the nuclear emulsion technology and the analysis of the opera experiment data
DESCRIPTION
The Nuclear Emulsion Technology and the Analysis of the OPERA Experiment Data. Tsutomu Fukuda Nagoya University, JAPAN On behalf of the OPERA Collaboration. DPF-APS 2009 , 28 JULY 2009, Wayne State University in Detroit. Recorded as silver grains along the line particle passed through. - PowerPoint PPT PresentationTRANSCRIPT
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The Nuclear Emulsion Technology and the Analysis of the OPERA
Experiment Data
Tsutomu Fukuda Nagoya University, JAPAN
On behalf of the OPERA Collaboration
DPF-APS 2009 , 28 JULY 2009, Wayne State University in Detroit
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Nuclear Emulsion Nuclear Emulsion is a special kind photographic film.
: AgBr micro crystal semiconductor (Band gap ~ 2.6eV). Signal is amplified by chemical process (developing).
50 micron
Microscopic Image
Recorded as silver grains along the line particle passed through
Resolution of 0.3 micron
Sub micron resolution 3D tracking
Nuclear Emulsion is used
1947 (C.Powell et al.)
Discovery of .
1971 (K.Niu et al.) Charm particle is discovered in cosmic-ray (called X-particle).
2001 (K.Niwa et al.) The first observation of at Fermi-Lab.
2009 ? First direct observation of
oscillation appearance
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OPERA experiment
Theory:In 1962, Maki, Nakagawa and Sakata conceived massive neutrino will oscillate.
Important experimental result (1):In 1998, Super-Kamiokande detected the behaviour of neutrino oscillation (atmospheric disappearance).
Important experimental result (2):In 2001, DONUT ( FermiLab experiment) succeeded in detecting by Emulsion Cloud Chamber (ECC).
Goal:The goal of OPERA is to detect oscillated from by ECC.
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Conceptual Design
• The detector is located on the CNGS (CERN Neutrinos to Gran Sasso) beam line at a distance from the neutrino source of 730km.• Δm23
2 = (2.43±0.13)×10-3 eV2 , sin22θ23 = 1.0
• # of events = 4300/year • expected detectable # of CC events ~ 2.5/year
Here, I will mainly talk about Emulsion Technology and Analysis.
INFN Gran Sasso
CERN SPS
730km
Appearance
Underground Laboratory
conventional beam
( m-2 / pot) 7.45x10-9
CC / pot / kton 5.44x10-17
< E > ( GeV ) 17 (e + e) / 0.85 % / 4.0 % prompt negligible
%7.1~27.1sin2sin 2322
232
E
LmP τμ
ECC detector ~ 1.3kton
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ECC (Emulsion Cloud Chamber)125mm
100mm
75.4mm
8.3kg10X0
Neutrino Beam
OPERA emulsion film
Lead plate : 1mm
210μm44μm
emulsionPlastic base
beam 1mm
Lead
OPERA film
57 emulsion films and 56 Pb plates piled up.
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Kink e 18 % 17 % h 49 %
Trident 3h (h h h) 15 %
How to detect tau neutrino
Flight Length: 280um
DONUT event
1mm
Emulsion
DONUT : Iron 1mmOPERA : Lead 1mm
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The OPERA Detector @ Gran Sasso(1400m underground)
Emulsion +Target Tracker Muon
spectrometer
Emulsion - Electronic Detectors Hybrid Detector
Emulsion Detector (ECC brick)
1.25 kton = 150,000 ECC bricks
ECC10cm
2.6cm
12.5cm
Changeable Sheet (CS)
T T
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Flow of Emulsion Analysis
1. Location
Emulsion analysis is performed in two main steps
2. Decay Search
Trigger on Electronic detector ↓Connection from Electronic Detector to Emulsion Detector ↓locating the neutrino interaction in Emulsion Detector
-
- (e-, h-, 3h)
hh
Searching for tau decay topology
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Vertex Location – trigger by electronic detectors –
CC-like(with muon)
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Vertex Location – trigger by electronic detectors –
NC-like(no muon)
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Vertex Location
The most probable ECC brick is tagged by Target Trackers
extraction
Only CS Developed →Scanning Check tracks from the interaction . half @ Gran Sasso, half @ Japan
CSECC
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Changeable Sheet (CS)
Electronic detectors don’t have enough resolution to identify the ECC
Brick where the interaction has occurred. To identify the brick, CS is needed.
Roles of CS
In the CS, only ν associated track is recorded.If track is found at CS. the daughter of ν interaction. Emulsion film of ECC are developed
In the case a track is NOT found Next Brick should be taken out.
extraction
?
Ratio of erasing > 99%
OPERA film produced in Japan. All accumulated background tracks were erased by “Refreshing”@ the underground G.S. lab.
Refresh: keeping the emulsion films at highrelative humidity(98%) and high temperature(30deg C) for 3days.
Two filmsEasily detached
Non refresh
After refresh
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Scanning speed/system: 75cm2/hHigh speed CCD camera (3 kHz)
Piezo-controlled objective lens
FPGA Hard-coded algorithms
Emulsion Data taking – automatic scanning system – European Scanning SystemJapanese Scanning System
Scanning speed/system: 20cm2/h
Customized commercialoptics and mechanics
asynchronous DAQ software
Nagoya: 4 systems (75cm2/h) 1 systems (20cm2/h) 5 sub systems (1cm2/h)
LNGS: 10 systems, Napoli: 5 systems Bern: 5 systems, Bari: 4 systems Salerno: 4 systems, Bologna: 4 systems Padova: 1 systems
Total 325cm2/h All system : 20cm2/h Total 660cm2/h
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CS Analysis
Emulsion track data consists its position, its slope and its darkness.
A real track is selected by the 4-layercoincidence and then validated by its quality.
In automatic data selection, Track read out Efficiency ~ 75% S/N ~ 1/2
Number of event 1473
Check done 1440
Found @ CS 1110
Next Brick; now going on 330
Current Status of CS
OPERA film OPERA film
To kill BG, 4 hold coincidence !!
Now going on
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ECC
Large area scan~100cm2
Point Scan~100x100m2
Lead
emul
sion
Lead
emul
sion
Lead
emul
sion
Lead
emul
sion
Lead
emul
sion
Lead
emul
sion
Lead
emul
sion
emul
sion
emul
sion
neutrino
Flow of Location – ECC –
CS TT
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y
z
beam
Event: 228913162Brick: 29373Type: CC
y
x
~1.3mm
An example of Found Neutrino Event (1)
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beam
y
z
y
x
Event: 228425652Brick: 16263Type: CC
An example of Found Neutrino Event (2)
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beam
y
z
y
x
Event: 228482662Brick: 53754Type: NC
An example of Found Neutrino Event (3)
19Now going on
Location Summary:Number of events identified (located) in ECC bricks under microscope
NC CC Total
Bricks received in labs 218 959 1177
Bricks measured 195 895 1090
CS to brick connection successful 178 849 1027
interactions located
in the bricks119 678 797
Interaction is upstream wall 12 46 58
interactions in the
dead material4 17 21
(In 1690 events triggered by Scintilator Target Trackers)
’08 Run only
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Decay Search – detect kink topology –
Short flight decay : 60%IP > 5umMin_pt > 250Mev/c
IP ~60% of tau leptons decay in the same Lead plate with vertex.
Long flight decay : 40%
θkink > 20mrad pt > 250Mev/c
~10% : In Film Decay~30% : Next Lead Decay
cτ = 87 micron
Kink detection track angle deference between tau and daughter
Kink detection minimum distance between daughter and vertex point
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Minimum distance between pairs of tracks from neutrino interaction (data, P>1GeV/c)
Minimum distance [micron]
Decay Search:High resolution to identify the topology of decay
IP of a decay daughter of (Monte Carlo)
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Physical value from ECC1.Momentum measurement by multiple coulomb scattering
P = 13.6 (MeV/c)
X0
x
1/P(GeV/c)-1
0.8GeV/c pion : P =0.79(GeV/c), dP/P =11%
1.5GeV/c pion : P =1.53(GeV/c), dP/P =16%
P(GeV/c)
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Physical value from ECC2. Electromagnetic shower
MCData
)(E
4.0~
GeV
@ a few GeVEnergy determination by calorimetric method
Test exp. @ CERN (May2001)
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Physical value from ECC3. Particle ID by dE/dX
Dar
knes
s
-- Darkness
dE
/dX
(M
eV g
-1cm
2 )Momentum(GeV/c)
Momentum-dE/dX
P
0.87 GeV/c
P
D
Entry 1063 tracks
Particle ID
In Emulsion,dE/dX is defined as darkness of track. = 0.98
= 0.54
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Event# 234539244, Brick# 51248
A charm candidate (1)
Kink angle = 209mrad
Flight Length= 1330micron
Decay Pt ~ 460MeV/c
1ry muon
Charm
1ry VTX is PL33. (100960, 52357)
depth=380micron up of film.
6 tracks found @ PL33.
CharmFlight length : 1330micron.Decay: in Lead (PL33-PL32 ) 340micron up of PL32.Kink angle : 209mrad.
Daughter Particle : muon (~2.2GeV)IP : 262micron.Decay Pt : ~ 460MeV/c
ax ay IP 1. 0.1325 0.0624 (PL33) 6.6 proton 2. 0.0097 -0.0663 (PL33) 4.5 3. 0.0876 0.6656 (PL33) 2.3 1ry mu 4. -0.0390 -0.1354 (PL33) 1.4 charm 5. 0.2215 0.4319 (PL33) 10.3 6. -0.0876 0.0418 (PL31) 18.9 e-pair 7. 0.0893 -0.0638 (PL33) 4.3
mu+
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A charm candidate (2)A charm candidate (2)
Flight length 3247.2 μmkink 0.204 radPdaughter 3.9 (+1.7 -0.9) GeVPT 796 MeV
4x10-4 % probability for a hadron re-interaction to have a PT > 600 MeV
side
face
pl50 pl51 pl52 pl53 pl54 pl 55 pl 56 pl57
Clear kink topology Two EM showers pointing to the vertex
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A Charm candidate (3)A Charm candidate (3)
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Summary
The goal of OPERA is to detect oscillation appearance.
OPERA developed Nuclear Emulsion Technology.
In 2008 Run, 1690 neutrino events were triggered in the target tracker.797 vertices were found in ECC bricks under microscope and the search is going on.
From the observation of charm candidates, the ability to detect kink or trident tau decay topologies is proven and its efficiency is being evaluated.
For the run of 2009 that started on June 1, we require 4.5E19 p.o.t. 4300 neutrino events should be collected in ECC targets. About 2.5 tau-neutrino interactions are expected to be detected.By 5 years, OPERA will get 10 events.
The OPERA detector suffered no damage following the L’Aquila earthquake.Great thanks to you for the huge support from all over the world!
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fin