What is Equilibrium partition coefficient?
The ratio k = Cs/CL of the solute concentrations in the solid and liquid at a solidifying interface. It is the ratio of the solidus and liquidus compositions, and a solute with k < 1 is rejected into the liquid and causes segregation.
Japanese name: 平衡分配係数
Equilibrium partition coefficient appears in 3 practice questions across 1 topic, including Solidification and cast structures.
Field: Solidification and cast structures
Reading it from the phase diagram
The equilibrium partition coefficient k is the ratio Cs/CL of the compositions given by the solidus and liquidus at a given temperature. In systems where both the liquidus and the solidus fall toward the solute-rich side, the solidus lies on the solute-poor side, so k < 1; it is about 0.17 for Al-Cu and about 0.2 for δ iron in Fe-C. Conversely, in systems where adding solute raises the melting point, k > 1. If the lines of the phase diagram are approximated as straight, k can be treated as nearly independent of temperature, and the freezing range can be written using k as ΔT₀ = mC₀(1 − k)/k. The farther k is from 1, the larger the difference in composition between solid and liquid and the wider the freezing range.
How segregation arises
In an alloy with k < 1, the first solid to form has a concentration of kC₀, lower than the alloy average, and the excess solute is rejected from the interface into the liquid. Because diffusion in the solid is slow, the dendrite cores stay lean, and the outer parts that solidify from the enriched liquid have higher concentrations. This creates uneven concentration between the dendrite cores and the interdendritic regions (microsegregation), and low-melting eutectics and compounds collect in the parts that solidify last. Solute piled up ahead of the interface also causes constitutional supercooling, which changes the shape of the interface.
Use in purification
Differences in k are also used to purify materials. If only part of a rod is melted and the molten zone is moved slowly in one direction, impurities with k < 1 are pushed into the liquid, carried along with the zone and collected at the end of the rod. Repeating this, known as zone refining (zone melting), has been used to purify germanium and silicon for semiconductors. Because k differs from impurity to impurity, impurities with k close to 1 are harder to remove. The change in dopant concentration along the length of a crystal pulled from the melt is a result of the same partitioning.
FAQ
What is the difference between the equilibrium and the effective partition coefficient?
The equilibrium partition coefficient is the ratio Cs/CL when equilibrium holds at the interface. In real solidification a solute-rich layer forms ahead of the interface, so the ratio of the solid concentration to the concentration in the bulk liquid (the effective partition coefficient) approaches 1 as the growth rate increases.
What happens when k is greater than 1?
The solid takes up more solute than the liquid, so the parts that solidify first are richest in solute. The liquid concentration falls as solidification proceeds, giving the reverse segregation with rich dendrite cores and lean interdendritic regions.
Does k change with temperature?
In systems where the solidus and liquidus are not straight it changes with temperature. However, when the freezing range is narrow or for estimates it is often treated as a constant, and the Scheil equation is also derived with constant k.