Quasinormal modes and strong cosmic censorship in the novel 4D Einstein-Gauss-Bonnet gravity

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dc.contributor.author Mishra, Akash K.
dc.date.accessioned 2020-04-20T07:26:30Z
dc.date.available 2020-04-20T07:26:30Z
dc.date.issued 2020-04
dc.identifier.citation Mishra, Akash K., "Quasinormal modes and strong cosmic censorship in the novel 4D Einstein-Gauss-Bonnet gravity", arXiv, Cornell University Library, DOI: arXiv:2004.01243, Apr. 2020. en_US
dc.identifier.uri http://arxiv.org/abs/2004.01243
dc.identifier.uri https://repository.iitgn.ac.in/handle/123456789/5330
dc.description.abstract The fate of strong cosmic censorship is ultimately linked to the extendibility of perturbation across the Cauchy Horizon and known to be violated in the near extremal region of a charged de Sitter black hole. Similar violations can also be realized in higher curvature theories, with the strength of violation becoming stronger as compared to general relativity. In this work, we extend this analysis further to study the validity of strong cosmic censorship conjecture in the context of the novel four-dimensional Einstein Gauss-Bonnet theory with respect to both scalar and electromagnetic perturbation.
dc.description.statementofresponsibility by Akash K Mishra
dc.language.iso en_US en_US
dc.publisher Cornell University Library en_US
dc.title Quasinormal modes and strong cosmic censorship in the novel 4D Einstein-Gauss-Bonnet gravity en_US
dc.type Pre-Print en_US
dc.relation.journal arXiv


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