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Wavefront Mapping for Absolute Atom Interferometry
Joseph Junca1,2, John Kitching1, William McGehee1
1National Institute of Standards and Technology, Boulder, Time and Frequency Division, Colorado 80305, USA.
Wavefront distortions in atom interferometry limit precision. This study introduces a method to measure and correct these distortions, paving the way for more accurate gravitational acceleration measurements.
Area of Science:
- Atomic physics
- Quantum optics
- Metrology
Background:
- Wavefront distortions in light-pulse atom interferometry introduce systematic uncertainty.
- Current limitations in measuring gravitational acceleration are at the 30 nm/s² level due to these distortions.
Purpose of the Study:
- To develop and demonstrate an in situ method for spatially resolving interferometer phase.
- To characterize and correct wavefront bias in Mach-Zehnder atom interferometers.
- To improve the precision of absolute gravitational acceleration measurements.
Main Methods:
- Utilized a Mach-Zehnder atom interferometer.
- Introduced controllable curvature to the Raman light using an adjustable collimation retro-reflector.
- Spatially resolved the interferometer phase to measure wavefront bias.
Main Results:
- Demonstrated measurement of bias due to parabolic wavefront curvature with 1 mrad uncertainty.
- Showed that finite-size corrections influence the measured phase curvature.
- Quantified the impact of wavefront distortions on atom interferometer measurements.
Conclusions:
- The developed measurement process can characterize and correct wavefront bias.
- This technique can reduce wavefront bias uncertainty below the nm/s² level in optimized atom interferometer gravimeters.
- Enables higher precision in absolute measurements of gravitational acceleration.
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