Results from the OPERA experiment in the CNGS beam

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

arxiv: v1 [hep-ex] 1 Oct 2015

Results from the OPERA experiment in the CNGS beam

RECENT RESULTS FROM THE OPERA EXPERIMENT

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

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

Updated results of the OPERA long baseline neutrino experiment

Latest results of OPERA

arxiv: v1 [hep-ex] 11 May 2013

Search for sterile neutrino mixing in the muon neutrino to tau neutrino appearance channel with the OPERA detector

Results from the OPERA experiment at the CNGS beam


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

Status of the OPERA experiment

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

The OPERA Experiment

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

The CERN-Gran Sasso Neutrino Program

Tau-neutrino production study in 400 GeV proton interactions

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

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

Neutrino physics with the SHiP experiment at CERN

Experimental results on the atmospheric muon charge ratio

Long Baseline Neutrinos

The CNGS neutrino beam

ICARUS T600 experiment: latest results and perspectives

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

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

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

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

FIRST NEUTRINO EVENTS IN THE OPERA EMULSION TARGET

The SHiP experiment and its detector for neutrino physics

- ICARUS status and near future

Recent results from Super-Kamiokande

Long Baseline Neutrino Experiments

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

Perspectives of neutrino oscillation physics with long baseline beams

Accelerator Neutrino Experiments News from Neutrino 2010 Athens

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

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

New Results from the MINOS Experiment

PoS(KAON13)012. R K Measurement with NA62 at CERN SPS. Giuseppe Ruggiero. CERN

CNGS beam monitor with LVD

Muon reconstruction performance in ATLAS at Run-2

Susanna Costanza. (Università degli Studi di Pavia & INFN Pavia) on behalf of the ALICE Collaboration

Recent T2K results on CP violation in the lepton sector

First results and status of the OPERA experiment

Performance of the ICARUS T600 detector

HARP (Hadron Production) Experiment at CERN

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

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

Relative branching ratio measurements of charmless B ± decays to three hadrons

A search for heavy and long-lived staus in the LHCb detector at s = 7 and 8 TeV

Measuring the neutrino mass hierarchy with atmospheric neutrinos in IceCube(-Gen2)

The CNGS project. Pasquale Migliozzi INFN - Napoli

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

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

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

Events with High P T Leptons and Missing P T and Anomalous Top at HERA

NOE, a Neutrino Oscillation Experiment at Gran Sasso Laboratory

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

Neutrino-Nucleus Scattering at MINERvA

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

New Limits on Heavy Neutrino from NA62

Identification of the Higgs boson produced in association with top quark pairs in proton-proton

Application of GLoBES: GLACIER on conventional neutrino beams

The HARP Experiment. G. Vidal-Sitjes (INFN-Ferrara) on behalf of the HARP Collaboration

Detecting ν τ appearance in the spectra of quasielastic CC events

MINOS Oscillation Results from The First Year of NuMI Beam Operation

Neutrino Oscillation Results from MINOS

New Results for ν µ ν e oscillations in MINOS

Physics with Tau Lepton Final States in ATLAS. Felix Friedrich on behalf of the ATLAS Collaboration

Measurement of the baryon number transport with LHCb

New Hadroproduction results from the HARP/PS214 experiment at CERN PS

MINOS experiment at Fermilab

Neutrino interaction systematic errors in MINOS and NOvA

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

Neutrino Oscillations

Heavy Hadron Production and Spectroscopy at ATLAS

Performance of muon and tau identification at ATLAS

arxiv:hep-ex/ v1 19 Jun 2004

arxiv:hep-ex/ v1 15 Oct 2004

Higgs and Z τ + τ in CMS

Lavinia-Elena Giubega

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

Hadronic D Decays and the D Meson Decay Constant with CLEO c

Neutrinos Induced Pion Production in MINERvA

Search for diffuse cosmic neutrino fluxes with the ANTARES detector

Neutrino Cross Sections and Scattering Physics

Results and Status from HARP and MIPP

IceCube Results & PINGU Perspectives

Anti-fiducial Muons in MINOS. Matthew Strait. University of Minnesota for the MINOS collaboration

HARP a hadron production experiment. Emilio Radicioni, INFN for the HARP collaboration

Recent Results from T2K and Future Prospects

Search for heavy BSM particles coupling to third generation quarks at CMS

PoS(ICHEP2016)293. The LArIAT experiment and the charged pion total interaction cross section results on liquid argon. Animesh Chatterjee

Latest results from MINOS

Recent results at the -meson region from the CMD-3 detector at the VEPP-2000 collider

Analysis of muon and electron neutrino charged current interactions in the T2K near detectors

Jet reconstruction in LHCb searching for Higgs-like particles

Transcription:

Results from the OPERA experiment in the CNGS beam A. Paoloni (INFN LNF) on behalf of the OPERA collaboration NUFACT 16 Quy Nhon, 3 August 16 14 physicists, 11 countries, 8 institutions

The OPERA project 1 8 9 9 val o r p Ap l ivi c of d En 4 6 ng ion t c ru ng t i s n con sio s f i m do m n o E C ri e e in g n e 8 Verify the μ oscillation at e det e El the atmospheric m scale. CNGS RUN ro cto 6 9 n ly k ric b s 15 cks i r b appearance event-by-event L = 73 km in an artificial μ beam. 1 Decommissioning Gran Sasso 1 1 1 1 3 1 4 1 5 CNGS RUN st 1 τ h nd τ 3h rd 3 τ μ th 4 τ h th 5 τ h

The detection technique long decays: kink Detect a few CC from ~. 6 kink mm 17 % e - e 18 % h n( ) multi-prong - 5 % + - - n( ) 14 % Modular detector of Emulsion Cloud Chambers (or bricks) Reconciles the needs for: the brick kink the bulk of CC Large mass N ( m) M target Extreme granularity m space resolution 1 X short decays: I.P. Pb

The OPERA experiment ~3o electronics racks BOREXINO Super Module 1 Veto Super Module Target 15k bricks 31 scintill. planes Brick Manipulator System RPC 35 m Muon 1 m Drift tubes Spectrometer m Hybrid apparatus: Emulsions + electronic detectors ``Brick-finding'' + several ancillary facilities off-site : Assembly/disassembly of bricks (LNGS) Brick Manipulator System (LNGS) Labelling and X ray marking (LNGS) Automatised development (LNGS) Scanning of CS doublets (LNGS+JP) Scanning bricks (Europe + JP)

CERN Neutrinos to Gran Sasso The oscillation peak for L= 73 km at ~ 1.5 GeV (similar to NuMI) but the beam is designed to observe leptons: < E > 17 GeV L / < E > 43 km/gev N( )~ Pr( ) x CC(E) x flux Fluxes: ( e+ e ) /.9 % /.1 % prompt (from Ds) negligible Interaction rates (1.8 x 1 pot ): ~ k CC+NC 66.4 CC (not efficiency corrected) Threshold for at ~ 3.5 GeV.

Collected data samples The 5 year long CNGS run has ended in 1. 1.8 x 1 p.o.t. collected 8% of the design (.5 x 1) 1.5 kton initial target mass (15 k bricks) 1955 neutrino interactions in the emulsion targets. Year Days p.o.t. (119) interactions 8 13 1.74 1698 9 155 3.53 3693 1 11 1 tot 187 43 57 965 4.9 4.75 3.86 17.97 448 5131 393 1955 Spectrum of muons from CC events measured in the spectrometers

Brick finding OPERA is a hybrid apparatus. Electronic detectors predictions to locate bricks with neutrino interactions. candidate event Accuracy of predictions by the electronic detectors: position: 1 cm slope: 3 mrad

Brick finding Changeable Sheets: the bridge from the cm scale of electronics detectors to m scale of emulsions. Electronic detector predictions to be confirmed by scanning of CS doublet. Up to 4 bricks ranked in probability are considered for research. candidate event

Vertex location and topology decay search in the brick Tracks in the CS are followed upstream until a stopping point is found. Vertex reconstruction by apposite algorithms. Search of decay topologies (e.g. large impact parameters IP). JHEP 11 (13) 36 Full MC simulation of and 1 samples. Data/MonteCarlo in reasonable agreement.

Validation with the CNGS charm events sample Charmed hadrons produced in CC events ( at the primary vertex) Charm and decays are topologically similar. Test for: reconstruction efficiencies, description of kinematic variables, charm background. 8-1 data sample: 54 ± 4 expected events 5 observed events Eur.Phys.J. C74 (14) 8, 986

candidate identification The brick is a complete stand-alone detector: Neutrino interaction vertex and decay topology reconstruction Measurement of charged particles' momenta by Multiple Coulomb Scattering (-3% resolution) e/ separation and energy measurement Kinematical cuts to increase S/B ratio:.3 GeV/c in presence of in the decay vertex For candidate events, Track Follow Down (TFD) procedure: All reconstructed event tracks followed from brick to brick, to enhance -identification (99%) improve /h discrimination (range measurement and nuclear interaction detection)

background characterization Monte Carlo simulation benchmarked on control samples. In order of decreasing relevance CC with charm production (all channels) IF the primary lepton is not identified and the daughter charge is not (or incorrectly) measured Hadronic interactions Background for h -,e-,e + e+ h+ + D h Large angle muon scattering Background for MC tuned on CHORUS data (cross section and fragmentation functions), validated with measured OPERA charm events. Reduced by ''track follow down'' procedure and large angle scanning FLUKA + pion test beam data Reduced by large angle scanning and nuclear fragment search Measurements in the literature (Lead form factor), improved MC simulations

events observed in OPERA

Fifth candidate: discovery of appearance OPERA - h- Phys. Rev. Lett. 115 (15) 118 VARIABLE VALUE Kink angle (mrad) 9 ± decay length (μm) 634 ± 3 Pry (GeV/c) 11+14-4 Pmisst (GeV/c).3±.1 ϕ (degrees) 151 ± 1

νµ ντ oscillation analysis results Decay channel 1h 3h µ e Total Expected background Charm Had. Re-interaction Large scattering Total.17±.3.17±.3.4±.1.3±.1.±.4.±.6.3±.1.±.1.±.1.±.1.4±.1.17±.3.4±.1.3±.1.5±.5 psum : scalar sum of the momenta of all particles measured in the emulsion films 1, 4, 5: 1h : 3h 3: expected signal events m =.44 1-3 ev Observed events.5±.1.73±.14.61±.1.78±.16.64±.53 3 1 1 5 Probability to be explained by background fluctuation p = 1.1x1-7 No oscillation hypothesis excluded at 5.1 m3 = 3.3 x 1-3 ev with a 9% confidence interval [., 5.] x 1-3 ev (assuming full mixing) Probability of observing 5 candidates (.9 S+B events expected): 17% Frequency of configurations being less probable than the observed one: 6.4%

event with 3 vertices: description Muonless event A primary and two secondary vertices found in emulsion, Electromagnetic activity ( s) at the kink point. Flight lengths: II: 13 m III: 116 m Invariant masses at both secondary vertices larger than 1 GeV.

event with 3 vertices: analysis Vertex can be a charmed particle decay. Vertex III not classified as interaction by standard selection cuts. Dedicated simulations and Artificial Neural Network (ANN) analysis have been performed. Event classified as interaction with charm production (first topology of this kind). 3.5 CL with respect to bkg only hypothesis. In total, less than.1 expected event. More details at ICNFP 16 17

disappearance OPERA Full data sample (8-1) Use of electronic detector data only and separation between CC and NC like events Fit using NC-like/CC-like ratio in which all mixing parameters are fixed to the PDG values but m3 energy deposited in the scintillator planes reweighting MC according to oscillation probability and minimizing between MC and data To reduce systematic effects coming from the beam uncertainty (no near detector), NC like over CC like ratio is used systematics under study Preliminary measurement of m3 consistent with the world average and the internal OPERA appearance results

e oscillation analysis 8-1 Fulls sample (17.97 x 119 p.o.t.): 34 e events observed. Expected number of events: oscillation:.9 ±.4 e A candidate e beam contamination: 36.7 ± 5 Other backgrounds ( e and mis-id): 1. ±.1 preliminary To increase signal/bkg ratio, E<3 GeV cut: 13 observed events for 1.4 ±. events from oscillation e 9. ± 1 events from background Work in progress to extract exclusion limits on sterile neutrino according to 3+1 model.

: preliminary results on sterile 3+1 model standard m41 vs 4 U 4 U 4 = sin ( ) Δ 31 P( )=4 U 3 U 3 sin (normal hierarchy) Δ 41 + 4 U 4 U 4 sin exotic + ℜ [U 4 U 4 U 3 U 3 ]sin Δ 31 sin Δ41 Δ31 4 ℑ[U 4 U 4 U 3 U 3 ]sin sin Δ41 Δ41 Δ 31 +8 ℜ[U 4 U 4 U 3 U 3 ]sin sin Δ 41 + 4 ℑ[U 4 U 4 U 3 U 3 ]sin Δ 31 sin Interference term Δ m ij L Δ = ij E - 9% CL exclusion limit on m41 lowered down to 1- ev for sin(θ ) >.5 - At large m41 : sin(θ ) <.119 at 9% CL Update of JHEP 156 (15) 69

Cosmic rays: R = N /N Highest-E region reached! opposite magnet polarities runs lower systematics Strong reduction of the charge ratio for multiple muon events single 1 Multi- Results compatible with a simple π-k model No significant contribution of the prompt component up to Eμ cos θ * 1 TeV Validity of Feynman scaling in the fragmentation region up to Eμ TeV (EΝ TeV) arxiv.org/abs/143.44 (accepted by Eur. Phys. J. C) Eur. Phys. J. C (14) 74, arxiv.org/abs/143.44

Conclusions 1.8 x 1 pot by CNGS from 8-1 (8% of design). 5 candidates so far with.5 expected background events. No oscillation hypothesis excluded at 5.1 σ. In addition to the standard analysis, observed also a neutrino interaction with charm production. Study on μ e sub-dominant oscillation channel in progress. First results from disappearance analysis shown. Sterile neutrino: limits on Uμ4 Uτ4 from appearance results. Cosmic ray physics: atmospheric in the highest energy region to date.