The time evolution of marginally trapped surfaces

DOI10.1088/0264-9381/26/8/085018zbMath1163.83003arXiv0811.4721OpenAlexW2078800371WikidataQ125304567 ScholiaQ125304567MaRDI QIDQ3627539

Lars Andersson, Walter Simon, Jan Metzger, Marc Mars

Publication date: 12 May 2009

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0811.4721

Mathematics Subject Classification ID

Black holes (83C57) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Space-time singularities, cosmic censorship, etc. (83C75)

Related Items (13)

Mathematical general relativity: A sampler ⋮ The merger of small and large black holes ⋮ Ultra-massive spacetimes ⋮ Beyond black holes: universal properties of ‘ultra-massive’ spacetimes ⋮ The influence of Penrose's singularity theorem in general relativity ⋮ Holography abhors visible trapped surfaces ⋮ A finite dimensional approach to light rays in general relativity ⋮ A2: mathematical relativity and other progress in classical gravity theory -- a session report ⋮ Geometric horizons in binary black hole mergers ⋮ INVOLUTE, MINIMAL, OUTER AND INCREASINGLY TRAPPED SURFACES ⋮ Black holes in Einstein–Maxwell theory ⋮ Eigenvalues of the MOTS stability operator for slowly rotating Kerr black holes ⋮ Coarse graining holographic black holes

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