Energy-dependent neutrino mixing parameters at oscillation experiments

Neutrino mixing parameters are subject to quantum corrections and hence scale dependent. This means that the associated production detection of neutrinos need not coincide since these processes characterized by different energy scales. We show that, in presence relatively light new physics, dependence can lead observable consequences long-baseline neutrino oscillation experiments, such as T2K NOvA, telescopes like IceCube. discuss some experimental signatures this scenario, including zero-baseline flavor transitions, sources CP-invariance violation, apparent inconsistencies among measurements angles at experiments or channels. Finally, we present simple, ultraviolet-complete models masses which running matrix below weak scale.