1 NuFact’01 WG1 : Neutrino Oscillation Physics May 24-30, 2001 An appearance experiment to search...

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1 NuFact’01 WG1 : Neutrino Oscillation Physics May 24-30, 2001 An appearance experiment to search for - oscillations in the CNGS beam CNGS1 scillation Project with Emulsion-tRacking Apparat May 25, Nagoya University M. Komatsu

Transcript of 1 NuFact’01 WG1 : Neutrino Oscillation Physics May 24-30, 2001 An appearance experiment to search...

Page 1: 1 NuFact’01 WG1 : Neutrino Oscillation Physics May 24-30, 2001 An appearance experiment to search for  -  oscillations in the CNGS beam CNGS1 O scillation.

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NuFact’01

WG1 : Neutrino Oscillation PhysicsMay 24-30, 2001

An appearance experiment to search for - oscillations

in the CNGS beam CNGS1

Oscillation Project with Emulsion-tRacking Apparatus

May 25, Nagoya University M. Komatsu

Page 2: 1 NuFact’01 WG1 : Neutrino Oscillation Physics May 24-30, 2001 An appearance experiment to search for  -  oscillations in the CNGS beam CNGS1 O scillation.

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The experimental technique

• Emulsion Cloud Chamber (ECC)– Emulsions for tracking, passive material as target– Basic technique works

• charmed “X-particle” first observed in cosmic rays (1971)• DONUT/FNAL beam-dump experiment: events observed

• m2 = (1.5 - 5) x10-3 eV2 ( SuperK) Mtarget ~ 2 kton of ECC

– large detector sensitivity, complexity– modular structure (“bricks”): basic performance is preserved

• Ongoing developments in the emulsion technique, required by the large vertex detector mass:

– industrially produced emulsion films– automatic scanning microscopes with ultra high-speed

Pb

Emulsion layers

1 mm

Experience with emulsions and/or searches : E531, CHORUS, NOMAD and DONUT

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~ 10 m

The detector at Gran Sasso(modular structure, configuration with three “supermodules”)

spectrometerMagnetised Iron Dipoles

Drift tubes and RPCs

target and decay detectorEach “supermodule” is

a sequence of 24 “modules” consisting of - a “wall” of Pb/emulsion “bricks”- planes of orthogonal scintillator strips

scintillator strips

brick wall

module

brick(56 Pb/Em. “cells”)

8 cm (10X0)

supermodule

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8 m

Target Trackers

Pb/Em. target

Electronic detectors select interaction brick

A “hybrid” experiment

Emulsion scanning vertex search

Extract selected brick  

Pb/Em. brick

8 cmPb 1 mm

Basic “cell”

Emulsion

decay search

spectrometer

e/ ID, kinematics ID, charge and p

(DONUT)

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Origami packed ECC brick for OPERA

Origami packing = vacuum packing (1) Protection against light and humidity variations. (2) Keep the position between films and Pb plates. (3) Vacuum preserved over 10 years

10X0 ( 56 emulsion films ) 8kg for each brick

12.5cm

235k bricks for 3 supermodules

Similar packing was usedfor E531,CHORUS,etc. DONUT did not use thispacking then we had trouble.

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Structure: OPERA ECC = DONUT ECC Material : Lead Iron

Better performance for physics analysis

has been detected in the DONUT

ECC hadron

Emulsion Cloud Chamber for detection

1mmFe plate

Emulsion film

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The First detection in ECC • Iron-Emulsion ECC target

– 50cm x 50cm x 7cm(47 Iron plate : 2.7X0)– Topology, momentum and e-ID in ECC

• Beam– 3.5x1017 POT , Apr.-Sep. ‘97– Approximately 1,100 three flavor neutrino interactions – 785 events in target region.

• Data taking– 337 events located and 289 decay search done.– We are waiting faster scanning system for high multipli

city at TT events. • Tau and charm events

– 6 tau events– 2 charged and 2 neutral charms

Page 8: 1 NuFact’01 WG1 : Neutrino Oscillation Physics May 24-30, 2001 An appearance experiment to search for  -  oscillations in the CNGS beam CNGS1 O scillation.

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6th tau event in DONUT ECC

cGeV

cGeV

cGeV

/208.09.18

/401.034.3

/132.077.7

7.2079.6

16.171.0

62.396.1

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Momentum measurement

in DONUT ECC

Momentum measurementby multiple scattering

Consistent result withmomentum measuredby spectrometer.

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• Developed in DONUT analysis– 3D tracking in emulsion using fast automatic scanning

system(UTS)– Reconstruct all tracks recorded in emulsion

• Application in CHORUS “Phase II”– 1.5mm x 1.5mm x 6.3mm(8 plates)– Tau search(0 events) and charm physics– Offline event reconstruction and event selection

• Data taking– 13,000 events/month (440 events/day)– Data taking finished for 107,590 events.

NETSCAN in CHORUS Phase II

We have started our phase II analysis with the aim of reaching our design sensitivity of P= 10-4

Page 11: 1 NuFact’01 WG1 : Neutrino Oscillation Physics May 24-30, 2001 An appearance experiment to search for  -  oscillations in the CNGS beam CNGS1 O scillation.

11Nov. ‘99

CHORUS Phase II data taking

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Netscan (Chorus phase II)

1.5 mm

1.5 mm

All track segments(6k hits)

8 plates overlappe

d

6.3 mm

Yellow : UpstreamRed : Downstream

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1.5 mm

1.5 mm

Small impact

parameter

Netscan (Chorus phase II) Yellow : Upstream

Red : Downstream

CC D0

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Charm search in CHORUS

NETSCAN • 108k Data sets are ready for analysis• Offline charm selection

– 23,244 CC events done– ~900 events selected (~4%)– 568+ charms (manual confirm is going on)

• ~70% purity for charm• ~15% hadronic re-interactions, electron pairs and other int.• The other ~15% are junk.

• Preliminary charm detection efficiency– Selection require TT track reconstruction

• Reconstruction efficiency for hadron tracks are 47-64%– 26,63,58 and 75% for 1,2,3 and 4 prong decays

• Lower efficiency for D+ and c+ due to long and short life tim

e.

Preliminary

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• Emulsion readout system– ‘94 : We decided to apply full automatic

scanning for CHORUS analysis.• Emulsion became “Tracking detector”.

– ‘96 : ECC for DONUT target• Pure tracking device

– ‘98 : Establish “NETSCAN”• Current readout system “UTS” make us possible to

perform volume scanning.

• These changes were driven by faster emulsion readout system.

• OPERA needs x20 faster readout system

The key technology for OPERA

Page 16: 1 NuFact’01 WG1 : Neutrino Oscillation Physics May 24-30, 2001 An appearance experiment to search for  -  oscillations in the CNGS beam CNGS1 O scillation.

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S-UTS Scanning speed: 20cm2/h 20 faster than the current system (UTS)

S-UTS

‘94 ‘96 ‘98 ‘01 NTS UTS S-UTS

Will be realized by Fast CCD camera (3 k frames/sec) Continuous movement of the X-Y stage Z movement controlled by piezo actuator

late summer 2001 first S-UTS

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Emulsion Scanning Lab in Nagoya

Upgraded for OPERA

CHORUS, DONUT,OPERA and R&D for next generation

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Interactions with 1.8 kton target x 5 years

~ 32000 NC+CC

~ 240 CC

for SuperK best fit : sin2 2 = 1 m2 = 3.2x10-3 eV2

The CNGS beam

Shared SPS operation 200 days/year 4.5x1019 pot / year

Nominal beam

( m-2 / pot) 7.45x10-9

CC / pot / kton 5.44x10-17

< E > ( GeV ) 17

(e + e) / 0.85 %

/ 2.0 %

prompt negligible

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AnalysisstepsBrick finding

Trigger

Vertex location

Decay search“long” or “short”

decays

decay mode

Kinematics

events

Classifyas / e

yes

no

Electronic detectors

Emulsions

Emulsions

Electronic detectors

eat 1ry vtx ? CHORUS

DONUT

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Summary of detection efficiencies(in % and including BR)

Decay mode DIS long QE long DIS short Overall*

e 3.0 2.6 1.3 3.7 2.7 2.8 - 2.7 h 2.2 2.8 - 2.3Total 8.0 8.3 1.3 8.7

* weighted sum of DIS and QE events

Channels considered in the Progress Report:

e (DIS+QE, long) (DIS+QE, long) Overall efficiency

Page 21: 1 NuFact’01 WG1 : Neutrino Oscillation Physics May 24-30, 2001 An appearance experiment to search for  -  oscillations in the CNGS beam CNGS1 O scillation.

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Expected background events (5 years data taking)

e h Total

Charm production 0.15 0.03 0.15 0.33e CC and 0 0.01 - - 0.01Large scattering - 0.10 - 0.10Hadron reinteractionswith kink topology

- - 0.10 0.10

SubTotal 0.16 0.13 0.25 0.54

Charm production 0.03 - - 0.03e CC and 0 «0.01 - - «0.01

SubTotal 0.03 - - 0.03

Total 0.19 0.13 0.25 0.57

Lo

ng

dec

ays

Sh

ort

de

cays

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m2 = 1.2x10-3 eV2

at full mixing

sin2 (2) = 6.0x10-3

at large m2

(average 90 % CL upper limit for a large number of exp.ts in the absence of a signal)

5 years

3 years

Sensitivity

5 years data taking

Page 23: 1 NuFact’01 WG1 : Neutrino Oscillation Physics May 24-30, 2001 An appearance experiment to search for  -  oscillations in the CNGS beam CNGS1 O scillation.

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• Full mixing

• 5 years with shared SPS operation

(2.25x1020 pot)

• Average target mass = 1.8 kton

(accounting for mass reduction with time, due to brick removal for analysis)

Expected events

events

decay m2 (10-3 eV2 ) b.g.1.5 3.2 5.0

e 1.7 7.7 18.5 0.19

1.3 5.7 13.8 0.13

h 1.1 4.9 11.8 0.25

Total 4.1 18.3 44.1 0.57

m2 (eV2)

eve

nts

e

xpe

cte

d in

5 y

ea

rs

(log

scal

e)

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Summary and conclusionsfor OPERA

• Experience with E531, CHORUS, NOMAD and DONUT

• OPERA : appearance and appearance and mm2 2 measurement at CNGSmeasurement at CNGS

• Basic technique (ECC) works; preserved by modularity Basic technique (ECC) works; preserved by modularity

• Large detector sensitivity, complexity

•Ongoing developments in the emulsion technique:– industrially produced emulsion films– automatic scanning microscopes with ultra high-speed

• The sensitivity covers the SuperK range; very low b.g.

• Start data taking in 2005

Page 25: 1 NuFact’01 WG1 : Neutrino Oscillation Physics May 24-30, 2001 An appearance experiment to search for  -  oscillations in the CNGS beam CNGS1 O scillation.

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Future Emulsion experimentfor neutrino factory

• ECC + fast readout system– It is possible to construct very massive detector.

ECC performance preserved by modularity for large detector.

– Using magnetic field: ID• Emulsion works even in strong magnetic field.

tee and ,,,,

ECC is ready for neutrino factory

Page 26: 1 NuFact’01 WG1 : Neutrino Oscillation Physics May 24-30, 2001 An appearance experiment to search for  -  oscillations in the CNGS beam CNGS1 O scillation.

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Industrially mass-produced emulsion film

Surface protection by gelatin layerfor Pb plate contact

Products by Fuji Film Co. Suitable for mass production: < 2 years for production for OPERA (13.6M films)Precise mechanical size : emulsion layer thickness (~ 1 m accuracy)

50m emulsion layer

200m base

50m emulsion layers

200m base

Page 27: 1 NuFact’01 WG1 : Neutrino Oscillation Physics May 24-30, 2001 An appearance experiment to search for  -  oscillations in the CNGS beam CNGS1 O scillation.

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Cross sectional view of an emulsion layer

30grains/100mgrain diameter ~ 0.6m

Ag grain after development

dx

= 0.06mCompton Electron

Fog

M.I.P. Track

100m

M.I.P. Track

intrinsic tracking accuracy

Intrinsic tracking resolution of the emulsion

Page 28: 1 NuFact’01 WG1 : Neutrino Oscillation Physics May 24-30, 2001 An appearance experiment to search for  -  oscillations in the CNGS beam CNGS1 O scillation.

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Electron identification in ECC brick

2h

2e

Shower detected

TEST experiment at CERN PS

Electron

Had

ron

(1) Different energy loss by multiple scattering E(x)=E0e (-x/X0) for electrons 2

e

E(x)=E0(1-(dE/dx)x) for hadrons 2h

(2) Detection of electromagnetic shower Requires low background track density controlled fading Sensitive to electrons close to the Pb critical energy

5X0

1 mm

5 cm

Page 29: 1 NuFact’01 WG1 : Neutrino Oscillation Physics May 24-30, 2001 An appearance experiment to search for  -  oscillations in the CNGS beam CNGS1 O scillation.

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detection and energy measurement in ECC brick

Improvement for missing PT analysis h decay mode

charged particle + 0 ( )

M = 157 24 MeV/c2

Test experiment at CERN PS

8 GeV/c - interaction in OPERA type ECC

Example of detection in DONUT( Fe not suited for energy measurement)

-

s from 0