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dc.contributor.authorHerman, David Leigh
dc.date.accessioned2013-02-27T12:59:25Z
dc.date.available2013-02-27T12:59:25Z
dc.date.issued2013-02-27
dc.identifier.urihttp://hdl.handle.net/10222/21376
dc.description.abstractThe main goal of this thesis is to present cosmological perturbation theory (based on the standard Friedmann cosmological model) in volume-preserving coordinates, which then provides a suitable basis for studies in cosmological averaging. We review perturbation theory to second order, allowing for averaging to second order in future research. To solve the averaging problem we need a method of covariantly and gauge invariantly averaging tensorial objects on a background manifold. This is a very difficult problem. However, the definition of an average takes on a particularly simple form when written in a system of volume-preserving coordinates. Therefore, we develop a three dimensional and a four dimensional volume-preserving coordinate gauge in this thesis that can be used for averaging in cosmological perturbation theory.en_US
dc.language.isoen_USen_US
dc.subjectCosmologyen_US
dc.subjectCosmological Averagingen_US
dc.subjectDifferential Geometryen_US
dc.subjectPerturbation Theory in Cosmologyen_US
dc.subjectGeneral Relativityen_US
dc.subjectThe Gauge Issueen_US
dc.titleVolume-Preserving Coordinate Gauges in Linear Perturbation Theoryen_US
dc.typeThesisen_US
dc.date.defence2012-12-21
dc.contributor.departmentDepartment of Mathematics & Statistics - Math Divisionen_US
dc.contributor.degreeMaster of Scienceen_US
dc.contributor.external-examinern/aen_US
dc.contributor.graduate-coordinatorDr. Sara Faridien_US
dc.contributor.thesis-readerDr. Robert van den Hoogenen_US
dc.contributor.thesis-readerDr. David Ironen_US
dc.contributor.thesis-supervisorDr. Alan Coleyen_US
dc.contributor.ethics-approvalNot Applicableen_US
dc.contributor.manuscriptsNot Applicableen_US
dc.contributor.copyright-releaseNot Applicableen_US
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