In weak GW backgrounds, the dynamical, spin, and AB phases of charged spin-1/2 interferometers all respond to the same tidal scale through a common geometric kernel but via distinct physical couplings.
In this configu- ration, the tidal field is transverse and does not generate a source forA (1) 0 at leading order
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Semiclassical phases of charged spin-$1/2$ matter-wave interferometers in gravitational wave backgrounds
In weak GW backgrounds, the dynamical, spin, and AB phases of charged spin-1/2 interferometers all respond to the same tidal scale through a common geometric kernel but via distinct physical couplings.