Neutrinos have two properties that make them fairly unique from other known particles: extremely low cross sections and flavor changing oscillations. With a good knowledge of the oscillation parameters soon in hand, it will become possible to detect low-energy atmospheric neutrinos sensitive to the forward elastic scattering off electrons in the Earth’s core providing a measurement of the core properties and the matter effect itself. As the dynamics of the Earth’s core are complicated and in a difficult to probe environment, additional information from upcoming neutrino experiments will provide feedback into our knowledge of geophysics as well as useful information about exoplanet formation and various new physics scenarios including dark matter. In addition, we can probe the existence of the matter effect in the Earth and constrain the nonstandard neutrino interaction parameter ${\epsilon }_{ee}^{\oplus }$. We show how DUNE’s sensitivity to low-energy atmospheric neutrino oscillations can provide a novel constraint on the density and radius of the Earth’s core at the 9% level and the Earth’s matter effect at the 5% level. Finally, we illuminate the physics behind low-energy atmospheric neutrino resonances in the Earth.

• Received 12 October 2021
• Accepted 8 December 2021

DOI:https://doi.org/10.1103/PhysRevD.104.113007

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP³.

Published by the American Physical Society