Performance of a Water Cherenkov Detector for e Appearance Shoei NAKAYAMA (ICRR, University of Tokyo) November 18-19, 2005 International Workshop on a.

Slides:



Advertisements
Similar presentations
Recent Results from Super-Kamiokande on Atmospheric Neutrino Measurements Choji Saji ICRR,Univ. of Tokyo for the Super-Kamiokande collaboration ICHEP 2004,
Advertisements

11-September-2005 C2CR2005, Prague 1 Super-Kamiokande Atmospheric Neutrino Results Kimihiro Okumura ICRR Univ. of Tokyo ( 11-September-2005.
Takaaki Kajita ICRR, Univ. of Tokyo Nufact05, Frascati, June 2005.
Super-Kamiokande Introduction Contained events and upward muons Updated results Oscillation analysis with a 3D flux Multi-ring events  0 /  ratio 3 decay.
Near detectors for long baseline neutrino experiments T. Nakaya (Kyoto) 1T. Nakaya.
Off-axis Simulations Peter Litchfield, Minnesota  What has been simulated?  Will the experiment work?  Can we choose a technology based on simulations?
Background Understanding and Suppression in Very Long Baseline Neutrino Oscillation Experiments with Water Cherenkov Detector Chiaki Yanagisawa Stony Brook.
Far Detector Fiducial Volume Study Andy Blake Cambridge University Thursday December 7 th 2006.
Identification of neutrino oscillations in the MINOS detector Daniel Cole
New results from K2K Makoto Yoshida (IPNS, KEK) for the K2K collaboration NuFACT02, July 4, 2002 London, UK.
Shoei NAKAYAMA (ICRR) for Super-Kamiokande Collaboration December 9, RCCN International Workshop Effect of solar terms to  23 determination in.
Preliminary Study of CC-Inclusive Events in the P0D using Global Reconstruction Rajarshi Das (w/ Walter Toki) Nu-Mu Prelim. Meeting Dec 2010 CSU.
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.
The Earth Matter Effect in the T2KK Experiment Ken-ichi Senda Grad. Univ. for Adv. Studies.
Apr. 4, KEK JHF-SK neutrino workshop 1 e appearance search Yoshihisa OBAYASHI (KEK - IPNS)
RECENT RESULTS IN K2K EXPERIMENT Shimpei YAMAMOTO (Kyoto Univ.) 10 th ICEPP 16-FEB-2004 Shimpei YAMAMOTO (Kyoto Univ.) 10 th ICEPP Symposium.
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.
TAUP Searches for nucleon decay and n-n oscillation in Super-Kamiokande Jun Kameda (ICRR, Univ. of Tokyo) for Super-Kamiokande collaboration Sep.
Latest Results from the MINOS Experiment Justin Evans, University College London for the MINOS Collaboration NOW th September 2008.
Yoshihisa OBAYASHI, Oct. Neutrino Oscillation Experiment between JHF – Super-Kamiokande Yoshihisa OBAYASHI (Kamioka Observatory, ICRR)
Measurements of neutrino charged current scattering in K2K Fine-Grained Detector Introduction Introduction K2K Near Detector K2K Near Detector CC interactions.
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.
Search for Sterile Neutrino Oscillations with MiniBooNE
Rencontres de Moriond (6 th March 2005) C. Mariani (INFN Rome) for K2K collaboration March 6 th, XLth Rencontres de Moriond.
Beam Extrapolation Fit Peter Litchfield  An update on the method I described at the September meeting  Objective;  To fit all data, nc and cc combined,
Neutrino Oscillations at Super-Kamiokande Soo-Bong Kim (Seoul National University)
Low Z Detector Simulations
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.
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.
Water Cherenkov detector - brief status report - Kenji Kaneyuki Research Center for Cosmic Neutrinos, ICRR, Univ. of Tokyo.
1 A study to clarify important systematic errors A.K.Ichikawa, Kyoto univ. We have just started not to be in a time blind with construction works. Activity.
1 Study of physics impacts of putting a far detector in Korea with GLoBES - work in progress - Eun-Ju Jeon Seoul National University Nov. 18, 2005 International.
Search for active neutrino disappearance using neutral-current interactions in the MINOS long-baseline experiment 2008/07/31 Tomonori Kusano Tohoku University.
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 ”
September 10, 2002M. Fechner1 Energy reconstruction in quasi elastic events unfolding physics and detector effects M. Fechner, Ecole Normale Supérieure.
Takaaki Kajita ICRR, Univ. of Tokyo KIAS, Seoul, Nov Fig: Senda NP-4.
PAC questions and Simulations Peter Litchfield, August 27 th Extent to which MIPP/MINER A can help estimate far detector backgrounds by extrapolation.
Measuring Neutrino Oscillations with the T2K Experiment Alfons Weber University of Oxford STFC/RAL Dec-2011.
Review of experimental results on atmospheric neutrinos Introduction Super-Kamiokande MACRO Soudan 2 Summary Univ. of Tokyo, Kamioka Observatory.
Hiroyuki Sekiya ICHEP2012 Jul 5 The Hyper-Kamiokande Experiment -Neutrino Physics Potentials- ICHEP2012 July Hiroyuki Sekiya ICRR,
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.
Constraint on  13 from the Super- Kamiokande atmospheric neutrino data Kimihiro Okumura (ICRR) for the Super-Kamiokande collaboration December 9, 2004.
 CC QE results from the NOvA prototype detector Jarek Nowak and Minerba Betancourt.
Current Status of the T2K Experiment Ryan Terri (for the T2K Collaboration) 31 May – 4 June 2010 Planck 2010, CERN.
Precision Measurement of Muon Neutrino Disappearance with T2K Alex Himmel Duke University for the The T2K Collaboration 37 th International Conference.
30th International Cosmic Ray Conference in Merida, Mexico Michael Smy UC Irvine Low Energy Event Reconstruction and Selection in Super-Kamiokande-III.
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
Preliminary T2K beam simulation using the G4 2km detector
L/E analysis of the atmospheric neutrino data from Super-Kamiokande
Update of the Fiducial calibration study in 2km WC detector
Yoshihisa OBAYASHI (KEK - IPNS)
Report of the T2KK Workshop
T2KK sensitivity as a function of L and Dm2
T2KK Sensitivity of Resolving q23 Octant Degeneracy
Naotoshi Okamura (YITP) NuFact05
Neutrino interaction measurements in K2K SciBar
Toward realistic evaluation of the T2KK physics potential
Impact of neutrino interaction uncertainties in T2K
Presentation transcript:

Performance of a Water Cherenkov Detector for e Appearance Shoei NAKAYAMA (ICRR, University of Tokyo) November 18-19, 2005 International Workshop on a Far Detector in Korea for the J-PARC Neutrino KIAS, Seoul, Korea

Motivation  SK : OA 2.5 o  A far detector in Korea has the option to choose a site for a smaller off-axis angle.  higher energy neutrino beam  Check the signal/BG separation performance for higher energy neutrinos   0 BG is dominant for e search.  efficient  0 BG rejection   

Current T2K Selection Criteria for e Appearance  Standard SK cuts : fiducial volume, fully-contained, Evis > 100 MeV single-ring electron-like PID no decay-e 0.35 < E rec < 0.85 GeV E rec = (m N E e -m e 2 /2)/(m N -E e +P e cos-e )  Further  0 cuts : cose < 0.9 L < 80, M 0 < 100 MeV/c 2 of  0 fitter (POLfit)

POL(Pattern of Light)fit –  0 fitter – 500 MeV/c  0 true P  2 = 55.5MeV/c rec.M  0 =140.4MeV/c 2 11 22 standard fitter POLfit Target: FCFV 1R-elike events L ≡ Likelihood(2 assump.) – Likelihood(electron assump.) Try to reconstruct two  rings Input: vertex, visible energy, and the 1 st  direction by the standard fitter Compare observed & expected (direct+scatter) charge Vary the 2 nd  direction and the energy fraction until the best match found  M 0 etc.

Events vs. Selections Event selections: 1.FCFV, E vis > ring 3. e-like 4. no decay-e < E rec <  0 cuts: - cos < L < 80, M 0 < 100 events/22.5kt/5yrs event selections  BG e signal e BG m 2 = 2.5x10 -3 eV 2 sin 2 2 13 = 0.1 S. Mine NP04

Events vs. Selections (cont ’ d)  CC BG  NC BG beam e BG e (CC) Signal FCFV E vis > ring 1313 (46%)277 (26%)114 (46%)243 (84%) e-like 51 (1.8%)219 (20%)111 (45%)240 (83%) no decay-e 15 (0.5%)195 (18%)92 (37%)222 (77%) 0.35 < E rec < (0.1%)58 (5%)27 (11%)173 (60%) cos < 0.9 L < 80 M < ±0.8 (0.3%) 16±0.4 (6%) 122±3 (42%) (events / 22.5kt / 5yrs) m 2 = 2.5x10 -3 eV 2 sin 2 2 13 = 0.1 S. Mine NP04 ~20% ~70%

This study uses …  the SK-I atmospheric MC sample to study the higher neutrino energy range than that of the OA2.5 beam MC contains both e and  events livetime: 100yrs  the maximum-likelihood analysis to select e CC signals efficiently pre-cut : FCFV, Evis>100MeV single-ring e-like no-decay-e

Dist. for making a e CC-enriched likelihood (1) E vis : 100 ~ 250 MeV 250 ~ 400 MeV  CC + NC e CCQE 400 ~ 600 MeV 600 ~ 900 MeV 900 ~ 1500 MeV 1500 ~ MeV ring-counting parameter

Dist. for making a e CC-enriched likelihood (2) 250 ~ 400 MeV  CC + NC e CCQE 400 ~ 600 MeV 600 ~ 900 MeV 900 ~ 1500 MeV 1500 ~ MeV PID parameter E vis : 100 ~ 250 MeV

Dist. for making a e CC-enriched likelihood (3) 250 ~ 400 MeV  CC + NC e CCQE 400 ~ 600 MeV 600 ~ 900 MeV 900 ~ 1500 MeV 1500 ~ MeV cos -e E vis : 100 ~ 250 MeV

Dist. for making a e CC-enriched likelihood (4) 250 ~ 400 MeV  CC + NC e CCQE 400 ~ 600 MeV 600 ~ 900 MeV 900 ~ 1500 MeV 1500 ~ MeV  0 mass by POLfit E vis : 100 ~ 250 MeV

Dist. for making a e CC-enriched likelihood (5) 250 ~ 400 MeV  CC + NC e CCQE 400 ~ 600 MeV 600 ~ 900 MeV 900 ~ 1500 MeV 1500 ~ MeV L by POLfit E vis : 100 ~ 250 MeV

Likelihood distribution  CC + NC e CCQE Likelihood FCFV, Evis>100MeV single-ring e-like no decay-e  good separation

Likelihood distributions for each energy range 250 ~ 400 MeV 400 ~ 600 MeV 600 ~ 900 MeV 900 ~ 1500 MeV 1500 ~ MeV E vis : 100 ~ 250 MeV Likelihood  CC + NC e CCQE

Events vs. Selections (100yr atm- MC) FCFV,evis : ring : e-like : no decay-e : likelihood : 43 (25.9%) 70 (39.5%) 59 (25.2%) 116 (22.5%) FCFV,evis : ring : e-like : no decay-e : likelihood : (90.8%) (83.3%) 9379 (78.2%) 7328 (58.9%) FCFV,evis : ring : e-like : no decay-e : likelihood : 290 (12.2%) 667 (25.5%) 325 (27.5%) 545 (39.5%) e CC  CC NC rec E : 0~ ~ ~ ~

Likelihood distributions for each sample rec E: 0~ ~ ~1.51.5~ e CC  CC NC

Efficiency by the likelihood cut e CC  CC NC rec E : 0~ ~ ~ ~ Efficiency Likelihood>0.0 Likelihood>0.5

Composition of e CC interactions in the final sample True neutrino energy (GeV) Fraction e CC QE e CC single  e CC multi  WC detector cannot reconstruct the neutrino energy of these events.

Summary  The signal/BG separation in a water Cherenkov detector for the e appearance experiment has been developed based on a likelihood analysis.  The performance of the signal/BG separation was checked in the higher neutrino energy for a smaller off-axis site of a far detector in Korea.  In the higher energy region, the performance of the separation is worse. In addition, the fraction of CC non-QE interaction in the final sample is larger, whose parent neutrino energy cannot be reconstructed correctly.

Supplement

Events vs. Selections (100yr atm- MC) FCFV,evis : ring : e-like : no decay-e : likelihood : 1 (25.0%) 61 (31.8%) 79 (32.5%) 147 (22.5%) FCFV,evis : ring : e-like : no decay-e : likelihood : (92.8%) (85.1%) (78.1%) 8818 (60.5%) FCFV,evis : ring : e-like : no decay-e : likelihood : 2 ( 3.9%) 204 (16.5%) 356 (20.7%) 1265 (27.9%) e CC  CC NC true E : 0~ ~ ~ ~

Likelihood distributions for each sample true E: 0~ ~ ~1.51.5~ e CC  CC NC

Efficiency by the likelihood cut e CC  CC NC true E : 0~ ~ ~ ~ Efficiency Likelihood>0.0 Likelihood>0.5