New general models for substrate and coating mechanical, thermoelastic, and thermorefractive noise in Michelson interferometers at high frequencies, validated against prior low-frequency models and Holometer data, then applied to GQuEST.
On vacuum fluctuations in quantum gravity and interferometer arm fluctuations,
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
verdicts
UNVERDICTED 3representative citing papers
Computes UV-finite noise spectra in interferometers from graviton fluctuations in vacuum/thermal/squeezed states and from massless scalar vacuum stress-energy, all Planck-suppressed.
Standard low-energy quantum gravity via effective graviton QFT predicts interferometer length variations of order the Planck length (~10^{-35} m), with no divergences indicating breakdown.
citing papers explorer
-
High-Frequency Thermal Noise in Michelson Interferometers
New general models for substrate and coating mechanical, thermoelastic, and thermorefractive noise in Michelson interferometers at high frequencies, validated against prior low-frequency models and Holometer data, then applied to GQuEST.
-
Geometric noise spectrum in interferometers
Computes UV-finite noise spectra in interferometers from graviton fluctuations in vacuum/thermal/squeezed states and from massless scalar vacuum stress-energy, all Planck-suppressed.
-
Response of interferometers to the vacuum of quantum gravity
Standard low-energy quantum gravity via effective graviton QFT predicts interferometer length variations of order the Planck length (~10^{-35} m), with no divergences indicating breakdown.