Level of holographic noise in interferometry

Details Level of holographic noise in interferometry Level of holographic noise in interferometry

2009-03-24

arxiv.org/abs/0903.4129v1

Phys.Rev.D79:087503,2009

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

2 pages

Scientific paper

10.1103/PhysRevD.79.087503

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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