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      Extricating New Physics Scenarios at DUNE with Higher Energy Beams

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      1 , 2 , , 3 , , 4 ,
      Scientific Reports
      Nature Publishing Group UK

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          Abstract

          The proposed Deep Underground Neutrino Experiment (DUNE) utilizes a wide-band on-axis tunable muon-(anti)neutrino beam with a baseline of 1300 km to search for CP violation with high precision. Given the long baseline, DUNE is also sensitive to effects due to matter induced non-standard neutrino interactions (NSI) which can interfere with the standard three-flavor oscillation paradigm. Hence it is desirable to design strategies to disentangle effects due to NSI from standard oscillations. In this article, we exploit the tunability of the DUNE neutrino beam over a wide-range of energies to devise an experimental strategy for separating oscillation effects due to NSI from the standard three-flavor oscillation scenario. Using χ 2 analysis, we obtain an optimal combination of beam tunes and distribution of run times in neutrino and anti-neutrino modes that would enable DUNE to isolate new physics scenarios from the standard. We can distinguish scenarios at 3 σ (5 σ) level for almost all (~50%) values of δ. To the best of our knowledge, our strategy is entirely new and has not been reported elsewhere.

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          Most cited references30

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          Simulation of long-baseline neutrino oscillation experiments with GLoBES

          We present the GLoBES (``General Long Baseline Experiment Simulator'') software package, which allows the simulation of long-baseline and reactor neutrino oscillation experiments. One part of the software is the abstract experiment definition language to define experiments with beam and full detector descriptions as accurate as possible. Many systematics options are provided, such as normalization and energy calibration errors, or the choice between spectral or total rate information. For the definition of experiments, a new transparent building block concept is introduced. In addition, an additional program provides the possibility to develop and test new experiment definitions quickly. Another part of GLoBES is the user's interface, which provides probability, rate, and \(\Delta \chi^2\) information for a given experiment or any combination of up to 32 experiments in C. Especially, the \(\Delta \chi^2\) functions allow a simulation with statistics only, systematics, correlations, and degeneracies. In particular, GLoBES can handle the full multi-parameter correlation among the oscillation parameters, external input, and matter density uncertainties.
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            Status of non-standard neutrino interactions

            (2013)
            The phenomenon of neutrino oscillations has been established as the leading mechanism behind neutrino flavor transitions, providing solid experimental evidence that neutrinos are massive and lepton flavors are mixed. Here we review sub-leading effects in neutrino flavor transitions known as non-standard neutrino interactions, which is currently the most explored description for effects beyond the standard paradigm of neutrino oscillations. In particular, we report on the phenomenology of non-standard neutrino interactions and their experimental and phenomenological bounds as well as future sensitivity and discovery reach.
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              General bounds on non-standard neutrino interactions

              We derive model-independent bounds on production and detection non-standard neutrino interactions (NSI). We find that the constraints for NSI parameters are around O(10^{-2}) to O(10^{-1}). Furthermore, we review and update the constraints on matter NSI. We conclude that the bounds on production and detection NSI are generally one order of magnitude stronger than their matter counterparts.
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                Author and article information

                Contributors
                masud@ific.uv.es
                mbishai@bnl.gov
                pm@jnu.ac.in
                Journal
                Sci Rep
                Sci Rep
                Scientific Reports
                Nature Publishing Group UK (London )
                2045-2322
                23 January 2019
                23 January 2019
                2019
                : 9
                : 352
                Affiliations
                [1 ]Astroparticle and High Energy Physics Group, Institut de Física Corpuscular – C.S.I.C./Universitat de València, Parc Cientific de Paterna., C/Catedratico José Beltrán, 2E-46980 Paterna, València Spain
                [2 ]ISNI 0000 0004 0610 8047, GRID grid.450311.2, Harish-Chandra Research Institute, ; Chattnag Road, Allahabad, 211 019 India
                [3 ]ISNI 0000 0001 2188 4229, GRID grid.202665.5, Brookhaven National Laboratory, ; P.O. Box 5000, Upton, NY 11973 USA
                [4 ]ISNI 0000 0004 0498 924X, GRID grid.10706.30, School of Physical Sciences, , Jawaharlal Nehru University, ; New Delhi, 110067 India
                Article
                36790
                10.1038/s41598-018-36790-6
                6344638
                30674996
                a2e6aa63-1041-40bb-8aa8-e21cf1ddda2e
                © The Author(s) 2019

                Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.

                History
                : 23 January 2018
                : 16 November 2018
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