A geodesic interferometer with a single photon in Kerr spacetime uses combined time-delay and polarization-rotation phases to estimate specific angular momentum with uncertainty characterization.
For this, we define the following quantities Λ =c 2|h||l|, Γ =m 2 cos2(θ), and Ω = 2σ 2 +ω 2
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The role of Wigner rotation in estimating the specific angular momentum of a Kerr spacetime
A geodesic interferometer with a single photon in Kerr spacetime uses combined time-delay and polarization-rotation phases to estimate specific angular momentum with uncertainty characterization.