Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/2920
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dc.contributor.advisorVirmani, Amitabhen_US
dc.contributor.authorKHAIRNAR, ANIKETen_US
dc.date.accessioned2019-05-07T02:59:42Z
dc.date.available2019-05-07T02:59:42Z
dc.date.issued2019-04en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/2920-
dc.description.abstractBMS symmetries have been argued to be the exact symmetries of quantum gravity theory in asymptotically flat spacetimes. If this is the case, then they should also be visible at timelike infinity as well. In this thesis, we introduce a notion of asymptotically flat spacetimes at timelike infinity and discuss boundary conditions that allow for BMS symmetries to act on the space of solutions. The BMS symmetries lead to non-trivial conserved charges and conservation laws.en_US
dc.language.isoenen_US
dc.subject2019
dc.subjectGeneral relativityen_US
dc.titleAsymptotic flatness at timelike infinityen_US
dc.typeThesisen_US
dc.type.degreeBS-MSen_US
dc.contributor.departmentDept. of Physicsen_US
dc.contributor.registration20141028en_US
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