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A Prototype Atom Interferometer to Detect Dark Matter and Gravitational Waves

  • C. F. A. Baynham
  • , R. Hobson
  • , O. Buchmueller
  • , D. Evans
  • , L. Hawkins
  • , L. Iannizzotto-Venezze
  • , A. Josset
  • , D. Lee
  • , E. Pasatembou
  • , B. E. Sauer
  • , M. R. Tarbutt
  • , T. Walker
  • , O. Ennis
  • , U. Chauhan
  • , A. Brzakalik
  • , S. Dey
  • , S. Hedges
  • , B. Stray
  • , M. Langlois
  • , K. Bongs
  • T. Hird, S. Lellouch, M. Holynski, B. Bostwick, J. Chen, Z. Eyler, V. Gibson, T. L. Harte, C. C. Hsu, M. Karzazi, C. Lu, B. Millward, J. Mitchell, N. Mouelle, B. Panchumarthi, J. Scheper, U. Schneider, X. Su, Y. Tang, K. Tkalcec, M. Zeuner, S. Zhang, Y. Zhi, L. Badurina, A. Beniwal, D. Blas, J. Carlton, J. Ellis, C. McCabe, G. Parish, D. Pathak Govardhan, V. Vaskonen, T. Bowcock, K. Bridges, A. Carroll, J. Coleman, G. Elertas, S. Hindley, C. Metelko, H. Throssell, J. N. Tinsley, E. Bentine, M. Booth, D. Bortoletto, N. Callaghan, C. Foot, C. Gomez-Monedero, K. Hughes, A. James, T. Leese, A. Lowe, J. March-Russell, J. Sander, J. Schelfhout, I. Shipsey, D. Weatherill, D. Wood, M. G. Bason, K. Hussain, H. Labiad, A. L. Marchant, T. C. Thornton, T. Valenzuela, S. N. Balashov, P. Majewski, D. Newbold, M. G. D. van der Grinten, Z. Pan, Z. Tam, I. Wilmut, K. Clarke, A. Vick

Research output: Working paper/PreprintPreprint

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Abstract

The AION project has built a tabletop prototype of a single-photon long-baseline atom interferometer using the 87Sr clock transition - a type of quantum sensor designed to search for dark matter and gravitational waves. Our prototype detector operates at the Standard Quantum Limit (SQL), producing a signal with no unexpected noise beyond atom shot noise. Importantly, the detector remains at the SQL even when additional laser phase noise is introduced, emulating conditions in a long-baseline detector such as AION or AEDGE where significant laser phase deviations will accumulate during long atom interrogation times. Our results mark a key milestone in extending atom interferometers to long baselines. Such interferometers can complement laser-interferometer gravitational wave detectors by accessing the mid-frequency gravitational wave band around 1 Hz, and can search for physics beyond the Standard Model.
Original languageEnglish
PublisherarXiv
Number of pages22
DOIs
Publication statusPublished - 12 Apr 2025

Bibliographical note

V2: minor fixes of author list issues and references

Keywords

  • hep-ex
  • astro-ph.IM
  • gr-qc
  • hep-ph
  • physics.atom-ph

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