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dc.contributor.authorKim, Yunho
dc.date.accessioned2021-10-29T04:05:49Z
dc.date.available2021-10-29T04:05:49Z
dc.date.issued2021en_AU
dc.identifier.urihttps://hdl.handle.net/2123/26707
dc.description.abstractThis thesis investigates black holes and gravitational waves in the framework of quadratic gravity. These subjects are introduced by first examining the current state of general relativity and how it is realised. The discussion then addresses the quantitative aspects of black holes, gravitational waves, and quadratic gravity. This is then followed by the exploration of the three main research topics. The first research topic investigates the induced charging of a black hole due to a topological term in quadratic gravity. The second research topic focuses on the approximate analytic non-Schwarzschild black hole solutions in quadratic gravity. Finally, gravitational waves generated by binary systems within quadratic gravity are studied, with a focus on the corrections produced by the massive scalar field and the massive spin-2 field.en_AU
dc.language.isoenen_AU
dc.subjectQuadratic Gravityen_AU
dc.subjectGeneral Relativityen_AU
dc.subjectBlack Holesen_AU
dc.subjectGravitational Wavesen_AU
dc.subjectModified theories of gravityen_AU
dc.subjectDifferential Geometryen_AU
dc.titleQuadratic Gravity with Black Holes and Gravitational Wavesen_AU
dc.typeThesis
dc.type.thesisDoctor of Philosophyen_AU
dc.rights.otherThe author retains copyright of this thesis. It may only be used for the purposes of research and study. It must not be used for any other purposes and may not be transmitted or shared with others without prior permission.en_AU
usyd.facultySeS faculties schools::Faculty of Science::School of Physicsen_AU
usyd.degreeDoctor of Philosophy Ph.D.en_AU
usyd.awardinginstThe University of Sydneyen_AU
usyd.advisorKobakhidze, Archil


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