Thermodynamics of Liquid Interfaces: Surface Free Energy and Surface Tension
In interfacial thermodynamics, surface tension is the macroscopic manifestation of microscopic molecular cohesion. Within the bulk interior of a pure liquid, every molecule is surrounded symmetrically by neighboring molecules, experiencing attractive van der Waals, dipole-dipole, and hydrogen-bonding interactions that average to zero net directional force. At the liquid-vapor interface, however, molecules experience an abrupt discontinuity in intermolecular attraction: the dense liquid phase exerts a strong inward pull toward the bulk, whereas the tenuous vapor phase exerts negligible outward force. Consequently, bringing a molecule from the interior bulk to the surface requires positive thermodynamic work to sever intermolecular bonds against the cohesive field. The fundamental Gibbs surface free energy is defined as: dG = -S·dT + V·dP + γ·dA + ∑ μ_i·dn_i. At constant temperature, pressure, and composition, surface tension is the partial molar surface free energy: γ = (∂G / ∂A)_{T,P,n}, expressed in joules per square meter (J/m² = N/m). In the CGS system, the unit is dynes per centimeter (1 dyn/cm = 1 mN/m = 10⁻³ N/m). Because nature spontaneously minimizes Gibbs free energy (dG ≤ 0), liquids adopt geometries that minimize interfacial area per unit volume, which is why free liquid droplets assume spherical shapes.