Universal thermodynamic topological classes of rotating black holes

In a recent study, Wei et al. (2024) [96] proposed a universal classification scheme that interprets black hole solutions, including the four-dimensional Schwarzschild, Reissner-Nordström (RN), Schwarzschild-AdS, and RN-AdS black hole solutions, as topological defects within the thermodynamic parameter space, and then divides black hole solutions into four distinct classes, denoted as W1−, W0+, W0−, and W1+, offering insights into deeper aspects of black hole thermodynamics and gravity. In this paper, we investigate the universal thermodynamic topological classification of the singly rotating Kerr black holes in all dimensions, as well as the four-dimensional Kerr-Newman black hole. We show that the innermost small black hole states of the d≥6 singly rotating Kerr black holes are thermodynamically unstable, while those of the four-dimensional Kerr-Newman black hole and the d=4,5 singly rotating Kerr black holes are thermodynamically stable. On the other hand, the outermost large black holes exhibit unstable behavior in all these cases. At the low-temperature limit, the d≥6 singly rotating Kerr black holes have one large thermodynamically unstable black hole state, while the four-dimensional Kerr-Newman black hole and the d=4,5 singly rotating Kerr black holes feature one large unstable branch and one small stable branch. Conversely, at the high-temperature limit, the d≥6 singly rotating Kerr black holes exhibit a small unstable black hole state, while the four-dimensional Kerr-Newman black hole and the d=4,5 singly rotating Kerr black holes have no black hole states at all. Consequently, we demonstrate that the d≥6 singly rotating Kerr black holes belong to the class W1−, whereas the four-dimensional Kerr-Newman and d=4,5 singly rotating Kerr black holes belong to the class W0+, thereby further support the conjecture proposed in Wei et al. (2024) [96].