Download presentation

Presentation is loading. Please wait.

Published byMikayla Fenno Modified over 2 years ago

1
1 Fundamentals of Microelectronics II CH9 Cascode Stages and Current Mirrors CH10 Differential Amplifiers CH11 Frequency Response CH12 Feedback

2
2 Chapter 9 Cascode Stages and Current Mirrors 9.1 Cascode Stage 9.2 Current Mirrors

3
CH 9 Cascode Stages and Current Mirrors3 Boosted Output Impedances

4
CH 9 Cascode Stages and Current Mirrors4 Bipolar Cascode Stage

5
CH 9 Cascode Stages and Current Mirrors5 Maximum Bipolar Cascode Output Impedance The maximum output impedance of a bipolar cascode is bounded by the ever-present r between emitter and ground of Q 1.

6
CH 9 Cascode Stages and Current Mirrors6 Example: Output Impedance Typically r is smaller than r O, so in general it is impossible to double the output impedance by degenerating Q 2 with a resistor.

7
CH 9 Cascode Stages and Current Mirrors7 PNP Cascode Stage

8
CH 9 Cascode Stages and Current Mirrors8 Another Interpretation of Bipolar Cascode Instead of treating cascode as Q 2 degenerating Q 1, we can also think of it as Q 1 stacking on top of Q 2 (current source) to boost Q 2 ’s output impedance.

9
CH 9 Cascode Stages and Current Mirrors9 False Cascodes When the emitter of Q 1 is connected to the emitter of Q 2, it’s no longer a cascode since Q 2 becomes a diode-connected device instead of a current source.

10
CH 9 Cascode Stages and Current Mirrors10 MOS Cascode Stage

11
CH 9 Cascode Stages and Current Mirrors11 Another Interpretation of MOS Cascode Similar to its bipolar counterpart, MOS cascode can be thought of as stacking a transistor on top of a current source. Unlike bipolar cascode, the output impedance is not limited by .

12
CH 9 Cascode Stages and Current Mirrors12 PMOS Cascode Stage

13
CH 9 Cascode Stages and Current Mirrors13 Example: Parasitic Resistance R P will lower the output impedance, since its parallel combination with r O1 will always be lower than r O1.

14
CH 9 Cascode Stages and Current Mirrors14 Short-Circuit Transconductance The short-circuit transconductance of a circuit measures its strength in converting input voltage to output current.

15
CH 9 Cascode Stages and Current Mirrors15 Transconductance Example

16
CH 9 Cascode Stages and Current Mirrors16 Derivation of Voltage Gain By representing a linear circuit with its Norton equivalent, the relationship between V out and V in can be expressed by the product of G m and R out.

17
CH 9 Cascode Stages and Current Mirrors17 Example: Voltage Gain

18
CH 9 Cascode Stages and Current Mirrors18 Comparison between Bipolar Cascode and CE Stage Since the output impedance of bipolar cascode is higher than that of the CE stage, we would expect its voltage gain to be higher as well.

19
CH 9 Cascode Stages and Current Mirrors19 Voltage Gain of Bipolar Cascode Amplifier Since r O is much larger than 1/g m, most of I C,Q1 flows into the diode-connected Q 2. Using R out as before, A V is easily calculated.

20
CH 9 Cascode Stages and Current Mirrors20 Alternate View of Cascode Amplifier A bipolar cascode amplifier is also a CE stage in series with a CB stage.

21
CH 9 Cascode Stages and Current Mirrors21 Practical Cascode Stage Since no current source can be ideal, the output impedance drops.

22
CH 9 Cascode Stages and Current Mirrors22 Improved Cascode Stage In order to preserve the high output impedance, a cascode PNP current source is used.

23
CH 9 Cascode Stages and Current Mirrors23 MOS Cascode Amplifier

24
CH 9 Cascode Stages and Current Mirrors24 Improved MOS Cascode Amplifier Similar to its bipolar counterpart, the output impedance of a MOS cascode amplifier can be improved by using a PMOS cascode current source.

25
CH 9 Cascode Stages and Current Mirrors25 Temperature and Supply Dependence of Bias Current Since V T, I S, n, and V TH all depend on temperature, I 1 for both bipolar and MOS depends on temperature and supply.

26
CH 9 Cascode Stages and Current Mirrors26 Concept of Current Mirror The motivation behind a current mirror is to sense the current from a “golden current source” and duplicate this “golden current” to other locations.

27
CH 9 Cascode Stages and Current Mirrors27 Bipolar Current Mirror Circuitry The diode-connected Q REF produces an output voltage V 1 that forces I copy1 = I REF, if Q 1 = Q REF.

28
CH 9 Cascode Stages and Current Mirrors28 Bad Current Mirror Example I Without shorting the collector and base of Q REF together, there will not be a path for the base currents to flow, therefore, I copy is zero.

29
CH 9 Cascode Stages and Current Mirrors29 Bad Current Mirror Example II Although a path for base currents exists, this technique of biasing is no better than resistive divider.

30
CH 9 Cascode Stages and Current Mirrors30 Multiple Copies of I REF Multiple copies of I REF can be generated at different locations by simply applying the idea of current mirror to more transistors.

31
CH 9 Cascode Stages and Current Mirrors31 Current Scaling By scaling the emitter area of Q j n times with respect to Q REF, I copy,j is also n times larger than I REF. This is equivalent to placing n unit-size transistors in parallel.

32
CH 9 Cascode Stages and Current Mirrors32 Example: Scaled Current

33
CH 9 Cascode Stages and Current Mirrors33 Fractional Scaling A fraction of I REF can be created on Q 1 by scaling up the emitter area of Q REF.

34
CH 9 Cascode Stages and Current Mirrors34 Example: Different Mirroring Ratio Using the idea of current scaling and fractional scaling, I copy2 is 0.5mA and I copy1 is 0.05mA respectively. All coming from a source of 0.2mA.

35
CH 9 Cascode Stages and Current Mirrors35 Mirroring Error Due to Base Currents

36
CH 9 Cascode Stages and Current Mirrors36 Improved Mirroring Accuracy Because of Q F, the base currents of Q REF and Q 1 are mostly supplied by Q F rather than I REF. Mirroring error is reduced times.

37
CH 9 Cascode Stages and Current Mirrors37 Example: Different Mirroring Ratio Accuracy

38
CH 9 Cascode Stages and Current Mirrors38 PNP Current Mirror PNP current mirror is used as a current source load to an NPN amplifier stage.

39
CH 9 Cascode Stages and Current Mirrors39 Generation of I REF for PNP Current Mirror

40
CH 9 Cascode Stages and Current Mirrors40 Example: Current Mirror with Discrete Devices Let Q REF and Q 1 be discrete NPN devices. I REF and I copy1 can vary in large magnitude due to I S mismatch.

41
CH 9 Cascode Stages and Current Mirrors41 MOS Current Mirror The same concept of current mirror can be applied to MOS transistors as well.

42
CH 9 Cascode Stages and Current Mirrors42 Bad MOS Current Mirror Example This is not a current mirror since the relationship between V X and I REF is not clearly defined. The only way to clearly define V X with I REF is to use a diode- connected MOS since it provides square-law I-V relationship.

43
CH 9 Cascode Stages and Current Mirrors43 Example: Current Scaling Similar to their bipolar counterpart, MOS current mirrors can also scale I REF up or down (I 1 = 0.2mA, I 2 = 0.5mA).

44
CH 9 Cascode Stages and Current Mirrors44 CMOS Current Mirror The idea of combining NMOS and PMOS to produce CMOS current mirror is shown above.

45
45 Chapter 10 Differential Amplifiers 10.1 General Considerations 10.2 Bipolar Differential Pair 10.3 MOS Differential Pair 10.4 Cascode Differential Amplifiers 10.5 Common-Mode Rejection 10.6 Differential Pair with Active Load

46
CH 10 Differential Amplifiers46 Audio Amplifier Example An audio amplifier is constructed above that takes on a rectified AC voltage as its supply and amplifies an audio signal from a microphone.

47
CH 10 Differential Amplifiers47 “Humming” Noise in Audio Amplifier Example However, V CC contains a ripple from rectification that leaks to the output and is perceived as a “humming” noise by the user.

48
CH 10 Differential Amplifiers48 Supply Ripple Rejection Since both node X and Y contain the ripple, their difference will be free of ripple.

49
CH 10 Differential Amplifiers49 Ripple-Free Differential Output Since the signal is taken as a difference between two nodes, an amplifier that senses differential signals is needed.

50
CH 10 Differential Amplifiers50 Common Inputs to Differential Amplifier Signals cannot be applied in phase to the inputs of a differential amplifier, since the outputs will also be in phase, producing zero differential output.

51
CH 10 Differential Amplifiers51 Differential Inputs to Differential Amplifier When the inputs are applied differentially, the outputs are 180° out of phase; enhancing each other when sensed differentially.

52
CH 10 Differential Amplifiers52 Differential Signals A pair of differential signals can be generated, among other ways, by a transformer. Differential signals have the property that they share the same average value to ground and are equal in magnitude but opposite in phase.

53
CH 10 Differential Amplifiers53 Single-ended vs. Differential Signals

54
CH 10 Differential Amplifiers54 Differential Pair With the addition of a tail current, the circuits above operate as an elegant, yet robust differential pair.

55
CH 10 Differential Amplifiers55 Common-Mode Response

56
CH 10 Differential Amplifiers56 Common-Mode Rejection Due to the fixed tail current source, the input common- mode value can vary without changing the output common- mode value.

57
CH 10 Differential Amplifiers57 Differential Response I

58
CH 10 Differential Amplifiers58 Differential Response II

59
CH 10 Differential Amplifiers59 Differential Pair Characteristics None-zero differential input produces variations in output currents and voltages, whereas common-mode input produces no variations.

60
CH 10 Differential Amplifiers60 Small-Signal Analysis Since the input to Q 1 and Q 2 rises and falls by the same amount, and their bases are tied together, the rise in I C1 has the same magnitude as the fall in I C2.

61
CH 10 Differential Amplifiers61 Virtual Ground For small changes at inputs, the g m ’s are the same, and the respective increase and decrease of I C1 and I C2 are the same, node P must stay constant to accommodate these changes. Therefore, node P can be viewed as AC ground.

62
CH 10 Differential Amplifiers62 Small-Signal Differential Gain Since the output changes by -2g m VR C and input by 2 V, the small signal gain is –g m R C, similar to that of the CE stage. However, to obtain same gain as the CE stage, power dissipation is doubled.

63
CH 10 Differential Amplifiers63 Large Signal Analysis

64
CH 10 Differential Amplifiers64 Input/Output Characteristics

65
CH 10 Differential Amplifiers65 Linear/Nonlinear Regions The left column operates in linear region, whereas the right column operates in nonlinear region.

66
CH 10 Differential Amplifiers66 Small-Signal Model

67
CH 10 Differential Amplifiers67 Half Circuits Since V P is grounded, we can treat the differential pair as two CE “half circuits”, with its gain equal to one half circuit’s single-ended gain.

68
CH 10 Differential Amplifiers68 Example: Differential Gain

69
CH 10 Differential Amplifiers69 Extension of Virtual Ground It can be shown that if R 1 = R 2, and points A and B go up and down by the same amount respectively, V X does not move.

70
CH 10 Differential Amplifiers70 Half Circuit Example I

71
CH 10 Differential Amplifiers71 Half Circuit Example II

72
CH 10 Differential Amplifiers72 Half Circuit Example III

73
CH 10 Differential Amplifiers73 Half Circuit Example IV

74
CH 10 Differential Amplifiers74 MOS Differential Pair’s Common-Mode Response Similar to its bipolar counterpart, MOS differential pair produces zero differential output as V CM changes.

75
CH 10 Differential Amplifiers75 Equilibrium Overdrive Voltage The equilibrium overdrive voltage is defined as the overdrive voltage seen by M 1 and M 2 when both of them carry a current of I SS /2.

76
CH 10 Differential Amplifiers76 Minimum Common-mode Output Voltage In order to maintain M 1 and M 2 in saturation, the common- mode output voltage cannot fall below the value above. This value usually limits voltage gain.

77
CH 10 Differential Amplifiers77 Differential Response

78
CH 10 Differential Amplifiers78 Small-Signal Response Similar to its bipolar counterpart, the MOS differential pair exhibits the same virtual ground node and small signal gain.

79
CH 10 Differential Amplifiers79 Power and Gain Tradeoff In order to obtain the source gain as a CS stage, a MOS differential pair must dissipate twice the amount of current. This power and gain tradeoff is also echoed in its bipolar counterpart.

80
CH 10 Differential Amplifiers80 MOS Differential Pair’s Large-Signal Response

81
CH 10 Differential Amplifiers81 Maximum Differential Input Voltage There exists a finite differential input voltage that completely steers the tail current from one transistor to the other. This value is known as the maximum differential input voltage.

82
CH 10 Differential Amplifiers82 Contrast Between MOS and Bipolar Differential Pairs In a MOS differential pair, there exists a finite differential input voltage to completely switch the current from one transistor to the other, whereas, in a bipolar pair that voltage is infinite.

83
CH 10 Differential Amplifiers83 The effects of Doubling the Tail Current Since I SS is doubled and W/L is unchanged, the equilibrium overdrive voltage for each transistor must increase by to accommodate this change, thus V in,max increases by as well. Moreover, since I SS is doubled, the differential output swing will double.

84
CH 10 Differential Amplifiers84 The effects of Doubling W/L Since W/L is doubled and the tail current remains unchanged, the equilibrium overdrive voltage will be lowered by to accommodate this change, thus V in,max will be lowered by as well. Moreover, the differential output swing will remain unchanged since neither I SS nor R D has changed

85
CH 10 Differential Amplifiers85 Small-Signal Analysis of MOS Differential Pair When the input differential signal is small compared to 4I SS / n C ox (W/L), the output differential current is linearly proportional to it, and small-signal model can be applied.

86
CH 10 Differential Amplifiers86 Virtual Ground and Half Circuit Applying the same analysis as the bipolar case, we will arrive at the same conclusion that node P will not move for small input signals and the concept of half circuit can be used to calculate the gain.

87
CH 10 Differential Amplifiers87 MOS Differential Pair Half Circuit Example I

88
CH 10 Differential Amplifiers88 MOS Differential Pair Half Circuit Example II

89
CH 10 Differential Amplifiers89 MOS Differential Pair Half Circuit Example III

90
CH 10 Differential Amplifiers90 Bipolar Cascode Differential Pair

91
CH 10 Differential Amplifiers91 Bipolar Telescopic Cascode

92
CH 10 Differential Amplifiers92 Example: Bipolar Telescopic Parasitic Resistance

93
CH 10 Differential Amplifiers93 MOS Cascode Differential Pair

94
CH 10 Differential Amplifiers94 MOS Telescopic Cascode

95
CH 10 Differential Amplifiers95 Example: MOS Telescopic Parasitic Resistance

96
CH 10 Differential Amplifiers96 Effect of Finite Tail Impedance If the tail current source is not ideal, then when a input CM voltage is applied, the currents in Q 1 and Q 2 and hence output CM voltage will change.

97
CH 10 Differential Amplifiers97 Input CM Noise with Ideal Tail Current

98
CH 10 Differential Amplifiers98 Input CM Noise with Non-ideal Tail Current

99
CH 10 Differential Amplifiers99 Comparison As it can be seen, the differential output voltages for both cases are the same. So for small input CM noise, the differential pair is not affected.

100
CH 10 Differential Amplifiers100 CM to DM Conversion, A CM-DM If finite tail impedance and asymmetry are both present, then the differential output signal will contain a portion of input common-mode signal.

101
CH 10 Differential Amplifiers101 Example: A CM-DM

102
CH 10 Differential Amplifiers102 CMRR CMRR defines the ratio of wanted amplified differential input signal to unwanted converted input common-mode noise that appears at the output.

103
CH 10 Differential Amplifiers103 Differential to Single-ended Conversion Many circuits require a differential to single-ended conversion, however, the above topology is not very good.

104
CH 10 Differential Amplifiers104 Supply Noise Corruption The most critical drawback of this topology is supply noise corruption, since no common-mode cancellation mechanism exists. Also, we lose half of the signal.

105
CH 10 Differential Amplifiers105 Better Alternative This circuit topology performs differential to single-ended conversion with no loss of gain.

106
CH 10 Differential Amplifiers106 Active Load With current mirror used as the load, the signal current produced by the Q 1 can be replicated onto Q 4. This type of load is different from the conventional “static load” and is known as an “active load”.

107
CH 10 Differential Amplifiers107 Differential Pair with Active Load The input differential pair decreases the current drawn from R L by I and the active load pushes an extra I into R L by current mirror action; these effects enhance each other.

108
CH 10 Differential Amplifiers108 Active Load vs. Static Load The load on the left responds to the input signal and enhances the single-ended output, whereas the load on the right does not.

109
CH 10 Differential Amplifiers109 MOS Differential Pair with Active Load Similar to its bipolar counterpart, MOS differential pair can also use active load to enhance its single-ended output.

110
CH 10 Differential Amplifiers110 Asymmetric Differential Pair Because of the vastly different resistance magnitude at the drains of M 1 and M 2, the voltage swings at these two nodes are different and therefore node P cannot be viewed as a virtual ground.

111
CH 10 Differential Amplifiers111 Thevenin Equivalent of the Input Pair

112
CH 10 Differential Amplifiers112 Simplified Differential Pair with Active Load

113
CH 10 Differential Amplifiers113 I A Proof of V A << V out

114
CH 10 Differential Amplifiers114 Chapter 11 Frequency Response 11.1 Fundamental Concepts 11.2 High-Frequency Models of Transistors 11.3 Analysis Procedure 11.4 Frequency Response of CE and CS Stages 11.5 Frequency Response of CB and CG Stages 11.6 Frequency Response of Followers 11.7 Frequency Response of Cascode Stage 11.8 Frequency Response of Differential Pairs 11.9 Additional Examples 114

115
CH 10 Differential Amplifiers115 Chapter Outline CH 11 Frequency Response115

116
CH 10 Differential Amplifiers116CH 11 Frequency Response116 High Frequency Roll-off of Amplifier As frequency of operation increases, the gain of amplifier decreases. This chapter analyzes this problem.

117
CH 10 Differential Amplifiers117 Example: Human Voice I Natural human voice spans a frequency range from 20Hz to 20KHz, however conventional telephone system passes frequencies from 400Hz to 3.5KHz. Therefore phone conversation differs from face-to-face conversation. CH 11 Frequency Response117 Natural Voice Telephone System

118
CH 10 Differential Amplifiers118 Example: Human Voice II CH 11 Frequency Response118 MouthRecorderAir MouthEarAir Skull Path traveled by the human voice to the voice recorder Path traveled by the human voice to the human ear Since the paths are different, the results will also be different.

119
CH 10 Differential Amplifiers119 Example: Video Signal Video signals without sufficient bandwidth become fuzzy as they fail to abruptly change the contrast of pictures from complete white into complete black. CH 11 Frequency Response119 High BandwidthLow Bandwidth

120
CH 10 Differential Amplifiers120 Gain Roll-off: Simple Low-pass Filter In this simple example, as frequency increases the impedance of C 1 decreases and the voltage divider consists of C 1 and R 1 attenuates V in to a greater extent at the output. CH 11 Frequency Response120

121
CH 10 Differential Amplifiers121CH 11 Frequency Response121 Gain Roll-off: Common Source The capacitive load, C L, is the culprit for gain roll-off since at high frequency, it will “steal” away some signal current and shunt it to ground.

122
CH 10 Differential Amplifiers122CH 11 Frequency Response122 Frequency Response of the CS Stage At low frequency, the capacitor is effectively open and the gain is flat. As frequency increases, the capacitor tends to a short and the gain starts to decrease. A special frequency is ω=1/(R D C L ), where the gain drops by 3dB.

123
CH 10 Differential Amplifiers123CH 11 Frequency Response123 Example: Figure of Merit This metric quantifies a circuit’s gain, bandwidth, and power dissipation. In the bipolar case, low temperature, supply, and load capacitance mark a superior figure of merit.

124
CH 10 Differential Amplifiers124 Example: Relationship between Frequency Response and Step Response CH 11 Frequency Response124 The relationship is such that as R 1 C 1 increases, the bandwidth drops and the step response becomes slower.

125
CH 10 Differential Amplifiers125CH 11 Frequency Response125 Bode Plot When we hit a zero, ω zj, the Bode magnitude rises with a slope of +20dB/dec. When we hit a pole, ω pj, the Bode magnitude falls with a slope of -20dB/dec

126
CH 10 Differential Amplifiers126CH 11 Frequency Response126 Example: Bode Plot The circuit only has one pole (no zero) at 1/(R D C L ), so the slope drops from 0 to -20dB/dec as we pass ω p1.

127
CH 10 Differential Amplifiers127CH 11 Frequency Response127 Pole Identification Example I

128
CH 10 Differential Amplifiers128CH 11 Frequency Response128 Pole Identification Example II

129
CH 10 Differential Amplifiers129CH 11 Frequency Response129 Circuit with Floating Capacitor The pole of a circuit is computed by finding the effective resistance and capacitance from a node to GROUND. The circuit above creates a problem since neither terminal of C F is grounded.

130
CH 10 Differential Amplifiers130CH 11 Frequency Response130 Miller’s Theorem If A v is the gain from node 1 to 2, then a floating impedance Z F can be converted to two grounded impedances Z 1 and Z 2.

131
CH 10 Differential Amplifiers131CH 11 Frequency Response131 Miller Multiplication With Miller’s theorem, we can separate the floating capacitor. However, the input capacitor is larger than the original floating capacitor. We call this Miller multiplication.

132
CH 10 Differential Amplifiers132CH 11 Frequency Response132 Example: Miller Theorem

133
CH 10 Differential Amplifiers133 High-Pass Filter Response The voltage division between a resistor and a capacitor can be configured such that the gain at low frequency is reduced. CH 11 Frequency Response133

134
CH 10 Differential Amplifiers134 Example: Audio Amplifier In order to successfully pass audio band frequencies (20 Hz-20 KHz), large input and output capacitances are needed. CH 11 Frequency Response134

135
CH 10 Differential Amplifiers135 Capacitive Coupling vs. Direct Coupling Capacitive coupling, also known as AC coupling, passes AC signals from Y to X while blocking DC contents. This technique allows independent bias conditions between stages. Direct coupling does not. Capacitive Coupling Direct Coupling CH 11 Frequency Response135

136
CH 10 Differential Amplifiers136 Typical Frequency Response Lower Corner Upper Corner CH 11 Frequency Response136

137
CH 10 Differential Amplifiers137CH 11 Frequency Response137 High-Frequency Bipolar Model At high frequency, capacitive effects come into play. C b represents the base charge, whereas C and C je are the junction capacitances.

138
CH 10 Differential Amplifiers138CH 11 Frequency Response138 High-Frequency Model of Integrated Bipolar Transistor Since an integrated bipolar circuit is fabricated on top of a substrate, another junction capacitance exists between the collector and substrate, namely C CS.

139
CH 10 Differential Amplifiers139CH 11 Frequency Response139 Example: Capacitance Identification

140
CH 10 Differential Amplifiers140CH 11 Frequency Response140 MOS Intrinsic Capacitances For a MOS, there exist oxide capacitance from gate to channel, junction capacitances from source/drain to substrate, and overlap capacitance from gate to source/drain.

141
CH 10 Differential Amplifiers141CH 11 Frequency Response141 Gate Oxide Capacitance Partition and Full Model The gate oxide capacitance is often partitioned between source and drain. In saturation, C 2 ~ C gate, and C 1 ~ 0. They are in parallel with the overlap capacitance to form C GS and C GD.

142
CH 10 Differential Amplifiers142CH 11 Frequency Response142 Example: Capacitance Identification

143
CH 10 Differential Amplifiers143CH 11 Frequency Response143 Transit Frequency Transit frequency, f T, is defined as the frequency where the current gain from input to output drops to 1.

144
CH 10 Differential Amplifiers144 Example: Transit Frequency Calculation CH 11 Frequency Response144

145
CH 10 Differential Amplifiers145 Analysis Summary The frequency response refers to the magnitude of the transfer function. Bode’s approximation simplifies the plotting of the frequency response if poles and zeros are known. In general, it is possible to associate a pole with each node in the signal path. Miller’s theorem helps to decompose floating capacitors into grounded elements. Bipolar and MOS devices exhibit various capacitances that limit the speed of circuits. CH 11 Frequency Response145

146
CH 10 Differential Amplifiers146 High Frequency Circuit Analysis Procedure Determine which capacitor impact the low-frequency region of the response and calculate the low-frequency pole (neglect transistor capacitance). Calculate the midband gain by replacing the capacitors with short circuits (neglect transistor capacitance). Include transistor capacitances. Merge capacitors connected to AC grounds and omit those that play no role in the circuit. Determine the high-frequency poles and zeros. Plot the frequency response using Bode’s rules or exact analysis. CH 11 Frequency Response146

147
CH 10 Differential Amplifiers147 Frequency Response of CS Stage with Bypassed Degeneration In order to increase the midband gain, a capacitor C b is placed in parallel with R s. The pole frequency must be well below the lowest signal frequency to avoid the effect of degeneration. CH 11 Frequency Response147

148
CH 10 Differential Amplifiers148CH 11 Frequency Response148 Unified Model for CE and CS Stages

149
CH 10 Differential Amplifiers149CH 11 Frequency Response149 Unified Model Using Miller’s Theorem

150
CH 10 Differential Amplifiers150 Example: CE Stage The input pole is the bottleneck for speed. CH 11 Frequency Response150

151
CH 10 Differential Amplifiers151 Example: Half Width CS Stage CH 11 Frequency Response151

152
CH 10 Differential Amplifiers152CH 11 Frequency Response152 Direct Analysis of CE and CS Stages Direct analysis yields different pole locations and an extra zero.

153
CH 10 Differential Amplifiers153CH 11 Frequency Response153 Example: CE and CS Direct Analysis

154
CH 10 Differential Amplifiers154 Example: Comparison Between Different Methods Miller’s Exact Dominant Pole CH 11 Frequency Response154

155
CH 10 Differential Amplifiers155CH 11 Frequency Response155 Input Impedance of CE and CS Stages

156
CH 10 Differential Amplifiers156 Low Frequency Response of CB and CG Stages As with CE and CS stages, the use of capacitive coupling leads to low-frequency roll-off in CB and CG stages (although a CB stage is shown above, a CG stage is similar). CH 11 Frequency Response156

157
CH 10 Differential Amplifiers157CH 11 Frequency Response157 Frequency Response of CB Stage

158
CH 10 Differential Amplifiers158CH 11 Frequency Response158 Frequency Response of CG Stage Similar to a CB stage, the input pole is on the order of f T, so rarely a speed bottleneck.

159
CH 10 Differential Amplifiers159CH 11 Frequency Response159 Example: CG Stage Pole Identification

160
CH 10 Differential Amplifiers160 Example: Frequency Response of CG Stage CH 11 Frequency Response160

161
CH 10 Differential Amplifiers161CH 11 Frequency Response161 Emitter and Source Followers The following will discuss the frequency response of emitter and source followers using direct analysis. Emitter follower is treated first and source follower is derived easily by allowing r to go to infinity.

162
CH 10 Differential Amplifiers162CH 11 Frequency Response162 Direct Analysis of Emitter Follower

163
CH 10 Differential Amplifiers163CH 11 Frequency Response163 Direct Analysis of Source Follower Stage

164
CH 10 Differential Amplifiers164 Example: Frequency Response of Source Follower CH 11 Frequency Response164

165
CH 10 Differential Amplifiers165CH 11 Frequency Response165 Example: Source Follower

166
CH 10 Differential Amplifiers166CH 11 Frequency Response166 Input Capacitance of Emitter/Source Follower

167
CH 10 Differential Amplifiers167CH 11 Frequency Response167 Example: Source Follower Input Capacitance

168
CH 10 Differential Amplifiers168CH 11 Frequency Response168 Output Impedance of Emitter Follower

169
CH 10 Differential Amplifiers169CH 11 Frequency Response169 Output Impedance of Source Follower

170
CH 10 Differential Amplifiers170CH 11 Frequency Response170 Active Inductor The plot above shows the output impedance of emitter and source followers. Since a follower’s primary duty is to lower the driving impedance (R S >1/g m ), the “active inductor” characteristic on the right is usually observed.

171
CH 10 Differential Amplifiers171CH 11 Frequency Response171 Example: Output Impedance

172
CH 10 Differential Amplifiers172CH 11 Frequency Response172 Frequency Response of Cascode Stage For cascode stages, there are three poles and Miller multiplication is smaller than in the CE/CS stage.

173
CH 10 Differential Amplifiers173CH 11 Frequency Response173 Poles of Bipolar Cascode

174
CH 10 Differential Amplifiers174CH 11 Frequency Response174 Poles of MOS Cascode

175
CH 10 Differential Amplifiers175 Example: Frequency Response of Cascode CH 11 Frequency Response175

176
CH 10 Differential Amplifiers176CH 11 Frequency Response176 MOS Cascode Example

177
CH 10 Differential Amplifiers177CH 11 Frequency Response177 I/O Impedance of Bipolar Cascode

178
CH 10 Differential Amplifiers178CH 11 Frequency Response178 I/O Impedance of MOS Cascode

179
CH 10 Differential Amplifiers179CH 11 Frequency Response179 Bipolar Differential Pair Frequency Response Since bipolar differential pair can be analyzed using half- circuit, its transfer function, I/O impedances, locations of poles/zeros are the same as that of the half circuit’s. Half Circuit

180
CH 10 Differential Amplifiers180CH 11 Frequency Response180 MOS Differential Pair Frequency Response Since MOS differential pair can be analyzed using half- circuit, its transfer function, I/O impedances, locations of poles/zeros are the same as that of the half circuit’s. Half Circuit

181
CH 10 Differential Amplifiers181CH 11 Frequency Response181 Example: MOS Differential Pair

182
CH 10 Differential Amplifiers182 Common Mode Frequency Response C ss will lower the total impedance between point P to ground at high frequency, leading to higher CM gain which degrades the CM rejection ratio. CH 11 Frequency Response182

183
CH 10 Differential Amplifiers183 Tail Node Capacitance Contribution Source-Body Capacitance of M 1, M 2 and M 3 Gate-Drain Capacitance of M 3 CH 11 Frequency Response183

184
CH 10 Differential Amplifiers184 Example: Capacitive Coupling CH 11 Frequency Response184

185
CH 10 Differential Amplifiers185 Example: IC Amplifier – Low Frequency Design CH 11 Frequency Response185

186
CH 10 Differential Amplifiers186 Example: IC Amplifier – Midband Design CH 11 Frequency Response186

187
CH 10 Differential Amplifiers187 Example: IC Amplifier – High Frequency Design CH 11 Frequency Response187

188
188 Chapter 12 Feedback 12.1 General Considerations 12.2 Types of Amplifiers 12.3 Sense and Return Techniques 12.4 Polarity of Feedback 12.5 Feedback Topologies 12.6 Effect of Finite I/O Impedances 12.7 Stability in Feedback Systems

189
CH 12 Feedback189 Negative Feedback System A negative feedback system consists of four components: 1) feedforward system, 2) sense mechanism, 3) feedback network, and 4) comparison mechanism.

190
CH 12 Feedback190 Close-loop Transfer Function

191
CH 12 Feedback191 Feedback Example A 1 is the feedforward network, R 1 and R 2 provide the sensing and feedback capabilities, and comparison is provided by differential input of A 1.

192
CH 12 Feedback192 Comparison Error As A 1 K increases, the error between the input and fed back signal decreases. Or the fed back signal approaches a good replica of the input. E

193
CH 12 Feedback193 Comparison Error

194
CH 12 Feedback194 Loop Gain When the input is grounded, and the loop is broken at an arbitrary location, the loop gain is measured to be KA 1.

195
CH 12 Feedback195 Example: Alternative Loop Gain Measurement

196
CH 12 Feedback196 Incorrect Calculation of Loop Gain Signal naturally flows from the input to the output of a feedforward/feedback system. If we apply the input the other way around, the “output” signal we get is not a result of the loop gain, but due to poor isolation.

197
CH 12 Feedback197 Gain Desensitization A large loop gain is needed to create a precise gain, one that does not depend on A 1, which can vary by ±20%.

198
CH 12 Feedback198 Ratio of Resistors When two resistors are composed of the same unit resistor, their ratio is very accurate. Since when they vary, they will vary together and maintain a constant ratio.

199
CH 12 Feedback199 Merits of Negative Feedback 1) Bandwidth enhancement 2) Modification of I/O Impedances 3) Linearization

200
CH 12 Feedback200 Bandwidth Enhancement Although negative feedback lowers the gain by (1+KA 0 ), it also extends the bandwidth by the same amount. Open Loop Closed Loop Negative Feedback

201
CH 12 Feedback201 Bandwidth Extension Example As the loop gain increases, we can see the decrease of the overall gain and the extension of the bandwidth.

202
CH 12 Feedback202 Example: Open Loop Parameters

203
CH 12 Feedback203 Example: Closed Loop Voltage Gain

204
CH 12 Feedback204 Example: Closed Loop I/O Impedance

205
CH 12 Feedback205 Example: Load Desensitization W/O Feedback Large Difference With Feedback Small Difference

206
CH 12 Feedback206 Linearization Before feedback After feedback

207
CH 12 Feedback207 Four Types of Amplifiers

208
CH 12 Feedback208 Ideal Models of the Four Amplifier Types

209
CH 12 Feedback209 Realistic Models of the Four Amplifier Types

210
CH 12 Feedback210 Examples of the Four Amplifier Types

211
CH 12 Feedback211 Sensing a Voltage In order to sense a voltage across two terminals, a voltmeter with ideally infinite impedance is used.

212
CH 12 Feedback212 Sensing and Returning a Voltage Similarly, for a feedback network to correctly sense the output voltage, its input impedance needs to be large. R 1 and R 2 also provide a mean to return the voltage. Feedback Network

213
CH 12 Feedback213 Sensing a Current A current is measured by inserting a current meter with ideally zero impedance in series with the conduction path. The current meter is composed of a small resistance r in parallel with a voltmeter.

214
CH 12 Feedback214 Sensing and Returning a Current Similarly for a feedback network to correctly sense the current, its input impedance has to be small. R S has to be small so that its voltage drop will not change I out. Feedback Network

215
CH 12 Feedback215 Addition of Two Voltage Sources In order to add or substrate two voltage sources, we place them in series. So the feedback network is placed in series with the input source. Feedback Network

216
CH 12 Feedback216 Practical Circuits to Subtract Two Voltage Sources Although not directly in series, V in and V F are being subtracted since the resultant currents, differential and single-ended, are proportional to the difference of V in and V F.

217
CH 12 Feedback217 Addition of Two Current Sources In order to add two current sources, we place them in parallel. So the feedback network is placed in parallel with the input signal. Feedback Network

218
CH 12 Feedback218 Practical Circuits to Subtract Two Current Sources Since M 1 and R F are in parallel with the input current source, their respective currents are being subtracted. Note, R F has to be large enough to approximate a current source.

219
CH 12 Feedback219 Example: Sense and Return R 1 and R 2 sense and return the output voltage to feedforward network consisting of M 1 - M 4. M 1 and M 2 also act as a voltage subtractor.

220
CH 12 Feedback220 Example: Feedback Factor

221
CH 12 Feedback221 Input Impedance of an Ideal Feedback Network To sense a voltage, the input impedance of an ideal feedback network must be infinite. To sense a current, the input impedance of an ideal feedback network must be zero.

222
CH 12 Feedback222 Output Impedance of an Ideal Feedback Network To return a voltage, the output impedance of an ideal feedback network must be zero. To return a current, the output impedance of an ideal feedback network must be infinite.

223
CH 12 Feedback223 Determining the Polarity of Feedback 1) Assume the input goes either up or down. 2) Follow the signal through the loop. 3) Determine whether the returned quantity enhances or opposes the original change.

224
CH 12 Feedback224 Polarity of Feedback Example I Negative Feedback

225
CH 12 Feedback225 Polarity of Feedback Example II Negative Feedback

226
CH 12 Feedback226 Polarity of Feedback Example III Positive Feedback

227
CH 12 Feedback227 Voltage-Voltage Feedback

228
CH 12 Feedback228 Example: Voltage-Voltage Feedback

229
CH 12 Feedback229 Input Impedance of a V-V Feedback A better voltage sensor

230
CH 12 Feedback230 Example: V-V Feedback Input Impedance

231
CH 12 Feedback231 Output Impedance of a V-V Feedback A better voltage source

232
CH 12 Feedback232 Example: V-V Feedback Output Impedance

233
CH 12 Feedback233 Voltage-Current Feedback

234
CH 12 Feedback234 Example: Voltage-Current Feedback

235
CH 12 Feedback235 Input Impedance of a V-C Feedback A better current sensor.

236
CH 12 Feedback236 Example: V-C Feedback Input Impedance

237
CH 12 Feedback237 Output Impedance of a V-C Feedback A better voltage source.

238
CH 12 Feedback238 Example: V-C Feedback Output Impedance

239
CH 12 Feedback239 Current-Voltage Feedback

240
CH 12 Feedback240 Example: Current-Voltage Feedback Laser

241
CH 12 Feedback241 Input Impedance of a C-V Feedback A better voltage sensor.

242
CH 12 Feedback242 Output Impedance of a C-V Feedback A better current source.

243
CH 12 Feedback243 Laser Example: Current-Voltage Feedback

244
CH 12 Feedback244 Wrong Technique for Measuring Output Impedance If we want to measure the output impedance of a C-V closed-loop feedback topology directly, we have to place V X in series with K and R out. Otherwise, the feedback will be disturbed.

245
CH 12 Feedback245 Current-Current Feedback

246
CH 12 Feedback246 Input Impedance of C-C Feedback A better current sensor.

247
CH 12 Feedback247 Output Impedance of C-C Feedback A better current source.

248
CH 12 Feedback248 Example: Test of Negative Feedback Negative Feedback Laser

249
CH 12 Feedback249 Example: C-C Negative Feedback Laser

250
CH 12 Feedback250 How to Break a Loop The correct way of breaking a loop is such that the loop does not know it has been broken. Therefore, we need to present the feedback network to both the input and the output of the feedforward amplifier.

251
CH 12 Feedback251 Rules for Breaking the Loop of Amplifier Types

252
CH 12 Feedback252 Intuitive Understanding of these Rules Since ideally, the input of the feedback network sees zero impedance (Z out of an ideal voltage source), the return replicate needs to be grounded. Similarly, the output of the feedback network sees an infinite impedance (Z in of an ideal voltage sensor), the sense replicate needs to be open. Similar ideas apply to the other types. Voltage-Voltage Feedback

253
CH 12 Feedback253 Rules for Calculating Feedback Factor

254
CH 12 Feedback254 Intuitive Understanding of these Rules Since the feedback senses voltage, the input of the feedback is a voltage source. Moreover, since the return quantity is also voltage, the output of the feedback is left open (a short means the output is always zero). Similar ideas apply to the other types. Voltage-Voltage Feedback

255
CH 12 Feedback255 Breaking the Loop Example I

256
CH 12 Feedback256 Feedback Factor Example I

257
CH 12 Feedback257 Breaking the Loop Example II

258
CH 12 Feedback258 Feedback Factor Example II

259
CH 12 Feedback259 Breaking the Loop Example IV

260
CH 12 Feedback260 Feedback Factor Example IV

261
CH 12 Feedback261 Breaking the Loop Example V

262
CH 12 Feedback262 Feedback Factor Example V

263
CH 12 Feedback263 Breaking the Loop Example VI

264
CH 12 Feedback264 Feedback Factor Example VI

265
CH 12 Feedback265 Breaking the Loop Example VII

266
CH 12 Feedback266 Feedback Factor Example VII

267
CH 12 Feedback267 Breaking the Loop Example VIII

268
CH 12 Feedback268 Feedback Factor Example VIII

269
CH 12 Feedback269 Example: Phase Response As it can be seen, the phase of H(jω) starts to drop at 1/10 of the pole, hits -45 o at the pole, and approaches -90 o at 10 times the pole.

270
CH 12 Feedback270 Example: Three-Pole System For a three-pole system, a finite frequency produces a phase of -180 o, which means an input signal that operates at this frequency will have its output inverted.

271
CH 12 Feedback271 Instability of a Negative Feedback Loop Substitute jω for s. If for a certain ω 1, KH(jω 1 ) reaches -1, the closed loop gain becomes infinite. This implies for a very small input signal at ω 1, the output can be very large. Thus the system becomes unstable.

272
CH 12 Feedback272 “Barkhausen’s Criteria” for Oscillation

273
CH 12 Feedback273 Time Evolution of Instability

274
CH 12 Feedback274 Oscillation Example This system oscillates, since there’s a finite frequency at which the phase is -180 o and the gain is greater than unity. In fact, this system exceeds the minimum oscillation requirement.

275
CH 12 Feedback275 Condition for Oscillation Although for both systems above, the frequencies at which |KH|=1 and KH=-180 o are different, the system on the left is still unstable because at KH=-180 o, |KH|>1. Whereas the system on the right is stable because at KH=-180 o, |KH|<1.

276
CH 12 Feedback276 Condition for Stability ω PX, (“phase crossover”), is the frequency at which KH=-180 o. ω GX, (“gain crossover”), is the frequency at which |KH|=1.

277
CH 12 Feedback277 Stability Example I

278
CH 12 Feedback278 Stability Example II

279
CH 12 Feedback279 Marginally Stable vs. Stable Marginally Stable Stable

280
CH 12 Feedback280 Phase Margin Phase Margin = H(ω GX )+180 The larger the phase margin, the more stable the negative feedback becomes

281
CH 12 Feedback281 Phase Margin Example

282
CH 12 Feedback282 Frequency Compensation Phase margin can be improved by moving ω GX closer to origin while maintaining ω PX unchanged.

283
CH 12 Feedback283 Frequency Compensation Example C comp is added to lower the dominant pole so that ω GX occurs at a lower frequency than before, which means phase margin increases.

284
CH 12 Feedback284 Frequency Compensation Procedure 1) We identify a PM, then -180 o +PM gives us the new ω GX, or ω PM. 2) On the magnitude plot at ω PM, we extrapolate up with a slope of +20dB/dec until we hit the low frequency gain then we look “down” and the frequency we see is our new dominant pole, ω P ’.

285
CH 12 Feedback285 Example: 45 o Phase Margin Compensation

286
CH 12 Feedback286 Miller Compensation To save chip area, Miller multiplication of a smaller capacitance creates an equivalent effect.

Similar presentations

© 2016 SlidePlayer.com Inc.

All rights reserved.

Ads by Google