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Dynamic behaviours of black hole phase transitions near quadruple points

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arxiv 2304.08969 v2 pith:FL3NOZBG submitted 2023-04-18 gr-qc hep-th

classification gr-qchep-th
keywords blackdynamicholephasequadrupletransitionsdistributionenergy
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Treating the horizon radius as an order parameter in a thermal fluctuation, the free energy landscape model sheds light on the dynamic behaviour of black hole phase transitions. Here we carry out the first investigation of the dynamics of the recently discovered multicriticality in black holes. We specifically consider black hole quadruple points in D=4 Einstein gravity coupled to non-linear electrodynamics. We observe thermodynamic phase transitions between the four stable phases at a quadruple point as well as the weak and strong oscillatory phenomena by numerically solving the Smoluchowski equation describing the evolution of the probability distribution function. We analyze the dynamic evolution of the different phases at various ensemble temperatures and find that the probability distribution of a final stationary state is closely tied to the structure of its off-shell Gibbs free energy.

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  1. High-order QED correction impacts on phase transition of the Euler-Heisenberg dS spacetime

    hep-th 2025-07 conditional novelty 5.0 of 10

    The dual-horizon coexistence region in Euler-Heisenberg de Sitter spacetime exhibits van der Waals-like phase transitions whose order depends on a nonlinear parameter, with a constant topological number W=+1.

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