Expand this Topic clickable element to expand a topic
Skip to content
Optica Publishing Group

Thermal Noise in Mirror Coatings for Gravitational Wave Detection

Not Accessible

Your library or personal account may give you access

Abstract

Mid-band sensitivity of gravitational-wave detectors is limited by Brownian noise in interferometer mirrors. We discuss connections between thermal noise and elastic dissipation in mirrors, and between that dissipation and the structure of amorphous films.

© 2017 Optical Society of America

PDF Article
More Like This
Thermal Noise in Mirror Coatings for Gravitational Wave Detection

M.M. Fejer and
MB.1 Optical Interference Coatings (OIC) 2016

Progress in the measurement and reduction of thermal noise in optical coatings for gravitational-wave detectors

M. Granata, A. Amato, G. Cagnoli, M. Coulon, J. Degallaix, D. Forest, L. Mereni, C. Michel, L. Pinard, B. Sassolas, and J. Teillon
FA.1 Optical Interference Coatings (OIC) 2019

Low thermal noise TiO2-doped GeO2 for gravitational wave detectors

Aaron Davenport, Gabriele Vajente, Nicholas Demos, Le Yang, Mariana Fazio, Alena Ananyeva, GariLynn Billingsley, François Schiettekatte, Martin Chicoine, Ashot Markosyan, Riccardo Bassiri, Martin M. Fejer, Slawek Gras, Mathew Evans, and Carmen S. Menoni
SF3O.3 CLEO: Science and Innovations (CLEO:S&I) 2022

Select as filters


Select Topics Cancel
© Copyright 2024 | Optica Publishing Group. All Rights Reserved