What is the thermodynamic foundation of vapor-liquid phase equilibrium (VLE), and how is phase coexistence defined?
Vapor-liquid phase equilibrium represents a state of thermodynamic coexistence between a liquid phase and its vapor phase. At equilibrium, three fundamental conditions must be simultaneously satisfied: (1) thermal equilibrium, requiring uniform temperature across both phases (T^L = T^V); (2) mechanical equilibrium, requiring uniform pressure across the interface (P^L = P^V = P); and (3) chemical equilibrium, requiring that the chemical potential of every chemical species i be identical in both phases: μ_i^L(T, P, x) = μ_i^V(T, P, y). Because chemical potential represents the escaping tendency of a substance from a phase, equality of chemical potentials ensures zero net mass transfer across the vapor-liquid interface.
In practical phase equilibrium calculations, chemical potential is related to fugacity f_i, where μ_i - μ_i° = RT ln(f_i / f_i°). The equilibrium condition therefore translates to equality of fugacities: f_i^L = f_i^V. In the vapor phase at low to moderate pressures (such as atmospheric pressure P = 101.3 kPa), vapor behaves as an ideal gas mixture, and the vapor fugacity is simply the partial pressure: f_i^V = y_i P. In the liquid phase, deviations from ideal solution behavior are captured by the activity coefficient γ_i: f_i^L = x_i γ_i f_i*, where f_i* is the fugacity of pure liquid i at system temperature and pressure, which equals the saturation vapor pressure P_i*(T) (neglecting the small Poynting pressure correction). Equating vapor and liquid fugacities yields the modified Raoult's law:
y_i P = x_i γ_i P_i*(T)
This fundamental relation governs all real distillation and boiling equilibria: it connects the directly measurable quantities (total pressure P, equilibrium temperature T, liquid composition x_i, and vapor composition y_i) to the microscopic intermolecular interactions quantified by the activity coefficient γ_i.