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  Designs of the frequency reference cavity for the AEI 10m Prototype Interferometer

Kawazoe, F., Taylor, J., Bertolini, A., Born, M., Chen, Y., Dahl, K., et al. (2010). Designs of the frequency reference cavity for the AEI 10m Prototype Interferometer. Journal of Physics: Conference Series, 228(1): 012028. doi:10.1088/1742-6596/228/1/012028.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0012-644A-B Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0012-6451-A
Genre: Conference Paper

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 Creators:
Kawazoe, F.1, Author              
Taylor, J.1, Author              
Bertolini, Alessandro1, Author              
Born, Michael1, Author              
Chen, Yanbei2, Author              
Dahl, Katrin1, Author              
Gering, Daniel1, Author              
Gossler, S.1, Author              
Gräf, Christian1, Author              
Heinzel, G.1, Author              
Hild, Stefan1, Author              
Kranz, Oliver1, Author              
Kühn, Gerrit1, Author              
Lück, H.1, Author              
Mossavi, K.1, Author              
Schnabel, R.1, Author              
Somiya, K.1, Author              
Strain, K.1, Author              
Wanner, Alexander1, Author              
Westphal, Tobias1, Author              
Willke, B.1, Author              Danzmann, K.1, Author               more..
Affiliations:
1Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, escidoc:24010              
2Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, escidoc:24013              

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 Abstract: The AEI 10 m Prototype is in its designing phase and will provide a test-bed for very sensitive interferometric experiments, such as the sub-SQL interferometer. It will test new techniques to reach - and even surpass - the Standard Quantum Limit. The experience and knowledge that can be gained from this experiment can be applied to large-scale interferometric gravitational detectors to improve the detector sensitivities. In order for the sub-SQL interferometer to achieve the required sensitivity all limiting noise sources need to be suppressed sufficiently. Noise sources can include seismic noise, thermal noise, and laser noise; laser frequency noise will be the main focus of this document. The laser frequency noise will be suppressed to a level of 10-4 √ Hz at 20 Hz dropping to below 10-6 √ Hz at 1kHz. The proposed design to suppress the laser frequency noise with a ring cavity is described in this paper.

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Language(s): eng - English
 Dates: 2010-07-29
 Publication Status: Published online
 Pages: -
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 Rev. Method: Peer
 Identifiers: eDoc: 442384
ISSN: 1742-6596
DOI: 10.1088/1742-6596/228/1/012028
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Title: The 8th Edoardo Amaldi Conference on Gravitational Waves (Amaldi 8)
Place of Event: Columbia University, New York
Start-/End Date: 2009-06-22 - 2009-06-26

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Title: Journal of Physics: Conference Series
Source Genre: Journal
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Publ. Info: UK : IOP Publishing Ltd.
Pages: - Volume / Issue: 228 (1) Sequence Number: 012028 Start / End Page: - Identifier: CoNE: http://pubman.mpdl.mpg.de/cone/journals/resource/111097776606042