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Neutrino flavor oscillations without flavor mixing angles

2000/08/31 by Keith R. Dienes, Ina Sarčević, Ina Sarcevic · 3 citations
Chemistry · Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Brane #Chemistry #Coupling (piping) #Flavor #Limit (mathematics) #Measurements of neutrino speed #Mixing (physics) #Neutrino #Neutrino Physics Research #Neutrino oscillation #Particle physics #Particle physics theoretical and experimental studies #Phenomenology (philosophy) #Physics #Quantum mechanics #Solar neutrino #Theoretical physics #hep-ph

paper · pdf · doi:10.1016/s0370-2693(01)00053-3

published as Phys.Lett. B500 (2001) 133-141 · 11 pages, LaTeX, 4 figures, version submitted to Phys. Lett. B

arxiv created 2000/09/15 · openalex publication_date 2001/02/01 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

We demonstrate that sizable neutrino flavor oscillations can be generated in a model with large extra spacetime dimensions even if the physics on the brane is flavor-diagonal, the bulk neutrino theory is flavor-neutral, and the brane/bulk couplings are flavor-blind. This is thus a compact model for addressing neutrino flavor oscillations in higher dimensions. We also discuss several phenomenological aspects of the ``bulk-mediated'' neutrino oscillations inherent in this model, and show that this model contains some potentially important new phenomenological features in the limit of large brane/bulk coupling.

Citations

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