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= 2 (4:24 GHz). To compute the poles, we obtain a and b from

BR

Wiley/Razavi/Fundamentals of Microelectronics [Razavi.cls v. 2006]

June 30, 2007 at 13:42

571 (1)

 

 

 

 

Sec. 11.6 Frequency Response of Followers

which, upon substitution in (11.102) and with the assumption r g,1 leads to

m

 

 

 

C

Vout

=

1 + gm s

;

 

as2

 

Vin

 

+ bs + 1

where

a= RS (C C + C CL + C CL) gm

b = R C

 

+ C

+ 1 + RS CL :

S

gm

r gm

 

 

The circuit thus exhibits a zero at

j!zj = gm ;

C

571

(11.105)

(11.106)

(11.107)

(11.108)

which, from (11.49), is near the fT of the transistor. The poles of the circuit can be computed using the dominant-pole approximation described in Section 11.4.4. In practice, however, the two poles do not fall far from each other, necessitating direct solution of the quadratic denominator.

The above results also apply to the source follower if r ! 1 and corresponding capacitance substitutions are made (CSB and CL are in parallel):

 

 

 

 

 

 

 

 

1 +

CGS

s

 

 

 

 

 

 

 

 

 

 

 

 

Vout

=

gm

 

;

 

 

 

 

(11.109)

 

 

 

 

 

 

Vin

 

as2 + bs + 1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

where

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

a = RS [C

 

C

GS

+ C

 

(C

SB

+ C

L

) + C

(C

+ C

L

)]

(11.110)

gm

GD

 

GD

 

 

 

 

GS

SB

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

b = R

S

C

+ CGD + CSB + CL :

 

 

 

 

 

 

 

 

(11.111)

 

GD

 

 

 

 

gm

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Example 11.21

A source follower is driven by a resistance of 200 and drives a load capacitance of 100 fF. Using the transistor parameters given in Example 11.18, plot the frequency response of the circuit.

Solution

The zero occurs at gm=CGS

Eqs. (11.110) and (11.111), respectively:

 

a = 2:58 10,21 s,2

(11.112)

 

b = 5:8 10,11 s

(11.113)

The two poles are then equal to

 

 

!p1

= 2 [,1:79 GHz + j(2:57 GHz)]

(11.114)

!p2

= 2 [,1:79 GHz , j(2:57 GHz)]:

(11.115)

BR

Wiley/Razavi/Fundamentals of Microelectronics [Razavi.cls v. 2006]

June 30, 2007 at 13:42

572 (1)

 

 

 

 

572

Chap. 11

Frequency Response

With the values chosen here, the poles are complex. Figure 11.40 plots the frequency response. The ,3-dB bandwidth is approximately equal to 3.5 GHz.

 

0

 

 

 

 

(dB)

−2

 

 

 

 

Response

 

 

 

 

−4

 

 

 

 

 

 

 

 

 

of Frequency

−6

 

 

 

 

−8

 

 

 

 

−10

 

 

 

 

Magnitude

 

 

 

 

−12

 

 

 

 

 

 

 

 

 

 

−14

107

108

109

1010

 

106

 

 

 

Frequency (Hz)

 

 

Figure 11.40

Exercise

For what value of gm do the two poles become real and equal?

Example 11.22

Determine the transfer function of the source follower shown in Fig. 11.41(a), where M2 acts as a current source.

 

 

 

 

CGD1

VDD

 

 

 

 

 

 

 

VDD

RS

X

CDB1

 

 

Vin

 

RS

 

M 1

Vin

M 1

CGS1

Y

Vout

 

 

 

 

 

 

 

 

 

Vout

 

CGD2

CDB2 + CSB1

 

Vb

 

Vb

 

CSB2

 

M

2

 

 

 

CGS2 M 2

 

 

 

 

 

 

 

(a)

 

(b)

 

Figure 11.41

BR

Wiley/Razavi/Fundamentals of Microelectronics [Razavi.cls v. 2006]

June 30, 2007 at 13:42

573 (1)

 

 

 

 

Sec. 11.6

Frequency Response of Followers

573

Solution

Noting that CGS2 and CSB2 play no role in the circuit, we include the transistor capacitances as illustrated in Fig. 11.41(b). The result resembles that in Fig. 11.38, but with CGD2 and CDB2 appearing in parallel with CSB1. Thus, (11.109) can be rewritten as

 

 

 

 

 

 

 

 

 

 

 

 

 

CGS1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Vout

(s) =

 

1 + gm1

s

;

 

 

 

(11.116)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Vin

 

 

 

as2 + bs + 1

 

 

 

 

where

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

a =

RS

[C

GD

1C

GS

1 + (C

GD

1 + C 1)(C

1 + C

GD

2 + C 2)] (11.117)

 

 

gm1

 

 

 

 

 

 

 

GS

SB

 

 

DB

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

b = RSCGD1 +

CGD1 + CSB1 + CGD2 + CDB2

:

 

(11.118)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

gm1

 

 

 

 

 

 

Exercise

Assuming M1 and M2 are identical and using the transistor parameters given in Example 11.18, calculate the pole frequencies.

11.6.1 Input and Output Impedances

In Chapter 5, we observed that the input resistance of the emitter follower is given by r + ( + 1)RL, where RL denotes the load resistance. Also, in Chapter 7, we noted that the source follower input resistance approaches infinity at low frequencies. We now employ an approximate but intuitive analysis to obtain the input capacitance of followers.

Consider the circuits shown in Fig. 11.42, where C and CGS appear between the input and output and can therefore be decomposed using Miller's theorem. Since the low-frequency gain is equal to

 

C µ

VCC

 

CGD

VDD

 

 

 

 

 

X

Q 1

 

X

CDB

 

 

= CGS

 

M 1

CXY = C π

Y

CXY

Y

 

 

 

 

 

R L

CL

 

R L

CL+ CSB

 

(a)

 

 

(b)

 

Figure 11.42 Input impedance of (a) emitter follower and (b) source follower.

Av =

RL

;

(11.119)

1

 

 

 

 

 

 

RL +

 

 

 

 

 

gm

 

 

BR

Wiley/Razavi/Fundamentals of Microelectronics [Razavi.cls v. 2006]

June 30, 2007 at 13:42

574 (1)

 

 

 

 

574

 

 

Chap. 11

Frequency Response

we note that the “input” component of

C or CGS is expressed as

 

CX = (1 , Av)CXY

(11.120)

 

1

 

(11.121)

 

=

 

CXY :

 

1 + gmRL

Interestingly, the input capacitance of the follower contains only a fraction of C or CGS, depending on how large gmRL is. Of course, C or CGD directly adds to this value to yield the total input capacitance.

Example 11.23

Estimate the input capacitance of the follower shown in Fig. 11.43. Assume 6= 0.

VDD

VinM 1

Vb

M 2

Figure 11.43

Solution

From Chapter 7, the low-frequency gain of the circuit can be written as

Av =

rO1jjrO2

:

(11.122)

 

1

 

 

 

 

rO1jjrO2 +

 

 

 

 

 

gm1

 

 

Also, from Fig. 11.42(b), the capacitance appearing between the input and output is equal to CGS1, thereby providing

Cin = CGD1

+ (1 , Av)CGS1

 

(11.123)

= CGD1

+

 

1

CGS1:

(11.124)

 

 

1 + gm1

(rO1jjrO2)

 

 

 

 

For example, if gm1(rO1jjrO2) 10, then only 9% of CGS1 appears at the input.

Exercise

Repeat the above example if = 0.

Let us now turn our attention to the output impedance of followers. Our study of the emitter follower in Chapter 5 revealed that the output resistance is equal to RS =( +1)+1=gm. Similarly, Chapter 7 indicated an output resistance of 1=gm for the source follower. At high frequencies, these circuits display an interesting behavior.

Consider the followers depicted in Fig. 11.44(a), where other capacitances and resistances are neglected for the sake of simplicity. As usual, RS represents the output resistance of a preceding stage or device. We first compute the output impedance of the emitter follower and subsequently

BR

Wiley/Razavi/Fundamentals of Microelectronics [Razavi.cls v. 2006]

June 30, 2007 at 13:42

575 (1)

 

 

 

 

Sec. 11.6

Frequency Response of Followers

 

 

 

 

575

 

VCC

 

VDD

RS

 

 

 

RS

RS

 

 

 

 

 

 

C π

r π Vπ

 

gm Vπ

Vin

Q 1

Vin

M 1

 

C π

 

CGS

 

 

 

 

 

 

 

 

 

 

 

I X

VX

 

Z out

 

Z out

 

 

 

 

 

 

 

 

 

 

 

(a)

 

 

(b)

 

 

Figure 11.44 (a) Output impedance of emitter and source followers, (b) small-signal model.

let r ! 1 to determine that of the source follower. From the equivalent circuit in Fig. 11.44(b), we have

(IX + gmV ) r jj 1 = ,V C s

and also

(IX + gmV )RS , V = VX :

Finding V from (11.125)

V = ,IX r

r C s + + 1

and substituting in (11.126), we obtain

VX = RSr C s + r + RS :

IX r C s + + 1

(11.125)

(11.126)

(11.127)

(11.128)

As expected, at low frequencies VX =IX = (r + RS)=( + 1) 1=gm + RS=( + 1). On the other hand, at very high frequencies, VX =IX = RS, a meaningful result considering that C becomes a short circuit.

The two extreme values calculated above for the output impedance of the emitter follower can be used to develop greater insight. Plotted in Fig. 11.45, the magnitude of this impedance falls with ! if RS < 1=gm + RS=( + 1) or rises with ! if RS > 1=gm + RS=( + 1). In analogy with the impedance of capacitors and inductors, we say Zout exhibits a capacitive behavior in the former case and an inductive behavior in the latter.

 

 

Zout

 

 

 

 

Zout

 

R S

 

+

1

 

 

 

 

 

 

 

R S

 

β + 1

g m

 

 

R S

 

 

 

 

 

 

 

1

 

 

 

 

 

R S

 

 

+

 

 

 

 

 

 

 

β + 1

g m

 

 

 

 

 

 

 

ω

 

 

ω

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

(a)

 

 

 

 

 

 

(b)

Figure 11.45 Output impedance of emitter follower as a function of frequency for (a) small RS and (b) large RS.

Which case is more likely to occur in practice? Since a follower serves to reduce the driving impedance, it is reasonable to assume that the follower low-frequency output impedance is lower

BR

Wiley/Razavi/Fundamentals of Microelectronics [Razavi.cls v. 2006]

June 30, 2007 at 13:42

576 (1)

 

 

 

 

576

Chap. 11

Frequency Response

than RS.17 Thus, the inductive behavior is more commonly encountered. ( It is even possible that the inductive output impedance leads to oscillation if the follower sees a certain amount of load capacitance.)

The above development can be extended to source followers by factoring r from the numerator and denominator of (11.128) and letting r and approach infinity:

VX =

RSCGSs + 1;

(11.129)

IX

CGSs + gm

 

where ( + 1)=r is replaced with gm, and C with CGD. The plots of Fig. 11.45 are redrawn for the source follower in Fig. 11.46, displaying a similar behavior.

Zout

Zout

 

1

R S

 

g m

 

 

 

R S

1

 

g m

 

ω

ω

 

(a)

 

(b)

Figure 11.46 Output impedance of source follower as a function of frequency for (a) small RS and (b) large RS.

The inductive impedance seen at the output of followers proves useful in the realization of “active inductors.”

Example 11.24

Figure 11.47 depicts a two-stage amplifier consisting of a CS circuit and a source follower. Assuming 6= 0 for M1 and M2 but = 0 for M3, and neglecting all capacitances except CGS3, compute the output impedance of the amplifier.

Vb

 

VDD

VDD

M 2

 

M 3

r O1 r O2

 

 

 

 

M 3

Vin

M 1

Vout

 

Z out

(a)

(b)

Figure 11.47

Solution

The source impedance seen by the follower is equal to the output resistance of the CS stage, which is equal to rO1jjrO2. Assuming RS = rO1jjrO2 in (11.129), we have

VX =

(rO1jjrO2)CGS3s + 1:

(11.130)

IX

CGS3s + gm3

 

17If the follower output resistance is greater than RS, then it is better to omit the follower!

BR

Wiley/Razavi/Fundamentals of Microelectronics [Razavi.cls v. 2006]

June 30, 2007 at 13:42

577 (1)

 

 

 

 

Sec. 11.7

Frequency Response of Cascode Stage

577

Exercise

Determine Zout in the above example if 6= 0 for M1-M3.

11.7 Frequency Response of Cascode Stage

Our analysis of the CE/CS stage in Section 11.4 and the CB/CG stage in Section 11.5 reveals that the former provides a relatively high input resistance but it suffers from Miller effect whereas the latter exhibits a relatively low input resistance but it is free from Miller effect. We wish to combine the desirable properties of the two topologies, obtaining a circuit with a relatively high input resistance and no or little Miller effect. Indeed, this thought process led to the invention of the cascode topology in the 1940s.

Consider the cascodes shown in Fig. 11.48. As mentioned in Chapter 9, this structure can be

VCC

 

 

VDD

 

 

RL

Vout

Vb1Q 2

C 1

RS Y

Vin Q 1

X

(a)

Figure 11.48 (a) Bipolar and (b) MOS cascode stages.

RL

Vout

 

Vb

M 2

 

CGD1

Y

 

Vin

RS

 

X

M

1

 

 

(b)

viewed as a CE/CS transistor, Q1 or M1, followed by a CB/CG device, Q2 or M2. As such, the circuit still exhibits a relatively high (for Q1) or infinite (for M1) input resistance while providing a voltage gain equal to gm1RL.18 But, how about the Miller multiplication of C 1 or CGD1? We must first compute the voltage gain from node X to node Y . Assuming rO = 1 for all transistors, we recognize that the impedance seen at Y is equal to 1=gm2, yielding a small-signal gain of

Av;XY = vY

 

(11.131)

vX

 

 

= ,gm1

:

(11.132)

gm2

 

 

In the bipolar cascode, gm1 = gm2 (why?), resulting in a gain of ,1. In the MOS counterpart, M1 and M2 need not be identical, but gm1 and gm2 are comparable because of their relatively weak dependence upon W=L. We therefore say the gain from X to Y remains near ,1 in most

18The voltage division between RS and r 1 lowers the gain slightly in the bipolar circuit.

BR

Wiley/Razavi/Fundamentals of Microelectronics [Razavi.cls v. 2006]

June 30, 2007 at 13:42

578 (1)

 

 

 

 

578

Chap. 11 Frequency Response

practical cases, concluding that the Miller effect of CXY = C 1 or CGD1 is given by

CX = (1 , Av;XY )CXY

(11.133)

2CXY :

(11.134)

This result stands in contrast to that expressed by (11.56), suggesting that the cascode transistor breaks the trade-off between the gain and the input capacitance due to Miller effect.

Let us continue our analysis and estimate the poles of the cascode topology with the aid of Miller's approximation. Illustrated in Fig. 11.49 is the bipolar cascode along with the transis-

 

VCC

 

 

 

RL

 

Vout

 

 

 

Vb1

Q 2

CCS2 + C µ2

 

 

RS

Y

 

 

X

 

 

Vin

Q 1

CCS1

+ C π2+ 2C µ1

C π1+ 2C µ1

 

 

 

 

Figure 11.49 Bipolar cascode including transistor capacitances.

tor capacitances. Note that the effect of C 1 at Y is also equal to (1 , A,1 )C 1

Associating one pole with each node gives

 

 

 

 

v;XY

 

 

 

 

 

j!p;X j =

 

 

 

1

 

 

 

 

 

 

 

 

 

 

 

 

(RSjjr 1)(C 1

+ 2C 1)

 

j!p;Y j =

 

 

 

1

 

 

 

 

 

1

(CCS1 + C 2 + 2C 1)

 

 

 

 

 

 

 

gm2

 

 

 

 

 

j!p;outj =

1

 

 

:

 

 

RL(CCS2

 

 

 

 

 

+ C 2)

= 2C 1.

(11.135)

(11.136)

(11.137)

It is interesting to note that the pole at node Y falls near the fT of Q2 if C 2 CCS1 + 2C 1. Even for comparable values of C 2 and CCS1 + 2C 1, we can say this pole is on the order of fT =2, a frequency typically much higher than the signal bandwidth. For this reason, the pole at node Y often has negligible effect on the frequency response of the cascode stage.

The MOS cascode is shown in Fig. 11.50 along with its capacitances after the use of Miller's approximation. Since the gain from X to Y in this case may not be equal to ,1, we use the actual value, ,gm1=gm2, to arrive at a more general solution. Associating one pole with each node, we have

j!p;X j =

 

 

 

1

 

 

 

 

(11.138)

 

 

 

 

 

 

 

 

 

 

 

gm1

CGD1]

 

 

 

 

 

 

 

 

 

RS[CGS1 + 1 + gm2

 

 

 

j!p;Y j =

 

 

 

 

 

1

 

 

 

(11.139)

1

 

 

 

gm2

CGD1

 

 

 

 

 

 

 

 

 

gm2

[CDB1

+ CGS2 +

1 + gm1

+ CSB2]

j!p;outj =

 

 

1

 

:

 

 

 

(11.140)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

RL(CDB2 + CGD2)

 

 

 

 

 

BR

Wiley/Razavi/Fundamentals of Microelectronics [Razavi.cls v. 2006]

June 30, 2007 at 13:42

579 (1)

 

 

 

 

Sec. 11.7

Frequency Response of Cascode Stage

 

 

 

 

 

 

 

 

 

579

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

VDD

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Vb

 

R L

 

 

 

 

 

 

 

Vout

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

M 2

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

CGD2 + CDB2

 

 

 

 

 

Vin

 

 

RS

 

X

 

Y

 

 

 

 

 

 

 

 

 

 

 

 

 

g m2

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

M 1

 

 

 

 

CGS2 + CGD1 (1+

) + CDB1

+ CSB2

 

CGS1

+ CGD1

(1+

g m1

)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

g m1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

g m2

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Figure 11.50 MOS cascode including transistor capacitances.

We note that !p;Y is still in the range of fT =2 if CGS2 and CDB1 + (1 + gm2=gm1)CGD1 are comparable.

Example 11.25

The CS stage studied in Example 11.18 is converted to a cascode topology. Assuming the two transistors are identical, estimate the poles, plot the frequency response, and compare the results with those of Example 11.18. Assume CDB = CSB.

Solution

Using the values given in Example 11.18, we write from Eqs. (11.138) (11.139), and (11.140):

j!p;X j = 2 (1:95 GHz)

(11.141)

j!p;Y j = 2 (1:73 GHz)

(11.142)

j!p;outj = 2 (442 MHz):

(11.143)

Note that the pole at node Y is quite lower than fT =2 in this particular example. Compared with the Miller approximation results obtained in Example 11.18, the input pole has risen considerably. Compared with the exact values derived in that example, the cascode bandwidth (442 MHz) is nearly twice as large. Figure 11.51 plots the frequency response of the cascode stage.

Exercise

Repeat the above example if the width of M2 and hence all of its capacitances are doubled. Assume gm2 = (100 ),1.

Example 11.26

In the cascode shown in Fig. 11.52, transistor M3 serves as a constant current source, allowing M1 to carry a larger current than M2. Estimate the poles of the circuit, assuming = 0.

Solution

Transistor M3 contributes CGD3 and CDB3 to node Y , thus lowering the corresponding pole magnitude. The circuit contains the following poles:

j!p;X j =

1

 

(11.144)

gm1

 

 

CGD1]

 

RS[CGS1 + 1 + gm2

BR

Wiley/Razavi/Fundamentals of Microelectronics [Razavi.cls v. 2006]

June 30, 2007 at 13:42

580 (1)

 

 

 

 

580

Chap. 11

Frequency Response

 

30

 

 

 

 

(dB)

20

 

 

 

 

Response

 

 

 

 

10

 

 

 

 

 

 

 

 

 

of Frequency

0

 

 

 

 

−10

 

 

 

 

Magnitude

−20

 

 

 

 

 

 

 

 

 

 

−30

107

108

109

1010

 

106

 

 

 

Frequency (Hz)

 

 

Figure 11.51

 

 

 

 

VDD

Vb2

 

M 3

RL

 

 

Vout

 

 

Vb1

 

 

 

M 2

 

Vin

RS

Y

 

 

X

M

1

 

 

 

Figure 11.52 .

j!p;Y j =

 

 

 

 

1

 

 

(11.145)

 

 

 

 

 

 

 

1

 

 

gm2

 

 

 

 

 

 

 

 

 

 

gm2

[CDB1

+ CGS2

+ 1 + gm1

CGD1

+ CGD3 + CDB3]

j!p;outj =

 

 

1

 

:

 

(11.146)

 

 

 

 

 

RL(CDB2 + CGD2)

 

 

 

 

 

 

Note that !p;X also reduces in magnitude because the addition of M3 lowers ID2 and hence gm2.

Exercise

Calculate the pole frequencies in the above example using the transistor parameters given in Example 11.18 for M1-M3.

From our studies of the cascode topology in Chapter 9 and in this chapter, we identify two important, distinct attributes of this circuit: (1) the ability to provide a high output impedance and

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