High speed InP-based heterojunction bipolar transistors Mark Rodwell University of California, Santa...
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Transcript of High speed InP-based heterojunction bipolar transistors Mark Rodwell University of California, Santa...
High speed InP-basedheterojunction bipolar transistors
Mark Rodwell
University of California, Santa Barbara
[email protected] 805-893-3244, 805-893-3262 fax
2001 ISCS Conference, October, Tokyo
How to Improve the Bandwidth of Bipolar Transistors ?
collex
Ebc
Ejecollectorbase RR
qI
kTC
qI
kTC
f
2
1
Thinner base, thinner collector higher f , but higher Rbb, Ccb
what parameters are really important in HBTs ?how do we improve HBT performance ?
HBT scaling: transit times
WE
WBC
WEB
x
L E
base
emitter
base
collector
WCreduce Tb by 2:1
b improved 2:1
reduce Tc by 2:1
c improved 2:1
note that Ccb has been doubled ..we had wanted it 2:1 smaller
nbb DT 2/2
satcb vT 2/
2:1 improved device speed: keep G's, R's, I's, V's constant, reduce 2:1 all C's,
's
EC WW ~ Assume
HBT scaling: lithographic dimensions
WE
WBC
WEB
x
L E
base
emitter
base
collector
WC
Ccb/Area has been doubled ..we had wanted it 2:1 smaller…must make area=LeWe 4:1 smallermust makeWe & Wc 4:1 smaller
Everticalcsheet
contact
contactspreadgapbb
L
R
RRRR
2,
Base Resistance Rbb must remain constant Le must remain ~ constant
reduce collector width 4:1reduce emitter width 4:1keep emitter length constant
2:1 improved device speed: keep G's, R's, I's, V's constant, reduce 2:1 all C's,
's
EC WW ~ Assume
HBT scaling: emitter resistivity, current density
WE
WBC
WEB
x
L E
base
emitter
base
collector
WC
Emitter Resistance Rex must remain constantbut emitter area=LeWe is 4:1 smallerresistance per unit area must be 4:1 smaller
increase current density 4:1reduce emitter resistivity 4:1
2:1 improved device speed: keep G's, R's, I's, V's constant, reduce 2:1 all C's,
's
Collector current must remain constantbut emitter area=LeWe is 4:1 smallerand collector area=LcWc is 4:1 smallercurrent density must be 4:1 larger
EC WW ~ Assume
for x 2 improvement of all parasitics: ft, fmax, logic speed…base 2: 1 thinnercollector 2:1 thinneremitter, collector junctions 4:1 narrowercurrent density 4:1 higheremitter Ohmic 4:1 less resistive
Scaling Laws for fast HBTs
Challenges with Scaling:Collector mesa HBT: collector under base Ohmics. Base Ohmics must be one transfer lengthsets minimum size for collector Emitter Ohmic: hard to improve…how ?Current Density: dissipation, reliabilityLoss of breakdownavalanche Vbr never less than collector Egap (1.12 V for Si, 1.4 V for InP) ….sufficient for logic, insufficient for power
emitterbase contact
collectorcontact
SI substrate
InGaAs subcollector
InP collector
InGaAscollector
InP subcollector
InGaAs base
undercutcollector junction
base contactemitter
base contact
SI substrate
base
sub collector
base contact pad
collectorcontact
polymer polymer
collector-base junction
Narrow-mesa with 1E20 carbon-doped base
undercut-collector
transferred-substrate
Transferred-Substrate HBT Process Flow UCSBONR
Ultra-high fmax Transferred-Substrate HBTs
• Substrate transfer provides access to both sides of device epitaxy
• Permits simultaneous scaling of emitter and collector widths
• Maximum frequency of oscillation
• Sub-micron scaling of emitter and collector widths has resulted in record values of extrapolated fmax
• Extrapolation begins where measurements end
• New 140-220 GHz Vector Network Analyzer (VNA) extends device measurement range
0
5
10
15
20
25
30
10 100 1000
Gai
ns,
dB
Frequency, GHz
fmax = 1.1 THz ??
f = 204 GHz
Mason's gain, U
H21
MSG
Emitter, 0.4 x 6 m2
Collector, 0.7 x 6 m2
Ic
= 6 mA, Vce
= 1.2 V
3000 Å collector400 Å base with 52 meV gradingAlInAs / GaInAs / GaInAs HBT
cbbbCRff 8/max
Michelle Lee
140-220 GHz network analysis
HP8510C network analyzer & Oleson Microwave Lab frequency Extenders
GGB waveguide-coupled probes
75-100 GHz network analysis
GGB waveguide-coupled probes HP W-band test set
1-50 GHz network analysis
GGB coax-connectorized probes HP 0.045-50 GHz test set
220 GHz On-Wafer Network AnalysisMiguel Urteaga
0
5
10
15
20
25
30
35
1 10 100Frequency, GHz
MSG
h21
Mason'sGain, U
• Submicron HBTs have very low Ccb (< 5 fF)
• HBT S12 is very small
• Standard 12-term VNA calibrations do not correct S12 background error due to probe-to-probe coupling
Solution
Embed transistors in sufficient length of transmission line to reduce coupling
Place calibration reference planes at transistor terminals
Line-Reflect-Line Calibration
Standards easily realized on-wafer
Does not require accurate characterization of reflect standards
Characteristics of Line Standards are well controlled in transferred-substrate microstrip wiring environment
Accurate Transistor Measurements Are Not Easy
Transistor in Embedded in LRL Test Structure
230 m 230 m
Corrupted 75-110 GHz measurements due toexcessive probe-to-probe coupling
140 150 160 170 180 190 200 210 220
freq, GHz
-0.15
-0.10
-0.05
0.00
0.05
0.10
0.15
0.20
0.25
0.30
freq (75.00GHz to 110.0GHz)
Can we trust the calibration ?
freq (140.0GHz to 220.0GHz)
S11 of throughAbout –40 dB
140-220 GHz calibration looks OK75-110 GHz calibration looks Great
S11 of openAbout 0.1 dB / 3o error
dBS21 of through line is off by less than 0.05 dB
S11 of openS11 of short S11 of through
75 80 85 90 95 100 105 110
freq, GHz
-70
-65
-60
-55
-50
-45
-40
Probe-Probe couplingis better than –45 dB
Miguel Urteaga
Submicron transferred-substrate HBTs
0.25 m emitter-base junction
0.4 m Schottky collector
Emitter: 0.3 x 18 m2, Collector: 0.7 x 18.6 m2
Ic = 5 mA, Vce = 1.1 V
Submicron InAlAs/InGaAs HBTs: Unbounded (?!?) Unilateral power gain 45-170 GHz
Gains are high at 200 GHzbut fmax can’t be determined
1E10 1E11 1E12
Freq.
-5
0
5
10
15
20
25
30
35
40
RF G
ains
U
MAG/MSG
h21
unbounded U
UCSBONR
emitter
collector
Miguel Urteaga
Negative Unilateral Power Gain ???
YES, if denominator is negative
This may occur for device with a negative output conductance (G22) or some positive feedback (G12)
12212211
2
1221
GGGG4
YY
U
1221L2211
2
1221
GGGGG4
YY
U
2-portNetwork G L
Select GL such that denominator is zero:
Can U be Negative?
What Does Negative U Mean?
Device with negative U will have infinite Unilateral Power Gain with the addition of a proper source or load impedance
AFTER Unilateralization• Network would have negative output resistance
• Can support one-port oscillation
• Can provide infinite two-port power gainU
Simple Hybrid- HBT model will NOT show negative U
Ccb Cancellation by Collector Space-Charge
collector space-charge layer
cbV
sat
cc
cbccb
base
v
TI
VT
A
V
Q
2
cb
cc
ccb V
IT
AC
1.8
2
2.2
2.4
2.6
2.8
0 1 2 3 4 5 6 7
IC, mA
measured0.64 fF decrease
Ccb
tota
l
Ic
Collector space charge screens field, Increasing voltage decreases velocity, modulates collector space-chargeoffsets modulation of base chargeCcb is reduced
Moll & Camnitz, Betser and Ritter
175 GHz Single-Stage AmplifierSubmicron HBT Program
UCSBMiguel Urteaga
-20
-15
-10
-5
0
5
10
140 150 160 170 180 190 200 210 220
S21S11S22
dB
Freq. (GHz)
0.2pF
50 301.2ps
50
300.2ps
801.2ps
0.6ps
801.2ps
50
IN
OUT
6.3 dB gain at 175 GHz
295 GHz f, & fmax HBT UCSBYoram Betser
Emitter 1 x 8 m2, Collector 2 x 8.5 m2.0
10
20
30
40
50
1 10 102
Gai
ns
(dB
)
Frequency (GHz)
h21
U
VCE
= 1 V, JC = 1.5 mA/um2
fMAX
= 295 GHz
f = 295 GHz
2000 Å collector300 Å base with 52 meV gradingAlInAs / GaInAs / GaInAs HBT
1E9 1E10 1E11 1E12
freq, Hz
-20
-15
-10
-5
0
5
10
15
20
dB(h
21)
UdB
(sho
rt..S
(2,1
))
m1freq=303.0GHzdB(short..S(2,1))=0.000
m1
m2freq=165.0GHzdB(short..S(2,1))=0.000
m2
0
1
2
3
4
5
6
7
8
0 1 2 3 4 5 6
Ic - V
ce characteristics
I c (m
A)
Vce
(volts)
IB in steps
of 20 uA
Fast InP DHBTs
f= 165 GHz; fmax = 303 GHz
5 V breakdown at 105 A/cm2
>9 V at 2*104 A/cm2
UCSBpk SundararajanM Dahlstrom
1x 8 micron emitter, 2x 10 micron collector
3 kÅ collector, 400 Å base
1E9 1E10 1E11 1E12
freq, Hz
-20
-15
-10
-5
0
5
10
15
20
dB(h
21)
UdB
(sho
rt..S
(2,1
))
m1freq=216.0GHzdB(short..S(2,1))=-1.086E-10
m1
f= 216 GHz;fmax = 210 GHz
0
2 104
4 104
6 104
8 104
1 105
0 1 2 3 4 5
Jc - V
ce characteristics
J c (A
/cm
2)
Vce
(volts)
4 V breakdown at 105 A/cm2
>6 V at 2*104 A/cm2
2 kÅ collector, 400 Å base
1x 8 micron emitter, 2x 10 micron collector
0
1
2
0 2 4 6 8
I C (
mA
)
VCE
(V)
Ib step = 20 A
0
10
20
30
40
1 10 100
Ga
ins
(dB
)Frequency (GHz)
U
h21
UCSBSangmin Lee
fmax = 425 GHz, ft = 139 GHz
InGaAs/InP DHBT, 3000 Å InP collector
0.5 m x 8 m emitter (mask)0.4 m x 7.5 m emitter (junction)1.2 m x 8.75 m collectorIc=4.5 mA, Vce=1.9 V
BVCEO = 8 V at JE =5*104 A/cm2
Is low DHBT f due to base-collector grade ?
480 Å grade 100 Å grade
collector velocity and grade: InP has higher Gamma-L separation than InGaAs→ Vsat should be higher in InP → ft should be higher, not lowerslow transport in InAlAs ? → thin grade !
0.5 m emitter, 0.25 m basecontacts
Narrow-Mesa HBTs: high fmax if high base doping
InP/InGaAs/InP Metamorphic DHBTon GaAs substrate
UCSB
165 GHz ft
92 GHz fmax
triple-mesa device(not transferred-substrate)
Growth: 400 Å base, 2000 Å collector GaAs substrate InP metamorphic buffer layer
(high thermal conductivity)Processing conventional mesa HBT narrow 2 um base mesaResults 165 GHz ft, 92 GHz fmax,
6 Volt BVCEO, =27
High Speed Amplifiers
18 dB, DC--50+ GHz
UCSBDino Mensa
PK Sundararajan
8.2 dB, DC-80 GHz
-20
-15
-10
-5
0
5
10
15
20
0 10 20 30 40 50
>397 GHz gain x bandwidth from 2 HBTs
S22
S11
S21
HBT distributed amplifier UCSBPK Sundararajan11 dB, DC-87 GHz
AFOSR
TWA with internal ft-doubler cells
18 GHz ADC
Design comparator is 75 GHz flip flop DC bias provided through 1 K resistors Integration obtained with 3 pF capacitors RTZ gated DAC
Integrated Circuit150 HBTs, 1.2 x 1.5 mm, 1.5 W
gm2
Bias
Bias
C
C
Rz
Rz
Integrator-1 Integrator-2
Bias
Bias
C
C
Master-Slave
Flip-flop
Clock
Out
Idac
gm1
DelayedClock
Vin
CurrentSumming
node
RL
RLRL
RL
UCSBS Jaganathan
75 GHz HBT master-slave latchconnected as Static frequency divider
technology: 400 Å base, 2000 Å collector HBT 0.7 um mask (0.6 um junction) x 12 um emitters 1.5 um mask (1.4 um junction) x 14 um collectors 1.8105 A/cm2 operation, 180 GHz ft, 260 GHz fmax
simulations: 95 GHz clock rate in SPICE
test data to date:tested, works over full 26-40 and 50-75 GHz bands
UCSBThomas Mathew
Hwe-Jong Kim
-0.14
-0.12
-0.1
-0.08
-0.06
-0.04
-0.02
0
0 50 100 150 200
fin=75GHz, f
out=37.5GHz
Vo
ut
(Vo
lts)
Time(ps)
-0.11
-0.1
-0.09
-0.08
-0.07
-0.06
-0.05
-0.04
-0.03
0 50 100 150 200
fin=69GHz, f
out=34.5GHz
Vo
ut(
Vo
lts)
Time(PS)
modulation is synthesizer 6 GHz subharmonic
3.92 V, 224 mA, 0.88 W
~3.5 dBm input power
MHBT slide
State-of-art in HBTs, 2000: cutoff frequencies
InP HBTs today 2x faster, & more scalable: Johnson limit, 2x faster at 5x larger dimensions
0 50 100 150 200 250 300 350
Frequency, GHz
SiGe
InP
AlGaAs/GaAs & GaInP/GaAs
f
fmax
f
f
fmax
fmax
~1 um emitters
~1 um emitters(0.4 um)
~0.1 um emitters
(UCSB t.s.device)
State-of-Art in HBTs, 2000: small-scale circuits
0 20 40 60 80 100
Frequency, GHz
A
SiGe
InP
amplifiers
logic
logic
amplifiers
Si / SiGe has rough parity in logic with InP despite lower f, fmax
due to higher current density, better emitter contacts
Si/SiGe has significantly slower amplifiers
Neither f nor fmax predicts digital speed
CcbVlogic/Ic is very important
collector capacitance reduction is critical increased III-V current density is critical
Rex must be very low for low Vlogic at high Jc
InP: Rbb , (b+c) , are already low, must remain so
What do we need for fast logic ?
clock clock clock clock
inin
out
outECL M-S latch
cexLOGIC
LOGIC
Ccb
becb
becbC
LOGIC
IRq
kTV
V
IR
CCR
CCI
V
6
leastat bemust swing logic The
resistance base the through
charge stored
collector base Supplying
resistance base the through
charging ecapacitancDepletion
swing logic the through
charging ecapacitancDepletion
:by DeterminedDelay Gate
bb
depletion,bb
depletion,
What HBT parameters determine logic speed ?
exCicex
bbcbc
cbdiffcbje
RIqkTVR
RIV
CCC
/6 as effect,indirect strong very has
from 17% ,)( from 12% ,/ from 68%
:imes transit tand sresistanceby Delays Sorting
) (e.g. charging 18%only , charging 38% , charging 44%
:escapacitancby Delays Sorting
log
logic
Caveats: assumes a specific UCSB InP HBT (0.7 um emitter, 1.2 um collector 3kÅ thick, 400 Å base, 1.5E5 A/cm^2)
ignores interconnect capacitance and delay, which is very significant
Cje Ccbx Ccbi b+c) ( I/V) totalV/ I 33.5% 6.7% 27.8% 68.4%V/ I 12.3% 12.3%(kT/q) I 1.4% 0.1% 0.4% 0.5% 2.5%Rex -1.3% 0.1% 0.3% 0.9% 0.1%Rbb 10.2% 2.8% 3.7% 16.7%total 43.8% 6.8% 31.3% 17.5% 100.0%
38%
Why isn't base+collector transit time so important ?
reductionsuch no see escapacitancDepletion
1:10~ is which ,/
of ratioby reduced ecapacitancdiffusion signal-Large
)()(Q
:Operation Signal-LargeUnder
/
)()()(Q
:Operation Signal-SmallUnder
base
base
qkT
V
VV
II
VqkT
IV
dV
dII
LOGIC
LOGICLOGIC
dccbCcb
beCcb
bebe
CcbCcb
Very strong features of Si-bipolars
Emitter Width:0.1 um
Emitter Current Density10 mA/um2
Polysilicon Emitter Contactmetal-semiconductor contactarea >> emitter junction area low Rex
Polysilicon base contactlow sheet resistance in extrinsic basesmall extrinsic collector-base junction area
InP HBT limits to yield: non-planar processEmitter contact
Etch to base
Liftoff base metal
Failure modes
Yield degrades as emitters arescaled to submicron dimensions
base contact
emittercontact
base contact
S.I. substrate
base
sub collector
S.I. substrate
base
sub collector
S.I. substrate
base
sub collector
emitter
S.I. substrate
base
sub collector
Emitter planarization, interconnects
base contact
liftoff failure:emitter-baseshort-circuit
S.I. substrate
base
sub collector
base contact
excessiveemitter undercut
S.I. substrate
base
sub collector
S.I. substrate
base
sub collector
planarization failure: interconnect breaks
Submicron HBT scaling:
Scaling HBTs for 2 x increased speed:2 x thinner layers, 4 x narrower junctions4 x higher current density, 4 x improved vertical contacts
Results with submicron III-V HBT scaling:300 GHz f, high (unmeasurable) fmax
6-dB 175 GHz amplifiers, 75 GHz true digital ICs
Challenges with HBT scaling for fast digital :collector width scaling, current density, emitter resistivityhigh-yield submicron emitter & collector processes
In Case of Questions
Scaling Laws, Collector Current Density, Ccb charging time
base
emitter
collector
subcollector
base
emitter
collector
subcollector
Base Push-Out (Kirk Effect)
Collector Depletion Layer Collapse
)2/)(/( 2 dxqNvJV dsatcb
)2/)(/( 2 dxvJqNV satdcb 2
minmax /)(4 dcbsat xVvJJ
Collector capacitance charging time is reduced by thinning the collector while increasing current
sat
C
CB
LOGICCLOGICcCLOGICcb v
T
A
A
V
VIVTAIVC
22
1/
emitter
collectorcollector