Please use this identifier to cite or link to this item: http://hdl.handle.net/123456789/2336
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dc.contributor.authorSatish, Shakti-
dc.date.accessioned2024-04-03T15:45:33Z-
dc.date.available2024-04-03T15:45:33Z-
dc.date.issued2023-05-
dc.identifier.urihttp://hdl.handle.net/123456789/2336-
dc.descriptionEMbargo Perioden_US
dc.description.abstractThe thesis proposes a test of General Relativity (GR) using gravitational wave data and is applicable to any tests of compact binaries as different tests are sensitive to different aspects of general relativity. The meta inspiral- merger-ringdown consistency test (IMRCT) involves inferring final mass and final spin of the remnant black hole, obtained from the analyses from two different tests of GR, and then checking for their consistency. We check the performance of the meta IMRCT using a standard set of null tests that are used in analysis of GW signals. The three theory agnostic tests we consider are the original Inspiral-Merger-Ringdown Consistency Test (IMRCT), pa- rameterized phasing (two varieties), and modified dispersion test. meta IM- RCT is a generalization of original IMRCT and provides another test of GR. The method is applied to GR and non-GR signals and to quasi-circular and eccentric signals to illustrate the method’s performance. Finally, the test is applied to the samples from the LIGO and Virgo Collaboration for various tests of GR applied to GW170817.en_US
dc.language.isoenen_US
dc.publisherIISER Mohalien_US
dc.subjectConsistency testen_US
dc.subjectInspiral-Merger-Ringdownen_US
dc.titleTesting general relativity with gravitational waves using meta Inspiral-Merger-Ringdown Consistency Testen_US
dc.typeThesisen_US
dc.guideLochan, Kinjalken_US
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