May 16 th 2006M. Bruschi – CSN1 Roma1/20 A. Bertin, M. Bruschi, D. Caforio, S. De Castro, L....
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Transcript of May 16 th 2006M. Bruschi – CSN1 Roma1/20 A. Bertin, M. Bruschi, D. Caforio, S. De Castro, L....
May 16th 2006 M. Bruschi – CSN1 Roma 1/20
A. Bertin, M. Bruschi, D. Caforio, S. De Castro, L. Fabbri, P. Faccioli, B. Giacobbe, F. Grimaldi, I. Massa, M. Piccinini, M. Poli,
C. Sbarra, ASbrizzi, N. Semprini-Cesari, R. Spighi, M. Villa, A. Vitale, A. Zoccoli
Stato del Luminometro (LUCID)
Outline: The Lucid detector Test beam results Tests on Bench The installation scenario The electronics Conclusions
May 16th 2006 M. Bruschi – CSN1 Roma 2/20
Activities of the Group since Sep.05
Main activities of the Bologna Group in LUCID: development of the electronics Preparation (electronics,daq) Test Beam @ Desy
(Nov. 05) and data analysis Monte Carlo: development and optimization of
the code (to reproduce the test beam results).Simulation of the backgrounds.
Test on bench @ CERN to check the detector performances and tune the MC
Discussion of the detector design and of the installation strategies
May 16th 2006 M. Bruschi – CSN1 Roma 3/20
LUCID: relative Luminosity MonitoringLUCID : “LUminosity measurement using Cerenkov Integrating DetectorA bundle of ~200 (per end) projective Al Cerenkov tubes around the beam pipe
Cerenkov radiator gas isobutane
Light fed into PMTs via quartz fibres
May 16th 2006 M. Bruschi – CSN1 Roma 4/20
LUCID position• Planned installation after the Big Wheels A/C.
May 16th 2006 M. Bruschi – CSN1 Roma 5/20
Test Beam @ Desy (Nov. 05):
The T22 teststand has a SiMS telescope - resolution ≈30µm
The T22 teststand has a SiMS telescope - resolution ≈30µm
(LUCID) (Roman Pot)
Cerenkov tubes
Test beam stand for Roman Pots
Winston cones
window of gas vessel window of gas vessel under pressure test under pressure test
Test Beam stand for LUCID
May 16th 2006 M. Bruschi – CSN1 Roma 6/20
Test Beam analysisData analysis performed in Bologna together with MC simulations. Fit of a typical ADC spectrum:
May 16th 2006 M. Bruschi – CSN1 Roma 7/20
Test Beam results
Pressure scan
C4H10
Number of pe’s/Cerenkov-tube for C4H10 at 1 atm. pressure is 5.3 C4F10 pressure scan - essentially the same as that of isobutan Fall of in signal a factor of two in 2 degrees ( nature of LUCID) Disagreement of a factor ~7 w.r.t. MC
Number of pe’s/Cerenkov-tube for C4H10 at 1 atm. pressure is 5.3 C4F10 pressure scan - essentially the same as that of isobutan Fall of in signal a factor of two in 2 degrees ( nature of LUCID) Disagreement of a factor ~7 w.r.t. MC
Angle scan
C4H10
1 bar
May 16th 2006 M. Bruschi – CSN1 Roma 8/20
Comparison with Monte Carlo
Stage A
Improvements in MC still ongoing (light diffusion, etc.) Checks of the detector performances on bench ongoing
Now MC predictions much closer to RD results: ~10 p.e.
May 16th 2006 M. Bruschi – CSN1 Roma 9/20
Test on bench: quantities studied
May 16th 2006 M. Bruschi – CSN1 Roma 10/20
Test on bench @ CERNPerformed under the Bologna responsibility:
Studies on all the different parts of the detector: tube reflectivity between 75% & 95% (depending on the incident angle, typ: 90%), variation up to 10% observed along the tube Not responsible of the poor performances light attenuation along the fibers is about 75% WC – Fiber light collection
May 16th 2006 M. Bruschi – CSN1 Roma 11/20
Test bench results
All quantities measured on bench.Quite good understanding of the detector performances.
May 16th 2006 M. Bruschi – CSN1 Roma 12/20
Possible improvements & next steps
Improvements on the detector;• Tubes: improvements in the internal surface (~ 1.1 - 1.2)• Winston cone: new design + internal surface (~ 1.2 - 1.7)• Fibers: improve fiber quality. ~2 less attenuation (at 300
nm), factor of ~2 large angular acceptance plus a larger (core)/(clad) area ratio (0.78 compared to 0.68) ( ~2)
• PM + Fibre: enlarge the light spectrum sensitivity of PM +fibers (UV range) (~ 2)
Possible improvements in light collection: factor ~6/7Next steps:• New tubes + WC + fibers will be delivered @ CERN middle
May Test on bench• Test beam @ CERN end of June to test the new detector• Test beam @ CERN in November to test the final detector
May 16th 2006 M. Bruschi – CSN1 Roma 13/20
Backup solution (under study)
• Place single miniature PMTs directly onto the end of each Winston cone?
• Advantages:– More light because of direct coupling– Lower electronics cost– Swap quartz fibres for (cheaper) signal
cables• Need to study:
– Radiation hardness of complete PMT system– Background Cerenkov light in window from
primary & secondary particles – Activation– Mechanical design
• Place single miniature PMTs directly onto the end of each Winston cone?
• Advantages:– More light because of direct coupling– Lower electronics cost– Swap quartz fibres for (cheaper) signal
cables• Need to study:
– Radiation hardness of complete PMT system– Background Cerenkov light in window from
primary & secondary particles – Activation– Mechanical design
HAMAMATSU R4296
PMT
May 16th 2006 M. Bruschi – CSN1 Roma 14/20
Detector installation• The installation of the detector early in
2007 is becoming tight. Need to wait for the test beam results. Problems for the electronic design until the detector performances are fixed.Detailed planning available. Still possible, but no contingency
• Investigating alternative scenarios for a reduced detector (e.g. 1 ring per side). Detector Completion at the first long shut-down (end 2008 ?). Presently under discussion.
May 16th 2006 M. Bruschi – CSN1 Roma 15/20
Purposes of the LUCID electronics
The Cerenkov tubes based ATLAS luminosity detector has the following main goals:
1. To measure the integrated luminosity per BX2. To measure the luminosity per BX3. To provide a trigger for interaction (at machine low
luminosity) and for diffractive physics
Logic blocks needed to achieve these three points:
• 1) ad hoc front end card• 2) ad hoc readout card • 3) ad hoc trigger card and a detector acceptance as
big as possible
May 16th 2006 M. Bruschi – CSN1 Roma 16/20
Changes in the electronics design since
fall 2005A very general scheme to fulfill the readout and trigger needs for LUCID was developed in fall 2005Since then, some important changes were achieved:
• Rearrangement of the main logic blocks between the detector and USA 15 (the readout will not be placed in an intermediate rack)
• Front end components (MAPMT, fibers, fed cards, cables) deployment in the nose shielding
• The front end system is now modular so allowing scalability
• A readout and trigger scheme for the backup solution is now available
May 16th 2006 M. Bruschi – CSN1 Roma 17/20
System Architecture
FRONT END (FEPCB)
Similar to Roman Pot FE:OPERA/MAROC chip Input: MAPMTOutput: DIGITIZEDINFORMATION onoptical Links (~1.5 Gb/s)
Analog Information onCoaxial (or diff. on tw. Pair)
19x2
MAPMT
GOL
LINKS+coax
LHC sync:TTCrq, CTRL sign.,etc
ROS
ROD
ROD
ROD
ROD
TRIGG.
CARD
HV FE CONTROL
PC
May 16th 2006 M. Bruschi – CSN1 Roma 18/20
The LUCID FED cards
•The front end system is now modular so allowing scalability•The MAROC Boards will be developed by LUND (thanks!)
TX Digital BoardGOL, FPGA, TX
ConnectorsBoard(HV,LV,RX,TX,analog)
MAROC Boards
Base board(only connectors andsignals routing)
ANALOG board(ampl.+line driv.)
RX Digital BoardTTCRQ, volt. reg.
May 16th 2006 M. Bruschi – CSN1 Roma 19/20
Conclusions/detector LUCID can rely on quite settled technologies both on the detector & the electronics side
Detailed studies on the detector in test-beam and laser tests and a lot more is known (simulation, mechanics, light detection, fiber readout, cabling, electronics placement, readout, etc…). Good chances to improve the light emission by about a factor 6-7.
Improved detector version will be tested in May on bench and in the test beam of June
Large impact of the Bologna Group on all the ongoing activities
Different installation scenarios under discussion. Aim for installation of LUCID in 2007.
May 16th 2006 M. Bruschi – CSN1 Roma 20/20
Conclusions/electronics The design of the front-end electronics has been
started (although we need a confirmation of the performances of the detector)
The front end electronics (both for the baseline and the backup solution) should be reasonably ready for february 2007
The project is now modular and can easily adapted in case we will decide for the LUCID readout backup solution
The development of the readout and trigger electronics could be a bit relaxed since we can use already available pieces of DAQ to give a luminosity measurement as soon as the front end electronics will be available
First version of MAROC chip including modifications for LUCID submitted on March 6th
May 16th 2006 M. Bruschi – CSN1 Roma 21/20
Backup slides on detector
May 16th 2006 M. Bruschi – CSN1 Roma 22/20
LUCID position:
MBTSTILE
ηMAX = 6.073ηMIN = 5.374
Detector goals: provide a relative luminosity measurement
(integrated and bunch by bunch) Provide η-coverage for diffractive physics
May 16th 2006 M. Bruschi – CSN1 Roma 23/20
Parametrization of PMT spectra
May 16th 2006 M. Bruschi – CSN1 Roma 24/20
Improvements: Winston cone
May 16th 2006 M. Bruschi – CSN1 Roma 25/20
Improvements: new fibers
May 16th 2006 M. Bruschi – CSN1 Roma 26/20
Fiber efficiencyA transmission has been made on the fibers used in the TB.
The quartz fibers have a better transmission than the plastic fibers but this is compensated for by a larger numerical aperture of the plastic (0.51) compared with the quartz (0.37). Same number of p.e. in the test beam
May 16th 2006 M. Bruschi – CSN1 Roma 27/20
May 16th 2006 M. Bruschi – CSN1 Roma 28/20
BACKUP SLIDES on electronics
May 16th 2006 M. Bruschi – CSN1 Roma 29/20
12 m
24 m 12 m
2 m(wall)
Rack?12 m
8 m(MAPMT out)
From MAPMT out to USA15 Total Cable Length: 8+12+12+24+12+2 = 70 mInside USA15: <25 m 80 m < Total Cable Length < 100 m
May 16th 2006 M. Bruschi – CSN1 Roma 30/20
Baseline Readout Scheme
LUCID1
Nose Sh. USA15~4m ~80-100 m
Optical fibers
MAPMTMAROCDRIVERS
COAX (or tw. pair) +Optical fibers
READOUTTRIGGER
Total number of channels: 168x7x2=2352 for 19x2 MAPMT
May 16th 2006 M. Bruschi – CSN1 Roma 31/20
Electronics and Cables placement
May 16th 2006 M. Bruschi – CSN1 Roma 32/20
Electronics
GOL
First version of MAROC chipincluding modifications for LUCIDsubmitted on March 6 th(thanks to the ORSAY group!)
May 16th 2006 M. Bruschi – CSN1 Roma 33/20
General Comments• The TDC in the readout block will be
probably be replaced by a simple gated coincidence
• In case the LUCID readout backup solution would be preferred, then:
- The MAROC chip will not be used
- The FED cards will contain only the ANALOG board
- The STRU unit of the readout card will be simplified
May 16th 2006 M. Bruschi – CSN1 Roma 34/20
Single Tube Readout Unitfor PMT (1 channel)
15 nsint
10 nsreset
25 ns
time
time
LHC Clock
LHC Int. Time
ADC GATE
TDC START
to thetrigger
unit
FanOut
TDC
GI+
ADC
Multiplicity per Tube
LUT
8
8
3
PMT output
STRU
Discr. (Prog.
Thr+NR)
TDC START
STOP
ADC GATE
May 16th 2006 M. Bruschi – CSN1 Roma 35/20
Possible Initial DAQ scheme for MAPMT readout (digital
part)
SBC
LTP
TTCVI
TTCEX
TTCOC
CTP
FilarCards(PCI IF)
ROS
EthernetLink
To LUCIDFED
2 ServerComputers
from LUCIDFED
May 16th 2006 M. Bruschi – CSN1 Roma 36/20
Q.ty Units MIN MAX MIN MAX
MAPMT 2 unit/ROD 1300 1400 2600 2800
MAROC 2 unit/ROD 25 500 50 1000 a multiproject of 20 keuro (shared?) is assumed
CONNECTIONS (incl. connectors)
coax cables 20 100m/ROD 80 80 1600 1600 suhner gx 02272 + SMB connectorsoptical fibers 1 100m/ROD 700 700 700 700 Optical fiber with connectors (bundle of 12)optical fiber 1 100m/ROD 100 100 100 100 Optical fiber for TTCRQHV cables 4 100m/ROD 100 100 400 400TOTAL CONNECTIONS 2800 2800FRONT END (FE)
GOL 9 unit/ROD 15 15 135 135TTCRQ 1 unit/ROD 100 100 100 100FPGA 1 unit/ROD 200 200 200 200Amplifier, drivers, voltage reg., etc 1 unit/ROD 300 300 300 300Agilent TX 1 unit/ROD 500 500 500 500Samtec connectors 8 unit/ROD 10 10 80 80TOTAL FRONT END (MATERIAL)/ROD 1315 1315
READ-OUT BOARD (ROD)
LHCb PS Gated Integrators 5 unit/ROD 100 150 500 750 purchased directly by LHCb outlet (2500 chip)8 bit ADC 40 MSPS 20 unit/ROD 5 10 100 200 investigate LHCb PS FE solutionTDC 10 unit/ROD 20 35 200 350 gated coincidence or CERN HPTDCTTCRQ 1 unit/ROD 100 100 100 100
S-LINK (incl. cable) 1 unit/ROD 200 200 200 200VME IF FPGA 1 unit/ROD 50 50 50 50CTRL LOGIC FPGA 1 unit/ROD 75 75 75 75STRU LUT,DPRAM,EVENT BUFF. FPGA 20 unit/ROD 75 100 1500 2000GOL 9 unit/ROD 15 15 135 135Agilent RX 1 unit/ROD 500 500 500 500TOTAL ROD (MATERIAL) 3360 4360
TRIGGER BOARD (TB)
TTCRQ 1 unit/TB 100 100 100 100
S-LINK (incl. cable) 1 unit/TB 200 200 200 200VME IF FPGA 1 unit/TB 50 50 50 50CTRL LOGIC FPGA 1 unit/TB 75 75 75 75TRIGGER PROCESSING UNIT FPGA 1 unit/TB 1500 1500 1500 1500TOTAL TB 1925 1925
VME+PC
VME 9U CRATES 2 unit 7500 7500 15000 15000VME CPU 2 unit 4000 4000 8000 8000PC 2 unit 1700 1700 3400 3400TOTAL SYSTEM 26400 26400
Item CommentsUNIT COST
(EURO)
TOTAL COST
(EURO)
ITEM UNITS PROD MIN MAXFACTOR (EURO) (EURO)
MAPMT 38 49400 53200MAROC 38 950 19000
FE 20 2 52600 52600ROD 20 2 134400 174400TB 1 2 3850 3850
CABLING 20 56000 56000
VME+PC 1 26400 26400
TOTAL 323600 385450
COSTS SUMMARY
COSTESTIMATE
(must be updated With MAROC boardsCost ~ 10k€)
May 16th 2006 M. Bruschi – CSN1 Roma 37/20
FED TIME SCHEDULE for FED
May 16th 2006 M. Bruschi – CSN1 Roma 38/20
Single PMT readout• The candidates PMT are Hamamatsu R2496
with quartz window• <IA> < 15 A (could be 30 A with active
divider) with HV=1250 V• Number of photons @ 1 bar 400 (MC/8 Feb.
2006)• QE ~ 20%• 15 A>400x0.2x1.6x10-19xGPMTx40MHzx0.3
GPMT≤105 QMAX~1.3 pC (signal duration 10 ns) Vsig ~ 13 mV
May 16th 2006 M. Bruschi – CSN1 Roma 39/20
stru 1stru 2
stru 20
SUM_OUT 1_1
SUM_OUT 1_2
SUM_OUT 2_10
GOL 1
GOL 2
GOL 9
GOLRX
LVDSS/P
3
3
3
LVDS 1_1 (to trig. unit)
LVDS 1_2 (to trig. unit)
LVDS 2_1 (to trig. unit)
LVDS 2_2 (to trig. unit)
stru 2
TTCRQ i.f.opt. lnkfrom TTCEX
VME P1VME I.F
DPRAMDPRAM
DPRAM
CTRLLOGIC
6 Bytes
6 Bytes
6 Bytes
EVENTBUFFER
s-LINKto ROS
from CTRL LOGICfrom CTRL LOGIC
160 MB/s
s-LINK Busy
LUCID ROD BOARD (22 units + spares) – VME 9U
Analog_In 1
Analog_In 2
Analog_In 20
GOL_In 1
GOL_In 2
GOL_In 9
~200 Bytes/ev
May 16th 2006 M. Bruschi – CSN1 Roma 40/20
SignalBuffer
TTCRQ i.f.opt. lnkfrom TTCEX
VME P1VME I.F
CTRLLOGIC
s-LINKto ROS 160 MB/s
s-LINK Busy
LUCID TRIGGER BOARD (1 unit + spares) – VME 9U
Detector
1
Detector
2
LVDS 1_1
LVDS 1_2
LVDS 22_1
LVDS 22_2
1
2
43
44
LVDS 23_1
LVDS 23_2
LVDS 44_1
LVDS 44_2
1
2
43
44
SignalBuffer
FPGA basedTRIGGER
PROCESSINGUNIT
44 ser. Inp594 bit/BX
44 ser. Inp594 bit/BX
to the L1 trigger
~200 Bytes/ev
Algorithm:MC simulations are needed
May 16th 2006 M. Bruschi – CSN1 Roma 41/20
MAPMT readout• The candidates MAPMT are Hamamatsu
H-7546-03 with UV glass (or quartz?)
• <IA> < 100 A (8 stage boosted divider) with HV=1000 V
• Number of p.e. per channel: 5
• (100 A/64)>5x1.6x10-19xGPMTx40MHzx0.3
GPMT≤1.6x105 QMAX~0.13 pC (signal duration 10 ns) Vsig ~ 1.3 mV
May 16th 2006 M. Bruschi – CSN1 Roma 42/20
MAROC analog output characteristics
• 25 mV/160 fC typical output from single fiber (130 fC)
~ 20 mV • Typical output from 7 fibers ~ 140 mV
May 16th 2006 M. Bruschi – CSN1 Roma 43/20
Cabling
• The readout of the front includes both analog and digital signals transmission
• For the analog ones:single ended on coaxial (but: differential on twisted pairs under consideration)
• For the digital ones: optical fiber is the baseline
May 16th 2006 M. Bruschi – CSN1 Roma 44/20
( )4
( )( , ( ), ) 2(3)
(2 10, . . )9 1 10 10 1
63 80 5.04
CABLES multiconductorHV
MAPMTCABLES LV power
LV GNDMAPMT
SUM MONITOR SIGNALS COAX CABLE sh tw pairsANALOG
MAPMT MAPMT MAPMT MAPMT MAPMT
Mbit GbitDIGITAL
MAPMT M
( )4
1.5 CABLES CABLES fibers
APMT Gbit MAPMT
Cables Summary
•Globally we will have 2x19=38 MAPMT
May 16th 2006 M. Bruschi – CSN1 Roma 45/20
May 16th 2006 M. Bruschi – CSN1 Roma 46/20
May 16th 2006 M. Bruschi – CSN1 Roma 47/20
May 16th 2006 M. Bruschi – CSN1 Roma 48/20
May 16th 2006 M. Bruschi – CSN1 Roma 49/20
General Considerations-III• For the description of the readout electronics I will refer essentially to the
baseline of the detector described in the LOI
• Detector:formed by two parts each one consisting of 200 Cherenkov counters (tubes) 5 layers/section x 40 tubes/layer x 7 fibers/tube x 2 sections = 2800 fibers
• Signal:Prompt particles coming from the IP (primaries) will traverse the full length of the counter and generate a large amplitude signal in the photo-detector
• Background I: Particles originating from secondary interaction of prompt particles in the
detector material and beam-pipe (secondaries) are softer and will traverse the counters at larger angles (multiple reflections), with shorter path lengths
Background I significantly smaller than signal• Background II:
Particles crossing the readout fibers will produce light only on the crossed fibers
Background II will have different pattern of hit fibers wrt signal