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Journal Article

DUNE as the Next-Generation Solar Neutrino Experiment

MPS-Authors

Capozzi,  Francesco
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Li,  Shirley Weishi
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Zhu,  Guanying
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Beacom,  John F.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

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Citation

Capozzi, F., Li, S. W., Zhu, G., & Beacom, J. F. (2019). DUNE as the Next-Generation Solar Neutrino Experiment. Physical Review Letters, 123, 131803. Retrieved from https://publications.mppmu.mpg.de/?action=search&mpi=MPP-2018-214.


Cite as: https://hdl.handle.net/21.11116/0000-0005-D683-5
Abstract
We show that the Deep Underground Neutrino Experiment (DUNE) has the potential to deliver world-leading results in solar neutrinos. Significant but realistic new efforts would be required. With an exposure of 100 kton-year, DUNE could detect $\gtrsim 10^5$ signal events above 5 MeV. Separate precision measurements of neutrino-mixing parameters and the $^8$B flux could be made using two detection channels ($\nu_e + \, ^{40}$Ar and $\nu_{e,\mu,\tau} + e^-$) and the day-night effect ($> 10 \sigma$). New particle physics may be revealed through the comparison of solar neutrinos (with matter effects) and reactor neutrinos (without), which is discrepant by $\sim 2 \sigma$ (and could become $5.6 \sigma$). New astrophysics may be revealed through the most precise measurement of the $^8$B flux (to 2.5%) and the first detection of the hep flux (to 11%). DUNE is required: No other experiment, even proposed, has been shown capable of fully realizing these discovery opportunities.