Wavefront Mapping for Absolute Atom Interferometry
Wavefront Mapping for Absolute Atom Interferometry
Wavefront distortions are a leading source of systematic uncertainty in light-pulse atom interferom- etry, limiting absolute measurements of gravitational acceleration at the 30 nm/s$^2$ level. Here, we demonstrate in situ spatially resolved measurement of the interferometer phase in a Mach-Zehnder atom interferometer as a tool to characterize and correct wavefront bias. By introducing controllable curvature of the Raman light using an adjustable collimation retro-reflector, we show that the bias due to parabolic wavefront curvature can be measured with 1 mrad uncertainty and that finite-size corrections impact the measured phase curvature. This measurement process could be adopted in optimized atom interferometer gravimeters to reduce wavefront bias uncertainty below the nm/s$^2$ level.
Joseph Junca、John Kitching、William McGehee
物理学
Joseph Junca,John Kitching,William McGehee.Wavefront Mapping for Absolute Atom Interferometry[EB/OL].(2025-07-30)[2025-08-07].https://arxiv.org/abs/2507.23052.点此复制
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