Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5353
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dc.contributor.authorMENON, DHANYA S.en_US
dc.contributor.authorVARDARAJAN, SUNEETAen_US
dc.date.accessioned2020-11-13T09:30:20Z
dc.date.available2020-11-13T09:30:20Z
dc.date.issued2020-11en_US
dc.identifier.citationPhysical Review D, 102(10).en_US
dc.identifier.issn2470-0010en_US
dc.identifier.issn2470-0029en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5353-
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.102.104026en_US
dc.description.abstractWe study nonlinear gravitational perturbations of vacuum Einstein equations, with Λ<0 in (n+2) dimensions, with n>2, generalizing previous studies for n = 2. We follow the formalism by Ishibashi, Kodama, and Seto to decompose the metric perturbations into tensor, vector, and scalar sectors, and simplify the Einstein equations. We study, for the first time, general tensor perturbations. We render the metric perturbations in each sector asymptotically anti–de Sitter. Finally, we analyze the resonant structure of the perturbed equations at second order for the five dimensional case, by a partial study of single mode tensor-type perturbations at the linear level. For the cases we studied, resonant terms vanish at second order.en_US
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.subjectPhysicsen_US
dc.subject2020en_US
dc.subject2020-NOV-WEEK2en_US
dc.subjectTOC-NOV-2020en_US
dc.titleNonlinear perturbations of higher dimensional anti–de Sitter spacetimeen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitlePhysical Review Den_US
dc.publication.originofpublisherForeignen_US
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