Cubic equations of state
Cubic equations of state (EOS) are a class of thermodynamic models that describe the relationship between pressure (P), volume (V), and temperature (T) for real fluids, expressed as cubic polynomials in molar volume or the compressibility factor (Z).[1] These equations extend the ideal gas law by incorporating corrections for finite molecular size and intermolecular attractions, enabling predictions of phase behavior, including liquid-vapor equilibria, across a wide range of conditions.[1] Originating in the late 19th century, they remain foundational in chemical engineering due to their simplicity, computational efficiency, and applicability to nonpolar hydrocarbons and mixtures.[1] The development of cubic EOS began with Johannes Diderik van der Waals's 1873 doctoral thesis, which introduced the first such equation to account for the continuity between gaseous and liquid states:P = \frac{RT}{V_m - b} - \frac{a}{V_m^2},
where R is the gas constant, Vm is molar volume, a represents attractive forces, and b accounts for molecular volume exclusions.[2] In 1949, Otto Redlich and J. N. S. Kwong modified this form to improve high-pressure predictions by making the attraction term temperature-dependent:
P = \frac{RT}{V_m - b} - \frac{a}{\sqrt{T} V_m (V_m + b)},
with parameters a and b derived from critical properties.[3] This evolution continued in 1972 when Giorgio Soave refined the Redlich-Kwong equation for better vapor pressure correlations in hydrocarbons, introducing a temperature function for the attraction parameter α(T).[4] The Peng-Robinson EOS, proposed in 1976 by Ding-Yu Peng and Donald B. Robinson, further enhanced liquid density accuracy and applicability to natural gas systems through an adjusted form of the repulsion term.[5] In general, cubic EOS share a common structure, often generalized as
P = \frac{RT}{V_m - b} - \frac{a(T)}{V_m(V_m + u b) + w b (V_m - b)},
where u and w are constants specific to each variant (e.g., u = 1, w = 0 for Redlich-Kwong; u = 2, w = −b for Peng-Robinson), and parameters are typically functions of critical temperature (Tc), critical pressure (Pc), and acentric factor (ω).[1] These models are extensively applied in process simulation software for vapor-liquid equilibrium calculations, reservoir engineering, and the design of separation processes involving petroleum fractions and CO2 systems.[1] Their advantages include ease of parameterization and ability to capture subcritical phase transitions via multiple real roots, though they exhibit limitations in predicting properties of polar or associating compounds and near-critical densities without modifications.[1]