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Formation of Trapped Surfaces from Past Null Infinity
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Formation of Trapped Surfaces from Past Null Infinity
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In this paper, we extend the results of Klainerman and Rodnianski in \cite{KR:Trapped}, which were obtained for a finite region, by showing similar results from past null infinity. This allows us to recover and extend the results from past null infinity in the work of Christodoulou \cite{Chr:book}.
Forward citations
Cited by 3 Pith papers
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Semi-Global Existence and Trapped Surface Formation for the Einstein-Vlasov System
Massless Vlasov matter in 3+1 dimensions, with large characteristic data and no symmetry, admits a semi-global smooth solution that forms a trapped surface when the initial null energy flux is large.
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Formation of Trapped Surfaces from Spacelike Initial Data
Short-pulse free scalars on a spacelike hypersurface yield asymptotically flat Cauchy data whose vacuum evolution forms trapped surfaces, including time-symmetric cases.
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Dynamical Formation of Black Holes due to Boundary Effect in Vacuum Gravity
The authors argue that vacuum Einstein evolution can push a boundary-curvature quantity across Yau's threshold, forcing an apparent horizon to form without gravitational collapse.
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