域之時,於Ga富化p型領域25a內,支配存在AlGaN組成比為整數比之Al
iGa
12-iN
12之p型之準安定AlGaN所成第1準安定p型領域的同時,於Al富化p型領域內,支配存在AlGaN組成比為整數比之Al
i+1Ga
11-iN
12之p型之準安定AlGaN所成第2準安定p型領域。此時,p型包覆層25之平均性之AlN莫耳分率Xpa之調整範圍係較上述較佳範圍(下限為(i+0.24)/12)為窄,AlN莫耳分率Xpa係調整成為(i+0.5)/12<Xpa<(i+1)/12之第1之適切範圍內,更佳為調整成為(i+0.5)/12<Xpa≦ (i+0.9)/12之第2之適切範圍內。
Furthermore, as a preferred embodiment of the p-
上述較佳實施形態中,經由將Ga富化p型領域25a與Al富化p型領域各別以安定度高之第1及第2準安定p型領域加以構成,可更抑制起因於結晶成長裝置之漂移等之混晶莫耳分率之變動,於p型包覆層25,產生載子之局部存在化之Ga富化p型領域25a,則對應於使用之第1準安定p型領域之AlN莫耳分率安定地加以形成。此結果,於p型包覆層25內,電流係優先安定流入Ga富化p型領域25a,更可達成發光元件1之特性變動之抑制。In the above-described preferred embodiment, by forming the Ga-rich p-
以上詳細說明之第4實施形態之發光元件1係電子阻障層23與p型包覆層25,具有形成平行由來於藍寶石基板11之主面11a之(0001)面之多段狀之平台的表面,於鄰接於橫方向之平台T間,形成對於(0001)面傾斜之傾斜領域IA,於電子阻障層23之傾斜領域IA內,形成較平台領域TA,AlN莫耳分率為低之Ga富化EB領域23a,更且,於p型包覆層25之傾斜領域IA內,形成較平台領域TA,AlN莫耳分率為低之Ga富化p型領域25a為特徵。The light-emitting
經由該特徵,第4實施形態之發光元件2係可在Ga富化p型領域25a內,產生載子(電洞)之局部存在化之故,如圖21模式性顯示,植入於p型包覆層25(p-clad)內之電洞(h+)係亦直接植入傾斜領域IA內,或擴散平台領域TA內,到達傾斜領域IA內。更且,在第1Ga富化領域23a內,亦產生載子(電洞)之局部存在化之故,植入於電子阻障層23內之電洞係從p型包覆層25之傾斜領域IA,亦直接植入電子阻障層23之傾斜領域IA內。因此,無p型包覆層25時,將從p型連接層24植入至薄膜之電子阻障層23之平台領域TA,直接到達阱層22之平台領域TA之電洞之一部分,從p型包覆層25之平台領域TA透導至傾斜領域IA內,經由電子阻障層23之傾斜領域IA,到達阱層22之傾斜領域IA內。作為結果,更可抑制內部量子效率之下降、及雙發光尖峰之產生。然而,於圖21中,與圖5相同,☆(星型)係顯示阱層之傾斜領域IA內之局部存在中心,●(黑圓)係顯示非發光再結合中心。By virtue of this feature, the light-emitting
[其他實施形態] 以下,對於上述第1至第4實施形態之變形例加以說明。 [Other Embodiments] Hereinafter, modifications of the above-described first to fourth embodiments will be described.
(1)上述第1至第4實施形態中,活性層22係設想以交互層積以AlGaN系半導體所構成之2層以上之阱層220、和以AlGaN系半導體或AlN系半導體所構成之1層以上之阻障層221的多重量子井構造加以構成之情形,但活性層22係阱層220為僅1層之單一量子井構造,不具備阻障層221(量子阻障層)之構成亦可。對於相關單一量子井構造,同樣明確可發揮以上述各實施形態所採用n型包覆層21、電子阻障層23等所造成之效果。(1) In the above-described first to fourth embodiments, the
(2)上述各實施形態中,作為n型包覆層21之成長條件之一例,說明有機金屬化合物氣相成長法所使用之原料氣體或載流氣體之供給量及流速係對應構成n型包覆層21,n型AlGaN層整體之平均AlN莫耳分率加以設定。即,n型包覆層21整體之平均AlN莫耳分率,則於上下方向設定成一定值之時,上述原料氣體等之供給量及流速係設想控制於一定之情形。但是,上述原料氣體等之供給量及流速係非一定要控制於一定。(2) In the above-mentioned embodiments, as an example of the growth conditions of the n-
(3)上述各實施形態中,第1領域R1及p電極26之平面所視形狀係作為一例,雖採用梳形形狀者,但該平面所視形狀係非限定於梳形形狀。又,可為複數存在第1領域R1,各別包圍於1個之第2領域R2之平面所視形狀亦可。(3) In each of the above-described embodiments, the shape of the first region R1 and the p-
(4)於上述各實施形態中,雖例示使用主面對於(0001)面具有偏角之藍寶石基板11,於AlN層12之表面,使用表現出多段狀之平台之基材部10之情形,該偏角之大小或設置偏角之方向(具體而言,傾斜(0001)面之方向,例如m軸方向或a軸方向等)係於AlN層12之表面,表現出多段狀之平台,只要形成層狀領域21a之成長開始點,可任意加以決定。(4) In the above-mentioned embodiments, although the
(5)上述各實施形態中,作為發光元件1,雖如圖1所例示,例示了具備包含藍寶石基板11之基材部10的發光元件1,但可經由將藍寶石基板11(更且,含於基材部10之一部分或全部之層)經由掀離等加以除去。更且,構成基材部10之基板係非限定於藍寶石基板。
[產業上的可利用性]
(5) In the above-described embodiments, as the light-emitting
本發明係可利用於具備閃鋅礦構造之AlGaN系半導體所成n型層、活性層、及p型層,層積於上下方向之發光元件構造部而成之氮化物半導體紫外線發光元件。The present invention is applicable to a nitride semiconductor ultraviolet light-emitting element formed by an AlGaN-based semiconductor having a sphalerite structure, an n-type layer, an active layer, and a p-type layer, which are laminated on a light-emitting element structure portion in the vertical direction.
1:氮化物半導體紫外線發光元件
10:基材部
11:藍寶石基板
11a:藍寶石基板之主面
12:AlN層
20:發光元件構造部
21:n型包覆層(n型層)
21a:層狀領域(n型層)
21b:n型本體領域(n型層)
22:活性層
220:阱層
220a:Ga富化阱領域
221:阻障層
221a:Ga富化阻障領域
23:電子阻障層(p型層)
23a:Ga富化EB領域
24:p型連接層(p型層)
25:p型包覆層(p型層)
25a:Ga富化p型領域
26:p電極
27:n電極
100:基板
101:AlGaN系半導體層
102:模板
103:n型AlGaN系半導體層
104:活性層
105:p型AlGaN系半導體層
106:p型連接層
107:n電極
108:p電極
BL:第1領域與第2領域的邊界線
IA:傾斜領域
R1:第1領域
R2:第2領域
T:平台
TA:平台領域
1: Nitride semiconductor ultraviolet light-emitting element
10: Substrate part
11:
[圖1]模式性顯示AlGaN之閃鋅礦結晶構造之圖。
[圖2]顯示從圖1所示閃鋅礦結晶構造之c軸方向所視A面之各位置與B面之各位置間之位置關係的平面圖。
[圖3]模式性顯示以整數比表示之AlGaN組成比之5個組合之各個A3面與B3面之Al與Ga之配置。
[圖4]模式性說明以往之氮化物半導體紫外線發光元件之阱層及電子阻障層內之載子之舉動圖。
[圖5]模式性說明本發明之第2特徵之氮化物半導體紫外線發光元件之阱層及電子阻障層內之載子之舉動圖。
[圖6]模式性顯示關於第1至第3實施形態之氮化物半導體紫外線發光元件之構造之一例的主要部剖面圖。
[圖7]模式性顯示伴隨n型包覆層內之Ga之質量移動之Ga富化n型領域及Al富化n型領域內之AlN莫耳分率之變化圖。
[圖8]模式性顯示圖6所示氮化物半導體紫外線發光元件之活性層之層積構造之一例的主要部剖面圖。
[圖9]顯示Ga富化阱領域220a之AlN莫耳分率為50%時之AlGaN阱層與AlGaN阻障層所成量子井構造之發光波長、和阱層之膜厚及阻障層之AlN莫耳分率之關係之圖表。
[圖10]顯示Ga富化阱領域220a之AlN莫耳分率為41.7%時之AlGaN阱層與AlGaN阻障層所成量子井構造之發光波長、和阱層之膜厚及阻障層之AlN莫耳分率之關係之圖表。
[圖11]顯示Ga富化阱領域220a之AlN莫耳分率為33.3%時之AlGaN阱層與AlGaN阻障層所成量子井構造之發光波長、和阱層之膜厚及阻障層之AlN莫耳分率之關係之圖表。
[圖12]顯示GaN阱層與AlGaN阻障層所成量子井構造之發光波長、和阱層之膜厚及阻障層之AlN莫耳分率之關係之圖表。
[圖13]模式性顯示將圖6所示氮化物半導體紫外線發光元件,從圖6之上側所視時之構造之一例的平面圖。
[圖14]顯示試料片A之CL法所成AlN莫耳分率之測定剖面之主要部分之SEM像。
[圖15]顯示試料片B之CL法所成AlN莫耳分率之測定剖面之主要部分之SEM像。
[圖16]顯示圖14所示試料片A之測定剖面上之5個Y座標上之第1及第2之CL光譜之圖。
[圖17]顯示圖15所示試料片B之測定剖面上之下側部分之4個Y座標上之第3及第4之CL光譜之圖。
[圖18]顯示圖15所示試料片B之測定剖面上之上側部分之5個Y座標上之第5及第6之CL光譜之圖。
[圖19]模式性顯示關於第4實施形態之氮化物半導體紫外線發光元件之構造之一例的主要部剖面圖。
[圖20]模式性顯示包含圖19所示氮化物半導體紫外線發光元件之活性層之主要部之層積構造之一例的主要部剖面圖。
[圖21]模式性說明關於第4實施形態之氮化物半導體紫外線發光元件之阱層、電子阻障層、及p型包覆層內之載子之舉動圖。
[圖22]模式性顯示一般之紫外線發光二極體之元件構造之一例的主要部剖面圖。
[圖23]顯示以往之氮化物半導體紫外線發光元件之n型包覆層、活性層、及電子阻障層內之剖面構造的HAADF-STEM像。
[ Fig. 1 ] A diagram schematically showing the sphalerite crystal structure of AlGaN.
[ Fig. 2] Fig. 2 is a plan view showing the positional relationship between each position of the A plane and each position of the B plane viewed from the c-axis direction of the sphalerite crystal structure shown in Fig. 1 .
[ Fig. 3] Fig. 3 schematically shows the arrangement of Al and Ga in each of the A3 face and the B3 face of five combinations of AlGaN composition ratios expressed as integer ratios.
[ Fig. 4] Fig. 4 is a diagram schematically illustrating the behavior of carriers in a well layer and an electron barrier layer of a conventional nitride semiconductor ultraviolet light emitting device.
[ Fig. 5] Fig. 5 is a diagram schematically illustrating the behavior of carriers in the well layer and the electron barrier layer of the nitride semiconductor ultraviolet light emitting device according to the second feature of the present invention.
[ Fig. 6] Fig. 6 is a cross-sectional view of a main part schematically showing an example of the structure of the nitride semiconductor ultraviolet light-emitting element according to the first to third embodiments.
[ Fig. 7] Fig. 7 is a diagram schematically showing a change in the molar ratio of AlN in the Ga-enriched n-type region and the Al-enriched n-type region accompanying the mass shift of Ga in the n-type cladding layer.
[ Fig. 8] Fig. 8 is a cross-sectional view of a main part schematically showing an example of the laminated structure of the active layer of the nitride semiconductor ultraviolet light emitting device shown in Fig. 6 .
[Fig. 9] shows the emission wavelength of the quantum well structure formed by the AlGaN well layer and the AlGaN barrier layer when the AlN molar fraction of the Ga-enriched
1:氮化物半導體紫外線發光元件 1: Nitride semiconductor ultraviolet light-emitting element
10:基材部 10: Substrate part
11:藍寶石基板 11: Sapphire substrate
11a:藍寶石基板之主面 11a: The main surface of the sapphire substrate
12:AlN層 12: AlN layer
20:發光元件構造部 20: Light-emitting element structure
21:n型包覆層(n型層) 21: n-type cladding layer (n-type layer)
21a:層狀領域(n型層) 21a: Layered field (n-type layer)
21b:n型本體領域(n型層) 21b: n-type body field (n-type layer)
22:活性層 22: Active layer
220:阱層 220: Well Layer
221:阻障層 221: Barrier Layer
23:電子阻障層(p型層) 23: Electronic barrier layer (p-type layer)
24:p型連接層(p型層) 24: p-type connection layer (p-type layer)
26:p電極 26:p electrode
27:n電極 27:n electrode
R1:第1領域
R1:
R2:第2領域
R2:
Claims (11)
Applications Claiming Priority (2)
Application Number | Priority Date | Filing Date | Title |
---|---|---|---|
PCT/JP2020/040069 WO2022091173A1 (en) | 2020-10-26 | 2020-10-26 | Nitride semiconductor ultraviolet light emitting element |
WOPCT/JP2020/040069 | 2020-10-26 |
Publications (1)
Publication Number | Publication Date |
---|---|
TW202218178A true TW202218178A (en) | 2022-05-01 |
Family
ID=81383745
Family Applications (1)
Application Number | Title | Priority Date | Filing Date |
---|---|---|---|
TW110126567A TW202218178A (en) | 2020-10-26 | 2021-07-20 | Nitride semiconductor ultraviolet light emitting element |
Country Status (3)
Country | Link |
---|---|
JP (1) | JPWO2022091173A1 (en) |
TW (1) | TW202218178A (en) |
WO (1) | WO2022091173A1 (en) |
Family Cites Families (4)
Publication number | Priority date | Publication date | Assignee | Title |
---|---|---|---|---|
TWI649895B (en) * | 2010-04-30 | 2019-02-01 | 美國波士頓大學信託會 | High-efficiency ultraviolet light-emitting diode with variable structure position |
WO2019159265A1 (en) * | 2018-02-14 | 2019-08-22 | 創光科学株式会社 | Nitride semiconductor ultraviolet light-emitting element |
JP7312056B2 (en) * | 2019-01-07 | 2023-07-20 | 日機装株式会社 | Semiconductor light emitting device and method for manufacturing semiconductor light emitting device |
JP6793863B2 (en) * | 2019-01-22 | 2020-12-02 | Dowaエレクトロニクス株式会社 | Manufacturing method of reflective electrode for deep ultraviolet light emitting element, manufacturing method of deep ultraviolet light emitting element and deep ultraviolet light emitting element |
-
2020
- 2020-10-26 WO PCT/JP2020/040069 patent/WO2022091173A1/en active Application Filing
- 2020-10-26 JP JP2022558606A patent/JPWO2022091173A1/ja active Pending
-
2021
- 2021-07-20 TW TW110126567A patent/TW202218178A/en unknown
Also Published As
Publication number | Publication date |
---|---|
JPWO2022091173A1 (en) | 2022-05-05 |
WO2022091173A1 (en) | 2022-05-05 |
Similar Documents
Publication | Publication Date | Title |
---|---|---|
KR102618238B1 (en) | Nitride semiconductor light emitting device | |
US9224595B2 (en) | Semiconductor optical element array and method of manufacturing the same | |
TWI703741B (en) | Nitride semiconductor ultraviolet light emitting element and manufacturing method of nitride semiconductor ultraviolet light emitting element | |
US11217726B2 (en) | Nitride semiconductor ultraviolet light-emitting element | |
US10995403B2 (en) | Method of forming aluminum nitride film and method of manufacturing semiconductor light-emitting element | |
TW202213814A (en) | Nitride semiconductor ultraviolet light emitting element | |
TWI828945B (en) | Nitride semiconductor ultraviolet light-emitting element | |
JP7421657B2 (en) | Nitride semiconductor ultraviolet light emitting device | |
WO2022009306A1 (en) | Nitride semiconductor uv light-emitting element and production method therefor | |
JP7406633B2 (en) | Nitride semiconductor ultraviolet light emitting device and manufacturing method thereof | |
TW202218178A (en) | Nitride semiconductor ultraviolet light emitting element | |
WO2022219731A1 (en) | Nitride semiconductor uv light-emitting element and production method therefor | |
WO2022149183A1 (en) | Method for producing nitride semiconductor ultraviolet light emitting element, and nitride semiconductor ultraviolet light emitting element | |
JP2017224841A (en) | Nitride semiconductor ultraviolet light-emitting element | |
WO2023203599A1 (en) | Nitride semiconductor ultraviolet light-emitting diode |