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Neutrino Interaction measurement in K2K experiment (1kton water Cherenkov detector) Jun Kameda(ICRR) for K2K collaboration RCCN international workshop at Kashiwa Dec. 10 th, 2004
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Contents 1.Introduction of K2K experiment and 1kton water Cherenkov neutrino detector. 2. Neutrino spectrum measurement 3. measurement of 0 production cross section
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K2K Collaboration Canada France Italy Japan Korea Poland Russia Spain Swiss U.S.A. 12 country, 27 institute, ~160 members.
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1. K2K experiment ( Long baseline neutrino oscillation experiment from KEK to Kamioka KEK 12GeV PS ν beamline beam monitor Front Neutrino detectors Super-Kamiokande (Far Detector) 50kton water Cherenkov 250km Almost pure ν μ beam (~98%) Wide band = 1.3GeV The first long baseline neutrino oscillation experiment using accelerator. Purpose: disappearance x e appearance ( e interaction study at ~ 1GeV region
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1-1 Front neutrino detectors 1kton water Cherenkov detector SciBar detector ( from Oct.2004) Muon Chamber To Super-Kamiokande νbeam SciFi detector Purpose: Measure neutrino flux at KEK Measure neutrino energy spectrum Study neutrino interactions
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1-3. 1kton water Cherekov detector (1kton detector) 1000t cylindrical water tank 680 20inch PMTs with 70cm spacing (same as SK) the same detection mechanism, analysis algorithms and interaction MC as Super-K. a smaller version of Super-Kamiokande (~1/50 volume) inside view
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Typical Neutrino Event of 1kton detector p Number of Cherenkov ring number of particles Ring direction particle direction Number of photons momentum Ring pattern & opening angle Particle ID ( e-like/ -like ) Reconstruction of the physics quantity: unrolled view Cherenkov light
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2. Measurement of the neutrino spectrum ν 200cm μ 1kton detector QE CC 1pi CC multi pi CC coh. pi NC θ μ Event Selection 25t fiducial volume Fully Contained (no escaping particles) 1-ring μ-like Quasi Elastic Enriched sample Fraction = ~60% ~ 1.1GeV
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2-1. Muon momentum & direction distribution QE CC 1pi CC multi pi CC coh. pi NC PμPμ deficit is observed in forward region θμθμ Data/MC In forward region, deficit was observed (~40% deficit < 10 degree) event/20 MeV/c
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Problem of neutrino Interaction ? Charged Current single- production (CC 1π ) Charged Current Coherent π production are most suspicious. Deficit was found in small (small q 2 ) region. as other detector (SciFi 、 SciBar) QE CC 1pi CC multi pi CC coh. pi NC θμθμ Reconstructed q2 ( assuming QE scatterng ).
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Suppression factor for 1pi production x q 2 /0.1 (q 2 <0.1GeV 2 region) Agreement between data & MC become better for both case. W/o coherent pion production Apply phenomenological suppression factors from SciBar. Data/MC
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DATA 2.Neutrino spectrum fit Fit observed (, ) 2-dim distribution by weighted sum of MC templates. MC Quasi- elastic non-Q.E. Template is prepared for each Parent Neutrino Energy bin ( 8bin) 、 and Q.E.and non-Q.E. interactions fitting parameter f i (8 bin) : Weight for I’th energy bin(8bins) Rnqe/qe : Q.E./ nQE ratio ε : systematic parameter α : norm. factor
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Analysis results for Toy MC data. w/ and w/o cut. No systematic biases are found. In the fitting, small angle region ( < 20deg.) is cut for 1kton detector. θμθμ cut f3f4f5 f6 f7f8f1f2 nqe/qe Effect of the cut in the spectrum fit Treatment of the deficit in small region in the spectrum fit e-scale
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2-3. Spectrum fit result f1 ( Eν<0.5GeV) 1.413 ± 0.416 f2 (0.5 <E<0.75) 1.136 ± 0.103 f3 (0.75<E<1.0 ) 1.097 ± 0.080 f4 (1.0 <E<1.5 ) 1.000 (fixed) f5 (1.5 <E<2.0 ) 0.856 ± 0.075 f6 (2.0 <E<2.5 ) 0.936 ± 0.172 f7 (2.5 <E<3.0 ) 0.776 ± 0.729 f8 (3.0 <E ) 1.000 (fixed) R(QE/nQE) 0.705 ± 0.113 E-scale 0.982 ± 0.005 We obtained the neutrino spectrum in 1kton detector. χ 2 = 51.8 / 60 d.o.f. Parent neutrino energy distribution for FC 1Ring m-like events. Nominal MC After fitting For neutrino oscillation analysis, global fitting is carried out using 1kton,SciBar and SciFi detectors.
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0 event analysis Main background for e search 0 can mimic an electron asymmetric decay Cherenkov ring overlapping / s separation single 0 events : good NC sample Precise understandnig of 0 production rate 、 0 momentum/angle distribution is important for these analyses. Motivation: 00 00
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Data set Period : 2000/Jan-Mar. 2001/Jan~Jul. (~ 3x10 19 pot) data MC Mass peak (MeV/c 2 ) data : 147.4 MC : 144.1 non- 0 BG very clean 0 sample Selection Criteria of 0 events 25t fiducial volume Fully-Contained number of rings = 2 both e-like PID M : 85 ~ 215 MeV/c 2 FC 2ring 0 : 2496 events
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0 momentum & angular dist. (FC 2ring 0 sample) Shape of the distributions well agree between Data & MC. # of FC 2ring 0 events ( MC is normalized by area ) Forward FC 2ring 0 sample : large NC fraction ~ 87 % Backward
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“ NC1 0 “ interaction 00 NC ? NC interaction accompanied with only one 0 and no other particle going out of a 16 O nucleus. (after nuclear re-scatterings) Generated 0 will be largely affected by nuclear effects in 16 O. We measure 0 production cross section after nuclear effects. N FC2R 0 obs x r pure x corr fid N NC1 0 = eff non-NC1 0 subtraction rec true fiducial correction detection and reconstruction efficiency “ NC1 0 “ ① ② FC 2ring 0 mom.
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NC1 0 production in true 25t (after corrections) N(NC1 0 ) : 3.69 ± 0.07 ± 0.37 x 10 3 stat. sys. data (inner: stat, outer: stat+sys) MC true (inner: MC stat, outer: MC stat + sys error on shape from our MC model uncertainties) normalized by the number of all events in 25t fiducial in 25 ton # of NC1 0 interactions
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N( CC) as normalization : N( CC) = N(FC +PC) 25t obs x (1 – BG non- ) x purity x corrfid / eff = 5.65 ± 0.03 ± 0.26 x 10 4 stat. sys in 25 ton FC single-ring -like FC multi-ring -like PC CC enriched sample ++ = 0.065 ± 0.001 ± 0.007 stat. sys. at the K2K beam energy, ~1.3 GeV Then, cf. (NC1 0 ) / ( CC) = 0.064 from NEUT (NC1 0 ) ( CC)
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Summary We measured the neutrino spectrum by 1kton detector We observed a deficit in forward direction. Phenomenological suppression factor give a better agreement between data/ MC, but we cannot have strong conclusion. In the spectrum fit, low region (<20deg) is cut. NC1 0 production rate and 0 momentum distribution is measured. We measured the cross section ratio (NC1 0 )/ ( CC) at K2K neutrino beam energy.
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Supplement
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① non-NC1 0 BG subtraction NC 1 0 : 71 % fraction in FC 2ring 0 00 00 00 00 or CC w/ invisible 6 % CC w/ invisible , 3 % NC w/ invisible 7 % 0 produced outside the nuclei 10 % cross section 6.3 % M A in QE,1 (+-10%) 0.2 % QE (total cross section +-10%) <<1 % 1 (total cross section +-10%) 0.9 % coherent (model dependence) 1.6 % DIS (model dependence) 5.1 % DIS (total cross section +-5%) 0.5 % CC/NC +-20% 3.2 % nuclear rescattering1.6 % absorption prob. +-30% 1.5 % inelastic scattering prob. +-30% 0.7 % 0 from nucleon(or interaction 2.3 % in water (2 nd interaction) total interaction prob. +-20% 2.3 % total: 6.9 % systematic error on BG subtraction
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1. Delivered protons on target Total Delivered POT Jun 1999 - Feb. 15, 2004 101.12x10 18 POT ( Jan. 16 - Feb. 15) 5.55x 10 18 POT POT/spill = ~ 5.4x10 12 Protons
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2. Muon Direction measured by muon monitor whole the K2K (I+II) run period Muon Direction was Stable within 1 mrad. +- 1mrad
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2-1. Muon momentum & direction distribution ν 200cm μ 1kton detector QE CC 1pi CC multi pi CC coh. pi NC θ μ PμPμ deficit is observed in forward region θμθμ Data/MC Event Selection 25t fiducial volume Fully Contained (no escaping particles) 1-ring μ-like ( QE enriched, fraction of Quasi elastic ~ 60% )
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