SiW ECAL Technological Prototype Test beam results Thibault Frisson (LAL, Orsay) on behalf of the CALICE collaboration.

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Presentation transcript:

SiW ECAL Technological Prototype Test beam results Thibault Frisson (LAL, Orsay) on behalf of the CALICE collaboration

SiW ECAL for a future LC SiW ECAL is one of the prototypes for future LC detectors Optimized for Particle Flow Algorithm: Basic Requirements: - Extreme high granularity - Compact and hermetic Basic Choices: - Tungsten as absorber material X0=3.5mm, RM=9mm, lI=96mm Narrow showers Assures compact design - Silicon as active material Support compact design Allows for pixelisation Large signal/noise ratio The SiW ECAL in the ILD Detector Oct. 24 2012 LCWS - Arlington 2012

Technological Prototype SiW ECAL R&D Physics Prototype Proof of principle 2003 - 2011 Technological Prototype Engineering challenges 2010 - ... LC detector ECAL : Channels : ~100 106 Total Weight : ~130 t Number of channels : 9720 Weight : ~ 200 Kg Number of channels : 45360 Weight : ~ 700 Kg Oct. 24 2012 LCWS - Arlington 2012

Physics prototype 30 layers of tungsten: 24 X0, 1 I Carbon-fibre mechanical structure 30 layers of tungsten: 24 X0, 1 I S/N ~ 8 E / E = 16.5/√E(GeV) + 1.1 % 10k channels Studied in various test beam facilities 2006-2011: DESY, CERN, FNAL, e-, , , p (1  180 GeV) [JINST 3, 2008] 6x6 PIN Diode Matrice – 1 x 1 cm2 Résistivity: 5kcm - 80 (pairs e/hole)/m 62 mm Thickness: 525µm Oct. 24 2012 LCWS - Arlington 2012

Technological prototype Technological solutions for the final detector Construction start: 2010 Test beam: 2012 Realistic dimensions Integrated front end electronic Small power consumption (Power pulsed electronics) Oct. 24 2012 LCWS - Arlington 2012

The road to the technological prototype Intermediate step: First test in beam Benchmark to go further U structure (single detection layer per slab) Si wafer: 9x9 cm2 – Thickness = 320 mm pixel size: 5x5 mm2 :lateral granularity = 4 x better than physics prototype SKIROC2 ASICs 4 ASICs per slab (1⁄4 final design) 4 SKIROCs x 64 channels = 256 channels/slab (See Rémi Cornat's Talk) Trigger delay Preamplifier (adjustable gain) Internal trigger (self-triggering capability) Oct. 24 2012 LCWS - Arlington 2012

total active channels = 1278 First test beam with the technological prototype DESY – April and July 2012 e- (1 - 5 GeV) 6 layers (FEV8) - Internal trigger Total = 1536 channels PreAmplifiers of noisy channels are switched off total active channels = 1278 PVC structure - position for tungsten plates (2.1 mm) Goals: - Determine signal over noise ratio of the detector - Operate first layers of the technological prototype - Establishment of calibration procedure for a large number of cells - Homogeneity of response (x,y scan of detector) Oct. 24 2012 LCWS - Arlington 2012

Calibration of ASICs Establishment of calibration procedure for a larger number of cells Trigger threshold - depends on the gain Trigger delay - depends on the trigger threshold Oct. 24 2012 LCWS - Arlington 2012

Beam spot Oct. 24 2012 LCWS - Arlington 2012

Detection efficiency At least 3 layers with hits Data: 3GeV – No W – XY scan Total number of events: 2,3.106 Track selection: At least 3 layers with hits Linear fit of the e- track Nhits<10 Inefficiencies due to: Switched off channels Too high trigger thresholds (80%-95% of the MIP) Should be improved with the next test beam (December) Data Simulation Data Simulation Oct. 24 2012 LCWS - Arlington 2012

Energy measurement 1 e- 2e- 3e- Electron sources: Oct. 24 2012 Beam delta rays Bremsstrahlung + gamma conversion (2e-) + Compton Oct. 24 2012 LCWS - Arlington 2012

Energy calibration Establishment of calibration procedure for a larger number of cells Homogeneity of response (x,y scan of detector) Data Simulation Oct. 24 2012 LCWS - Arlington 2012

Signal over noise ratio R&D target is 10:1 S/N > 10 (for all gains available with SKIROC2) Oct. 24 2012 LCWS - Arlington 2012

5 W plates between layers Event display 2 e- (3 GeV, no tungsten) 3 e- (3 GeV, no tungsten) 1 e- (5 GeV) 5 W plates between layers 1 cosmic + 1 e- (3 GeV, no tungsten) Oct. 24 2012 LCWS - Arlington 2012

Test beam in December Power pulsing Conclusion Successful beam test Excellent stability of the DAQ Stable operation of the wafers and the electronic Establishment of calibration procedure for a larger number of cells Homogeneity of response studies Energy calibration Detection efficiency Determination of the signal over noise ratio: S/N > 10 Hardware effects revealed. Data and detector about to be understood. Test beam in December Power pulsing Oct. 24 2012 LCWS - Arlington 2012

Thanks Frédéric, Mickael, Patrick, Rémi and Stéphane Special thanks to our experts: Frédéric, Mickael, Patrick, Rémi and Stéphane And to everyone who took part in the preparation of the test beam: - LLR, LAL+OMEGA, LPNHE - Kyushu University, Tokyo University, Nippon Dental University - SKKU Oct. 24 2012 LCWS - Arlington 2012

Back up Oct. 24 2012 LCWS - Arlington 2012

Noise width Oct. 24 2012 LCWS - Arlington 2012