Current Status of the T2K Experiment Ryan Terri (for the T2K Collaboration) 31 May – 4 June 2010 Planck 2010, CERN.

Slides:



Advertisements
Similar presentations
Neutrino Oscillation Appearance with OPERA Amina ZGHICHE Oscillation Project with Emulsion tRacking Apparatus.
Advertisements

First Neutrino Oscillation Results from T2K Costas Andreopoulos STFC, Rutherford Appleton Lab.
11-September-2005 C2CR2005, Prague 1 Super-Kamiokande Atmospheric Neutrino Results Kimihiro Okumura ICRR Univ. of Tokyo ( 11-September-2005.
Super-Kamiokande Introduction Contained events and upward muons Updated results Oscillation analysis with a 3D flux Multi-ring events  0 /  ratio 3 decay.
G. Sullivan - Princeton - Mar 2002 What Have We Learned from Super-K? –Before Super-K –SK-I ( ) Atmospheric Solar –SNO & SK-I Active solar –SK.
J-PARC PAC ‘07 Imperial College/RAL Dave Wark Status of the T2K Experiment Dave Wark Imperial/RAL J-PARC PAC KEK July 6, 2007.
T2K – Canada Accelerator & Detector Status D. Karlen University of Victoria & TRIUMF ACOT meeting, May 12, 2007.
Sinergia strategy meeting of Swiss neutrino groups Mark A. Rayner – Université de Genève 10 th July 2014, Bern Hyper-Kamiokande 1 – 2 km detector Hyper-Kamiokande.
Performance of a Water Cherenkov Detector for e Appearance Shoei NAKAYAMA (ICRR, University of Tokyo) November 18-19, 2005 International Workshop on a.
CHIPP 2 October 2006 Alain Blondel HARP-K2K-T2K 1. The K2K and T2K experiments 2. beam related uncertainties 3. HARP and results 4. K2K and results 5.
T2K experiment at J-PARC Epiphany 2010D. Kiełczewska1 For T2K Collaboration Danuta Kiełczewska Warsaw University & Sołtan Institute for Nuclear Studies.
New results from K2K Makoto Yoshida (IPNS, KEK) for the K2K collaboration NuFACT02, July 4, 2002 London, UK.
1 Indications of Electron Neutrino Appearance at T2K Melanie Day University of Rochester On Behalf of the T2K Collaboration 9/20/11.
1 Tokai 2 Kamioka Status and Prospects Antonin Vacheret for the T2K Collaboration Tuesday 7th September NOW 2010, Otranto, Lecce, Italy.
First Anti-Neutrino Oscillation Results from the T2K Experiment
1 V. Antonelli, G. Battistoni, P. Ferrario 1, S. Forte (Università degli Studi di Milano e I.N.F.N. Sezione di Milano and 1 University of Valencia) Standard.
5/1/20110 SciBooNE and MiniBooNE Kendall Mahn TRIUMF For the SciBooNE and MiniBooNE collaborations A search for   disappearance with:
Recent results from the K2K experiment Yoshinari Hayato (KEK/IPNS) for the K2K collaboration Introduction Summary of the results in 2001 Overview of the.
The Earth Matter Effect in the T2KK Experiment Ken-ichi Senda Grad. Univ. for Adv. Studies.
Q&A on T2K construction of beam line near detectors budget collaboration (contribution from each) T2KK.
Dec. 13, 2001Yoshihisa OBAYASHI, Neutrino and Anti-Neutrino Cross Sections and CP Phase Measurement Yoshihisa OBAYASHI (KEK-IPNS) NuInt01,
Fermilab Neutrino Program Jim Strait Neutrino Discussion at CERN 26 November 2013.
Fermilab, May, 2003 Takaaki Kajita, ICRR, U. Tokyo ・ Introduction ・ JHF-Kamioka neutrino project -overview- ・ Physics in phase-I ・ Phase-II ・ Summary Outline.
The NOvA Experiment Ji Liu On behalf of the NOvA collaboration College of William and Mary APS April Meeting April 1, 2012.
Bruno Pontecorvo Pontecorvo Prize is very special for us: All the important works done by Super- Kamiokande point back to Bruno Pontecorvo – 1957 First.
TAUP Searches for nucleon decay and n-n oscillation in Super-Kamiokande Jun Kameda (ICRR, Univ. of Tokyo) for Super-Kamiokande collaboration Sep.
1 DISCOVERY OF ATMOSPHERIC MUON NEUTRINO OSCILLATIONS Prologue First Hint in Kamiokande Second Hint in Kamiokande Evidence found in Super-Kamiokande Nov-12.
JHF-Kamioka Neutrino Oscillation Experiment using JHF 50 GeV PS Y.Itow ICRR,Univ.of Tokyo Jul27,2002 Jul27,2002 ICHEP02 Amsterdam Introduction Facility.
Preliminary Results from the MINER A Experiment Deborah Harris Fermilab on behalf of the MINERvA Collaboration.
DOE Review 3/18/03Steve Brice FNALPage 1 MiniBooNE Status Steve Brice Fermilab Overview Beam – Primary Beam – Secondary Beam Detector – Calibration – Triggering.
Yoshihisa OBAYASHI, Oct. Neutrino Oscillation Experiment between JHF – Super-Kamiokande Yoshihisa OBAYASHI (Kamioka Observatory, ICRR)
1 Long Baseline Neutrino Experiment in Japan III International Workshop on “Neutrino Oscillations in Venice” Koichiro Nishikawa Kyoto University February.
NuFact02, July 2002, London Takaaki Kajita, ICRR, U.Tokyo For the K2K collab. and JHF-Kamioka WG.
Takaaki Kajita, ICRR, Univ. of Tokyo NOW2004, Sep 2004.
Search for Sterile Neutrino Oscillations with MiniBooNE
Neutrino Oscillations at Super-Kamiokande Soo-Bong Kim (Seoul National University)
Michel Gonin – Ecole Polytechnique – France : SUPER NOVA SN1987A Super-Kamiokande Introduction neutrino oscillations mixing matrices Introduction.
Medium baseline neutrino oscillation searches Andrew Bazarko, Princeton University Les Houches, 20 June 2001 LSND: MeVdecay at rest MeVdecay in flight.
Accelerator-based Long-Baseline Neutrino Oscillation Experiments Kam-Biu Luk University of California, Berkeley and Lawrence Berkeley National Laboratory.
MiniBooNE MiniBooNE Motivation LSND Signal Interpreting the LSND Signal MiniBooNE Overview Experimental Setup Neutrino Events in the Detector The Oscillation.
1 Status of the T2K long baseline neutrino oscillation experiment Atsuko K. Ichikawa (Kyoto univeristy) For the T2K Collaboration.
2 July 2002 S. Kahn BNL Homestake Long Baseline1 A Super-Neutrino Beam from BNL to Homestake Steve Kahn For the BNL-Homestake Collaboration Presented at.
Recent Results from Super-K Kate Scholberg, Duke University June 7, 2005 Delphi, Greece.
T2K Status Report. The Accelerator Complex a Beamline Performance 3 First T2K run completed January to June x protons accumulated.
CP phase and mass hierarchy Ken-ichi Senda Graduate University for Advanced Studies (SOKENDAI) &KEK This talk is based on K. Hagiwara, N. Okamura, KS PLB.
April 26, McGrew 1 Goals of the Near Detector Complex at T2K Clark McGrew Stony Brook University Road Map The Requirements The Technique.
Cherenkov Tracking Calorimeters D. Casper University of California, Irvine.
NUMI NUMI/MINOS Status J. Musser for the MINOS Collatoration 2002 FNAL Users Meeting.
Recent Results from T2K Jonathan Perkin on behalf of the T2K collaboration.
Measuring Neutrino Oscillations with the T2K Experiment Alfons Weber University of Oxford STFC/RAL Dec-2011.
T2K: ND280 status, progress, and plans Steven Dytman, (Vittorio Paolone) University of Pittsburgh (Representing the T2K collaboration) NUFACT10 XII International.
XLVth Rencontres de Moriond Status of the T2K experiment K. Matsuoka (Kyoto Univ.) for the T2K collaboration Contents Physics motivations (neutrino oscillation)
Hiroyuki Sekiya ICHEP2012 Jul 5 The Hyper-Kamiokande Experiment -Neutrino Physics Potentials- ICHEP2012 July Hiroyuki Sekiya ICRR,
Status of the NO A Experiment Kirk Bays (Caltech) on behalf of the NO A collaboration Lake Louise Winter Institute Saturday, Feb 22, 2014.
Neutrino Interaction measurement in K2K experiment (1kton water Cherenkov detector) Jun Kameda(ICRR) for K2K collaboration RCCN international workshop.
Observation Gamma rays from neutral current quasi-elastic in the T2K experiment Huang Kunxian for half of T2K collaboration Mar. 24, Univ.
T2K neutrino oscillation results Kei Ieki for the T2K collaboration Lake Louise Winter Institute 2014/2/22 1 ν T okai K amioka.
 CC QE results from the NOvA prototype detector Jarek Nowak and Minerba Betancourt.
T2K Experiment Results & Prospects Alfons Weber University of Oxford & STFC/RAL For the T2K Collaboration.
Status of Super-Kamiokande, K2K and JHF ACFA LC Yuichi Oyama (KEK) for Super-Kamiokande collaboration, K2K collaboration and JHF collaboration.
Precision Measurement of Muon Neutrino Disappearance with T2K Alex Himmel Duke University for the The T2K Collaboration 37 th International Conference.
Recent Results from the T2K ND280 detector Jonathan Perkin on behalf of the T2K collaboration KAMIOKA TOKAI 295 km.
T2K Oscillation Strategies Kevin McFarland (University of Rochester) on behalf of the T2K Collaboration Neutrino Factories 2010 October 24 th 2010.
NNN 2011: The d Experiment Joshua Albert Duke University For the T2K Collaboration November 8, 2011.
The XXII International Conference on Neutrino Physics and Astrophysics in Santa Fe, New Mexico, June 13-19, 2006 The T2K 2KM Water Cherenkov Detector M.
Neutral Current Interactions in MINOS Alexandre Sousa, University of Oxford for the MINOS Collaboration Neutrino Events in MINOS Neutrino interactions.
T2K : New physics results
Naotoshi Okamura (YITP) NuFact05
Toward realistic evaluation of the T2KK physics potential
Impact of neutrino interaction uncertainties in T2K
Presentation transcript:

Current Status of the T2K Experiment Ryan Terri (for the T2K Collaboration) 31 May – 4 June 2010 Planck 2010, CERN

The T2K Experiment 日本 Japan 295 km ND280 INGrid 2Terri, Planck 2010, T2K Status 12 countries (Canada, France, Germany, Italy, Japan, Korea, Poland, Russia, Spain, Switzerland, UK, USA) 62 institutes ~500 collaborators Super-Kamiokande

Neutrino Oscillations Solar & reactor Atmospheric & accelerator Reactor & accelerator  23 = 37˚ ~ 53˚  m 23 2 ≈ 2.4 x 10 –3 eV 2  12 ≈ 34.4˚±1.3˚  m 12 2 ≈ 8 x 10 –5 eV 2  13 < 10˚ by CHOOZ In 1998, Super-Kamiokande reports neutrinos have mass*, which is the first physics beyond the Standard Model Flavor eigenstates are not the same as mass eigenstates *Super-Kamiokande Collaboration, PRL 81, 1562 (1998) 3Terri, Planck 2010, T2K Status L [km] E [GeV]  m 2 [eV 2 ] 2 flavor approximation

T2K Oscillation Physics Goals Precision measurement of atmospheric neutrino oscillation parameters – Is  23 maximal? First measurement of  13 – … or at least best limit – If we can measure  13, what is  CP ? 2.4 x (0.75 MW beamx5x10 7 s) sin²2θ 12 = sin²2θ 23 = 1.0 ∆m² 12 = 7.6x10-5eV² δ CP =0 4 Terri, Planck 2010, T2K Status l p l ll Select CCQE-enhanced samples: single Cherenkov ring that’s muon-like for disappearance or e-like for appearance (with additional cuts for larger S/B)  Super-K event display Sharp edge e Fuzzy ring Background constraints on sterile neutrino searches Investigate neutrino mass hierarchy Is U MNS unitary? CCQE

J-PARC Beamline 1: 181 MeV LINAC 2: 3 GeV Synchrotron (RCS) 6: 30 GeV Main Ring 6 bunches w/ 581 ns between each bunch 0.3 Hz rep rate 3: Neutrino Beamline & Target Station – Carbon target encased in first of 3 magnetic horns which currently operate at 250 kA – Muon monitor at end of 110 m decay volume 4: The Pit – 280 m downstream of target – Houses on- and off-axis Near Detectors 5 within 1 mrad of off-axis angle Currently receiving 50 kW of beam power Towards SK Terri, Planck 2010, T2K Status

Neutrino Beam Flux Off-axis angle of 2.5 o Beam closer to being monoenergetic Suppressed high energy tail Higher intensity in region of interest Fewer non-CCQE interactions 6Terri, Planck 2010, T2K Status     Off-axis beam

On-Axis Near Detector (INGRID) Monitors beam direction and flux with ~1-day statistics using beam profile Can see beam bunch structure 7Terri, Planck 2010, T2K Status

The Off-Axis Detector 8 01:57 JST, Feb. 5, 2010 P0D TPC1TPC2TPC3 FGD1FGD2DSECAL beam beam Magnet on (0.188 T) Still undergoing calibration Rest of ECAL to be installed this summer beam directionmagnet open Measure neutrino flux and cross section UA1 Magnet 0.2 T field Includes a water target in P0D and FGD2 Understand interactions at SK Tracker Region: Fine Grained Detectors (FGDs) & TPCs Particle Tracking (p,  ) & identification P0D Measure NC  0 rate ECAL (Downtream Currently Installed) Surrounds tracker and P0D Capture EM energy SMRD Muon ranging instrumentation in the magnet yoke Terri, Planck 2010, T2K Status

Super-Kamiokande 50 kton water Cherenkov detector Located in the Japanese Alps in Western Japan 22.5 kton fiducial volume ” Inner Detector (ID) PMTs, 39% photo- coverage ” Outer Detector (OD) PMTs w/ WLS Plates New electronics installed and taking data successfully 42 m 39 m 9Terri, Planck 2010, T2K Status

Blasting Current # of Candidate Events for T2K Oscillation Analyses ClassR29R30 TotalExp. BG T2K-FC e-03 T2K-FC + FV + E visible >30 MeV e-04 T2K-OD For 3.4x10 18 POT: 10Terri, Planck 2010, T2K Status >99% livetime Event rate cross check: Accidental flash events due to work at SK tank. (1hour SK dead) (1day binning) Fitted 581ns-interval bunch position Bunch structure is observed for SK FCFV events and OD events

Summary/Outlook T2K is a long-baseline neutrino oscillation experiment – Will make precision measurement of the atmospheric neutrino oscillation parameters – From January 2010, started  → e search – Use these measurements as stepping stone for more exotic neutrino model searches T2K is currently collecting data and will through June – Will resume in Fall 2010 – Beam now achieves over 50 kW of power Try continuous operation at >100 kW after summer shutdown – Near Detector is seeing events consistent with beam Some commissioning still to be done for off-axis detector – SK has seen its first potential events for an oscillation analysis Initial results expected later on this year 11Terri, Planck 2010, T2K Status

A Possible Interpretation of Physics Beyond the Standard Model: “There is a theory which states that if ever anyone discovers exactly what the Universe is for and why it is here, it will instantly disappear and be replaced by something even more bizarre and inexplicable. There is another theory which states that this has already happened.” -Douglas Adams, Hitchhiker’s Guide to the Galaxy 12Terri, Planck 2010, T2K Status

SUPPLEMENTARY SLIDES 13Terri, Planck 2010, T2K Status

T2K Sensitivity to  13 after 5 years of nominal data taking Terri, Planck 2010, T2K Status MW beam x 5 yr x 10 7 s/yr, sin²2θ 12 = , sin²2θ 23 = 1.0, ∆m² 12 = 7.6x10-5eV², δ CP =0

Neutrino Beamline & Planned Upgrades for Increased Intensity New kicker magnet to be installed Increase # of bunches in proton beam from 6 to 8 Increase rep rate & # of protons/bunch Terri, Planck 2010, T2K Status15 INGRID ND280 Beam dump  monitor Target & horns Main Ring

First Event Candidate At Super-K Terri, Planck 2010, T2K Status16 Fully Contained, in the fiducial volume (FCFV) 2 showering rings: invariant mass = 133 MeV/c 2 momentum = 148 MeV/c Feb. 24, 2010  view

SK sub-GeV Decay Electron Detection Efficiency Terri, Planck 2010, T2K Status17 SK-IV dataSK-III data Decay curve (calculation) Ndecay-e=1 88.7%72.6% Decay curve (calculation) Ndecay-e=1 Preliminary