Critical Inter-Horizon Thermal Dynamics on the Lukewarm Reissner-Nordström-de Sitter Manifold

Résumé

We reinterpret the lukewarm sector of four-dimensional Reissner--Nordström--de Sitter black holes as the exact zero-dissipation thermal manifold of an effective two-horizon nonequilibrium system. In the fixed-charge sector, the inter-horizon thermal affinity controls the entropy production and vanishes precisely on the lukewarm branch. The corresponding linearized thermal mode is governed by an exact relaxation coefficient \(K_L(ρ)\), with \(ρ=r_+/r_c\), and changes stability at the critical ratio \[ ρ_*=\frac{1+\sqrt{3}-\sqrt{2}\,3^{1/4}}{2}\approx 0.4354, \] where the relaxation time diverges as \(τ\sim |ρ-ρ_*|^{-1}\). We then encode this critical structure in a minimal Bragg--Williams functional and an Onsager--Machlup action for the effective trajectories of the thermal mode. In this way, the lukewarm branch is promoted from a geometric equal-temperature locus to a critical inter-horizon thermal manifold.

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