Similar documents
Perspectives of neutrino oscillation physics with long baseline beams

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

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

arxiv: v1 [hep-ex] 1 Oct 2015

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

Results from the OPERA experiment in the CNGS beam

Results from the OPERA experiment in the CNGS beam

The CNGS project. Pasquale Migliozzi INFN - Napoli

The CERN-Gran Sasso Neutrino Program

RECENT RESULTS FROM THE OPERA EXPERIMENT

arxiv: v1 [hep-ex] 11 May 2013

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

Latest results of OPERA

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

K2K and T2K experiments

Tau-neutrino production study in 400 GeV proton interactions

The OPERA Experiment

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

FIRST NEUTRINO EVENTS IN THE OPERA EMULSION TARGET

Status of the OPERA experiment

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

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

- ICARUS status and near future

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

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

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

Neutrino Experiments: Lecture 2 M. Shaevitz Columbia University

Long Baseline Neutrino Experiments

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

Performance of the ICARUS T600 detector

First results and status of the OPERA experiment

Results from the OPERA experiment at the CNGS beam

Neutrino Oscillations

Neutrino Oscillations Physics at DUNE

Detector Basics III. Mark Messier Indiana University. Neutrino Summer School Fermilab July 9, 2008

ICARUS T600 experiment: latest results and perspectives

Long Baseline Neutrinos

MINOS. Physics Program and Construction Status. Karol Lang The University of Texas at Austin. YITP: Neutrinos and Implications for Physics Beyond

Neutrino physics with the SHiP experiment at CERN

Hadron Production Experiments and Neutrino Beams

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

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

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

arxiv:hep-ex/ v1 19 Jun 2004

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

The ICARUS Project FRONTIERS IN CONTEMPORARY PHYSICS II. Vanderbilt University, March 5-10, Sergio Navas (ETH Zürich) " Atmospheric neutrinos

Neutrino Oscillations

The CNGS neutrino beam

MiniBooNE Progress and Little Muon Counter Overview

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

Why understanding neutrino interactions is important for oscillation physics

HARP (Hadron Production) Experiment at CERN

From Here to a Neutrino Factory: Neutrino Oscillations Now and Again

BNL Very Long Baseline Neutrino Oscillation Expt.

The SHiP experiment and its detector for neutrino physics

Today: Part I: Neutrino oscillations: beam experiments. Part II: Next tutorials: making distributions with histograms and ntuples

Physics Projects for a Future CERN LNGS Neutrino Programme

Recent T2K results on CP violation in the lepton sector

2 ATLAS operations and data taking

Status of the LHCb Experiment. Ueli Strauman, University of Zurich, Switzerland. Sept. 13, 2001

Neutrino Cross Section Measurements for Long-Baseline Acceleratorbased Neutrino Oscillation Experiments

NOE, a Neutrino Oscillation Experiment at Gran Sasso Laboratory

Particle Detectors. Summer Student Lectures 2007 Werner Riegler, CERN, History of Instrumentation History of Particle Physics

Particle production vs. energy: how do simulation results match experimental measurements?

Atmospheric Neutrinos MINOS MINOS Far Detector Type of Atmospheric Neutrinos at MINOS Two MINOS Atmospheric Analyses.

Neutrino-Nucleus Scattering at MINERvA

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

Indication of ν µ ν e appearance in the T2K EXPERIMENT

Neutrino Detectors for future facilities - III

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

Neutrino Nucleus Deep Inelastic Scattering at MINERvA

Conventional neutrino experiments

Observation of tau neutrino interactions

Jonathan Asaadi Syracuse University

Sensitivity of the DUNE Experiment to CP Violation. Lisa Whitehead Koerner University of Houston for the DUNE Collaboration

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

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

Existing and future long-baseline neutrino oscillation experiments

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

Hadronic vs e + e - colliders

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

First neutrino beam and cosmic tracks. GDR neutrino

Neutrinos & the MINOS Experiment

Application of GLoBES: GLACIER on conventional neutrino beams

Experimental Search for the Decay

Accelerator neutrino experiments

Results From The HARP Experiment

Experimental results on the atmospheric muon charge ratio

New Results for ν µ ν e oscillations in MINOS

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

Muon Alignment at CMS

A NEW TECHNIQUE FOR DETERMINING CHARGE AND MOMENTUM OF ELECTRONS AND POSITRONS USING CALORIMETRY AND SILICON TRACKING. Qun Fan & Arie Bodek

Particle Identification: Computer reconstruction of a UA1 event with an identified electron as a candidate for a W >eν event

BNL Very Long Baseline Neutrino Oscillation Expt.

Neutrino Energy Reconstruction Methods Using Electron Scattering Data. Afroditi Papadopoulou Pre-conference, EINN /29/17

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

Neutrinos Induced Pion Production in MINERvA

Review of νe Appearance Oscillation Experiments

Recent Results from Alysia Marino, University of Colorado at Boulder Neutrino Flux Workshop, University of Pittsburgh, Dec 6 8,2012

Transcription:

Detectors at (1994-1998) CHORUS NOMAD Roberto Petti Neutrino beam

NETSCAN location (Phase II): Pick up all track segments (θ < 0.4 rad) in the scanning volume (1.5 x 1.5 mm 2 8 plates) Offline analysis of emulsion data At least 2-segment connected tracks Reconstruct full vertex topology Track segments from 8 plates overlapped Eliminate passingthrough tracks Roberto Petti

Automatic microscope at : Megapixel CCD and XYZ stage 71 cm High Performance optics 36 cm Roberto Petti

MOTIVATIONS FOR CNGS n m disappearance in Super-K: SuperK n m - n t 1.2 < Dm 2 < 5.4 x 10-3 ev 2 at 90% CL 1.0 7.0 99% Best fit Dm 2 = 2.4 x 10-3 ev 2 n m disappearance in K2K: Expected (no osc.) 80.6 + 7.3-8.0 Detected 56 (~ 2s effect) Oscillation dip in the E ν spectrum at m 2 ~ 3 x 10-3 ev 2? n t appearance in Super-K Poor S/B ratio ~ 0.7%, statistical significance ~ 2s Roberto Petti Sterile ν disfavoured at ~ 99% events K2K? n energy (GeV)

CNGS status: civil engineering Roberto Petti

CNGS status: schedule today Roberto Petti

THE OPERA DETECTOR n supermodule m spectrometer Magnetised Iron Dipoles Drift tubes and RPCs ~ 10 m brick (56 Pb/Em. cells ) module 8 cm (10X 0 ) n target and t decay detector Each supermodule is a sequence of 24 modules consisting of - a wall of Pb/emulsion bricks Roberto Petti - two planes of orthogonal scintillator strips brick wall scintillator strips 235,000 bricks

Status of the experiment Approved as CNGS1 in 2000 Construction & test of full-scale prototypes completed Target tracker module Wall support structure Starting final construction Roberto Petti Magnet during construction

THE DONUT BENCHMARK ν τ has been detected in the DONUT ECC t hadron 1mm Fe plate Emulsion film Structure: OPERA ECC = DONUT ECC Material : Lead Iron Better performance for physics analysis Test for the OPERA technology Roberto Petti

Long decay topology: Long decays Search for a kink with an angle q kink > 20 mrad leptonic channels hadronic channels t fi e, m t fi h, r kink P q kink Require large P T = P*q kink at 2ry vtx. leptonic channels > 100, 250 Mev/c hadronic channels > 600, 300 Mev/c n m NC t Additional kinematic cuts at 1ry vtx. for the hadronic channels F t-h > p/2 P t miss < 1 GeV/c 1 t p/2 n m NC Φ τ-h P t miss (GeV/c) Roberto Petti

Short decay topology: emulsion film plastic base At least two additional 1ry tracks for vertex reconstruction P > 1.0 GeV/c I.P. Pb P Require a large impact parameter I.P. > 5 to 20 mm Short decays leptonic channels t fi e, m Signal Additional kinematic cuts on minimal mass/p T for n e CC/charm rejection (P T ) min > 50 Mev/c t fi e (M inv ) min > 3 GeV/c t fi m 80% 0.2% Background Roberto Petti Mass (GeV/c 2 )

Experimental sensitivity (5 years, 1.8kt): 90 % CL upper limit obtained on average by a large ensemble of experiments, in the absence of signal events Dm 2 < 1.2x10-3 ev 2 at full mixing sin 2 (2q) < 5.7x10-3 at large Dm 2 Uncertainties on background (±33%) and on efficiencies (±15%) included Roberto Petti

Probability of ns significance: Schematic view of the Super-K allowed region Simulate a large number of experiments with oscillation parameters generated according to the Super-K probability distribution Dm 2 22% 68% 9% N ns events are required for a ns significance Evaluate the fraction P ns of experiments observing N ns events sin 2 2q N 4s = 6 Run P 3s (%) P 4s (%) 3 y 88 82 P 4s 5 y 96 90 1 10 100 Distribution of events observed Roberto Petti

THE ICARUS DETECTOR Basic element T600 LAr modules (TPC) Proposed baseline T600 + 2 * T1200 (3000 t) electronics, cooling, etc. T1200 T1200 T600 Cross section Roberto Petti T600 First T600 constructed and tested

THE T600 DETECTOR View of the inner detector 4 m 4 m 20 m LAr Cryostat (half-module) Roberto Petti

2 Data from T600 Drift coord. (m) 1 Full 2D View from the Collection Wire Plane 3 2 2 4 6 Wire coord. (m) 12 18 1 2 El.m. shower Zoom views 2 m stop and decay in e Run 201 - Evt 12 3 Roberto Petti El.m. shower Detail of a long (14 m) m track with d-ray spots

2 Drift Coord. (m) Full 2D view from the Collection Wire Plane 2 4 6 Wire coord. (m) 12 18 Zoom View 3.9 m 1.3 m Run 308 - Evt 7 Roberto Petti Large el.m. shower