Inference finds consistency between a neutrino flavor evolution model and Earth-based solar neutrino measurements

Caroline Laber-Smith, A. A. Ahmetaj, Eve Armstrong, A. Baha Balantekin, Amol V. Patwardhan, M. Margarette Sanchez, and Sherry Wong
Phys. Rev. D 107, 023013 – Published 17 January 2023

Abstract

We continue examining statistical data assimilation, an inference methodology, to infer solutions to neutrino flavor evolution, for the first time using real—rather than simulated—data. The model represents neutrinos streaming from the Sun’s center and undergoing a Mikheyev-Smirnov-Wolfenstein resonance in flavor space, due to the radially varying electron number density. The model neutrino energies are chosen to correspond to experimental bins in the Sudbury Neutrino Observatory and Borexino experiments, which measure electron-flavor survival probability at Earth. The procedure successfully finds consistency between the observed fluxes and the model, if the Mikheyev-Smirnov-Wolfenstein resonance—that is, flavor evolution due to solar electrons—is included in the dynamical equations representing the model.

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  • Received 12 October 2022
  • Accepted 8 December 2022

DOI:https://doi.org/10.1103/PhysRevD.107.023013

© 2023 American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

Caroline Laber-Smith1,*, A. A. Ahmetaj2,†, Eve Armstrong2,3,‡, A. Baha Balantekin1,§, Amol V. Patwardhan4,∥, M. Margarette Sanchez2,¶, and Sherry Wong5,**

  • 1Department of Physics, University of Wisconsin: Madison, Madison, Wisconsin 53706, USA
  • 2Department of Physics, New York Institute of Technology, New York, New York 10023, USA
  • 3Department of Astrophysics, American Museum of Natural History, New York, New York 10024, USA
  • 4SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
  • 5Department of Astronomy, University of Wisconsin: Madison, Madison, Wisconsin 53706, USA

  • *Corresponding author. labersmith@wisc.edu
  • aahmet03@nyit.edu
  • earmst01@nyit.edu
  • §baha@physics.wisc.edu
  • apatward@slac.stanford.edu
  • msanch11@nyit.edu
  • **bwong24@wisc.edu

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Issue

Vol. 107, Iss. 2 — 15 January 2023

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