Differential-mode charge transfer amplifier

Amplifiers – With periodic switching input-output

Reexamination Certificate

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Details

C330S258000, C327S124000, C327S554000

Reexamination Certificate

active

06249181

ABSTRACT:

BACKGROUND OF THE INVENTION
1. The Field of the Invention
The present invention relates to systems and methods for amplifying electrical signals. More specifically, the present invention relates to systems and methods for performing amplification by charge transfer.
2. The Prior State of the Art
There are many circuits and methods conventionally available for amplifying an electrical signal. One type of amplifier is called a charge transfer amplifier. Charge transfer amplifiers operate on the principle of capacitive charge sharing. Voltage amplification is achieved by transferring a specific amount of charge between appropriately sized capacitors through an active device.
FIG. 1
illustrates a charge transfer amplifier
100
that utilizes an nMOS transistor N
1
to transfer charge between capacitors CT and CO. The operation of the nMOS charge transfer amplifier
100
will now be described in order to illustrate the basic principle of charge transfer amplification.
The nMOS charge transfer amplifier
100
operates in a cycle of three phases including a reset phase, a precharge phase, and an amplify phase.
FIG. 2
is a signal timing diagram for two input signals S
1
and S
2
with respect to the cycle phase that the nMOS charge transfer amplifier
100
is operating in whether that phase be (a) the reset phase, (b) the precharge phase or (c) the amplify phase. The two input signals S
1
and S
2
control corresponding switches S
1
and S
2
of FIG.
1
.
The cycle begins with the (a) reset phase in which the signal S
1
is high indicating that the switch S
1
is closed, and in which the signal S
2
is low indicating that the switch S
2
is open. Since the switch S
1
is closed, the upper terminal of capacitor CT (i.e., node A) is discharged through the switch S
1
to voltage Vss while the switch S
2
is open thus isolating the nMOS transistor N
1
as well as node B and the upper terminal of capacitor CO from the precharge voltage V
PR
thereby preventing static current flow through the nMOS transistor N
1
.
After the reset phase is the (b) precharge phase in which the signal S
1
is low indicating that switch S
1
is open, and in which the signal S
2
is high indicating that the switch S
2
is closed. Thus, the upper terminal of the capacitor CO (i.e., node B) is charged to the precharge voltage V
PR
. This precharge voltage V
PR
is high enough that current flows from node B to the capacitor CT (and node A) through the nMOS transistor N
1
. For example, if the precharge voltage V
PR
is at least equal to the input voltage V
IN
at the gate of the nMOS transistor N
1
, then the discharge continues until the voltage at the capacitor CT increases to be equal to the input voltage V
IN
minus the threshold voltage (hereinafter “V
TN
”) of the nMOS transistor N
1
. At that point, the nMOS transistor N
1
enters the cutoff region and current flow to the capacitor C
T
substantially ceases. Thus, at the end of the precharge phase, the capacitor CO ideally has a voltage of V
PR
while the capacitor CT has a voltage of V
PR
−V
TN
.
After the precharge phase is the (c) amplify phase in which both signals S
1
and S
2
are low indicating that both switches S
1
and S
2
are open. During the amplify phase, an incrementally positive input voltage change &Dgr;V
IN
at the gate of the nMOS transistor N
1
will cause the nMOS transistor N
1
to turn on thereby allowing current to flow through the nMOS transistor N
1
until the nMOS transistor is again cutoff. For small incrementally positive voltage changes &Dgr;V
IN
, the nMOS transistor N
1
will cutoff when the voltage on upper terminal of the capacitor CT (i.e., node A) increases by the incrementally positive voltage change &Dgr;V
IN
. The amount of charge transferred to the capacitor CT in order to produce this effect is equal to the incrementally positive voltage change &Dgr;V
IN
times the capacitance C
T
of the capacitor CT.
Since the charge &Dgr;V
IN
×C
T
transferred to the capacitor CT came from node B through transistor N
1
, the charge &Dgr;V
IN
×C
T
was drawn from the capacitor CO. Thus, the voltage at the capacitor CO and the output voltage V
OUT
will change by &Dgr;V
IN
×(C
T
/C
0
). If the capacitance C
T
is greater than the capacitance C
0
, amplification occurs.
One advantage of the nMOS charge transfer amplifier
100
is that the voltage gain and power consumption may be controlled by setting the capacitance of the capacitors CO and CT as well as by setting the capacitance ratio C
T
/C
0
.
Another advantage of charge transfer amplifiers in general is that the circuit performance is generally unaffected by the absolute values of the supply voltage Vss and Vdd as long as these voltages permit proper biasing during the reset and precharge phases. In other words, charge transfer amplifiers have high supply voltage scalability in that no changes are needed for a charge transfer amplifier to operate using a wide range of supply voltages Vss and Vdd.
Although the nMOS charge transfer amplifier
100
has these advantages, there are at least two disadvantages to amplifying using the nMOS charge transfer amplifier
100
.
First, amplification only occurs if the input gate voltage change &Dgr;V
IN
is positive. A negative gate voltage change &Dgr;V
IN
would only cause the nMOS transistor N
1
to enter deeper into the cutoff region. Thus, charge transfer between node A and node B would be stifled thereby preventing amplification.
Second, leakage currents inherent in transistor N
1
will alter the expected zero-bias (i.e., no input signal) conditions on capacitors CT and CO during the amplify phase. This leakage current may be caused by current undesirably leaking from the source/drain diffusion regions of the nMOS transistor N
1
into the substrate in which they are formed. Leakage current may also be caused by current flowing between the source and drain terminals of the nMOS transistor N
1
even though the nMOS transistor N
1
is substantially cutoff. Either way, this leakage current effectively produces a voltage error V
ERROR
at the output terminal that introduces amplification error. The voltage error V
ERROR
becomes very large over time and is highly affected by temperature conditions. Instead of ideally producing a proportionally amplified output voltage V
OUT
according to the formula V
OUT
=&Dgr;V
IN
×(C
T
/C
0
), the amplifier would produce an output voltage V
OUT
with an error factor according to the formula V
OUT
=&Dgr;V
IN
×(C
T
/C
0
)−V
ERROR
.
FIG. 3
shows a conventional CMOS charge transfer amplifier
300
that substantially overcomes the above-described limitations of the nMOS charge transfer amplifier
100
. The CMOS charge transfer amplifier
300
includes the nMOS charge transfer amplifier
100
described above. For clarity, the nMOS charge transfer amplifier
100
is shown in
FIG. 3
as being enclosed by a dotted box. The CMOS charge transfer amplifier
300
also includes a partially overlapping pMOS charge transfer amplifier
301
which is shown in
FIG. 3
enclosed by a dashed box for clarity. The pMOS charge transfer amplifier
301
shares the voltage input line
302
, the voltage output line
303
and the precharge line
304
with the nMOS charge transfer amplifier
100
. The pMOS charge transfer amplifier
301
is structured similar to the nMOS charge transfer amplifier
100
except that the pMOS charge transfer amplifier
301
uses a pMOS transistor P
1
instead of an nMOS transistor N
1
for transferring charge between capacitors. Also, node A′ of the pMOS charge transfer amplifier
301
is reset to a high voltage Vdd instead of the low voltage Vss and is capacitively coupled to the high voltage Vdd instead of the low voltage Vss.
The general operation of the pMOS charge transfer amplifier
301
for negative input voltage changes &Dgr;V
IN
is similar to the operation of the nMOS charge transfer amplifier
100
for positive voltage changes &Dgr;V
IN
. Thus, the input signals S
1
and S
2
of
FIG. 2
are used in the operation of the CMOS ch

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