new chod prototype tests at cern

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New CHOD prototype tests at CERN. V. Duk, I. Mannelli + help from Claudio Cerri, Riccardo Fantechi, Luigi Di Lella. 1. plan. Current status of the New CHOD Setup for tests at CERN First results with Standard Tile Conclusions. 2. Current status of the New CHOD. - PowerPoint PPT Presentation

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New CHOD prototype tests

at CERN

V. Duk, I. Mannelli + help from

Claudio Cerri, Riccardo Fantechi, Luigi Di Lella

128.08.2013 V.Duk, I.Mannelli

2

plan

28.08.2013 V.Duk, I.Mannelli

1.Current status of the New

CHOD

2.Setup for tests at CERN

3.First results with Standard Tile

4.Conclusions

3

Current status of the New CHOD

28.08.2013 V.Duk, I.Mannelli

Design from Italo:1 plane148 slabs 265x107x30 (Standard Tile)Fiber readout, 18 fibers per slabPM or SiPM readoutSiPM: 2 readout channels per slab in coincidence

See Italo’s talk at MUV/CHOD WG, 05.06.2013

4

Tests of the new CHOD

28.08.2013 V.Duk, I.Mannelli

Protvino:EJ200 100x100x20, 200x100x20, 300x100x20Bicron 150x150x20Fiber&direct SiPM readout (SiPM CPTA-146, PM Hamamatsu 7400U, SenSL)Direct PM readout (Hamamatsu 7400U)Talks at weekly meetings (28.02.2013, 23.05.2013) and MUV/CHOD WG (05.06.2013, 28.08.2013)Mainz:Protvino scintillator 420x60x10, 390x100x15Fibers with d=1.2 mmPM readout (Hamamatsu R6095)Talk at MUV/CHOD WG 10.04.2013

Standard Tile: 265x107x30

Naples:Mainz setup Double SiPM readout (Hamamatsu 6x6 mm)

CERN:Standard Tile Double SiPM readout (Hamamatsu 3x3 mm)Talk at Weekly meeting 18.07.2013

5

Setup at CERN

28.08.2013 V.Duk, I.Mannelli

Scintillator(made in Protvino):265x107x30

Fibers:BCF-92, d=1.0 mm18 fibers glued (9 from one side, 9 from the other)

Readout: 2 SiPM Hamamatsu S10931-050P 3x3 mm2

Preamplifier from Frascati

2 trigger counters:80x40x10 (top), 40x40x5 (bottom)PMT readout~500-600 ps time resolution per counter

Data acquisition:Lecroy Wafesurfer 44xs (2.5 GS/s)

Main goal: to test Standard Tile

scintillator

PM(top)

PM(bottom)

2nd Standard Tile from Ferdi in preparation

Fiber arrangement

6

Data & analysis

28.08.2013 V.Duk, I.Mannelli

Data sample:22.08.2013, 3369 triggers

Trigger: PM(top) & PM(bottom)Offline threshold for time measurements: 50mV

“software CFD” correction:Calculate maximum UmaxTake time at 0.2*Umax

Data recording: Lecroy Wavesurfer 44xs, 4 channels with an external triggerCH1: PM(top)CH2: PM(bottom)CH3: SiPM(right)CH4: SiPM(left)

7

Signals from PMs

28.08.2013 V.Duk, I.Mannelli

Small amplitudes: inclined muons

Large amplitudes (peak at 300-400mV): MIP

Amp, V Amp, V

8

Signals from SiPMs

28.08.2013 V.Duk, I.Mannelli

1 p.e. ~ 20 mV<A> ~ 600 mV

Good light yield:> 30 p.e.

Amp, V Amp, V

9

Amplitude correlations

28.08.2013 V.Duk, I.Mannelli

PM:amplitude configuration can be small-small, big-small, big-big (good particle)Large amplitudes correspond to slewing corrections

SiPM:Good correlation

Transparent scintillator

Amp, V

Amp, V Amp, V

Amp, V

Amp, V

Amp, V

Amp, V

dt, ns

10

Time resolutions

28.08.2013 V.Duk, I.Mannelli

Time resolutions from solving system of equations:SiPM left: ~0.56 nsSiPM right: ~0.48 nsTrigger: ~0.78 ns

SiPM time: software CFD correction

PM time: no time correction

T(SiPM left) –T(trg)

σ ~ 0.96 ns

T(SiPM right)–T(trg)

dT(SiPM)T(SiPM,mean) – T(trg)

σ ~ 0.84 ns

σ ~ 0.74 ns

σ ~ 0.92 ns

dt, ns dt, ns

dt, ns dt, ns

11

High PM amplitudes

28.08.2013 V.Duk, I.Mannelli

Time resolutions from solving system of equations:SiPM left: ~0.54 nsSiPM right: ~0.49 nsTrigger: ~0.66 ns

T(SiPM left) –T(trg) T(SiPM right)–T(trg)

dT(SiPM)T(SiPM,mean) – T(trg)

σ ~ 0.85 ns

σ ~ 0.72 ns

σ ~ 0.73 ns

σ ~ 0.82 ns

dt, ns dt, ns

dt, ns dt, ns

SiPM time: software CFD correction

PM time: no time correction

12

conclusions

28.08.2013 V.Duk, I.Mannelli

Standard Tile is prepared

Setup is working

Time resolution ~0.5ns obtained (after corrections)

Np.e.>30

THANK YOU!!!

1328.08.2013 V.Duk, I.Mannelli

spares

14

PM time resolution

28.08.2013 V.Duk, I.Mannelli

dt, ns dt, ns

dt, ns dt, ns

15

Risetime (Tmax – T0.2max)

28.08.2013 V.Duk, I.Mannelli

dt, ns dt, ns

dt, ns dt, ns

16

Temperature effects

28.08.2013 V.Duk, I.Mannelli

Change in T

Change in V(breakdown)

Change in risetime/amplit

ude

Change in HV-V(breakdown)

Change in gain

17

Selected events

28.08.2013 V.Duk, I.Mannelli

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