A conjectured inequality bounding black hole entropy by its specific heat is proven for a special static class and verified for many rotating and charged black holes.
Gravitational Radiation in an Expanding Universe
3 Pith papers cite this work, alongside 461 external citations. Polarity classification is still indexing.
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Adapts Sbierski's proof to establish future C^0-inextendibility for warped-product black hole spacetimes with closed, connected, homogeneous, orientable fibres, including nonvacuum cases and multiple horizons.
Claims a new metric unifying Kerr black holes with FLRW cosmology for arbitrary scale factor a(t), predicting stationary mass and contracting ergosphere and horizon.
citing papers explorer
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Black Hole Entropy Bounded by the Specific Heat
A conjectured inequality bounding black hole entropy by its specific heat is proven for a special static class and verified for many rotating and charged black holes.
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$C^0$-inextendibility of a class of warped-product black hole spacetimes
Adapts Sbierski's proof to establish future C^0-inextendibility for warped-product black hole spacetimes with closed, connected, homogeneous, orientable fibres, including nonvacuum cases and multiple horizons.
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Gravitational Field of a Rotating Mass on an Expanding Universe
Claims a new metric unifying Kerr black holes with FLRW cosmology for arbitrary scale factor a(t), predicting stationary mass and contracting ergosphere and horizon.