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Published September 9, 2016 | Published
Journal Article Open

First Measurements of High Frequency Cross-Spectra from a Pair of Large Michelson Interferometers

Abstract

Measurements are reported of the cross-correlation of spectra of differential position signals from the Fermilab Holometer, a pair of co-located 39 m long, high power Michelson interferometers with flat, broadband frequency response in the MHz range. The instrument obtains sensitivity to high frequency correlated signals far exceeding any previous measurement in a broad frequency band extending beyond the 3.8 MHz inverse light crossing time of the apparatus. The dominant but uncorrelated shot noise is averaged down over 2 × 10⁸ independent spectral measurements with 381 Hz frequency resolution to obtain 2.1 × 10⁻²⁰ m/√H̅z̅ sensitivity to stationary signals. For signal bandwidths Δf > 11 kHz, the sensitivity to strain h or shear power spectral density of classical or exotic origin surpasses a milestone PSD_(δh) < tₚ where tₚ = 5.39 × 10⁻⁴⁴/Hz is the Planck time.

Additional Information

© 2016 American Physical Society. (Received 9 May 2016; published 9 September 2016) This work was supported by the Department of Energy at Fermilab under Contract No. DE-AC02-07CH11359 and the Early Career Research Program (FNAL FWP 11-03), and by grants from the John Templeton Foundation, the National Science Foundation (Grants No. PHY-1205254, No. DGE-0909667, No. DGE-0638477, and No. DGE-1144082), NASA (Grant No. NNX09AR38G), the Fermi Research Alliance, the Ford Foundation, the Kavli Institute for Cosmological Physics, University of Chicago/Fermilab Strategic Collaborative Initiatives, and the Universities Research Association Visiting Scholars Program. The Holometer team gratefully acknowledges the extensive support and contributions of Bradford Boonstra, Benjamin Brubaker, Marcin Burdzy, Herman Cease, Tim Cunneen, Steve Dixon, Bill Dymond, Valera Frolov, Jose Gallegos, Hank Glass, Emily Griffith, Hartmut Grote, Gaston Gutierrez, Evan Hall, Sten Hansen, Young-Kee Kim, Mark Kozlovsky, Dan Lambert, Scott McCormick, Erik Ramberg, Doug Rudd, Geoffrey Schmit, Alex Sippel, Jason Steffen, Sali Sylejmani, David Tanner, Jim Volk, William Wester, and James Williams for the design and construction of the apparatus.

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Published - PhysRevLett.117.111102.pdf

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August 22, 2023
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