OPERA : CERN-LNGS Long Base ν μ→ ν τ Appearance Experiment COLLABORATION 36 groups ~ 165 physicists Russia INR Moscow, ITEP Moscow, JINR Dubna, Obninsk.

Slides:



Advertisements
Similar presentations
May 11 th, 2007 LNF Scient. Comm M.Spinetti 1 OPERA/CNGS1 O scillation P roject with E mulsion-t R acking A pparatus 1. Electronic detectors status of.
Advertisements

Oscillation Project with Emulsion tRacking Apparatus F. Juget Institut de Physique Université de Neuchâtel Neutrino-CH meeting, Neuchâtel June
Neutrino Oscillation Appearance with OPERA Amina ZGHICHE Oscillation Project with Emulsion tRacking Apparatus.
1 Status of the OPERA long-baseline neutrino experiment Magali Besnier PIC 07- Annecy June 27 th 2007.
Emulsion scanning: present status and plans for the coming run Giovanni De Lellis.
OPERA experiment T.Toshito (Nagoya univ. Japan) for the OPERA collaboration Apr
3/1/05 Status of the SHBD for the NUMI OPERA exposure D. Autiero IPN Lyon  Reminder about the proposed setup for the SHBD  Status of the sub-detectors.
Status of OPERA N. Naganawa (Nagoya University) Flavor physics.
Kouji Narita Nagoya University, Japan CHORUS collaboration Study of charm production in neutrino interactions.
The OPERA Experiment 12 th Topical Seminar on Innovative Particle and Radiation Detectors (IPRD10) 7-10 June 2010, Siena, Italy Jonas Knüsel Albert Einstein.
Hybrid emulsion detector for the neutrino factory Giovanni De Lellis University of Naples“Federico II” Recall the physics case The detector technology.
Status of the OPERA experiment Yoshiaki Nonoyama Nagoya Univ.
DONUT Reinhard Schwienhorst DOE review 7/28/1999.
Status and the preliminary results of the OPERA experiment V.Tioukov (INFN, Napoli) on behalf of the OPERA collaboration V. Tioukov QFTHEP11, Sochi.
The OPERA long baseline neutrino experiment: status and first results Luigi Salvatore Esposito Laboratori Nazionali del Gran Sasso on behalf of the OPERA.
A. Chukanov On behalf of OPERA collaboration JINR, Dubna TAUP 2011, Munich, 5-9 september, 2011.
Gran Sasso, 19/03/2003 OPERA Project Board meetingH. Pessard / 1 Brick Manipulator System (BMS) project uEvolutions and final design n Brick sliding and.
Status and results from the OPERA experiment Tsutomu FUKUDA ( Nagoya University ) On behalf of the OPERA Collaboration NNN10, 14 Dec 2010, Toyama International.
ICHEP 2004, Beijing H. Pessard/ OPERA - 1 The OPERA experiment CNGS long-baseline program in Europe  Search for  appearance in a  beam: prove   
Recent results of OPERA experiment T. Shiraishi - Nagoya University On behalf of The OPERA Collaboration Belgium ULB Brussels Croatia IRB Zagreb France.
The OPERA experiment Oscillation Project with Emulsion tRacking Apparatus Collaboration: Belgium (IIHE(ULB-VUB) Brussels), Bulgaria (Sofia University),
MTM Bologna, 17/6/ 2005 We know that in Nature there are three kinds of neutrinos and in particular atmospheric neutrinos show a deficit of  This effect,
1 The OPERA emulsion detector for a long-baseline neutrino oscillation experiment H.Shibuya Toho Univ., Japan K.Hoshino, M.Komatsu, K.Niwa Nagoya Univ.,
Caren Hagner, Universität HamburgDESY Seminar, OPERA and its Tau Neutrino Candidate  Neutrino mass, mixing and neutrino oscillations  OPERA.
September 11th, 2006LNGS and the Neutrinos from CERN OPERA 1 OPERA O scillation P roject with E mulsion-t R acking A pparatus.
R. ZimmermannDortmund, April OPERA physics motivation - CNGS physics motivation - CNGS OPERA detector OPERA detector ν τ appearance ν τ appearance.
OPERA Experiment, Brick Finding Program A. Chukanov Joint Institute for Nuclear Research ISU, 12 th February, 2007.
Tsutomu Fukuda Nagoya University, JAPAN
Status and results from OPERA Tomoko Ariga LHEP, University of Bern on behalf of OPERA Swiss groups of Bern and ETHZ.
The OPERA neutrino oscillation experiment Paolo Strolin University and INFN, Napoli.
Operation of and results from OPERA Ciro Pistillo LHEP Bern University CHIPP Plenary meeting Lausanne, EPFL-LPHE September
First neutrino events in the OPERA emulsion target Ciro Pistillo LHEP Bern University for the OPERA collaboration Rencontres de Moriond: Electroweak interactions.
LNGS Scientific Committee Status of OPERA/CNGS1 April 8 th, 2005 Yves Déclais on behalf of the OPERA Collaboration.
Status of the OPERA Neutrino Oscillation Experiment 5-8 January 2010, Cracow, Poland Sergey Dmitrievsky Joint Institute for Nuclear Research, Dubna on.
1 Recent results on the observation of    oscillation in the OPERA experiment NakatsukaYuji Nagoya University On behalf of OPERA collaboration ICISE.
OPERA Maximiliano Sioli (Bologna University and INFN) for the OPERA Collaboration NOW 2006, Conca Specchiulla, Sep 9-16, 2006  → 
Hamburg Björn Wonsak 1 First results and status of the OPERA experiment Focussed on the electronic detector, especially the presicion tracker (PT)
CHORUS Results on Charm Physics Belgium (Brussels, Louvain-la-Neuve), CERN, Germany (Berlin, Münster), Israel (Haifa), Italy (Bari, Cagliari, Ferrara,
Observation of ν μ → ν τ oscillations in the CNGS beam with the OPERA experiment M. De Serio University of Bari & INFN Bari On behalf of the OPERA Collaboration.
New results from the OPERA experiment
   The European Long Baseline Program Les Houches, 21 June 2001 Dario Autiero CERN/EP Many thanks to A. Rubbia for providing material about ICARUS.
Neutrino Oscillations Studies with the Opera Experiment
1 NuFact’01 WG1 : Neutrino Oscillation Physics May 24-30, 2001 An appearance experiment to search for  -  oscillations in the CNGS beam CNGS1 O scillation.
100  m Nuclear emulsions are made of micro- crystals of silver halides (AgBr) dispersed in a gelatin layer. The energy released by ionizing particles.
1 The OPERA Long Baseline Neutrino Experiment: status and first results Introduction Detector overview CNGS neutrino beam start-up First neutrino events.
NOON04 Status of OPERA1 Status of OPERA OPERA Collaboration Nagoya University M. Komatsu.
Accelerator-based Long-Baseline Neutrino Oscillation Experiments Kam-Biu Luk University of California, Berkeley and Lawrence Berkeley National Laboratory.
Recent results of the OPERA search for       oscillations T. OMURA On behalf of The OPERA Collaboration 1/17 Belgium ULB Brussels Croatia IRB Zagreb.
OPERA Experiment, Brick Finding Program A. Chukanov Joint Institute for Nuclear Research Dubna, 25 th January, 2007.
Status and oscillation results of the OPERA experiment Florian Brunet LAPP - Annecy 24th Rencontres de Blois 29/05/2012.
NBI2006 Starting OPERA data-taking with the CNGS beam D.Autiero IN2P3/IPN Lyon 5/9/2006.
The synergy of the golden and silver channels at the Neutrino Factory Pasquale Migliozzi INFN - Napoli Work done in collaboration with D.Autiero, G.De.
2008 European School of High-Energy Physics - Trest, Czech Republic - 19 August - 1st September Target Tracker Data Analysis In OPERA Experiment S. Dmitrievsky,
Emulsion Test Beam first results Annarita Buonaura, Valeri Tioukov On behalf of Napoli emulsion group This activity was supported by AIDA2020.
HEP Conference 2009, Krakow, PolandH. Pessard / 1 Henri Pessard / LAPP Annecy (on behalf of the OPERA Collaboration) Status of the OPERA neutrino experiment.
Esperimento OPERA Commissione II INFN Roma 28 Settembre 2010 CNGS beam Detector operation Run 2008, 2009, 2010 Richieste finanziarie S. Simone Università.
Electromagnetic shower reconstruction with emulsion films in the OPERA experiment F. Juget IPH Université de Neuchâtel On behalf of the OPERA collaboration.
1 Latest results from the OPERA experiment Introduction Experimental setup: CNGS and detector Data Analysis and Oscillation results  appearance  disappearance.
OPERA : CERN-LNGS Long Base νμ→ντ Appearance Experiment
Current Status of The OPERA Experiment
Experience from Antoine Cazes, nuFact’08 Valencia
Rome, Funding Agencies meeting
More results from the OPERA experiment
The OPERA long baseline neutrino experiment : status and first results. Magali Besnier Laboratoire d’Annecy-le-Vieux de Physique des Particules On behalf.
Latest results from the OPERA experiment
Status of the OPERA experiment
OPERA Stato dell’esperimento Run 2007
Results from OPERA Pablo del Amo Sánchez for the OPERA collaboration
Workshop on Nuclear Track Emulsion and its Future
OPERETTE TEST BEAM EXPERIMENT :
Presentation transcript:

OPERA : CERN-LNGS Long Base ν μ→ ν τ Appearance Experiment COLLABORATION 36 groups ~ 165 physicists Russia INR Moscow, ITEP Moscow, JINR Dubna, Obninsk Belgium IIHE(ULB-VUB) Brussels France LAPP Annecy, IPNL Lyon, LAL Orsay, IRES Strasbourg Germany * Berlin, Hagen, Hamburg, Münster, Rostock Israel Technion Haifa Italy Bari, Bologna, LNF Frascati, L’Aquila, LNGS, Naples, Padova, Rome, Salerno Japan Aichi, Toho, Kobe, Nagoya, Utsunomiya Switzerland Bern, Neuchâtel Turkey METU Ankara China IHEP Beijing, Shandong Croatia Zagreb University Bulgaria Sofia University

Venice2 OPERA : CERN-LNGS Long Base ν μ→ ν τ Appearance Experiment Motivations: Direct observation of ν μ -> ν  oscillation by detection of ν τ + Pb CC interaction in initially pure ν μ beam (0.8% ν e, 2% ν μ ) ν μ -> ν e observation: θ 13 measurement

OPERA : CERN-LNGS Neutrino Beam (CNGS) 4.5x10 19 pot / year ~ 17 GeV

Venice4 Emulsion Cloud Chamber (ECC) –Emulsions for tracking, passive material as target –Basic technique established: charmed “X-particle” first observed in cosmic rays (1971) DONUT/FNAL beam-dump experiment:  events observed  m 2 = ( ) x eV 2   M target ~ 2 kton –large detector  sensitivity, complexity –modular structure (“bricks”): basic performance is preserved Pb Emulsion layers  1 mm Experience with emulsions and/or  searches : E531, CHORUS, NOMAD and DONUT Experimental technique

Venice5 8 m Pb/Em. target Electronic detectors: target tracker, μ spectrometer, veto counters  find the brick with interaction   ID, charge & p Emulsion analysis  vertex  decay kink  e/ γ /μ/π ID, multiple scattering, kinematics Extract selected brick Pb/Em. ECC brick 8 cm Pb 1 mm Basic “cell” Emulsion OPERA Detector: Supermodule structure

Venice6 Underground assembly space ( ) 4 m corridor 48 m Hall B Borexino Hall C Pb-emulsion stacking brick packing BAM Emulsion storage OPERA Detector: Disposition in LNGS underground lab

Venice7 31 target planes / spectrometer ( bricks, 1766 tons)   Front damping structure Rear damping structure Electronic barrack Mechanical structure and risk analysis study accepted by safety authorities OPERA Detector: Disposition in LNGS underground lab

Venice8 ECC Brick 10X 0 ( 57 emulsion films ) Packing Options: Vacuum Mechanical

Venice9 Day by day experiment operation scheme Emulsion Scanning stations  locate interaction   detection Gran Sasso  tag interaction  extract ECC brick ECC brick 30bricks/day  cosmic ray exposure  develop emulsion sheet etc.

Venice10 OPERA Event rate OPERA ktons νμCCνμCC νμNCνμNC 7300 νμCCνμCC 510 νeCCνeCC 194 νeCCνeCC 17 __ 5 years /year in shared mode Δm2Δm2 OPERA 1 x eV x eV x eV ν τ CC interactions efficient beam monitoring Possible improvements: proton intensity increase  1.5 running in dedicated mode  1.7  up to 80 events per day in OPERA to be taken into account for the scanning power 2.55

Venice11 Number of events: full mixing, 5 years 4.5(6.76)x10 19 pot / year signal (  m 2 = 1.3 x eV 2 ) signal (  m 2 = 2.0 x eV 2 ) signal (  m 2 = 3.0 x eV 2 ) BKGD Final Design 3.1(4.7)7.3(11)16.4(24.6)0.7(1.06) 5 YEARS5 YEARS x 1.5 44 44 33 33

Venice12 CNGS schedule

Venice13 Spectrometer :Magnet, RPC, XPC and Precision Tracker Veto and Beam monitoring Target : Brick wall and Target Tracker DAQ Brick production and Handling Scanning and Computing OPERA construction tasks and schedule

Venice14 OPERA construction tasks and schedule

Venice15 Spectrometer construction slabs base coil Fe (5 cm) RPC 12 Fe slabs in total 8.2 m B= 1.55 T Total Fe weight ~ 1 kton Tests at Frascati lab

Venice16 Spectrometer construction Aug 2003

Venice17 Spectrometer construction Dec 2003

Precision tracker Electronics FE : board ready TDC : chip tested, board being designed DAQ : running HV board : final design in progress Full size prototype as seen from the top Performance: efficiency: 99.1% resolution:  300 μm

Venice19  XY planes, 7000m 2 in total  Scintillator strips 7m x 2.5cm x1cm  AMCRYS-H (Kharkov) + Kuraray WLS  1000 MaPMT Hamamatsu 64channels  Dedicated Front End electronics for gain correction  Autotriggerable and 1/5 p.e 7m Target tracker

Venice20 Target tracker first wall constructed (Strasbourg)

Venice21 Produce about 8 modules/week. Delivery at GS (modules already calibrated): 1.16 modulesFebruary modulesMay modulesJuly modulesSeptember modulesNovember modulesJanuary modulesMarch modulesMay modulesJuly modulesSeptember 2005 TT installation: 31/03/2004 to 18/01/2006 TT Walls will be mounted outside (about 15 walls prepared in advance) and slided inside the detector after each brick wall installation. Target tracker delivery

Venice Mbits switch 1) A Smart (Ethernet capable) F/E card  TT : at the PM level  RPC, PT : plane or station level 2) A distributed synchronization scheme (time + deterministic commands) 3) A network architecture with different levels of switches up to the event building work stations Same architecture for : target tracker, RPC and Precision tracker The 3 ingredients of the DAQ architecture

Venice23  Pb 1 mm   Lead from Boliden Mass production starts April 2003 (~ m 2 ) Refreshing done in the Tono Mine in Japan : 2 years duration One batch sent to LNGS every 2 months starting august 2003  emulsion storage LNGS (Hall B) june mm 100mm ECC components: emulsion & lead

Venice24 Naples-Frascati wall VV cable VV cable loop driving system CCD Camera The Vacuum sucker Vehicle (VV) 50 bricks/day ~ 3 hours Brick Manipulator prototype (LAPP Annecy)

Venice25 Routine  5cm 2 /hr Near future  20cm 2 /hr S-UTS prototype at Nagoya Dedicated hardware Hard coded algorithms European prototype Commercial products Software algorithms   ~ 2mrad  x ~ 0.5  m Emulsion scanning

Venice26 Emulsion scanning: ν τ → τ - →  - simulated & reconstructed event

Venice27 1.november 2003 started SM1 Magnet RPC installation 2.June 2004starts SM1 Target installation 3.January 2005BAM and BMS installation 4.July 2005 starts filling bricks Important milestones

Venice28  Important Physics Program First evidence of  -  appearance in few years data taking In a five years run: 7(11) signal x eV 2 ) and 0.7(1.) background events Studies to improve efficiency and to reduce the background Multi prong  decay channel under study Measurement of  13 ( See talk by P.Migliozzi )  Detector construction and installation Mass production started Large and complex detector installation started Detector (and CNGS beam !) will be ready in 2006 Conclusions

Venice29 OPERA Sensitivity 5 years 3 years  m 2 = 1.2x10 -3 eV 2 at full mixing sin 2 (2  ) = 6.0x10 -3 at large  m 2 5 years data taking

Venice30 Brick Assembling Machine (BAM) schedule Final specifications: December 2002 End of market search: March 2003 Technical audit:April 2003 Call for tenders:May to October 2003 Firm selection:November 2003 Ordering:December-January 2003 Construction and tests in the firm:January 2003 to February 2005 Delivery at Gran Sasso laboratory:March 2005 Assembly, installation:April 2005 Production acceptance tests at Gran Sasso: May to July 2005 Brick mass production:September 2005 to August 2006