Structural thermal noise in gram-scale mirror oscillators

Structural thermal noise in gram-scale mirror oscillators

The thermal noise associated with mechanical dissipation is a ubiquitous limitation to the sensitivity of precision experiments ranging from frequency stabilization to gravitational wave interferometry. We report on the thermal noise limits to the performance of 1 gm mirror oscillators that are part...

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Bibliographic Details
Main Authors: Neben, Abraham Richard (Contributor), Bodiya, Timothy Paul (Contributor), Wipf, Christopher (Contributor), Oelker, Eric Glenn (Contributor), Corbitt, Thomas R. (Contributor), Mavalvala, Nergis (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor), LIGO (Observatory : Massachusetts Institute of Technology) (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2013-04-03T13:46:20Z.
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