Physics of gravitational waves in presence of positive cosmological constant[HBNI Th132]

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dc.contributor.author Sk Jahanur Hoque
dc.date.accessioned 2018-05-17T11:17:28Z
dc.date.available 2018-05-17T11:17:28Z
dc.date.issued 2017
dc.date.submitted 2017
dc.identifier.uri https://dspace.imsc.res.in/xmlui/handle/123456789/419
dc.description.abstract Cosmological observations over past couple of decades favour our universe with a tiny positive cosmological constant. Even a tiniest value of cosmological constant, profoundly alters the asymptotic structure of space-time. This suggests that weak gravitational waves should be re-looked at as ripples on the de Sitter background.The thesis deals with different aspects weak gravitational waves on the de Sitter background. We obtain the gravitational radiation field of compactly supported source. This is given by gauge invariant part of retarded solution, expressed in terms source multi-pole moments. en_US
dc.publisher.publisher The Institute of Mathematical Sciences
dc.subject Gravitational Waves en_US
dc.subject Cosmological Horizon en_US
dc.subject Quadrupole Formula en_US
dc.subject HBNI Th132 en_US
dc.title Physics of gravitational waves in presence of positive cosmological constant[HBNI Th132] en_US
dc.type.degree Ph.D en_US
dc.type.institution HBNI en_US
dc.description.advisor Ghanashyam Date
dc.description.pages 186p. en_US
dc.type.mainsub Physics en_US
dc.type.hbnibos Physical Sciences


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