Improving the sensitivity of future GW observatories in the 1-10 Hz band: Newtonian and seismic noise

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dc.identifier.uri http://dx.doi.org/10.15488/1857
dc.identifier.uri http://www.repo.uni-hannover.de/handle/123456789/1882
dc.contributor.author Beker, M.G.
dc.contributor.author Cella, G.
dc.contributor.author DeSalvo, R.
dc.contributor.author Doets, M.
dc.contributor.author Grote, Hartmut
dc.contributor.author Harms, J.
dc.contributor.author Hennes, E.
dc.contributor.author Mandic, V.
dc.contributor.author Rabeling, D.S.
dc.contributor.author van den Brand, J.F.J.
dc.contributor.author van Leeuwen, C.M.
dc.date.accessioned 2017-09-07T13:27:57Z
dc.date.available 2017-09-07T13:27:57Z
dc.date.issued 2011
dc.identifier.citation Beker, M.G.; Cella, G.; DeSalvo, R.; Doets, M.; Grote, H. et al.: Improving the sensitivity of future GW observatories in the 1-10 Hz band: Newtonian and seismic noise. In: General Relativity and Gravitation 43 (2011), Nr. 2, S. 623-656. DOI: https://doi.org/10.1007/s10714-010-1011-7
dc.description.abstract The next generation gravitational wave interferometric detectors will likely be underground detectors to extend the GW detection frequency band to frequencies below the Newtonian noise limit. Newtonian noise originates from the continuous motion of the Earth's crust driven by human activity, tidal stresses and seismic motion, and from mass density fluctuations in the atmosphere. It is calculated that on Earth's surface, on a typical day, it will exceed the expected GW signals at frequencies below 10 Hz. The noise will decrease underground by an unknown amount. It is important to investigate and to quantify this expected reduction and its effect on the sensitivity of future detectors, to plan for further improvement strategies. We report about some of these aspects. Analytical models can be used in the simplest scenarios to get a better qualitative and semi-quantitative understanding. As more complete modeling can be done numerically, we will discuss also some results obtained with a finite-element-based modeling tool. The method is verified by comparing its results with the results of analytic calculations for surface detectors. A key point about noise models is their initial parameters and conditions, which require detailed information about seismic motion in a real scenario. We will describe an effort to characterize the seismic activity at the Homestake mine which is currently in progress. This activity is specifically aimed to provide informations and to explore the site as a possible candidate for an underground observatory. Although the only compelling reason to put the interferometer underground is to reduce the Newtonian noise, we expect that the more stable underground environment will have a more general positive impact on the sensitivity. We will end this report with some considerations about seismic and suspension noise. eng
dc.description.sponsorship Netherlands Organization for Scientific Research (NWO)
dc.description.sponsorship National Science Foundation
dc.language.iso eng
dc.publisher Heidelberg : Springer Verlag
dc.relation.ispartofseries General Relativity and Gravitation 43 (2011), Nr. 2
dc.rights CC BY-NC 4.0 Unported
dc.rights.uri https://creativecommons.org/licenses/by-nc/4.0/
dc.subject Gravitational waves eng
dc.subject Noises eng
dc.subject Gravitationswelle ger
dc.subject.ddc 530 | Physik ger
dc.title Improving the sensitivity of future GW observatories in the 1-10 Hz band: Newtonian and seismic noise
dc.type article
dc.type Text
dc.relation.issn 00017701
dc.relation.doi https://doi.org/10.1007/s10714-010-1011-7
dc.bibliographicCitation.issue 2
dc.bibliographicCitation.volume 43
dc.bibliographicCitation.firstPage 623
dc.bibliographicCitation.lastPage 656
dc.description.version publishedVersion
tib.accessRights frei zug�nglich


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