An enhanced constraint damping property holds for the linearized Einstein equations on any subextremal Kerr metric.
The non-linear stability of the Schwarzschild family of black holes
7 Pith papers cite this work. Polarity classification is still indexing.
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The spacetime Penrose inequality holds under the quasi final state hypothesis via tangentially maximal hypersurfaces that reduce the problem to the known Riemannian Penrose inequality.
A weak null singularity forms inside generic subextremal strictly rotating black holes, with the metric continuously extendible but not Lipschitz extendible.
Constructs bifurcating families of asymptotically AdS hairy black holes from RN-AdS, providing a counterexample to no-hair and rigorous holographic superconductors.
Proves global stability of Minkowski spacetime under small perturbations in a centre-normalised outgoing null-geodesic gauge by combining r^p estimates on Weyl components with transport equations along a regular central axis.
GW250114 data confirm the remnant is consistent with a Kerr black hole and bound the dominant quadrupolar mode frequency to within a few percent of the GR prediction, with constraints tighter than prior multi-event catalogs.
Dynamical evolution of Schwarzschild black holes produces new interior singularities absent in the static case, with resolution imposing highly restrictive conditions on gravitational collapse.
citing papers explorer
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Constraint damping on subextremal Kerr spacetimes
An enhanced constraint damping property holds for the linearized Einstein equations on any subextremal Kerr metric.
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The spacetime Penrose inequality under a quasi final state hypothesis
The spacetime Penrose inequality holds under the quasi final state hypothesis via tangentially maximal hypersurfaces that reduce the problem to the known Riemannian Penrose inequality.
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The formation of a weak null singularity in the interior of generic rotating black holes
A weak null singularity forms inside generic subextremal strictly rotating black holes, with the metric continuously extendible but not Lipschitz extendible.
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Asymptotically Anti-de Sitter Spherically Symmetric Hairy Black Holes
Constructs bifurcating families of asymptotically AdS hairy black holes from RN-AdS, providing a counterexample to no-hair and rigorous holographic superconductors.
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Stability of the Minkowski spacetime in Newman-Unti gauge
Proves global stability of Minkowski spacetime under small perturbations in a centre-normalised outgoing null-geodesic gauge by combining r^p estimates on Weyl components with transport equations along a regular central axis.
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Black Hole Spectroscopy and Tests of General Relativity with GW250114
GW250114 data confirm the remnant is consistent with a Kerr black hole and bound the dominant quadrupolar mode frequency to within a few percent of the GR prediction, with constraints tighter than prior multi-event catalogs.
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Interior Dynamics of Regular Schwarzschild Black Holes
Dynamical evolution of Schwarzschild black holes produces new interior singularities absent in the static case, with resolution imposing highly restrictive conditions on gravitational collapse.