TW200308088A - Bipolar transistor with graded base layer - Google Patents
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Abstract
Description
200308088 玫、發明說明: 【發明所屬之技術領域】 本發明係關於電晶體,尤其係關於具分級基極層的雙 極電晶體。 【先前技術】 雙極接合電晶體(bipolar junction transistor,BJT) 和異貝接合雙極電晶體(heter〇juncti〇n bip〇iar transistor,HBT)的積體電路(integrated circuit,IC)已 經發展成為多種應用的重要科技,尤其是做為無線手機、 微波儀器以及光纖通訊系統之高速電路(每秒大於一百億 位=)胃的功率放大器。預期未來的需求乃需要具有較低操 作電壓、車交高頻率的表現、較高附加功率的效率以及較低 製造成本的元件。BJT &順的打開電壓(1)乃定義成 達到一疋之固定集極電流密度(Jc)所需要的基極—射極電 麼(vbe)。對於供應電壓受限於電池科技和其他組件之功率 需求的低功率應用而言,此打開電壓可以限制元件的 性。 …中的射極、基極和集極係由-種半導體材料 所裝成,HBT係、由兩種不相似的半導體材料所製成, 射極半導體材料的能帶間隙(bandgap、energy要: 做成基極之半導體材料的能帶間隙來得大。此導致 到集極的載子注入效率優於饥,此乃因為建立了阻= 子注入從基極回到射極的阻障。選擇具有較小能帶間隙的 200308088 基極可降低打開„,此乃因為從基極到集極之載子注入 j率的增加會在給定的基極—射極電壓下增加集極的電流 密度。 然而,HBT的半導體材料於異質接合處之能帶對齊具 有突然不連續的缺點,此可導致纟m的射極—基極界面 處有傳導能帶的突峰(spike)。此傳導能帶突峰的效應是阻 礙了電子從基極出來傳輸到集極。因Λ,電子待在基極比 較久,導致再結合的程度增加以及集極電流增益(/5dc)的 減少。如上所討論的,由於異質接合雙極電晶體的打開電 壓乃定義成達到-定之固定集極電流密度所需要的基極〜 射極電壓,所以降低集極電流增益有效地提昇順的打開 電壓。因此,HBT半導體材料的製造需要進一步改良,^ 降低打開電壓,藉此改善低電壓操作的元件。 本發明提供一種HBT,其具有η㉟換雜的集極、形成 於集極上而由In—V族材料(包括鋼和氮)所組成的基極、 以及形成於基極上之n型摻雜的射極。基極層的族 材料具有大約LSxiPd3到大約7〇xl〇19cm_3的碳摻雜濃 度。在一較佳的具體態樣中,基極層包括鎵、銦、砷和氮 元素。相對於GaAs的能帶間隙而言,銦和氮的存在減少了 此材料的能帶間隙。此外,此材料中的換雜濃度為高,而 片電阻(Rsb)為低。相對於具有類似摻雜濃度之基極 層的HBT而言,這些因素導致較低的打開電壓。 200308088 在-較佳的具體態樣中,⑴巧崎物材料系統可 :由化學…MSl_A來代表。已知當少量的氮併入 〜-x nxAs時’此材料的能帶間隙會實質地降下來。再者 :因為氮以相反於銦的方向來推動晶格常數,所以把錮對 虱的適當比例加入此材料,可以長出晶格匹配力⑽的 〇〜_χΙηχΑδι_Α合金。因此可以消除導致能量間隙增加和材 料差排不配的多餘應變。因此選擇能降低或消除應變之銦 對氮的比例。在本發明的較佳具體態樣中,ηβτ之基極層 Ga^xInxAs卜yNy 中的 x=3y 〇 3 在具有GaAs的傳統HBT中,隨著溫度的增加,以致電 洞注入射極程度較高,$間電荷層的再結合電流較高,並 且基極中的擴散長度可能較短,故電流增益典型上會降低 。在具有GalnAsN基極層的HBT中,隨著溫度的增加,發 現電流增益有顯著的增加(每rc大約升高〇3%)。此結果 乃解釋為擴散長度隨著溫度的增加而有所增加。如果能帶 底部的電子乃侷限於它們是至少部份地局部化的狀態=π 則預期會有此種效應,並且隨著溫度的增加,它們^上述 狀態熱激發到電子可以更輕易擴散的其他狀態。因此,以 GalnAsN設計構成基極層則改進了本發明Ηβτ的溫度特徵 ’並且減少了對於溫度補償次電路的需求。 相對於具有GaAs基極層的傳統Ηβτ而言,具有 GalnAsN基極層的HBT已經改善了共同的射極輸出特徵。舉 例而吕,具有GalnAsN基極層之HBT的偏移(0ffset)電壓和 拐曲(knee)電壓要比具有GaAs基極層的傳統HBT來得低。 200308088 在一具體態樣中’電晶體是雙重異質接合雙極電晶體 (double heterojunction bipolar transistor , DHBT),其 組成基極的半導體材料乃異於製成射極和集極的半導體材 料在的較佳具體態樣中,GainAsN基極層可以由化 學式Ga^xIrixAsi-yNy來代表,集極是GaAs,並且射極是選 自 InGaP 、 AlInGaP 和 AlGaAs 〇 本發明的另一個較佳具體態樣係關於HBT或DHBT,其 中降低了傳導能帶突峰的高度,同時降低了基極層的能帶 間隙(Egb)。傳導能帶突峰是由在基極/射極異質接合或基 極/集極異質接合處的傳導能帶不連續所引起的。藉由使 β θ勺曰“口匹配於射極和/或集極層而減少了晶格應變 2則降低了傳導能帶突峰。此典型上是由控制基極層中之 氮和銦的濃度所做到的。基極層最好具有化學式‘ χΙηχΑ~-Λ,其中X大約等於3y。 在一具體態樣中,基極可以在組成上加以分級,以製 出能帶間隙在集極處比較小而能帶間隙在射極處比較大之 ::的能帶間隙層。基極層的能帶間隙在基極層與集極接 ,最好比在基極層與射極接觸的表面處低大約 ZOmeV到大約12〇meV。基 到射極呈線性地變化越過基極層听間隙更好則是從集極 陳二氮和麵到GaAS半導雜村料t降低了材料的能帶間 半導體材料的能帶間隙要比GaAs ,A極芦ό明之組成分級的㈣-山^必基極層中 ^曰的能帶間隙在集極處減少得要比在射極處來得大 200308088 °然而’相較於GaAs越過基極層的能帶間隙而言,上述能 ▼間隙典型上平均減少大約lOmeV到大約300meV。在一具 體恶樣中’相較於GaAs越過基極層的能帶間隙而言,上述 月b f間隙典型上平均減少大約8〇meV到大約3〇〇meV。在另 具體怨樣中,相較於GaAs越過基極層的能帶間隙而言, 上述能帶間隙典型上平均減少大約l〇meV到大約2〇〇meV。 此降低的能帶間隙導致具有組成分級之GanIMShNy基 極層的HBT的打開電壓(Vbe,。。)要比具有基極層的hBT 來得低,此乃因為Vbe〇n中的主要決定者是基極中的固有 載子濃度。固有載子濃度(ni)由以下公式所計算: ni=NcNvexp(-Eg/kT) 隹上迷公式中,Nc是傳 .....w匁双祗反,文200308088 Description of the invention: [Technical field to which the invention belongs] The present invention relates to a transistor, and more particularly to a bipolar transistor having a graded base layer. [Previous technology] Integrated circuits (ICs) of bipolar junction transistors (BJT) and heterojunction bipolar transistors (HBT) have been developed into An important technology for a variety of applications, especially as a high-speed circuit (greater than 10 billion bits per second =) of gastric power amplifiers for wireless handsets, microwave instruments, and fiber optic communication systems. It is expected that future demand will require components with lower operating voltages, high-frequency performance, higher added power efficiency, and lower manufacturing costs. The BJT & synchronous turn-on voltage (1) is defined as the base-emitter voltage (vbe) required to reach a fixed collector current density (Jc). For low power applications where the supply voltage is limited by the power requirements of battery technology and other components, this turn-on voltage can limit the performance of the component. The emitter, base, and collector in… are made of one kind of semiconductor material, HBT is made of two dissimilar semiconductor materials, and the band gap of the emitter semiconductor material (bandgap, energy is: The band gap of the semiconductor material used to make the base is large. This results in a carrier injection efficiency to the collector that is better than hunger. This is due to the establishment of a barrier = a barrier for the injection of the carrier from the base back to the emitter. The 200308088 base with a smaller band gap can reduce the opening because the increase in the rate of carrier injection j from the base to the collector will increase the collector current density at a given base-emitter voltage. However, the band alignment of HBT semiconductor materials at heterojunctions has the disadvantage of sudden discontinuity, which can lead to spikes in the conduction band at the emitter-base interface of 纟 m. This conduction band bursts The effect of the peak is to prevent the electrons from transmitting from the base to the collector. Due to Λ, the electrons stay at the base for a longer time, resulting in an increase in the degree of recombination and a reduction in the collector current gain (/ 5dc). As discussed above, Due to the heterojunction of bipolar transistors The opening voltage is defined as the base-emitter voltage required to reach a fixed collector current density, so reducing the collector current gain effectively increases the forward opening voltage. Therefore, the manufacturing of HBT semiconductor materials needs further improvement. The voltage is turned on, thereby improving low-voltage operation elements. The present invention provides an HBT having an η㉟-doped collector, a base formed on the collector and composed of In-V group materials (including steel and nitrogen), And an n-type doped emitter formed on the base. The family material of the base layer has a carbon doping concentration of about LSxiPd3 to about 70 × 1019 cm_3. In a preferred embodiment, the base layer includes Gallium, indium, arsenic, and nitrogen elements. Compared to the band gap of GaAs, the presence of indium and nitrogen reduces the band gap of this material. In addition, the impurity concentration in this material is high, and the sheet resistance (Rsb ) Is low. Compared to HBTs with a similar doping concentration of the base layer, these factors lead to lower turn-on voltages. 200308088 In a preferred embodiment, the oscillating material system can: … MSl_A It is known that when a small amount of nitrogen is incorporated into ~ -x nxAs, the band gap of this material will substantially decrease. Furthermore: because nitrogen promotes the lattice constant in a direction opposite to indium, the Adding this material in the proper proportion of lice can grow a lattice-matching alloy 〇 ~ _χΙηχΑδι_Α. Therefore, it can eliminate the excess strain that leads to the increase of energy gap and the mismatch of materials. Therefore, the indium to nitrogen can be selected to reduce or eliminate strain In a preferred embodiment of the present invention, x = 3y in the base layer Ga ^ xInxAs and yNy of ηβτ. In a conventional HBT with GaAs, as the temperature increases, a hole is injected into the emitter. To a higher degree, the recombination current of the charge layer between $ is higher, and the diffusion length in the base may be shorter, so the current gain is typically reduced. In HBT with a GalnAsN base layer, as the temperature was increased, a significant increase in current gain was found (approximately 0.3% increase per rc). This result is explained as the diffusion length increases with increasing temperature. If the electrons at the bottom of the band are limited to a state where they are at least partially localized = π, this effect is expected, and as the temperature increases, they are thermally excited to other states where the electrons can diffuse more easily status. Therefore, constructing the base layer with a GalnAsN design improves the temperature characteristics of the β? Of the present invention and reduces the need for a temperature-compensated secondary circuit. Compared to the conventional Ηβτ with a GaAs base layer, HBT with a GalnAsN base layer has improved common emitter output characteristics. For example, the offset voltage and knee voltage of an HBT with a GalnAsN base layer are lower than that of a conventional HBT with a GaAs base layer. 200308088 In a specific aspect, the 'transistor is a double heterojunction bipolar transistor (DHBT). The semiconductor material constituting the base is different from the semiconductor material made of the emitter and collector. In a preferred embodiment, the GainAsN base layer can be represented by the chemical formula Ga ^ xIrixAsi-yNy, the collector is GaAs, and the emitter is selected from InGaP, AlInGaP, and AlGaAs. Another preferred embodiment of the present invention is HBT or DHBT, which reduces the height of the peak of the conduction band, and at the same time reduces the band gap (Egb) of the base layer. The conduction band spike is caused by a discontinuity in the conduction band at the base / emitter heterojunction or base / collector heterojunction. Reducing the lattice strain by matching the β θ to the emitter and / or collector layer reduces the conduction band spikes. This is typically controlled by the nitrogen and indium in the base layer. The concentration is done. The base layer preferably has the chemical formula 'χΙηχΑ ~ -Λ, where X is approximately equal to 3y. In a specific aspect, the base can be graded in composition to make a band gap at the collector The band gap is smaller and the band gap is larger at the emitter: The band gap layer of the ::. The band gap of the base layer is connected to the collector at the base layer, and it is better than the one in which the base layer is in contact with the emitter. The surface is about ZOmeV to about 120meV lower. The base-to-emitter changes linearly across the base layer and the listening gap is better. The band gap of semiconductor materials between bands is larger than that of GaAs and A poles. The band gap in the ㈣-mount ^ base layer is reduced at the collector than at the emitter. 200308088 ° However, compared to the band gap of GaAs across the base layer, the above energy gap typically decreases by about 10 on average. meV to about 300 meV. In a specific case, compared to the band gap of GaAs across the base layer, the above-mentioned monthly bf gap typically decreases by an average of about 80 meV to about 300 meV. In another specific complaint, In this case, the band gaps typically decrease by an average of about 10 meV to about 200 meV compared to the band gaps where GaAs crosses the base layer. This reduced band gap results in a GanIMShNy group with a composition hierarchy. The turn-on voltage (Vbe, ...) of the HBT of the electrode layer is lower than that of hBT with the base layer, because the main determinant in Vbeon is the intrinsic carrier concentration in the base. The intrinsic carrier concentration ( ni) is calculated by the following formula: ni = NcNvexp (-Eg / kT) In the formula above, Nc is a pass ..... w 匁 双 匁 反, text
共^貝能帶狀態的有效疼ί碎· P H At -Wt OB 曰、 J4度,Eg疋能帶間隙;T是溫度;而k 疋波錄又*數。從公式可以看出基極中的固有載子濃度大 大地受到用於基極中之材料的能帶間隙所控制。 將基極層的能帶間隙從基極—射極界面的較大能㈣ 隙T級到基極—集極界面的較小能帶間隙,此則引入了準 ,場,其使電子加速料_雙極電晶體中的基極層。電 場增加了基極中的電子速度,竑w 威v 了集極傳輸時間,此則 改善了 RF(radio frequency,射頻) 耵頭)表現以及增加了集極電 >瓜增益(也稱為dc電流增益)。在 UDrr 」在具有重摻雜之集極層的 HBT情況中,dc增益d)乃受 贼人』r性基極(η = 1)中的整 體再結合。dc «流增益可以由公式⑴來估計: /5 dc « ^ ^ /Wb 10 200308088 在公式⑴中,〉是基極中之次要載子的平均速度、 是基極中之次要載子的壽命;而Wb是基極的厚度。相較於 未分級的―基極層而言,將具有㈣㈣基極声之 謝中的基極層加以適當分級,由於增加電子速度料故 ,則導致石dc有顯著的增加。The effective state of the energy band state is broken. P H At -Wt OB, J4 degrees, Eg band gap; T is the temperature; and k 疋 wave record and * number. It can be seen from the formula that the intrinsic carrier concentration in the base is largely controlled by the band gap of the material used in the base. The band gap of the base layer is changed from the larger energy gap T of the base-emitter interface to the smaller band gap of the base-collector interface, which introduces a quasi-field, which makes the electrons accelerate _ Base layer in a bipolar transistor. The electric field increases the speed of the electrons in the base, 竑 w, vv, and the collector transmission time, which improves the performance of the RF (radio frequency), and increases the collector's gain (also called dc). Current gain). In the case of UDrr ”in HBT with a heavily doped collector layer, the dc gain d) is subject to the overall recombination in a thief’ r-type base (η = 1). dc «current gain can be estimated by formula ⑴: / 5 dc« ^ ^ / Wb 10 200308088 In formula〉,> is the average speed of the secondary carriers in the base, and is the secondary carrier's average speed in the base. Lifetime; and Wb is the thickness of the base. Compared with the ungraded-base layer, the base layer in the gravitational base sound is appropriately classified. Due to the increase of the electron velocity material, there is a significant increase in stone dc.
為了達成在基極層厚度上加以分級的能帶間隙,基極 層乃製備成在基極層的第—表面處(靠近集極)之銦和/或 氮的濃度要比在基極層的第二表面處(靠近射極)來得高。 銦和/或氮的含量變化最好是呈線性地變化越過基極層, 而造成線性分級的能帶間隙。摻雜物(例如碳)的濃度在整 個基極層中最好維持固定不變。在—具體態樣中,% xiMs卜Λ基極層(例如刪的基極層)乃分級成在集極處 X和3y大約等於〇. 〇卜而在射極處乃分級成X和打大約 等於零在另具體愁樣中,Gai_»hNy基極層從在基 極層與集極接觸的表面處χ值在大約02到大約⑽的範 圍,分級成在基極層與射極接觸的表面處χ值在大約0」 到零的範圍,前提是在基極層與集極接觸之表面處的χ值 要比在基極層與射極接觸的表面處來得大。在此具體態樣 中,y在整個基極層中可以維持固定不變,或者可以加以 線性分級。當y是線性分級時,基極層從在基極層與集極 接觸的表面處y值在大約〇· 2到大约〇. 〇2的範圍,分級成 在基極層與射極接觸的表面處y值在大約〇.丨到零的範圍 ,則提疋在基極層與集極接觸之表面處的y值要比在基極 層與射極接觸的表面處來得大。在一較佳的具體態樣中, 11 200308088 x在集極處大約是〇· 06,並且線性分級成在射極處的大約 〇· 01。在一更佳的具體態樣中,X在集極處大約是〇· 06, 並且線性分級成在射極處的大約〇〇1,同時y在整個基極 層中大約是0. 001。 在另一具體態樣中,本發明係一種形成分級之半導體 層的方法,此分級的半導體層從第一表面經過該層到第二 表面具有基本上線性分級的能帶間隙以及基本上固定不變 之摻雜X移動性的乘積。此方法包括: (a) 比較多個校正層的摻雜x移動性的乘積,其中每 一層係在沉積週期表之ΠΙ或V族原子的有機金屬化合物 或者沉積碳的四_化碳化合物當中任一者之明確區分的流 動速率下所形成,藉此決定形成基本上固定不變的摻雜χ 移動丨生乘積所需要之有機金屬化合物和四_化碳的相對流 動速率;以及 (b) 在該相對流動速率下,將有機金屬化合物和四齒 化碳化合物流動於一表面上,以形成基本上固定不變之摻雜 χ移動性的乘積,而在沉積期間改變該流動速率,藉此形成 在整個分級之半導體層中基本上呈線性分級的能帶間隙。 基極層也可以對摻雜物加以分級,如此使得靠近集極 的摻雜物濃度比較高,經過基極的厚度而逐漸減少到基極 一射極異質接合。 另一種使傳導能帶突峰達到最小的方法是在異質接合 處包括一或多個過渡層。可以採用具有低能帶間隙之挫折 (set back)層、分級能帶間隙層、摻雜突峰或其組合的過 12 200308088 渡層,來使傳導能帶突峰達到最小…卜,-或多個晶格 匹配層可以存在於基極和射極之間或者基極和集極之間, 以減少材料在異質接合處的晶格應變。 本^明也提供一種製造贿# DHBT的方法。此方法包 在η ^^雜的GaAs集極上長出由蘇、姻、石申和氮所組成 的基極層。基極層可以採用内部和,或外部的碳來源來成 長’以提供摻雜碳的基極層。然後在基極層上長出η型摻 雜的射極層。吏用内部和外部的碳來源以提供用於基極層 的碳摻雜物…幫助形成碳摻雜物濃度比較高的材料。 典型上’ I用本發明的方法達到大@ UxlO^W到大約 的摻雜物程度。纟—較佳的具體態樣中,以本 勺方法可以達到大約3 〇xl〇19cm_3到大約7·〇χ1〇19^3 :多雜物私度。材料中更高的摻雜物濃度會降低材料的片 =阻和^間隙。因此’ HBT和DHBT之基極層中的播雜物 /辰度愈面,則元件的打開電壓就愈低。 本發明也提供-種由化學式Gai xIMsi A所代表的材 4,其中X # y分別獨立地為大約i.㈣G_4到大約 Uxio'x最好大約等於3” "口 3y更好則是大約等於 .0卜在一具體態樣中,此材料乃摻雜以大約ΐ 5χΐ〇ΐ9Μ_3 到大約7.〇x1〇1W濃度的碳。在一特定的具體態樣中, 碳摻雜物的濃度是大約3.〇xl〇lw到大約7.〇χΐ〇ι^_3。 降低打開電射以對於基於GaAs之有線和無線rf電 路的電壓預算做更好的管理’該等電路乃受制於標準的固 定電壓供應或者受制於電池輸出。降低打開電產也可以改 13 200308088 變基於GaAs之HBT中之多種基極電流成分的相對大小。之 前已經顯示為接合溫度與施加應力兩者之函數的dc電流增 益穩定度’乃嚴重地依賴著基極電流成分的相對大小。低 的打開電壓所造成之逆向電洞注人的減少,係有利於元件 的溫度穩定度和長期可靠度。因&,具有高摻雜物濃度之 相對上’又有應、交的GaixInxAShNy基極材料可以顯著提昇 基於GaAs之HBT和DHBT的RF表現。 【實施方式】 從底下本發明之較佳具體態樣的更特定敘述,本發明 前述和其他的目的、特色和優點將會變得明顯,該等較佳 的具體態樣乃圖解說明於所附的圖式,其中相似的來考字 以指f同視圖中的相同部份。圖式未必是按照比㈣, 而是強調示範本發明的原理。 ΙΠ-ν族材料是晶格包括至少—種選自週㈣⑴⑴ 之X*素以及至種選自週期表V(A)攔之元素的半 。,一具體態樣中,IU-V族材料是一種包括録、錮、石申 和氮的晶格。ΗI - V族;γ ^材料好可以由化學式Gai_xIMsi_ χ θ更好則疋大約等於⑭。在-最佳的具體態樣 τ,X和3y是大約〇. 〇1。 在此所用的「過渡声 广 ·.In order to achieve a graded band gap in the thickness of the base layer, the base layer is prepared so that the concentration of indium and / or nitrogen at the first surface of the base layer (near the collector) is higher than that of the base layer. Comes high at the second surface (near the emitter). The content of indium and / or nitrogen is preferably changed linearly across the base layer, resulting in a linearly graded band gap. The concentration of dopants (e.g. carbon) is preferably maintained constant throughout the base layer. In a specific aspect, the% xiMs Λ base layer (for example, the deleted base layer) is classified into X and 3y at the collector, which is approximately equal to 0.00, and at the emitter, it is classified into X and approximately Equal to zero In another specific example, the Gai_ »hNy base layer ranges from a value of about χ to about ⑽ at the surface where the base layer is in contact with the collector, and is graded at the surface where the base layer is in contact with the emitter. The value of χ is in the range of about 0 ″ to zero, provided that the value of χ at the surface where the base layer is in contact with the collector is larger than at the surface where the base layer is in contact with the emitter. In this specific aspect, y can be kept constant throughout the base layer, or it can be linearly graded. When y is linearly graded, the base layer is graded into a surface in which the base layer is in contact with the emitter from a value in the range of about 0.2 to about 0.02 at the surface where the base layer is in contact with the collector. If the value of y is in the range of about 0.1 to zero, then the value of y at the surface where the base layer is in contact with the collector is greater than at the surface where the base layer is in contact with the emitter. In a preferred embodiment, 11 200308088 x is approximately 0.06 at the collector and linearly graded to approximately 0.01 at the emitter. In a better specific aspect, X is about 0.06 at the collector and linearly graded to about 0.001 at the emitter, while y is about 0.001 in the entire base layer. In another specific aspect, the present invention is a method for forming a graded semiconductor layer. The graded semiconductor layer has a substantially linear graded band gap from the first surface through the layer to the second surface and is substantially fixed. Instead, the product of X mobility is doped. This method includes: (a) comparing the dopant x mobility product of multiple correction layers, where each layer is selected from the group consisting of an organometallic compound of a III or V atom of the periodic table or a carbon tetracarbon compound of deposited carbon; One is formed at a clearly differentiated flow rate, thereby determining the relative flow rates of the organometallic compound and carbon tetraoxide required to form a substantially constant doped χ shift product; and (b) in At this relative flow rate, an organometallic compound and a tetradentate carbon compound are flowed on a surface to form a substantially fixed product of doped χ mobility, and the flow rate is changed during deposition, thereby forming There is a substantially linearly graded band gap in the entire graded semiconductor layer. The base layer can also grade the dopants, so that the concentration of the dopants near the collector is relatively high, and gradually decreases to the base-emitter heterojunction through the thickness of the base. Another way to minimize conduction band spikes is to include one or more transition layers at the heterojunction. A set back layer with a low band gap, a graded band gap layer, a doped spike, or a combination thereof can be used to minimize the conduction band spikes ...…, or more A lattice matching layer may exist between the base and the emitter or between the base and the collector to reduce the lattice strain of the material at the heterojunction. Ben Ming also provides a method of making bribe # DHBT. This method includes growing a base layer consisting of Su, Yin, Shishen, and Ni on a GaAs collector that is heterogeneous. The base layer can be grown using internal and external carbon sources to provide a carbon-doped base layer. An n-doped emitter layer is then grown on the base layer. Internal and external carbon sources are used to provide carbon dopants for the base layer ... to help form materials with a higher concentration of carbon dopants. Typically, the method of the present invention achieves a large dopant level of about UxlO ^ W to about.纟 —In a preferred embodiment, this method can achieve about 30 × 1019cm_3 to about 7.0 × 1019 ^ 3: the privacy of multiple debris. Higher dopant concentrations in the material will reduce the sheet resistance and gap of the material. Therefore, the higher the surface area of the impurities / chronicity in the base layer of 'HBT and DHBT, the lower the turn-on voltage of the device. The present invention also provides a material 4 represented by the chemical formula Gai xIMsi A, where X # y is independently about i. ㈣G_4 to about Uxio'x is preferably approximately equal to 3 "" port 3y is more preferably approximately equal to .0 In a specific aspect, the material is doped with carbon at a concentration of about ΐ5χΐ〇ΐ9Μ_3 to about 7.0x101W. In a specific embodiment, the concentration of the carbon dopant is about 3.〇xl0lw to about 7.〇χΐ〇ι ^ _3. Lower the power of the radio to better manage the voltage budget of GaAs-based wired and wireless RF circuits. These circuits are subject to standard fixed voltage Supply or subject to battery output. Lowering the power generation can also be changed. 13 200308088 Changing the relative size of various base current components in HBT based on GaAs. The dc current gain has been shown to be stable as a function of both junction temperature and applied stress. 'Degree' is heavily dependent on the relative size of the base current component. The reduction in reverse hole injection caused by the low turn-on voltage is conducive to the temperature stability and long-term reliability of the device. Because of & Debris concentration Relatively speaking, the corresponding GaixInxAShNy base material can significantly improve the RF performance of GaAs-based HBT and DHBT. [Embodiment] From the more specific description of the preferred embodiment of the present invention, the foregoing and other aspects of the present invention The purpose, features, and advantages of this will become apparent. The better specific aspects are illustrated in the attached drawings, where similar words are used to refer to the same parts in the same view. The drawings may not be It is based on the ratio ㈣, but emphasizes the principle of exemplifying the present invention. The materials of group ΙΠ-ν are crystal lattices including at least one X * prime selected from Zhou Yi and half of the elements selected from V (A) of the periodic table. In a specific aspect, the IU-V group material is a crystal lattice including 录, 锢, Shishen, and nitrogen. Η Group I-V; γ ^ The material can be better by the chemical formula Gai_xIMsi_ χ θ is better, ⑭ is approximately equal to ⑭ . In-the best specific aspect τ, X and 3y is about 〇1. The "transition sound is wide ..."
之 的 曰 j (transitional layer)—詞 指介於基極/射極異質接合 ° 、之間或基極/集極異質接合 間的層,並且且右佶里暂拉 、有使八貝接合之傳導能帶突峰達到最小 14 200308088 二ί =達到最小的-種方法是使㈣列 帶間二:最:=!/集極的異質接合_,過渡層的能 、”:、類m 層逐漸減低到最靠近基極的過 〜層類似地’在射極/基極的異質接合 =隙=近射極的過渡層逐漸減低到最靠近::: 渡層。使傳導能帶突峰達到最小的另一種 分級之能帶間隙的過渡層。過 ’①吏用”有 ♦ u此 段增的此咿間隙可以藉由將 物濃度加以分級而分級。舉例而言,過 可以在接近基極處較高,而在接近集極或射極處 逐漸地降低。另外可以選擇的是使用晶格應變,以提供且 有分級之能帶間隙的過渡層。舉例來說,過渡層可以在:且 成上加以分級,以使接觸基極的表面有最小的晶格應變, 而增加接觸集極或射極之表面的晶格應變。使傳導能帶突 峰達到最小的另-種方法是使用具有摻雜物濃度突峰的過 渡層。使傳導能帶突峰達到最小的上述一或多種方法可以 用於本發明的ΗΒΤβ適合本發明之ΗΒΤ的過渡層包括 、InGaAs 和 InGaAsN 〇 晶格匹配層是長在具有不同晶格常數之材料上的一層 。晶格匹配層典型上的厚度為大約5〇〇人或更小,並且^ 本上符合底下層的晶格常數。如果晶格匹配材料沒有應變 ,則此導致介於底下層的能帶間隙和晶格匹配材料的能帶 間隙之間的能帶間隙。形成晶格匹配層的方法乃熟於此技 藝者所已知的,並且可以見於Ferry等人之「砷化鎵科技 」(Gallium Arsenide Technology)的第 303〜328 頁(1985 15 200308088 年,印第安那州Indianapolis的Howard W· Sams股份有 限公司出版),其所教導的併於此以為參考。適合本發明 之晶格匹配層的一個材料範例是I nGaP。 組成之基極層的HBT和DHBT 本發明的HBT和DHBT可以使用適當之金屬有機化學氣 相沉積(metal organic chemical vapor deposition , MOCVD)的磊晶成長系統來製備。M〇CVD磊晶成長系統的適 當範例為AIXTR0N 2400和AIXTR0N 2600平台。在以本發 明方法所製備的HBT和DHBT中,典型而言,在當場去除吸 附的氧化物之後可以成長未摻雜的GaAs緩衝層。舉例而言 ’包含高濃度之η型摻雜物(例如摻雜物濃度大約 lxl〇18cnr3到大約9χ1018αιΓ3)的次集極層可以在大約7〇(rc 的溫度下成長。具有低濃度之η型摻雜物(例如摻雜物濃度 大約5xl〇i5cm_3到大約5xl〇16cm-3)的集極層可以在大約7〇〇 c的溫度下成長於次集極層上。次集極和集極最好是 。次集極層典型的厚度為大約4000A到大約6000A,而集 極層典型的厚度為大約3000A到大約5000人。在一具體態 樣中,次集極和/或集極中的摻雜物是矽。 晶格匹配的InGaP穿隧層可以視需要選擇性地在典型 的成長條件下生長於集極上。晶格匹配層一般的厚度為大 約500A或更小,最好是大約200A或更小,並且其摻雜物 濃度為大約lxl〇16cnT3到大約lxl〇18cm-3。 一或多個過渡層可以視需要選擇性地在典型的成長條 件下生長於晶格匹配層上或集極上(如果沒有使用晶格匹 16 200308088 配層的話)。過渡層可以由n型摻雜的GaAs、n型摻雜的 InGaAs或η型摻雜的InGaAsN所製備。過渡層可以視需要 述擇性地在成分上或摻雜物上加以分級,或者可以包含摻 雜物的突峰。過渡層典型的厚度為大約75A到大約25A。 如果沒有使用晶格匹配層或過渡層,則在集極上成長摻雜 喊的InGaAsN基極層。 基極層是在低於大約750°C的溫度下成長,並且典型 上大約400Λ到大約1500Λ厚。在一較佳的具體態樣中, 基極層是在大約50(TC到大約60(TC的溫度下成長。摻雜碳 的InGaAsN基極層可以視需要選擇性地成長於過渡層上或 晶格匹配層上(如果沒有使用過渡層的話)。基極層可以使 用適當的鎵來源(例如三甲基鎵或三乙基鎵)、砷來源(例如 胂、三丁基胂或三甲基胂)、銦來源(例如三曱基銦)和氮來 源(例如氨或二曱基聯氨)來成長。偏好使用砷來源對鎵來 源的低莫耳比例。典型上,砷來源對鎵來源的莫耳比例是 小於大約3· 5。該比例更好是大約2· 〇到大約3· 0。調整氮 和銦來源的程度’以得到包括大約〇 〇1%到大約2〇%的銦和 大約0. 01%到大約20%的氮之材料。在一較佳的具體態樣中 ’基極層的銦含量是氮含量的大約三倍。在一更佳的具體 態樣中’銦含量是大約1%,而氮含量是大約0· 3%。在本發 明中,具有大約1.5xl〇19cm-3到大約7.〇xl019cnT3之高碳摻 雜物濃度的InGaAsN層,可以使用外部碳來源或有機金屬 來源(尤其是鎵來源)來獲得。外部碳來源的適當範例是四 漠化%。四氣化碳也是有效的外部碳來源。 17 200308088 在基極和射極之間可以視需要選擇性地由n型摻雜的 GaAs、η型摻雜的inGaAs或η型摻雜的InGaAsN長出一或 多個過渡層。在基極和射極之間的過渡層摻雜得比較輕( 例如大約5.〇xl〇15cnT3到大約5·〇χ1016αιΓ3),並且可以視 品要選擇性地包含摻雜物的突峰。過渡層最好是大約2 5人 到大約75Α厚。 射極層是在大約700°C的溫度下成長於基極上,或者 可以視需要選擇性地成長於過渡層上,並且典型上大約 400A到大約1500A厚。射極層例如包括inGap、Ai in(jap 或AlGaAs。在一較佳的具體態樣中,射極層包括InGap。 射極層可以η型摻雜成大約1· 0xl017cnr3到大約 9·0χ1017〇ιτ3的濃度。包含高濃度的n型摻雜物(例如大約 1.0xl018cnT3到大約9χ1018〇η-3^ GaAs的射極接觸層,可 以視需要選擇性地在大約70(TC的溫度下成長於射極上。 典型而言’射極接觸層是大約1 000A到大約2〇〇〇人厚。 具有漸進的銦組成和高濃度之η型摻雜物(例如大約 5xl〇i8cnr3到大約5xl〇19cm-3)的InGaAs層乃成長於射極接 觸層上。此層典型上大約400A到大約ιοοοΑ厚。 範例1 為了示範降低基極層之能帶間隙和/或使射極/基極 異質接合處之傳導能帶突峰達到最小的效果,比較了三種 不同之基於GaAs的雙極電晶體結構:GaAs射極/GaAs基 極的BJT、InGaP / GaAs的HBT以及本發明之InGaP / GalnAsN的DHBT。用於底下實驗的InGaP/GaInAsN训耵 18 200308088 的般代表結構乃圖解於圖1。由於基極和集極都是由 GaAs所形成,故在射極/基極界面處只有一個異質接合。J (transitional layer) —The word refers to the layer between the base / emitter heterojunction °, between, or between the base / collector heterojunction, and temporarily pulls the right side of the The peak of the conduction energy band reaches a minimum of 14 200308088. Two = The minimum is reached-a method is to make the inter-band two: the most: =! / Collector heterojunction_, the energy of the transition layer, ":, the m-like layer gradually The layer that is reduced to the closest to the base is similarly 'heterojunction at emitter / base = gap = near-emitter transition layer is gradually reduced to the nearest ::: crossing layer. Minimize the peak of conduction band Another kind of grading band gap transition layer. If you use this method, you can increase the gradual gap by grading the concentration of the material. For example, 过 can be higher near the base and gradually lower near the collector or emitter. Alternatively, a lattice strain can be used to provide a transition layer with graded band gaps. For example, the transition layer can be graded on the substrate to minimize the lattice strain on the surface contacting the base and increase the lattice strain on the surface contacting the collector or emitter. Another way to minimize the spikes in the conduction band is to use a transition layer with spikes in dopant concentration. One or more of the above methods for minimizing the peak of the conduction energy band can be used in the present invention. The BTT β suitable transition layers for the BTT of the present invention include InGaAs and InGaAsN. The lattice matching layer is grown on materials with different lattice constants. Layer. The lattice matching layer typically has a thickness of about 500 people or less and conforms to the lattice constant of the underlying layer. If the lattice matching material is not strained, this results in a band gap between the band gap of the underlying layer and the band gap of the lattice matching material. The method of forming the lattice matching layer is familiar to those skilled in the art and can be found on pages 303-328 of Gallium Arsenide Technology by Ferry et al. (1985 15 200308088, Indiana) Published by Howard W. Sams, Inc. of Indianapolis), which is taught and incorporated herein by reference. An example of a material suitable for the lattice matching layer of the present invention is InGaP. HBT and DHBT of the composed base layer The HBT and DHBT of the present invention can be prepared by using an appropriate epitaxial growth system of metal organic chemical vapor deposition (MOCVD). Suitable examples of MoCVD epitaxial growth systems are the AIXTR0N 2400 and AIXTR0N 2600 platforms. In HBT and DHBT prepared by the method of the present invention, typically, an undoped GaAs buffer layer can be grown after removing the adsorbed oxide on the spot. For example, a secondary collector layer containing a high concentration of an n-type dopant (eg, a dopant concentration of about 1 × 1018cnr3 to about 9 × 1018αιΓ3) can be grown at a temperature of about 70 ° (rc). The collector layer of a dopant (eg, a dopant concentration of about 5 × 10 5 cm_3 to about 5 × 10 16 cm-3) can be grown on the sub-collector layer at a temperature of about 700 ° C. The sub-collector and the collector are most Well, the typical thickness of the secondary collector layer is about 4000A to about 6000A, and the typical thickness of the collector layer is about 3000A to about 5000 people. In a specific aspect, the secondary collector and / or the dopant in the collector are The impurity is silicon. The lattice-matched InGaP tunneling layer can be selectively grown on the collector under typical growth conditions as needed. The thickness of the lattice-matching layer is generally about 500 A or less, preferably about 200 A or less. It is smaller, and its dopant concentration is about 1x1016cnT3 to about 1x1018cm-3. One or more transition layers can be selectively grown on the lattice matching layer or the collector under typical growth conditions as needed (If not using Lattice 16 200308088 ). The transition layer can be prepared from n-doped GaAs, n-doped InGaAs, or n-doped InGaAsN. The transition layer can be selectively graded on the composition or dopant as required, or Can contain spikes of dopants. The typical thickness of the transition layer is about 75A to about 25A. If no lattice matching layer or transition layer is used, the doped InGaAsN base layer is grown on the collector. The base layer is Grows at a temperature below about 750 ° C, and is typically about 400Λ to about 1500Λ thick. In a preferred embodiment, the base layer is grown at a temperature of about 50 ° C to about 60 ° C The carbon-doped InGaAsN base layer can be selectively grown on the transition layer or the lattice matching layer (if no transition layer is used). The base layer can use an appropriate gallium source (such as trimethylgallium) Or triethylgallium), arsenic sources (such as europium, tributylphosphonium, or trimethylphosphonium), indium sources (such as trifluorenylindium), and nitrogen sources (such as ammonia or difluorenylhydrazine). Use a low molar ratio of arsenic source to gallium source. In type, the molar ratio of the arsenic source to the gallium source is less than about 3.5. The ratio is more preferably about 2.0 to about 3.0. The degree of nitrogen and indium sources is adjusted to include about 0.01% To about 20% indium and about 0.01% to about 20% nitrogen. In a preferred embodiment, the 'base layer's indium content is about three times the nitrogen content. In a more preferred embodiment In a specific aspect, the content of indium is about 1%, and the content of nitrogen is about 0.3%. In the present invention, the high carbon dopant concentration of about 1.5x1019cm-3 to about 7.0xl019cnT3 The InGaAsN layer can be obtained using an external carbon source or an organic metal source (especially a gallium source). A suitable example of an external carbon source is% desertification. Tetragasified carbon is also an effective external carbon source. 17 200308088 One or more transition layers can optionally be grown between the base and the emitter from n-doped GaAs, n-doped inGaAs, or n-doped InGaAsN, as needed. The transition layer between the base and the emitter is relatively lightly doped (for example, about 5.0x1015cnT3 to about 5.0x1016αι3), and it can be seen that the dopants are selectively included in the spikes. The transition layer is preferably about 25 to about 75A thick. The emitter layer is grown on the base at a temperature of about 700 ° C, or can be selectively grown on the transition layer as needed, and is typically about 400A to about 1500A thick. The emitter layer includes, for example, inGap, Ai in (jap, or AlGaAs. In a preferred embodiment, the emitter layer includes InGap. The emitter layer may be n-type doped to about 1.0 × 1017cnr3 to about 9.0 × 1017〇ττ3 The concentration of the emitter contact layer containing a high concentration of n-type dopants (for example, about 1.0 × 1018cnT3 to about 9 × 1018〇η-3 ^ GaAs can be selectively grown on the emitter at a temperature of about 70 ° C. if necessary The 'emitter contact layer is typically about 1000 A to about 2000 people thick. It has a progressive indium composition and a high concentration of n-type dopants (eg, about 5x10i8cnr3 to about 5x1019cm-3) The InGaAs layer is grown on the emitter contact layer. This layer is typically about 400A to about ιοοοΑ thick. Example 1 To demonstrate the reduction of the band gap of the base layer and / or the conduction energy of the emitter / base heterojunction The peak effect is minimized, and three different GaAs-based bipolar transistor structures are compared: GaAs emitter / GaAs base BJT, InGaP / GaAs HBT, and the InGaP / GalAsAs DHBT of the present invention. It is used below Experimental InGaP / GaInAsN Training 18 200308088 Representative is the general structure illustrated in Figure 1. Since the base and collector electrodes are formed of GaAs, so that only a heterojunction at the emitter / base interface.
InGaP/GaAs HBT之GaAs基極層的能帶間隙要比InGap/ GalnAsN DHBT的基極層來得大。由於GaAs/ GaAs bjt的射 極、集極和基極都是由GaAs所做的,故其沒有異質接合。 所以使用GaAs BJT結構做為參考,以決定基極/射極界面 處的傳導能帶突峰對於InGaP/GaAs HBT的集極電流特性 有何衝擊(如果有的話)。在圖i的DHBT中,係選擇hG# 做為射極,而基極為Gai xInxAsi yNy,此乃因為InGap的能 帶間隙很寬,並且其傳導能帶對齊於GaiXA基極 的傳導能帶。圖 1 之 inGaP / GaInAsN DHBT 和 InGaP / GaAs HBT的比較係用於決定具有較低能帶間隙的基極層對於集 極電流密度的效應。 用於底下討論的GaAs元件都具有以M0CVD長出之摻雜 碳的基極層,其中摻雜物濃度從大約15xl〇19cnr3變化到 大約6·5χ1019cnr3,而厚度從大約500人變化到大約15〇〇入 ’以致基極片電阻(Rsb)在1〇〇Ω/□到4〇〇ω/□之間。大 面積元件(L=75 // mx75 // m)乃使用簡單的溼式蝕刻法來製造 ’並且在共同的基極架構中測試。逐量添加比較少量的銦 (X〜1%)和氮(y〜0· 3%),以形成兩組不同的InGaP / GainAsN DHBT。每一組的成長都已最佳化,以維持高而均勻的碳摻 雜物程度(>2.5><1019cnr3)、良好的移動性(〜85 cm2/V-s)以 及高的dc電流增益(Rsb〜30〇ω/□時乃>6〇)。The band gap of the GaAs base layer of InGaP / GaAs HBT is larger than that of the base layer of InGap / GalnAsN DHBT. Since the emitter, collector, and base of GaAs / GaAs bjt are made of GaAs, there is no heterojunction. Therefore, the GaAs BJT structure is used as a reference to determine the impact of the conduction band spike at the base / emitter interface on the collector current characteristics of the InGaP / GaAs HBT (if any). In the DHBT in Figure i, hG # is selected as the emitter and the base is Gai x InxAsi yNy. This is because the band gap of InGap is wide and its conduction band is aligned with the conduction band of the GaiXA base. The comparison between inGaP / GaInAsN DHBT and InGaP / GaAs HBT in Figure 1 is used to determine the effect of the base layer with lower band gap on the collector current density. The GaAs elements used for the discussion below all have a base layer of doped carbon grown by MOCVD, where the dopant concentration varies from about 15 × 1019cnr3 to about 6.5 × 1019cnr3, and the thickness varies from about 500 people to about 15 °. 〇 入 ′ so that the base sheet resistance (Rsb) is between 100Ω / □ to 400ω / □. Large-area components (L = 75 // mx75 // m) are fabricated using a simple wet etch method and tested in a common base architecture. A relatively small amount of indium (X ~ 1%) and nitrogen (y ~ 0.3%) are added one by one to form two different sets of InGaP / GainAsN DHBT. The growth of each group has been optimized to maintain a high and uniform carbon dopant level (> 2.5 > < 1019cnr3), good mobility (~ 85 cm2 / Vs), and high dc current gain (Rsb ~ 30〇ω / □ when it is > 6〇).
繪製具有相當的基極片電阻之GaAs / GaAs BJT、InGaP 19 200308088 / GaAs HBT 以及 InGaP / GalnAsN DHBT 的典型 Gummel 圖, 並且重疊於圖 2。InGaP/GaAs HBT 和 GaAs/GaAs BJT 的 集極電流在超過電流的五個數量級(五個1 〇)都是無法分辨 的,直到有效串聯電阻的差異影響到電流一電壓特性為止 。另一方面,InGaP / GalnAsN DHBT的集極電流在很廣的偏 壓範圍中是GaAs / GaAs BJT和InGaP / GaAs HBT的兩倍, 此對應於1·78 A/cm2的集極電流密度(jc)下的打開電壓減 少了 25.0mV。BJT中之低偏壓基極電流(n=2成分)所觀察 到的增加,乃與能帶間隙所驅動之空間電荷再結合的增加 一致。InGaP / GalnAsN DHBT中之集極電流的中性基極再結 合成分被驅動成高於InGaP / GaAs HBT,此乃因為集極電 流有所增加,以及次要載子壽命有所降低或者載子速度 (Inb,Icwb/ u r)有所增加。以迄今所製備的InGap /Draw typical Gummel diagrams of GaAs / GaAs BJT, InGaP 19 200308088 / GaAs HBT, and InGaP / GalnAsN DHBT with equivalent base sheet resistance, and overlay them in Figure 2. The collector currents of InGaP / GaAs HBT and GaAs / GaAs BJT are indistinguishable by more than five orders of magnitude (five 10) until the difference in effective series resistance affects the current-voltage characteristics. On the other hand, the collector current of InGaP / GalnAsN DHBT is twice that of GaAs / GaAs BJT and InGaP / GaAs HBT in a wide bias range, which corresponds to a collector current density of 1.78 A / cm2 (jc The on voltage at) is reduced by 25.0mV. The observed increase in the low-bias base current (n = 2 component) in BJT is consistent with the increase in recombination of the space charge driven by the band gap. The neutral base recombination component of the collector current in InGaP / GalnAsN DHBT is driven higher than InGaP / GaAs HBT because the collector current is increased and the secondary carrier life is reduced or the carrier speed is reduced. (Inb, Icwb / ur) increased. InGap /
GalnAsN DHBT元件而言,基極片電阻為234Ω/□的元件已 經達到68的尖峰dc電流增益,此對應於打開電壓有 11· 5mV的降低,而基極片電阻為303 Ω/□的元件已經達到 66的尖峰dc電流增益,此對應於打開電壓有25 〇mV的降 低。對於這幾種結構而言,此代表了已知最高的增兴對美 〇.3)〇0&1.χΙηχΑδιθγΝ^; 的能帶間隙降低是觀察到之打開電壓降低的原因,士 (77。〇發光所示範的。DCXRD測量顯示基極芦 ° _咖 曰日日格不匹 配是最小的(<250arcsec)。 在普及的限制中’以基極一射極電壓(v 、炎 be )為函數之攀 極電晶體的理想集極電流密度可以近似為: (2) 200308088For GalnAsN DHBT components, components with a base sheet resistance of 234 Ω / □ have reached a peak dc current gain of 68, which corresponds to a decrease in the turn-on voltage of 11.5 mV, while components with a base sheet resistance of 303 Ω / □ have A peak dc current gain of 66 is reached, which corresponds to a reduction of 25 mV of the turn-on voltage. For these several structures, this represents the highest known boost to the United States 0.3) 0 & 1.χΙηχΑδιθγN ^; The decrease in the band gap is the reason for the decrease in the opening voltage observed, J. (77. 〇 Luminescence is demonstrated. DCXRD measurement shows that the base electrode has a minimum degree of mismatch (<250arcsec). In the limits of popularization, 'the base-emitter voltage (v, inflammation be) is The ideal collector current density of a function climbing electrode can be approximated as: (2) 200308088
Jc = (qDnn2ib/pbwb)exp(qVbe/kT) 其中Jc = (qDnn2ib / pbwb) exp (qVbe / kT) where
Pb和wb 基極搀雜和寬度;Pb and wb base doping and width;
Dn 擴散係數Dn diffusion coefficient
Rib 基極中的固有載子濃度 將nib表示成基極層能帶間隙(Egb)的函數,並且以基 極片電阻(Rsb)來改寫基極摻雜和寬度的乘積,則打開電^ 可以表示成基極片電阻的對數函數·· (3)The intrinsic carrier concentration in the Rib base represents nib as a function of the band gap (Egb) of the base layer, and the product of the base doping and width is rewritten with the base sheet resistance (Rsb). Logarithmic function expressed as base sheet resistance (3)
Vbe = -A ln(Rsb) + V( 而 A=(kT/q) (4) 以及 V〇=Egb/q-(kT/q)ln(q2// NcNvDn/Jc) (5) 其中Nc和Nv是傳導能帶和共價能帶中狀態的有效密度 ’而#是基極層中的主要載子移動性。 圖 3 繪出多個 inGaP / GaAs hbt、GaAs / GaAs BJT 和 InGaP / GalnAsN DHBT 當 Jc=l· 78 A/cm2 時以基極片電阻為 函數的打開電壓。InGaP / GaAs HBT和GaAs / GaAs BJT沒 有任何傳導能帶突峰,其打開電壓都定性地呈現對於基極 片電阻有著如方程式(2)所期望之相同的對數依存關係。定 量而言,基極一射極電壓(Vbj隨著基極片電阻的變化並不 如方程式(3)所代表的來得劇烈(a=〇. 〇i74mV,而非 〇· 0252mV)。然而,A所觀察到的降低乃與經過薄基極GaAs 雙極元件的準彈道(qUasiballistic)傳輸一致。 與GaAs / GaAs BJT的特性做比較所引出的結論是: InGaP / GaAs HBT之傳導能帶突峰的有效高度可以為零, 21 200308088 而集極電流展現理想的(n=1)行為。因此,InGaP / GaAs HBT可加以設計成基本上不具有傳導能帶突峰。之前對於 AlGaAs / GaAs ΗΒΤ的研究也發現類似的結果。為了進一步 降低這些元件在固定之基極片電阻下的打開電壓,則需要 使用具有較低能帶間隙而仍維持傳導能帶連續性的基極材 料。可以使用GahlrixAs^yNy來降低Egb,同時維持接近晶 格匹配的情況。如圖3所見,兩組InGaP / GaInAsN DHBT 的打開電壓遵循著對基極片電阻的對數依存關係,此顯示 傳導此▼犬峰大約為零。此外,相較於觀察的InGap / GaAs HBT和GaAs/ GaAs BJT而言,其中一組的打開電壓向 下位移了 11.5mV而另一組向下位移了 25 〇mV(兩虛線)。 上述實驗顯示基於GaAs之HBT的打開電壓可以使用 InGaP/GalnAsN DHBT結構而下降到低於GaAs BJT的打開 電壓。低的打開電壓係透過兩個關鍵步驟所達成的。藉由 選擇基極和射極半導體材料(其傳導能帶大約在相同的能 P白)而首先使基極一射極界面最佳化,以抑制傳導能帶 突峰。此乃使用InGaP或AlGaAs做為射極材料和㈣做 為基極材料而成功地做到。然後藉由降低基極層的能帶間 隙而使打_進一步地降低。此乃藉由添加銦和氮兩者 至基極層而達成,同時仍然維持整個聰結構的晶格匹配 。以適當的成長參數可以做到使集極電流密度增加兩倍, 而不會顯著犧牲基極摻雜或次要載子的壽命(υ4Ω/口 日Μ -一68)。這些結果顯示制Gai JMsi—Α材料提供了一 種降低基於GaAs # ΗΒΤ和DHBT之打開電屢的方法。由於 22 200308088 在GaAs中併入銦和氮降低了材料的能帶間隙,則較大百分 比的銦和氮加入基極中,如果維持高的p型摻雜濃度,可 期望基於GaAs之HBT和DHBT的打開電壓有較大的降低。Vbe = -A ln (Rsb) + V (and A = (kT / q) (4) and V〇 = Egb / q- (kT / q) ln (q2 // NcNvDn / Jc) (5) where Nc and Nv is the effective density of states in the conduction and covalent energy bands, and # is the major carrier mobility in the base layer. Figure 3 plots multiple inGaP / GaAs hbt, GaAs / GaAs BJT, and InGaP / GalnAsN DHBT When Jc = l · 78 A / cm2, the opening voltage is a function of the resistance of the base sheet. InGaP / GaAs HBT and GaAs / GaAs BJT do not have any conduction band spikes, and their opening voltages are qualitatively exhibited for the base sheet resistance. Has the same log-dependent relationship as expected by equation (2). Quantitatively, the change in base-emitter voltage (Vbj with the resistance of the base sheet is not as dramatic as represented by equation (3) (a = 〇 〇i74mV instead of 0.252mV). However, the reduction observed by A is consistent with the quasi-ballistic (qUasiballistic) transmission through a thin base GaAs bipolar element. It is derived from a comparison with the characteristics of GaAs / GaAs BJT The conclusion is: the effective height of the conduction band spike of InGaP / GaAs HBT can be zero, 21 200308088 and the collector current shows ideal (n = 1 ) Behavior. Therefore, InGaP / GaAs HBT can be designed to have substantially no conduction band spikes. Previous studies on AlGaAs / GaAs ΗΒΤ also found similar results. In order to further reduce these components under fixed base sheet resistance Turn-on voltage, you need to use a base material with a lower band gap and still maintain the continuity of the conduction band. GahlrixAs ^ yNy can be used to reduce Egb while maintaining close to lattice matching. As seen in Figure 3, two The turn-on voltage of the group InGaP / GaInAsN DHBT follows the logarithmic dependence on the resistance of the base sheet, which shows that the conduction can be approximately zero. In addition, compared to the observed InGap / GaAs HBT and GaAs / GaAs BJT, The turn-on voltage of one group was shifted down by 11.5mV and the other group was shifted by 25 mV (two dashed lines). The above experiments show that the turn-on voltage of HBT based on GaAs can be reduced to below using the InGaP / GalnAsN DHBT structure. GaAs BJT turn-on voltage. The low turn-on voltage is achieved through two key steps. By selecting the base and emitter semiconductor materials (the conduction band of At the same energy (P white), first optimize the base-emitter interface to suppress the conduction band spikes. This is successfully done using InGaP or AlGaAs as the emitter material and plutonium as the base material. Here. Then, by reducing the band gap of the base layer, the hitting is further reduced. This is achieved by adding both indium and nitrogen to the base layer while still maintaining the lattice matching of the entire Satoshi structure. With proper growth parameters, it is possible to triple the collector current density without significantly sacrificing the base doping or the lifetime of the secondary carriers (υ4Ω / port M-68). These results show that making Gai JMsi-A materials provides a way to reduce the turn-on time based on GaAs # ΗΒΤ and DHBT. Since 22 200308088 incorporation of indium and nitrogen in GaAs reduces the band gap of the material, a larger percentage of indium and nitrogen is added to the base. If high p-type doping concentrations are maintained, HBT and DHBT based on GaAs can be expected There is a large decrease in the turn-on voltage.
GalnAsN基極的能帶間隙降低乃假設是觀察到之打開 電壓降低的原因,已經由低溫(77。趵發光所確認。圖4比 較 InGaP/GalnAsN DHBT 和傳統的 InGaP/GaAs Ηβτ 的發 光光譜。來自InGaP/ GaAs HBT的基極層訊號是在比集極 還要低的能量(1.455eV對1.507eV),此係因為高摻雜程度 所帶來的能帶間隙窄化效應所致。來自InGaP / GaInAsN DHBT的基極層訊號出現在L 408eV已被降低了,此係因為 此帶間隙窄化效應以及基極層中加入銦和氮所引起的基極 層能帶間隙降低所致。在此比較中,摻雜程度是相當的, 而相較於GaAs基極的能帶間隙而言,此建議基極層訊號位 置有47meV的降低可以相當於GalnAsN基極的基極層能帶 間隙降低。此發光訊號的位移與測得打開電壓降低45mv關 聯得很好。在沒有傳導能帶突峰的情形下,打開電壓的降 低可以直接關聯於基極層能帶間隙的降低。The decrease in the band gap of the GalnAsN base is assumed to be the cause of the observed decrease in the opening voltage, which has been confirmed by the low temperature (77. Erbium luminescence. Figure 4 compares the emission spectra of InGaP / GalnAsN DHBT and the traditional InGaP / GaAs Ηβτ. From The base layer signal of InGaP / GaAs HBT is at a lower energy than the collector (1.455eV vs. 1.507eV), which is due to the narrowing effect of the band gap caused by the high doping level. From InGaP / The signal of the base layer of GaInAsN DHBT appearing at L 408eV has been reduced, which is due to the band gap narrowing effect and the reduction of the base layer band gap caused by adding indium and nitrogen to the base layer. Compare here However, compared with the band gap of the GaAs base, a reduction of 47 meV in the signal position of the base layer can be equivalent to the reduction of the band gap of the base layer of the GalnAsN base. The displacement of the luminous signal correlates well with the measured decrease of the on-voltage of 45mv. In the absence of a conduction band spike, the decrease in the on-voltage can be directly related to the reduction of the band gap of the base layer.
圖5所示的DCXRD光譜示範了添加碳摻雜物和銦至 GaAs半導體的效應。圖5顯示來自inGaP / GaInAsN DHBT 以及相當基極厚度的標準InGaP/ GaAs HBT兩者的DCXRD 光譜。在InGaP / GaAs HBT中,基極層可看成是GaAs基板 尖峰之右手邊的肩部,大約對應於+ g〇 arcsec的位置,此 乃由於4x1 〇19cm-3的高濃度碳摻雜物所產生之拉伸應變的 緣故。由於添加了銦,此特別之InGaP / GaInAsN DHBT結 23 200308088 構的基極層尖峰是在—425 arcsec。一The DCXRD spectrum shown in Figure 5 demonstrates the effect of adding a carbon dopant and indium to a GaAs semiconductor. Figure 5 shows DCXRD spectra from both inGaP / GaInAsN DHBT and standard InGaP / GaAs HBT with equivalent base thickness. In InGaP / GaAs HBT, the base layer can be regarded as the shoulder on the right-hand side of the GaAs substrate spike, which corresponds to the position of + g〇arcsec. This is due to the high concentration of 4x1 〇19cm-3 carbon dopants. The resulting tensile strain. Due to the addition of indium, the base layer spike of this particular InGaP / GaInAsN DHBT junction 23 200308088 structure is at -425 arcsec. One
GalnAsN基極的尖峰仿罟日翩 ^ ,又 έ ,相關於 』的大峰位置疋錮、氮和碳濃度的函數 銦至GaAs則增加了壓縮應變, 〖、口 來補償之。 1兩者則以拉伸應變The peaks of the GalnAsN base are similar to 罟, and they are related to the position of the large peak 疋 锢, a function of nitrogen and carbon concentrations. Indium to GaAs increase the compressive strain, which is compensated for by the mouth. 1 both with tensile strain
當銦(和氮)加入摻雜碳的GaA ^ ^ ^ Λ 了、、再得回的Ρ型摻雜程 度,乃而要小心的成長最佳化。 ^ ^ α ^ J Λ田挪传的基極片電阻 和基極厚度值的組合來獲得有作用之摻雜程度的粗 。基極摻雜也可以藉由首先選擇性地_至基極層的 ’然後得M PGlarcm 口輪廊圖來加以確認。圖6比較When indium (and nitrogen) is added to the carbon-doped GaA ^ ^ ^ Λ, the P-type doping degree is returned, but the growth must be optimized carefully. ^ ^ α ^ J Λ The combination of the base sheet resistance and the thickness of the base plate to obtain a useful degree of doping. The base doping can also be confirmed by first selectively selecting ′ to the base layer and then obtaining the M PGlarcm port profile. Figure 6 comparison
GaAs基極層和GaInAsN基極層的此種p〇lar〇n c—v摻雜= 廓圖。在兩種情況中,摻雜程度超過了 3χ1〇19α_3。 π 圖7Α顯示另一種可選擇的DHBT結構,其具有固定組 成的GalnAsN基極層,該基極層在射極/基極和集極/基 極的接合之間採用過渡層。此外,在過渡層和集極之間ς 用晶格匹配的I nGaP穿隨層。Such p-laron c-v doping of the GaAs base layer and the GaInAsN base layer = profile. In both cases, the degree of doping exceeded 3 × 1019α_3. Figure 7A shows another alternative DHBT structure with a fixed composition GalnAsN base layer that uses a transition layer between the emitter / base and collector / base junctions. In addition, a lattice-matched InGaP penetrating layer is used between the transition layer and the collector.
AJLM成分級之基極層的DHBT 具有組成分級之基極層的DHBT中的所有層,可以類似 於具有固定組成之基極層的DHBT的方式成長,例外的是從 電晶體之一接合經過基極層到另一接合而做為分級能帶間 隙的基極層。舉例而言,如果沒有使用晶袼匹配層或過渡 層,則摻雜碳且能帶間隙分級的GalnAsN基極層可以長在 集極上。換雜碳且分級的(jalnAsN基極層可以視需要選擇 性地生長於過渡層上或晶袼匹配層上(如果沒有使用過渡 層的話)。基極層可以在低於大約750°C的溫度下成長,並 24 200308088 且典型上大約400A到大約1500A厚。在一具體態樣中, 基極層是在大約500°C到大約60(TC的溫度下成長。基極層 可以使用適當的鎵來源(例如三甲基鎵或三乙基鎵)、砷來 源(例如胂、二(二級丁基)胂或三甲基胂)、銦來源(例如三 甲基銦)和氮來源(例如氨、二甲基聯氨或三級丁基胺)來成 長。偏好使用砷來源對鎵來源的低莫耳比例。典型上,砷 來源對鎵來源的莫耳比例是小於大約3· 5。該比例更好是 大、、々2 · 0到大約3. 0。可以調整氮和銦來源的程度,以得 到其中III族元素是大約0·01%到大約2〇%的銦以及y族元 素是大約0.01%到大約20%的氮之材料。在一特定的具體態 樣中,III族元素銦的含量從基極/集極接合處的大約1〇% 到20%變化到基極/射極接合處的大約〇 〇1%到5%,並且V 族το素氮的含量基本上是固定在大約〇·3%。在另一具體態 樣中,基極層的銦含量是氮含量的大約三倍。如之前所討 論的具有固定組成之InGaAsN基極層,相信具有大約 1· 5χ10%πτ3到大約7· 〇xl〇19cm-3之高碳摻雜物濃度的 InGaAsN層除了鎵來源外還可以再使用外部碳來源(例如四 鹵化石反)來獲得。使用的外部碳來源例如可以是四溴化碳 。四氣化碳也是有效的外部碳來源。 由於當成銦來源氣體來使用的有機銦化合物對 InGaAsN基極層所貢獻之碳摻雜物的量,乃不同於當成鎵 來源氣體來使用的有機鎵化合物,故在成長基極層的期間 ,典型上會調整碳摻雜物來源氣體的流動速率,如此以於 組成分級之InGaAsN基極層中維持固定不變的碳摻雜濃度 25 200308088 。在一具體態樣中,組成分級的基極層上之碳來源氣體的 流動速率變化乃使用底下所述的方法來決定。 —Μ名1nGaAsN和^半導體層的碏^ 士甲基銦來源流動速率之校正避序 。製備至少兩組校正用HBT,其中每—組包含至少兩個 成員(可以使用DHBT來代替HBT)。所有校正用Ηβτ的基極 層厚度理想上是相同的,但這並非一項要求,並且每一個 HBT具有固定不變的組成’例如固定組成# LAW或 MaAs基極層和在該層中都固定不㈣碳摻雜物濃度。每 一組是在不同於另-組的In或¥族添加物(例如⑴族用 銦! V族用氮)之來源氣體流動速率下成長,如此每一組的 成員具有不同於別組成員的鎵,、砷和氮組成。舉例來 :’採用銦做為影響能帶間隙分級的添加物。特定組的每 :個成員係於不同的外部碳來源(例如四漠化碳或四氣化 碳)流動速率下成長’所以特定組的每一個成員具有不同 的碳摻雜物程度。決定每-個成員之摻雜X移動性的乘積 蚀並且對碳來源的流動速率加以作圖。每一組之成員的摻 ” X移動性的乘積乃與碳來源氣體流動速率成比例地變化 。五組’之摻雜X移動性的乘積對四漠化碳的流動 乃緣於圖8。另外可以選擇的是每一組校正用ΗΒΤ或 由維持固定流動速率的碳來源氣體(例如四演化碳)而形^ :組中的個別樣品或可在相對於其他來源氣體的 -動速率下以不同Μ⑴族或V族添加物流動速率 26 200308088 獲ί于固疋的換雜x移動性 來源氣體的流動速率,乃辞二積所需之奴來源氣體對於銦 劃-條線橫越圖8(例如一:=固定的摻雜x移動性乘積處 ^ 條千仃於X軸的線)來得到。此線 與:一組直?交又的地方則代表了當設於該組的銦來源氣 體f動速率時獲得此摻雜x移動性之乘積值所需的外部碳來 源流動速率。對於—固定之摻雜X移動性的乘積值而言,外 部碳來源流動速率對銦來源氣體流動速率則繪於圖9。不同 之摻雜X移動性的乘積可以相同方式緣出類似的線。 每個HBT的集極電流乃繪成基極-射極電M(Vbe)的函 數’並且所得曲線則與具有GaAs基極層而其他皆盥:所比 較的該組成員相同t HBT(例如具有相同的摻雜物濃度、相 同的基極、射極和集極層厚度...等等)的圖形做比較。在 特定集極電流4 @曲線之間的電壓差別是基極—射極電壓 vbe的改變uvbe),此乃歸因於基極層的形成期間所添加的 銦和氮所造成之基極層能帶間隙較低的緣故。圖丨〇顯示具 有GalnAsN基極層之HBT和具有GaAs基極層之HBT的集極 電流以vbe為函數的圖形。兩曲線之間所劃的水平箭頭是 △ Vbe。將所有組別的每個成員的△ vbe加以決定,並對碳 來源氣體流動速率加以繪圖。用於形成圖8的五組HBT之 每一成員的△ Vbe對四溴化碳流動速率乃繪於圖u。注咅 到一組成員的△ vbe跨越了該組一範圍的△ Vbe,此範圍可 以找出最適合的直線。這些直線則用於決定(内插)或許可 使用特定組別的相同銦來源氣體流動速率但碳來源氣體# 動速率異於該組其他成員而成長之HBT的△ Vbe。 27 200308088 、、r骑:*疋之摻雜X移動性的乘積而言,係以銦來 體〜動速率為函數呈線性地變化,就如當固定之摻雜 移動性乘積的内插△ Vbe繪成銷來源氣體流動速率的函數 時所可以看到的。圖12顯示用於圖u之五組的此種圖形 圖12所示的@形乃用於決定在基極/射極和基極/集 =合,得到想要之△ L所需要的銦來源氣體流動速率。 —旦決定了銦來源氣體的流動速率,則使用圖9來決定在 此,來源*L體流動速率下所需的碳來源氣體流動速率,以 二得所要之摻雜物X移動性的乘積。依照相同的程序以決 疋在基極/集極接合處所要的銦來源氣體流動速率和碳來 源乳體流動速率,以於組成分級的GalnAs或GalnAsN層中 、隹持所要固疋的摻雜物x移動性乘積。當基極層從基極/ 集極接合成長至基極/射極接合時,銦來源氣體流動速率 和碳㈣氣體流動速率乃相對於鎵和珅的程度而線性地變 化到攻些接合處之這些來源氣體所決定的值,以獲得具有 所要之能帶間隙等級的線性分級基極層。 /、 範例2 用於底下討論的GaAs元件都具有以M0CVD長出之摻雜 奴的基極層,其中摻雜物濃度從大約3〇xl〇19cm_3變化到 大約5.〇xl〇i9cm_3,而厚度從大約5〇〇人變化到大約π⑽人 ,以致基極片電阻(RSb)在100Ω/□到650 Ω/□之間。大 面積元件(L=75 // mx75 /z m)乃使用簡單的溼式蝕刻法來製造 ,並且在共同的基極架構中測試。逐量添加比較少量的銦 28 200308088 (x〜1%到6%)和氮(y〜0· 3%),以形成兩組不同的/ GalnAsN DHBT。每一組的成長都已最佳化,以維持高&而均 句的碳換雜物程度(>2. 5xl〇i9cm-3)、良好的移動性(〜奶 cmVV-s)以及高的dc電流增益(Rsb〜300 Ω/□時乃>6〇)。用 於底下實驗而具有組成分級之GaInAsN基極層的dhbt結構 乃顯示於圖13。具有組成分級的基極層之另外可以選擇的 DHBT結構乃顯示於圖⑺和7C。用於底下實驗而具有固定 組成之GalnAsN基極層的DHBT結構乃顯示於圖14供比較 〇 圖15顯示具有相當的打開電壓和基極片電阻的固定基 極之DHBT和分級基極《DHBT的—圖。分級基極結^ 中之基極電流的中性基極成分乃顯著較低,其展現的尖峰 dc電流增益可以是固定基極結構的兩倍以上。圖16比較 類似而有厚度變化之固定和分級的麵結構以基極片電阻 為函數的dc電流增益。增益對基極片電阻的比例增加是很 明顯的。隸D腿之增线基極片電阻的比例乃視所用的 成長條件和整體結構的特定細節而定,但是已經觀察到且 有分級基極層之DHBT的dc電流增益要比具有固定基極層 之DHBT —致增加50%到1〇〇%。 圖17和18比較分級基極結構和兩個固定基極結構的AJLM composition-level base layer DHBT All layers in DHBT with a composition-graded base layer can be grown similar to DHBT with a fixed-layer base layer, with the exception of joining from one of the transistors through the base The electrode layer is bonded to another as the base layer of the graded band gap. For example, if a crystalline terbium matching layer or a transition layer is not used, a GalnAsN base layer doped with carbon and capable of band gap classification can be grown on the collector. Heterocarbon and graded (jalnAsN base layer can be selectively grown on the transition layer or crystal matching layer if not used). The base layer can be at a temperature below about 750 ° C It grows below 24 200308088 and is typically about 400A to about 1500A thick. In a specific aspect, the base layer is grown at a temperature of about 500 ° C to about 60 ° C. The base layer may use appropriate gallium Sources (such as trimethylgallium or triethylgallium), arsenic sources (such as thorium, di (secondary butyl) rhenium, or trimethylphosphonium), indium sources (such as trimethylindium), and nitrogen sources (such as ammonia , Dimethyl hydrazine or tertiary butyl amine) to grow. Prefer to use low molar ratio of arsenic source to gallium source. Typically, the molar ratio of arsenic source to gallium source is less than about 3.5. This ratio It is more preferably large, 々2 · 0 to about 3.0. The degree of nitrogen and indium sources can be adjusted to obtain a group III element in which about 0.01% to about 20% indium and a group y element are about 0.01% to about 20% nitrogen material. In a specific embodiment, the group III The content of elemental indium varies from about 10% to 20% of the base / collector junction to about 0.01% to 5% of the base / emitter junction, and the content of the V group το element nitrogen is basically It is fixed at about 0.3%. In another specific aspect, the indium content of the base layer is about three times the nitrogen content. As previously discussed, the InGaAsN base layer with a fixed composition is believed to have about 1.5 × 10 The InGaAsN layer with a high carbon dopant concentration from% πτ3 to about 7.0 × 1019 cm-3 can be obtained by using an external carbon source (such as tetrahalide inversion) in addition to the gallium source. The external carbon source used can be, for example, It is carbon tetrabromide. Tetragasified carbon is also an effective external carbon source. The amount of carbon dopants contributed to the InGaAsN base layer by the organic indium compound used as an indium source gas is different from that used as a gallium source gas. Organic gallium compounds to be used, so during the growth of the base layer, the flow rate of the carbon dopant source gas is typically adjusted, so that a constant carbon doping concentration is maintained in the composition-graded InGaAsN base layer 25 200308088. In one In the body shape, the change in the flow rate of the carbon source gas on the grading base layer is determined using the method described below. — Correction of the flow rate of the methyl indium source for the 1nGaAsN and semiconductor layers Prepare at least two sets of HBTs for calibration, each of which contains at least two members (DHBT can be used instead of HBT). The thickness of the base layer for all calibrations Ηβτ is ideally the same, but this is not a requirement. And each HBT has a fixed composition, such as a fixed composition # LAW or MaAs base layer and a fixed carbon dopant concentration in this layer. Each group is different from the other-group of In or ¥ Additives (such as indium for the Li family! Group V uses nitrogen) to grow at a source gas flow rate such that members of each group have gallium, arsenic, and nitrogen compositions that are different from those of other groups. For example: 'Indium is used as an additive that affects band gap classification. Each member of a particular group grows at a different external carbon source (such as four desertified carbon or four gasified carbon) at a flow rate ', so each member of a particular group has a different degree of carbon dopant. The product etch of the doping X mobility of each member is determined and the flow rate of the carbon source is plotted. The product of the doped X mobility of the members of each group changes in proportion to the flow rate of the carbon source gas. The flow of the doped X mobility of the five groups to the flow of the four desertified carbon is due to Figure 8. In addition, You can choose between each group of ΗΒΤ or shaped by a carbon source gas (such as tetragenetic carbon) that maintains a fixed flow rate ^: Individual samples in the group may be different at different dynamic rates relative to other source gases M⑴ or V additive flow rate 26 200308088 The flow rate of the heterogeneous x mobility source gas obtained from the solid source is the slave source gas required for the second product. The indium is drawn across the line-Figure 8 (for example One: = fixed doping x mobility product ^ line of thousands of lines on the X axis). This line is related to: a set of straight? Intersections represent the indium source gas f set in the set The external carbon source flow rate required to obtain the product of this doping x mobility at the dynamic rate. For the product of the fixed doping x mobility, the external carbon source flow rate is plotted against the indium source gas flow rate. Figure 9. Multiplication of different doped X mobility A similar line can be derived in the same way. The collector current of each HBT is plotted as a function of the base-emitter electricity M (Vbe) 'and the resulting curve is compared with a GaAs base layer and everything else: compared The members of the group are compared for graphs of the same t HBT (for example, with the same dopant concentration, the same base, emitter and collector layer thickness, etc.). The voltage difference is the change in the base-emitter voltage vbe (uvbe), which is due to the lower band gap of the base layer caused by the indium and nitrogen added during the formation of the base layer. Figure 丨 〇 shows The graph of the collector current of HBT with GalnAsN base layer and HBT with GaAs base layer is a function of vbe. The horizontal arrow drawn between the two curves is △ Vbe. △ vbe of each member of all groups Determine and plot the carbon source gas flow rate. The ΔVbe versus carbon tetrabromide flow rate used to form each member of the five groups of HBTs in Figure 8 is plotted in Figure u. Note the delta to a group of members vbe spans a range of △ Vbe in this group, this range can find the most suitable These straight lines are used to determine (interpolate) or allow the use of the same indium source gas flow rate for a particular group, but the carbon source gas # kinetic velocity differs from the other members of the group and grows △ Vbe. 27 200308088 、 r ride: the product of the doping X mobility of * 疋, linearly changes with the function of indium to the movement rate as a function of the interpolation of the fixed doping mobility product △ Vbe is plotted as the pin source It can be seen as a function of the gas flow rate. Figure 12 shows such a graph for the five groups of Figure u. The @shape shown in Figure 12 is used to determine the base / emitter and base / set = combination. To obtain the required indium source gas flow rate for the desired ΔL. -Once the flow rate of the indium source gas is determined, use Figure 9 to determine the flow rate of the carbon source gas at the source * L body flow rate, which is the product of the mobility of the desired dopant X. Follow the same procedure to determine the required indium source gas flow rate and carbon source emulsion flow rate at the base / collector junction, so that the composition-classified GalnAs or GalnAsN layer holds the dopants to be fixed. x mobility product. When the base layer grows from the base / collector junction to the base / emitter junction, the indium source gas flow rate and carbon hafnium gas flow rate change linearly with respect to the extent of gallium and thorium to the junctions. These source gases determine values to obtain a linear graded base layer with the desired band gap rating. /, Example 2 The GaAs elements used for the discussion below all have a doped base layer grown by M0CVD, where the dopant concentration is changed from about 30 × 1019 cm_3 to about 5.0 × 10 × 9 cm_3, and the thickness is From about 500 people to about π⑽ people, so that the base sheet resistance (RSb) is between 100Ω / □ to 650 Ω / □. Large-area components (L = 75 // mx75 / z m) are manufactured using a simple wet etch method and tested in a common base architecture. A relatively small amount of indium 28 200308088 (x ~ 1% to 6%) and nitrogen (y ~ 0.3%) were added in small amounts to form two different sets of / GalnAsN DHBT. The growth of each group has been optimized to maintain a high & uniform carbon exchange level (> 2.5xl0i9cm-3), good mobility (~ milk cmVV-s), and high Dc current gain (Rsb ~ 300 Ω / □ is> 6〇). The dhbt structure with a compositionally graded GaInAsN base layer used in the following experiments is shown in FIG. An alternative DHBT structure with a compositionally graded base layer is shown in Figures ⑺ and 7C. The DHBT structure of the GalnAsN base layer with a fixed composition used in the bottom experiment is shown in Fig. 14 for comparison. Fig. 15 shows the fixed base DHBT and the graded base DHBT with equivalent open voltage and base sheet resistance. —Figure. The neutral base component of the base current in the graded base junction is significantly lower, and the peak dc current gain it exhibits can be more than twice that of the fixed base structure. Figure 16 compares dc current gains of similar fixed and graded surface structures with varying thicknesses as a function of base sheet resistance. The increase in the ratio of the gain to the base sheet resistance is obvious. The ratio of the base line resistance of the increasing leg of the D leg depends on the growth conditions used and the specific details of the overall structure, but it has been observed that the dc current gain of DHBT with a hierarchical base layer is greater than that of a fixed base layer DHBT caused a 50% to 100% increase. Figures 17 and 18 compare the structure of a hierarchical base structure with two fixed base structures.
Gummel圖和增益曲線。第-個固定基極結構的基極組成對 應=分級基極在基射極接合處的基極層㈣。第二個 2疋基極結構的基極組成對應於分級基極在基極/集極接 合處的基極層組成。分級基極結構的打開電麼乃介於兩個 29 200308088 終點結構之間,不渦 、朝向基極/射極終點方向加權。分級 基極結構的dc電汸掷y, 一 9 a要比終點結構高出50%到95%,此 顯示&電流增益的大部分增加係來自於電子速度的增加。Gummel plot and gain curve. The base composition of the first fixed base structure corresponds to the base layer 分级 of the graded base at the base-emitter junction. The base composition of the second 2 疋 base structure corresponds to the base layer composition of the hierarchical base at the base / collector junction. The opening of the hierarchical base structure is between the two end structures, which are not vortexed and weighted towards the base / emitter end point. The dc electrical throw of the grading base structure is 9% higher than the end structure by 50% to 95%. This shows that most of the increase in the current gain is due to the increase in electron velocity.
使用HP 85l〇C參數分析器在2指、4/zrax4/zm射極面 積的το件上進彳了晶圓上的叮測試。使用斷路和短路結構去 除後埋的墊寄生,以及使用小訊號電流增益(則之— 20dB/10的斜率來外插電流增益的切斷頻率(卜)。圖η综 合了兩種結構上的ft與集極電流密度⑹的依附關係。圖 囷解說月了在肖定偏壓點下小訊號增益對頻率的關係 。隨著Jc增加以及基極過渡時間(η)開始在整個過渡時間 中扣/貝限制的角色,儘管分級基極結構的基極厚度較大( 固定不變的基極層是⑽⑽厚,而分級的基極層是8〇⑽厚) ,分級基極結構的ft仍變得顯著大於固定組成的結構。 60nm之固定組成GaInAsN基極的尖峰匕是53 GHz,而 80nm之組成分級GaInAsN基極的尖峰匕是6〇 GHz。因此, 電流增益的切斷頻率增加13 %。An HP 8510C parameter analyzer was used to perform a test on a wafer on a 2-fin, 4 / zrax4 / zm emitter area το piece. Use open and short structures to remove the buried pad parasitics, and use a small signal current gain (then — a slope of 20dB / 10 to extrapolate the cutoff frequency of the current gain (b). Figure η synthesizes ft on the two structures Dependence on the collector current density 。. Figure 囷 illustrates the relationship between the small signal gain and frequency under the Schottky bias point. As Jc increases and the base transition time (η) starts to deduct / In the restricted role, although the base thickness of the hierarchical base structure is relatively large (the fixed base layer is thicker and the hierarchical base layer is 80 thicker), the ft of the hierarchical base structure still becomes The structure is significantly larger than the fixed composition. The spike of the fixed composition GaInAsN base at 60nm is 53 GHz, and the spike of the graded GaInAsN base at 80nm is 60GHz. Therefore, the cutoff frequency of the current gain is increased by 13%.
為了好好比較具有固定和分級之GaInAsN基極層的 DHBT與傳統之GaAs HBT的RF結果,圖19的f t數值繪成 可以施加於電晶體之零輸入電流崩潰電壓(BU的函數。 此圖與引述文獻之傳統GaAs HBT的尖峰或近尖峰ft數值 做比較。預期傳統之GaAs HBT的ft數值分布相當廣,因 為此資料彙編自使用不同蠢晶結構、元件尺寸和測試條件 的許多組,並且只是要給出目前工業標準的概況。BVce。經 常必須由引述的集極厚度來估計,而假設有如圖21所示的 30 200308088 集極厚度(Xc)、BVcb◦和BVce◦之間的關係。亦如圖21所示 的疋ft對BVce〇之預期依存關係的三個簡單計算,其假設 經過集極之空間電荷層的過渡時間(r _)係藉由電子飽和 (飄移)速度(vs)而單純地關聯於人。在基線計算中,如同 :、〇A GaAs基極層之亂伯個。計算所預期的,“假 設為1.115 ps,並且剩餘之射極和集極過渡時間的總和( r e+τ c)則視為 〇·95 ps。 審視圖21顯示:雖然固定組成之的匕並未 完全位於傳統基於GaAs之體的預期範圍之外,不過其顯 然是在該分布的下端。分級的基極結構則有顯著的改:’。 第二個計算“b減少A 2/3的基線)建議:基極過渡時_ 對於固定組成的結構而言乃降低大約5⑽。相較於固定组 成的基極層而t,此顯示載子速度在分級的基極層中達到 兩倍的增加,此係因為載子速度的兩倍(2χ)增加配合基極 厚度增加的33%乃預期導出rb減少為1/2 χ 4/3 = 2/3。 第三個計算(…咸” 1/3以及(r,rc)減少為1/2的基 線)則近似出採用薄的和/或分級基極結構以及具有改呈 之7^件佈局和尺寸(以使…。和^達到最小)下的情形 範例3 為了改進放大器效率以及因而降低操作電壓和延長電 池壽命,故想要減低偏移電壓(VcEsat)和拐曲電壓⑹。減 低偏移電壓的一種方法是使基極/射極和基極/集極二極 體對之打開電壓的不對稱性㈣最小。_集極能 31 200308088 為寬的DHBT已經顯示可產生低# u,但是實際上此 導致較高的Vk並且降低效率,此乃因為難以控制基極/集 極異質接合處的位能阻障。 插入具有兩能帶間隙的薄層(穿隧集極),則允許同時 降低vCE,sat和vk,而改善了元件的效率。圖22顯示具有分 級的GalnAsN基極層和穿隧集極之DHBT的圖解。基極層係 分級成使得射極和集極接合之間在能帶間隙上有大約 40meV的能量差異。在基極和集極之間製出1〇〇人厚的穿隧 集極,其係由高能帶間隙材料A,。』所組成。圖心員 不圖22之DHBT的能帶間隙圖解。卯耵乃使用簡單的溼式 蝕刻法製成大面積元件(L=75〆 mx75" ,並且在共同的基 極和共同的射極架構中測試。圖24顯示其—圖,而 圖25顯示圖22之DHBT的共同射極特徵。如圖24和託所 可以看到的,元件具有大約〇.12V的低偏移電壓。 等效者 雖然已經參考較佳的具體態樣來特別顯示和描述本發 明,但是熟於此技藝者將理解到:在不偏離本發明由所附 申請專利範圍所包含的範圍之下,其中可以在型式和細節 上做出多種改變。 【圖式簡單說明】 (一)圖式部分 圖1圖解說明本發明之較佳具體態樣的InGaP / GalnAsN DHBT結構,其中X大約等於3y。 32 200308088 圖2是Gummel圖,其圖解說明對於本發明的InGaP/ GalnAsN DHBT 以及先前技藝的 InGaP/GaAs HBT 和 GaAs/ GaAs B JT而言,以打開電壓為函數的基極和集極電流。 圖3圖解說明對於本發明的InGaP/ GalnAsN DHBT以 及先前技藝的InGaP / GaAs HBT和GaAs / GaAs BJT而言, 以基極片電阻為函數的打開電壓(當Jc=1.78 A/cm2時)。 圖4圖解說明本發明的InGaP/GalnAsN DHBT以及先 前技藝的InGaP/GaAs HBT兩者在名義基極厚度1 000A、 77°K下所測量的發光光讀。#刻移掉InGaAs和GaAs覆蓋 層而選擇性地終止於InGaP射極頂端之後才進行發光測量 。InGaP/GaAs HBT 和 InGaP/ GalnAsN DHBT 兩者之 η 型 GaAs集極的能帶間隙為1. 507eV。InGaP / GaAs HBT之ρ型 GaAs基極層的能帶間隙為1. 455eV,而InGaP / GalnAsN DHBT之ρ型GalnAsN基極層的能帶間隙為1. 408eV。 圖5圖解說明本發明的InGaP/ GalnAsN DHBT以及先 前技藝的InGaP / GaAs HBT兩者在名義基極厚度1500A下 的雙重晶體 X 光繞射(double crystal x-ray diffraction ,DCXRD)光譜。基極層尖峰的位置有標示出來。 圖6是Polaron C-V輪廓圖,其圖解說明越過本發明 的 InGaP/ GalnAsN DHBT 以及先前技藝的 InGaP/GaAs HBT 中之基極層厚度的載子濃度。InGaP / GalnAsN DHBT以及 InGaP / GaAs HBT的名義基極厚度都是ΙΟΟΟΑ。選擇性地向 下餘刻到基極層頂端之後才得到兩者的Polaron輪廓。 圖7A圖解說明較佳的InGaP / GalnAsN DHBT結構,其 33 200308088 在射極和基極之間有過渡層,而扁隹 ^ ^ ^ 阳在集極和基極之間有過渡 層和晶格匹配層。 圖7B和7C圖解說明另外可以選擇的InGap/GaInAsN DHBT結構’其具有組成分級的基極層。 圖8是在固定不變之銦來源氣體流動速率下成長的摻 雜碳之GalnAsN基極層中,摻雜X移動性的乘積以四溴化碳 流動速率為函數的圖形(「TMIF」是三甲基銦的流動)。 圖9是獲得固定不變的摻雜)<移動性乘積而同時長出 才多雜奴之組成分級的GainAsN基極層所需要之if對四溴 化碳流動速率的圖形。 圖10疋顯示InGaP / GalnAsN HBT的打開電壓要比 InGaP / GaAs HBT來得低的圖形。 圖11是在固定不變之TMIF下成長的摻雜碳之 GalnAsN基極層中的△ Vbe對四溴化碳流動速率的圖形。 圖12是△ TMIF的圖形。 圖13是用於範例2的實驗而具有組成分級之基極層的 DHBT結構。 圖14是用於範例2的實驗而具有固定組成之基極層的 DHBT結構。 圖15是Gummel圖,其比較具有固定組成之GaInAsN 基極層的DHBT和具有組成分級之GalnAsN基極層的DHBT。 圖1 6是比較具有固定組成之GalnAsN基極層的dhbt 和具有組成分級之GalnAsN基極層的DHBT,其DC電流增 益以基極片電阻為函數的圖形。 34 200308088 圖17是Gummel圖,其比較具有組成分級之GalnAsN 基極層的DHBT和具有固定組成之GalnAsN基極層的兩個 DHBT。 圖18是比較具有組成分級之GalnAsN基極層的DHBT 和具有固定組成之GalnAsN基極層的兩個DHBT,其DC電 流增益以集極電流密度為函數的圖形。 圖19是比較具有固定組成之GalnAsN基極層的DHBT 和具有組成分級之GalnAsN基極層的DHBT,其外插電流增 益切斷頻率以集極電流密度為函數的圖形。 圖2 0是比較具有固定組成之G a I n A s N基極層的D Η B T 和具有組成分級之GalnAsN基極層的DHBT,其小訊號電流 增益以頻率為函數的圖形。 圖21是比較具有固定組成之GalnAsN基極層的DHBT 和具有組成分級之GalnAsN基極層的DHBT對於具有GaAs 基極層的傳統HBT而言,其尖峰f t以BVce。為函數的圖形 〇 圖22是顯示具有分級的GalnAsN基極層和穿隧集極之 DHBT的組成表。 圖23是圖22所述之DHBT的能帶間隙圖解。 圖24是圖22所述之DHBT的Gummel圖。 圖25顯示圖22所述之DHBT的共同射極特徵。 (二)元件代表符號 (無)In order to properly compare the RF results of DHBT with a fixed and graded GaInAsN base layer with traditional GaAs HBT, the ft value in Figure 19 is plotted as a function of the zero input current breakdown voltage (BU that can be applied to the transistor. This figure and quote The ft values of the traditional GaAs HBT are compared in the literature. The ft values of the traditional GaAs HBT are expected to be quite broad because this information is compiled from many groups using different stupid crystal structures, component sizes, and test conditions, and is only intended to Give an overview of current industry standards. BVce. Often must be estimated from the quoted collector thickness, assuming a relationship between 30 200308088 collector thickness (Xc), BVcb◦, and BVce◦ as shown in Figure 21. See also Three simple calculations of the expected dependence of 疋 ft on BVce0 shown in Figure 21 assume that the transition time (r _) through the space charge layer of the collector is pure by the electron saturation (drift) velocity (vs). Ground is related to people. In the baseline calculation, it is like:, 〇A GaAs base layer disorder. The calculation is expected, "assuming 1.115 ps, and the total of the remaining emitter and collector transition time (R e + τ c) is regarded as 0.95 ps. Examination view 21 shows that although the fixed composition of the dagger is not completely outside the expected range of the traditional GaAs-based body, it is clearly at the lower end of the distribution The graded base structure has a significant improvement: '. The second calculation "b reduces the baseline of A 2/3) Suggestion: When the base transition _ for a structure with a fixed composition is reduced by about 5⑽. Compared to the base layer with a fixed composition, t, this shows that the carrier speed has been increased twice in the graded base layer. This is because the carrier speed doubles (2χ) and the base thickness increases by 33. % Is the expected reduction in rb to 1/2 χ 4/3 = 2/3. The third calculation (... salty 1/3 and (r, rc) reduced to 1/2 baseline) approximates the use of a thin and / or hierarchical base structure and a modified layout and size of 7 ( In order to minimize the value of… and ^) Example 3 In order to improve the efficiency of the amplifier and thus reduce the operating voltage and extend the battery life, it is desirable to reduce the offset voltage (VcEsat) and the corner voltage ⑹. The method is to minimize the asymmetry 打开 of the turn-on voltage of the base / emitter and base / collector diode pairs. _ Collector Energy 31 200308088 Wide DHBT has been shown to produce low # u, but in fact this This results in higher Vk and reduced efficiency because it is difficult to control the potential barrier at the base / collector heterojunction. Insertion of a thin layer (tunneling collector) with a two-band gap allows simultaneous reduction of vCE, sat and vk, which improves the efficiency of the device. Figure 22 shows a diagram of a graded GalnAsN base layer and a tunneling collector DHBT. The base layer system is graded such that there is a band gap between the emitter and collector junctions There is an energy difference of about 40 meV. Between the base and collector A 100-thick-thick tunneling collector was made, which is composed of a high-band gap material A. ". The figure shows the band gap diagram of DHBT in Figure 22. The simple wet method is used. A large area element (L = 75〆mx75 < ") was made by etching, and tested in a common base and common emitter architecture. Figure 24 shows its graph, and Figure 25 shows the common emitter characteristics of the DHBT in Figure 22 As can be seen in Figure 24 and the drawing, the element has a low offset voltage of about 0.12V. Although the equivalent has been particularly shown and described with reference to the preferred specific aspects, the person skilled in the art is familiar with it It will be understood that, without departing from the scope of the present invention, which is encompassed by the scope of the appended patent application, various changes can be made in type and detail. [Simplified description of the drawings] (I) Schematic illustration of the drawings InGaP / GalnAsN DHBT structure of a preferred embodiment of the present invention, where X is approximately equal to 3y. 32 200308088 Figure 2 is a Gummel diagram illustrating the InGaP / GalnAsN DHBT of the present invention and the prior art InGaP / GaAs HBT and GaAs / GaAs B JT Base and collector currents as a function of turn-on voltage. Figure 3 illustrates the turn-on as a function of the resistance of the base sheet for the InGaP / GalnAsN DHBT of the present invention and the prior art InGaP / GaAs HBT and GaAs / GaAs BJT. Voltage (when Jc = 1.78 A / cm2). Figure 4 illustrates the luminescence of the InGaP / GalnAsN DHBT of the present invention and the InGaP / GaAs HBT of the prior art measured at a nominal base thickness of 1,000A and 77 ° K. read. #Etch the InGaAs and GaAs coatings and selectively terminate at the top of the InGaP emitter before measuring the luminescence. The band gap of the η-type GaAs collector of both InGaP / GaAs HBT and InGaP / GalnAsN DHBT is 1.507eV. The band gap of the p-type GaAs base layer of InGaP / GaAs HBT is 1. 455eV, while the band gap of the p-type GalnAsN base layer of InGaP / GalnAsN DHBT is 1. 408eV. Fig. 5 illustrates a double crystal x-ray diffraction (DCXRD) spectrum of the InGaP / GalAsAs DHBT of the present invention and the prior art InGaP / GaAs HBT at a nominal base thickness of 1500A. The location of the base layer spikes is indicated. Figure 6 is a Polaron C-V profile diagram illustrating the carrier concentration across the base layer thickness in the InGaP / GalnAsN DHBT of the present invention and the InGaP / GaAs HBT of the prior art. The nominal base thicknesses of both InGaP / GalnAsN DHBT and InGaP / GaAs HBT are 100 OA. The Polaron contours of the two were obtained after selectively etched down to the top of the base layer. FIG. 7A illustrates a better InGaP / GalnAsN DHBT structure. 33 200308088 has a transition layer between the emitter and the base, and 隹 ^ ^ ^ has a transition layer and a lattice match between the collector and the base. Floor. Figures 7B and 7C illustrate an alternative, InGap / GaInAsN DHBT structure ' having a compositionally graded base layer. Figure 8 is a graph of the product of doped X mobility in a carbon-doped GalnAsN base layer grown at a constant indium source gas flow rate as a function of carbon tetrabromide flow rate ("TMIF" is three Flow of methyl indium). Figure 9 is a graph of the flow rate of if-to-tetrabromide required for obtaining a GainAsN base layer with a graded composition of the mobility product while growing a heterogeneous dopant. Figure 10 (a) shows a graph in which the turn-on voltage of InGaP / GalnAsN HBT is lower than that of InGaP / GaAs HBT. FIG. 11 is a graph of the ΔVbe vs. carbon tetrabromide flow rate in a carbon-doped GalnAsN base layer grown under a fixed TMIF. Figure 12 is a graph of Δ TMIF. Fig. 13 is a DHBT structure having a composition-graded base layer used in the experiment of Example 2. Fig. 14 is a DHBT structure with a fixed base layer used in the experiment of Example 2. FIG. 15 is a Gummel diagram comparing a DHBT having a fixed composition GaInAsN base layer and a DHBT having a compositionally graded GalnAsN base layer. Figure 16 is a graph comparing the DC current gain of a dhbt with a fixed composition of the GalnAsN base layer and a DHBT with a compositionally graded GalnAsN base layer as a function of the base sheet resistance. 34 200308088 Figure 17 is a Gummel diagram comparing a DHBT with a compositionally graded GalnAsN base layer and two DHBTs with a fixed composition of the GalnAsN base layer. Figure 18 is a graph comparing the DC current gain of a DHBT with a GalnAsN base layer with a composition hierarchy and two DHBTs with a GalnAsN base layer with a fixed composition as a function of collector current density. Figure 19 is a graph comparing the extrapolated current gain cut-off frequency of a DHBT with a fixed composition of the GalnAsN base layer and a DHBT with a compositionally graded GalnAsN base layer as a function of the collector current density. Fig. 20 is a graph comparing the small signal current gain of the G a I n A s N base layer with a fixed composition to D Η B T with a compositionally graded GalnAsN base layer as a function of frequency. FIG. 21 is a comparison between the DHBT with a fixed composition of the GalnAsN base layer and the DHBT with a compositionally graded GalnAsN base layer. For a conventional HBT with a GaAs base layer, the peak f t is BVce. Graph as a function. Figure 22 is a table showing the composition of a DHBT with a hierarchical GalnAsN base layer and a tunneling collector. FIG. 23 is a diagram of a band gap of the DHBT described in FIG. 22. FIG. 24 is a Gummel diagram of the DHBT described in FIG. 22. FIG. 25 shows common emitter characteristics of the DHBT described in FIG. 22. (Two) the symbol of the component (none)
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| US10/121,444 US6847060B2 (en) | 2000-11-27 | 2002-04-10 | Bipolar transistor with graded base layer |
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| CN104900689B (en) * | 2015-06-08 | 2019-05-17 | 中国科学院半导体研究所 | Reduce the GaN base HBT epitaxial structure and growing method of base resistance rate |
| CN106653826B (en) * | 2016-12-26 | 2019-01-08 | 厦门市三安集成电路有限公司 | A kind of compound semiconductor heterojunction bipolar transistor |
| CN110649088A (en) * | 2019-09-30 | 2020-01-03 | 厦门市三安集成电路有限公司 | Epitaxial structure and low turn-on voltage transistors |
| CN114859200B (en) * | 2022-04-28 | 2024-04-12 | 西安唐晶量子科技有限公司 | Method for evaluating material characteristics of base layer of InGaP/GaAs HBT epitaxial wafer |
| CN116344585A (en) * | 2023-03-29 | 2023-06-27 | 绍兴中芯集成电路制造股份有限公司 | Heterojunction bipolar transistor and method of manufacturing the same |
| CN117116763B (en) * | 2023-10-25 | 2024-01-23 | 新磊半导体科技(苏州)股份有限公司 | Molecular beam epitaxial growth method of carbon doped HBT device |
| CN117766389B (en) * | 2023-12-26 | 2025-07-04 | 全磊光电股份有限公司 | Heterojunction bipolar transistor and MOCVD epitaxial growth method thereof |
Family Cites Families (4)
| Publication number | Priority date | Publication date | Assignee | Title |
|---|---|---|---|---|
| JP2000133654A (en) * | 1998-10-23 | 2000-05-12 | Furukawa Electric Co Ltd:The | Manufacturing method of bipolar transistor |
| JP2000223497A (en) * | 1999-01-28 | 2000-08-11 | Furukawa Electric Co Ltd:The | Heterojunction bipolar transistor and manufacturing method thereof |
| FR2795871B1 (en) * | 1999-07-01 | 2001-09-14 | Picogiga Sa | HETEROJUNCTION TRANSISTOR III-V, IN PARTICULAR HEMT FIELD-EFFECT TRANSISTOR OR BIPOLAR HETEROJUNCTION TRANSISTOR |
| CN1111313C (en) * | 1999-07-02 | 2003-06-11 | 北京工业大学 | Bipolar heterojunction transistor |
-
2003
- 2003-03-31 CN CNB038075970A patent/CN100448024C/en not_active Expired - Lifetime
- 2003-03-31 JP JP2003585186A patent/JP2005522883A/en active Pending
- 2003-03-31 AU AU2003223423A patent/AU2003223423A1/en not_active Abandoned
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Cited By (1)
| Publication number | Priority date | Publication date | Assignee | Title |
|---|---|---|---|---|
| US9397204B2 (en) | 2013-03-19 | 2016-07-19 | Murata Manufacturing Co., Ltd. | Heterojunction bipolar transistor with two base layers |
Also Published As
| Publication number | Publication date |
|---|---|
| JP2005522883A (en) | 2005-07-28 |
| AU2003223423A1 (en) | 2003-10-27 |
| CN100448024C (en) | 2008-12-31 |
| TWI288479B (en) | 2007-10-11 |
| CN1647281A (en) | 2005-07-27 |
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