Insight into the Microstructures of Black Holes with Quantum-Triggered Violations
Haximjan Abdusattar
TL;DR
This work applies Ruppeiner thermodynamic geometry to charged AdS black holes with quantum conformal anomaly, exploring how the central charge $\alpha_{ m c}$ and electric charge $Q$ modify $P$-$V$ criticality and the microscopic structure. By computing coexisting volumes and the normalized thermodynamic curvature $R_N$ across three parameter regimes ($\alpha_c\le 0$, $0<\alpha_c< Q^{2}/8$, and $\alpha_c=Q^{2}/8$), the authors reveal universal critical behavior with a $t^{2}$ scaling of $R_N$ at criticality and regime-dependent coefficients, including $-\tfrac{1}{8}$ for $\alpha_c\le 0$ and $-2\pm\sqrt{3}$ or other values for the quantum-anomalous cases. They demonstrate that quantum conformal anomaly can induce multiple critical points, temperature-independent singularities, and sign changes in microstructure interactions, providing geometric fingerprints of quantum-corrected black hole thermodynamics. The results offer a geometric window into the microscopic degrees of freedom of quantum-corrected spacetimes and suggest universal features that may extend to other quantum-gravity-inspired black hole systems.
Abstract
In this study, we investigate the microstructures of a charged AdS (Anti-de Sitter) black hole exhibiting quantum anomalies through the lens of Ruppeiner geometry. Previous research has established that black holes undergo $P$-$V$ phase transitions and exhibit critical phenomena near their critical points, characterized by four critical exponents that typically obey scaling laws predicted by mean-field theory. However, recent findings have revealed that black holes with quantum anomalies can violate these scaling laws. Motivated by these discoveries, we employ Ruppeiner geometry to probe the thermodynamic fluctuations and gain insights into the microstructure of such black holes. Our analysis aims to elucidate how quantum effects modify the microscopic properties of spacetime, offering a novel perspective on the understanding of black hole thermodynamics.
