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Precision Measurement of Muon Neutrino Disappearance with T2K Alex Himmel Duke University for the The T2K Collaboration 37 th International Conference on High Energy Physics Valencia, Spain July 3 rd, 2014
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New: Study effects of multi- nucleon interactions Neutrino Physics at T2K Alex Himmel2 Neutrino Interactions Next Talk See Posters from E. Scantamburlo and L. Haegel Talk from A. Hillairet on Saturday
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The T2K Experiment Alex Himmel3 J-PARC ND280, INGRID Super-K ν N 295 km
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J-PARC Neutrino Beam 2.5° off-axis angle – Peak at oscillation minimum – Fewer backgrounds from high energy – Monitored by the INGRID on-axis detector Alex Himmel4 p π+π+ µ+µ+ νµνµ Graphite Target 3 Focusing Horns Decay Volume Beam Dump Muon Monitors to SK 2.5° off-axis On-axis 2°
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Accumulated POT Alex Himmel5 Runs 1-46.57×10 20 POT Run 5: Includes 0.5×10 20 POT ν-mode beam (8% of our goal)
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Analysis Step 1: Flux simulation in Fluka and Geant Constrain with NA61 hadron production data 10-15% flux uncertainty at SK Alex Himmel6 Flux and cross section models, constrained by external data E ν (GeV) σ/E (10 -38 cm 2 /GeV) T2K Peak E NEUT simulation with nuclear effects Constrain effective parameters to external data (mostly MiniBooNE) ~15% uncertainty in CCQE rate
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Analysis Step 2: Alex Himmel7 Fit ND280 data to constrain flux and cross section parameters Multi-function detector – Trackers, TPCs, EM calorimeters, µ detector and π 0 detector – Magnetized with UA1 magnet – 280 m from target, 2.5° off-axis Posters from E. Scantamburlo and L. Haegel
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Analysis Step 2: Alex Himmel8 Fit ND280 data to constrain flux and cross section parameters CC 0π64% QE CC 1π + 40% Resonance CC other68% DIS – Fit for p and θ in CCν µ samples – Use exclusive subsamples to isolate cross section components MC Pre-fit MC post-fit Data ND280 CC 0π A. Hillairet’s talk on Saturday
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Alex Himmel9 Flux Error Before Fit Flux Error After Fit Xsec Error Before Fit Xsec Error After Fit Flux and cross section errors at SK reduced from > 20% to 2.7% Total Error on SK expectation: 8.1%* Analysis Step 2: Fit ND280 data to constrain flux and cross section parameters *Now reduced to 7.6% in joint analyses
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Analysis Step 3: Alex Himmel10 Select ν μ CCQE events at Super-K Use ring shape to separate µ and e Select for CCQE final states – 1 ring – ≤ 1 decay electron Use p µ and θ beam to reconstruct E ν Water Cherenkov Detector 50 ktonnes of ultrapure water 40% photocoverage
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Alex Himmel11 Analysis Step 3: Select ν μ CCQE events at SuperK 120 Events 98.5% CC ν μ Data 81.0%ν μ CCQE 17.5% ν μ CC non-QE 1.5%NC
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Alex Himmel12 Fit for oscillations Extract θ 23, Δm 2 32 Analysis Step 4: Normal HierarchyInverted Hierarchy Maximal Disappearance Data (120 events) – No oscillations (446 events) – Best oscillation fit Data/No osc. – Best fit/No osc.
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Alex Himmel Best fit at maximal disappearance – Result narrower than sensitivity by 0.04 in sin 2 (θ 23 ) Most precise measurement of sin 2 (θ 23 )! Normal Hierarchy T2K68% dashed, 90% solid SK90% MINOS90% 13 Analysis Step 4: Fit for oscillations Extract θ 23, Δm 2 32
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Alex Himmel14 Multinucleon Interactions Neutrinos may interact with multiple nucleons – Looks CCQE, but has different kinematics – Potential explanation for discrepancies in M A measurements Studied potential for bias in our result from neglecting multinucleon interactions νμνμ μ-μ- p p
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Alex Himmel15 Multinucleon Interactions For the current analysis, the effect is small relative to our total error – Mean biases were small (<1%) – However, there is the potential for biases in sin 2 θ 23 similar in size to our current systematic error Future analyses will include multinucleon interactions in the default cross-section model with systematic uncertainties Bias in sin 2 θ 23 from fake experiments Bias in Δm 2 32 from fake experiments Mean bias: -0.2% RMS bias:0.6% Mean bias: 0.3% RMS bias:3.6%
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Conclusions Alex Himmel Analyzed 6.57×10 20 POT of neutrino data – Accumulated our first 0.5×10 20 POT of antineutrino data Made the most precise measurement of sin 2 θ 23 and favor maximal disappearance Only 8% of our goal POT accumulated so far 16 Dashed:current systematics Solid: no systematics
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Backup Slides Alex Himmel17
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Alex Himmel18 Error on # of ν µ Events ND280-constrained Φ & σ2.7% Unconstrained cross section 4.9% SK efficiency & hadronic interactions in water 5.6% Other oscillation parameters 0.2% Total8.1% Flux Error Before Fit Flux Error After Fit Xsec Error After Fit Xsec Error Before Fit Flux and cross section would be > 20% without ND280 constraint Analysis Step 2: Fit ND280 data to constrain flux and cross section parameters
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Analysis Structure Alex Himmel19 Flux Simulation Cross section model External σ data Hadron prod. from NA61 Initial Φ estimate, and errors Initial σ estimate, and errors Fit to ND280 data Post-fit Φ, σ estimate, errors Fit to SK data
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Sensitivity vs. Data Fit Alex Himmel20
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Multinucleon Interactions Long-standing tension over M A in CCQE interactions – “Natural” value of 1.0 GeV from e-scattering – >1.2 GeV in ν scattering New models involving 2p-2h/np-nh interactions have been proposed to reconcile the tension Several papers have investigated the possible effect on T2K or a T2K-like experiment Alex Himmel21 O. Lalakulich and U. Mosel, Phys. Rev. C 86, 054606 (2012). D. Meloni and M. Martini, Phys. Lett. B 716, 186 (2012). P. Coloma, et al, arXiv:1311.4506 (2013).
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Multinucleon Study in T2K Multi-nucleon interactions: – increase the CCQE-like cross-section and – introduce energy reconstruction biases (no longer 2 body QE kinematics) MC study to investigate this possible bias directly – ν µ disappearance – more sensitive to the spectral shape – We introduce a 2p-2h model into both ND280 and SK fake data – Replace π-less Δ decay already in NEUT Alex Himmel22 J. Nieves et. al., PRC83, 045501 (2011) for lepton kinematics J. Sobczyk, PRC86, 015504 (2012) for nucleon ejection (ND280-only)
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Biases in Oscillation Fits Alex Himmel23 Nieves Nominal BiasRMSData Fit Errors Δm 2 32 (10 -3 eV 2 ) -0.005(-0.2%)0.014(0.6%)±0.10 sin 2 θ 23 0.0012(0.3%)0.016(3.6%)±0.055
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