Level of holographic noise in interferometry

  title={Level of holographic noise in interferometry},
  author={Igor I. Smolyaninov},
  journal={Physical Review D},
The level of holographic noise expected to be observed in interferometric gravitational wave detectors such as GEO600 is reexamined. 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. 

The detection of low-energy Quantum Gravity fluctuations with entangled states

We propose a thought experiment to detect low-energy Quantum Gravity phenomena using Quantum Optical Information Technologies. Gravitational field perturbations, such as gravitational waves and