Stability of MOTS in totally geodesic null horizons
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Publication:2902307
DOI10.1088/0264-9381/29/14/145019zbMath1248.83097arXiv1205.1724OpenAlexW2095547387MaRDI QIDQ2902307
Publication date: 17 August 2012
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1205.1724
Black holes (83C57) Applications of differential geometry to physics (53Z05) Space-time singularities, cosmic censorship, etc. (83C75) Equations of motion in general relativity and gravitational theory (83C10)
Related Items (11)
Extremal surface barriers ⋮ Equations for general shells ⋮ Stability of black holes and black branes ⋮ Dynamical symmetry enhancement near \(\mathcal{N} =2\), \(D=4\) gauged supergravity horizons ⋮ A note on the positive mass theorem with boundary ⋮ Multiple Killing horizons: the initial value formulation for Λ -vacuum ⋮ The trapping effect on degenerate horizons ⋮ Quasi-round MOTSs and stability of the Schwarzschild null Penrose inequality ⋮ Eigenvalues of the MOTS stability operator for slowly rotating Kerr black holes ⋮ Multiple Killing horizons ⋮ Classification of near-horizon geometries of extremal black holes
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