♨️Thermodynamics of Fluids Unit 8 – Phase Equilibria and Stability
Phase equilibria and stability are crucial concepts in thermodynamics, governing how substances transition between states. This unit explores the conditions for phase coexistence, the criteria for system stability, and the tools used to predict and analyze phase behavior.
Students will learn about Gibbs free energy, chemical potential, and fugacity, as well as how to interpret phase diagrams. The unit also covers equilibrium conditions, stability criteria, and practical applications in various industries and natural systems.
Phase equilibrium occurs when two or more phases coexist in a system with no net transfer of mass or energy between them
Stability refers to a system's ability to maintain its state when subjected to small perturbations
Gibbs free energy (G) is a thermodynamic potential that determines the stability and spontaneity of a process at constant temperature and pressure
Defined as G=H−TS, where H is enthalpy, T is temperature, and S is entropy
Chemical potential (μ) is the partial molar Gibbs free energy and represents the change in G when a component is added to a system
Fugacity (f) is a measure of a component's tendency to escape from a phase, related to its chemical potential
Activity (a) is the effective concentration of a component in a mixture, accounting for non-ideal behavior
Raoult's law states that the vapor pressure of a component in an ideal solution is proportional to its mole fraction in the liquid phase
Henry's law describes the solubility of a gas in a liquid at low concentrations, where the gas's partial pressure is proportional to its mole fraction in the liquid
Thermodynamic Principles
First law of thermodynamics states that energy cannot be created or destroyed, only converted from one form to another
Expressed as ΔU=Q+W, where ΔU is the change in internal energy, Q is heat added, and W is work done
Second law of thermodynamics introduces the concept of entropy (S), a measure of the system's disorder or randomness
States that the entropy of an isolated system always increases or remains constant
Third law of thermodynamics establishes the absolute zero of entropy, stating that a perfect crystal at 0 K has zero entropy
Fundamental equation of thermodynamics relates the change in internal energy to changes in entropy, volume, and composition
dU=TdS−PdV+∑μidNi, where P is pressure, V is volume, and Ni is the number of moles of component i
Maxwell relations are derived from the fundamental equation and relate partial derivatives of thermodynamic properties
Gibbs-Duhem equation constrains the changes in chemical potentials of components in a mixture at constant temperature and pressure
Phase Diagrams and Their Interpretation
Phase diagrams graphically represent the equilibrium states of a system as a function of thermodynamic variables (e.g., temperature, pressure, composition)
Common types include pressure-temperature (P-T), temperature-composition (T-x), and pressure-composition (P-x) diagrams
Phase boundaries separate regions of the diagram where different phases are stable
Represent conditions at which two or more phases coexist in equilibrium
Triple point is a unique condition where three phases coexist in equilibrium
Critical point represents the highest temperature and pressure at which vapor-liquid equilibrium can exist
Tie lines connect the compositions of coexisting phases in a two-phase region
Lever rule determines the relative amounts of each phase present at a given overall composition
Eutectic point is the lowest temperature at which a liquid phase can exist in a binary system
Gibbs Phase Rule
Gibbs phase rule relates the number of degrees of freedom (F), components (C), and phases (P) in a system at equilibrium
Expressed as F=C−P+2
Degrees of freedom represent the number of independent variables that can be changed without altering the number of phases in equilibrium
For a single-component system, the maximum number of degrees of freedom is 2 (usually temperature and pressure)
In a binary system, the maximum number of degrees of freedom is 3 (temperature, pressure, and composition)
Applying the phase rule helps determine the variance of a system and the conditions under which phase transitions occur
Equilibrium Conditions
Chemical equilibrium is achieved when the chemical potentials of each component are equal in all phases
Expressed as μiα=μiβ=...=μiπ, where α, β, and π represent different phases
Thermal equilibrium requires the temperature to be uniform throughout the system
Mechanical equilibrium is reached when the pressure is the same in all phases
Gibbs energy minimization principle states that a system at constant temperature and pressure will minimize its Gibbs free energy at equilibrium
Common models for describing phase equilibria include ideal solution, regular solution, and activity coefficient models (e.g., Wilson, NRTL, UNIQUAC)
Equilibrium constants (K) relate the activities or fugacities of components in different phases at equilibrium
For vapor-liquid equilibrium, Ki=yi/xi, where yi and xi are the mole fractions of component i in the vapor and liquid phases, respectively
Stability Criteria
Thermodynamic stability requires that a system's Gibbs free energy is at a global minimum with respect to all possible perturbations
Mathematical conditions for stability involve the second derivatives of Gibbs free energy with respect to relevant variables
For example, (∂2G/∂T2)P>0 and (∂2G/∂P2)T>0 for thermal and mechanical stability, respectively
Spinodal curve represents the limit of metastability, beyond which a phase becomes unstable and spontaneously separates
Binodal curve (or coexistence curve) represents the equilibrium compositions of two phases in a binary system
Metastable regions exist between the binodal and spinodal curves, where a phase is stable with respect to small perturbations but unstable to large fluctuations
Gibbs stability criteria involve the determinant of the Hessian matrix of second derivatives of Gibbs free energy
A phase is stable if the determinant and all its principal minors are positive
Applications in Real Systems
Vapor-liquid equilibrium (VLE) is crucial in the design and operation of distillation columns, absorbers, and strippers
Liquid-liquid extraction (LLE) relies on the equilibrium distribution of a solute between two immiscible liquid phases
Solid-liquid equilibrium (SLE) is important in crystallization processes, such as in the pharmaceutical and food industries
Gas hydrates are solid compounds that form at high pressures and low temperatures, relevant in natural gas processing and flow assurance
Adsorption processes involve the equilibrium distribution of a solute between a fluid phase and a solid surface
Phase behavior of polymer solutions and blends is essential in the plastics and materials industries
Geochemical systems, such as mineral-fluid equilibria, are important in understanding the formation and evolution of Earth's crust
Biological systems, such as lipid membranes and protein folding, involve complex phase behavior and stability considerations
Problem-Solving Techniques
Identify the number of components, phases, and degrees of freedom using Gibbs phase rule
Determine the appropriate thermodynamic model for the system (e.g., ideal solution, activity coefficient models)
Write equilibrium conditions based on equality of chemical potentials or fugacities
Use mass balances and phase diagram information to set up a system of equations
Solve the system of equations numerically or analytically to obtain equilibrium compositions and phase amounts
Interpret the results in terms of phase stability, critical points, and other relevant features
Perform sensitivity analyses to assess the impact of uncertainties in model parameters or input data
Validate the results against experimental data or known phase behavior trends
Consider the limitations and assumptions of the chosen thermodynamic model and their implications for the solution