Abstract
Black hole thermodynamics, confined to the semi-classical regime, cannot address the thermodynamic stability of a black hole in flat space. Here we show that inclusion of a correction beyond the semi-classical approximation makes a black hole thermodynamically stable. This stability is reached through a phase transition. By using Ehrenfest’s scheme we further prove that this is a glassy phase transition with a Prigogine–Defay ratio close to 3. This value is well within the desired bound (2 to 5) for a glassy phase transition. Thus our analysis indicates a very close connection between the phase transition phenomena of a black hole and glass forming systems. Finally, we discuss the robustness of our results by considering different normalisations for the correction term.
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Banerjee, R., Modak, S.K. & Samanta, S. Glassy phase transition and stability in black holes. Eur. Phys. J. C 70, 317–328 (2010). https://doi.org/10.1140/epjc/s10052-010-1443-y
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DOI: https://doi.org/10.1140/epjc/s10052-010-1443-y