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T2K Experiment Results & Prospects. Alfons Weber University of Oxford & STFC/RAL For the T2K Collaboration. Content. Neutrino Oscillations I ntroduction The T2K Experiment Beam Near Detector Far Detector Results Disappearance analysis Appearance search Future potential
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T2K ExperimentResults & Prospects Alfons Weber University of Oxford & STFC/RAL For the T2K Collaboration
Content • Neutrino Oscillations • Introduction • The T2K Experiment • Beam • Near Detector • Far Detector • Results • Disappearance analysis • Appearance search • Future potential • The hunt for CP-violation A.Weber, FLASY2014, Brighton
Mass eigenstates m1, m2, m3 weak“flavour eigenstates” Unitary mixing matrix: 3 mixing angles & complex phases Neutrino MixingThe PMNS Matrix • Assume that neutrinos do have mass: • mass eigenstates weak interaction eigenstates • Analogue to CKM-Matrix in quark sector! Pontecorvo-Maki-Nakagawa-Sakata A.Weber, FLASY2014, Brighton
Oscillation Signatures eappearance: determine 13constrain dCP disappearance: determine 23 and m232 Events Ratio of obs/expected Reconstructed ν Energy (MeV) Reconstructed ν Energy (MeV) Reconstructed ν Energy (MeV) A.Weber, FLASY2014, Brighton
The T2K Experiment • A Long-baseline Experiment to study neutrino oscillations • Baseline 295 km • Beam power up to 230 kW • Detectors Near and far A.Weber, FLASY2014, Brighton
Producing Neutrinos off-axis (2.5°) (30 GeV from MR synchrotron) π→μν 118 m Using NA61 data to constrain hadron production 0º A.Weber, FLASY2014, Brighton
Data Taken • Data Set: 6.57 x 1020PoT (8% of design goal) • Increase power in future • More protons / bunch • Higher repetition rate A.Weber, FLASY2014, Brighton
ND280 detector TPC1 TPC2 TPC3 νμ FGD2 FGD1 • Off-axis: ND280 • 0.2 T magnet (UA1/NOMAD) • Plastic scintillator detectors:Fine Grained Detector (FGD), π0detector (P0D), ECalsand SMRD,Time projection chambers (TPC) • On-axis: INGRID A.Weber, FLASY2014, Brighton
Some ND distribution CC 1π+ CC 0π CC Other BEFORE FIT AFTER FIT • Select different event classes in near detector • Negative muon & something/nothing • Constrains flux and cross section uncertainties A.Weber, FLASY2014, Brighton
Reduced Systematics A.Weber, FLASY2014, Brighton
Far Detector A.Weber, FLASY2014, Brighton
Far Detector Events A.Weber, FLASY2014, Brighton
Electron Neutrino Appearance • Event Selection • Fully contained, • no π0 • No decay electrons A.Weber, FLASY2014, Brighton
Appearance Result Phys. Rev. Lett. 112, 061802 (2014) A.Weber, FLASY2014, Brighton
Compare with Reactors • Comparing with reactor measurements • best overlap is for the normal hierarchy δcp=–π/2. • Need to increase θ23to account for high event rate • Lucky point! Note: Marginalized over 23 and m232 A.Weber, FLASY2014, Brighton
Disappearance Measurement Maximal mixing is not the same as maximumdisappearance if θ13is not zero! 120 selected events NH: sin2(θ23) = 0.514 NH: Δm232 = 2.51x10-3 eV2 A.Weber, FLASY2014, Brighton
The World Scene A.Weber, FLASY2014, Brighton
Putting it All Together A.Weber, FLASY2014, Brighton
Run Status The width of the beam is comparable to the measured Gaussians in the previous runs. Measured with INGRID The detectors are all working well. Here is our first identified anti-neutrino event from an anti-neutrino test run! μ+ ND280 anti-ν event A.Weber, FLASY2014, Brighton
Future Sensitivity “Lucky! (+: Sin22θ=0.1, δCP=-90)” NH 50% ν/50% anti-ν (true NH) 100% ν (true NH) T2K: 50% ν/50% anti-ν 100% ν (true NH) w/ Reactor constraint 50% ν/50% anti-ν (true NH) w/ Reactor constraint No systematics 5% error on signal, 10% on background T2K best sensitivity: 50% ν/50% anti-ν Anti-nu running: large new physics program. A.Weber, FLASY2014, Brighton
Future Sensitivity (II) “Unlucky! (+: Sin22θ=0.1, δCP=0)” 50% ν/50% anti-ν (true NH) 100% ν (true NH) 50% ν/50% anti-ν (true NH) w/ Reactor constraint 100% ν (true NH) w/ Reactor constraint A.Weber, FLASY2014, Brighton
T2K and NOvA T2K: 50% ν/50% anti-ν NH IH No systematics 5% error on signal, 10% on background A.Weber, FLASY2014, Brighton
Summary and Conclusion • T2K has taken 8% of its nominal PoT • World leading results • 7.3σ electron neutrino appearance • Most precise measurement of θ23 • Combination with reactor measurements • Hint that δCP = -π/2 • Improved sensitivity with data to come • Can be lucky to “discover” CP violation • More results to come • Cross sections, sterile neutrinos, exotics… A.Weber, FLASY2014, Brighton
Who is Who νμ disappearance Solar neutrino oscillation ν–less double beta decay νedisappearance inνμbeam Or reactor neutrino experiments A.Weber, FLASY2014, Brighton
Ubies? Open questions: Normal Hierarchy or Inverted Hierarchy? A.Weber, FLASY2014, Brighton
NA61/SHINE ~13m ~10m • hadron(π, K) yield • 30 GeV p + C • High-acceptance • ToFsand spectrometers • 2cm thin target (4%λI) • π+ analysis: • dE/dx only analysis low momenta (Phys.Rev.C84.2011.034604) • dE/dx+ToFanalysishigh momenta(Phys.Rev.C85.2011.035210) A.Weber, FLASY2014, Brighton
Predicted Flux νμ νe νμ • Primary pions modelled with NA61 data • νμ flux • Pions dominant at low energy • Kaons important in tail • νeflux • For low energy from muons A.Weber, FLASY2014, Brighton
CC Interaction A.Weber, FLASY2014, Brighton