The OPERA Experiment

Similar documents
A. Chukanov On behalf of OPERA collaboration JINR, Dubna TAUP 2011, Munich, 5-9 september, 2011

Latest Results from the OPERA Experiment (and new Charge Reconstruction)

OPERA physics programme, experimental concept, first results with beam and cosmic, short term prospects.

RECENT RESULTS FROM THE OPERA EXPERIMENT

arxiv: v1 [hep-ex] 1 Oct 2015

PoS(HEP2005)177. Status of the OPERA experiment. Francesco Di Capua. Universita Federico II and INFN.

Results from the OPERA experiment in the CNGS beam

Results from the OPERA experiment in the CNGS beam

OPERA. physics motivation - CNGS OPERA detector ν τ appearance physics program R. Zimmermann Dortmund, April

Updated results of the OPERA long baseline neutrino experiment


NEUTRINOS FROM CERN TO GRAN SASSO: THE CNGS PROJECT

arxiv: v1 [hep-ex] 11 May 2013

The CERN-Gran Sasso Neutrino Program

Search for nu tau appearance via neutrino oscillations in the nu mu CNGS beam with the OPERA experiment

Latest results of OPERA

Measurement of the neutrino velocity with the OPERA detector in the CNGS beam

Tau-neutrino production study in 400 GeV proton interactions

Long Baseline Neutrino Oscillation Experiments

FIRST NEUTRINO EVENTS IN THE OPERA EMULSION TARGET

Tau-neutrino production study at CERN SPS: Novel approach by the DsTau experiment

in collaboration with LNF-SEA: U. Denni, G. Papalino LNF-SPAS: A. Cecchetti

Detecting ν τ s: the CHORUS and OPERA experience. Pasquale Migliozzi

CNGS experimental program: OPERA and ICARUS

Results from the OPERA experiment at the CNGS beam

Measurement of the neutrino velocity with the OPERA detector in the CNGS beam

Measurement of the neutrino velocity with the OPERA detector in the CNGS beam

Measurement of the neutrino velocity with the OPERA detector in the CNGS beam

First results and status of the OPERA experiment

Neutrino physics with the SHiP experiment at CERN

Status of the OPERA experiment

Study of ν τ production by measuring D s τ events in 400 GeV proton interactions: Test of lepton universality in neutrino charged-current interactions

The OPERA Neutrino Velocity Measurement. Presented by Björn Wonsak

The CNGS project. Pasquale Migliozzi INFN - Napoli

The CNGS neutrino beam

arxiv: v1 [hep-ex] 17 Feb 2014 SEARCH FOR NEUTRINO OSCILLATIONS IN APPEARANCE MODE WITH THE OPERA EXPERIMENT

Experimental results on the atmospheric muon charge ratio

Recent T2K results on CP violation in the lepton sector

OPERA results on neutrino oscillations, cosmic rays and neutrino velocity. G. Rosa Rome, Oct. 11th 2011 Dept. Of Physics Sapienza University

ICARUS T600 experiment: latest results and perspectives

Measurement of the neutrino velocity with the OPERA detector in the CNGS beam

Accelerator Neutrino Experiments News from Neutrino 2010 Athens

- ICARUS status and near future

CNGS beam monitor with LVD

NINJAExperiment: NINJA. Tsutomu Fukuda(IAR, Nagoya University) on behalf of NINJA collaboration

The SHiP experiment. Colloquia: IFAE A. Paoloni( ) on behalf of the SHiP Collaboration. 1. Introduction

Perspectives of neutrino oscillation physics with long baseline beams

The atmospheric muon charge ratio: a probe to constrain the atmospheric ν µ / ν µ ratio

Neutrino Oscillations

PoS(Nufact08)003. Status and Prospects of Long Baseline ν Oscillation Experiments

Long Baseline Neutrinos

The SHiP experiment and its detector for neutrino physics

Neutrino Oscillations

K2K and T2K experiments

Long Baseline Neutrino Experiments

New Results for ν µ ν e oscillations in MINOS

Measurement of q 13 in Neutrino Oscillation Experiments. Stefan Roth, RWTH Aachen Seminar, DESY, 21 st /22 nd January 2014

arxiv:hep-ph/ v1 16 May 2003

New Results from the MINOS Experiment

PHYS 5326 Lecture #2. Wednesday, Jan. 24, 2007 Dr. Jae Yu. Wednesday, Jan. 24, 2007 PHYS 5326, Spring 2007 Jae Yu

Observation of tau neutrino interactions

Particle Detectors. Summer Student Lectures 2007 Werner Riegler, CERN, History of Instrumentation History of Particle Physics

Application of GLoBES: GLACIER on conventional neutrino beams

MINOS. Luke A. Corwin, for MINOS Collaboration Indiana University XIV International Workshop On Neutrino Telescopes 2011 March 15

T2K and the MAINZ Photon Beam

NEUTRINO INTERACTION ANALYSIS WITH AN AUTOMATIC SCANNING SYSTEM IN THE OPERA EXPERIMENT

Long Baseline Neutrino Oscillation Experiments

Results from HARP. Malcolm Ellis On behalf of the HARP collaboration DPF Meeting Riverside, August 2004

Results from T2K. Alex Finch Lancaster University ND280 T2K

Performance of the ICARUS T600 detector

Reconstruction of. events in LHCb. Benjamin Carron

First neutrino beam and cosmic tracks. GDR neutrino

Neutrino Experiments: Lecture 2 M. Shaevitz Columbia University

arxiv: v1 [hep-ex] 11 May 2017

Muon commissioning and Exclusive B production at CMS with the first LHC data

Electroweak Physics at the Tevatron

MINOS. Physics Program and Construction Status. Karol Lang The University of Texas at Austin. YITP: Neutrinos and Implications for Physics Beyond

PoS(NEUTEL2015)037. The NOvA Experiment. G. Pawloski University of Minnesota Minneapolis, Minnesota 55455, USA

Neutrinos & the MINOS Experiment

Chart of Elementary Particles

Search for heavy neutrinos in kaon decays

Study of the charged current interactions of the CNGS neutrino beam in the OPERA detector target

PoS(NOW2016)003. T2K oscillation results. Lorenzo Magaletti. INFN Sezione di Bari

Neutrino mixing II. Can ν e ν µ ν τ? If this happens:

PoS(DIS 2010)190. Diboson production at CMS

SHiP: a new facility with a dedicated detector for neutrino physics

AN EXPERIMENTAL OVERVIEW OF NEUTRINO PHYSICS. Kate Scholberg, Duke University TASI 2008, Boulder, CO

Detector Basics III. Mark Messier Indiana University. Neutrino Summer School Fermilab July 9, 2008

Why understanding neutrino interactions is important for oscillation physics

A method for detecting ν τ appearance in the spectra of quasielastic CC events

SciBar and future K2K physics. F.Sánchez Universitat Aútonoma de Barcelona Institut de Física d'altes Energies

NEW νe Appearance Results from the. T2K Experiment. Matthew Malek Imperial College London. University of Birmingham HEP Seminar 13 June 2012

Recent Results from T2K and Future Prospects

Detectors for astroparticle physics

From Here to a Neutrino Factory: Neutrino Oscillations Now and Again

Reconstruction and identification of hadronic τ decays with ATLAS

Correlated Background measurement in Double Chooz experiment

NA62: Ultra-Rare Kaon Decays

Università degli Studi di Napoli Federico II

A multipurpose detector for low energy

Transcription:

The OPERA Experiment Observation of a First ν τ Candidate Event in ν µ ν τ Appearance Search Group Report Annika Hollnagel University of Hamburg Institute for Experimental Physics DPG Frühjahrstagung 2011, Karlsruhe Universität Hamburg 1 01.04.2011 The OPERA Experiment

Overview 1 The OPERA Experiment 2 The First ν τ Candidate Event 3 Conclusion & Outlook Universität Hamburg 2 01.04.2011 The OPERA Experiment

The OPERA Experiment Universität Hamburg 3 01.04.2011 The OPERA Experiment

The OPERA Experiment OPERA: Oscillation Project with Emulsion Tracking Apperatus. Goal: Appearance search Direct observation of ν µ ν τ oscillations. Concept: High-intensity long-baseline ν µ-beam from CERN to LNGS. Detection of τ lepton production & decay. Requirements: µm-precision: τ lepton decay after 600 µm. Large target mass: Small ν interaction cross sections. Realisation: Hybrid detector Electronic detector parts (ED). Emulsion cloud chamber photo emulsions (ECC). Universität Hamburg 4 01.04.2011 The OPERA Experiment

τ Detection ν τ signal: ν τ CC interactions and τ lepton decay with kink topology: Background processes: ν µ CC reactions with charm production & undetected 1ry µ: Hadronic re-interactions in lead. Large-angle µ scattering. Universität Hamburg 5 01.04.2011 The OPERA Experiment

LNGS LNGS: Laboratori Nazionali del Gran Sasso. Location: Below Mt. Corno Grande of Gran Sasso, Italy. Baseline: 732 km away from the ν µ source at CERN. Vertical rock coverage: 1 300 m (3 400 m w.e.). Number of cosmic µ: 1 m 2 h 1. Universität Hamburg 6 01.04.2011 The OPERA Experiment

The CNGS Beam CNGS: CERN Neutrinos to Gran Sasso. E p 400 GeV p.o.t. 2008 1.78 10 19 p.o.t. 2009 3.52 10 19 p.o.t. 2010 4.04 10 19 p.o.t. 2011 expected 4.5 10 19 Nominal p.o.t./year 4.5 10 19 Total p.o.t. expected 22.5 10 19 E ν 17.9 GeV ν e/ν µ (CC) 0.89 % ν µ/ν µ (CC) 2.4 % ν e/ν µ (CC) 0.06 % ν τ /ν µ (CC) < 10 4 % Universität Hamburg 7 01.04.2011 The OPERA Experiment

The OPERA Hybrid Detector 2 identical Super Modules (SM), each consisting of: Target area. Magnetic spectrometer. Universität Hamburg 8 01.04.2011 The OPERA Experiment

Target Area Emulsion Cloud Chamber (ECC) bricks: Each brick: 57 2 photo emulsions on plastic bases ( 0.3 mm), 56 lead plates (1 mm). In total: 150 000 bricks of 8.3 kg lead each ( 1.28 kt target mass). Universität Hamburg 9 01.04.2011 The OPERA Experiment

Event Reconstruction ED reconstruction: Provision of time resolution. ν interaction vertex localisation. CC/NC separation. µ identfication & momentum measurement. Hadronic shower energy reconstruction. Universität Hamburg 10 01.04.2011 The OPERA Experiment

Event Reconstruction ECC event reconstruction: Reconstruction of 3D track segments. Rejection of passing-through and low-energy tracks. Vertex reconstruction. Decay search procedure. Universität Hamburg 11 01.04.2011 The OPERA Experiment

The First ν τ Candidate Event Universität Hamburg 12 01.04.2011 The OPERA Experiment

The First ν τ Candidate Event ED view: 22th of August 2009, 19:27h (UTC). Muonless event 9234119599. Universität Hamburg 13 01.04.2011 The OPERA Experiment

The First ν τ Candidate Event ED view: Probability of undetected large-angle µ scattering: 1% by track follow-down (5% nominal value expected at the time of the experiment proposal, assumed for this analysis). Universität Hamburg 14 01.04.2011 The OPERA Experiment

The First ν τ Candidate Event ECC reconstruction: Primary ν interaction: 7 tracks attached to 1ry vertex. Tracks 4, 8: Visible kink. Track 8: Attached to 2ry vertex, IP = (55 ± 4) µm w.r.t. 1ry vertex. Electromagnetic showers γ1, γ2: Attached to 2ry vertex. Universität Hamburg 15 01.04.2011 The OPERA Experiment

The First ν τ Candidate Event ECC reconstruction: Track No Particle type p [GeV] 1 hadron 0.78 +0.13 0.10 2 p 0.60 ± 0.05 3 hadron 1.97 +0.33 0.25 5 hadron 1.30 +0.22 0.16 6 pion 0.36 +0.18 0.09 7 from prompt neutral 0.49 +0.29 0.13 Universität Hamburg 16 01.04.2011 The OPERA Experiment

The First ν τ Candidate Event Kink angle: Selection criteria: θ kink > 20 mrad. ν τ candidate event: θ kink = (41 ± 2) mrad. Universität Hamburg 17 01.04.2011 The OPERA Experiment

The First ν τ Candidate Event Decay length: Selection criteria: Decay vertex has to be within 2 lead plates downstream of 1ry vertex. ν τ candidate event: decaylength = (1335 ± 35) µm ( 15cτ). Universität Hamburg 18 01.04.2011 The OPERA Experiment

The First ν τ Candidate Event Daughter momentum: Selection criteria: p daughter > 2 GeVc 1. ν τ candidate event: p daughter = (12 +6 3 ) GeVc 1. Universität Hamburg 19 01.04.2011 The OPERA Experiment

The First ν τ Candidate Event Daughter transverse momentum: Selection criteria: p t,daughter > 0.6 GeVc 1 if no γ attached, p t,daughter > 0.3 GeVc 1 if 1γ attached. Rejection of hadronic re-interactions. ν τ candidate event: p t,daughter = (0.47 +0.23 0.12 ) GeVc 1. Universität Hamburg 20 01.04.2011 The OPERA Experiment

The First ν τ Candidate Event Missing transverse momentum: Selection criteria: p t,miss < 1 GeVc 1. Rejection of NC interactions. ν τ candidate event: p t,miss = (0.57 +0.32 0.17 ) GeVc 1. Universität Hamburg 21 01.04.2011 The OPERA Experiment

The First ν τ Candidate Event Angle between parent track and hadronic shower axis: Selection criteria: φ > π/2. ν τ candidate event: φ = (3.01 ± 0.03) rad. Universität Hamburg 22 01.04.2011 The OPERA Experiment

The First ν τ Candidate Event Kinematical cuts: All kinematical cuts for the 1-prong hadronic τ decay channel with 1 γ attached are passed. Invariant mass of the decay products: Invariant mass of the γγ-system: (120 ± 20 ± 35) MeV. Consistent with π 0 mass (135 MeV). Invariant mass of the π γγ-system: (640 +125+100 80 90 ) MeV. Consistent with ρ (770) mass (775 MeV). (ρ (770) being created in 25% of τ decays: τ ρ (π π 0 )ν τ.) Universität Hamburg 23 01.04.2011 The OPERA Experiment

Significance of ν τ Observation Observation for 1088 decay-searched events: 1 event (1-prong hadronic τ decay channel). Background expectation (1-prong hadronic τ decay channel): Number of hadronic re-interaction events: 0.011. Number of charm events: 0.007. 0.018 ± 0.007 (syst.) events. 1.8 % probability that the observed event is a background event. 2.36 σ significance of ν τ observation in OPERA. Background expectation (all τ decay modes): Number of background events: 0.045 ± 0.020 (syst.). 4.5 % probability that the observed event is a background event. 2.01 σ significance of ν τ observation in OPERA. Universität Hamburg 24 01.04.2011 The OPERA Experiment

Significance of ν τ Observation Observation for 1088 decay-searched events: 1 event (1-prong hadronic τ decay channel). Assumptions: m 2 23 = 2.5 10 3 ev 2. sin 2 2θ 23 = 1. Signal expectation (1-prong hadronic τ decay channel): Number of ν τ CC events: 0.16 ± 0.04 (syst.). Signal expectation (all τ decay modes): Number of ν τ CC events: 0.54 ± 0.13 (syst.). Result (for sin 2 2θ 23 = 1): Exclusion of: m 2 23 > 7.5 10 3 ev 2 at 90% CL. Universität Hamburg 25 01.04.2011 The OPERA Experiment

Event Statistics Analysis status: Vertex located: 3 108 events. Decay search performed: 2 614 events. Universität Hamburg 26 01.04.2011 The OPERA Experiment

Conclusion & Outlook Universität Hamburg 27 01.04.2011 The OPERA Experiment

Conclusion & Outlook Conclusion: Observation of a first ν τ candidate event in ν µ ν τ oscillations (22th of August 2009). Paper published in Physics Letters B: Observation of a first ν τ candidate event in the OPERA experiment in the CNGS beam, Agafonova et al. / Physics Letters B 691 (2010) 138 145. Outlook: New ν µ ν τ paper with full statistics of 2008 & 2009 data soon to be published. Data taking foreseen for 2011 & 2012 (LHC closed for maintenance and upgrade in 2013). Universität Hamburg 28 01.04.2011 The OPERA Experiment

Thank you for your attention! Universität Hamburg 29 01.04.2011 The OPERA Experiment

The OPERA Collaboration Belgium: IIHE-ULB Brussels Croatia: IRB Zagreb France: LAPP Annecy IPNL Lyon IPHC Strasbourg Germany: Uni Hamburg Israel: Technion Haifa Italy: Bari Bologna LNF Frascati LNGS l Aquila Naples Padova Rome Salerno Japan: Aichi Toho Kobe Nagoya Utsunomiya Korea: Jinju Russia: INR RAS Moscow LPI RAS Moscow ITEP Moscow SINP MSU Moscow JINR Dubna Switzerland: Bern ETH Zurich Tunisia: CNSTN Tunis Turkey: METU Ankara Universität Hamburg 30 01.04.2011 The OPERA Experiment

Backup Slides Universität Hamburg 31 01.04.2011 The OPERA Experiment

3-Flavour Oscillation Formalism Neutrino mixing of mass and flavour eigenstates: ) ) ) ( νe ν µ ν τ = ( Ue1 U e2 U e3 U µ1 U µ2 U µ3 U τ1 U τ2 U τ3 U ( ν1 Pontecorvo-Maki-Nakagawa-Sakata (PMNS) matrix: ( 1 ) ( ) ( ) ( ) 0 0 c13 0 s 13 e iδ c12 s 12 0 e iɛ 1 /2 0 0 U = 0 c 23 s 23 0 1 0 s 12 c 12 0 0 e iɛ 2/2 0 0 s 23 c 23 s 13 e iδ 0 c 13 0 0 1 0 0 1 Atmospheric terms Unknown terms Solar terms Majorana terms SuperKamiokande DoubleChooz, T2K KamLAND MINOS, OPERA with s ij = sin θ ij and c ij = cos θ ij. ν 2 ν 3 Universität Hamburg 32 01.04.2011 The OPERA Experiment

Oscillation Parameters OPERA physics reach: Black dot: sin 2 2θ 23 = 1. m23 2 = 2.4 10 3 ev 2. Grey band: OPERA allowed region (90 % CL). 22.5 10 19 p.o.t.. Oscillation parameters - present situation: matm 2 = m2 3 m2 2 2 10 3 ev 2 msol 2 = m2 2 m2 1 8 10 5 ev 2 θ 23 45 θ 12 33 θ 13 < 13 δ? Universität Hamburg 33 01.04.2011 The OPERA Experiment

τ Detection τ creation in ν τ CC reactions: ν τ + N τ + X τ decay modes (1-prong): Muonic: τ µ + ν τ + ν µ (BR 17.4 %) Electronic: τ e + ν τ + ν e (BR 17.9 %) Hadronic: τ h + ν τ + X 0 (BR 49.2 %) τ decay modes (3-prong): Hadronic: τ 2h + h + + ν τ + X 0 (BR 15.0 %) τ decay length: 600 µm. Universität Hamburg 34 01.04.2011 The OPERA Experiment

Beam Characteristics at LNGS Oscillation probability: P(ν µ ν τ ) sin 2 2θ 23 cos 4 θ 13 sin 2 ( m23 2 L 4E ) ν µ-beam energy: Optimsed for τ detection. Universität Hamburg 35 01.04.2011 The OPERA Experiment

Beam Characteristics at LNGS Oscillation probability: P(ν µ ν τ ) sin 2 2θ 23 cos 4 θ 13 sin 2 ( m23 2 L 4E ) Location: OPERA detector is at off-peak position. Longer baseline: Increase in ν τ flux would be cancelled by greater ν µ beam divergence. Universität Hamburg 36 01.04.2011 The OPERA Experiment

The OPERA Hybrid Detector VETO system: 2 planes of glass resistive plate chambers in front of the detector. Rejection of upstream ν interactions. Universität Hamburg 37 01.04.2011 The OPERA Experiment

The OPERA Hybrid Detector Brick Manipulator System (BMS): Brick extraction: Via 2 automatic robots (1 per semi-wall), parallel to CNGS data taking. Extraction speed: 25 ν interaction-bricks per 8 h-shift. Universität Hamburg 38 01.04.2011 The OPERA Experiment

Magnetic Spectrometer Magnetic spectrometer: Each SM: Downstream of the target area. Dipole Magnets. Resistive Plate Chambers (RPC & XPC). High Precision Trackers (HPT). Universität Hamburg 39 01.04.2011 The OPERA Experiment

Magnetic Spectrometer Dipole magnets: Each SM: Copper coils with 24 iron slabs. Magnetic field: 1.53 T. Deflection of charged particles. Universität Hamburg 40 01.04.2011 The OPERA Experiment

Magnetic Spectrometer Resistive Plate Chambers (RPC & XPC): Each SM: 24 planes of RPC within the magnet, horizontally and vertically aligned (RPC), 2 extra planes upstream of the magnet, tilted by 42.6 (XPC). Bakelite resistive plate chambers. Hadronic energy reconstruction. µ identification: By range measurement. Universität Hamburg 41 01.04.2011 The OPERA Experiment

Magnetic Spectrometer High Precision Trackers (HPT): Each SM: 6 walls of vertical drift tubes. Spacial resolution: 250 µm. Resolution: 20 % for p < 30 GeV. Precise measurement of the angular deflection of charged particles. Universität Hamburg 42 01.04.2011 The OPERA Experiment

Target Area Target area: Target Trackers (TT). Emulsion Cloud Chamber (ECC) bricks. Universität Hamburg 43 01.04.2011 The OPERA Experiment

Target Area Target Trackers (TT): Each SM: 31 walls of plastic scintillator strips, horizontally and vertically aligned. Position accuracy: 8 mm. Angular accuracy: 20 mrad. Brick finding efficiency: 80 %. Universität Hamburg 44 01.04.2011 The OPERA Experiment

Target Area Changeable Sheets (CS): Each brick: 2 extra emulsion sheets on the downstream side. Second check whether the ν interaction occurred inside the brick. Universität Hamburg 45 01.04.2011 The OPERA Experiment

Target Area ECC photo emulsions: Basic detector elements: AgBr crystals of 0.2 µm size. Intrinsic resolution: 50 nm. Hadronic momentum measurement via Multiple Coulomb Scattering. π/µ separation at low energies via de/dx measurements. e identification and energy measurements for e, γ. Universität Hamburg 46 01.04.2011 The OPERA Experiment

Event Reconstruction Europe: Japan: ECC Scanning and alignment: CS & ECC brick scanning: Conducted by automatic microscopes at scanning labs in Europe & Japan. CS & ECC brick alignment: Via X-rays and cosmic ray-tracks. Universität Hamburg 47 01.04.2011 The OPERA Experiment

Event Reconstruction ECC vertex reconstruction: Scan-back of tracks found in CS. Volume-scan of 1 cm 2 around supposed vertex. Universität Hamburg 48 01.04.2011 The OPERA Experiment

Event Reconstruction Short decay: Long decay: Impact parameter b. Kink angle θ kink. Decay search procedure: In-track decay search. Extra-track search. Measurement of θ kink or b. Universität Hamburg 49 01.04.2011 The OPERA Experiment

A Typical ν µ Event (CC) ED view: ECC reconstruction: Universität Hamburg 50 01.04.2011 The OPERA Experiment

A Typical ν µ Event (NC) ED view: ECC reconstruction: Universität Hamburg 51 01.04.2011 The OPERA Experiment

A ν µ Charm Event ED view: ECC reconstruction: Universität Hamburg 52 01.04.2011 The OPERA Experiment

A ν e Event ECC reconstruction: Universität Hamburg 53 01.04.2011 The OPERA Experiment

The First ν τ Candidate Event γ-attachment to the vertices: distance from IP w.r.t. IP w.r.t. Probability Probability 2ry vertex 1ry vertex 2ry vertex of attachment of attachment (resolution) (resolution) to 1ry vertex to 2ry vertex γ1 2.2 mm 45.0(11) µm 7.5(7) µm < 10 3 0.32 γ2 12.6 mm 85.6(56) µm 22(50) µm 0.10 0.82 Universität Hamburg 54 01.04.2011 The OPERA Experiment

The First ν τ Candidate Event Angle between parent track and hadronic shower axis: Selection criteria: φ > π/2. ν τ candidate event: φ = (3.01 ± 0.03) rad. Universität Hamburg 55 01.04.2011 The OPERA Experiment

OPERA Expected Performance Assumptions: sin 2 2θ 23 = 1. m 2 23 = 2.5 10 3 ev 2. Total exposure of 22.5 10 19 p.o.t.. Expected performance: Number of ν µ CC + NC interactions: 23600. Number of ν e + ν e CC interactions: 160. Number of ν τ CC interactions: 115. τ decay BR Number of Number of channel [%] signal events BG events τ µ 17.7 2.9 0.17 τ e 17.8 3.5 0.17 τ h 49.5 3.1 0.24 τ 3h 15.0 0.9 0.17 Total 10.4 0.75 Universität Hamburg 56 01.04.2011 The OPERA Experiment

Conclusion & Outlook Other topics: ν µ ν µ oscillation disappearance search. ν µ ν e oscillation appearance search. Atmospheric neutrino oscillation study. Universität Hamburg 57 01.04.2011 The OPERA Experiment