Departure function
In thermodynamics, a departure function is defined for any thermodynamic property as the difference between the property as computed for an ideal gas and the property of the species as it exists in the real world, for a specified temperature T and pressure P. Common departure functions include those for enthalpy, entropy, and internal energy. Departure functions are often used to "transform" hard problems involving nonideal fluids into easier problems involving state changes of ideal gases. The "easier" problems can then be solved directly, and the departure function allows one to transform back to the nonideal fluid and calculate the properties of the fluid.
Departure functions can be computed via calculus from an equation of state.
Departure functions for Peng-Robinson equation of state
The Peng-Robinson equation of state relates the three interdependent state properties pressure P, temperature T, and molar volume Vm. From the state properties (P, Vm, T), one may compute the departure function for enthalpy per mole (denoted H) and entropy per mole (S)[1]:
Where is defined in the Peng-Robinson equation of state, Tr is the reduced temperature, Pr is the reduced pressure, z is the compressibility factor, and
Typically, one knows two of the three state properties (P, Vm, T), and must compute the third directly from the Peng-Robinson equation of state. To calculate the third state property, it is necessary to know three constants for the species at hand: the critical temperature Tc, critical pressure Pc, and the acentric factor ω. But once these constants are known, it is possible to evaluate all of the above expressions and hence determine the enthalpy and entropy departures.
References
- ^ Kyle, B.G. Chemical and Process Thermodynamics, 3rd Ed. Prentice Hall PTR, 1999. p. 118-123.