Search for exotic contributions to atmospheric neutrino oscillations
G. Battistoni, Y. Becherini, S. Cecchini, M. Cozzi, H. Dekhissi, L. Esposito, G. Giacomelli, M. Giorgini, G. Mandrioli, S. Manzoor, A. Margiotta, L. Patrizii, V. Popa, M. Sioli, G. Sirri, M. Spurio, V. Togo
Abstract
The energy spectrum of neutrino-induced upward-going muons in MACRO was analysed in terms of relativity principles violating effects, keeping standard mass-induced atmospheric neutrino oscillations as the dominant effect. The data disfavor these possibilities even at a sub-dominant level; stringent 90% C.L. limits are placed on the Lorentz invariance violation parameter |Δv| < 6 × 10-24 at 2θv = 0 and |Δv| < 2.5 ÷5 × 10-26 at 2θv = 1. The limits can be re-interpreted as bounds on the Equivalence Principle violation parameters.
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