Numerical collapse in 4+1D vacuum gravity with Λ>0 forms a Schwarzschild–de Sitter black hole at 99% of the extremal mass, suggesting the extremal limit — and a third-law violation — may be reachable.
Gravitational collapse to extremal black holes and the third law of black hole ther- modynamics
4 Pith papers cite this work. Polarity classification is still indexing.
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For any number n of aligned black holes the axis potentials are necessarily rational functions depending on a finite number of parameters.
Numerical solutions reveal that the threshold of black hole formation in charged Vlasov matter shifts from stationary horizonless shells to extremal black holes past a critical charge-to-mass ratio of unity.
Derives junction conditions in STVG/MOG and constructs two models of gravitational collapse that form extremal or sub-extremal RN-like black holes.
citing papers explorer
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Near--extremal gravitational collapse in 4+1 dimensions: Schwarzschild--de--Sitter space
Numerical collapse in 4+1D vacuum gravity with Λ>0 forms a Schwarzschild–de Sitter black hole at 99% of the extremal mass, suggesting the extremal limit — and a third-law violation — may be reachable.
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The balance problem for $n$ aligned black holes
For any number n of aligned black holes the axis potentials are necessarily rational functions depending on a finite number of parameters.
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Gravitational collapse in the vicinity of the extremal black hole critical point
Numerical solutions reveal that the threshold of black hole formation in charged Vlasov matter shifts from stationary horizonless shells to extremal black holes past a critical charge-to-mass ratio of unity.
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Junction Conditions and Gravitational Collapse in Scalar-Tensor-Vector Gravity
Derives junction conditions in STVG/MOG and constructs two models of gravitational collapse that form extremal or sub-extremal RN-like black holes.