Apparent multiple Delta m^2_32 in muon anti-neutrino and muon neutrino survival oscillations from non-standard interaction matter effect
arXiv:1006.5720 · doi:10.1103/PhysRevD.82.113010
Abstract
Neutrinos propagating through matter may participate in forward coherent neutral-current-like scattering arising from non-standard interactions as well as from the Mikheyev-Smirnov-Wolfenstein matter potential . We show that at fixed long baselines through matter of constant density, the non-standard interaction potential can contribute an additional term to the oscillation phase whose sign differs for $\anumu$ versus $\numu$ propagation in matter. Its presence can cause different apparent to be erroneously inferred on the basis of oscillations in vacuum, with values lying above (for $\anumu$) or below (for $\numu$) the actual for the case where is predominantly real-valued and of sign opposite to . An NSI scenario invoking only is shown to be capable of accounting for a disparity recently reported between oscillation survival for $\anumu$ and $\numu$ fluxes measured at by the MINOS experiment. Implications for mantle traversal by atmospheric neutrinos are examined. The NSI matter potential with non-maximal mixing could evade conventional atmospheric neutrino analyses which do not distinguish $\numu$ from $\anumu$ on an event-by-event basis.
arXiv comment7 pages, 5 figures. Accepted for publication in Physical Review D
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