Material loss angles from direct measurements of broadband thermal noise
arXiv:1501.06371 · doi:10.1103/PhysRevD.91.022005
Abstract
We estimate the loss angles of the materials currently used in the highly reflective test-mass coatings of interferometric detectors of gravitational waves, namely Silica, Tantala, and Ti-dop ed Tantala, from direct measurement of coating thermal noise in an optical interferometer testbench, the Caltech TNI. We also present a simple predictive theory for the material properties of amorphous glassy oxide mixtures, which gives results in good agreement with our measurements on Ti-doped Tantala. Alternative measure ment methods and results are reviewed, and some critical issues are discussed.
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- Structure and morphology of low mechanical loss TiO-doped TaO
- Audio-band Coating Thermal Noise Measurement for Advanced LIGO with a Multi-mode Optical Resonator
- Correlated evolution of structure and mechanical loss of a sputtered silica film
- Electric noise spectra of a near-surface nitrogen vacancy center diamond with a protective layer
- Brownian Thermal Noise in Functional Optical Surfaces
- Highly reflective low-noise etalon-based meta-mirror
- Minimum Noise Optical Coatings for Interferometric Detectors of Gravitational Waves
- Fabry -Perot filters with Tunable Josephson Junction Defects
- A new method of probing mechanical losses of coatings at cryogenic temperatures
- Switching Times in Fabry-Perot Measurements