emulsion detector for future neutrino research possibility of the technology
DESCRIPTION
Emulsion Detector for Future Neutrino Research Possibility of the Technology. NAKAMURA M. (NAGOYA Univ.). CONTENTS. Emulsion Detector Overview New Study. Emulsion Spectrometer Emulsion in Magnetic field Expected scanning power in near future. Intrinsic position resolution. - PowerPoint PPT PresentationTRANSCRIPT
Emulsion Detector for Future Neutrino Research
Possibility of the Technology
NAKAMURA M. (NAGOYA Univ.)
CONTENTS
• Emulsion Detector Overview
• New Study. Emulsion Spectrometer
Emulsion in Magnetic field
• Expected scanning power in near future
Cross sectional view of an emulsion layer
30grains/100mgrain diameter ~ 0.6m
Ag grain after development
dx
= 0.06m
Compton Electron
Fog
M.I.P. Track
100m
M.I.P. Track
Intrinsic position resolution
One Emulsion Layer = vector chamber with 60nm position resolution
& ~1mrad Angular resolution (100micron layer)
Achievement in OPERA R&D
• Nuclear Emulsion Films
Suited for Mass production ~ 100,000m2
Uniform quality
Refresh function R&D by
Nagoya Univ. & Fujifilm
• Fast Scanning systems
in Japan & Europe
125mm
100mm
Refresh
Cosmic-rays
Emulsion film accumulates all signals during its live time
:No dead time.
Compton electrons by γ rays of natural radio activity
Before Refresh After Refresh
We can reset the accumulated images by Refreshing.
Before use or re-use
OPERA ECC Brick
10cm
12.5cm8cm
8kg: Portable Unit for 2~10kton detectors
Tau detection :
DONUT -> OPERA
Topological decay detection:
Kinematical analysis: Momentum measurement by Multiple Coulomb Scatterings (or Emulsion Spectrometer) Electron ID by shower detection Particle ID by dE/dX measurement
Decay search
τ
Fe
film
dE/dX measurement
Pb Film
P=1.2GeV/c
Hadron+
@KEK/PS
dE/dX
dE/dX = measurement
~number of grains
P
dE/dX measurement : TEST exp at KEK0.4 GeV/c 0.5 GeV/c 0.6 GeV/c
0.74 GeV/c 0.87 GeV/c 1.14 GeV/c 2.0 GeV/c
P P P
PP
P
π π π
π π π
D
D D D D
P&π
Entry 1610 tracks Entry 1345 tracks Entry 1175 tracks Entry 1206 tracks
Entry 996 tracks Entry 1310 tracks Entry 1278 tracks
• Using only 5 ~ 6 films.• VPH, measured by the system, is ~propotional to dE/dX.
VPH
P
π
P andπ
Using 5 ~ 6 films.VPH, measured by the system, is ~propotional to dE/dX. Error bar is 1σof the distribution. At 2 GeV/c , proton and pion are not separated in 5 or 6 OPERA films.VPH of proton below 0.6GeV/c is saturated.
Particle ID by dE/dx Measurement
K
dE/dx(MeV ・ cm2/g)
Momentum(GeV/c)
VPH
e
KEK Beam Test Preliminary
50GeV electrons + muons
Electron ID
Test Exp. @ CERN
Electron energy measurement
MC Data
)(E
4.0~
GeV
@ a few GeVEnergy determination by calorimetric method( in study)
Test exp. @ CERN
Emulsion in Magnetic Field
• Charge Sign determination + increase sensitivity + increase BG-rejection power
o scanning load (mention later) o cost??
• We have experience in CHORUS/ET(Emulsion Tracker)
Structure for MC study
Stainless steel or Lead Film
Air Gap
DONUT/OPERA type target + Emulsion spectrometer
B
~ 3Xo ~10Xo
Assumption: accuracy of film by film alignment =10 micron (conservative).(Ex. 20mm gap structure gives 0.5mrad angular resolution.)
mu
Charge determination (0.5T) MC
P(GeV/ c) Eff. 20mm Eff. 30mm1 99.93% 99.96%2 99.95% 99.97%3 99.94% 99.67%4 99.90% 99.98%5 99.83% 99.96%6 99.58% 99.97%7 98.98% 99.97%8 97.97% 99.96%9 96.78% 99.97%
10 95.32% 99.95%
10mm Gap
20mm Gap
>=30mm Gap
Momentum resolution(0.5T) MC
10mm Gap
20mm Gap
30mm Gap
40mm Gap
50mm Gap
P(GeV/ c) Eff. 20mm Eff. 30mm1 99.980% 99.994%2 99.983% 99.993%3 99.979% 99.993%4 99.981% 99.992%5 99.973% 99.998%6 99.978% 99.996%7 99.981% 99.994%8 99.976% 99.990%9 99.966% 99.995%
10 99.947% 99.994%
Charge determination (1.0T) MC
10mm Gap
>=20mm Gap
Momentum resolution(1.0T) MC
10mm Gap
20mm Gap
30mm Gap
40mm Gap50mm Gap
Summary of the MC study• Emulsion Spectrometer ( B 0.5T,Gap > 20mm, ≧
Total Length~10cm) has power to determine sign & momentum efficiently.
• Further MC study: Investigate the Possibility to open the sensitivity
for hadronic and electric decay mode. Sensitivity >~ x 3 (like OPERA)
• Technological R&D : Unique track connection How to keep air gap Test exp.
Emulsion Film Read-out
Emulsion Readout History
• E531, E653, etc . (~1994) – Semi-automatic scanning
• CHORUS phase I– Track selector, New TS (1994~)
• DONUT, CHORUS phase II– UTS (1998~) Net scan (angle: |<0.4).
• OPERA
Automatic Automatic ScanningScanning
Bottle necks in the Read-out System
Speed of Image Data taking
Movement of Z Stage
Field of View :
Objective Lens
Movement of X-Y stage
Overcome the Bottle necks
Stage moves at constant velocity
Synchronized motion to cancel relative velo.
Ultra High Speed Imager with Real Time processing
• Ultra High Speed Imager– 120 fps -> 3000 fps
• Image taking by follow shot– X-Y stage : Non-stop – Objective lens: Driven by piezo electr
ic devices ( fres>2kHz ) .
• Enlarging size of Field of View– Effective FOV: 100m×100m-> 140m×140m
1cm2/h -> 60cm2/h
SUTS + Old stage
0.008
0.25
3
60
0.001
0.01
0.1
1
10
100
TS(TTL) NTS(CPLD) UTS(FPGA) S-UTS
Scanning System Historyviews/sec(1view=120×90 m2)
Evolution of the Scanning Power
Our code name (device technology)
CHORUS DONUT OPERA
Expected evolution of the Scanning Power in near future
• Enlarge a Field of View × (1.25)2 reduce objective mag. × 50 -> × 40
• Speed up Image data taking ×4 Ultra High Speed Camera 3kfps->12kfps.
400cm2/hours/system. (~1m2/day/system)
How many events?Scanning Power
1 m2/day/system~ 100events/day/system
( OPERA like ECC 1event/brick ~100cm2/event)
~25,000events/year/system
Normally one lab has ~10 system
~250,000 events/year/lab.
Events in Neutrino Factory
160,000 events/kton
(L=3000km,1021mu+ decays)
Event selection for 10kton
• 10kton Total event: 1,600,000
= 1,600,000/250,000
~ 6 Lab ・ year
Loose-selection is Acceptable.
• During the RUN : Extract and Analyze wrong sign muon events.
End of the RUN : Extract all bricks which have tagged neutrino interactions in it.
L3 Magnet 0.5T
OPERA 1SM 850t Or Modified ATLAS TROID
Related Works
• OPERA Exposure will start at the middle of 2006. Scanning in many Labs (Japan, Italy, France, Swiss….)• PEANUT Test exp. at NUMI near detector site. Start neutrino exposure at Aug. 2005. Plan: Test of “ ECC in Magnet” with Permanent magnet (2006).
OPERA 1st Super Module
2nd Super Module
PEANUT Detector :DONUT SFT+ Mini Brick Wall
MINOS Near detector as mu ID
Location of Neutrino interactions in ECC brick
1. Pick up tracks in the most downstream plate
Neutrino
2. Follow tracks to the interaction veretex
P measurement using Multiple Scattering
rms
rms 1
n n : number of measurements
For example: 10 GeV/c has rms deflection of 0.3m
Kinematical AnalysisMomentum
measurement
Momentum measurement
Low dE/dX
Higher dE/dX
Consistent with Pion
Consistent with Proton
P measurement using Multiple Scattering
Expected Value for pion
Expected Value for proton
Resolution p