1

L22:L22:Grain Boundary, Grain Boundary,

Surface Energies, Surface Energies, MeasurementMeasurement

27-750, Spring 2006A.D. RollettCarnegie

Mellon

MRSEC

2

Interfacial Energies

• Practical Applications: Rain-X for windshields. Alters the water/glass:glass/vapor ratio so that the contact angle is increased.

“streaky” “clear”

3

Impact on Materials

• Surface grooving where grain boundaries intersect free surfaces leads to surface roughness, possibly break-up of thin films.

• Excess free energy of interfaces (virtually all circumstances) implies a driving force for reduction in total surface area, e.g. grain growth (but not recrystallization).

• Interfacial Excess Free Energy:=

4

Herring Equations

• We can demonstrate the effect of interfacial energies at the (triple) junctions of boundaries.

• Equal g.b. energies on 3 g.b.s:

120°

1

2 3

1=2=3

5 Definition of Dihedral Angle

• Dihedral angle, := angle between the tangents to an adjacent pair of boundaries (unsigned). In a triple junction, the dihedral angle is assigned to the opposing boundary.

120°

1

2 3

1=2=3

1 : dihedralangle for g.b.1

6

Isotropic Material

• An material with uniform grain boundary energy should have dihedral angles equal to 120°.

• Likely in real materials? No! Low angle boundaries (crystalline materials) always have a dislocation structure and therefore a monotonic increase in energy with misorientation angle (Read-Shockley model).

7

Unequal energies

• If the interfacial energies are not equal, then the dihedral angles change. A low g.b. energy on boundary 1 increases the corresponding dihedral angle.

1>120°

1

2 3

1<2=3

8 Unequal Energies, contd.

• A high g.b. energy on boundary 1 decreases the corresponding dihedral angle.

• Note that the dihedral angles depend on all the energies.

1< 120°

1

2 3

1>2=3

9

Wetting

• For a large enough ratio, wetting can occur, i.e. replacement of one boundary by the other two at the TJ.

1< 120°

1

2 3

1>2=3

Balance vertical forces 1 = 22cos(1/2)

Wetting 1 2 2

3cos

1

2cos

10

Experimental

Methods for g.b. energy

measurementG. Gottstein &

L. Shvindlerman, Grain Boundary Migration in Metals, CRC (1999)

11 Triple Junction Quantities

3

χ1χ

b 1^

b2^

b3^

2

n^ 1

n 2^

n3^

gA

gB

gC

φ2

12 Triple Junction Quantities

• Grain boundary tangent (at a TJ): b• Grain boundary normal (at a TJ): n• Grain boundary inclination, measured anti-clockwise with respect to a(n arbitrarily chosen) reference direction (at a TJ):

• Grain boundary dihedral angle: • Grain orientation:g

13 Force Balance Equations/ Herring

Equations• The Herring equations[(1951). Surface tension as a motivation for sintering. The Physics of Powder Metallurgy. New York, McGraw-Hill Book Co.: 143-179] are force balance equations at a TJ. They rely on a local equilibrium in terms of free energy.

• A virtual displacement, r, of the TJ (L in the figure) results in no change in free energy.

14 Derivation of Herring Equs.

1

2

3

L

r

A virtual displacement, r, of the TJ results in no change in free energy.

15

Force Balance

• Consider only interfacial energy: vector sum of the forces must be zero to satisfy equilibrium.

• These equations can be rearranged to give the Young equations (sine law):

γ1b1 +γ2b2 +γ3b3 =r 0

γ1

sinχ1

=γ2

sinχ2

=γ3

sinχ3

16

Inclination Dependence

• Interfacial energy can depend on inclination, i.e. which crystallographic plane is involved.

• Example? The coherent twin boundary is obviously low energy as compared to the incoherent twin boundary (e.g. Cu, Ag). The misorientation (60° about <111>) is the same, so inclination is the only difference.

17 Twin: coherent vs. incoherent

• Porter & Easterling fig. 3.12/p123

18

The torque term

1

2

3

L

r

d

Change in inclination causes a change in its energy,tending to twist it (either back or forwards)

ˆ n 1

19 Inclination Dependence, contd.

• For local equilibrium at a TJ, what matters is the rate of change of energy with inclination, i.e. the torque on the boundary.

• Recall that the virtual displacement twists each boundary, i.e. changes its inclination.

• Re-express the force balance as (:

j

ˆ

b j{

j = 1

3

∑ + ∂σj

∂φj

( ) ˆ n j }

=

r

0

torque termssurfacetensionterms

20

Herring’s Relations

C. Herring in The Physics of Powder Metallurgy. (McGraw Hill, New York, 1951) pp. 143-79

Θi

∂ γi

∂ϑ

ˆ l

gb ˆ t 3

s ˆ t

s ˆ t

ˆ n 3

ˆ n

ˆ n

iˆ t i + = 0ˆ n i∂i∂θ

21

Torque effects

• The effect of inclination seems esoteric: should one be concerned about it?

• Yes! Twin boundaries are only one example where inclination has an obvious effect. Other types of grain boundary (to be explored later) also have low energies at unique misorientations.

• Torque effects can result in inequalities* instead of equalities for dihedral angles.

* B.L. Adams, et al. (1999). “Extracting Grain Boundary and Surface Energy from Measurement of Triple Junction Geometry.” Interface Science 7: 321-337.

22 Aluminum foil, cross section

• Torque term literally twists the boundary away from being perpendicular to the surface

θL

θS

surface

23

Why Triple Junctions?

• For isotropic g.b. energy, 4-fold junctions split into two 3-fold junctions with a reduction in free energy:

90° 120°

24

The “n-6 Rule”

• The “n-6 rule” is the rule previously shown pictorially that predicts the growth or shrinkage of grains (in 2D only) based solely on their number of sides/edges. For n>6, grain grows; for n<6, grain shrinks.

• Originally derived for gas bubbles by von Neumann (1948) and written up as a discussion on a paper by Cyril Stanley Smith (W.W. Mullins’ advisor).

25 Curvature and Sides on a Grain

• Shrinkage/growth depends on which way the grain boundaries migrate, which in turn depends on their curvature.

• velocity = mobility * driving force;driving force = g.b. stiffness *

curvaturev = Mf = M ( ”)

• We can integrate the curvature around the perimeter of a grain in order to obtain the net change in area of the grain.

26 Integrating inclination angle to

obtain curvature• Curvature = rate of change of tangent with arc length, s:

= d/ds• Integrate around the perimeter (isolated grain with no triple junctions), k= M :dA

dt=−k dφ =−2πk∫

27 Effect of TJs on curvature

• Each TJ in effect subtracts a finite angle from the total turning angle to complete the perimeter of a grain:

1

2

3

3

28

Isotropic Case

• In the isotropic case, the turning angle (change in inclination angle) is 60°.

• For the average grain with <n>=6, the sum of the turning angles = 6n =360°.

• Therefore all the change in direction of the perimeter of an n=6 grain is accommodated by the dihedral angles at the TJs, which means no change in area.

29

Isotropy, n<6, n>6• If the number of TJs is less than 6, then not all the change in angle is accommodated by the TJs and the g.b.s linking the TJs must be curved such that their centers of curvature lie inside the grain, i.e. shrinkage

• If n>6, converse occurs and centers of curvature lie outside the grain, i.e. growth.

• Final result: dA/dt = πk/6(n-6)• Known as the von Neumann-Mullins Law.

30

Test of the n-6 Rule• Grain growth

experiments in a thin film of 2D polycrystalline succinonitrile (bcc organic, much used for solidification studies) were analyzed by Palmer et al.

• Averaging the rate of change of area in each size class produced an excellent fit to the (n-6) rule.

• Scripta metall. 30, 633-637 (1994). Note the scatter in

dA/dt within each size class

31

Grain Growth• One interesting feature of grain growth is that, in a given

material subjected to annealing at the same temperature, the only difference between the various microstructures is the average grain size. Or, expressed another way, the microstructures (limited to the description of the boundary network) are self-similar and cannot be distinguished from one another unless the magnification is known. This characteristic of grain growth has been shown by Mullins (1986) to be related to the kinetics of grain growth. The kinetics of grain growth can be deduced in a very simple manner based on the available driving force.

• Curvature is present in essentially all grain boundary networks and statistical self-similarity in structure is observed both in experiment and simulation. This latter observation is extremely useful because it permits an assumption to be made that the average curvature in a network is inversely proportional to the grain size. In other words, provided that self-similarity and isotropy hold, the driving force for grain boundary migration is inversely proportional to grain size.

32

Grain Growth Kinetics• The rate of change of the mean size, d<r>/dt, must be

related to the migration rate of boundaries in the system. Thus we have a mechanism for grain coarsening (grain growth) and a quantitative relationship to a single measure of the microstructure. This allows us to write the following equations.

v = M / r = d<r>/dtOne can then integrate and obtain

<r>2 - <rt=0>2= M t

• In this, the constant is geometrical factor of order unity (to be discussed later). In Hillert’s theory, = 0.25. From simulations, ~ 0.40.

33 Experimental grain growth data

• Data from Grey & Higgins (1973) for zone-refined Pb with Sn additions, showing deviations from the ideal grain growth law (n<0.5).

• In general, the grain growth exponent (in terms of radius) is often appreciably less than the theoretical value of 0.5

34

Grain Growth Theory• The main objective in grain growth theory is to be able to describe both the coarsening rate and the grain size distribution with (mathematical) functions.

• What is the answer? Unfortunately only a partial answer exists and it is not obvious that a unique answer is available, especially if realistic (anisotropic) boundary properties are included.

• Hillert (1965) adapted particle coarsening theory by Lifshitz-Slyozov and Wagner [Scripta metall. 13, 227-238].

35 Hillert Normal Grain Growth Theory

• Coarsening rate:<r>2 - <rt=0>2 = 0.25 k t = 0.25 M t

• Grain size distribution (2D), f:

Here, = r/<r>.

€

f ρ( ) =23 e2ρ

2− ρ( )4 exp

−4

2− ρ

⎧ ⎨ ⎩

⎫ ⎬ ⎭

36 Grain Size Distributions• (a) Comparison of

theoretical distributions due to Hillert (dotted line), Louat (dashed) and the log-normal (solid) distribution. The histogram is taken from the 2D computer simulations of Anderson, Srolovitz et al. (b) Histogram showing the same computer simulation results compared with experimental distributions for Al (solid line) by Beck and MgO (dashed) by Aboav and Langdon.

37 Development of Hillert Theory

• Where does the solution come from?• The most basic aspect of any particle coarsening theory is that it must satisfy the continuity requirement, which simply says that the (time) rate of change of the number of particles of a given size is the difference between the numbers leaving and entering that size class.

• The number entering is the number fraction (density), f, in the class below times the rate of increase, v. Similarly for the size class above.

∂f/∂t = ∂/∂r(fv)

38 Grain Growth Theory (1)

• Expanding the continuity requirement gives the following:

• Assuming that a time-invariant (quasi-stationary) solution is possible, and transforming the equation into terms of the relative size, :

• Clearly, all that is needed is an equation for the distribution, f, and the velocity of grains, v.

€

∂f

∂t=

∂

∂rfv( ) = f

∂v

∂r+ v

∂f

∂r

€

4 f ρ( ) + ρ∂f ρ( )

∂t−

∂

∂ρv ρ( ) f ρ( )( ) = 0

39 Grain Growth Theory (2)

• General theories also must satisfy volume conservation:

• In this case, the assumption of self-similarity allows us to assume a solution for the distribution function in terms of only (and not time).

€

r 3 f 0dr = constant0

∞

∫

40 Grain Growth Theory (3)

• A critical part of the Hillert theory is the link between the n-6 rule and the assumed relationship between the rate of change, v=dr/dt.

• N-6 rule: dr/dt = Mπ/3r)(n-6)• Hillert: dr/dt = M /2{1/<r>-1/r}

= M /2<r> { - 1}• Note that Hillert’s (critical) assumption means that there is a linear relationship between size and the number of sides:

n = 6{1 +0.5 (r/<r> - 1)} =3 {1 + }

41 Anisotropic grain boundary energy

• If the energies are not isotropic, the dihedral angles vary with the nature of the g.b.s making up each TJ.

• Changes in dihedral angle affect the turning angle.

• See: Rollett and Mullins (1996). “On the growth of abnormal grains.” Scripta metall. et mater. 36(9): 975-980. An explanation of this theory is given in the second section of this set of slides.

42

v = Mf, revisited

• If the g.b. energy is inclination dependent, then equation is modified: g.b. energy term includes the second derivative. Derivative evaluated along directions of principal curvature.

r v = ˆ n imi(γi +γi φ1φ1

)κ i1 +(γi +γi φ2φ2)κ i2

• Care required: curvatures have sign; sign ofvelocity depends on convention for normal.

43

Sign of Curvature

(a) singly curved; (b) zero curvature, zero force; (c) equal principal curvatures, opposite signs, zero (net) force.

Porter & Easterling, fig. 3.20, p130

44 Example of importance of interface stiffness• The Monte Carlo model is commonly used for simulating grain growth and recrystallization.

• It is based on a discrete lattice of points in which a boundary is the dividing line between points of differing orientation. In effect, boundary energy is a broken bond model.

• This means that certain orientations (inclinations) of boundaries will have low energies because fewer broken bonds per unit length are needed.

• This has been analyzed by Karma, Srolovitz and others.

45

Broken bond model, 2D

• We can estimate the boundary energy by counting the lengths of steps and ledges.

θsin LN =

θcos LM =

[10]

|)sin||cos(|)( θθ +=+= JNMLJBC

0

0.5

1

1.5

0

30

60

90

120

210

240

270

300

330

Energy,

46Interface stiffness

• At the singular point, the second derivative goes strongly positive, thereby compensating for the low density of defects at that orientation that otherwise controls the mobility!

-0.02

-0.015

-0.01

-0.005

0

0.005

0.01

0.015

0.02

-0.001

0

0.001

0.002

0.003

0.004

0.005

0 50 100 150 200 250 300 350

d/dθ

d/dθ

<0>Angle from

47How to Measure Dihedral Angles and Curvatures: 2D

microstructuresImage Processing

(1)

(2) Fit conic sections to each grain boundary:Q(x,y)=Ax2+ Bxy+ Cy2+ Dx+ Ey+F = 0

Assume a quadratic curve is adequate to describe the shape of a grain boundary.

48

(3) Calculate the tangent angle and curvature at a triple junction from the fitted conic function, Q(x,y):Q(x,y)=Ax2+

Bxy+ Cy2+ Dx+ Ey+F=0

′ y =dydx

=−(2Ax+By +D)Bx+2Cy+E

′ ′ y =d2ydx2 =

−(2A+2B ′ y +2C ′ y 2 )2Cy +Bx +E

κ =′ ′ y

(1+ ′ y 2 )32

; θtan=tan−1 ′ y

Measuring Dihedral Angles and Curvatures

49 Application to G.B. Properties

• In principle, one can measure many different triple junctions to characterize crystallography, dihedral angles and curvature.

• From these measurements one can extract the relative properties of the grain boundaries.

50

Energy Extraction

D. Kinderlehrer, et al. , Proc. of the Twelfth International Conference on Textures of Materials, Montréal, Canada, (1999) 1643.

(sin2) 1 - (sin1) 2 = 0

(sin3) 2 - (sin2) 3 = 0

sin2 -sin1 0 0 …0

0 sin3 -sin2 0 ...0 * * 0 0 ...0

0 0 * * 0

1

2

3

n

= 0Measurements atmany TJs; bin thedihedral angles by g.b. type; average the sineach TJ gives a pair of equations

51

Mobility Extraction

(11sin1)m1 + (22sin2)m2 + (33sin3)m3 = 0

11sin1 22sin2 33sin3 0 0 …0

0 * * * 0 ...0

* 0 * * 0 ...0

0 0 * * * 0

m1

m2

m3

mn

= 0

52

Summary (1)• Force balance at triple junctions leads to the Herring equations. These include both surface tension and torque terms.

• If the interfacial energy does not depend on inclination, the torque terms are zero and Herring equations reduce to the Young equations, also known as the sine law.

• In 2D, the curvature of a grain boundary can be integrated to obtain the ‘n-6’ rule that predicts the growth (shrinkage) of a grain.

• Normal grain growth is associated with self-similarity of the evolving structures which in turn requires the area to be linear in time.

• Hillert extended particle coarsening theory to predict a stable grain size distribution and coarsening rate.

53 Extensions of Herring Equations and Grain

Growth Theory• The next two sections explain the use of the capillarity vector and an extension of grain growth theory to the situation of anisotropic grain boundary properties.

54

Capillarity Vector

• The capillarity vector is a convenient quantity to use in force balances at junctions of surfaces.

• It is derived from the variation in (excess free) energy of a surface.

• In effect, the capillarity vector combines both the surface tension (so-called) and the torque terms into a single quantity

55

Equilibrium at TJ

• The utility of the capillarity vector, can be illustrated by re-writing Herring’s equations as follows, where l123 is the triple line (tangent) vector.

(1 + 2 + 3) x l123 = 0

• Note that the cross product with the TJ tangent implies resolution of forces perpendicular to the TJ.

56 Capillarity vector definition

• Following Hoffman & Cahn [1972, “A vector thermodynamics for anisotropic surfaces. I. Fundamentals and application to plane surface junctions.” Surface Science 31: 368-388.], define a unit surface normal vector to the surface, , and a scalar field, r( ), where r is a radius from the origin. Typically, the normal is defined w.r.t. crystal axes.

ˆ n ˆ n

57

• Definition: grad(r)• From which, d(r) = grad(r)• dr (1)• Giving, d(r) = •(rd + dr)

• Compare with the rule for products: d(r) =rd dr

gives: • = and, •d = d 3

• Combining total derivative of (2) and (3):

d d = d + d •d 0 = • d

ˆ n ˆ n

ˆ n ˆ n

ˆ n ˆ n ˆ n ˆ n

58

• The physical consequence of Eq (2) is that the component of that is normal to the associated surface, n, is equal to the surface energy, .

n =

• Can also define a tangential component of the vector, t, that is parallel to the surface:

t = - = (∂∂θmaxwhere the tangent vector is associated with the maximum rate of change of energy.

ˆ n

ˆ n ˆ t 0

59 Young Equns, with Torques

• Contrast the capillarity vector expression with the expanded Young eqns.:

γ1

1−ε2 −ε3( )sinχ1 + ε3 −ε2( )cosχ1

=

γ2

1−ε1 −ε3( )sinχ2 + ε1 −ε3( )cosχ2

=

γ3

1−ε1 −ε2( )sinχ1 + ε2 −ε1( )cosχ3

εi =1γi

∂γ i

∂φi

60 Expanded Young Equations

• Project the force balance along each grain boundary normal in turn, so as to eliminate one tangent term at a time:σ j

ˆ b j +∂σ∂φ

⎛

⎝ ⎜ ⎜

⎞

⎠ ⎟ ⎟

j

ˆ n j

⎧ ⎨ ⎪

⎩ ⎪

⎫ ⎬ ⎪

⎭ ⎪ ⋅n1=0, εi =

1σi

∂σ∂φ

⎛

⎝ ⎜ ⎜

⎞

⎠ ⎟ ⎟ ij=1

3

∑

σ1ε1+σ2sinχ3+σ2ε2cosχ3 −σ3sinχ2 +σ3ε3cosχ2

σ1ε1σ2sinχ3/σ2sinχ3 +σ2sinχ3+σ2ε2cosχ3=σ3sinχ2+σ3ε3cosχ2

1+σ1ε1/σ2sinχ3( )σ2sinχ3+σ2ε2cosχ3=σ3 sinχ2 +ε3cosχ2( )

1+σ1ε1/σ2sinχ3( )sinχ3+ε2cosχ3{ }σ2 =σ3 sinχ2 +ε3cosχ2( )

61

Summary

• The capillarity vector allows the force balance at a triple junction to be expressed more compactly and elegantly.

• It is important to remember that the Herring equations become inequalities if the inclination dependence (torque terms) are too strong.