The OPERA Experiment

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1 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 The OPERA Experiment

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

3 The OPERA Experiment Universität Hamburg The OPERA Experiment

4 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 The OPERA Experiment

5 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 The OPERA Experiment

6 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: m (3 400 m w.e.). Number of cosmic µ: 1 m 2 h 1. Universität Hamburg The OPERA Experiment

7 The CNGS Beam CNGS: CERN Neutrinos to Gran Sasso. E p 400 GeV p.o.t p.o.t p.o.t p.o.t expected Nominal p.o.t./year Total p.o.t. expected 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 The OPERA Experiment

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

9 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: bricks of 8.3 kg lead each ( 1.28 kt target mass). Universität Hamburg The OPERA Experiment

10 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 The OPERA Experiment

11 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 The OPERA Experiment

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

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

14 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 The OPERA Experiment

15 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 The OPERA Experiment

16 The First ν τ Candidate Event ECC reconstruction: Track No Particle type p [GeV] 1 hadron p 0.60 ± hadron hadron pion from prompt neutral Universität Hamburg The OPERA Experiment

17 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 The OPERA Experiment

18 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 The OPERA Experiment

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

20 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 = ( ) GeVc 1. Universität Hamburg The OPERA Experiment

21 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 = ( ) GeVc 1. Universität Hamburg The OPERA Experiment

22 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 The OPERA Experiment

23 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: ( ) 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 The OPERA Experiment

24 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: Number of charm events: ± (syst.) events. 1.8 % probability that the observed event is a background event σ significance of ν τ observation in OPERA. Background expectation (all τ decay modes): Number of background events: ± (syst.). 4.5 % probability that the observed event is a background event σ significance of ν τ observation in OPERA. Universität Hamburg The OPERA Experiment

25 Significance of ν τ Observation Observation for 1088 decay-searched events: 1 event (1-prong hadronic τ decay channel). Assumptions: m 2 23 = 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 > ev 2 at 90% CL. Universität Hamburg The OPERA Experiment

26 Event Statistics Analysis status: Vertex located: events. Decay search performed: events. Universität Hamburg The OPERA Experiment

27 Conclusion & Outlook Universität Hamburg The OPERA Experiment

28 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) 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 The OPERA Experiment

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

30 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 The OPERA Experiment

31 Backup Slides Universität Hamburg The OPERA Experiment

32 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 s 12 c e iɛ 2/2 0 0 s 23 c 23 s 13 e iδ 0 c 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 The OPERA Experiment

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

34 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 The OPERA Experiment

35 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 The OPERA Experiment

36 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 The OPERA Experiment

37 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 The OPERA Experiment

38 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 The OPERA Experiment

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

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

41 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 The OPERA Experiment

42 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 The OPERA Experiment

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

44 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 The OPERA Experiment

45 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 The OPERA Experiment

46 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 The OPERA Experiment

47 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 The OPERA Experiment

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

49 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 The OPERA Experiment

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

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

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

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

54 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 < γ mm 85.6(56) µm 22(50) µm Universität Hamburg The OPERA Experiment

55 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 The OPERA Experiment

56 OPERA Expected Performance Assumptions: sin 2 2θ 23 = 1. m 2 23 = ev 2. Total exposure of p.o.t.. Expected performance: Number of ν µ CC + NC interactions: 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 τ e τ h τ 3h Total Universität Hamburg The OPERA Experiment

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

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