Extremal Vanishing Horizon Kerr-AdS Black Holes at Ultraspinning Limit
arXiv:1708.08654 · doi:10.1007/JHEP01(2018)042
Abstract
By utilizing the ultraspinning limit we generate a new class of extremal vanishing horizon (EVH) black holes in odd dimensions (). Starting from the general multi-spinning Kerr-AdS metrics, we show the EVH limit commutes with the ultraspinning limit, in which the resulting solutions possess a non-compact but finite area manifold for all slices. We also demonstrate the near horizon geometries of obtained ultraspinning EVH solutions contain an AdS throats, where it would be a BTZ black hole in the near EVH cases. The commutativity of the ultraspinning and near horizon limits for EVH solutions is confirmed as well. Furthermore, we discuss only the five-dimensional case near the EVH point can be viewed as a super-entropic black hole. We also show that the thermodynamics of the obtained solutions agree with the BTZ black hole. Moreover we investigate the EVH/CFT proposal, demonstrating the entropy of d dual CFT and Bekenstein-Hawking entropy are equivalent.
arXiv comment29 pages, 3 figures, references added, typos corrected, revised version to match published version
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