Phase equilibria is a crucial concept in thermodynamics. It occurs when multiple phases of a substance coexist in balance, with no net mass transfer. This requires equal , , and for each component across all phases.
Phase diagrams visually represent phase equilibria. They show regions of stability for different phases and boundaries where phases coexist. Understanding these diagrams is key to predicting phase behavior and solving real-world thermodynamic problems.
Phase Equilibria and Phase Diagrams
Concept of phase equilibria
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Phase Diagram – Foundations of Chemical and Biological Engineering I View original
Occurs when two or more phases of a substance coexist in a state of dynamic balance with no net transfer of mass between phases
Phases have equal chemical potentials (μi) for each component i
Requires thermal equilibrium with equal temperature (T) among phases, mechanical equilibrium with equal pressure (P) among phases, and chemical equilibrium with equal chemical potential (μi) for each component i in all phases
Examples: Ice and water coexisting at 0°C and 1 atm, water and water vapor coexisting at 100°C and 1 atm
Construction of phase diagrams
Single-component phase diagrams
Pressure-temperature (P-T) diagrams show regions of stability for , liquid, and phases with lines representing phase boundaries where two phases coexist
represents coexistence of all three phases
is the terminus of the liquid-gas
Pressure-volume (P-V) diagrams use isotherms to represent constant temperature, regions to represent single-phase states, and tie lines to connect coexisting phases
Binary phase diagrams
Temperature- (T-x) diagrams at constant pressure show phase behavior of two-component mixtures
Liquidus line indicates temperature at which a solid phase begins to form
Solidus line indicates temperature at which the last liquid phase disappears
Eutectic point represents the lowest temperature of the mixture
Pressure-composition (P-x) diagrams at constant temperature show phase behavior of two-component mixtures under varying pressure with vapor-liquid equilibrium (VLE) and liquid-liquid equilibrium (LLE) curves
Types of phase transitions
First-order phase transitions involve a discontinuous change in properties (density, enthalpy) with latent heat associated with the transition
Examples: Melting, vaporization,
Second-order phase transitions involve a continuous change in properties with no latent heat associated with the transition
Examples: Superconductivity, ferromagnetism
Solid-solid phase transitions involve transitions between different crystal structures
Examples: Allotropic transformations (graphite to diamond)
Application of Gibbs phase rule
: F=C−P+2, where F is degrees of freedom (variance), C is number of components, and P is number of phases
Degrees of freedom represent the number of intensive variables (temperature, pressure, composition) that can be independently varied without changing the number of phases in equilibrium
Applications
Single-component systems: F=3−P
Triple point: F=0 (no degrees of freedom)
Phase boundaries: F=1 (univariant)
Binary systems: F=4−P
Eutectic point: F=1 (univariant)
Problem-solving with phase diagrams
Reading phase diagrams involves identifying phases present at given conditions and determining phase compositions and relative amounts
Lever rule is used to calculate the relative amounts of phases in a two-phase region, where lever arm lengths are inversely proportional to the mass fractions of the phases
Tie lines connect coexisting phases in a two-phase region with endpoints representing the compositions of the individual phases
Phase transformations involve
Heating and cooling processes to determine the sequence of phase changes and calculate the amount of heat absorbed or released
Pressure changes to predict phase changes along isotherms and determine the effect on phase equilibria
Thermodynamic Principles in Phase Equilibria
Gibbs free energy (G) is the thermodynamic potential at constant temperature and pressure
Criterion for phase stability: Minimum Gibbs free energy
Phase equilibria: Equal Gibbs free energy for each component in all phases
Chemical potential (μi) is the partial molar Gibbs free energy of component i and measures the tendency of a component to change phases
Phase equilibria: Equal chemical potential for each component in all phases
Fugacity (fi) and activity (ai) are the effective partial pressure and effective concentration of component i, related to chemical potential by μi=μi0+RTln(fi/fi0)=μi0+RTlnai
Phase equilibria: Equal fugacity or activity for each component in all phases
Clapeyron equation relates the slope of a phase boundary (dP/dT) to the changes in molar volume (ΔVm) and molar entropy (ΔSm) during a phase transition: dP/dT=ΔSm/ΔVm=ΔHm/(TΔVm)
Useful for solid-liquid and solid-solid phase transitions
is a specific form of the Clapeyron equation for vaporization, assuming ideal gas behavior and negligible volume of the condensed phase: ln(P2/P1)=−(ΔHvap/R)(1/T2−1/T1)