Within the semiclassical short-pulse approximation, exact flat-spacetime phase shifts are obtained for Mach-Zehnder, resonant, and LMT clock and two-photon atom interferometers, including the closed form ω_a(1+ω_a/2m)(e^{-gT/c}-1)^2 c/g.
Exact Semiclassical Phase Shifts for Relativistic Atom Interferometers in Flat Spacetime
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abstract
Atom interferometry is a sensitive tool for measuring relativistic effects, but there are no known non-trivial exact solutions for relativistic atom interferometer phase shifts. Here we derive relativistically exact expressions within the usual semiclassical approximation for a wide range of experimentally interesting atom interferometer pulse sequences in flat spacetime, including Mach-Zehnder, resonant, and large momentum transfer interferometer geometries. As an example, the leading order phase shift $\omega_a g T^2/c$ for a Mach-Zehnder clock atom interferometer is found to become $\omega_a \left(1 + \frac{\omega_a}{2m}\right)(e^{-gT/c}-1)^2 c/g$ when all relativistic kinematics are included. We calculate exact phase shifts for both clock (single-photon) interferometers and Raman or Bragg (two-photon) interferometers.
fields
physics.atom-ph 1years
2026 1verdicts
ACCEPT 1representative citing papers
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Exact Semiclassical Phase Shifts for Relativistic Atom Interferometers in Flat Spacetime
Within the semiclassical short-pulse approximation, exact flat-spacetime phase shifts are obtained for Mach-Zehnder, resonant, and LMT clock and two-photon atom interferometers, including the closed form ω_a(1+ω_a/2m)(e^{-gT/c}-1)^2 c/g.