Systematic error in the internal friction measurement of coatings for gravitational wave detectors

Citations Over Time

Abstract

Low internal friction coatings are key components of advanced technologies such as optical atomic clocks and high-finesse optical cavities and often lie at the forefront of the most advanced experiments in physics. Notably, increasing the sensitivity of gravitational-wave detectors depends in a very large part on developing new coatings, which entails developing more suitable methods and models to investigate their loss angle. In fact, the most sensitive region of the detection band in such detectors is limited by the coating thermal noise, which is related to the loss angle of the coating. Until now, models which describe only ideal physical properties have been adopted, wondering about the use of one or more loss angles to describe the mechanical properties of coatings. Here we show the presence of a systematic error ascribed to inhomogeneity of the sample at its edges in measuring the coating loss angle. We present a model for disk-shaped resonators, largely used in loss angle measurements, and we compare the theory with measurements showing how this systematic error impacts on the accuracy with which the loss model parameters are known.

Related Papers

• → High Finesse Opto-Mechanical Cavity with a Movable Thirty-Micron-Size Mirror(2006)72 cited
• → High-finesse (Al,Ga)As interference filters grown by molecular beam epitaxy(1988)37 cited
• → High-finesse large band Fabry-Perot fibre filter with superimposed chirped Bragg gratings(2002)25 cited
• → Versatile micro-fabricated mirrors with finesse >700,000(2021)2 cited
• → High-finesse optical enhancement cavity and its finesse measurement(2023)