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arXiv · 0903.4129

Level of holographic noise in interferometry

Igor I. Smolyaninov
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Abstract

The level of holographic noise expected to be observed in interferometric gravitational wave detectors such as GEO600 is re-examined. It is demonstrated that earlier estimates are based on assumed linear diffractive behavior of Planck radiation. Since nonlinear effects, such as self-focusing, are expected to appear at much lower energies, the expected level of holographic noise must be reduced by many orders of magnitude.

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Igor I. Smolyaninov. 2009-03-24. Level of holographic noise in interferometry. https://doi.org/10.1103/physrevd.79.087503

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