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Future Global in time einsteinian spacetimes with U(1) isometry group
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abstract
We prove that spacetimes satisfying the vacuum Einstein equations on a manifold of the form $\Sigma \times U(1)\times R$ where $\Sigma $ is a compact surface of genus $G>1$ and where the Cauchy data is invariant with respect to U(1) and sufficiently small exist for an infinite proper time in the expanding direction.
Forward citations
Cited by 2 Pith papers
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Nonlinear stability of Einstein-de Sitter universes
Near-flat initial data for Einstein-Euler with polytropic equation of state n>3 on T^{3} produce future-global solutions that homogenise and asymptote to Einstein-de Sitter.
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On Axially Symmetric Perturbations of Kerr Black Hole Spacetimes
For subextremal Kerr spacetimes, the paper constructs a positive-definite, conserved Hamiltonian energy for axially symmetric linear perturbations, indicating a form of linear stability within this symmetry class.
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