star mrpc tof: project overview bnl january 26, 2006 geary eppley rice university

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STAR MRPC TOF: Project Overview BNL January 26, 2006 Geary Eppley Rice University

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Page 1: STAR MRPC TOF: Project Overview BNL January 26, 2006 Geary Eppley Rice University

STAR MRPC TOF: Project Overview

BNL

January 26, 2006

Geary Eppley

Rice University

Page 2: STAR MRPC TOF: Project Overview BNL January 26, 2006 Geary Eppley Rice University

Design considerations

• The integration space available for TOF in STAR is that currently occupied by the CTB.

• The space is about 2.2m from the beam line: requires precision time measurement.

• The clearance between the TPC and EMC is about 10 cm.

• The space has a uniform 0.5T magnetic field parallel to the beam.

• There is limited space for “nearby” electronics outside the magnet steel.

ZCal

SiliconVertexTracker

CentralTriggerBarrel orTOF

FTPCs

TimeProjectionChamber

Barrel EMCalorimeter

VertexPositionDetectors

EndcapCalorimeter

Magnet

Coils

TPCEndcap &MWPC

ZCal

RICH

Page 3: STAR MRPC TOF: Project Overview BNL January 26, 2006 Geary Eppley Rice University

MRPC development

• Multigap glass RPCs developed in the late 1990s at CERN, C. Williams, et.al.

• STAR TOF group designed STAR-specific MRPC modules that would fit existing CTB trays and tested them at CERN in 2000 & 2001.

Page 4: STAR MRPC TOF: Project Overview BNL January 26, 2006 Geary Eppley Rice University

MRPC prototypes in STAR

• One tray of MRPC modules has been installed in STAR for Runs 3, 4, & 5.

• An improved tray design each year but some modules have been installed for all 3 years.

• Runs 3 & 4 used CAMAC electronics.

• Prototype HPTDC based electronics used in Run 5 and Run 6

Page 5: STAR MRPC TOF: Project Overview BNL January 26, 2006 Geary Eppley Rice University

Electronics integral to tray

• 95% of the electronics resides on the tray inside the cover

• 4 external electronics boxes located on the magnet steel connect the 23k-channel system to STAR trigger and DAQ

Page 6: STAR MRPC TOF: Project Overview BNL January 26, 2006 Geary Eppley Rice University

Tray specifications

• There are 32, 6-channel modules per tray.

• The active area covers about 87% of -0.9<eta<0.9

• Occupancy in central AuAu is ~12%.

• HV provides +-7 kV.

• Gas mixture: 95% r134a, 5% isobutane.

• Average noise rates are ~15 Hz/channel with greater than 100% correlation.

• Detection efficiency is ~95%.

Page 7: STAR MRPC TOF: Project Overview BNL January 26, 2006 Geary Eppley Rice University

Time measuring

• Absolute times are recorded and buffered by the HPTDC for all hits above threshold.

• A single 40 MHz oscillator provides the clock for the 2882 HPTDCs in the system.

• Both start and stop detectors use the HPTDC to record times eliminating systematic uncertainty from the choice of counter.

• Each HPTDC has a 21 bit clock counter providing a 51 us clock period. The HPTDCs are reset by a signal with a common origin at the beginning of each run giving each HPTDC a different phase that may be learned from the data.

• Since this phase is always the same, the phase becomes a powerful tool to monitor the integrity of the data through buffering, trigger matching, event building, transmission to DAQ, and global event building.

Page 8: STAR MRPC TOF: Project Overview BNL January 26, 2006 Geary Eppley Rice University

Total time resolution from Run 5:

200GeV CuCu, 105ps 62GeV CuCu, 124ps

Page 9: STAR MRPC TOF: Project Overview BNL January 26, 2006 Geary Eppley Rice University

Time resolution by channel

Page 10: STAR MRPC TOF: Project Overview BNL January 26, 2006 Geary Eppley Rice University

Timing results, Runs 3, 4, &5:

~80~82~20HF

~89~105~ 55200GeV Cu Cu (ToT)Run V

~92~125~ 8562GeV Cu Cu (ToT)

~82~86~27FF/RFF

~86~96~40FF/RFF, w/o E pVPD

200GeV (Au+Au)

~89~105~5562GeV (Au+Au)

Run IV

~80~160~140200GeV p+p

~85~120~85200GeV d+AuRun III

TOFr

(stop-side)

TOFr

(total)pVPD

Time Resolution (ps)

Operation conditions

~80~82~20HF

~89~105~ 55200GeV Cu Cu (ToT)Run V

~92~125~ 8562GeV Cu Cu (ToT)

~82~86~27FF/RFF

~86~96~40FF/RFF, w/o E pVPD

200GeV (Au+Au)

~89~105~5562GeV (Au+Au)

Run IV

~80~160~140200GeV p+p

~85~120~85200GeV d+AuRun III

TOFr

(stop-side)

TOFr

(total)pVPD

Time Resolution (ps)

Operation conditions

Page 11: STAR MRPC TOF: Project Overview BNL January 26, 2006 Geary Eppley Rice University

STAR TOF publications:

• Physics– Open charm yields in d+Au collisions: STAR Collaboration, Phys.Rev.Lett. 94

(2005) 062301.– Cronin effect of identified particle at RHIC: STAR Collaboration, Phys.Lett.B 616

(2005) 8.

• Technical– B. Bonner et al., Nucl.Instr.Meth.A 478 (2002) 176.– M. Shao et al., Nucl.Instr.Meth.A 492 (2002) 344.– W.J. Llope et al., Nucl.Instr.Meth.A 522 (2004) 252.– F. Geurts et al., Nucl.Instr.Meth.A 533 (2004) 60.– J. Wu et al., Nucl.Instr.Meth.A 538 (2005) 243.– Y. Wang et al., Nucl.Instr.Meth.A 538 (2005) 425.– Y.E. Zhao et al., Nucl.Instr.Meth.A 547 (2005) 334.

Page 12: STAR MRPC TOF: Project Overview BNL January 26, 2006 Geary Eppley Rice University

Organization chart

Page 13: STAR MRPC TOF: Project Overview BNL January 26, 2006 Geary Eppley Rice University

Manufacturing overview

• Module production and test, electronics production and test, and tray assembly and test each have a duration of ~2.2 years.

• Module production begins ~3 months before the start of tray assembly and electronics production ~1.5 months before the start of tray assembly.

• Modules are thoroughly tested in China with integral HV wire and signal cables.

• Electronics cards are tested in groups of 17, 1 tray, with their integral cables and sent to the tray assembly site as a set.

• Modules are assembled into trays, the electronics added, and tested for 2-4 weeks as a complete detector unit.

• Tested trays are shipped to BNL as complete detector units ready for insertion into STAR.

• Trays are re-tested at BNL: HV current, noise rates, gas leak test

• Test beam at BNL for selected trays?

Page 14: STAR MRPC TOF: Project Overview BNL January 26, 2006 Geary Eppley Rice University

Gantt chart

Page 15: STAR MRPC TOF: Project Overview BNL January 26, 2006 Geary Eppley Rice University

TOF system functional requirements

Number of stop detector channels 23040 total, 192 per tray Number of “live” channels >175 per tray Number of start detector channels 38 Noise rate per channel (stop-side) <50 Hz Tray high-voltage current (no beam) <50 nA System overall timing resolution <100 15ps, in Au+Au collisions Electronic overall timing resolution, single channel <45 ps Total power consumption <40 kW Average single hit efficiency >90% Level 0 trigger multiplicity rate 9.4 MHz Level 0 trigger multiplicity latency 700 ns Pre-Level 0 time-stamp buffer size 128 time-stamp pairs per 2 channels Average dead time per hit <50 ns Maximum time stamp acquisition rate per channel 2 MHz Bandwidth from pre-level 0 buffer to pre-Level 2 Buffer

80 M-bit/s/tray: >10k events/s/tray

Bandwidth from pre-Level 2 buffer to DAQ 5 G-bit/s: >2k events/s

Page 16: STAR MRPC TOF: Project Overview BNL January 26, 2006 Geary Eppley Rice University

Current project status:

• Cosmic ray testing of the TINO front-end board is ongoing.

• Automated TINO board production has been achieved.

• Upgraded 38-channel start detector under construction.

• Based on a recommendation from the review, the China TOF project built a few new modules with highly resistive electrodes. Due to difficulties involved with the manufacturing process, the China groups decided to stick with the graphite-tape electrodes.

• Layout of the first prototype THUB is underway.

• The project started officially January 1. We hope to get the university accounts open before the end of February.

Page 17: STAR MRPC TOF: Project Overview BNL January 26, 2006 Geary Eppley Rice University

TOF Gas system

• The TOF system will operate on a gas mixture of 90 parts r134a and 5 parts isobutane.

• The system will vent ~12 pounds r134a per day during STAR operations

• The system will be sealed but not operate during shutdown periods.

• The isobutane/r134a ratio is set by the factory calibration of the mass flow meters. It will also be monitored by an isobutane analyzer.

• The aggregate gas circulation rate through the trays is ~450 l/h.

• The gas is re-circulated and dried maintaining H2O<20 ppm, O2<30 ppm.

• The system is interfaced to STAR slow controls through a shared disk. Isobutane content is alarmed to insure non-flammable gas. Gas flow is alarmed to maintain safe operation of the trays.

Page 18: STAR MRPC TOF: Project Overview BNL January 26, 2006 Geary Eppley Rice University

TOF gas system schematic

Page 19: STAR MRPC TOF: Project Overview BNL January 26, 2006 Geary Eppley Rice University

DOE review recommendation

• Investigate using SF6 or C4F10: Improves MRPC operational characteristics.

• Our reply: Our AGS 11-week test run data confirms this: SF6 greatly extends the HV plateau from <500v to >1000v.

• Using SF6 will allow running at a higher voltage and improve timing resolution.

• We will investigate:– Developing standards for gas-tight integrity– Adding gas leak SF6 detectors– Adding positive air flow in the TOF tray area