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      Testing NSI suggested by the solar neutrino tension in T2HKK and DUNE

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          Abstract

          It has been known that a tension between the mass-squared differences obtained from the solar neutrino and KamLAND experiments may be solved by introducing the Non-Standard flavor-dependent Interaction (NSI) in neutrino propagation. We discuss the possibility to test such a hypothesis by the future long baseline neutrino experiments T2HKK and DUNE. Assuming that NSI does not exist, we give the excluded region in the (\(\epsilon_D\), \(\epsilon_N\))-plane, where \(\epsilon_D\) and \(\epsilon_N\) are the parameters which appear in the solar neutrino analysis with NSI. It is found that the best-fit value from the solar neutrino and KamLAND data (global analysis) can be tested at more than 10\(\sigma\) (3\(\sigma\)) by the two experiments for most the parameter space.

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          Global constraints on absolute neutrino masses and their ordering

          Within the standard three-neutrino framework, the absolute neutrino masses and their ordering (either normal, NO, or inverted, IO) are currently unknown. However, the combination of current data coming from oscillation experiments, neutrinoless double beta decay searches, and cosmological surveys, can provide interesting constraints for such unknowns in the sub-eV mass range, down to O(0.1) eV in some cases. We discuss current limits on absolute neutrino mass observables by performing a global data analysis, that includes the latest results from oscillation experiments, neutrinoless double beta decay bounds from the KamLAND-Zen experiment, and constraints from representative combinations of Planck measurements and other cosmological data sets. In general, NO appears to be somewhat favored with respect to IO at the level of ~2 sigma, mainly by neutrino oscillation data (especially atmospheric), corroborated by cosmological data in some cases. Detailed constraints are obtained via the chi^2 method, by expanding the parameter space either around separate minima in NO and IO, or around the absolute minimum in any ordering. Implications for upcoming oscillation and non-oscillation neutrino experiments, including beta-decay searches, are also discussed.
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            Hints for leptonic CP violation or New Physics?

            One of the major open questions in the neutrino sector is the issue of leptonic CP violation. Current global oscillation data shows a mild preference for a large, potentially maximal value for the Dirac CP phase in the neutrino mixing matrix. In this letter, we point out that New Physics in the form of neutral-current like non-standard interactions with real couplings would likely yield a similar conclusion even if CP in the neutrino sector were conserved. Therefore, the claim for a discovery of leptonic CP violation will require a robust ability to test New Physics scenarios.
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              Which long-baseline neutrino experiments are preferable?

              We discuss the physics of superbeam upgrades, where we focus on T2KK, a NuMI beam line based experiment NOvA*, and a wide band beam (WBB) experiment independent of the NuMI beam line. For T2KK, we find that the Japan-Korea baseline helps resolve parameter degeneracies, but the improvement due to correlated systematics between the two detectors (using identical detectors) is only moderate. For an upgrade of NOvA with a liquid argon detector, we demonstrate that the Ash River site is preferred compared to alternatives, such as at the second oscillation maximum, and is the optimal site within the U.S. For a WBB experiment, we find that high proton energies and long decay tunnels are preferable. We compare water Cherenkov and liquid argon technologies, and find the break-even point in detector cost at about 4:1. In order to compare the physics potential of the different experimental configurations, we use the concept of exposure to normalize the performance. We find that experiments with WBBs are the best experimental concept. NOvA* could be competitive with sufficient luminosity. If \(\sin^2 2\theta_{13}\) > 0.01, a WBB experiment can perform better than a neutrino factory.
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                Author and article information

                Journal
                24 September 2017
                Article
                1709.08264
                b5d6ddbc-8ef6-4d30-a989-fc97f37ec87c

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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                9 pages, 4 figures, 2 tables
                hep-ph

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