Strong cosmic censorship in spherical symmetry for two-ended asymptotically flat initial data I. The interior of the black hole region
Annals of mathematics, Tome 190 (2019) no. 1, pp. 1-111

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This is the first and main paper of a two-part series, in which we prove the $C^{2}$-formulation of the strong cosmic censorship conjecture for the Einstein–Maxwell-(real)-scalar-field system in spherical symmetry for two-ended asymptotically flat data. For this model, it is known through the works of Dafermos and Dafermos–Rodnianski that the maximal globally hyperbolic future development of any admissible two-ended asymptotically flat Cauchy initial data set possesses a non-empty Cauchy horizon, across which the spacetime is $C^{0}$-future-extendible. (In particular, the $C^{0}$-formulation of the strong cosmic censorship conjecture is false.) Nevertheless, the main conclusion of the present series of papers is that for a generic (in the sense of being open and dense relative to appropriate topologies) class of such data, the spacetime is future-inextendible with a Lorentzian metric of higher regularity (specifically, $C^{2}$).

DOI : 10.4007/annals.2019.190.1.1

Jonathan Luk 1 ; Sung-Jin Oh 2

1 Stanford University, Palo Alto, CA
2 Korea Institute for Advanced Study, Seoul, Korea
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Jonathan Luk; Sung-Jin Oh. Strong cosmic censorship in spherical symmetry for two-ended asymptotically flat initial data I. The interior of the black hole region. Annals of mathematics, Tome 190 (2019) no. 1, pp. 1-111. doi: 10.4007/annals.2019.190.1.1

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