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  The AEI 10 m Prototype Interferometer frequency control using the reference cavity and its angular control

Kawazoe, F., Bergmann, G., Bertolini, A., Born, M., Chen, Y., Cummning, A. V., et al. (2012). The AEI 10 m Prototype Interferometer frequency control using the reference cavity and its angular control. Journal of Physics: Conference Series, 363: 012012.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-000F-A49D-4 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-000F-A49E-2
Genre: Conference Paper

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JoPCS_363_1_012012.pdf (Any fulltext), 579KB
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 Creators:
Kawazoe, Fumiko1, Author              
Bergmann, Gerald, Author
Bertolini, Alessandro1, Author              
Born, Michael1, Author              
Chen, Yanbei, Author
Cummning, Alan V, Author
Cunningham, Liam, Author
Dahl, Katrin1, Author              
Gräf, Christian1, Author              
Hammond, Giles, Author
Heinzel, Gerhard1, Author              
Hild, Stefan1, Author              
Huttner, Sabina H, Author
Jones, Russell, Author
Köhlenbeck, Sina, Author
Kühn, Gerrit1, Author              
Lück, Harald1, Author              
Mossavi, Kasem1, Author              
Pöld, Jan Hendrik1, Author              
Somiya, Kentaro1, Author              
van Veggel, A Marielle, AuthorWanner, Alexander1, Author              Westphal, Tobias1, Author              Willke, Benno1, Author              Strain, Kenneth A.1, Author              Goßler, Stefan1, Author              Danzmann, Karsten1, Author               more..
Affiliations:
1Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, escidoc:24010              

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 Abstract: The main purpose of the AEI 10 m Prototype is to reach and eventually surpass the Standard Quantum Limit at frequencies ranging from 20 Hz to 1 kHz with a 10 m arm-length Michelson interferometer named the sub-SQL interferometer. The frequency control system uses a 20 m optical path length triangular suspended cavity named the reference cavity, with the goal of suppressing frequency noise of the input laser to a level of ~ 10-4 Hz/ at 20 Hz rolling off to below 6 × 10-6 Hz/ above 1 kHz. It is expected that tight angular control of the reference cavity's mirrors is necessary to reach this stringent requirement.

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 Dates: 2012
 Publication Status: Published in print
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 Identifiers: DOI: 10.1088/1742-6596/363/1/012012
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Title: 9th Edoardo Amaldi conference on gravitational waves (Amaldi 9) and the 2011 Numerical Relativity – Data Analysis meeting (NRDA 2011)
Place of Event: Cardiff
Start-/End Date: 2011-07-10 - 2011-07-15

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Title: Journal of Physics: Conference Series
Source Genre: Journal
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Publ. Info: Bristol : IOP Publ.
Pages: - Volume / Issue: 363 Sequence Number: 012012 Start / End Page: - Identifier: ISSN: 1742-6588
CoNE: http://pubman.mpdl.mpg.de/cone/journals/resource/111097776606042