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Obstruction-free gluing for the Einstein equations
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Obstruction-free gluing for the Einstein equations
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In this paper we develop a new approach to the gluing problem in General Relativity, that is, the problem of matching two solutions of the Einstein equations along a spacelike or characteristic (null) hypersurface. In contrast to the previous constructions, the new perspective actively utilizes the nonlinearity of the constraint equations. As a result, we are able to remove the $10$-dimensional spaces of obstructions to the null and spacelike (asymptotically flat) gluing problems, previously known in the literature. In particular, we show that any asymptotically flat spacelike initial data can be glued to the Schwarzschild initial data of mass $M$ for any $M>0$ sufficiently large. More generally, compared to the celebrated result of Corvino-Schoen, our methods allow us to choose ourselves the Kerr spacelike initial data that is being glued onto. As in our earlier work, our primary focus is the analysis of the null problem, where we develop a new technique of combining low-frequency linear analysis with high-frequency nonlinear control. The corresponding spacelike results are derived a posteriori by solving a characteristic initial value problem.
Forward citations
Cited by 3 Pith papers
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Weak cosmic censorship for the circularly symmetric Einstein-scalar field system in $2+1$ dimensions
Proves weak cosmic censorship for circularly symmetric Einstein-scalar field system in 2+1D with Λ<0: maximal developments of generic C^k initial data (k≥2) contain no naked singularities.
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Weak cosmic censorship for the circularly symmetric Einstein-scalar field system in $2+1$ dimensions
Proves that for any integer k≥2, the maximal development of generic C^k initial data for the circularly symmetric Einstein-scalar field system with Λ<0 in 2+1 dimensions contains no naked singularities.
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Formation of extremal Reissner-Nordstr\"om black holes: insights from numerics
For several scalar-field profiles, extremal Reissner-Nordström black holes can be glued from collapse only above a profile-dependent threshold in eM, and only for scalar masses below about m/e≈0.28.
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