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The microscopic structure of black holes remains a challenging subject. Inthis paper, based on the well-accepted fact that black holes can be mapped tothermodynamic systems, we make a preliminary exploration of the microscopicstructure of the thermodynamically stable Schwarzschild anti-de-Sitter (SAdS)black hole. In accordance with the number density and thermodynamic scalarcurvature, we give the interaction potential among the molecules ofthermodynamically stable SAdS black holes and analyze its effectiveness.Moreover, we derive the thermo-correction to the equation of state for suchblack holes that arises from interactions among black-hole molecules usingvirial coefficients.

Interaction potential and thermo-correction to the equation of state for thermally stable Schwarzschild Anti-de Sitter black holes