Millimeter-Wave Bist Paper
Transcript of Millimeter-Wave Bist Paper
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Millimeter-Wave BiST and BiSC using a High-
Definition Sub-Ranged Detector in 90nm CMOSSleiman Bou Sleiman
1, Amneh Akour
1,2, Waleed Khalil
2, Mohammed Ismail
1,2
Analog VLSI Lab1
and ElectroScience Lab2, ECE Department
The Ohio State University
Columbus, OH{bousles, akoura, khalil, ismail}@ece.osu.edu
AbstractA wideband CMOS mm-Wave amplitude detector for
on-chip self-test and calibration is presented. The high-
conversion-gain detector enables accurate on-chip amplitude
measurements and allows for the prediction of key RF
parameters. The detector operates across the 60GHz band and
achieves a dynamic range of 0-0.5V and a sensitivity of -9V/V.
The detectors practical use in mm-wave Built-in-Self-Test
(BiST) and Built-in-Self-Calibration (BiSC) circuits is
demonstrated using a 60 GHz CMOS LNA. Simulation results
show that the LNA gain, compression point, and intermodulation
distortion are predicted with minimal error. The detector and
LNA are built in IBMs 90nm CMOS technology.
I. INTRODUCTION
dvances in semiconductor technology allowed for the
implementation of high performance RF blocks in
CMOS, opening the doors for a full System-on-Chip
(SoC) solution. More recently, CMOS technology is sought
for the millimeter-Wave (mmW) regime albeit many
challenges and critical shortcomings with respect to SoC
integration. mmW and RF circuits, unlike the more robust
digital circuits, suffer from low yield due to process, power
supply, and temperature (PVT) variations and require several
expensive silicon cycles to meet their specifications.
Additionally, parasitics more pronounced at mmW than at
RF quickly come into play and increase the adverse
variability and hence the performance uncertainty of a given
chip. For this reason, the design of mmW/RF IC blocks in
platform baseband SoCs has so far been restricted.
Countering the advantages of decreasing feature size into
the nanometer regime, process variations even in digital
circuits are getting more amplified. This necessitates the
need for a new approach to RF and mmW design through
integration of on-chip Built-in-Self-Test (BiST) and Built-in-
Self-Calibration (BiSC) circuits. While highly beneficial in
GHz RF circuits, BiST(SC) have not been widely
implemented as design complexity was contained by
allowing for overdesign and some area/power sacrifices.
However in mmW and as devices scale down and parasitics
play ever-critical roles, the design complexity becomes very
quickly unbound. Two key components of the new design paradigm are block/system self-awareness and block/system
programmability. The first component is achieved with
accurate and efficient BiST as a precursor to implementing the
latter by leveraging the more robust digital capabilities of
SoCs. In other words, this is achieved using digitally-assisted
mmW circuits within calibration loops to alleviate mmW
shortcomings (Fig. 1.)
In Section II, we present a compact, non-invasive, and
efficient mmW amplitude detector serving the needs for both
BiST and BiSC. In Section III, we verify our detector using a
60 GHz LNA as circuit-under-test/calibration (CUT/C).
II. DETECTORDESIGN
A. Detector RequirementsTo enable testing and measurements of single blocks or an
aggregate of blocks in a transceiver, multiple detectors can be
inserted to extract the signal amplitudes at different points or
conversely a single detector with switches connecting it to thevarious measurement points. Opting for the first configuration,
we need to design area-efficient detectors whereas if targeting
the second, we need to have a very wide dynamic range
detector, as the signal varies considerably along the chain.
Other requirements include low power, wideband operation,
and more importantly high input impedance so as not to load
the circuit it connects to. Another important consideration
when dealing with complete on-chip measurements is the need
for high RF-to- DC conversion gain. A high conversion gain
is very desirable for self-test and self-calibration as it eases the
requirements on the digitizing ADC (see Fig. 1.) However,
with decreasing power supply voltages, an increase in
conversion gain limits the dynamic range. Previous detectors
described in the literature [1]-[7] do not offer high resolutionand most suffer from a low RF-to-DC conversion gain of
around -1V/V (see Fig. 2, [7] uses a 3.3V supply). In the next
section, we present a detector that fulfils the aforementioned
requirements, and to the authors best knowledge, the
implementation presented is the first to operate at mm-Wave
frequencies.
Fig. 1. Radio transceiver architecture with possible BiST and BiSC
configurations using loopback.
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B. Proposed Detector ArchitectureOur proposed architecture is shown in Fig. 3. It is an
implementation of an architecture similar to [1], however it
does not employ a feedback resistor for biasing but depends
on a separate gate biasing circuit. The input transistor is biased
in the subthreshold region and its saturated drain current can
be expressed as [9]
T
GS
n
0DnnV
Vexp
L
WII (1)
where ID0 is a current constant independent of gate-to-source
voltage, (W/L)n is the aspect ratio of the NMOS transistor, n is
a process dependent term related to depletion region
characteristics [4], and VT is the thermal voltage.
Superimposing a small sinusoidal input voltage, Vacos(t) on
the gate bias, Vbias, the following power series approximation
of the current equation holds:
)t2cos(nV2
V)tcos(
nV
V
nV2
V1I
)t(cosnV
V
2
1)tcos(
nV
V1I
nV
)tcos(VexpI
nV
)tcos(VVexp
L
WII
2
T
a
T
a
2
T
a0B
2
2
T
a
T
a0B
T
a0B
T
abias
n
0Dn
(2)
whereIB0 [=ID0(W/L)nexp(Vbias/nVT)] is the dc-bias current ofthe transistor. Initially charged to VDD, DCout is then
discharged by the drain current In through the NMOS
transistor. This creates a negative I-V relationship with respect
to an increase in the mmW signal amplitude. As the detector
output is low-pass filtered by the RC load, it reacts to the dc
component ofIn given by2
T
a0BnDC
nV2
V1II (4)
A high conversion gain can then be achieved with proper
device sizing and biasing. However, in order to achieve a wide
dynamic (i.e. amplitude) range, the detector should employ
several modes of operation each covering an overlapping sub-
range of amplitudes. This is achieved by appropriatelychanging the gate biasing of the input NMOS device: by
decreasing the gate bias, higher amplitude signals are needed
to turn the input transistor on. Using a 3-bit programmable
mode select voltage bias circuit, and setting the overlap to
50mVamp (Vbias=35mV), we achieve 8 modes of operation
covering a wide signal range from 0 to 0.5Vamp. As shown in
Fig. 4, the linear region of the response is between 0.2V and
1V (for a 1.2V supply) providing a slope of around -9V/V . To
reduce the loading impact of the detector, its input impedance
is kept greater than 800 across the 60 GHz band. Further,
the detectors wideband operation is also validated across the
60 GHz band. The complete circuit is built in IBMs 90nm
CMOS technology. As test and calibration do not need to run
all the time but only intermittently, low power requirements
(a)
(b)Fig. 3. The proposed mmW-amplitude detector: (a) Circuit core, (b)
Programmable mode select
]Fig. 4. mmWave-to-dc response of the proposed mmW-amplitudedetector
IN
DCout
Vbias
Pbias
d
VDD
Detector Core
VDD
Vbias
A1 A2 A3 A7
Thermometer-code
A7..1
Mode2..0
Programmable Mode Select
0
0.2
0.4
0.6
0.8
1
1.2
0 0.1 0.2 0.3 0.4 0.5
DCDetectorOutput(V)
High-Frequency Signal Amplitude (V)[55-65 GHz]
MODE0 MODE1 MODE2
MODE3 MODE4 MODE5
MODE6 MODE7
Fig. 2. Response of various detectors in literature
0
0.20.4
0.6
0.8
1
1.2
1.4
1.6
0 0.5 1
DCOutput(V)
Input RF Amplitude (V)
Huang
wang
Fan
Valdes
Jonsson
[6][4][8][7]
[1,2]
50mV
-9V/V
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are not critical for the detector circuits since the detector and
its bias circuit can be simply turned off using switches or
power gating.
C. Detector usage in BiST and BiSCThe detector can be used to quantify a number of transceiver
parameters such as gain, linearity, compression points, and
even IQ mismatchas presented in [10]. Since the detector is
followed by an ADC, a quantized detector response can eitherbe saved in a lookup table or fitted into an equation: possibly
as a function of slope (-9V/V), mode (50mV shifts), or
piecewise linear reconstruction to enable prediction of signal
amplitude. For example, using an 8-bit ADC and saving the
first modes response in a lookup table, a quantized detector
output of 128 (= 256/2, DCout = 1.2/2 = 0.6V) equates to a
0.09Vamp signal in mode0, +50mV per additional mode (ormore accurately +60mVbetween mode0 and mode1, +50mV
hereafter).
In the context of a self-calibration loop, the detector can be
used as an optimization indicator, e.g. following an
optimization step; a decrease inDCoutof a detector monitoring
a specific circuit node indicates an increase in the amplitude of
the signal at that node.
III. BIST AND CALIBRATION OF A60GHZ LNA
The LNA is the first gain stage in the receiver path and
hence needs to be designed to meet tight specifications for the
whole receiver. At 60 GHz, the design of the LNA becomes
very challenging as even the smallest parasitics or disruptions
in operating conditions can completely alter the circuit
performance.
In the following we demonstrate the feasibility of the
proposed detector for test and calibration of the LNA under
test, shown in Fig. 5 [11].
A. Built-in-Self-TestThe accuracy of the proposed detector is verified byconnecting it to a 60 GHz LNA and applying known input
amplitudes. It is worth noting that the detector is verified not
to load the LNA, a critical aspect of this design (see Fig. 7). A
complete on-chip solution to such a BiST configuration
requires loopback between transmitter and receiver chains. In
our demonstration, two detectors are used to sense the input
and output signals and output a dc voltage which is then
quantized (8-bits) and analyzed (see Fig. 6). The detectors
biasing is dynamically adjusted when its output is not
between 0.2 and 1V. In this example, we measure the gain
and compression point by sweeping the input amplitude and
predicting both the LNAs input and output signal amplitudes.
At each sweep instance, a gain value can be computed and
after a sufficient number of iterations, a gain curve is obtained
where the 1dB compression point is readily deduced.
Knowledge of the LNA gain enables more sophisticated tests,
such as two-tone tests for intermodulation (IM) measurements.
The IM3 amplitude can be extracted from the detector output
by measuring the input and output of the LNA and comparing
the latter with the expected output given no distortion (=
inputpredicted gain): the discrepancy between these twosignals is attributed to the IM amplitude. It should be noted
that in the case of two-tone tests, DCout becomes a low-frequency oscillating signal whose mean is to be considered in
the IM3 extraction [10]. The results of this sweep showing the
actual and predicted values using the detector are shown in
Fig. 8. It can be verified that the detector is able to match the
real gain with a maximum 0.3dB error, the 1dB compression
point and IIP3 to within 0.4dB, shown below in Table I.Table I
Actual vs Predicted values for LNA
Actual Predicted Error
Gain, A [dB] 10.14 10.45 0.3
P1dB [dBm] -9.73 -9.32 0.4
IIP3 [dBm] 3.9 4.3 0.4
B. Built-in-Self-CalibrationTo satisfy the growing number of corners, LNAs and
other mmW circuits need to incorporate some dynamic, rather
than static, structures that allow their operating points to adjust
and guarantee optimal operation under varying conditions, as
shown in Fig. 9. To enable the calibration loop, the previous
BiST setup is augmented with an optimization block that runs
a specific algorithm for each CUT/C. In the simple case of a
single tuning knob, the BiSC can perform an algorithm similar
to Fig. 10 which sweeps through the possible digital codes,
while holding the input constant, and keeps track of the
detector output: the code resulting in the minimum-
IN
Vbias
VDD
MatchingCircuit
CPW
Vbias
VDD
MatchingCircuit
CPW
Vbias
VDD
MatchingCircuit
CPW
MatchingCircuit OUT
Fig. 5. Three-stage cascade common-source LNA with interstage
matching
Fig 6. BiST and BiSC setup for the LNA
Fig. 7. Effect of the detectors on the LNA gain, input match, and NoiseFigure
CUT(LNA)
DET DET
BiST BiSCcontrolled
loopback
mmW/RF
Digital
-25
-20
-15
-10
-5
0
5
10
5.50E+10 6.00E+10 6.50E+10
dB S21 S21
NF NF
S11 S11
with detector w/o detector
55GHz 60GHz 65GHz
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DCout/maximum-mode is retained to be applied to the circuit
once the calibration run is finished.The LNA therefore needs to include tuning knobs
programmable voltage-biasing in [11]and possibly variable
passives for matching as in [12].
IV. CONCLUSION AND FUTURE WORK
In this paper, we present the design and implementation of a
wideband mmW amplitude detector largely suited for BiST
and BiSC. The detector is shown to measure, with certain
accuracy, key parameters of a 60 GHz LNA. Ongoing work to
embed programmability in the LNA will enable closing of the
calibration loop.
REFERENCES[1] F. Jonsson, H. Olsson, RF detector for on -chip amplitude
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Fig. 9. Digitally-programmable mmW/RF designed with codes
covering a range of operations always including an optimal point
Fig. 10. Example of a simple calibration algorithm running in the
digital part of the SoC and controlling the mmW/RF circuit
Fig. 8. Measurements for LNA gain and linearity. Left: simulated and predicted gain curve, and gain compression point. Right: fundamental and
IM3 component curves, dotted lines show the LNAs simulated fundamental/IM3 behavior, solid lines are extended data-fitted lines from
extracted fundamental/IM3 amplitudes.
-8
-7
-6
-5
-4
-3
-2
-1
0
1
2
-18 -16 -14 -12 -10 -8 -6
OutputSign
alPower(dBm)
Simulated Gain Curve
Predicted Gain Curve
-1dB Line, w.r.t. predicted curve-45
-35
-25
-15
-5
5
15
-20 -15 -10 -5 0 5
OutputSign
alPower(dBm)
Series1
Series2
Linear (trend)
Linear (Series4)
Input Signal Power (dBm)
FundamentalIM3Predicted fund/IM3Simulated fund/IM3
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