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Plane-symmetric spacetimes with positive cosmological constant: the case of stiff fluids

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Publication:451144
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DOI10.4310/ATMP.2011.v15.n4.a6zbMath1247.83012arXiv1011.4571MaRDI QIDQ451144

Philippe G. LeFloch, Sophonie Blaise Tchapnda

Publication date: 21 September 2012

Published in: Advances in Theoretical and Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1011.4571



Mathematics Subject Classification ID

Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05)


Related Items (5)

Future global nonlinear stability of surface symmetric solutions of the Einstein–Vlasov system with a cosmological constant ⋮ Weakly regular \(T^2\)-symmetric spacetimes. The future causal geometry of Gowdy spacetimes ⋮ A de Sitter no-hair theorem for 3+1d cosmologies with isometry group forming 2-dimensional orbits ⋮ Proof of the cosmic no-hair conjecture in the \(\mathbb{T}^3\)-Gowdy symmetric Einstein-Vlasov setting ⋮ The global future stability of the FLRW solutions to the Dust-Einstein system with a positive cosmological constant




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