• Open Access

Quasi-Dirac neutrino oscillations at DUNE and JUNO

G. Anamiati, V. De Romeri, M. Hirsch, C. A. Ternes, and M. Tórtola
Phys. Rev. D 100, 035032 – Published 28 August 2019

Abstract

Quasi-Dirac neutrinos are obtained when the Lagrangian density of a neutrino mass model contains both Dirac and Majorana mass terms, and the Majorana terms are sufficiently small. This type of neutrino introduces new mixing angles and mass splittings into the Hamiltonian, which will modify the standard neutrino oscillation probabilities. In this paper, we focus on the case where the new mass splittings are too small to be measured, but new angles and phases are present. We perform a sensitivity study for this scenario for the upcoming experiments DUNE and JUNO, finding that they will improve current bounds on the relevant parameters. Finally, we also explore the discovery potential of both experiments, assuming that neutrinos are indeed quasi-Dirac particles.

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  • Received 10 July 2019

DOI:https://doi.org/10.1103/PhysRevD.100.035032

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

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

G. Anamiati1,*, V. De Romeri1,†, M. Hirsch1,‡, C. A. Ternes1,§, and M. Tórtola1,2,∥

  • 1Instituto de Física Corpuscular, CSIC-Universitat de València, 46980 Paterna, Spain
  • 2Departament de Física Teòrica, Universitat de València, 46100 Burjassot, Spain

  • *anamiati@ific.uv.es
  • deromeri@ific.uv.es
  • mahirsch@ific.uv.es
  • §chternes@ific.uv.es
  • mariam@ific.uv.es

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Issue

Vol. 100, Iss. 3 — 1 August 2019

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