A 22dB PSRR Enhancement in a Two-Stage CMOS Opamp Using Tail Compensation Paul M. Furth, Sri Harsh Pakala, Annajirao Garimella and Chaitanya Mohan VLSI Laboratory, Klipsch School of Electrical and Computer Engineering, New Mexico State University, Las Cruces, NM 88003, USA Email: pfurth@nmsu.edu, sriharsh@nmsu.edu, garimella@ieee.org Abstract— A new compensation technique known as tail compensation is applied to a two-stage CMOS operational amplifier. The compensation is established by a capacitor connected between the output node and the source node of the differential amplifier. For the selected opamp topology, tail compensation allows better performance in terms of bandwidth and power supply rejection ratio (PSRR) when compared to Miller and cascode compensation. Operational amplifiers using Miller, cascode and tail compensation were fabricated in a 0.5-µm 2P3M CMOS process. The circuits operate at a total quiescent current of 90 µA with ±1.5V power supplies. Experimental results show that tail compensation increases the unity-gain frequency by 60% and 25% and improves PSRR from the positive rail by 22 dB and 26 dB over a frequency range from 23 kHz to 3.0 MHz compared to Miller and cascode compensation, respectively. nearly zero; hence the main motivation for selecting node VX in the compensation path. From node V1 to node VOU T power supply noise is injected through the parasitic capacitance Cgd in the tail compensation technique. As such, PSRR begins to degrade at moderate rather than low frequencies. Index Terms—Tail compensation, Miller compensation, power supply rejection ratio, two-stage opamps. !"# !$# !%# Fig. 1. Primary VDD signal path created in (a) Miller (b) cascode and (c) proposed tail compensation schemes. I. I NTRODUCTION Power supply rejection ratio (PSRR) often determines the performance limit of sensitive analog circuitry such as ADCs, PLLs, VCOs and LDOs [1], [2]. Indeed, whenever the supply voltage is generated by a switched-mode power supply, ripple noise is unavoidable. In portable communications devices, which utilize transceiver circuits operating at high frequencies, supply ripple may even cause stability degradation at the frequency of transmission [3]. While many existing techniques, such as Miller and cascode compensation [4]–[19], ensure stability of a closed-loop amplifier, in some circumstances they lead to poor PSRR. Referring to Fig. 1, let V1 be the output of the first stage and VOU T be the output of the second stage of a two stage CMOS opamp. Miller compensation is placed between nodes V1 and VOU T and cascode compensation between nodes VY and VOU T , where node VY is the source of the cascoding transistor. The gain from VDD to nodes V1 [8] and VY is very nearly unity, as will be demonstrated later. In this way, power supply noise is easily induced through the large compensation capacitors to the output node, resulting in the degradation of PSRR at low frequencies. To this end, we introduce a new compensation technique called “tail” compensation which does not create a path from a node contaminated by VDD noise. In this technique, as shown in Fig. 1(c), the compensating capacitor CT is connected to the low impedance tail current node VX of the amplifier. As will be demonstrated later, the gain from VDD to VX is very 978-1-4673-1556-2/12/$31.00@2012 IEEE &'' &'' &'' $% &*+, $% &) !" ! ## *- .! ## &!"# !" &( &*+, &) ** &!"# &*+, *23 &) &!"# !" ! ## &$/0 *# !$" ! &1 II. CMOS T WO -S TAGE A MPLIFIER The circuit implementation of a two-stage operational amplifier with Miller, cascode and the proposed tail compensation schemes is shown in Fig. 2. The circuit consists of two stages, a differential pair with single-ended load (M1 -M8 ) and a common-source output stage (M12 -M13 ). Generally the effective transconductance of a differential amplifier equals the transconductance of differential input transistors M1 , M2 . In this case, the load of the first stage is cascode current source M3 -M4 . The current through M1 is not mirrored to node V1 ; hence, the effective transconductance of the first stage reduces to 0.5gm1 = 0.5gm2 . The current through transistor M1 is utilized to create a feed-forward path to node VOU T through mirror M5 -M6 and transistors M9 -M12 . The mirror formed by transistors M11 M12 has a dimension ratio of 1:K, thus giving rise to a feed-forward transconductance of 0.5Kgm1 . In this way, the current generated through the M1 branch is utilized for two purposes: (i) enhancing the negative going slew-rate and (ii) biasing the output stage of the amplifier. The common-source transistor M13 in the second stage is similarly sized K times the unit-sized PMOS transistor. Bias voltages and currents are generated by transistors M14 -M19 and resistors Rb . A. Op-amp Gain Let the output resistance and equivalent capacitance to ground of the first and second stages be denoted by R1 and VDD M19 M6 M9 VBP M13 Ib Ib VCP M18 M10 VY M5 VCN Rb Ib V IN-­ M1 Ib CC VCN M14 M7 m=2 Bias Circuit Tail M8 m=2 M11 m=K M12 Output Stage First Stage Feed-­forward Path CL RL CT VBN M17 M16 VOUT VIN+ 2Ib VBN Miller CM RM M2 VX M15 Fig. 2. Cascode M3 V1 Rb V SS m=K M4 VBP Schematic of two-stage operational amplifier illustrating Miller, cascode, and tail compensation techniques. C1 , and ROU T and COU T , respectively. Also, let the transconductance, output resistance, gate-to-source, and gate-to-drain capacitances of an individual transistor Mi be represented by gmi , roM i , Cgsi and Cgdi , respectively. Referring to Fig. 2, the gains of the first and second stages are AV 1 = −0.5gm2 R1 , AV 2 = −g m13 ROU T ! ! "#$ ± (1) '() .*+"#$ where R1 = roM 2 ||(gm3 roM 3 roM 4 ) ≈ roM 2 and ROU T = (roM 12 ||roM 13 ||RL ). The overall gain of the two-stage amplifier, including the feed-forward path is AV = AV 1 AV 2 + 0.5Kgm1 ROU T . The amplifier of Fig. 2 is implemented using all three compensation techniques – Miller, cascode, and tail – in order to clearly differentiate the performance of the proposed tail compensation technique. The tail compensation capacitor CT is introduced between node VOU T and node VX , a node with a low input resistance of (1/gm1 )||(1/gm2 ). The output of the first stage is isolated from the feedback network by the current buffer [12], [13] formed by transistor M2 . Current fed back through� M2 establishes the� dominant low-frequency pole at −1 ωp1 = R1 ( C2T )gm13 ROU T . III. S MALL S IGNAL A NALYSIS Small-signal models of the three compensation topologies are shown in Fig. 3. Three LHP poles and two LHP zeros were derived for each topology. A summary of the equations of poles and zeros and their unity-gain frequencies (ωU GF ) along with their approximate frequencies for each compensation network are given in Table I. These theoretical values are computed with values from a SPICE operating point analysis using 0.5-µm transistor models. As one can observe, the dominant pole ωp1 in each configuration-Miller, cascode and tail-is established by compensating capacitances CM , CC and CT , respectively. The effect of the first non-dominant pole ωp2 is approximately nullified through careful placement of the first LHP zero ωz1 . The second zero ωz2 is at very high frequencies (f > 150 MHz); hence, it has negligible effect on opamp stability. The non-dominant poles ωp2 and ωp3 depend on output &! ! ", " "#$$%&! '()*%+,-.#(+ ! 123 ! %% ! .*/0"! %123 ! %! . *0 . *0 ", '()4 .*/"#$ '-,/(0%! '()*%+,-.#(+ &123 1%%023(&4-&0!5-.6 "$# %3 (2) B. Tail Compensation "! &- %- ! .*+ "#$6 "5 ± ! ! .*/ "! ! ! ! 7-#$!'()*%+,-.#(+ .*+"" 6±" # #$! 5 " ! 123 ! % .7/0 &! %! ! ! .*/0"! %123 4 .*/""#$8±"5# &123 1%%023(&4-&0!5-.6 "%# Fig. 3. Small signal model of opamps in Fig. 2 using (a) Miller and cascode compensation and (b) proposed tail compensation. capacitor COU T . Zero ωz1 depends only on the compensation capacitors. The non-dominant poles in Miller and cascode are real, whereas those in tail compensation are a complex pole pair with a theoretically computed damping factor Q = 0.76. IV. P OWER S UPPLY R EJECTION R ATIO A NALYSIS The PSRR small signal models of the three different compensation schemes are shown in Fig. 4. The opamp is connected in a unity-gain configuration and an AC signal in series with the DC power supply voltage is placed at the VDD terminal. The ratio VDD /VOU T defines PSRR. There are several differences in the PSRR small-signal models of Fig. 4 compared to the small-signal models of Fig. 3. Since PSRR is measured in unity-gain configuration, input VIN + is now at ground and VOU T is connected to VIN − . Looking at the first stage of Fig. 4, the effect of transistor M2 on node V1 is seen in resistance roM 2 and the effect of the unity-gain feedback is through transconductance −0.5g m2 VOU T . Node V1 is also loaded by Cgs13 to VDD . For common-mode voltage signals, in particular VDD , node VX is TABLE I E QUATIONS FOR AC S MALL - SIGNAL MODELS AND THEIR THEORETICALLY COMPUTED LOCATIONS Pole/Zero Miller (Fig. 3(a)) ωp1 1 f (Hz) Cascode (Fig. 3(a)) 5k 1 R1 CM gm13 ROU T gm13 CM C1 CM +COU T (C1 +CM ) ωp2 1 RM ωp3 ωz1 � 1 C1 + 1 CM + 1 COU T 1 RM C M � ωU GF Pole ωp1,P SRR �C OU T CC gm3 R1 g�m13 CC +C1 (CC +COU T ) 1 +gm3 R1 C 1 170M gm2 gm13 2COU T CM � 1 CC + 1 COU T gm3 CC 8M gm13 KC1 ωz2 Tail (Fig. 3(b)) f (Hz) 4k 1 R1 (CT /2)gm13 ROU T 4.5k complex pole pair ωp2,3 15M R1 CC gm13 ROU T 3M � f (Hz) 16M � 66M 14M � gm1 gm13 C1 Cgd13 +Cgd13 COU T +C1 COU T gm2 CT 10.4M 250M gm13 KC1 250M gm13 C1 156M 6.2M gm2 2CC 8.3M gm2 CT 10.4M TABLE II E QUATIONS FOR THE LOCATION OF PSRR DOMINANT POLES Miller (Fig. 4(a)) f (Hz) (roM 2 CM gm13 roM 13 )−1 Cascode (Fig. 4(a)) 1.5k (roM 2 CC gm13 roM 13 f (Hz) )−1 1.2k Tail (Fig. 4(b)) (roM 2 Cgd13 gm13 roM 13 f (Hz) )−1 23k open, since it is loaded by cascode current source M7 -M8 (see Fig. 2). Therefore, whatever current enters node VX through transistor M1 must circulate back through transistor M2 onto node V1 . The current entering node VX through transistor M1 , VDD /roM 1 , appears at node V1 as a dependent current source, as shown in Fig. 4. A final difference between the two models in the first stage is that the impedance of the cascode buffer 1/gm3 in Fig. 4(a) is now attached to VDD . Differences in the second stage of the PSRR small-signal model are that transconductance gm13 in parallel with re� sistance roM 13 now go to VDD , rather than ground. ROU T is the equivalent resistance to ground at node VOU T , where � ROU T = ROU T ||roM 13 . All other differences in the second stage are due to measuring PSRR in unity-gain configuration, wherein VIN + is tied to ground and VOU T to VIN − . As mentioned earlier, the reason for degraded PSRR performance in Miller and cascode compensation techniques is that noise from VDD appears unattenuated at nodes V1 and VY . Small-signal analysis of the PSRR models in Fig. 4 yield the following gain equations from VDD to nodes V1 , VY , and VX . !"#$%&'(!%)*'+#",-%+ The dominant pole determines the shape of the PSRR frequency response, which is a single-pole system for frequencies below the unity-gain frequency fU GF . A summary of the dominant pole equations are shown in Table II. In Miller and cascode compensation, the dominant poles are created by capacitors CM and CC , with theoretically computed values of 1.5 kHz and 1.2 kHz, respectively. However, in tail compensation the dominant pole is caused by the small parasitic capacitance Cgd13 of transistor M13 and not the large compensation capacitor CT . This leads to the dominant pole occurring at the moderate frequency of 23 kHz, leading to a higher PSRR for moderate-to-high frequencies. !"" !"" $%&# ( /* !2 '()#* !# (/#*"!"".!# # $ (/* !2 '' $%&#* !+,- '& 1& $%&0 .(/0 !+,- '(4#* ! 3( /#!+,! 5¶+,- '+,- .-//'0(!%)*'+#",-%+ "%# 1"-/(!%)*'+#",-%+ !"" ' (4#* !"" $%&# .(6/0!5 '()#* !# $%&0 (/#* "! "" .!# # !5 $ ( /0 $ ≈ ≈ 1 VY ≈ 1, ≈1 gm13 roM 13 VDD 1 gm2 roM 13 (K + roM 2 gm13 ) 1+ (3) Using small-signal parameters, the gain VX /VDD ≈ 2.5 × 10−4 , which is close to 0. The PSRR at low frequencies, P SRRDC , is the same for Miller, cascode and tail compensation, and is given by P SRRDC = 0.5gm2 roM 2 gm13 roM 13 . (4) $%&#* V. E XPERIMENTAL R ESULTS AND C ONCLUSIONS '- !+,- 3(/# "!+,- .!5# 5¶+,- '+,- The three designs were implemented in a 0.5-µm 2P3M CMOS process. A chip micrograph is shown Fig. 5. Measurements were performed using power supplies ±1.5V and a total bias current of 90 µA. The output load consisted of a 40 kΩ resistor in parallel with a 20 pF capacitor. Simulated openloop gain for all three schemes was 69 dB. To achieve a phase margin of 63o , the required compensation capacitors-CM , CC and CT -were 1.25 pF, 1.55 pF and 2.75 pF, respectively. $ $ (/# V1 VDD VX VDD "&# Fig. 4. PSRR Small signal model of opamps in Fig. 2 showing (a) Miller and cascode compensation and (b) proposed tail compensation. Measured transient waveforms of the amplifiers in an inverting configuration with a gain of −1V /V are shown in Fig. 6. While the Miller and cascode compensated designs achieved a measured fU GF of 6.4 MHz and 8.2 MHz, respectively, fU GF for the tail compensated design was 10.3 MHz, an improvement of 60% over Miller and 25% over cascode. (a) (c) Fig. 5. Chip micrograph showing (a) Miller (b) cascode and (c) tail compensated designs. Dimensions in Table III. 1 0.5 Input Miller Cascode Tail Vout (V) 0 −0.5 −1 −1.5 −2 −2.5 0 0.5 1 1.5 2 2.5 3 3.5 4 4.5 Time (µs) Fig. 6. Measured transient responses with input VIN = 1.6 Vpk−pk at 200 kHz. Amplifiers are in a unity-gain inverting configuration. (Offset added for visibility). PSRR was experimentally verified by configuring the amplifier as a voltage follower and adding a 100 mVpk−pk sinusoid to the VDD rail. Fig. 7 shows the measured PSRR responses. The tail compensated design outperforms the Miller and cascode compensated designs by approximately 22 dB for frequencies in the range of 23 kHz to 3 MHz. Dominant poles for PSRR for the three compensation networks closely correlate with the analytical values computed in Table II. 80 70 22 dB PSRR (dB) 60 50 40 30 20 10 0 1 10 Fig. 7. Miller Compensation Cascode Compensation Tail Compensation 2 10 3 10 4 10 Frequency (Hz) TABLE III S UMMARY OF M EASURED R ESULTS Parameter/Design Miller Cascode Tail UGF (MHz) 6.4 8.2 10.3 SR+/SR- (V/µs) (10%-90%) 6.3/2.9 5.8/3.0 3.4/5.1 PSRR @ 100 kHz (dB) 44 40 66 PSRR @ 3 MHz (dB) 14 8 36 Circuit area (µm x µm) 177 x 74 181 x 74 200 x 74 R EFERENCES (b) −3 supply noise sensitive analog applications, tail compensation may prove beneficial, due to its increased fU GF and enhanced PSRR performance. 5 10 6 10 Measured PSRR of the three different compensation schemes. 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