The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh...

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The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting 4 th May

Transcript of The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh...

Page 1: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

The thermodynamics of phase transformations

Robin Perry

School of Physics and Astronomy,

Edinburgh

Introduction to Computer Simulation of Alloys meeting 4th May 2010

Page 2: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

1. Preamble: phase diagrams of metal alloys

Page 3: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

1. Preamble: phase diagrams of metal alloys

2. Gibbs free energy, equilibrium and chemical potential, Gibbs phase rule

3. Single component systems

1. dG(T)

2. Clausius-Clapeyron equation and the phase diagram of titanium

4. Binary (two component) systems

1. Ideal solutions

2. Regular solutions

3. Activity

4. Real solutions, ordered phases and Intermediate phases

5. Binary phase diagrams

1. Miscibility gap

2. Ordered alloys

3. Eutectics and peritectics

4. Additional useful relationships

5. Ternary diagrams

6. Kinetics of Phase transformations

Contents

Page 4: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

2. Gibbs free energy, equilibrium and chemical potential, Gibbs phase rule

Definition of terms :

Phase, K: portion of the system with homogeneous properties and composition. Physically distinct.

Components, C : chemical compounds that make up a system

Gibbs free energy, G (J/mol): measure of relative stability of a phase at constant temperature and pressure

G = E + PV TS + N

Intensive variables : Temperature, T (K); Pressure, P (Pa);

Extensive variables : Internal energy E (J/mol); Volume, V (m3), Entropy (J/K mol) particle number, N; Chemical potential (J/mol)

Solids/liquid transitions in metals: PV small ignore

Page 5: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

Equilibrium : the most stable state defined by lowest possible G dG = 0

equilibriummetastable

E.g. Metastable : DiamondEquilibrium : Graphite

Solid : Low atomic kinetic energy or E low T and small S

Liquid : Large E high T and large S

Chemical potential or partial molar free energy governs how the free energy changes with respect to the addition/subtraction of atoms.

This is particularly important in alloy or binary systems.(particle numbers will change)

2. Gibbs free energy, equilibrium and chemical potential, Gibbs phase rule

Page 6: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

2. Gibbs free energy, equilibrium and chemical potential, Gibbs phase rule

Gibbs phase rule for equilibrium phase :

Examples :Single component system C=1 and F = 3 K

If 1 phases in equilibrium (e.g. solid) 2 degrees of freedom i.e. can change T and P without changing the phase

If 2 phases in equilibrium (e.g. solid and liquid) 1 degree of freedom i.e. T is dependent on P (or vice-versa)

If 3 phases in equilibrium (e.g. solid, liquid and ) 0 degrees of freedom. 3 phases exist only at one fixed T and P.

Number of degrees of freedom F = C – K +2

C, number of components

K, number of phases in equilibrium

Page 7: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

3. Single component systems

For purposes of most discussions :

fix pressure (unless otherwise stated)

For pressure dependence:

Similar arguments apply : Vliquid > Vsolid so increasing P implies liquid to solid transition

From thermodynamics: Sliquid > Ssolid

G

T (K)TM

Gsolid

Gliquid

Phase transition occurs when:

Gsolid=Gliquid

Assumption: Closed system ignore d

Page 8: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

Clausius Clapeyron Equation

Lessdense

moredense

Lessdense

moredense

(intermediate)

Page 9: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

4. Binary (two component) systems : Ideal solutions

Two species in the mixture: consider mole fractions XA and XB XA + XB = 1

G1 = XAGA + XBGB

Two contributions to G from mixing two components together:

1. G1 – weighted molar average of the two components

2. Free Energy of mixing

GMIX = Hmix - T SMIX

Where Hmix is the heat absorbed or evolved during mixing or heat of solution

SMIX is the entropy difference between the mixed and unmixed states

Page 10: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

4. Binary (two component) systems : Ideal solutions

Simplest case : Ideal solution : HMIX = 0

Some assumptions : 1. Free energy change is only due to entropy2. Species A and B have the same crystal structure

(no volume change)3. A and B mix to form substitutional solid solution

- total number of microstates of system or total number of distinguishable ways of arranging the atoms

Using Stirling’s approximation and NakB=R

Boltzmann equation: S = kB ln ( ) S is the configurational entropy

GMIX = RT(XAlnXA + XBlnXB)

Mixing components lowers the free energy!M

olar

Fre

e E

nerg

y

Page 11: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

4. Binary (two component) systems : The chemical potential

Chemical potential : governs the response of the system to adding component

Two component system need to consider partial molar A and B.

Total molar Gibbs free energy = SdT + AXA + BXB (+VdP)

Simplified equations for an ideal liquid:

AXA = GA +RTlnXA

BXB = GB +RTlnXB

I.e. A is the free energy of component A in the mixture

Page 12: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

4. Binary (two component) systems : Regular solutions and atomic bonding

Generally: HMIX0 i.e. internal energy of the system must be considered

In a binary, 3 types of bonds: A-A, B-B, A-B of energies AA, BB, AB

Define: HMIX= CAB where CAB is the number of A-B bonds and = AB ½(AA +BB)

HMIX= XAXBWhere =Naz, z=bonds per atom

If <0 A-B bonding preferred

If >0 AA, BB bonding preferred

GMIX = HMIX + RT(XAlnXA + XBlnXB)

Point of note:

GMIX always decreases on addition of solute

Page 13: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

Mixing always occurs at high Temp. despite bonding

Mixing if A and B atoms bond

A and B atoms repel Phase separation in to 2 phases.

Free energy curves for various conditions:

Page 14: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

4. Binary (two component) systems : Activity, a of a component

-RTln aA

0 1XB

-RTln aB

B

A

GMIX

A = GA + RT ln aA GA

GBActivity is simply related to chemical potential by:

B = GB + RT ln aB

It is another means of describing the state of the system. Low activity means that the atoms are reluctant to leave the solution (which implies, for example, a low vapour pressure).

i.e. For homogeneous mixing, <0 aA<XA and aB<XB

So the activity is the tendency of a component to leave solution

Page 15: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

For low concentrations of B (XB<<1)

Henry’s Law (or everything dissolves)

Raoult’s LawAnd…

Homogeneous mixing

HMIX > 0

HMIX < 0

Page 16: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

5. Binary phase diagrams : The Lever rule

Phase diagrams can be used to get quantitative information on the relative concentrations of phases using the Lever rule :

At temperature, T and molar fraction X0, the solid and liquid phase will coexist in equilibrium according the ratio:

Temperature

A B

T

Solid, S

Liquid, L

X0

ll

nl = nl

i.e. ~25% solid and ~75% liquid at X0

Where n/n is ratio of liquid to solid

Page 17: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

Solid to liquid phase diagram in a two component system : A and B are completely miscible and ideal solutions

Page 18: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

5. Binary phase diagrams : The Miscibility gap

A B

T1

G

liquid

solid L

Common tangent

A B

G

Sa b c d

T2

S

A B

T3

G

L

e f

HMIX > 0

A BXB

liquidT1

T2

T3e f

Single phase, mixed solid

2 phase: (A+B) and (B+A)Compositions e and f ;“The miscibility gap”

Page 19: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

Titanium-Vanadium revisited

(bcc)

(hcp)

What can we deduce?

1. Ti and V atoms bond weakly

2. There are no ordered phases

3. (Ti,V) phase : mixture of Ti and V in a fcc structure

4. Ti (hcp) phase does not dissolve V well

Blue : single phase

White : two phase(bcc)

Page 20: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

Equilibrium in heterogenous systems

For systems with phase separation ( and ) of two stable structures (e.g. fcc and bcc), we must draw free energy curves.

G is the curve for A and B in fcc structure ( phase)

G is the curve for A and B in bcc structure ( phase)

For: X0<e phase only

X0>e phase only

If e<X0>e then minimum free energy is Ge

And two phases are present

(ratio given by the Lever rule – see later)

When two phases exist in equilibrium, the activities of

the components must be equal in the two phases:

Common tangent

Page 21: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

4. Binary (two component) systems : Ordered phases

Previous model gross oversimplification : need to consider size difference between A and B (strain effects) and type/strength of chemical bonding between A and B.

Ordered substitutional

Ordered phases occur for (close to) integer ratios.

i.e. 1:1 or 3:1 mixtures.

But entropy of mixing is very small so increasing temperature can disorder the phase. At some critical temperature, long range order will disappear.

Ordered structures can also tolerate deviations from stoichiometry. This gives the broad regions on the phase diagram

Systems with strong A-B bonds can form Ordered and/or intermediate phases

Page 22: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

The Copper-Gold systemRandom mixture

Single phases Mixed phases

N.B. Always read the legend!!! (blue is not always ‘singe phase’)

(fcc)(fcc)

Page 23: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

An intermediate phase is a mixture that has different structure to that of either component

Range of stability depends on structure and type of bonding (Ionic, metallic, covalent…)

Intermetallic phases are intermediate phase of integer stoichiometry e.g. Ni3Al

Narrow stability range broad stability range

Page 24: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

5. Binary phase diagrams : Ordered phasesHMIX < 0

i.e. A and B attract

Weak attraction Strong attraction

Ordered phase extends to liquid phase

1 phase, solid

Ordered phase

Peak in liquidus line : attraction between atoms

Page 25: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

5. Binary phase diagrams : Simple Eutectic systems

HMIX 0 ; A and B have different crystal structures;

Phase is A with B dissolved (crystal structure A)

Phase is B with A dissolved (crystal structure B)

Single phase

Two phase

Eutectic point

Page 26: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

Example : http://www.soton.ac.uk/~pasr1/index.htm

Eutectic systems and phase diagrams

Page 27: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

5. Binary phase diagrams : Peritectics and incongruent melting

• Sometimes ordered phases are not stable as a liquid. These compounds

have peritectic phase diagrams and display incongruent melting.

• Incongruent melting is when a compound melts and decomposes into its

components and does not form a liquid phase.

• These systems present a particular challenge to material scientists to make in

a single phase. Techniques like hot pouring must be used.

Page 28: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

So

lid so

lutio

n K

(+Na

)

So

lid so

lutio

n

Na

(+K)

(bcc)

(hcp)

(bcc)

Peritectic line (3 phase equil.)

L + KNa2

L + Na(K)

L + K(Na)

K(Na) + KNa2

KNa2 + Na(K)

Page 29: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

5. Binary phase diagrams : Additional equations

A. Equilibrium vacancy concentration

So far we have assumed that every atomic site in the lattice is occupied. But this is not always so. Vacancies can exist in the lattice.

Removing atoms: increase internal energy (broken bonds) and increases configuration entropy (randomness).

Define an equilibrium concentration of vacancies XV (that gives a minimum free energy)

GV=HV TSV

Where HV is the increase in enthalpy per mole of vacancies added and SV is the change in thermal entropy on adding the vacancies (changes in vibrational frequencies etc.).XV is typically 10-4-10-3 at the melting point of the solid.

B. Gibbs-Duhem relationship

This relates the change in chemical potential that results from a change in alloy composition:

Page 30: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

5. Binary phase diagrams : Ternary phase diagrams

These are complicated.

• 3 elements so triangles are at fixed temperature

• Vertical sections as a function of T and P are often given.

Blue – single phaseWhite – two phaseYellow – three phase

Page 31: The thermodynamics of phase transformations Robin Perry School of Physics and Astronomy, Edinburgh Introduction to Computer Simulation of Alloys meeting.

6. Kinetics of phase transformations

So far we have only discussed systems in equilibrium. But we have said nothing of rate of a phase transformation. This is the science of Kinetics.

G is the driving force of the transformation.

Ga is the activation free energy barrier.

Atoms must obtain enough thermal energy to overcome this barrier.

General equation for the rate of the transformation is the Arrhenius rate equation:

i.e. high temperature implies faster rateN.B. some rates are very long e.g. diamond graphite