# Critical phenomena and chemical potential of charged AdS black hole

**Authors:** Shao-Wen Wei, Bin Liang, Yu-Xiao Liu

arXiv: 1705.08596 · 2017-12-20

## TL;DR

This paper investigates the thermodynamics and phase transitions of a five-dimensional charged AdS black hole, focusing on the chemical potential related to the cosmological constant interpreted as the number of colors in the boundary gauge theory, revealing critical phenomena and phase diagrams.

## Contribution

It introduces a novel analysis of black hole thermodynamics using the gauge theory parameter N as a thermodynamic variable and explores the critical behavior and phase structure in this context.

## Key findings

- Existence of small-large black hole phase transition.
- Charge-independent reduced thermodynamic quantities.
- Determination of critical exponents near the second-order phase transition.

## Abstract

We study the thermodynamics and the chemical potential for a five-dimensional charged AdS black hole by treating the cosmological constant as the number of colors $N$ in the boundary gauge theory and its conjugate quantity as the associated chemical potential $\mu$. It is found that there exists a small-large black hole phase transition. The critical phenomena are investigated in the $N^{2}$-$\mu$ chart. In particular, in the reduced parameter space, all the thermodynamic quantities can be rescaled with the black hole charge such that these reduced quantities are charge-independent. Then we obtain the coexistence curve and the phase diagram. The latent heat is also numerically calculated. Moreover, the heat capacity and the thermodynamic scalar are studied. The result indicates that the information of the first-order black hole phase transition is encoded in the heat capacity and scalar. However, the phase transition point cannot be directly calculated with them. Nevertheless, the critical point linked to a second-order phase transition can be determined by either the heat capacity or the scalar. In addition, we calculate the critical exponents of the heat capacity and the scalar for the saturated small and large black holes near the critical point.

## Full text

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## Figures

49 figures with captions in the complete paper: https://tomesphere.com/paper/1705.08596/full.md

## References

32 references — full list in the complete paper: https://tomesphere.com/paper/1705.08596/full.md

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Source: https://tomesphere.com/paper/1705.08596