The Holometer: an instrument to probe Planckian quantum geometry
Abstract
This paper describes the Fermilab Holometer, an instrument for measuring correlations of position variations over a four-dimensional volume of space-time. The apparatus consists of two co-located, but independent and isolated, 40 m power-recycled Michelson interferometers, whose outputs are cross-correlated to 25 MHz. The data are sensitive to correlations of differential position across the apparatus over a broad band of frequencies up to and exceeding the inverse light crossing time, 7.6 MHz. A noise model constrained by diagnostic and environmental data distinguishes among physical origins of measured correlations, and is used to verify shot-noise-limited performance. These features allow searches for exotic quantum correlations that depart from classical trajectories at spacelike separations, with a strain noise power spectral density sensitivity smaller than the Planck time. The Holometer in current and future configurations is projected to provide precision tests of a wide class of models of quantum geometry at the Planck scale, beyond those already constrained by currently operating gravitational wave observatories.
Additional Information
© 2017 IOP Publishing Ltd. Received 24 November 2016, revised 1 February 2017. Accepted for publication 6 February 2017. Published 28 February 2017. 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. O.K. was supported by the Basic Science Research Program (Grant No. NRF-2016R1D1A1B03934333) of the National Research Foundation of Korea (NRF) funded by the Ministry of Education. 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, 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.Attached Files
Published - Chou_2017_Class._Quantum_Grav._34_065005.pdf
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Additional details
- Eprint ID
- 117782
- Resolver ID
- CaltechAUTHORS:20221108-543491000.3
- Department of Energy (DOE)
- DE-AC02-07CH11359
- Fermilab
- FNAL FWP 11-03
- John Templeton Foundation
- NSF
- PHY-1205254
- NSF Graduate Research Fellowship
- DGE-0909667
- NSF Graduate Research Fellowship
- DGE-1144082
- NASA
- NNX09AR38G
- Fermi Research Alliance
- Ford Foundation
- Kavli Institute for Cosmological Physics
- National Research Foundation of Korea
- NRF-2016R1D1A1B03934333
- Created
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2022-11-09Created from EPrint's datestamp field
- Updated
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2022-11-09Created from EPrint's last_modified field