On the nature of Hawking's incompleteness for the Einstein-vacuum equations: the regime of moderately spatially anisotropic initial data
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Publication:2119365
DOI10.4171/JEMS/1092MaRDI QIDQ2119365
Publication date: 29 March 2022
Published in: Journal of the European Mathematical Society (JEMS) (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1804.06825
constant mean curvaturesingularity theorembig bangcurvature singularitygeodesically incompletestable blowuptransported spatial coordinatesHawking's theoremkasner solutionsmaximal globally hyperbolic development
Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Space-time singularities, cosmic censorship, etc. (83C75) Singularity in context of PDEs (35A21) Einstein equations (35Q76)
Related Items (9)
Future dynamics of FLRW for the massless-scalar field system with positive cosmological constant ⋮ Stability of AVTD behavior Within the polarized \(\mathbb{T}^2\)-symmetric vacuum spacetimes ⋮ Stable cosmological Kaluza-Klein spacetimes ⋮ Stable Big Bang formation for Einstein’s equations: The complete sub-critical regime ⋮ The robustness of slow contraction and the shape of the scalar field potential ⋮ Asymptotically Kasner-like singularities ⋮ Localized big bang stability for the Einstein-scalar field equations ⋮ Wave asymptotics at a cosmological time-singularity: classical and quantum scalar fields ⋮ Cyclic spacetimes through singularity scattering maps. The laws of quiescent bounces
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