Epstein curves in the hyperbolic disk equate the Schwarzian action to curve length and enclosed area while equaling the derivative of Loewner energy, yielding immediate non-negativity proofs via isoperimetric inequality.
Random disks of constant curvature: the lattice story.Preprint
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Inner horizon saddles supply the semiclassical correction -exp(A_inner/4G) to near-extremal black-hole entropy and motivate a spectral KSW criterion for well-defined one-loop effects around complex gravitational saddles.
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Epstein curves and holography of the Schwarzian action
Epstein curves in the hyperbolic disk equate the Schwarzian action to curve length and enclosed area while equaling the derivative of Loewner energy, yielding immediate non-negativity proofs via isoperimetric inequality.
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Inner Horizon Saddles and a Spectral KSW Criterion
Inner horizon saddles supply the semiclassical correction -exp(A_inner/4G) to near-extremal black-hole entropy and motivate a spectral KSW criterion for well-defined one-loop effects around complex gravitational saddles.