1 / 33

D0 Tracking – From the Inside Out

D0 Tracking – From the Inside Out. Opportunity to reflect on experience – what we wanted to achieve, where we succeeded and where we failed Outline RunII and it’s evolution Silicon Tracker Fiber tracker Muon system High luminosity effects Operations Conclusions.

nitara
Download Presentation

D0 Tracking – From the Inside Out

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. D0 Tracking – From the Inside Out Opportunity to reflect on experience – what we wanted to achieve, where we succeeded and where we failed Outline • RunII and it’s evolution • Silicon Tracker • Fiber tracker • Muon system • High luminosity effects • Operations • Conclusions R. Lipton, Fermilab

  2. Landscape circa 1990 • The Physics Landscape: • LHC/SSC will be on by 1997 and dominate high pt physics • Top quark not yet discovered • CDF shows B physics capability of collider detectors and utility of vertex detectors • B factories ? • Mixed high pT and B physics emphasis in design Let’s go back to 1990 – D0 wasconsidering an upgrade as theoriginal (RunI) detector was being installed to accommodate an upgraded Tevatron/Main Injector • Reduced crossing interval 3.2ms → 396(132) ns • Magnet – a break from the UA1 inspired no magnet philosophy • Improved tracking • Improved muon detector • Silicon vertex detector • Develop a tracking culture R. Lipton, Fermilab

  3. Run One D0 Experience • Detailed MARS and Geant muon shielding simulations. • neutrons were a problem • complex shield design • timing important • Use small angle stereo in central tracker, small and large angle in silicon, short barrels • Add an inner scintillation counter layer to reduce muon pT threshold • Disk/barrel design of the silicon tracker to preserve high h resolution • Small angle muon chambers were very busy – can they be adequately shielded and keep good high h acceptance? • D0 tracker performed very poorly in rz – chambers used charge division and delay lines for z information. • CDF had much better J/y → mm yields than D0, due to thinner iron, lower pT. • Can good high h tracking be preserved in spite of the long luminous region? R. Lipton, Fermilab

  4. 132 ns 396 ns The Shifting Playing field 10 int/xing • Integrated luminosity 2 fb-1 →15 fb-1(IIb) →between 4 and 8 fb-1 • Crossing interval was planned to decrease from 396 ns to 132 ns in RunIIb. It will now stay at 396 ns • There was hope that the luminous region would decrease from 30 to 15 cm. • Actual instantaneous luminosity can be ~2x average due to bunch-to-bunch variations • Luminosity leveling? 8x10312x1032 5x1032 R. Lipton, Fermilab

  5. Tracker hardware design was based on large acceptance in h. Used mixed disk/barrel system to maintain good resolution and efficiency with long (~25cm) luminous region Large area “H disks” – precise point at high Z to maintain momentum resolution Route cables between barrel ladders – no lost spaceat the barrel/disk interface Resulted in a complex silicon mechanical design and a challenge to the Monte Carlo Tracker Design R. Lipton, Fermilab

  6. D0SMT Disk/Barrel Design Support andcables disk barrel R. Lipton, Fermilab

  7. The D0 Run2 Detector Muon System Fiber Tracker D0SMT R. Lipton, Fermilab

  8. Tracker Technology Decisions • Original silicon detector design was for 2 fb-1. RunIIb physics studies (Higgs) indicated that experiments (and accelerator) should attempt 15 fb-1 (2002) • Silicon technology was based on SSC R&D (double-sided) subsequent LHC R&D showed this was not the best choice • Rad hard chip technology being phased out at many vendors • We had the ~last run at UTMC for SVX2 (1996) • Chip design tools poor • Replaced by deep submicron ~2002 • D0 decided to use SVX2 rather than SVX3 • Bird in the hand (~working chip … little did we know) • Did not need multiple buffering at L1 (now limit to trigger) • Too much work to develop simultaneous low noise readout/daq (probably true-big effort at CDF) • VLPC/SciFi development for tracking – all new technology – high risk but excellent for fast triggering R. Lipton, Fermilab

  9. Tracker Parameters • [s(pT)/pT]2 ~ 0.0152 + (0.0014pT)2 • s(PV) ~35 mm • s(IP) ~15 mm, pT >10 GeV Maximum 12 hits at h=0ignoring overlaps R. Lipton, Fermilab

  10. Time in store noisy F-Wedges 'good' F-Wedge SMT Operations F wedge noise • SVX2 chip is not very robust • Needs to be read out every ~30 seconds or current goes up causing trips– heartbeat trigger installed • Very sensitive to supply voltage, signal quality • Channels come and go ~ 15% disabled at any one time • Wedge detectors from Micron show serious “grassy” noise – beginning several months after the start of RunII bias current R. Lipton, Fermilab

  11. Microdischarge • Many double sided detectors have low p-side microdischarge junction breakdown voltage • Limits voltage applied to a side – not total bias • The sensitive side switches from p to n after type inversion • The total voltage allowedincreases after type because the oxide chargelowers the n-side fields • Not yet a practical limit tooperations R. Lipton, Fermilab

  12. Booster Radiation Studies • Spare detectors were exposed to 8 GeV booster proton irradiation • Full readout/laser test measurements at each point • Most behaved “normally” • Double metal 90 degree detectors (DSDM) showed anomalous Vbias slope limit to SMT lifetime? 1 fb-1 R. Lipton, Fermilab

  13. L3 DSDM L1 DSDM L4 DS L2 DS SMT Radiation Studies • We now have enough experience to measure long term behavior • Use charge collection and n-side noise • Charge collection data taken at regular intervals • DSDM detectors now look normal – probably charge annealing in PECVD dielectric • Expect the SMT to survive to 5-7 fb-1 R. Lipton, Fermilab

  14. Vdepletion Warm-up during shutdown SMT Radiation Studies • Measure flux using leakage current evolution • Measure depletion voltage with charge collection and noise Noise vs voltage R. Lipton, Fermilab

  15. Run II Results R. Lipton, Fermilab

  16. 2003 beam loss incident Beam Protection • Beam losses are not uncommon • 2003 CDF Roman Pot into beam • Kicker prefires, Quenches, Shot setup • LHC/TeV ~ 1000 in beam power • D0 has two radiation monitoring/abort systems • BLM - argon gas ion chambers circa 1980 • Originally developed for AD/CDF • Provides Tevatron abort@12 rad/s • 10 m from IP • NIKHEF finger diodes • 24 one cm photodiodes 2.6 cm to 9.5 cm from beam • 106 dynamic range – scaler/ADC • Not used for abort due to SMT readout noise Holes in 2 upstream components R. Lipton, Fermilab

  17. Beam Monitoring • Large dynamic range and low radius of the fingers allow detailed studies of beam effects and incidents • Understand losses at various stages of the cycle – for some losses have dominated by luminosity Scaler count rate vs time as solenoidramps down – looper plateau ~0.8 T Finger scalers Finger ADCs Shot Setup R. Lipton, Fermilab

  18. Fiber Tracker – CFT/CPS • CFT - 8 doublet layers of 0.835 mm fibers (xu,xv..) use high QE VLPC technology • Few layers-require high e • High occupancy for inner layers • Fewer hits than gas-based chamber, but more radiation hard, amenable to fast (L1) track trigger with FPGAs • CPS – layer of triangular scintillator outside of solenoid Fiber tracker Clear waveguides R. Lipton, Fermilab

  19. Mean pedestal (ADC) CFT Operations • AFE – readout of VLPC system for CFT and preshower • SVX2 dynamic range ~200 MIPS front end integrator is subject to saturation at high L • Discriminator crosstalk to ADC • Crossing-to-crossing pedestal variations • Replacing AFE with AFEII • No SVX2 • New trip-t chip – clean discriminator output and timing crossing R. Lipton, Fermilab

  20. Tracking Performance Low momentumtracking option de/dx particle ID R. Lipton, Fermilab

  21. No Shielding D0 Shielding Muon System Muons are at the heart of much D0 physics • Run II optimization • Chambers at high h were too noisy • Most noise hits are out of time with collision muons • Detailed study/model of shielding • Lower pt threshold for B physics to ~1.5 GeV • Detailed shielding redesign • 50 cm of steel – hadrons and e/g • 12 cm of polyethylene - neutrons • 5 cm of lead - gamma rays • Reduction in particle fluxes by a factor of 50-100 (GEANT/MARS) • Run 1 muon detector occupancies have been in the 5-10% level • Run 2 muon detector occupancies are in the 0.05-0.1% level R. Lipton, Fermilab

  22. Run I Small angle muon chambers “Typical” Run I event Run II R. Lipton, Fermilab

  23. Muon Chambers and Counters R. Lipton, Fermilab

  24. Muon System • Added fast counters to reject halo • Added counter layer before m filter with 1.5 GeV Pt threshold • Level 1 muon-track match trigger • Result: x150 J/y yield over Run I competitive B physics Run 1 Muon h in J/psi events R. Lipton, Fermilab

  25. Monte Carlo • Difficult to properly model complex SMT cable paths • Use e+e- conversions to map material and validateMC • Initial version was missing top of support cylinder • Inclusion of ladder and support details is an ongoing effort • Tracking system resolutions and errors still not fully understood. Data Monte Carlo R. Lipton, Fermilab

  26. Understanding Uncertainties • Are the assigned uncertainties correct? • Hit position algorithm based on cluster size • Study IP resolution of PV tracks based on hit patterns • Scale to fit beam convoluted IP distribution • Hampered by the loss of raw hit data early in the data stream R. Lipton, Fermilab

  27. Tracking CPU • Tracking CPU time has always been a problem in this design – minimal layer in outer tracker • Currently our L3 rate is limited to 50 hz - the rate at which data can be reconstructed – will be raised • Serious problem at high luminosity Black = total tracking Red = pattern rec Green = HTF patt rec Blue = AA patt rec Pink = track fit HTF, not AA, is the current “culprit” Improvement by better treatment of large (looper) clusters R. Lipton, Fermilab

  28. 0 MB 4 MB 8 MB High Luminosity Tracking With our current hardware and algorithms both efficiency and purity will degrade at high luminosity R. Lipton, Fermilab

  29. Study of Luminosity Effects in Data J/y →mm as a function of the number of tracks in the event R. Lipton, Fermilab

  30. Coping with High Luminosity • AFE II project (CFT readout) • Fix saturation, pedestals, add timing to CFT • Layer 0 (M. Weber) • Tracking algorithms – tradeoffs between thresholds and speed • Luminosity leveling – vary b during the store to provide uniform luminosity with similar integral • Trigger upgrades R. Lipton, Fermilab

  31. Operations • Experiment is collecting data efficiently ~ 5% dead time • Solenoid magnet developed a heat leak – limited to ~96% of full field • Limit thermal and ramp cycles • Operational channels • SMT ~ 87% • CFT ~ 99% (was 99.9%) • Muon – 99.8% • CAL ~ 99.9% R. Lipton, Fermilab

  32. What we did .. Right • Carefully tested most detector types – extensive system tests • Excellent mechanical quality and stability • Tracking system provides excellent h and momentum acceptance, tracking to 180 MeV • Muon system design shielding and timing • It all works to produce physics Wrong • Upgrade was ambitious – all detectors should be properly supported in hardware and software • Hardware and software groups did not always interact effectively. • Cost and schedule was too much of an early concern • Changing plans from FNAL and accelerator R. Lipton, Fermilab

  33. Conclusions Bs mixing WZ → trileptons W mass B semileptonic R. Lipton, Fermilab

More Related