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dc.contributor.authorMarín, Antonio Francisco García
dc.date.accessioned2010-10-12T18:23:14Z
dc.date.available2010-10-12T18:23:14Z
dc.date.issued2007
dc.identifier.urihttp://hdl.handle.net/11858/00-1735-0000-0001-30D5-6
dc.description.abstractGravitational waves were predicted by Albert Einstein in 1916 as a consequence of his theory of general relativity. Hulse and Taylor provided indirect experimental evidence of their existence based on the increasing rotation frequency of a pulsar in the binary star system PSR 1913+16. They were awarded with the Nobel price in 1993. The direct detection of gravitational waves is expected to be one of the most exciting advances in physics in the next year...
dc.format.extent180 S.
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherUniv. Hannover
dc.rights.urihttp://e-docs.geo-leo.de/rights
dc.subject.ddc522
dc.subject.gokTCE 100
dc.subject.gokTCE 500
dc.titleMinimisation of optical pathlength noise for the detection of gravitational waves with the spaceborne laser interferometer LISA and LISA pathfinder
dc.typemonograph
dc.subject.gokverbalAstrometrische und interferometrische Instrumente
dc.subject.gokverbalSonstige Instrumente {Astronomische Instrumente}
dc.identifier.doi10.23689/fidgeo-80
dc.identifier.ppn555905810
dc.identifier.urnurn:nbn:de:gbv:089-5559058107
dc.type.versionpublishedVersion
dc.relation.collectionAstronomie, Astrophysik, Weltraumforschung
dc.description.typethesis


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