Thermodynamic topology of Einstein-Maxwell-Dilaton Theories

TL;DR

This paper explores the thermodynamic topology of charged AdS black holes in Einstein-Maxwell-Dilaton theories, revealing how scalar couplings influence phase transitions and stability through a topological framework.

Contribution

It introduces a topological classification of black hole thermodynamics in EMD theories, including new phases and the impact of dilaton coupling variations.

Findings

Identification of topological phase transitions near critical dilaton coupling.

Classification of black hole solutions into a novel topological class W^{0- ightarrow 1+}.

Demonstration that Gubser-Rocha models belong to this topological class.

Abstract

We present a systematic investigation of the thermodynamic topology for a broad class of asymptotically charged Anti-de Sitter (AdS) black holes in Einstein-Maxwell-Dilaton (EMD) theories, examining how scalar coupling parameters and spacetime dimensions influence black hole thermodynamics. Employing a topological approach that utilizes the torsion number of vector fields constructed from the generalized free energy, we characterize black hole states as topological defects within the thermodynamic parameter space. Through analytical solutions spanning dimensions $d = 4$, $d=5$, and $d=6$, including the Gubser-Rocha model, we demonstrate that variations in the dilaton coupling constant $\delta$, particularly near its critical value $\delta_c$, induce transitions between distinct thermodynamic topological phases. Our analysis reveals that certain black hole solutions constitute a novel class designated as $W^{0-\leftrightarrow 1+}$, characterized by a torsion number $W = 1$ that corresponds to a unique stability structure. We establish that Gubser-Rocha models belong to this topological classification. These results significantly expand the existing classification framework while reinforcing thermodynamic topology as a robust analytical tool for probing the universal properties of black holes in both gravitational and holographic contexts. The findings provide new insights into the relationship between microscopic couplings and macroscopic thermodynamic behavior in extended gravity theories.