Neutrino flavor oscillations in a curved space-time
Luca Visinelli

TL;DR
This paper derives a general expression for neutrino flavor oscillation phase shifts in curved spacetime using WKB approximation, and applies it to black hole and cosmological models.
Contribution
It introduces a novel method to calculate neutrino phase shifts in arbitrary gravitational fields, extending previous flat spacetime analyses.
Findings
Derived a general phase shift formula for neutrinos in curved spacetime
Applied the formula to Kerr-Newman black hole and FRW cosmology
Provided insights into neutrino oscillations influenced by gravity
Abstract
Using a WKB approximation of the Dirac equation in a curved spacetime, we obtain the expression for the phase shift between two neutrino mass eigenstates in a generic gravitational field. We apply this expression to two specific space-time geometries, namely the Kerr-Newman metric describing a rotating and charged black hole, and the Friedmann-Robertson-Walker metric.
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