dc.identifier.uri | http://dx.doi.org/10.15488/1419 | |
dc.identifier.uri | http://www.repo.uni-hannover.de/handle/123456789/1444 | |
dc.contributor.author | Kawazoe, Fumiko | |
dc.contributor.author | Taylor, John Robert | |
dc.contributor.author | Bertolini, Alessandro | |
dc.contributor.author | Born, Michael | |
dc.contributor.author | Chen, Yanbei | |
dc.contributor.author | Dahl, Katrin | |
dc.contributor.author | Gering, Daniel | |
dc.contributor.author | Goßler, Stefan | |
dc.contributor.author | Gräf, Christian | |
dc.contributor.author | Heinzel, Gerhard | |
dc.contributor.author | Hild, Stefan | |
dc.contributor.author | Kranz, Oliver | |
dc.contributor.author | Kühn, Gerrit | |
dc.contributor.author | Lück, Harald | |
dc.contributor.author | Mossavi, Kasem | |
dc.contributor.author | Schnabel, Roman | |
dc.contributor.author | Somiya, Kentaro | |
dc.contributor.author | Strain, Kenneth A. | |
dc.contributor.author | Wanner, Alexander | |
dc.contributor.author | Westphal, Tobias | |
dc.contributor.author | Willke, Benno | |
dc.contributor.author | Danzmann, Karsten | |
dc.date.accessioned | 2017-04-28T08:05:14Z | |
dc.date.available | 2017-04-28T08:05:14Z | |
dc.date.issued | 2010 | |
dc.identifier.citation | Kawazoe, F.; Taylor, J.R.; Bertolini, A.; Born, M.; Chen, Y. et al.: Designs of the frequency reference cavity for the AEI 10 m Prototype interferometer. In: Journal of Physics: Conference Series 228 (2010), 12028. DOI: https://doi.org/10.1088/1742-6596/228/1/012028 | |
dc.description.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/√Hz at 20 Hz dropping to below 10-6 Hz/√Hz at 1kHz. The proposed design to suppress the laser frequency noise with a ring cavity is described in this paper. | eng |
dc.language.iso | eng | |
dc.publisher | Bristol : IOP Publishing Ltd. | |
dc.relation.ispartofseries | Journal of Physics: Conference Series 228 (2010) | |
dc.rights | CC BY 3.0 Unported | |
dc.rights.uri | https://creativecommons.org/licenses/by/3.0/ | |
dc.subject | Detector sensitivity | eng |
dc.subject | Frequency reference | eng |
dc.subject | Laser frequency | eng |
dc.subject | Laser noise | eng |
dc.subject | Noise source | eng |
dc.subject | Ring cavities | eng |
dc.subject | Seismic noise | eng |
dc.subject | Standard quantum limits | eng |
dc.subject | Acoustic noise | eng |
dc.subject | Gravitational effects | eng |
dc.subject | Gravity waves | eng |
dc.subject | Interferometry | eng |
dc.subject | Interferometers | eng |
dc.subject | Gravitationswelle | ger |
dc.subject.classification | Konferenzschrift | ger |
dc.subject.ddc | 530 | Physik | ger |
dc.title | Designs of the frequency reference cavity for the AEI 10 m Prototype interferometer | eng |
dc.type | Article | |
dc.type | Text | |
dc.relation.issn | 1742-6588 | |
dc.relation.doi | https://doi.org/10.1088/1742-6596/228/1/012028 | |
dc.bibliographicCitation.volume | 228 | |
dc.bibliographicCitation.firstPage | 12028 | |
dc.description.version | publishedVersion | |
tib.accessRights | frei zug�nglich |
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