Abstract
Our recent theoretical research [Phys. Lett. A 305 (2002) 18] showed that the actual thermal noise of mirrors with an inhomogeneous loss in interferometric gravitational wave detectors is largely different from the traditional evaluation by modal expansion. We have tested this prediction experimentally using an oscillator similar to a mirror. The experimental result was consistent with our previous Letter.
Original language | English |
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Pages (from-to) | 79-86 |
Number of pages | 8 |
Journal | Physics Letters, Section A: General, Atomic and Solid State Physics |
Volume | 321 |
Issue number | 2 |
DOIs | |
State | Published - 2004/01/26 |
Keywords
- Direct approach
- Drum
- Inhomogeneous loss
- Interferometric gravitational wave detector
- Modal expansion
- Thermal noise of mirror
ASJC Scopus subject areas
- General Physics and Astronomy