Late-time linear growth of holographic TEE is governed by an interior critical surface Ac whose existence is guaranteed by NEC under Kasner asymptotics, with vacuum maximizing real growth and minimizing imaginary part.
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In a holographic superfluid, the speed of a topological-defect-driven invasion front has a maximum at a particular quench endpoint, which the authors propose as a new nonequilibrium supercritical crossover line.
The nonlinear coefficient λ controls the inverse periodicity of Kasner exponent oscillations in the interior of holographic black holes near the superfluid critical point.
Scalarized black holes in EMS theory lack smooth Cauchy horizons and form Kasner singularities, with a scaling relation between Kasner parameter and charge-to-mass ratio near criticality.
In O(d,d) symmetric gravity with curvature corrections, black brane singularities are not resolved but approach with altered Kasner exponents, while a dilaton generates negative cosmological constants at small coupling.
citing papers explorer
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Linear Growth of Holographic Time-like Entanglement Entropy and Kasner exponents
Late-time linear growth of holographic TEE is governed by an interior critical surface Ac whose existence is guaranteed by NEC under Kasner asymptotics, with vacuum maximizing real growth and minimizing imaginary part.
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Nonequilibrium crossover in the supercritical region from quench dynamics
In a holographic superfluid, the speed of a topological-defect-driven invasion front has a maximum at a particular quench endpoint, which the authors propose as a new nonequilibrium supercritical crossover line.
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Interior structure of black holes with nonlinear terms
The nonlinear coefficient λ controls the inverse periodicity of Kasner exponent oscillations in the interior of holographic black holes near the superfluid critical point.
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Critical phenomenon inside asymptotically flat black holes with spontaneous scalarization
Scalarized black holes in EMS theory lack smooth Cauchy horizons and form Kasner singularities, with a scaling relation between Kasner parameter and charge-to-mass ratio near criticality.
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$O(d,d)$ symmetric gravity and finite coupling holography
In O(d,d) symmetric gravity with curvature corrections, black brane singularities are not resolved but approach with altered Kasner exponents, while a dilaton generates negative cosmological constants at small coupling.