Gain fractions of future neutrino oscillation facilities over T2K and NOvA
arXiv:1303.0003 · doi:10.1007/JHEP07(2013)159
Abstract
We evaluate the probability of future neutrino oscillation facilities to discover leptonic CP violation and/or measure the neutrino mass hierarchy. We study how this probability is affected by positive or negative hints for these observables to be found at T2K and NOvA. We consider the following facilities: LBNE; T2HK; and the 10 GeV Neutrino Factory (NF10), and show how their discovery probabilities change with the running time of T2K and NOvA conditioned to their results. We find that, if after 15 years T2K and NOvA have not observed a 90% CL hint of CP violation, then LBNE and T2HK have less than a 10% chance of achieving a 5sigma discovery, whereas NF10 still has a ca 40% chance to do so. Conversely, if T2K and NOvA have an early 90% CL hint in 5 years from now, T2HK has a rather large chance to achieve a 5sigma CP violation discovery (75% or 55%, depending on whether the mass hierarchy is known or not). This is to be compared with the 90% (30%) probability that NF10 (LBNE) would have to observe the same signal at 5sigma. A hierarchy measurement at 5sigma is achievable at both LBNE and NF10 with more than 90% probability, irrespectively of the outcome of T2K and NOvA. We also find that if LBNE or a similar very long baseline super-beam is the only next generation facility to be built, then it is very useful to continue running T2K and NOvA (or at least T2K) beyond their original schedule in order to increase the CP violation discovery chances, given their complementarity.
JHEP style, 23 pages, 9 pdf figures
References in corpus (23)
- Observation of electron-antineutrino disappearance at Daya Bay
- Indication of Electron Neutrino Appearance from an Accelerator-produced Off-axis Muon Neutrino Beam
- Measurement of Neutrino Oscillation by the K2K Experiment
- New features in the simulation of neutrino oscillation experiments with GLoBES 3.0
- Measurement of the solar neutrino capture rate with gallium metal. III: Results for the 2002--2007 data-taking period
- Global status of neutrino oscillation parameters after Neutrino-2012
- Global fit to three neutrino mixing: critical look at present precision
- Solar neutrino measurements in Super-Kamiokande-II
- NOvA Proposal to Build a 30 Kiloton Off-Axis Detector to Study Neutrino Oscillations in the Fermilab NuMI Beamline
- Physics potential of the CERN-MEMPHYS neutrino oscillation project
- Determining the Neutrino Mass Hierarchy with INO, T2K, NOvA and Reactor Experiments
- Experimental Requirements to Determine the Neutrino Mass Hierarchy Using Reactor Neutrinos
- Statistical Evaluation of Experimental Determinations of Neutrino Mass Hierarchy
- Mass hierarchy, 2-3 mixing and CP-phase with Huge Atmospheric Neutrino Detectors
- Systematic uncertainties in long-baseline neutrino oscillations for large
- Potential of optimized NOvA for large theta(13) & combined performance with a LArTPC & T2K
- A low energy neutrino factory for large
- Mass hierarchy discrimination with atmospheric neutrinos in large volume ice/water Cherenkov detectors
- What is the probability that and CP violation will be discovered in future neutrino oscillation experiments?
- Exploring the Earth matter effect with atmospheric neutrinos in ice
- The -contamination of the golden muon sample at the Neutrino Factory
- Medium Baseline Reactor Neutrino Experiments with 2 Identical Detectors
- Measurements of the CKM angle gamma in tree-dominated decays at LHCb
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- Quantifying the sensitivity of oscillation experiments to the neutrino mass ordering
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- New look at the degeneracies in the neutrino oscillation parameters, and their resolution by T2K, NOA and ICAL
- Testing atmospheric mixing sum rules at precision neutrino facilities
- On the Bayesian approach to neutrino mass ordering
- Exploring the three flavor effects with future superbeams using liquid argon detectors
- Synergies between neutrino oscillation experiments: An `adequate' configuration for LBNO