Building blocks for future detectors: Silicon test masses and 1550 nm laser light

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dc.identifier.uri http://dx.doi.org/10.15488/1415
dc.identifier.uri http://www.repo.uni-hannover.de/handle/123456789/1440
dc.contributor.author Schnabel, Roman
dc.contributor.author Britzger, M.
dc.contributor.author Brückner, F.
dc.contributor.author Burmeister, O.
dc.contributor.author Danzmann, Karsten
dc.contributor.author Dück, J.
dc.contributor.author Eberle, Tobias
dc.contributor.author Friedrich, Daniel
dc.contributor.author Lück, Harald
dc.contributor.author Mehmet, Moritz
dc.contributor.author Nawrodt, Ronny
dc.contributor.author Steinlechner, S.
dc.contributor.author Willke, Benno
dc.date.accessioned 2017-04-28T08:05:13Z
dc.date.available 2017-04-28T08:05:13Z
dc.date.issued 2010
dc.identifier.citation Schnabel, R.; Britzger, M.; Brückner, F.; Burmeister, O.; Danzmann, K. et al.: Building blocks for future detectors: Silicon test masses and 1550 nm laser light. In: Journal of Physics: Conference Series 228 (2010), 12029. DOI: https://doi.org/10.1088/1742-6596/228/1/012029
dc.description.abstract Current interferometric gravitational wave detectors use the combination of quasi-monochromatic, continuous-wave laser light at 1064 nm and fused silica test masses at room temperature. Detectors of the third generation, such as the Einstein-Telescope, will involve a considerable sensitivity increase. The combination of 1550 nm laser radiation and crystalline silicon test masses at low temperatures might be important ingredients in order to achieve the sensitivity goal. Here we compare some properties of the fused silica and silicon test mass materials relevant for decreasing the thermal noise in future detectors as well as the recent technology achievements in the preparation of laser radiation at 1064 nm and 1550 nm relevant for decreasing the quantum noise. We conclude that silicon test masses and 1550 nm laser light have the potential to form the future building blocks of gravitational wave detection. eng
dc.description.sponsorship DFG/EXC/QUEST
dc.description.sponsorship DFG/SFB/TR7
dc.description.sponsorship EC/FP7/2007-2013
dc.language.iso eng
dc.publisher Bristol : IOP Publishing Ltd.
dc.relation.ispartof 8th Edoardo Amaldi Conference on Gravitational Waves, June 21-26, 2009, New York, NY, USA
dc.relation.ispartofseries Journal of Physics: Conference Series 228 (2010)
dc.rights CC BY 3.0
dc.rights.uri https://creativecommons.org/licenses/by/3.0/
dc.subject 1064 nm eng
dc.subject 1550 nm eng
dc.subject Building blockes eng
dc.subject Crystalline silicons eng
dc.subject Gravitational wave detectors eng
dc.subject Gravitational-wave detection eng
dc.subject Laser lights eng
dc.subject Low temperatures eng
dc.subject Quasi-monochromatic eng
dc.subject Room temperature eng
dc.subject Sensitivity increase eng
dc.subject Third generation eng
dc.subject Gravitational effects eng
dc.subject Gravity waves eng
dc.subject Laser radiation eng
dc.subject Radiation detectors eng
dc.subject Silica eng
dc.subject Silicon detectors eng
dc.subject Testing eng
dc.subject Fused silica eng
dc.subject Gravitationswelle ger
dc.subject.ddc 530 | Physik ger
dc.title Building blocks for future detectors: Silicon test masses and 1550 nm laser light
dc.type article
dc.type conferenceObject
dc.type Text
dc.relation.issn 1742-6588
dc.relation.doi https://doi.org/10.1088/1742-6596/228/1/012029
dc.bibliographicCitation.volume 228
dc.bibliographicCitation.firstPage 12029
dc.description.version publishedVersion
tib.accessRights frei zug�nglich


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