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.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 | 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.classification | Konferenzschrift | ger |
dc.subject.ddc | 530 | Physik | ger |
dc.title | Building blocks for future detectors: Silicon test masses and 1550 nm laser light | eng |
dc.type | Article | |
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 |
Die folgenden Lizenzbestimmungen sind mit dieser Ressource verbunden: