2016
DOI: 10.1103/physrevlett.117.111102
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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 colocated 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 d… Show more

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Cited by 51 publications
(63 citation statements)
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“…With Planck length normalization, the predicted signal is detectable. Assuming sensitivity similar to that already achieved with the Fermilab Holometer [8,15], a highly significant detection is expected after several hours of integration. With several hundred hours of data, the program should be able to probe an order of magnitude lower.…”
Section: E Bent Michelson Interferometersupporting
confidence: 63%
See 1 more Smart Citation
“…With Planck length normalization, the predicted signal is detectable. Assuming sensitivity similar to that already achieved with the Fermilab Holometer [8,15], a highly significant detection is expected after several hours of integration. With several hundred hours of data, the program should be able to probe an order of magnitude lower.…”
Section: E Bent Michelson Interferometersupporting
confidence: 63%
“…As in previous estimates of holographic geometrical fluctuations with similar displacement magnitude [9][10][11][12][13][14], directions in this model on scale R fluctuate on timescale ≈ R/c, with a variance of about ∆θ 2 R ≈ l P /R, which leads to a signal with a power spectral density of fractional displacement noise about equal to a Planck time [8]. However, purely rotational fluctuations would a E-mail: o.kwon@kaist.ac.kr arXiv:1607.03048v4 [gr-qc] 8 Jun 2017 2 not have been detected in current experiments that constrain holographic fluctuations with this sensitivity [15], due to their purely radial light paths. As shown below, a definitive signature of rotational correlations can be measured using modified experimental configurations.…”
Section: Introductionmentioning
confidence: 99%
“…As seen above, the component of light that propagates in a transverse direction accumulates an exotic phase displacement that grows like a Planck random walk. The predicted amplitude of the effect is large enough to detect with the sensitivity already achieved by a correlated, superluminally sampled dual interferometer system [10,11].…”
Section: Experimental Observablesmentioning
confidence: 97%
“…This maintains the same form of straightforward linearity used in the previous section, just with longer functional support. In particular, the maximum normalization of this model, corresponding to Ξ(τ = 0)/L = 2 P ≡ ct P / √ π, was used as a "baseline model" to estimate experimental sensitivity for design purposes and tested during the initial run of the Holometer [35,36]. Figure 5 shows the full range of models reflecting a generalized understanding of linearity in this framework of overlapping causal diamonds (and consistent with the constraints outlined in Section II B).…”
Section: B General Class: Models Spanning ±2lmentioning
confidence: 99%