Near horizon extremal geometry perturbations: dynamical field perturbations vs. parametric variations

DOI10.1007/JHEP10(2014)111zbMath1333.83088arXiv1407.1992OpenAlexW3100921636MaRDI QIDQ271157

Ali Seraj, Kamal Hajian

Publication date: 7 April 2016

Published in: Journal of High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1407.1992

zbMATH Keywords

black holesclassical theories of gravityspace-time symmetries

Mathematics Subject Classification ID

Black holes (83C57) Space-time singularities, cosmic censorship, etc. (83C75)

Related Items

Black hole non-uniqueness via spacetime topology in five dimensions ⋮ Symplectic and Killing symmetries of \(\mathrm{AdS}_3\) gravity: holographic vs boundary gravitons ⋮ Wiggling throat of extremal black holes ⋮ Near-horizon extremal geometries: coadjoint orbits and quantization ⋮ JT gravity and near-extremal thermodynamics for Kerr black holes in \(AdS_{4, 5}\) for rotating perturbations ⋮ Conserved charges and first law of thermodynamics for Kerr-de Sitter black holes ⋮ Extremal vanishing horizon Kerr-AdS black holes at ultraspinning limit ⋮ Near horizon structure of extremal vanishing horizon black holes ⋮ Symplectic Structure of Extremal Black Holes ⋮ The Kerr/CFT correspondence and its extensions

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