A uniqueness theorem for degenerate Kerr-Newman black holes
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Publication:625726
DOI10.1007/s00023-010-0038-3zbMath1211.83018arXiv1002.1737OpenAlexW3099993373MaRDI QIDQ625726
Luc Nguyen, Piotr T. Chrusciel
Publication date: 25 February 2011
Published in: Annales Henri Poincaré (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1002.1737
Black holes (83C57) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (15)
Mathematical general relativity: A sampler ⋮ Convexity of reduced energy and mass angular momentum inequalities ⋮ Deformations of the Kerr-(A)dS near horizon geometry ⋮ Uniqueness of the extremal Schwarzschild de Sitter spacetime ⋮ Towards a classification of vacuum near-horizons geometries ⋮ Non-existence of multiple-black-hole solutions close to Kerr-Newman ⋮ Stability and instability of extreme Reissner-Nordström black hole spacetimes for linear scalar perturbations. I ⋮ Late-time asymptotics for the wave equation on extremal Reissner-Nordström backgrounds ⋮ Non-existence of stationary two-black-hole configurations: the degenerate case ⋮ Moduli space of supersymmetric solitons and black holes in five dimensions ⋮ Bounding horizon area by angular momentum, charge, and cosmological constant in 5-dimensional minimal supergravity ⋮ Stability and instability of extreme Reissner-Nordström black hole spacetimes for linear scalar perturbations. II ⋮ Decay of axisymmetric solutions of the wave equation on extreme Kerr backgrounds ⋮ Stationary black holes: uniqueness and beyond ⋮ Classification of near-horizon geometries of extremal black holes
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