Design and construction of an optical test bed for LISA imaging systems and tilt-to-length coupling

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dc.identifier.uri http://dx.doi.org/10.15488/5173
dc.identifier.uri https://www.repo.uni-hannover.de/handle/123456789/5220
dc.contributor.author Chwalla, M.
dc.contributor.author Danzmann, Karsten
dc.contributor.author Fernández Barranco, G.
dc.contributor.author Fitzsimons, E.
dc.contributor.author Gerberding, Oliver
dc.contributor.author Heinzel, Gerhard
dc.contributor.author Killow, Christian J.
dc.contributor.author Lieser, M.
dc.contributor.author Perreur-Lloyd, M.
dc.contributor.author Robertson, D.I.
dc.contributor.author Schuster, Sönke
dc.contributor.author Schwarze, Thomas S.
dc.contributor.author Tröbs, M.
dc.contributor.author Ward, H.
dc.contributor.author Zwetz, M.
dc.date.accessioned 2019-08-15T07:18:15Z
dc.date.available 2019-08-15T07:18:15Z
dc.date.issued 2016
dc.identifier.citation Chwalla, M.; Danzmann, Karsten; Fernández Barranco, G.; Fitzsimons, E.; Gerberding, Oliver et al.: Design and construction of an optical test bed for LISA imaging systems and tilt-to-length coupling. In: Classical and Quantum Gravity 33 (2016), Nr. 24, Art. 245015. DOI: https://doi.org/10.1088/0264-9381/33/24/245015
dc.description.abstract The laser interferometer space antenna (LISA) is a future space-based interferometric gravitational-wave detector consisting of three spacecraft in a triangular configuration. The interferometric measurements of path length changes between satellites will be performed on optical benches in the satellites. Angular misalignments of the interfering beams couple into the length measurement and represent a significant noise source. Imaging systems will be used to reduce this tilt-to-length coupling.; We designed and constructed an optical test bed to experimentally investigate tilt-to-length coupling. It consists of two separate structures, a minimal optical bench and a telescope simulator. The minimal optical bench comprises the science interferometer where the local laser is interfered with light from a remote spacecraft. In our experiment, a simulated version of this received beam is generated on the telescope simulator. The telescope simulator provides a tilting beam, a reference interferometer and an additional static beam as a phase reference. The tilting beam can either be a flat-top beam or a Gaussian beam. We avoid tilt-to-length coupling in the reference interferometer by using a small photo diode placed at an image of the beam rotation point. We show that the test bed is operational with an initial measurement of tilt-to-length coupling without imaging systems.; Furthermore, we show the design of two different imaging systems whose performance will be investigated in future experiments. eng
dc.language.iso eng
dc.publisher Bristol : IOP Publishing
dc.relation.ispartofseries Classical and Quantum Gravity 33 (2016), Nr. 24
dc.rights CC BY 3.0 Unported
dc.rights.uri https://creativecommons.org/licenses/by/3.0/
dc.subject Coupling eng
dc.subject Laser beam quality eng
dc.subject Optics eng
dc.subject Physics eng
dc.subject nterferometry eng
dc.subject Beam (structure) eng
dc.subject Length measurement eng
dc.subject Gaussian beam eng
dc.subject Telescope eng
dc.subject Laser eng
dc.subject Quantum mechanics eng
dc.subject.ddc 530 | Physik ger
dc.title Design and construction of an optical test bed for LISA imaging systems and tilt-to-length coupling eng
dc.type Article
dc.type Text
dc.relation.issn 0264-9381
dc.relation.doi https://doi.org/10.1088/0264-9381/33/24/245015
dc.bibliographicCitation.issue 24
dc.bibliographicCitation.volume 33
dc.bibliographicCitation.firstPage 245015
dc.description.version publishedVersion
tib.accessRights frei zug�nglich


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