k1.8 meeting report from e05 group toshiyuki gogami 26 dec 2014

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K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

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Page 1: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

K1.8 meetingReport from E05 group

Toshiyuki Gogami26 Dec 2014

Page 2: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

Contents

Cosmic ray test of (Prototype) Water Cherenkov detector

PMT comparison (H11284 vs. H6522)Position dependence (y-dependence)Normal acrylic window UVT acrylic window

Page 3: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

Goal of development of Water Cherenkov detector

Goal: NPE for 1.3 GeV/c K+ 50(NPE for β=1 particle 60)

p rejection eff. > 90%K+ survival ratio > 99%for 1.3 GeV/c @ trigger

Page 4: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

Experimental setup

Unit: mm

Page 5: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014
Page 6: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

Coordinate definition

Data were taken with y = -25.0, -12.5, 0.0, 12.5, 25.0 cm

Wat

er C

here

nkov

y

0

H6522

H11284(CH1)

(CH2)(CH3)

Scintillator

Scintillator

BA (QE~25%)

SBA (QE~35%)

Window: Normal Acrylic

Page 7: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

Calibration with LED data

ch/N.P.E.

ch/N.P.E.

ch/N.P.E.CH1

CH2

CH3Fitting function: E.H.Bellamy et al. , NIM A 339, 468-476 (1994)

Page 8: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

ADC Number of Photo Electron

y = -25.0 cmwith WC TDC cut

Gaussian fitting N.P.E.

Page 9: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

Results (y=0)

Wat

er C

here

nkov

y

0

H6522

H11284

Scintillator

𝑁𝑃𝐸 30𝑁𝑃𝐸 30

𝑁𝑃𝐸 40

Same ?

Now checkingwith cosmic ray.

In simulation almost same

Page 10: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

The number of photoelectrons(ratio)

±20%

Page 11: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

WindowNormal acrylic UVT acrylic

H11284

Scintillator

𝑁𝑃𝐸 40

Normal Acrylic

H11284

Scintillator

𝑁𝑃𝐸 100

UVT acrylic(Acrylite#000)

Page 12: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

Summary

Cosmic ray test of (Prototype) Water Cherenkov detector

PMT comparison (Normal acrylic window)H6522: NPE~30H11284: NPE~40

Position dependence±20% in 30 cm Sum of top and bottom PMTs expect to be flat.

WindowNormal acrylic window + H11284: NPE~40 UVT acrylic window + H11284: NPE~100

Goal for one segment: 60 Goal for one PMT: 30

Page 13: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

OutlookCosmic ray test

• Other windows• Individual difference of PMT• Grease

Geant4 simulation• Effects on trigger due to reactions in water • p rejection efficiency and K+ survival ratio

Design• Can be thinner ?• Frame

Page 14: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

Backup

Page 15: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

Cap design for window test

Page 16: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014
Page 17: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014
Page 18: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014
Page 19: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014
Page 20: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014
Page 21: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014
Page 22: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014
Page 23: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014
Page 24: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

Prototype water Cherenkov detector

Page 25: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

Geant4 (S-2S)

Page 26: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

Pedestal movement

CH1 CH2

CH3

Pedestal parameter was applied for run by run.

Page 27: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

The number of photoelectron(absolute value)

39.7±0.4

57.4±0.5

H6522H11284

Page 28: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

The number of photoelectron(ratio)

±20%

Could be due to geometrical advantage.

Page 29: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

Cosmic ray test witha window of Acrylite#000

WC

Scintillators

Page 30: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

TOF detector

(idea)

Page 31: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014
Page 32: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014
Page 33: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014
Page 34: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014
Page 35: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

Speed of light in S-2S TOF detector

Page 36: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

Experimental setup

90SrTOP view

Side view

Measured the time difference between signals from two PMTs.

Channel 1 Channel 2

Page 37: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

Experimental setup (Photograph)

TOF

90Sr

TOF 90Sr

ZOOM

center

Page 38: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

Time difference between two PMT signals

Fitting with Gaussian function

Time difference

Page 39: K1.8 meeting Report from E05 group Toshiyuki Gogami 26 Dec 2014

Results

Fitting results NO. NAME VALUE ERROR SIZE DERIVATIVE 1 p0 2.07196e-02 2.22470e-02 1.79174e-04 1.76260e-032 p1 1.57154e+01 1.16172e-02 9.35617e-05 2.69538e-02

The effective speed of light in TOF detector: [m/s]

Fitting with linear function:[0] + [1]*x