Takaaki Kajita, ICRR, Univ. of Tokyo NOW2004, Sep 2004
Outline SK Atmospheric neutrino results , L/E, and 3 flavor analysis K2K from K2K-I and -II T2K (Future long baseline experiment) Summary Only 2 and 3 flavor neutrino oscillations
SK collaboration: Japan, USA, Korea, Poland
Event classification and statistics Fully Contained (FC) (E ~1GeV) (12180) Partially Contained (PC) (E ~10GeV) (911) Through-going (E ~100GeV) (1842) Stopping (E ~10GeV) (418) Red: observed number of events in SK-1 (total number = 15351)
Recent improvements New flux based on the 3 dimensional calculation Tuned neutrino interaction MC based on the K2K data 15 37 systematic error terms (S.Moriyama’s talk) 3D 1D (deg)
Super-K atmospheric neutrino data 1489day FC+PC data day upward going muon data CC e CC
Binning for 2 flavor oscillation analysis E Single- Ring Multi- Ring Up-stop Up-through 18 momentum bins x 10 zenith bins = 180 bins in total Single- Ring e PC Each box has 10 zenith bins Multi- GeV Sub- GeV CC e CC
Neutrino oscillation parameters 90%C.L. 2 m2=2.1x10 -3,sin 2 2 =1.00 (full paper will be published soon)
oscillation decoherence decay Further evidence for oscillations Strong constraint on oscillation parameters, especially m 2 -like multi-GeV + PC Should observe this dip! SK collab. hep-ex/
Selection criteria Following events are not used: ★ horizontally going events ★ low energy events Select events with high L/E resolution ( (L/E) < 70%) FC single-ring -like Full oscillation 1/2 oscillation (L/E)=70% Similar cut for: FC multi-ring -like, OD stopping PC, and OD through-going PC 2121 FC -like and 605 PC
L/E distribution MC (no osc.) 1489 days FC+PC Evidence for oscillatory signature Mostly down-going Mostly up-going Osc. Decay Decoh. Decay and decoherence disfavored at 3.4 and 3.8 levels, respectively.
Allowed neutrino oscillation parameters 2 min =37.9/40 m 2 =2.4x10 -3,sin 2 2 =1.00 (sin 2 2 =1.02, 2 min =37.8/40 d.o.f) 1.9x10 -3 < m 23 2 < 3.0x10 -3 eV < sin 2 2 23 (90% C.L.) Stronger constraint on m 2 Consistent with that of the standard zenith angle analysis
Search for non-zero 13 Electron appearance in the 5 – 10GeV(E ) upward going events. s 2 13=0.05 s 2 13=0.00 null oscillation MC, SK 20yrs Electron appearance 1+multi-ring, e-like, GeV cos E (GeV) cos Matter effect ( m 12 2 =0 assumed)
Super-K e-like data Multi-GeV, single-ring e-like Multi-GeV, multi-ring e-like (special) No evidence for excess of upward-going e-like events
Binning for 3flavor analysis E Single- Ring Multi- Ring Up-stop Up-through 37 momentum bins x 10 zenith bins = 370 bins in total Multi- Ring e Single- Ring e PC- stop PC- through Same as 2 flavor analysis Different binning from 2 flavor Special in the 3 flavor ana. Fewer number of events per bin Poisson statistics to claculate 2 Multi- GeV Sub- GeV CC e CC
3 flavor analysis from Super-K Normal prelim. sin 2 13 sin 2 23 sin 2 13 m2m2
3 flavor analysis from Super-K Inverted prelim. sin 2 13 m2m2 sin 2 23 sin 2 13 No evidence for non-zero 13 (No information on the mass hierarchy)
Studies in progress…. Search for tau neutrino interactions Oscillation analysis with the solar terms Simulated interaction Event rate = 1/kton/year Only upward going Statistical estimate of the interactions P.Lipari NOON sub-GeV e-like events Peres, Smirnov NPB 680 (2004) 479 Also, M.Maltoni, this meeting, hep-ph/
SK-II atmospheric neutrino data DATA MC (no oscillation, normalized by live time) Live time FC + PC days Upward going days MC (oscillation, m 2 =2.1×10 -3 eV 2, normalized by live time) SK-II event Preliminary!
K2K Collaboration 250km JAPAN, KOREA, U.S.A., POLAND, CANADA, ITALY, FRANCE, SPAIN, SWITZERLAND, RUSSIA More details: K.Kaneyuki’s talk
K2K Analysis Overview Near detectors #, p and (E )near KEK Observation # and E rec. Expectation # and E rec. (sin 2 2 , m 2 ) SK Far/Near Ratio (E )far int. MC Far/Near Ratio E (GeV) beam MC w/ PION Monitor 12GeV PS (8.9×10 19 POT for Analysis)
Near detectors 1KT Water Cherenkov Detector (1KT) Scintillating-fiber/Water sandwich Detector (SciFi) Scintillator Bar Detector (SciBar) after 2003 Muon Range Detector (MRD) Muon range detector
Front detector measurements: momentum and angular distributions (deg.) 090 p (MeV/c) kton water Cherenkov Also, measurements by SciFi, SciBar and MRD detectors. Prediction of the number of events( ) and spectrum at SK. QE 11 NC Dis Coh
Event selection in Super-Kamiokande T SK T spill GPS SK TOF=0.83msec 108 events obs’d Decay electron cut E vis > 20MeV No activity in outer detector Event vertex in fiducial volume E vis > 30MeV Analysis time window 500 sec 5 sec T DIFF. (s) events exp’d
Summary of K2K-SK events K2KDATAMC FC 22.5kt ring -like e-like 98.8 Multi Ring preliminary K2K I+II
K2K energy spectrum (based on single-ring -like events) MC normalization: number of events E rec [GeV] Number of events Deficit of events MC (no osc.) MC (osc.) preliminary
Best fit values. sin 2 2 1.53 m 2 = 2.12 eV 2 Best fit values in the physical region. sin 2 2 1.00 m 2 = 2.73 eV 2 logL=0.64 Best fit oscillation parameters sin 2 2 =1.53 can occurr due to a a statistical fluctuation with 14.4% probability. Toy MC sin 2 2 m2m % preliminary 1.53
Allowed parameter region m 2 [eV 2 ] sin 2 2 preliminary Best fit values (in the physical region) sin 2 2 = 1.00 m 2 [eV 2 ] = 2.7 m 2 =(1.7~3.5)×10 -3 eV 2 (90% sin 2 2 =1.0 K2K SK(zenith) SK (L/E) 90%CL
K2K Super-Kamiokande 250km J-PARC JAERI Collaboration (at present): Canada, China, France, Italy, Japan, Korea, Poland, Russia, Spain, Switzerland, UK, USA T2K
T2K main physics goals Discovery of non-zero 13 Precise measurement of sin 2 2 23 and m 23 2 (Discovery of non maximal 23 ?) Discovery of non-zero CP phase 1st phase 2nd phase If 13 ≠0 observed
J-PARC Facility Nuclear and Particle Experimental Facility Materials and Life Science Experimental Facility Neutrino to Kamiokande Linac (350m) 3 GeV Synchrotron (25 Hz, 1MW) Nuclear Transmutation 50 GeV Synchrotron (0.75 MW) J-PARC = Japan Proton Accelerator Research Complex Under construction, expected completion (Phase-I)= end 2007 LINAC 3GeV 50GeV dipole magnets 50GeV
T2K neutrino facility Near detectors (280m, and 2km(not approved yet) To SK T2KK2K E(GeV)50 12 Int.(10 12 ppp) 3306 Rate(Hz) Power(MW) OA3° OA0° OA2° OA2.5° Off axis beam facility
Measurement of m 2 and sin 2 2 23 Data sample: SK Monte Carlo, Fully-contained single- ring, muon-like events. Event fraction Typical JHF neutrino energy Important to run the experiment with low energy beam. π π E from E and
~ OA 2.5 deg. ~ Reconstructed neutrino energy distribution No oscillation reconstructed E (GeV) non-QE m 2 = 2.5 x10 -3 eV 2 Quasi Elastic reconstructed E (GeV)
Precise measurement of 23, m 2 23 Assumed systematic errors normalization non-qe/qe ratio E scale Spectrum shape Spectrum width ( 5%) ( 1%) (20%) ( 5%) ( m 2 23 ) <1×10 -4 eV 2 (sin 2 2 23 )~0.01 True m 23 2 (10 -3 eV 2 )
13 Present status: BG (NC 0 ….) Signal for non- zero 13 ( e ) sin 2 13 Allowed
Measurement of e sin 2 2 13 (CC+NC)Beam e Osc’d e Signal+BG Expected signal for CHOO Z limit reconstructed E (GeV) exp’d signal+BG total BG BG Number of events m 2 (eV 2 ) sin 2 2 13 BG=10% Updated More details: K.Kaneyuki’s talk
T2K Phase-II ★ 0.77 → 4 MW beam power ★~ 1 Mton detector (Hyper-Kamiokande) CP Violation 10 6 events (both and anti- )
Assumptions Solid line: w/ matter Dashed line: w/o matter (not updated to the most recent solar parameters)
sin 2 2 13 =0.1 m 31 <0 m 31 >0 90%C.L. stat only 90%C.L. stat+2% syst. 3 stat only 3 stat+2% syst. # of e - events including BG # of e + events including BG CP phase Expected CP violation signal (example) Neutrino run=2years, anti-neutrino run=6.8years, 4MW, 0.54Mton fid. Vol.
3 CP sensitivity no BG signal stat only (signal+BG) stat only stat+2%syst. stat+5%syst. stat+10%syst. CHOOZ excluded sin 2 2 13 m 31 2 ~3x10 -3 eV 2 JHF-I: No indication for sin 2 2θ 13 3 CP sensitivity : | |>20 o for sin 2 2 13 >0.01 with 2% syst. sin 2 2 13 sin
Beam Transfer line from 3GeV to Material and Life science Facility) Decay Volume ~110m OA2 o OA3 o Target Station ~15m Dump ~10m Neutrino facility construction Construction started Expected completion: early 2009
Present atmospheric neutrino data from SK are nicely explained by oscillations with; m 2 =1.9 – 3.0 × eV 2 sin 2 2 > 0.90 (SK L/E analysis) Recent L/E analysis has shown evidence for “oscillatory” signature. No sub-dominant oscillation seen yet. K2K has confirmed neutrino oscillations using the accelerator beam. Neutrino oscillation results from K2K are in good agreement with the SK results. T2K, a precision neutrino oscillation experiment, will start in If non-zero 13 is observed in T2K phase-I, we would like to proceed to T2K phase-II to measure the CP phase.
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