NuFact02, July 2002, London Takaaki Kajita, ICRR, U.Tokyo For the K2K collab. and JHF-Kamioka WG.

Slides:

Advertisements

Similar presentations

HARP Anselmo Cervera Villanueva University of Geneva (Switzerland) K2K Neutrino CH Meeting Neuchâtel, June 21-22, 2004.

Advertisements

Expected Sensitivity of the NO A  Disappearance Analysis Kirk Bays (Caltech) for the NO A Collaboration April 14, 2013 APS DPF Denver Kirk Bays, APS DPF.

Super-Kamiokande Introduction Contained events and upward muons Updated results Oscillation analysis with a 3D flux Multi-ring events  0 /  ratio 3 decay.

MINERvA Overview MINERvA is studying neutrino interactions in unprecedented detail on a variety of different nuclei Low Energy (LE) Beam Goals: – Study.

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.

T2K neutrino experiment at JPARC Approved since 2003, first beam in April Priorities : 1. search for, and measurement of,   e appearance  sin.

K2K ： KEK-to-Kamioka Long Baseline Neutrino Oscillation Experiment Kenzo NAKAMURA KEK For the K2K Collaboration Les Houches EuroConference on Neutrino.

Near detectors for long baseline neutrino experiments T. Nakaya (Kyoto) 1T. Nakaya.

Neutrino-CH 19 October 2006 Alain Blondel HARP and K2K 1. The K2K experiments 2. beam related uncertainties 3. HARP and results 4. K2K and results 5. conclusions.

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.

Neutrino Study Group Dec 21, 2001 Brookhaven Neutrino Super-BeamStephen Kahn Page 1 Horn and Solenoid Capture Systems for a BNL Neutrino Superbeam Steve.

Status of the OPERA experiment Yoshiaki Nonoyama Nagoya Univ.

10/24/2005Zelimir Djurcic-PANIC05-Santa Fe Zelimir Djurcic Physics Department Columbia University Backgrounds in Backgrounds in neutrino appearance signal.

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.

Atmospheric Neutrino Oscillations in Soudan 2

Expected Sensitivity of the NO A  Disappearance Analysis Kirk Bays (Caltech) for the NO A Collaboration April 14, 2013 APS DPF Denver Kirk Bays, APS DPF.

Recent results from the K2K experiment Yoshinari Hayato (KEK/IPNS) for the K2K collaboration Introduction Summary of the results in 2001 Overview of the.

Present status of oscillation studies by atmospheric neutrino experiments ν μ → ν τ 2 flavor oscillations 3 flavor analysis Non-standard explanations Search.

Current and Near Future Long Baseline Experiments Stéphane T’Jampens CEA Saclay DSM/DAPNIA/SPP.

Status of E391a Search for K L    decay G.Y.Lim IPNS, 32nd ICHEP 19 th August 2004 Beijing.

RECENT RESULTS IN K2K EXPERIMENT Shimpei YAMAMOTO (Kyoto Univ.) 10 th ICEPP 16-FEB-2004 Shimpei YAMAMOTO (Kyoto Univ.) 10 th ICEPP Symposium.

Long Baseline Experiments at Fermilab Maury Goodman.

K2K NC  0 production Shoei NAKAYAMA (ICRR, Univ. of Tokyo) for the K2K Collaboration July 28, NuFact04.

Dec. 13, 2001Yoshihisa OBAYASHI, Neutrino and Anti-Neutrino Cross Sections and CP Phase Measurement Yoshihisa OBAYASHI (KEK-IPNS) NuInt01,

Fermilab, May, 2003 Takaaki Kajita, ICRR, U. Tokyo ・ Introduction ・ JHF-Kamioka neutrino project -overview- ・ Physics in phase-I ・ Phase-II ・ Summary Outline.

Bruno Pontecorvo Pontecorvo Prize is very special for us: All the important works done by Super- Kamiokande point back to Bruno Pontecorvo – 1957 First.

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.

1 The JHF-Kamioka Neutrino experiment 1.Introduction 2.Overview of the experiment 3.Physics sensitivity in Phase-I 4.Physics sensitivity in Phase-II 5.Summary.

Counting Electrons to Measure the Neutrino Mass Hierarchy J. Brunner 17/04/2013 APC.

Atmospheric neutrinos

Kevin McFarland, “  and , oh my” 1 5 July 2002 The Delicate Minutia of Fluxes, Neutrino Cross-Sections, and Detectors Near and Far: Kevin McFarland.

Yoshihisa OBAYASHI, Oct. Neutrino Oscillation Experiment between JHF – Super-Kamiokande Yoshihisa OBAYASHI (Kamioka Observatory, ICRR)

Overview of the KEK Neutrino Beam Facility and its Operation Summary after September 2000 FNAL) K.H. Tanaka for the KEK-PS Beam Channel Group.

A review on the long baseline neutrino experiments Pasquale Migliozzi INFN, Sezione Napoli, Italy.

Measurements of neutrino charged current scattering in K2K Fine-Grained Detector Introduction Introduction K2K Near Detector K2K Near Detector CC interactions.

1 Long Baseline Neutrino Experiment in Japan III International Workshop on “Neutrino Oscillations in Venice” Koichiro Nishikawa Kyoto University February.

Overview of the KEK Neutrino Beam Facility and its Operation Summary after December 2002 (Recovery of SK) K.H. Tanaka for the KEK-PS Beam Channel Group.

Takaaki Kajita, ICRR, Univ. of Tokyo NOW2004, Sep 2004.

Road Map of Neutrino Physics in Japan Largely my personal view Don’t take too seriously K. Nakamura KEK NuFact04 July 30, 2004.

HARP measurements of pion yield for neutrino experiments Issei Kato (Kyoto University) for the HARP collaboration Contents: 1.HARP experiment Physics motivations.

Rencontres de Moriond (6 th March 2005) C. Mariani (INFN Rome) for K2K collaboration March 6 th, XLth Rencontres de Moriond.

1 M. Yokoyama (Kyoto University) for K2K collaboration June 10 th, U.

Neutrino Oscillations at Super-Kamiokande Soo-Bong Kim (Seoul National University)

Accelerator-based Long-Baseline Neutrino Oscillation Experiments Kam-Biu Luk University of California, Berkeley and Lawrence Berkeley National Laboratory.

1 Status of the T2K long baseline neutrino oscillation experiment Atsuko K. Ichikawa (Kyoto univeristy) For the T2K Collaboration.

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.

April 26, McGrew 1 Goals of the Near Detector Complex at T2K Clark McGrew Stony Brook University Road Map The Requirements The Technique.

K2K near detector: Measurement of the  flux in absence of oscillations and of the beam direction 3 different detectors: 1 Kton Water Čerenkov: Small replica.

Cherenkov Tracking Calorimeters D. Casper University of California, Irvine.

Spring school “Bruno Touschek” (19 th May 2005) C. Mariani (INFN Rome) May 19 th, LNF Spring School “ Bruno Touschek ”

1 Translation from Near to Far at K2K T.Kobayashi IPNS, KEK for K2K beam monitor group (K.Nishikawa, T.Hasegawa, T.Inagaki, T.Maruyama, T.Nakaya,....)

Review of experimental results on atmospheric neutrinos Introduction Super-Kamiokande MACRO Soudan 2 Summary Univ. of Tokyo, Kamioka Observatory.

Neutrino Interaction measurement in K2K experiment (1kton water Cherenkov detector) Jun Kameda(ICRR) for K2K collaboration RCCN international workshop.

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.

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.

T2K Oscillation Strategies Kevin McFarland (University of Rochester) on behalf of the T2K Collaboration Neutrino Factories 2010 October 24 th 2010.

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.

K2K and JHF-nu muon monitor Jun Kameda (KEK) 1. K2K muon monitor 2. JHF-ν muon monitor 3. Summary International workshop on Neutrino Beam Instrumentation,

T2K : New physics results

K2K and JHF-nu muon monitor

Status of the OPERA experiment

F.Sánchez for the K2K collaboration UAB/IFAE

Neutrino interaction measurements in K2K SciBar

Toward realistic evaluation of the T2KK physics potential

Impact of neutrino interaction uncertainties in T2K

Presentation transcript:

NuFact02, July 2002, London Takaaki Kajita, ICRR, U.Tokyo For the K2K collab. and JHF-Kamioka WG

K2K near detector system Basic idea for JHF near detectors Summary Outline

Bird’s Eye Neutrino Beam Line 200m Front (Near) Detector K2K

K2K near detector flux and direction 312 ton (1ev / 20spills) 6 ton25 tonFid. Vol.: (MRD) (SciFi) (1Kton) 300m from the target

Beam direction? (MRD) profile x profile center x (cm) profile center y (cm) June 99 Apr. 01  1mrad (0.5GeV < Eμ < 1.0GeV) (1.0GeV < Eμ < 2.5GeV) ±3-4 mrad. accuracy required.

Role of the SciFi detector p μ SciFi MRD Max osc. Fraction of non-quasi-elastic events must be understood well.

1kton water Cherenkov detector Predict the Super-Kamiokande flux. Overall normalization error on Nsk for Nov99~ Error (%) KTon±4.4 SK±3.0 Flux+3.7  3.4 Far/Near+5.6  7.3 NC/CC+0.2  0.3 nQE/QE+0.5  0.8 others±0.7 Total+8.6  9.7 KTon: dominated by fid vol error SK: similar to Kton. List of uncertainties: ⇒ energy scale ⇒ FC event selection ⇒ Particle ID ⇒ Ring counting ⇒ Fiducial volume ⇒ Angular resolution ⇒ Threshold ⇒ Events θ > 90 degree.

K2K near detector upgrade Full Active (solid) Scintillator Tracker »High efficiency for a short (<4cm) track. »Detect a proton down to 350 MeV/c. »PID (p/π) by dE/dx and momentum »Fine segments (1.3×2.5×300cm ). 14,400 channels Monte Carlo μ p 3m 1.8m Δm 2 =3×10 -3 eV 2 Eν=600MeV. Lower energy ν interactions should be studied. 45, pot

JHF near detectors 280m First near from the target Target Second near ～ 2km from the target Decay pipe (L=130m) ν

Required accuracy Discovery of non-zero θ 13 Precise measurement of θ 23 and Δm. CP violation JHF-Phase IJHF-Phase II (with Hyper-K) 2 5% 2% ★ Main near detector should be water Ch. ★ Near detector pos. must be >1.5km. Flux detector

Some information on the beam…. Number of events /100MeV/yr Eν(GeV) Max. osc. (must be predicted accurately) Background (must be understood well)

Event rate & Far/near ratio Distance from target (km) Water Cherenkov : (Total mass > 100 tons) ( φ far / φ near )×(L far / L near ) Not a good place…. OK ! 0123 E ν (GeV)

Near Beam profile monitor Cannot be water Cherenkov Detailed study of neutrino No detailed design….., but could be something like: ・・・・ 10m ? 0 deg. Super-K ※ This profile is obsolete… Just to give the idea….

Near Details : not designed yet 9.2m φ 15.2m 8m 4m Total mass : 1000ton Fid. Mass : 100ton ν beam Fine grained scintillater detector 5m 8m Water Cherenkov detector Muon detector

Stopping point distribution of muons ν Edge of the fid vol. 2m 4m Detector surface Measured by muon detector

The detector should look like…. Water Ch. Scintillator detector Muon counter Surface building

Summary Multi component K2K near detector system is essential to understand the neutrino beam and interactions. In the JHF-Kamioka neutrino project, the near detector system should be similar to the K2K system. However, in JHF, the distance between the target and the near detector should be > 2km.

End

Beam energy stability ? (MRD, 1Kton) Every month E μ (GeV) MRD1Kton P μ (GeV/c)