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The universal crossover from thermodynamics and dynamics of supercritical RN-AdS black hole

Published 7 Apr 2025 in gr-qc, astro-ph.CO, hep-ph, and hep-th | (2504.04995v1)

Abstract: We study the properties of supercritical Reissner-Nordstr\"om Anti-de Sitter (RN-AdS) black holes in the extended phase space with the pressure defines as the cosmological constant. Supercritical black holes exist in the region where both temperature and pressure exceed the critical point, known as the supercritical region. The conventional view states that black holes in this regime are indistinguishable between large and small phases. However, recent research reveals that the supercritical regime exhibits universal gas-like and liquid-like phase separation, which shed light on the study on the supercritical region of RN-AdS black holes in the extended phase space. In this work, we calculate the thermodynamic potential and quasinormal modes (QNMs) of RN-AdS black holes, and identify transition curves between two different states in supercritical region using thermodynamic and dynamic methods. On one hand, we find the thermodynamic crossover curve (Widom line) by defining the scaled variance $\Omega$ (a higher-order derivative of Gibbs free energy). On the other hand, we identify the dynamic crossover curve (Frenkel line) by analyzing transitions between distinct QNM decay modes.

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