Towards a gravitational wave observatory designer: sensitivity limits of spaceborne detectors

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dc.identifier.uri http://dx.doi.org/10.15488/379
dc.identifier.uri http://www.repo.uni-hannover.de/handle/123456789/402
dc.contributor.author Barke, Simon
dc.contributor.author Wang, Y.
dc.contributor.author Delgado, Juan Jose Esteban
dc.contributor.author Troebs, Michael
dc.contributor.author Heinzel, Gerhard
dc.contributor.author Danzmann, Karsten
dc.date.accessioned 2016-08-12T08:08:29Z
dc.date.available 2016-08-12T08:08:29Z
dc.date.issued 2015-05-07
dc.identifier.citation Barke, Simon; Wang, Y.; Delgado, J. J. Esteban; Troebs, Michael; Heinzel, Gerhard; Danzmann, Karsten: Towards a gravitational wave observatory designer: sensitivity limits of spaceborne detectors. In: Classical And Quantum Gravity 32 (2015), Nr. 9, 95004. DOI: http://dx.doi.org/10.1088/0264-9381/32/9/095004
dc.description.abstract The most promising concept for low frequency (millihertz to hertz) gravitational wave observatories are laser interferometric detectors in space. It is usually assumed that the noise floor for such a detector is dominated by optical shot noise in the signal readout. For this to be true, a careful balance of mission parameters is crucial to keep all other parasitic disturbances below shot noise. We developed a web application that uses over 30 input parameters and considers many important technical noise sources and noise suppression techniques to derive a realistic position noise budget. It optimizes free parameters automatically and generates a detailed report on all individual noise contributions. Thus one can easily explore the entire parameter space and design a realistic gravitational wave observatory. In this document we describe the different parameters, present all underlying calculations, and compare the final observatory's sensitivity with astrophysical sources of gravitational waves. We use as an example parameters currently assumed to be likely applied to a space mission proposed to be launched in 2034 by the European Space Agency. The web application itself is publicly available on the Internet at http://spacegravity.org/designer. Future versions of the web application will incorporate the frequency dependence of different noise sources and include a more detailed model of the observatory's residual acceleration noise. eng
dc.language.iso eng
dc.publisher Bristol : IOP Publishing Ltd.
dc.relation.ispartofseries Classical And Quantum Gravity 32 (2015), Nr. 9
dc.rights CC BY 3.0 Unported
dc.rights.uri https://creativecommons.org/licenses/by/3.0/de/
dc.subject gravitational waves eng
dc.subject laser interferometry eng
dc.subject shot noise eng
dc.subject laser interferometer space antenna eng
dc.subject LISA eng
dc.subject eLISA eng
dc.subject OGO eng
dc.subject lisa eng
dc.subject interferometers eng
dc.subject sensors eng
dc.subject systems eng
dc.subject noise eng
dc.subject Gravitationswelle ger
dc.subject.ddc 530 | Physik ger
dc.title Towards a gravitational wave observatory designer: sensitivity limits of spaceborne detectors eng
dc.type article
dc.type Text
dc.relation.essn 1361-6382
dc.relation.issn 0264-9381
dc.relation.doi http://dx.doi.org/10.1088/0264-9381/32/9/095004
dc.bibliographicCitation.issue 9
dc.bibliographicCitation.volume 32
dc.bibliographicCitation.firstPage 95004
dc.description.version publishedVersion
tib.accessRights frei zug�nglich


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