This tutorial will teach you all you really want to know about phase diagrams and maybe a little more. If you are uncertain about your termodynamic knowledge please first follow the crack course on thermodynamics and modeling
Even if you are just interested in understanding binary phase diagrams you should follow carefully the sections on unary and modeling first. Unary diagrams are simpler than binaries and many facts and terms will understood more easily for unary systems and using thermodynamic models. In the binary section you are expected to be familiar with many terms first explained in the unary and model sections.
It is the hope of the author that when you have reached the binary section you will be so interested to read also the ternary and multicomponent section because these diagrams are the really useful ones and they are, in fact, much simpler than the binary phase diagrams.
In almost all 2-dimensional scientific diagrams you have come across until now the lines in a diagram express some explicit functional relationship between the dependent variable (usually the x axis) and independent variable (usually the y axis) like y=f(x). This is not true for phase diagrams. |
A phase diagram is more like a map. On a map you do not expect any relation between the x and y coordinates of the line defining the border between land and sea or between two countries for eaxmple. In the same way the lines in a phase diagram do not express any relationship between the two axis variables. The lines in a phase diagram simply separate regions with different sets of stable phases at equilibrium. The condition of equilibrium is the reason thermodynamics and phase diagrams are closely connected. Later, when you feel confident using equilibrium phase diagram, we will show you how to and understand phase diagram when the phases are not in full equilibrium ... |
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You may also have dealt with functions of several variables and found it difficult to visualize things in more than 3 dimensions. On the other hand, if you learned quantum mechanics you are familiar with reciprocal space with an infinite number of dimensions so then it should be no problem to handle realities than cannot be visualized in just 2 or 3 dimensions.
The thermodynamic properties of the phases vary with the state variables used as axis in the diagram and a new phase may become stable, or a stable phase may become unstable, at a certain set of values of these axis variables. Such a change of the set of stable phases is a point on a line in the phase diagram. As the properties of phases vary continuously the point will become a line, surface or hyper-surface when varying the one, two or more axis variables.
Most phase diagrams are 2-dimensional because that is the most easy to draw. But one may draw 1-dimensional and 3-dimensional phase diagrams although the latter kind is more for show. In reality the dimensionallity of a phase diagram for a system is determined by Gibbs phase rule (explaned later) which states that the dimensionality (in most cases) should be equal to n+1 where n is the number of components. So only unary systems can be drawn completely in a 2-dimensional phase diagram. But if pressure is kept constant can use 2-dimensional phase diagrams also for binary systems. Most real systems have many components and one has to section or project the real multidimensional phase diagram in different ways to obtain a 2-dimensional phase diagram
The 1-dimensional phase diagram for pure H2O at 1 bar is shown in this figure. At varying temperatures this molecule can be solid (ice), liquid (water) and gas (steam). The temperatures for these transformations is shown by tic marks on the temperature axis. This phase diagram is shown here as we have all experience of the phase transformations associated with water. Note that the transformations from ice to liquid water (freezing point) and from liquid to gas (boiling point) occurs at a specific temperature. We know there are many properties that vary with the temperature for example the volume. In the next diagram, which is not a phase diagram, the volume of water is shown as a function of temperature. Note that there are discontinuities in the volume at the temperatures where the phase changes. This is because the properties of each phase depend on its structure and the volume of H2O as ice, liquid and gas are independent of each other. The figure is drawn by hand and the changes are not to scale. You can notice the volume of ice is larger than that of liquid water at the freezing point which means that ice floats on liquid water. The volume change from liquid to gas is much larger and the gas has a larger volume at 100 oC than the same amount of liquid. If we allow the pressure to vary the temperatures for these transformations will change. At low pressure at high altitude the boling point is much lower as a phase with large molar volume becomes more stable at low pressure. The volume change associated with the freezing is much smaller and the freezing point is not affected so much. But as the volume of ice is higher than that of liquid the freezing point increases also with lower pressure. The temperature-pressure phase diagram of H2O will be discussed later. Adding another component to the system will also change these transformation temperatures. And that is the main topic in all 2-dimensional phase diagrams shown later. |
The 1-dimensional phase diagram for H2O. |
Volume as function of temperature for H2O. This is NOT a phase diagram. |
The diagram to the right is the binary phase diagram for the Ag-Cu system at atmospheric pressure. For easier explanation the different areas have been colored, in most other cases all areas will be white. The vertical borders of the diagram are the pure elements. At low temperature both pure elements are solid and can dissolve a small amount of the other element, those areas are yellow. At some temperature the elements melt and in the upper red part the liquid phase is stable across the whole system. When crossing one of the lines from the yellow or red to the blue areas one has two phases stable, in this case liquid and either solid Ag or Cu. Finally in the green area, below the horizontal line connecting the two yellow areas and the lowest point of the red area, one has two solid phases. One of the solid phases is almost pure Ag and the other almost pure Cu. The mutual solubility decreases at lower temperature as the yellow areas becomes more narrow (and the green wider). The first important step in understanding 2-dimensional phase diagram is that it consists of different kind of areas with different number of stable phases. |
In a single phase area there is a single phase stable for the values of the axis variables. For a point in an area with two or more phases stable there is no phase stable for the values of the axis variables for the point but one has a combination of two or more phases with properties that can be added together to give the axis value for the point. And in some important cases one can still deduce the properties of the stable phases.
To give a taste of what will learn we show you a colored phase diagram for a multicomponent steel to the right. This alloy has 8 elements Cr, C, Co, Si, Mn, W, V and the rest Fe. The nominal composition, in mass (weight) percent is given below. It is a so called high speed steel used for for high temperature cutting for example in drills and saws.
Each colored area has a different set of stable phases, there are up to 6 phases stable in some areas. The colors have been added to make the diagram it look nicer (or more lika a map). Areas with the same color does not have the same set of phases. The phase diagram is not exactly for this alloy as the carbon content is varying along the horisontal axis, but the diagram is useful because carbon is a very light element and can easily diffuse in or out of the material and as you can see the set of stable phases changes a lot with the carbon content. The vertical axis is the temperature in Kelvin and it is useful to know the phase changes when the material is heated and this kind of material may be used up to 1000 K without loosing its hardness. The content of the other alloying elements, except Fe, is constant in the whole diagram. |
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These multicomponent phase diagrams can be calculated from databases with assessed thermodynamic models and that is why there is a section on models in this tutorial. We will look at it again at the end of the course to understand it better.
You may not believe it but it is much easier to understand these kinds of multi-component phase diagrams that binary phase diagrams. One reason for that is that they can be used just to know the set of stable phases for the aqes values. In binary and ternary phase diagrams one can extract more information, for example the composition of the phases in equilibrium.
Along the lines separating the colored areas in the phase diagram at least one phase must be just stable, i.e. have zero amount. The lines are thus often called a ``zero phase amount'' or ``zero phase fraction'' (ZPF) lines.
Two ZPF lines may meet and at that point at least two phases must have zero amount. Depending on the type of diagram one can draw different conclusions how the lines should extrapolate from this point.In phase diagrams some of the points where the ZPF lines meet have a special importance. These points are called invariant points because the number of phases with zero fraction at these points is equal to the degrees of freedom in the phase diagram. Depending on the axis in the diagram an invariant point is sometimes an invariant line.
A big difference beween maps and phase diagrams are that a map always have distances as axis. In a phase diagram one can have either extensive quantities, for example composition or volume, or intensive quantities (potentials) for example temperature, pressure or chemical potential. This means that the lines has to be interpreted sligtly differently depending on the the axis of the diagram.
Another big difference is that a 2-dimensional phase diagram, except for unary systems, is always a section or projection of a multi-dimensional reality. This means there are things "hidden" outside the plane of the diagram that it is sometimes useful to be aware of.
A summary of the lines in a phase diagram:
A 2-dimensional phase diagram, like any map, consists of areas separated by lines. In all phase diagrams the "fundamental" lines are all ZPF lines (except the borders of the diagram). Note that a ZPF line may have more than one phase with zero fraction along the line, for example when the axis are potentials.
But quite often those who draw phase diagrams like to put additional lines to explain other features like microstructures or metatstable states. It may take some experience to identify the ZPF lines from other added lines.
In phase diagrams with the composition along at least one axis, some of the ZPF lines are known as solubility lines. A solubility line is the border of a single phase region giving the limit of solubility of a component in that phase. As the solubility line is also a ZPF line the amount of another phase is zero along the solubility line. But in general the ZPF lines are not solubility lines.
You will often find another important kind of line in the phase diagram that is called tie-line. A tie-line connects two phases in equilibrium across a two-phase region. In some ternary phase diagrams one can even have "tie-triangles" which means that three tie-lines join the 3 phases in equilibrium as a triangle and inside the triangle one has 3 phases stable.
It is possible for a tie-line to coincide with a ZPF line. An important case are the "invariant lines" in binary phase diagrams with temperature and composition as axis. The line representing the invariant equilibria at constant temperature joins together 3 phases in equilibrium. This invariant line can be split into 3 different ZPF lines and 3 different tie-lines, and this tutorial will make this fact very easy to understand.
In multicomponent systems one can have more than 3 phases in equilibrium and at the end of this tutorial you will be able to visualize multidimensional "tie-planes" joining together compositions of 4 or more phases in equilibrium. But do not worry, they will never appear as lines in phase diagrams.
The most important fact about an area in a phase diagram is that it has a fixed set of stable phases. But one can additionally classify the ares into 3 kinds:
The phase diagrams can be divided into several different types:
Many of these types are overlapping but they will all be explained in this tutorial. You may also have heard about other types of phase diagrams because people like to invent names for each particular feature like "eutectic phase diagram".
Example coffee+sugar and water+salt
More advanced experimental techniques
We will frequently refer to thermodynamic models to describe the origin of different features of the phase diagram. It is much easier to explain them this way and the development and use of multicomponent phase diagrams is impossible without thermodynamic modeling. Please follow the crack course in thermodynamics if you feel uncertain about this subject.
For the modeling of phase diagrams the Gibbs energy per mole components Gm(T,P,xi ) is the most frequently used thermodynamic function because most phase diagrams is at fixed pressure. Only in very special cases, like the phase diagram for pure water, Helmhotz energy per mole component Am(T,V,xi ) must be used because the Gibbs energy cannot handle a miscibility gap in volume.
If you are not sure what a phase is please review the thermodynamics crack course. Just in brief:
A phase must have a continuous Gibbs energy function and the first and second derivatives of the Gibbs energy, must also be continuous, there can be no discontinuety in any quantity for a single phase. If one has such a discontinuety that is an indication of a phase change. The Gibbs energy per mole, Gm of a phase is usually very smooth function of T P and composition. Also the derivatives of Gm, i.e. entropy, volume and chemical potentials, are often very smooth.
The second derivatives of the Gibbs energy, i.e. the heat capacity CP thermal expansivity \alpha, isothermal compressibility \kappa and the stability function \omega must be continuouos but can have more drastic changes. The third derivatives of Gm for a phase does not have to be continuous.
An example of a drastic change in the heat capacity is shown in Fig.~\ref{fg:cpiron} for the heat capacity for pure iron. The ferromagnetic transition in bcc makes the heat capacity approach infinity at the Curie temperature. But according to theory the heat capacity must be continuous. Another example is the stability function shown in Fig.~\ref{fg:b2} which shows its value in the B2 phase in Al-Ni.
The derivative of the Gibbs energy with respect to a component i, at fixed T, P and amount of all other components, is the chemical potental of that component and denoted $\mu_i$
In all kinds phase diagram the total amount of the components is irrelevant, one has the same equilibrium if the system is 1 mole or 1 g. The system size is denoted N for moles and B for mass.
For systems with 2 or more components one can also vary the composition of the system (as noted earlier the total size is irrelevant for the equilibrium). The amount of different components is denoted Ni or Bi for the number of moles or mass of component i. Most often the amounts is not given as total number but as fraction or percent and the notation is xi for mole fraction and wi for mass fraction. There is no shorthand notation for mole or mass percent. For computer input and output italics and indices can usually not be used and the notation x(i) and w(i) is used.
When using the Gibbs energy per mole to describe a thermodynamic system the natural variables are T (temperature), P (pressure) and the mole fractions xi of the components. Their conjugate quantities S (entropy), V (volume) and chemical potentials $\mu_i$ are also quantities that can vary.
Other thermodynamic quantities that are useful are the H (enthalpy). G, A and H are also called state functions and for a closed system at constant T and P the Gibbs energy should be at a minimum. A closed system at constant T and V should have have a minimum for the Helmholtz energy at equilibrium. If you feel uncertain about these statements please review the thermodynamics crack course.
The value of extensive state variables depend on the size of the system and are different in different phases at equilibrium. Examples are G, S, V, Ni, etc.
The value of extensive state variables is independent on the size of the system. Examples are T, P, $\mu_i$.
The composition of a system may also be varied through $\mu_i$, the chemical potential or ai, the activity, of component i. The chemical potential is defined as the partial derivative of the Gibbs energy relative to the amount of the component, keeping T, P and the amounts of all other components fixed.
Most phase diagrams are for constant pressure and for varying T and one composition, xi of the system. But note that in physics phase diagrams are often calculated for constant V and varying activity ai. This may lead to some surprising relations
The thermodynamic variables always appear in pairs, like T and S, P and V and Ni and $\mu_i$ in the expression for the Gibbs energy
where the latter is written for one mole of material. In each pair one variable is extensive and the other intensive.
We will frequently refer to a rule established by Gibbs giving the degrees of freedom of a system, f. In a system with n components and p stable phases at variable T and P the degrees of freedom is f=n-p+2. If P is fixed then f=n-p+1 and if both T and P are fixed f=n-p. The value of f must be zero or positive. If it is zero it means one has in {\em invariant} point in the phase diagram. At an invariant point the set of stable phases is maximum and whatever change is made in the axis the set of phases will change.
If the degrees of freedom is 1 it means one can change one variable in the system and still have the same set of stable phases. But the change must not be too large, another phase may appear or one stable phase may become unstable.
The Gibbs phase rule applies strictly only to phase diagrams with only potentials as axis variables. If one has an extensive variable as one axis, like in most binary phase diagrams, one must apply the rule with some care.
In a single phase region one has just one stable phase. The meaning of the word ``region'' is that the same phase remains stable for (small) variations of the conditions.
In a two-phase region there are two phases stable. In the two-phase region one can always draw tie-line connecting the points representing the phases that are in equilibrium. Depending on the type of diagram one can be in the plane of the diagram and even parallel to one of the axis or it can be outside the plane. The word "region" means that for (small) changes of the axis variables one will still have the same set of stable phases but their amount and composition may change.
A tie-line is a line that ``ties together'' phases that are in equilibrium. The German name ``Konod'' is also often used. In binary phase diagrams with temperature and composition on the axis one can fill the two-phase regions with horisontal tie-lines connecting the phases that are in equilibrium.
A tie-line should be a straight between the phases in equilibrium but in some diagrams, that are not really phase diagramsm but may look like and be used as, the tie-lines can be curved.