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04/10/2026 | Press release | Archived content

Wavefront mapping for absolute atom interferometry

Published
April 10, 2026

Author(s)

Joseph Junca, John Kitching, William McGehee

Abstract

Wavefront distortions are a leading source of systematic uncertainty in light-pulse atom interferometry, limiting absolute measurements of gravitational acceleration at the 30 nm/s2 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. We introduce controllable curvature of the Raman light using an adjustable collimation retro-reflector, and we show that finite-size corrections impact the measured phase curvature as well as the integrated interferometer phase. The parabolic wavefront bias is measured with < 1 mrad of phase uncertainty, and this measurement process could be adopted in optimized atom interferometer gravimeters to reduce wavefront bias uncertainty below the nm/s2 level.
Citation
Physical Review Letters
Pub Type
Journals

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Keywords

atom interferometry, wavefront, optical aberrations

Citation

Junca, J. , Kitching, J. and McGehee, W. (2026), Wavefront mapping for absolute atom interferometry, Physical Review Letters, [online], https://tsapps.nist.gov/publication/get_pdf.cfm?pub_id=960317 (Accessed April 25, 2026)
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NIST - National Institute of Standards and Technology published this content on April 10, 2026, and is solely responsible for the information contained herein. Distributed via Public Technologies (PUBT), unedited and unaltered, on April 25, 2026 at 09:21 UTC. If you believe the information included in the content is inaccurate or outdated and requires editing or removal, please contact us at [email protected]