Abstract

Neutrino oscillations in matter provide a unique probe of new physics. Leveraging the advent of neutrino appearance data from NOvA and T2K in recent years, we investigate the presence of CP-violating neutrino nonstandard interactions in the oscillation data. We first show how to very simply approximate the expected NSI parameters to resolve differences between two long-baseline appearance experiments analytically. Then, by combining recent NOvA and T2K data, we find a tantalizing hint of CP-violating NSI preferring a new complex phase that is close to maximal: ϕ_{eμ} or ϕ_{eτ}≈3π/2 with |ε_{eμ}| or |ε_{eτ}|∼0.2. We then compare the results from long-baseline data to constraints from IceCube and COHERENT.

Highlights

  • Introduction.—Neutrino oscillations have provided the only particle physics evidence for new physics beyond the standard model (BSM) to date [1,2], making it an excellent place to probe new physics scenarios

  • The environment may modify the phases due to an interaction. Such an interaction exists in the standard model (SM) and is called the Wolfenstein matter effect [3], wherein a neutrino in the electron state of the flavor basis experiences a potential with the background electrons via a charged-current (CC) interaction

  • In the same paper that pointed out the SM matter effect, Wolfenstein suggested the possibility of a new interaction that provides a matter effect, so-called neutrino nonstandard interactions (NSI) [3,4,5]

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Summary

Introduction

Introduction.—Neutrino oscillations have provided the only particle physics evidence for new physics beyond the standard model (BSM) to date [1,2], making it an excellent place to probe new physics scenarios. By diagonalizing U†M2U þ N, one finds the vacuum parameters that a long-baseline accelerator experiment would extract in the presence of NSI at a given energy.

Results
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