search for oscillations: status of the opera experiment

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ICHEP 2012, Melbourne, 5 July 2012 SEARCH FOR OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT Marilisa De Serio Università degli Studi di Bari & INFN On behalf of the OPERA Collaboration

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SEARCH FOR      OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT. Marilisa De Serio Università degli Studi di Bari & INFN On behalf of the OPERA Collaboration. SEARCH FOR      OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT. The OPERA experiment: Physics goal - PowerPoint PPT Presentation

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Page 1: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

ICHEP 2012, Melbourne, 5 July 2012

SEARCH FOR OSCILLATIONS:

STATUS OF THE OPERA EXPERIMENT

Marilisa De Serio Università degli Studi di Bari & INFN On behalf of the OPERA Collaboration

Page 2: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 2

The OPERA experiment:

Physics goal detection principle Detector Status of data-taking and analysis

oscillation results

Preliminary results on e oscillation search

SEARCH FOR OSCILLATIONS:

STATUS OF THE OPERA EXPERIMENT

Page 3: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 3

Hall C Laboratori Nazionali Gran Sasso

OPERA: Oscillation Project with Emulsion tRacking Apparatus

L = 732 kmCERNLNGS

Long baseline neutrino oscillation experimentLong baseline neutrino oscillation experiment

Aim: Direct detection of Aim: Direct detection of oscillations in appearance mode oscillations in appearance mode

covering the whole interesting region of the parameter space covering the whole interesting region of the parameter space

indicated by atmospheric neutrino dataindicated by atmospheric neutrino data

CNGS (CERN Neutrinos to Gran Sasso)CNGS (CERN Neutrinos to Gran Sasso) beam beam

optimised for optimised for appearanceappearance

Page 4: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 4

CNGS beam

Gran Sasso National Laboratory

INFN - LNGSL’Aquila (Italy), 120 km from Rome

1400 m rock shield (cosmic flux reduction ~ 10-6)

Largest underground laboratory for astro-particle physics

Conventional beam

Nominal intensity: 22.5 x 1019 p.o.t. Expected events: 7.6 signal, 0.8 background[New Journal of Physics 14 (2012) 033017]

Page 5: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 5

detection principle

Event-by-event separation of Event-by-event separation of CC interactions CC interactions

from dominant from dominant interactions by direct observation interactions by direct observation

of of lepton decay lepton decay

Requirements:Requirements:

Large target mass to compensate for Large target mass to compensate for smallsmall neutrino neutrino

interaction cross-sectioninteraction cross-section

Micrometric resolution to observe Micrometric resolution to observe decay decay kinkkink

Nuclear emulsionsNuclear emulsionsTarget segmented into basic units called bricks.

Brick: sandwich of 57 emulsion films interleaved with 1mm-thick lead plates

Total target mass 1.25 kt (about 150000 bricks)

10 cm

12.5 cm

decay channel

B.R. (%)

17.7

e 17.8

h 49.5

3h 15.0

Page 6: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 6

detection principle

Event-by-event separation of Event-by-event separation of CC CC interactions interactions

from dominant from dominant interactions by direct interactions by direct observation observation

of of lepton decay lepton decayRequirements:Requirements:

Large target mass to compensate for Large target mass to compensate for smallsmall neutrino neutrino

interaction cross-sectioninteraction cross-section

Micrometric resolution to observe Micrometric resolution to observe decay decay kinkkink

Nuclear emulsionsNuclear emulsions

High muon identification efficiency to reduce High muon identification efficiency to reduce

charm background; event region pre-selection charm background; event region pre-selection

Electronic detectorsElectronic detectors

Target segmented into basic units called bricks. Brick: sandwich of 57 emulsion films

interleaved with 1mm-thick lead plates

Total target mass 1.25 kt (about 150000 bricks)

10 cm

12.5 cm

decay channel

B.R. (%)

17.7

e 17.8

h 49.5

3h 15.0

Page 7: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 7

OPERA detector

First candidate

10 mm

25 mradTT – brick connection

Changeable Sheets (CS): pair of emulsion films

acting as TT – brick interface

Page 8: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 8

OPERA detector

Each brick is a stand-alone detector Each brick is a stand-alone detector

with sub-micrometric resolution.with sub-micrometric resolution.

(Mean 104.3 m)events (MC) NC+CC events (MC)NC+CC events (Data)

(Mean 2.3 m)

• Momentum measurement by multiple Coulomb scatteringMomentum measurement by multiple Coulomb scattering

• E.m. shower detection and energy measurementE.m. shower detection and energy measurement

• Detection of highly-ionizing nuclear fragments produced Detection of highly-ionizing nuclear fragments produced

in hadronic interactions in hadronic interactions (discrimination between interactions and decays)(discrimination between interactions and decays)

Page 9: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 9

Run Protons on target

SPSefficienc

y

In-target events

2008 1.78x101

9

61% 1698

2009 3.52x101

9

70% 3557

2010 4.04x101

9 81% 3912

2011 4.84x101

9 78% 4210

Status of the experiment

Run 2012 in progress.Foreseen integrated intensity

at the end of the run: 18.9 x 1019 p.o.t.

( 84% of nominal intensity)

compatible with the expectations for the analysed sample

Located neutrino interactions

4611

Fully analysed events 4126

candidate events 2

Page 10: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 10

Decay vertex: - h 0

First candidate

First direct detection of oscillations in appearance mode

VARIABLE AVERAGE Selection criteria

kink (mrad) 41 ± 2 >20

decay length (m)

1335 ± 35within 2 lead

plates

P daughter (GeV/c)

12 +6-3 >2

Pt (MeV/c) 470 +230-120 >300 ( attached)

missing Pt (MeV/c)

570 +320-170 <1000

(deg) 173 ± 2 >90

oscillation search

Page 11: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 11

2000 m

New candidate

oscillation search

2-prong interaction with one track showing a secondary vertex

compatible with the hypothesis of - h+ h- h-

Page 12: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 12

New candidate

Event kinematics

No muon detected at the primary vertex:

track other than lepton candidate not compatible with muon hypothesis

based on momentum – range correlation

oscillation search

Page 13: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 13

Satisfying the specified criteria for 3hadron decay

candidatecut

New candidate oscillation

search

Page 14: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 14

oscillation search:

summary

Run StatusNumber of analysed events

Expected τ events

(Preliminary)

Observedτ

candidate events

Expected BG

(Preliminary)

2008 - 2009 Finished 2783 1

2010 - 2011Analysis

in progress1343 1

2012 Started

Total 4126 2.1 2 0.2

PreliminaryPreliminary

Page 15: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 15

Control sample for detection efficiency:

charm production and decay(flight length and decay topologies

similar to those of the lepton)

Charmed hadron – muon angle in the plane transverse

to direction

Expected events: 51 7.5Observed events: 49

oscillation search:

control sample

Page 16: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 16

e oscillation search

Systematic search for electron neutrinos applied to 505 events without muon in the final state

(runs 2008 – 2009)

Expected events: 19.2 (beam) + 1.5 (oscillated)Observed events: 19

E = 15.6 GeV

Page 17: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 17

e oscillation search

Systematic search for electron neutrinos applied to 505 events without muon in the final state

(runs 2008 – 2009)

Expected events: 19.2 (beam) + 1.5 (oscillated)Observed events: 19

E < 20 GeV (improve S/N ratio)

Expected events: 3.7 (beam) + 1.1 (oscillated)Observed events: 4

E = 15.6 GeV

PreliminaryPreliminary

m23=2.45E-3Sin223=0.51

E < 20 GeV

Page 18: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 18

Conclusions and Outlooks

OPERA is successfully collecting data since 2008. OPERA is successfully collecting data since 2008.

We expect to reach We expect to reach 18.9 x 1018.9 x 101919 integrated p.o.t. integrated p.o.t. by the end of 2012 run, by the end of 2012 run,

corresponding to corresponding to 84% of the nominal intensity. 84% of the nominal intensity.

oscillation search: oscillation search:

2 2 candidate events observed so far candidate events observed so far

(expected: 2 signal, 0.2 BG – (expected: 2 signal, 0.2 BG – preliminarypreliminary - ) - )

A few more events are under study.A few more events are under study.

ee oscillation search: oscillation search:

19 19 ee events observed in 2008 – 2009 statistics, events observed in 2008 – 2009 statistics,

4 with E4 with E < 20 GeV (expected: 1.1 oscillated, 3.7 BG). < 20 GeV (expected: 1.1 oscillated, 3.7 BG).

Statistics will be improved by a factor of Statistics will be improved by a factor of 3 3

set constraints in the high set constraints in the high mm22 region region

Page 19: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

Thank you!

Page 20: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 20

Control sample: charm events(flight length and decay topologies similar to those of the )

oscillation analysis 2008-2009

2738 located and fully analysed events ( 4.8 x 1019 p.o.t.)

1 candidate observed in the h channel

Expected: 0.49±0.12 signal events, 0.05±0.01 background events

Expected (all decay channels): 1.65±0.41 signal events,

0.16±0.03 background events

New Journal of Physics 14 (2012) 033017

Page 21: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 21

Hadronic tracks produced in interactions showing kink topology:

14 m of tracks scanned No events in the signal region 10 events in reference region (Pt 200 600 MeV/c), 10.8 expected

90% C.L. upper limit of 1.0 x 10-3 kinks/NC event

oscillation analysis 2008-2009

Signal region

Reference region

4 GeV/c pion interactions in test beam bricks:

190 m of tracks scanned 534 interactions found 214 kinks detected No events in the signal region

Hadronic interaction background

Page 22: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 22

Background reduction: black track search

Highly ionizing nuclear fragments produced in hadronic interactions

oscillation analysis 2008-2009

Background reduction: track follow-down

Tracks produced in potentially interesting interactions are followed in downstream bricks

to detect secondary interactions and/or apply momentum-range consistency checks:

Misidentified muons from charm events:5% 3.3%

Factor 100 BG reduction in µ channel due to muon mismatch

in CC and NC interactions

Page 23: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 23

oscillation search: study of hadronic interactionsComparison between data and MC (Fluka)

Page 24: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 24

• Event sample : ー 505 NC-like events (runs 2008 and 2009)

• For each event:

– Extrapolate 1ry tracks to CS

– For each track, search for shower signal in CS

– If shower-like tracks are found, measure additional volume

around 1ry track.

• Results: – 96 events selected– 19 e interactions confirmed

e oscillation search

Page 25: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 25

e oscillation search

A close-up of an electron pair

as seen in emulsion

1micron

Gamma-ray

Background events

Low-energy electrons produced in gamma conversion are difficult to recognise in emulsion

Background source

Estimated background in 2008-2009 sample:

0.16 events

Page 26: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 26

Performance of the Electronic detectors

New Journal of Physics 13 (2011) 053051

Muon identification efficiency ~ 95%(track length × density > 660 g cm-2)

Muon momentum reconstruction

Deposited energy in the TT – CC events

m.i.p. 5 photo-electrons (2.15 MeV)

Page 27: SEARCH FOR          OSCILLATIONS: STATUS OF THE OPERA EXPERIMENT

M. De Serio ICHEP 2012, Melbourne, 5 July 2012 27