Please use this identifier to cite or link to this item: http://bura.brunel.ac.uk/handle/2438/4801
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dc.contributor.authorVeitch, PJ-
dc.contributor.authorBlair, DG-
dc.contributor.authorLinthorne, NP-
dc.contributor.authorMann, LD-
dc.contributor.authorRamm, DK-
dc.date.accessioned2011-03-11T15:18:26Z-
dc.date.available2011-03-11T15:18:26Z-
dc.date.issued1987-
dc.identifier.citationReview of Scientific Instruments, 58(10): 1910-1916, Oct 1987en_US
dc.identifier.issn0034-6748-
dc.identifier.urihttp://bura.brunel.ac.uk/handle/2438/4801-
dc.descriptionCopyright @ American Institute of Physicsen_US
dc.description.abstractA 1.5‐tonne Nb gravitational radiation antenna is described. Problems associated with a noncontacting magnetically levitated parametric upconverter transducer are discussed, and a system using a bonded microwave reentrant cavity and bonded mechanical impedance transformer is described and analyzed in detail. It is shown that such an antenna can be expected to achieve a noise temperature of ∼1 mK. An ultralow phase noise tunable microwave source for the transducer pump signal is described, as well as precision bonding techniques which yield a mechanical positioning accuracy of 10−6 m, and a reproducibility of 10−8 m.en_US
dc.description.sponsorshipThe research was supported by the Australian Research Grants Scheme and the Australian Telecommunications and Electronics Research Board.en_US
dc.language.isoenen_US
dc.publisherAmerican Institute of Physicsen_US
dc.titleDevelopment of a 1.5-tonne niobium gravitational radiational antennaen_US
dc.typeResearch Paperen_US
dc.identifier.doihttp://dx.doi.org/10.1063/1.1139488-
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Dept of Life Sciences Research Papers

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