Gravitomagnetic Sagnac Effect for Matter Waves: Atom Interferometry in the Lense–Thirring Field of a Rotating Mass
Norbert Levente Kis
Abstract
We derive the phase shift of a matter-wave interferometer in the gravitomagnetic field of a rotating body. By combining the Lense–Thirring metric in theweak-field, slow-rotation limit with the path-integral formulation of atom interferometry, we obtain an exact expression for the gravitomagnetic Sagnac phase:∆ϕ = (2m/ℏ) Ag · dl, where Ag is the gravitomagnetic vector potential. Foran Earth-orbiting atom interferometer, the predicted phase shift is ∆ϕ ∼ 10−1102 rad depending on the interferometer geometry and atomic species, placing itwithin reach of current cold-atom technology. A space-based implementation wouldimprove the sensitivity to the Lense–Thirring effect by two to three orders of magnitude compared to Gravity Probe B, providing a direct test of general relativitywith quantum systems