Perturbative and Non-Perturbative Contributions to Black Hole Thermodynamics with String Clouds and Dark Matter Backgrounds
This paper investigates how perturbative logarithmic and non-perturbative exponential quantum corrections modify the thermodynamic properties, stability, and phase structure of black holes immersed in a perfect fluid dark matter background with a cloud of strings in anti-de Sitter spacetime, revealing that while non-perturbative effects are significant only near the Planck scale, neither correction type yields a van der Waals-like critical point.