2004/08/05 by Olga Mena, Stephen Parke · 11 citations
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Neutrino Physics Research #Particle physics theoretical and experimental studies #hep-ph
paper · pdf · doi:10.1103/physrevd.70.093011
published as Phys.Rev.D70:093011,2004 · 15 pages, Latex, 4 postscript figures. Submitted to New Journal of Physics, ``Focus on Neutrino Physics'' issue
arxiv created 2004/08/05 · openalex publication_date 2004/11/18 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/01
In the overlap region, for the normal and inverted hierarchies, of the neutrino-antineutrino bi-probability space for \ensuremathν_\ensuremathμ\ensuremath→\ensuremathνe appearance, we derive a simple identity between the solutions in the (sin22\ensuremathθ13, sin\ensuremathδ) plane for the different hierarchies. The parameter sin22\ensuremathθ13 sets the scale of the \ensuremathν_\ensuremathμ\ensuremath→\ensuremathνe appearance probabilities at the atmospheric \ensuremathδmatm2\ensuremath≈2.4\ifmmode×\else\texttimes\fi10^\ensuremath-3 eV2 whereas sin\ensuremathδ controls the amount of CP violation in the lepton sector. The identity between the solutions is that the difference in the values of sin\ensuremathδ for the two hierarchies equals twice the value of √sin22\ensuremathθ13 divided by the critical value of √sin22\ensuremathθ13. We apply this identity to the two proposed long baseline experiments, T2K and NOvA, and we show how it can be used to provide a simple understanding of when and why fake solutions are excluded when two or more experiments are combined. This identity demonstrates the true complementarity of T2K and NOvA.