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

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Oswald Blair
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1 Latest Results from the OPERA Experiment (and new Charge Reconstruction) on behalf of the OPERA Collaboration University of Hamburg Institute for Experimental Physics

2 Overview The OPERA Experiment Oscillation Search: νμ ντ Oscillation Search: νμ νe Charge Reconstruction with AMM Conclusion and Outlook Slide 2

3 The OPERA Experiment OPERA: Oscillation Project with Emulsion Tracking Apparatus L P( νμ ν τ ) sin (2 θ 23)sin (Δ m ) 4E Appearance measurement: First direct observation of νμ ν τ oscillation Observation of ν interactions and decay of τ leptons τ Slide 3

4 The OPERA Experiment LNGS CERN Realisation: High-energy long-baseline pure νμ beam <Eν> = 17 GeV ~ 730 km distance from CERN to LNGS Large target mass with μm precision: Emulsion Cloud Chambers (ECC): lead plates and nuclear emulsion films Spectrometer for background reduction Slide 4

5 ντ Detection ντ signal: τ-- creation in ντ CC interaction Decay of the τ-- lepton after ~ 600 μm Topology: 'kink' characteristic of the tau decay (missing energy) Slide 5

6 ντ Detection ντ signal: Background processes: μ+ τ-- creation in ντ CC interaction Decay of the τ-- lepton after ~ 600 μm Topology: 'kink' characteristic of the tau decay (missing energy) νμ CC interactions with charm production & undetected muon(s) Hadronic re-interactions of secondary hadrons in lead Large-angle μ scattering Slide 6

7 The OPERA Hybrid Detector Y Z Slide 7

8 The OPERA Hybrid Detector Y Z SM2 SM1 Slide 8

9 The OPERA Hybrid Detector target B B Y Z magnetic spectrometer Slide 9

10 The OPERA Hybrid Detector target μ ν X B B Y Z magnetic spectrometer Slide 10

11 The OPERA Hybrid Detector target μ ν X B B Y Z magnetic spectrometer Slide 11

12 The OPERA Hybrid Detector target μ ν X B B Y Z magnetic spectrometer Slide 12

13 The OPERA Hybrid Detector target μ ν X B B Y Z magnetic spectrometer Slide 13

14 The OPERA Hybrid Detector Target target μ ν X B B Y Z magnetic spectrometer Slide 14

15 SM1 νμ ντ Oscillation Search (main goal) Slide 15

16 The 4th ντ Candidate Event SM1 ECC reconstruction Primary vertex: 4 tracks Red track: tau decay secondary candidate after 1.09 mm Decay channel: τ 1h Slide 16

17 Charm Control Sample OPERA data set arxiv: ECC 54 ± 4 charm events expected 50 observed in control sample Reconstructed νμ CC interaction with a charmed hadron in the final state Slide 17

18 νμ ντ Analysis Overview * 1019 p.o.t total (~80% of the proposal) and ν target interactions Data sample: OPERA recent results at Neutrino events ( : two most probable bricks, : first most probable brick) 4 signal events observed vs expected background events p-value for background fluctuation 1.03 * 10-5 No oscillation hypothesis excluded at 4.2 σ τ decay channel Expected signal Δm232 = 2.32 mev2 Background analyzed sample τ- μ ± ± τ- e ± ± τ- h ± ± τ- 3h 0.57 ± ± Overall 2.10 ± ± Observed events Slide 18

19 SM1 νμ νe Oscillation Search Slide 19

JHEP 1307 (2013) 004 1µm resolution in the ECC Films

20 νe Appearance νe searched in 505 (~ 30% full statistic) Neutrino Interactions without a Muon in the final state JHEP 1307 (2013) 004 1µm resolution in the ECC Films separation of e+ e- pairs and single e νe interaction in ECC Slide 20

21 νe Appearance Distribution of reconstructed Energy of the νe Events JHEP 1307 (2013) 004 Compatible with no oscillation hypothesis Expected Background for 3-flavour Analysis: 19.8 Observed Events : 19 Slide 21

22 νe Appearance Exclusion limits for a fourth sterile neutrino JHEP 1307 (2013) 004 sin2(2θnew) < 7.2 x 10-3 (90% CL) at large values of Δm2 Slide 22

23 SM1 Charge Reconstruction with the new Angular Matching Method Slide 23

24 Angular Matching Method (AMM) The idea of the method: Spectrometer Top View Track measured: in front and behind the magnetic field Precision Tracker Check if both track segments fit the same circle Construct a weight to indicate the accuracy of fit (from 0 to 1) Slide 24

25 Impurity with AMM arxiv: Impurity: nw : number of wrong charge sign determination nc : number of events with charge sign determination Realistic beam Monte Carlo (MC II) Impurity for one super module OPERA standard method Angular Matching Method Slide 25

26 SM1 Conclusion and Outlook Slide 26

27 Conclusion CNGS beamsm1 concluded: * 1019 p.o.t. (80% of the proposed) ν beam target interactions τ appearance: Confirmed ντ candidate events: 4 Non oscillation excluded at 4.2 σ (conservative approximation) e appearance: Measured events compatible with no oscillation hypothesis Limit for sterile neutrino sin2(2θnew) < 7.2 x 10-3 (90% CL) at high Δm2 Slide 27

28 Outlook τ appearance: SM1 Completing scanning and analysis Improve background studies Likelihood fit e appearance: Analysis with full data sample Angular Matching Method (AMM): Capability to reduce charm background Slide 28

29 SM1 Thank you for your attention! Slide 29

30 OPERA Publications N. Agafonova etsm1 al. [OPERA Collaboration], Evidence for νμ ντ appearance in the CNGS neutrino bean with the OPERA experiment, Phys. Rev. D 89, (R) (2014) N. Agafonova et al. [OPERA Collaboration], Search for νμ νe oscillations with the OPERA experiment in the CNGS beam, JHEP 1307 (2013) 004 N. Agafonova et al. [OPERA Collaboration], The Angular Matching Method for the Muon Charge Sign Measurement in the OPERA Experiment, arxiv: (2014) Slide 30

31 SM1 Backup Slide 31

32 Visible Energy of all Tau Candidates Sum of the momenta of charged particles and γ s measured in emulsion Slide 32

33 The CNGS νμ Beam CNGS: CERN Neutrinos to Gran Sasso Slide 33

34 The CNGS νμ Beam CNGS: CERN Neutrinos to Gran Sasso Baseline: ~ 730 km distance form CERN to LNGS Slide 34

35 LNGS LNGS: Laboratori Nazionali del Gran Sasso Location: Below mountain Corno Grande of Gran Sasso, Italy Vertical rock coverage: 1400 m (3800 m.w.e.) Cosmic μ rate: ~ 1 m-2 h-1 Slide 35

36 The Target Area SM1 Target Area consist of: Emulsion Cloud Chambers (ECC) called bricks 31 walls of holder infrastructure for ECC bricks and Target Tracker (TT) Slide 36

bricks and Target Tracker (TT) plastic scintillator strips

37 The Target Area SM1 Target Area consist of: Emulsion Cloud Chambers (ECC) called bricks 31 walls of holder infrastructure for ECC bricks and Target Tracker (TT) plastic scintillator strips (horizontal & vertical) Changeable Sheets (CS): 2 extra emulsion sheets Slide 37

corresponding to ~ 10 X0) Total: ~ 150 000 bricks of 8.3 kg each (~ 1.

38 Emulsion Cloud Chamber Emulsion Cloud Chamber (ECC) bricks: Per brick: 57 x 2 nuclear emulsions in plastic base, 56 lead plates (altogether corresponding to ~ 10 X0) Total: ~ bricks of 8.3 kg each (~ 1.25 kt total target mass) Spatial / angular resulution: ~ 1 μm / ~ 2 mrad Slide 38

39 Event Reconstruction SM1 Event Reconstruction performed in 2 steps: Brick search with ED Emulsion (ECC): Emulsions scanned by automatic microscopes Track & ν interaction vertex reconstruction Kinematical analysis Slide 39

40 Magnetic Spectrometer SM1 Magnetic Spectrometer: Downstream of each target area Consist of: Dipol magnets with 1.53 T Resistive Plate Chamber (RPC & XPC) detectors Precision Tracker (PT) drift tubes Slide 40

41 Event Reconstruction SM1 Event Reconstruction performed in 2 steps: Electronic detector: ν interaction vertex localisation (with Target Tracker) μ identification (CC/NC separation) & momentum measurement Hadronic shower energy estimation Triggers ECC event reconstruction Slide 41

42 Event Reconstruction SM1 τ decay search procedure: In-track kink search Search for extra tracks Measurement of the kink angle θkink or the impact parameter b long decay short decay Slide 42

43 The 1st ντ Candidate Event ECC reconstruction: SM1 Primary vertex: 7 tracks Red / cyan track(s): kink after 1.35 mm Decay channel: τ h (τ- ρ- (π- π0)ντ) Slide 43

44 The 2nd ντ Candidate Event ECC reconstruction: SM1 Primary vertex: 2 tracks Red track: 3-prong decay after 1.54 mm Decay channel: τ 3h Slide 44

45 The 3th ντ Candidate Event ECC reconstruction: SM1 Primary vertex: 2 tracks Red track: after mm Decay channel: τ μ Slide 45

46 Charm Bachground ECC reconstruction: Hadron production with charm SM1 Topology similar to τ-decay (modes and lifetime) But with μ at primary vertex Good control sample Slide 46

47 Charm Bachground SM1 OPERA recent results at Neutrino 2014 Slide 47

48 Charm Bachground data analysis: SM1 Slide 48

49 SM1 Charge Reconstruction with AMM Slide 49

50 The OPERA Hybrid Detector target μ ν X B B Y Z magnetic spectrometer Slide 50

51 The OPERA Hybrid Detector target μ ν X B B Y Z magnetic spectrometer Slide 51

52 The OPERA Hybrid Detector Top View Side View Target target μ ν X B B Y Z magnetic spectrometer Slide 52

53 The OPERA Hybrid Detector Top View Side View Target target μ ν X B B Y Z magnetic spectrometer Slide 53

54 The OPERA Hybrid Detector Top View muon track Target Target μ ν X B B drift tube wall Slide 54

55 The OPERA Hybrid Detector Top View muon track Target Target μ ν X B B for a perfect circle (neglecting energy loss): drift tube wall α1 = α 2 Slide 55

56 Angular Matching Method (AMM) SM1 1. Calculate the asymmetry: Slide 56

57 Angular Matching Method (AMM) SM1 1. Calculate the asymmetry: arxiv: Plot the distribution: Slide 57

58 Angular Matching Method (AMM) 3. Definition of weight: SM1 Area under the distribution from the edges to the measured absolute value Maximum weight at peak center: w = 100% At the edges: w 0% Weight: green area arxiv: weight calibration fit measured Δ(α)rel Slide 58

59 Angular Matching Method (AMM) 3. Definition of weight: SM1 Area under the distribution from the edges to the measured absolute value Maximum weight at peak center: w = 100% At the edges: w 0% Weight: green area arxiv: weight calibration fit measured Δ(α)rel Slide 59

60 Angular Matching Method (AMM) SM1 Wrong charge sign measurements mostly have a low weight Monte Carlo event: Muon was simulated measured charge sign -1 weight: drift tube walls magnet arm Slide 60

61 Angular Matching Method (AMM) Low weight SM1 indicates something strange Real data event measured charge sign: weight: drift tube walls magnet arm Slide 61

62 Angular Matching Method (AMM) Real data event SM1 measured charge sign -1 weight: reconstructed track most likely track drift tube walls magnet arm Slide 62

63 Find strange events with AMM Low weight SM1 indicates something strange happens real date: showered particle weight magnet arm drift tube walls drift tube walls Slide 63

64 Impurity with AMM Impurity for real data SM1 Four charge measurements Three in agreement, one in disagreement charge sign not equal in both super modules arxiv: number of all events Impurity for one super module measurement in disagreement are accumulated at low absolute weights Slide 64

65 Paper about the AMM on arxiv SM1 Slide 65

RECENT RESULTS FROM THE OPERA EXPERIMENT

RECENT RESULTS FROM THE OPERA EXPERIMENT P. DEL AMO SANCHEZ on behalf of the OPERA Collaboration LAPP, 9, Chemin du Bellevue, BP 110 74941 Annecy-le-Vieux, FRANCE The OPERA neutrino experiment recently