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

Slides:



Advertisements
Similar presentations
Recent Discoveries in Neutrino Physics: Understanding Neutrino Oscillations 2-3 neutrino detectors with variable baseline 1500 ft nuclear reactor Determining.
Advertisements

A long-baseline experiment with the IHEP neutrino beam Y. Efremenko detector Presented by.
Super-Kamiokande Introduction Contained events and upward muons Updated results Oscillation analysis with a 3D flux Multi-ring events  0 /  ratio 3 decay.
T2K neutrino experiment at JPARC Approved since 2003, first beam in April Priorities : 1. search for, and measurement of,   e appearance  sin.
Performance of a Water Cherenkov Detector for e Appearance Shoei NAKAYAMA (ICRR, University of Tokyo) November 18-19, 2005 International Workshop on a.
F.Sanchez (UAB/IFAE)ISS Meeting, Detector Parallel Meeting. Jan 2006 Low Energy Neutrino Interactions & Near Detectors F.Sánchez Universitat Autònoma de.
Reactor & Accelerator Thanks to Bob McKeown for many of the slides.
Alain Blondel Detectors UNO (400kton Water Cherenkov) Liquid Ar TPC (~100kton)
Background Understanding and Suppression in Very Long Baseline Neutrino Oscillation Experiments with Water Cherenkov Detector Chiaki Yanagisawa Stony Brook.
Superbeam long baseline experiments Takashi Kobayashi KEK Neutrino Summer
Neutrino Study Group Dec 21, 2001 Brookhaven Neutrino Super-BeamStephen Kahn Page 1 Horn and Solenoid Capture Systems for a BNL Neutrino Superbeam Steve.
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.
Future Accelerator-based Oscillation Experiment (JHFnu, Off-axis) Changgen Yang Institute of High Energy Physics Beijing.
JHF2K neutrino beam line A. K. Ichikawa KEK 2002/7/2 Overview Primary Proton beamline Target Decay Volume Strategy to change peak energy.
Sampling Detectors for e Detection and Identification Adam Para, Fermilab NuFact02 Imperial College Interest de jour: what is sin 2 2  13  oscillations.
Future Accelerator Based Neutrino Experiments Takashi Kobayashi Institute of Particle and Nuclear Studies, High Energy Accelerator Research Organization.
Neutrino Oscillation Detectors: a (Re?)View Where we are? Where are we going? How do we get there? More questions than answers Adam Para, Fermilab NuFact.
Recent results from the K2K experiment Yoshinari Hayato (KEK/IPNS) for the K2K collaboration Introduction Summary of the results in 2001 Overview of the.
Resolving neutrino parameter degeneracy 3rd International Workshop on a Far Detector in Korea for the J-PARC Neutrino Beam Sep. 30 and Oct , Univ.
The Earth Matter Effect in the T2KK Experiment Ken-ichi Senda Grad. Univ. for Adv. Studies.
Douglas Michael California Institute of Technology NuFACT 03 June 5, 2003 What’s a Super Beam? The Physics Some of the common features Specific Proposals.
Apr. 4, KEK JHF-SK neutrino workshop 1 e appearance search Yoshihisa OBAYASHI (KEK - IPNS)
Sterile Neutrino Oscillations and CP-Violation Implications for MiniBooNE NuFact’07 Okayama, Japan Georgia Karagiorgi, Columbia University August 10, 2007.
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.
1 Super muon-neutrino beam Takashi Kobayashi IPNS, KEK Fact02 July 1, 2002 Imperial College London Contents 1.Introduction 2.“Super-beam” long baseline.
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.
Long Baseline Neutrino Beams and Large Detectors Nicholas P. Samios Istanbul, Turkey October 27, 2008.
Counting Electrons to Measure the Neutrino Mass Hierarchy J. Brunner 17/04/2013 APC.
Hyper-Kamiokande project and R&D status Hyper-K project Motivation Detector Physics potential study photo-sensor development Summary Kamioka.
Yoshihisa OBAYASHI, Oct. Neutrino Oscillation Experiment between JHF – Super-Kamiokande Yoshihisa OBAYASHI (Kamioka Observatory, ICRR)
Search for Electron Neutrino Appearance in MINOS Mhair Orchanian California Institute of Technology On behalf of the MINOS Collaboration DPF 2011 Meeting.
A review on the long baseline neutrino experiments Pasquale Migliozzi INFN, Sezione Napoli, Italy.
1 Long Baseline Neutrino Experiment in Japan III International Workshop on “Neutrino Oscillations in Venice” Koichiro Nishikawa Kyoto University February.
1 Recent Results from Neutrino Experiments and Plans for the Neutrino Super Beam in Japan Discovery of neutrino oscillations  finite neutrino masses (
NuFact02, July 2002, London Takaaki Kajita, ICRR, U.Tokyo For the K2K collab. and JHF-Kamioka WG.
Road Map of Neutrino Physics in Japan Largely my personal view Don’t take too seriously K. Nakamura KEK NuFact04 July 30, 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.
1 Constraining ME Flux Using ν + e Elastic Scattering Wenting Tan Hampton University Jaewon Park University of Rochester.
MiniBooNE MiniBooNE Motivation LSND Signal Interpreting the LSND Signal MiniBooNE Overview Experimental Setup Neutrino Events in the Detector The Oscillation.
Low Z Detector Simulations
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.
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.
Search for active neutrino disappearance using neutral-current interactions in the MINOS long-baseline experiment 2008/07/31 Tomonori Kusano Tohoku University.
PAC questions and Simulations Peter Litchfield, August 27 th Extent to which MIPP/MINER A can help estimate far detector backgrounds by extrapolation.
Hiroyuki Sekiya ICHEP2012 Jul 5 The Hyper-Kamiokande Experiment -Neutrino Physics Potentials- ICHEP2012 July Hiroyuki Sekiya ICRR,
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.
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.
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.
Physics with the ICARUS T1800 detector
Yoshihisa OBAYASHI (KEK - IPNS)
Prospects of J-PARC Neutrino Program
T2KK sensitivity as a function of L and Dm2
T2KK Sensitivity of Resolving q23 Octant Degeneracy
Fine-Grained Near Detector(s) at JHF: Purpose and Thoughts
Naotoshi Okamura (YITP) NuFact05
Toward realistic evaluation of the T2KK physics potential
Impact of neutrino interaction uncertainties in T2K
Conventional Neutrino Beam Experiment : JHF – Super-Kamiokande
Presentation transcript:

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

Yoshihisa OBAYASHI, Introduction MNS Matrix: WHY CP ? –In the Quark Sector, CP is violated. –Then, also in the Lepton Sector? → Leptogenesys –CP Measurement is a final goal of flavor physics

Dec. 13, 2001Yoshihisa OBAYASHI, CP Phase Measurement In the case of conventional (super) beam, – –cf: NuFact: Oscillation Probability P(   e ): CPV

Dec. 13, 2001Yoshihisa OBAYASHI, Assumed Scenario on physics ~2010  →   oscillation is established by Atm, LBL – sin 2 2 23 ~ 1.0 – m 2 23 ~ 3 x eV 2 LMA solution is established by Sol, KamLAND – sin 2 2 12 ~ 0.8 – m 2 12 ~ 5 x eV 2 Finite  13 is found by JHF1 (, Atm) – sin 2 2 13 ~ 0.03 MiniBooNE excluded LSND result (Still) Unknown parameters: – CP phase  and sign of m 2

Dec. 13, 2001Yoshihisa OBAYASHI,  → e oscillation probability Asymmetry can be seen at oscillation maximum ~0.7GeV 295km Solid lines: w/ matter, Dashed lines: w/o matter

Dec. 13, 2001Yoshihisa OBAYASHI, JHF-Kamioka Experiments Phase I: 2007 (?) ~201x –~1MW 50GeV PS → 22.5kt detector (Super-Kamiokande)  → x disapp.,  → e app., NC measurement Phase II: 201x(?)~202y(??) –~4MW 50GeV PS → ~1Mt detector (Hyper-Kamiokande) CPV search, Proton Decay, km KEK Kamioka Tokai Hyper-K SK JHF

Dec. 13, 2001Yoshihisa OBAYASHI, Beams Off Axis Beam Switch and by changing polarity of horn magnets Neutrino Flux is almost the same between and beams  Target Horns Decay Pipe Far Det POT/yr (1st phase)

Dec. 13, 2001Yoshihisa OBAYASHI, Cross Sections Quasi elastic interactions dominate below ~1GeV

Dec. 13, 2001Yoshihisa OBAYASHI, Expected Neutrino Events (w/o osc.) # of far det. is factor 3 smaller than –Running time of beam need to be longer Wrong sign contribution is 3x3~10 times large for beam –Cause fake CP asymmetry

Dec. 13, 2001Yoshihisa OBAYASHI, Selection for e appearance search Select e CCqe interactions –Vertex is in the fiducial volume –Single EM shower ring –No decay electron observed –Evis > 100MeV ( reject NC elastic ) –Tight e/  separation see next slide –Reconstructed E cut 0.4 < E(GeV) < 1.2

Dec. 13, 2001Yoshihisa OBAYASHI, Tight e/  separation cose :  from  0 tend to have a forward peak E( 2 )/E( 1 + 2 ): Large for BG Likelihood diff. between 1-ring and 2-rings Invariant mass: Small for e

Dec. 13, 2001Yoshihisa OBAYASHI, Expected Signal & Backgrounds By the present tools, –BG level is ~5x larger than expected CP asymmetry. –We need to achieve ~5% precision of BG subtraction if we want to see 3 effect. ~90% of  BG (50~60% of total BG) are from  0 Beam e app. Signal w/o CP Effect of CP Background in Hyper-K total w/ w/ m 12 2 = 5x10 -5 eV 2 m 23 2 = 3x10 -3 eV 2 sin 2 2 13 = 0.03 sin 2 2 23 = 1 sin 2 2 12 = 0.8  = 45 deg 5 x pot x 450 kt (  ) 1.83 x x 450 kt pot () Off axis 2deg beam No matter effect considered

Dec. 13, 2001Yoshihisa OBAYASHI, Cross Section (& Efficiency) Difference We want to know Observable Then Asymmetry Parameter Only the difference of r,r between neutrino and anti neutrino appear in the asymmetry

Dec. 13, 2001Yoshihisa OBAYASHI, Cross Section Difference CCqe cross section ratio of e /  –Difference between neutrino and anti-neutrino is at most 5% within the energy window ~5%

Dec. 13, 2001Yoshihisa OBAYASHI, CP Measurement Matter effect becomes larger for large  13 Black circles represent 3 contour for phase 2 of JHF running

Dec. 13, 2001Yoshihisa OBAYASHI, BG subtraction vs Sensitivity Sensitivity strongly depends on systematic uncertainty of BG subtraction. If BG sys. = 2%: –sin 2 2 13 =0.01 → sin>0.55(33 o ) –large  13 → sin>0.25(14 o ) Sensitivity improves with better BG rejection  Better BG rejection and smaller uncertainty in BG subtraction are strongly preferred in the CP measurement Chooz  m 31 ~3x10 -3 eV 2 JHF1 cannot discover  13 (3)

Dec. 13, 2001Yoshihisa OBAYASHI, Items for the Improvement of Sensitivity ~90% of  BG are from  0 –Improve the hardware (Hyper-K) Timing resolution, Light scattering and reflection, Segment... –Improve the software Reconstruction algorithm,... –Measure NC  0 Front detector Energy scan with Narrow Band Beam ~50% of BG are from e –Measure e /  Front detector –Narrower energy window Improvement of energy resolution ~50% of BG are from high energy tail of beam –Tune the beam line and reduce HE tail Measurement of wrong sign contamination –Magnetized detector? –Recoiled neutron detector?

Dec. 13, 2001Yoshihisa OBAYASHI, Conclusion Phase 2 of JHF-Kamioka experiment aims at measuring CP violation Better BG rejection and smaller uncertainty in BG subtraction are strongly preferred in the CP measurement Let's Complete MNS matrix!