Results from T2K and Prospects for Hyper Kamiokande

Slides:



Advertisements
Similar presentations
J. Strait Fermilab October 21, 2005 The Neutrino Detector of the Future: A Massive Liquid Argon TPC.
Advertisements

1 3+2 Neutrino Phenomenology and Studies at MiniBooNE PHENO 2007 Symposium May 7-9, 2007 U. Wisconsin, Madison Georgia Karagiorgi, Columbia University.
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.
P AUL N IENABER S AINT M ARY ’ S U NIVERSITY OF M INNESOTA FOR THE M INI B OO NE C OLLABORATION J ULY DPF2009.
MiniBooNE: (Anti)Neutrino Appearance and Disappeareance Results SUSY11 01 Sep, 2011 Warren Huelsnitz, LANL 1.
T2K neutrino experiment at JPARC Approved since 2003, first beam in April Priorities : 1. search for, and measurement of,   e appearance  sin.
Near Detector Working Group for ISS Neutrino Factory Scoping Study Meeting 24 January 2006 Paul Soler University of Glasgow/RAL.
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.
F.Sanchez (UAB/IFAE)ISS Meeting, Detector Parallel Meeting. Jan 2006 Low Energy Neutrino Interactions & Near Detectors F.Sánchez Universitat Autònoma de.
NuMI Offaxis Near Detector and Backgrounds Stanley Wojcicki Stanford University Cambridge Offaxis workshop January 12, 2004.
Alain Blondel Detectors UNO (400kton Water Cherenkov) Liquid Ar TPC (~100kton)
1 Neutrinos: Past, Present and Future Robert C. Webb Physics Department Texas A&M University Robert C. Webb Physics Department Texas A&M University.
2/21/2008 P5 neutrino session1 Conventional neutrino experiments Heidi Schellman P5 February 21, 2008.
T2K experiment at J-PARC Epiphany 2010D. Kiełczewska1 For T2K Collaboration Danuta Kiełczewska Warsaw University & Sołtan Institute for Nuclear Studies.
Toyota National College of Technology A.Takamura Collaboration with K.Kimura and T.Yoshikawa GLoBES 2007 Measuring the Leptonic CP Phase in Oscillations.
1 SciBar for Booster Neutrinos T. Nakaya (Kyoto) March 30, 2005.
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.
PINGU – An IceCube extension for low-energy neutrinos Uli Katz on behalf of the PINGU Collaboration European Strategy for Neutrino Oscillation.
The Earth Matter Effect in the T2KK Experiment Ken-ichi Senda Grad. Univ. for Adv. Studies.
Long Baseline Experiments at Fermilab Maury Goodman.
Future Neutrino Physics Mitch Soderberg Fermilab Institutional Review June 6-9, 2011.
Sterile Neutrino Oscillations and CP-Violation Implications for MiniBooNE NuFact’07 Okayama, Japan Georgia Karagiorgi, Columbia University August 10, 2007.
Dec. 13, 2001Yoshihisa OBAYASHI, Neutrino and Anti-Neutrino Cross Sections and CP Phase Measurement Yoshihisa OBAYASHI (KEK-IPNS) NuInt01,
The NOvA Experiment Ji Liu On behalf of the NOvA collaboration College of William and Mary APS April Meeting April 1, 2012.
Latest Results from the MINOS Experiment Justin Evans, University College London for the MINOS Collaboration NOW th September 2008.
Counting Electrons to Measure the Neutrino Mass Hierarchy J. Brunner 17/04/2013 APC.
If  13 is large, then what ? Hisakazu Minakata Tokyo Metropolitan University.
1 Luca Stanco, INFN-Padova (for the OPERA collaboration) Search for sterile neutrinos at Long-BL The present scenario and the “sterile” issue at 1 eV mass.
Plan to go forward Peter Wilson SBN Program Coordinator 27 September 2014.
Michel Gonin – Ecole Polytechnique – France : SUPER NOVA SN1987A Super-Kamiokande Introduction neutrino oscillations mixing matrices Introduction.
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.
Results and Implications from MiniBooNE: Neutrino Oscillations and Cross Sections 15 th Lomonosov Conference, 19 Aug 2011 Warren Huelsnitz, LANL
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.
PPAP Review 09 Imperial College/RAL Dave Wark Future Neutrino Oscillation Experiments Dave Wark Imperial/RAL PPAP Birmingham July 15 th, 2009.
T2K Experiment Results & Prospects Alfons Weber University of Oxford & STFC/RAL For the T2K Collaboration.
ICARUS-LBNE project A. Guglielmi 1.LBNE-ICARUS Padova meeting 2.SPS-C C. Rubbia presentation.
MINERνA Overview  MINERνA is studying neutrino interactions in unprecedented detail on a variety of different nuclei  Low Energy (LE) Beam Goals: t Study.
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.
/18 N eutrino E xperiment with S pectrometer S i n E urope Search for sterile neutrinos at CERN G. Sirri INFN Bologna on behalf of the NESSiE Collaboration.
Neutrino Oscillations and T2K
L/E analysis of the atmospheric neutrino data from Super-Kamiokande
LBL Oscillation H. Minakata (Tokyo Metropolitan U.)
HARPO Analysis.
Oxford University/RAL
Current Status of the T2K Experiment
Neutrino oscillations with the T2K experiment
Future physics at nuSTORM
ND280 upgrades Alain Blondel T2K meeting 3June15
Yoshihisa OBAYASHI (KEK - IPNS)
The Neutrino Oscillation Industry
Prospects of J-PARC Neutrino Program
T2KK sensitivity as a function of L and Dm2
T2KK Sensitivity of Resolving q23 Octant Degeneracy
6. Preliminary Results from MINOS
Title : SciBooNE -- Experimental study of neutrino cross-sections for a long baseline neutrino oscillation experiment and the development of the detectors.
Impact of neutrino interaction uncertainties in T2K
Determination of Neutrino Mass Hierarchy at an Intermediate Baseline
Gary Feldman P5 Meeting 21 February
A High Intensity Neutrino Oscillation Facility in Europe
Mass Hierarchy in LBL experiments
Conventional Neutrino Beam Experiment : JHF – Super-Kamiokande
Fermilab Proton Beams: Program Perspectives Greg Bock Fermilab Science and Engineering at Henderson-DUSEL Capstone Workshop Stony Brook May 5,
What is μ-e Conversion ? μ μ-+(A,Z)→e-+(A,Z) muon decay in orbit
FNAL-E954: SciBooNE Decay region 50 m MiniBooNE Detector SciBar
The Neutrino Oscillation Industry
Based on material presented at various meetings
Presentation transcript:

Results from T2K and Prospects for Hyper Kamiokande Dave Wark Prague Colloquium Nov. 2nd, 2017 Warning: I have stolen slides mercilessly from my colleagues, including many from Mark Hartz’s talk at KEK on August 4th of this year.

Some Ancient History… Question in the late 50’s: Are the neutrinos in these reactions the same thing?: n → p + e + ν p → m + ν m → e + ν + ν If so, why no m → e + g via diagrams like?: m n e g IVB

Today this would be interpreted as a neutrino oscillation experiment, and in a different world that could have confused things greatly! m event e event

#

CCQE rel. s max!

e p0 m Background from NC interactions nm disappearance signal ne In this energy range, Super Kamiokande well understood, Excellent for separating electrons, m, p0

We are running again. Power ramping up, currently ~440 kW We are running again. Power ramping up, currently ~440 kW. Running in RHC mode.

Many fake data studies have been done to test sensitivity and robustness of analysis to different assumptions about neutrino interaction models. Still preliminary, but current results indicate 23 mixing parameters are more sensitive than d. Watch this space. Results are informing designs of upgrades to the ND280 ND

T2K is moving towards T2K II, with 20 x 1021 p.o.t. Requires better control of systematics!

Find DSNR neutrinos. . . Meanwhile, in Super-K… Slash PDK background. . . Tell n from anti-n. . .

Uprades to the detector will be done next summer. Gd loading will be done depending on T2K schedule.

To get project moving as quickly as possible, currently only discussing one tank in Japan. Second tank to be added later, but maybe not in Japan?

Simulations show significant improvements in Systematics!

Included in shortlist of future large projects by the Science Council of Japan Upgrade to the beam to reach 1.3 MW already approved (funding not started yet) Hyper Kamiokande was identified as the highest priority project in the new MEXT Roadmap published this summer. This is “approval” in the Japanese system. Next step (and last before construction start) is the Ministry of Finance – some money may start next year, with full budget to follow.

Conclusions (I) T2K has surpassed all its construction goals with only about 1/3 of its design protons on target, largely as a result of a very favourable value of sin2q13. T2K sees a high rate of electron neutrino appearance which favours CP violation at ~2 sigma. T2K sees a low rate of muon neutrino survival which favours maximal disappearance. The combination favours NH, but with very limited significance. All these conclusions are statistically weak, so more data is definitely needed. The nuclear physics of neutrino interactions has proven more complex and more important than was appreciated when the experiment was originally built, so we need more theoretical work and more and better near detector data (and probably ancillary experiments such as a high-pressure TPC).

Conclusions (II) Upgrades are planned to the near detectors to address the experimental end of this and the first steps are underway with WAGASCI/BabyMIND. The community as a whole is attacking the uncertainties in neutrino interactions, which will severally limit future experiments if not better understood. T2K II will provide a rich data set to further explore the physics of oscillations and give more sensitivity to MH and CP> Definitive measurements will require bigger detectors! Hyper Kamiokande is moving towards construction start with first data in the latter half of the 2020’s. All these activities are short of manpower! JOIN US!