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The OPERA experiment at LNGS

The OPERA experiment at LNGS. Chiara Sirignano on behalf of the OPERA collaboration Salerno University & INFN. QUARKS – 2010 16 th International Seminar on High Energy Physics Kolomna, Russia, June 6-12 2010. Outline. Introduction The OPERA Detector at work Data Analysis

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The OPERA experiment at LNGS

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  1. The OPERA experiment at LNGS Chiara Sirignano on behalf of the OPERA collaboration Salerno University & INFN QUARKS – 2010 16th International Seminar on High Energy Physics Kolomna, Russia, June 6-12 2010

  2. Outline • Introduction • The OPERA Detector at work • Data Analysis • OPERA latest news …

  3. 732 Km Oscillation Project with Emulsion tRacking Apparatus • Long baseline neutrino physics experiment • CNGS quasi - pure nm beam, <L> = 732 km, <E> = 17 GeV • Appearance signal nmnt (by productnmne ) • Hybrid setup (Nuclear Emulsions + electronics) • Atmospheric neutrino data allowed region oscillation search

  4. Belgium IIHE-ULB Brussels Russia INR RAS Moscow NPI RAS Moscow ITEP Moscow SINP MSU Moscow JINR Dubna Italy Bari Bologna LNF Frascati L’Aquila, LNGS Naples Padova Rome Salerno Croatia IRB Zagreb France LAPP Annecy IPNL Lyon IPHC Strasbourg Tunisia CNSTN Tunis Japan Aichi Toho Kobe Nagoya Utsunomiya Turkey METU Ankara Germany Hamburg Münster Rostock Israel Technion Haifa Korea Jinju The OPERA Collaboration 180 physicists, 33 institutions in 12 countries Switzerland Bern ETH Zurich http://operaweb.lngs.infn.it

  5. Physics motivation • Super-K (1998) : atmospheric neutrino anomaly interpretable as µ-> oscillation • CHOOZ (reactor) : µ->e oscillation could not explain the anomaly • K2K and MINOS (accelerator): confirmation of the Super –K µdisappearance signal

  6. Nuclear emulsions + Lead (ECC) “active target” • 3D particle reconstruction • Sub-micron spatial resolution tdecay kink t ~ 1 mm nt Challenge Detection of  CC interaction in a quasi- pure nm beam and direct observation of the t lepton decay topologies. • t -m - nt nm (17.4%) • t - e- nt ne (17.8%) • t - h-nt n(po) (49.5%) • t -p+ p- p-ntn(po) (14.5%) High background rejection

  7. - nm n No oscillation - nm nt Oscillation ~1 mm nt events topological signature Expected data sample after 5 years • Target: ~ 1250 tons, 22.5E19 p.o.t. • > 20000 neutrino interactions • ~ 100 nt interactions • ~ 10 nt identified • < 1 background event

  8. GPS L = 732 Km CNGS neutrino beam CERN  730 km LNGS The beam is optimized to maximize the number of n t CC interactions

  9. The largest underground laboratory in the world (180 000 m3 ) about 3100 m.w.e. shielding CNGS C OPERA B A 1 cosmic muon /m2/h LNGS – Gran Sasso National Lab

  10. OPERA detector RPC RPC Target Drift tubes Target Veto Muon Spectrometer Muon Spectrometer 10 m 10 m 20 m • 53 BRICK WALLS • ~150000 bricks • ~1.25 kton Brick Manipulator System • HIGH PRECISION TRACKERS • spatial resolution < 0.5 mm • TARGET TRACKERS • Trigger task • Brick identification • 2 x 31 scintillating strip walls read with PMT • 0.8 cm resolution • INNER TRACKERS • 990-ton dipole magnets • (B = 1.55 T) • RPC resolution ~1.3 cm (Ref. JINST 4 (2009) P04018)

  11. SM1 SM2 • Extract Brick and CS, scan CS. • Confirm the event in the ECC brick. • Develop the brick and send to scanning labs. Target area (ECC + CS + TT) Brick Manipulator System Muon spectrometer (Magnet+RPC+PT)

  12. ECC target brick 75.4mm 1 mm 125mm CS sheet   8.3kg 10X0 Pb  beam 100mm 2 emulsion layers (42 m thick) poured on a 200 m plastic base OPERA emulsion film (Fuji Japan ) • 57 emulsion films + 2 CS interface sheet • 56 * 1 mm Pb (lead + 0.04 % Ca) plates Lead plate (Goslar Germany)

  13. Interface emulsion films: high signal/noise ratio for event trigger and scanning time reduction TT 2.6 cm ECC 10cm 12.5cm Changeable Sheet (CS) CS interface sheet Position accuracy of the electronic predictions Angular accuracy of the electronic predictions

  14. Emulsion films scanning EU: ESS (European Scanning System) Japan: SUTS (Super Ultra Track Selector) • Scanning speed/system: 75cm2/h • High speed CCD camera (3 kHz),Piezo-controlled objective lens • FPGA Hard-coded algorithms • Scanning speed/system: 20cm2/h • Customized commercial opticsand mechanics • Asynchronous DAQ software Both systems demonstrate: • ~ 0.3 m spatial resolution • ~ 2 mrad angular resolution • ~ 95% base track detection efficiency

  15. CSd nm 2 1 … 53 57 48 49 50 51 52 54 55 56 Vertex finding Track follow-up film by film: • alignment using cosmic ray tracks • definition of the stopping point  ~2 µm Ref. JINST 4 (2009) P06020 Volume scanning (~2 cm3) around the stopping point

  16. lead emulsion IP DZ Decay search Data The IP evaluation is a crucial point in order to detect decay topologies Muon I.P. tm (MC) IP(mm) IP of the muon tracks attached to the neutrino vertices found

  17. OPERA status 2000: approval of the CNGS project2003: start of detector construction 2004: end of CNGS beam civil engineering 2006: commissioning run (empty detector’s target) • 7.6E17 pot 2007: short pilot run (40% target) • 8.2E17 pot, 38 ν events in the target 2008: 1st physics run • 1.78E19 pot, 1663 ν events in the target, 0.7 ντ expected 2009: 2nd physics run • 3.52E19 pot, 3693 ν events in the target, ~2 ντexpected in total 2010: 3rd physics run (May – November) • hope to reach more than 4 E 19 pot 1 year CNGS nominal: 4.5E19 pot

  18. Performance Plot

  19. NC/CC events: Data vs MC } • Visible NC/CC takes into account: • NC/CC true ratio (0.3) • Target interactions selectionefficiency • Muon ID efficiencies • Events migrations due to misidentification CC - NC -- NC excess in data described by MC when including BCK due to external interactions: -- NC/CC ratio by cutting harder on the fiducial volume: Data 2008: NC/CC= 0.230 ± 0.014 (stat.) Data 2009: NC/CC= 0.228 ± 0.009 (stat.) MC:NC/CC= 0.236 ± 0.005 (stat.)

  20. Run 2008 event location (completed) Cs scanning and brick selection Scanned Found Scanned Located neutrino interactions Located interactions in ECC , then used for the decay search

  21. Run 2009 event location (in progress) CS scanning results

  22. Event location details (Run 2009)

  23. Charm events (I) x-view 1ry muon • Charm topology analogous to  (similar lifetime): reference sample for the decay finding efficiency • Systematic decay search completed on 1088 neutrino located interactions • 20 events found showing a charm decay topology 1ry vertex kink Event in Europe (D0  4 prong) daughter muon Event in Japan (kink) 1.3 mm

  24. Primary vertex Decay vertex Charm events (II)

  25. Test beam data samples of pions and several MC samples were produced and used for the development of the method. Very detailed results are given and should be considered as reference ones for further MCS investigations. 9 8 7 6 5 4 3 2 1 Prec (GeV) p test beam 1 2 3 4 5 6 7 8 Pbeam (GeV) Particles momenta measuremnts by MCS Measurements were performed also on several selected soft muon events registered in the OPERA detector s = (22±4)%

  26. ne CC interaction 6 electron neutrino interactions were found in a subsample of 800 CC located interactions.

  27. Example of reconstructed ’s in real neutrino interactions g reconstruction (I) Important for  hadronic decay channels (signal vs background discrimination)

  28. g reconstruction (II)

  29. Conclusions • The OPERA experiment at LNGS was designed and successfully constructed to ensure the detection of neutrino oscillations in appearance mode through the study of the nm -> nt channel. • The analysis of neutrino data taken in the CERN CNGS beam in the 2008-2009 runs is successfully on going. • Decay event topologies due to charmed particles have been observed in • agreement with expectations, as well as events induced by prompt ne present in • the CNGS beam.

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