Internal structure of charged AdS black holes

Show simple item record Bhattacharjee, Srijit Sarkar, Sudipta Virmani, Amitabh 2016-07-20T09:30:52Z 2016-07-20T09:30:52Z 2016-06
dc.identifier.citation Bhattacharjee, Srijit; Sarkar, Sudipta and Virmani, Amitabh, “Internal structure of charged AdS black holes”, Physical Review D, DOI: 10.1103/PhysRevD.93.124029, vol. 93, no. 12, Jun. 2016.
dc.identifier.issn 2470-0010
dc.identifier.issn 2470-0029
dc.description.abstract When an electrically charged black hole is perturbed, its inner horizon becomes a singularity, often referred to as the Poisson-Israel mass inflation singularity. Ori constructed a model of this phenomenon for asymptotically flat black holes, in which the metric can be determined explicitly in the mass inflation region. In this paper we implement the Ori model for charged AdS black holes. We find that the mass function inflates faster than the flat space case as the inner horizon is approached. Nevertheless, the mass inflation singularity is still a weak singularity: Although spacetime curvature becomes infinite, tidal distortions remain finite on physical objects attempting to cross it. en_US
dc.description.statementofresponsibility by Srijit Bhattacharjee, Sudipta Sarkar and Amitabh Virmani
dc.format.extent vol. 93, no. 12
dc.language.iso en_US en_US
dc.publisher American Physical Society en_US
dc.title Internal structure of charged AdS black holes en_US
dc.type Article en_US
dc.relation.journal Physical Review D

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