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This paper focuses on the next detectors for gravitational wave astronomy which will be required after the current ground based detectors have completed their initial observations, and probably achieved the first direct detection of gravitational waves. The next detectors will need to have greater sensitivity, while also enabling the world array of detectors to have improved angular resolution to...
Thermal noise is a fundamental noise source in a range of precision measurement systems including interferometric gravitational wave detectors where it is particularly important at frequencies less than 100Hz. To achieve the sensitivity levels desired for the coming generation of Advanced gravitational wave detectors requires careful choices for the materials used in the mirror suspensions, mirror...
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