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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Main Authors: Neben, Abraham Richard, Bodiya, Timothy Paul, Wipf, Christopher, Oelker, Eric Glenn, Corbitt, Thomas R., Mavalvala, Nergis
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: IOP Publishing 2013
Online Access:http://hdl.handle.net/1721.1/78263
https://orcid.org/0000-0003-0219-9706
https://orcid.org/0000-0003-2815-7387
https://orcid.org/0000-0001-7776-7240
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author Neben, Abraham Richard
Bodiya, Timothy Paul
Wipf, Christopher
Oelker, Eric Glenn
Corbitt, Thomas R.
Mavalvala, Nergis
author2 Massachusetts Institute of Technology. Department of Physics
author_facet Massachusetts Institute of Technology. Department of Physics
Neben, Abraham Richard
Bodiya, Timothy Paul
Wipf, Christopher
Oelker, Eric Glenn
Corbitt, Thomas R.
Mavalvala, Nergis
author_sort Neben, Abraham Richard
collection MIT
description 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 of a cavity optomechanics experiment to observe quantum radiation pressure noise. Thermal noise limits the observed cavity displacement spectrum from 80 Hz to 5 kHz. We present a calculation of the thermal noise, based on finite element analysis of the dissipation due to structural damping, and find it to be in excellent agreement with the experimental result. We conclude with the predicted thermal noise for an improved oscillator design, which should be capable of revealing the noise that arises from quantum backaction in this system.
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spelling mit-1721.1/782632022-09-26T11:23:08Z Structural thermal noise in gram-scale mirror oscillators Neben, Abraham Richard Bodiya, Timothy Paul Wipf, Christopher Oelker, Eric Glenn Corbitt, Thomas R. Mavalvala, Nergis Massachusetts Institute of Technology. Department of Physics MIT Kavli Institute for Astrophysics and Space Research LIGO (Observatory : Massachusetts Institute of Technology) Neben, Abraham Richard Bodiya, Timothy Paul Wipf, Christopher Oelker, Eric Glenn Corbitt, Thomas R. Mavalvala, Nergis 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 of a cavity optomechanics experiment to observe quantum radiation pressure noise. Thermal noise limits the observed cavity displacement spectrum from 80 Hz to 5 kHz. We present a calculation of the thermal noise, based on finite element analysis of the dissipation due to structural damping, and find it to be in excellent agreement with the experimental result. We conclude with the predicted thermal noise for an improved oscillator design, which should be capable of revealing the noise that arises from quantum backaction in this system. National Science Foundation (U.S.) (Grant PHY-1068772) 2013-04-03T13:46:20Z 2013-04-03T13:46:20Z 2012-11 2012-07 Article http://purl.org/eprint/type/JournalArticle 1367-2630 http://hdl.handle.net/1721.1/78263 Neben, Abraham R et al. “Structural Thermal Noise in Gram-scale Mirror Oscillators.” New Journal of Physics 14.11 (2012): 115008. https://orcid.org/0000-0003-0219-9706 https://orcid.org/0000-0003-2815-7387 https://orcid.org/0000-0001-7776-7240 en_US http://dx.doi.org/10.1088/1367-2630/14/11/115008 New Journal of Physics Creative Commons Attribution 3.0 http://creativecommons.org/licenses/by-nc/3.0 application/pdf IOP Publishing IOP
spellingShingle Neben, Abraham Richard
Bodiya, Timothy Paul
Wipf, Christopher
Oelker, Eric Glenn
Corbitt, Thomas R.
Mavalvala, Nergis
Structural thermal noise in gram-scale mirror oscillators
title Structural thermal noise in gram-scale mirror oscillators
title_full Structural thermal noise in gram-scale mirror oscillators
title_fullStr Structural thermal noise in gram-scale mirror oscillators
title_full_unstemmed Structural thermal noise in gram-scale mirror oscillators
title_short Structural thermal noise in gram-scale mirror oscillators
title_sort structural thermal noise in gram scale mirror oscillators
url http://hdl.handle.net/1721.1/78263
https://orcid.org/0000-0003-0219-9706
https://orcid.org/0000-0003-2815-7387
https://orcid.org/0000-0001-7776-7240
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