Performance of the LHCb RICH detectors On behalf of the LHCb-RICH Collaboration Sajan Easo Rutherford-Appleton Laboratory IEEE-NSS: Dresden, Germany, 21-10-2008.

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Presentation transcript:

Performance of the LHCb RICH detectors On behalf of the LHCb-RICH Collaboration Sajan Easo Rutherford-Appleton Laboratory IEEE-NSS: Dresden, Germany,

2 Outline  Two RICH detectors in LHCb:  HPDs (Hybrid Photon Detectors ):  Results from Commissioning :  Performance from Simulations: Photoelectron yields, Cherenkov angle resolutions PID performance Monitoring magnetic field distortions Time alignment of readout Description Characterization Design features of the RICH system Components of RICH1 and RICH2

Acceptance : from 10 mrad to 250 mrad (vertical), 300 mrad (horizontal) Optimized to study the decays of B-Hadrons Probe physics beyond the standard model Precision measurements of CKM angles The LHCb Experiment at the LHC Particle identification at LHCb:  K separation in GeV/c Two RICH detectors:RICH1, RICH2 RICH1RICH2 3 Forward Spectrometer

LHCb-RICH C 4 F 10 gas n=1.0014, L~85cm Up to ~60 GeV/c CF 4 gas n=1.0005, L ~ 200 cm Up to ~100 GeV/c Cherenkov Angle Silica Aerogel n=1.03, L=5cm 1-10 GeV/c RICH1RICH2 4 Several test beam studies over 10 years Latest test beam results : Presentation (N56-3) by H.Skottowe at this conference.

Spherical Mirrors Lightweight carbon fibre mirrors 1.4% radiation length. RICH1 Detector Glass Planar Mirrors Gas Enclosure supports mirrors and aerogel, contains C 4 F 10 Photon detector plane 14 by 7 Array of Hybrid Photon Detectors (HPDs) Upper Magnetic Shielding Protects HPDs from B field, supports upper HPDs Beryllium beampipe (defines RICH1 inner acceptance) 4 m 1.175m Quartz Window Entrance Window sealed to LHCb-Vertex Detector Exit Window made of Carbon fibre and PMMI foam. Aerogel Tiles 5

RICH1-HPD Array Aerogel in RICH1: 16 tiles made at Novisibirsk Tile size up to 20cm*20cm*5cm. Rayleigh Scattering: Non-scattered Transmission = A exp –(Ct/λ 4 ) where typically A=0.93 C=  m 4 cm -1 t=5cm,  wavelength Prototype Aerogel tests: NIMA 553(2005) p 356 Also N30-218: D.L.Perego RICH1 Detector Spherical Mirrors Aerogel Tiles Mirrors : Size 640mm X 835 mm, made from Carbon Fiber Reinforced Polymer by CMA (USA). Coating: Al (80nm)+ MgF 2 (160nm) by SESO(France) (NIMA 595 (2008) p. 197 ) Mirror D 0 ~ 1.2 mm 6

RICH2 Detector 8m Spherical Mirrors each made from 28 glass hexagonal segments Flat Mirrors each made from 20 square glass segments RICH2 entrance / exit windows : carbon fibre and PMI foam sandwich Magnetic Shields (12 tons) protect the HPD planes 9 by 16 array of HPDs inside shieldings 2m HPD Column in RICH2 Mirrors installed within an alignment precision of 0.3 mrad Signals from HPD sent via a 100 m optical cable to LHCb-DAQ

Hybrid Photon Detectors 484 HPDs covering 3.3 m 2 with > 64% active area fraction. Typical Threshold = 970 e -, Noise = 130 e –, Signal = 5000 e – All the HPDs characterized using dedicated test stations : (NIMA 595 (2008) p 142 ) Dark Counts: below 5 KHz/cm 2 (specification: max 20 KHz/cm 2 ) 98% of HPDs produced well within specifications for LHCb. Vacuum Quality: Look for signs of IFB (Ion Feed Back): Typical rate of IFB hits = 0.04 % (specification: max 1%). Recently, some HPDs from early production batches seem to have developed a larger rate; they are replaced with new tubes and the old tubes are being investigated in detail. Photodetectors: Pixel HPDs Developed in collaboration with industry. (Photonics-DEP: main partner) 8 Prototype developments:NIMA 530(2004) p. 82, NIMA 449(2000) p.48

RICH Commissioning: Magnetic Field Distortions Magnetic fields distort the photoelectron trajectory : image distortions and loss of signal Overall shielding + individual shielding around HPDs : avoid loss of signal. RICH1: max field ~600 Gauss  below 24 Gauss OK for HPD operation. RICH2: max field ~150 Gauss  below 6 Gauss Monitoring and correcting for image distortions in situ: RICH2:  Send a pattern from a projector into the HPD array  Measure the image with/without the Field  Parametrize rotation of the image and correct for it Average Rotation (rad) Position resolutions after corrections :  x = 0.76 mm,  y = 0.73 mm = Resolutions from HPD pixel size alone. RICH1 : A similar distortion monitoring system using an array of LEDs is being commissioned. 9 Max. effect of magnetic field

RICH Commissioning: Time Alignment LHC beam dump  Muons  LHCb : used for time alignment of RICH with LHCb trigger Events Display: Integrated over a few events Typical Delay time scan between laser pulse and HPD readout 10 RICH readout system fully integrated to LHCb online system RICH1 Delay RICH2 : Muon hits RICH1: Muon hits

Performance From Simulations Full simulation: PYTHIA  EVTGEN  GEANT4  Digitization (TNS: vol 52, No.5 (2005), p 1665) Pattern recognition and PID: Global Likelihood method (NIMA 433(1999) P 257 ). Aero- gel C 4 F 10 CF 4 Chromatic Emission Pt Pixel PSF Overall RICH+Tracking  Current yields from fully contained isolated saturated tracks:  Single photoelectron Cherenkov angle resolutions in mrad (Data Challenge 2006) The yields include the backgrounds from various reflections and backscattering within the HPD which contribute ~15% to the yield. AerogelC 4 F 10 CF Kaon Identification Performance 11

RICH Calibration  MC free calibration : Select events from real data in the channel D *+ --> D 0  +, D 0  K +   Selection of events mainly from the narrow mass difference (145.4 MeV) between D* and D 0  Calibrate the results of RICH PID performance for the pions and kaons selected, in bins of P and Pt of the corresponding tracks. Identified using MC Truth Identified using D* K  K,Pr  --> K, Pr  Dedicated trigger to provide 10 7 events in one year of data.  Other possibilities : Select     and Ks   +    from the data for calibration. 12 Efficiency

Summary The two RICH detectors are successfully installed in LHCb These detectors are read out as part of the LHCb data acquisition system and they are being commissioned with LHC beams. Using fully simulated data the performance of the detectors are evaluated and procedures for alignment and calibration are developed. We are eagerly waiting for LHC collisions to get real data and to see Cherenkov rings ! 13

14 Spare Slides

Optical Configuration of RICH1 and RICH2 Directions of bb production Spare Slides 15 RICH Readout configuration RICH2 HPD column

RICH1- Photo Spare Slides 16 RICH2 HPD array RICH2: Pixel resolution after Field corrections. Pixel chip

17 Spare slides Hits integrated on RICH2 HPD array using photons from a pulsed laser Effect of Magnetic field Inside RICH2 HPD Pattern from a Projector into RIC H2