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Wieman: 1LBNL
Micro-vertex
STAR Collaboration Meeting Aug 2003
LBNLHoward Wieman, Fred Bieser, Robin Gareus (Heidelberg), Howard Matis,
Marcus Oldenburg, Gulshan Rai, Fabrice Retiere, Kai Schweda, Hans-Georg Ritter, Eugene Yamamoto
UCIYandong Chen, Stuart Kleinfelder
BNL Instrumentation DivConsulting
OSUIvan Kotov
PurdueDennis Reichhold
Wieman: 2LBNL
Today's topics
• Monolithic APS CMOS, new development of photo-gate – Purpose
– Modeling
– First silicon results
• Mechanical work– Vibration measurements
– Light weight silicon support, another approach
– Thin beam pipes
Wieman: 3LBNL
• CDS removal of fixed pattern noise and KTC reset noise on the chip (standard diode requires CDS off chip)
• Increase signal by reducing signal spreading to adjacent pixels. The photo gate permits large geometry without adding capacitance to the sense node.
Photo gate purpose - addresses standard diode limitations
P-
P
P+
Standard diode geometry
Standard APS diode structure
Wieman: 4LBNL
photo gate
source follower gate
reset gate
transfer gate
row select gate
sense node drain
• Large photo-gate to collect large fraction of the charge on a single pixel, directly on the p- epi layer
• Small transfer gate also directly on p- epi layer
• Small drain (minimum capacitance) connected to source follower gate (sense node)
Photo-gate geometry
20 m
x -2 m- 1 m 1 m5 nm
8 m
0.1 m
0.4 m
P epi 1.4x1015 1/cm3
N+ 1x1020 1/cm3
photo gate transfer gate
drain
x = 0.4 and 0.8 m
(simulation quantities)
Wieman: 5LBNL
Photo-gate issues in standard CMOS
• No double poly process – possible poor transfer between gates because of low transverse field
• Floating n well between gates, a bad solution to the transfer problem with single poly
• Sub-micron process may solve problem
single poly, limitation of CMOS
double poly, standard for CCDs
photo gatetransfer gate drain
floating n well
Wieman: 6LBNL
Photo gate/transfer gate operation
photogate
transgate1.8 V V
drain2.4 V
photogate
transgate
drain
V phg = 0.8 Vtransfer mode
V phg = 2.4 Vcollection mode
Wieman: 7LBNL
Photo gate/transfer gate with 800 nm separation
photogate
transgate1.8 V V
drain2.4 V
photogate
transgate
drain
V phg = 0.8 Vtransfer mode
V phg = 2.4 Vcollection mode
Wieman: 8LBNL
Drain current after light injection
• 400 nm between photo gate and transfer gate, no floating n well
• Nano amp drain current
• Rapid electron transfer - complete in 60 ns
photo gate
transfer gate drain
Light injection
60 ns
Wieman: 9LBNL
First silicon tests, comparing photo-gate with standard diode structure
Photo-gate directly to sense node drain
DC bias:V photo-gate 0.6 VV drain 2.4 V
Output signal for Fe55 X-ray test
Issue:
ADC
Linear
ADC
Log
diode
Photo-gate 1
Photo-gate 2
diode - fullcharge collection
Why is the signal spread out – is it surface traps under the gate?
Wieman: 10LBNL
Mechanical Concept• Single end
support for rapid installation and removal
– For beampipe bake out
– Insurance for beam excursion damage
• Readout electronics in end support module
Low Mass Carbon fiber tube
Thin silicon ladders under tension
Aluminum Kapton cables under tension
Wieman: 11LBNL
Tension concept
Wieman: 12LBNL
Tension concept
Wieman: 13LBNL
50 m Silicon
9
Thinned and polished wafers, a standard industrial process
Thinned Silicon wire bonded to cable, both supported under tension
Used in wind tunnel test
Wieman: 14LBNL
Air cooling and vibration
• 1-2 m/s air cools 100 mW/cm2
• TV holography shows 2 m vibration for tensioned silicon structure
TV holography vibration map
Lucite wind tunnel Thin silicon ladder,tension support
Laser light source
Camera
Wieman: 15LBNL
Thin stiff ladder concept
• Under construction
• Will be tested for vibration in our wind tunnel
carbon composite(75 m)
aluminum kapton cable(100 m)
silicon chips(50 m)
21.6 mm
254 mm
Wieman: 16LBNL
Self supporting ladder concept
Outer shell carries extended beam pipe gravitational loads
Free end access for detector insertion
Wieman: 17LBNL
A thinner beam pipeElastic Bucking InstabilityEuler 1757
Eigen solution
Critical buckling force
The challenge: increase moment of inertia along y without increasing material
16 cm
4 cm
Aluminum 150 m thick
critical pressure 5.5 atmospheres
Increase I with corrugations
0.03 atmos. with no corrugation
Wieman: 18LBNL
Conclusion
• Present monolithic CMOS APS detector technology suitable for slow 10-20 ms readout (examples at LBNL/UCI and LEPSI/IRES)
• Fast readout not ready yet, but progress is being made
• Radiation hardness good enough for RHIC
• Mechanical concepts progressing
• R&D is fun, but…
• Proposal due this December
Wieman: 19LBNL
Test of diode variation
• No Fe55 signal
• Will test with more statistics
p- epi
np p
Puzzle:
Wieman: 20LBNL
Rejection of primary tracks
• For large rejection ratios must set cut at several times multiple scattering angle
• At these large angles single coulomb scattering dominates and materials contribute linearly
Beam pipe x/X0 = .17 %Si x/X0 = .05 %C Comp x/X0 = .03 %Al Kapton x/X0 = .03 %
Leakage fraction
0
0.6
1.2
total Be beam pipe 600 micronsSi 50 micronAl Kapton cable
Wieman: 21LBNL
Photo-gate Fe55 X-Ray test
• Charge collection histogram for CMOS APS – comparing two photo-gate structures to standard diode structure
• Photo-gate coupled directly to drain – no transfer gate• Photo-gate shows more complete charge collection, but…
ADC ADC
Log Linear
diode
Photo-gate 1
Photo-gate 2
full diodecharge collection
Wieman: 22LBNL
Drain current after light injection, floating n well delay
V
photo gate
transfer gate drain
floating n well
Light injection
Potential before and after injection
V=Q/C (very small)
drain currentlogdrain current
linear
200 s 200 sSmaller the signal the higher the effective resistance and the slower the transfer
Wieman: 23LBNL
Radiation resistance
• Radiation tests of the LBNL APS at the 88” cyclotron
55 MeV protons 30 year RHIC operation at 4 x design luminosity
Wieman: 24LBNL
Properties, LBNL APS
MIP (most probable) 440 e
Node C, measured with Fe55 Xray 6.1 fF
Gain ~26 V/e
Noise ( 1 pixel, CDS, Ileak subtr ) 17 e rms
Signal/Noise (9 pixel sum, CDS) 9
Signal/Noise (potential, single pix) 26
kTC reset noise (measured) 50 e rms
kTC reset noise (expected) 30 e rms
Leakage Current 0.9 fA
Wieman: 25LBNL
Silicon Cost
Ladders per Wafer 5
Ladders per Detector 24
Yield 60%
Number of Detector Copies 4
Number of Wafers 32
Wafer Cost Each 2-5 k$
Wafer Costs 64-160 k$
Mask Cost 150-200 k$
Total 214-360 k$
8 inch wafers
20 mm x 170 mm ladders