Measurement of the mechanical loss of a cooled reflective coating for gravitational wave detection
arXiv:gr-qc/0601031 · doi:10.1103/PhysRevD.74.022002
Abstract
We have measured the mechanical loss of a dielectric multilayer reflective coating (ion-beam sputtered SiO and TaO) in cooled mirrors. The loss was nearly independent of the temperature (4 K 300 K), frequency, optical loss, and stress caused by the coating, and the details of the manufacturing processes. The loss angle was . The temperature independence of this loss implies that the amplitude of the coating thermal noise, which is a severe limit in any precise measurement, is proportional to the square root of the temperature. Sapphire mirrors at 20 K satisfy the requirement concerning the thermal noise of even future interferometric gravitational wave detector projects on the ground, for example, LCGT.
8 pages, 6 figures, 3 tables : accepted version (by Physical Review D)
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- Evaluation of heat extraction through sapphire fibers for the GW observatory KAGRA
- An ultra-low dissipation micro-oscillator for quantum opto-mechanics
- Thermal noise and mechanical loss of SiO/TaO optical coatings at cryogenic temperatures
- Coating thermal noise of a finite-size cylindrical mirror
- Technology for the next gravitational wave detectors
- Particle swarm optimization of the sensitivity of a cryogenic gravitational wave detector
- Effect of energy deposited by cosmic-ray particles on interferometric gravitational wave detectors
- Inhomogeneous mechanical losses in micro-oscillators with high reflectivity coating
- Parametric instabilities in the LCGT arm cavity
- A new method of probing mechanical losses of coatings at cryogenic temperatures
- Folding Gravitational-Wave Interferometers