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Generalized Maxwell equal area law and black holes in complex free energy

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arxiv 2305.05916 v4 pith:VWYZVDSL submitted 2023-05-10 gr-qc hep-th

classification gr-qchep-th
keywords thermodynamicblackphaseareaenergyequalfreegeneralized
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Maxwell equal area law is an important and traditional analytical tool in thermodynamic phase transition, especially in the calculation of gas-liquid phase transition, which reconciles the theoretical calculation with the experimental results. Undoubtedly, its importance is also self-evident for the black hole thermodynamic system. In this study, we construct a generalized Maxwell equal area law, which allows different states of thermodynamic systems to be within the generalized free energy. The black hole thermodynamic characteristics are spontaneously emerged in the free energy landscape. Furthermore, by analytic continuation, we utilize the properties of analytical functions to investigate some universal characteristics of thermodynamic phase transitions in black holes, and preliminarily establish the counterpart of thermodynamic phase transitions in the complex domain.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Resolved Maxwell-Boundary Normal Forms and Exact Reentrant Scaling in Accelerating AdS Black Holes

    hep-th 2026-07 accept novelty 8.0 of 10

    The charged accelerating AdS black hole has an exact reentrant-turning locus for all 0<µ<0.2026, with the pressure and temperature windows vanishing as µ⁴ and µ³ and a universal blow-up profile bT = 2√bP − bP.

  2. Unifying topological, geometric, and complex classifications of black hole thermodynamics

    gr-qc 2026-04 unverdicted novelty 7.0 of 10

    Three classification schemes for black hole thermodynamics are equivalent, with the count of temperature extrema determining the class in each framework.

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