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“Phase Transformation in Materials”

Eun Soo Park

Office: 33-313

Telephone: 880-7221 Email: espark@snu.ac.kr

Office hours: by an appointment

2018 Fall

09.13.2018

1

(2)

2

Contents for previous class

- Chemical potential and Activity

- Gibbs Free Energy in Binary System - Binary System

Ideal solution

Regular solution

mixture/ solution / compound

G

2

= G

1

+ ΔG

mix

J/mol G

1

= X

A

G

A

+ X

B

G

B

J/mol

(∆H

mix

=0) G

mix

RT ( X

A

ln X

A

X

B

ln X

B

)

mix

AB

    

AB

1   

AA BB

H P where ( )

2

) ln

ln

(

A A B B

B A B

B A

A

G X G X X RT X X X X

X

G      

  

  

A

    G' n

• μ

A

= G

A

+ RTlna

A

(3)

3

Chemical potential

 

A A

dG' dn

The increase of the total free energy of the system by the increase of very small quantity of A, dn

A

, will be proportional to μ

A

.

dn

A

~ small enough

(∵

A

depends on the composition of phase)

(T, P, n

B

: constant )

G = H-TS = E+PV-TS

For A-B binary solution, dG'  

A

dn

A

 

B

dn

B

    

A A

 

B B

dG' SdT VdP dn dn

For variable T and P

1) Ideal solution 1.3 Binary Solutions

A

: partial molar free energy of A or chemical potential of A

  

  A   A T, P, nB

G' n

  

  B   B T, P, nA

G' n

(4)

1) Ideal solution 1.3 Binary Solutions

μ

B

μ

A

X

B

Fig. 1.12 The relationship between the free energy curve and

 

A A

 

B B

G X X

B B

B A

A

A

RT X X G RT X X

G ln ) ( ln )

(   

(5)

5

Contents for today’s class II

- Ideal Solution/ Regular Solution/ Real solution

(6)

Q1: What is “Regular Solution”?

∆G

mix

= ∆H

mix

- T∆S

mix

1.3 Binary Solutions

(7)

Ideal solution : H

mix

= 0

Quasi-chemical model assumes that heat of mixing, H

mix

, is only due to the bond energies between adjacent atoms.

Structure model of a binary solution

Regular Solutions

∆G

mix

= ∆H

mix

- T∆S

mix

1.3 Binary Solutions

Assumption: the volumes of pure A and B are equal and do not change during mixing so that the interatomic distance and bond energies are independent of composition.

This type of behavior is exceptional in practice and usually mixing is endothermic or exothermic.

Fig. 1.13 The different types of interatomic bond in a solid solution.

7

(8)

Q2: How can you estimate

“ΔH mix of regular solution”?

Gibbs Free Energy of Regular Solutions

∆H

mix

= ΩX

A

X

B

where Ω = N

a

(9)

Bond energy Number of bond A-A 

AA

P

AA

B-B 

BB

P

BB

A-B 

AB

P

AB

AA AA   BB BB   AB AB

E P P P

mix

AB

    

AB

1   

AA BB

H P where ( )

2

Internal energy of the solution

Regular Solutions

1.3 Binary Solutions

9

(10)

 H

mix

 0

Completely random arrangement

ideal solution

AB

a A B

a

P N zX X bonds per mole N : Avogadro's number

z : number of bonds per atom

∆H

mix

= ΩX

A

X

B

where Ω = N

a

 H

mix

 P

AB

Regular Solutions

 0

 ( )

2 1

BB AA

AB

 

  

 0 P

AB

  0 P

AB

 0

If Ω >0, 1.3 Binary Solutions

(1) (2)

(3)

Fig. 1.14 The variation of ΔHmixwith composition for a regular solution.

(11)

Q3: How can you estimate

“Molar Free energy for regular solution”?

) ln

ln

(

A A B B

B A B

B A

A

G X G X X RT X X X X

X

G      

G

2

= G

1

+ ΔG

mix

∆H

mix

-T∆S

mix

11

Gibbs Free Energy of Regular Solutions

(12)

Regular Solutions

Reference state

Pure metal G

A0

G

B0

 0

) ln

ln

(

A A B B

B A B

B A

A

G X G X X RT X X X X

X

G      

G

2

= G

1

+ ΔG

mix

∆G

mix

= ∆H

mix

- T∆S

mix

∆H

mix

-T∆S

mix

(13)

Q4: “Correlation between chemical potential and free energy”?

Gibbs Free Energy of Binary Solutions

13

(14)

1

 

A A

 

B B

G X X Jmol

For 1 mole of the solution (T, P: constant ) G = E+PV-TS

G = H-TS

2) regular solution

A B B

A B

A B A B

AX X X X X X X X X

X  (  ) 22

B B

B B

A A

A A

X RT

X G

X RT

X G

ln )

1 (

ln )

1 (

2 2

) ln

ln

(

A A B B

B A B

B A

A

G X G X X RT X X X X

X

G      

) ln

) 1

( (

) ln

) 1

(

(

A A 2 A B B B 2 B

A

G X RT X X G X RT X

X         

  

  

A A A

B B B

G RTln X G RTln X

Correlation between chemical potential and free energy

Ideal solution

복잡해졌네 --;;

Regular solution

(15)

Q5: What is “activity”?

Gibbs Free Energy of Binary Solutions

15

(16)

Activity, a : effective concentration for mass action

ideal solution regular solution

μ

A

= G

A

+ RTlna

A

μ

B

= G

B

+ RTlna

B

  

  

A A A

B B B

G RTln X G RTln X

B B

B B

A A

A

A

G   ( 1  X )

2

RT ln X   G   ( 1  X )

2

RT ln X

  a

B

)

2

1 ( )

ln(

B

B

B

X

RT X

a  

(17)

 1

A A

X 1 a

A A

X a

Degree of non-ideality

17

(18)

- A ttraction + Repulsion

mix

AB

    

AB

1   

AA BB

H P where ( )

2

(19)

Variation of activity with composition (a) a

B

, (b) a

A

a

B

a

A

Line 1 : (a) a

B

=X

B

, (b) a

A

=X

A

Line 2 : (a) a

B

<X

B

, (b) a

A

<X

A

Line 3 : (a) a

B

>X

B

, (b) a

A

>X

A

ideal solution…Rault’s law ΔH

mix

<0

ΔH

mix

>0

B in A

random mixing

A in B

random mixing

19

(20)

Q6: “Chemical equilibrium of multi‐phases”?

Gibbs Free Energy of Binary Solutions

(21)

21

(22)

2

(23)

23

- Chemical potential and Activity

- Gibbs Free Energy in Binary System - Binary System

Ideal solution

Regular solution

mixture/ solution / compound

G

2

= G

1

+ ΔG

mix

J/mol G

1

= X

A

G

A

+ X

B

G

B

J/mol

(∆H

mix

=0) G

mix

RT ( X

A

ln X

A

X

B

ln X

B

)

mix

AB

    

AB

1   

AA BB

H P where ( )

2

) ln

ln

(

A A B B

B A B

B A

A

G X G X X RT X X X X

X

G      

  

  

A

 

A

 

T, P, nB

G' n

• μ

A

= G

A

+ RTlna

A

μ는 조성에 의해 결정되기 때문에 dnA가 매우 작아서 조성변화 없어야

23

(24)

Contents for today’s class II

- Ideal Solution/ Regular Solution/ Real solution

(25)

Q7: What is “Real Solution”?

25

sufficient disorder + lowest internal E

(26)

 > 0, H

mix

> 0

 < 0, H

mix

< 0

Ideal or Regular solution : over simplification of reality

Real solution: sufficient disorder + lowest internal E

Ordered alloys Clustering

Config. Entropy Sk ln w + mixing enthalpy ∆H

mix

= ΩX

A

X

B where Ω = Na

P

AB

 0

Sthermal= 0

Internal E P

AA

, P

BB

∆G

mix

= ∆H

mix

- T∆S

mix

1.3 Binary Solutions

strain effect

Interstitial solution

(27)

* The degree of ordering or clustering will decrease as temp.

increases due to the increasing importance of entropy .

∆G

mix

= ∆H

mix

- T∆S

mix

High temp. Entropy effect Solution stability

27

(28)

2) In systems where there is a size difference between the atom e.g. interstitial solid solutions,

E = ∆H

mix

+ elastic strain

quasi- chemical model ~ underestimate ∆E due to no consideration of elastic strain field

New mathematical models are needed to describe these solutions.

1.3 Binary Solutions

Real solution: sufficient disorder + lowest internal E

(29)

Q8: Ordered phase I:

“Short range order (SRO)” in solution

29

(30)

• Ω < 0 ⇒ contain short-range order (SRO) SRO parameter = s _ degree of ordering

 

AB AB

AB AB

P P (random)

s P (max) P (random)

Ordered phase  < 0, H

mix

< 0

1.3 Binary Solutions

∆Ω = N

a

P

AB

(max) P

AB

(random) P

AB

with SRO

SRO (Short Range Ordering) or LRO (Long Range Ordering)

Fig. 1.19 (a) Random A-B solution with a total of 100 atoms and X =X =0.5, P ~100, S=0.

(31)

5 nm

31

(32)

[2211]Laves (1120) (0132)

(33)

Q9: Ordered phase II:

“Long range order (LRO)”

33

(①superlattice, ②intermediate phase, ③intermetallic compound)

(34)

* Solid solution → ordered phase

 random mixing

 entropy ↑

negative enthalpy ↓

Large composition range

 G ↓

* Compound : AB, A

2

B…

 entropy↓

 covalent, ionic contribution.

 enthalpy more negative ↓

Small composition range

 G ↓

 0

H

mixS

 0

H

mixS

(35)

* The degree of ordering or clustering will decrease as temp.

increases due to the increasing importance of entropy .

∆G

mix

= ∆H

mix

- T∆S

mix

High temp. Entropy effect Solution stability

35

(36)

Q9‐a : Superlattice

(37)

* In solutions with compositions that are close to a simple ratio of A:B atoms another type of order can be found.

* This is known as long-range order (LRO) CuAu, Cu

3

Au and many other intermetallics show LRO.

* A superlattice forms in materials with LRO

Ordered phase  < 0, H

mix

< 0

Cu–Au alloy

High temp.

Disordered Structure

Low temp.

CuAu superlattice Cu

3

Au superlattice 1.3 Binary Solutions

(The atom sites are no longer equivalent but can be labelled as A-sites and B-sites.)

37

(38)

(a)L2

0

:

CuZn/FeCo/NiAl/CoAl/

FeAl/AgMg/AuCd/NiZn

Superlattice formation

: order-disorder transformation

β brass superlattice viewed as two inter-penetrating cubic lattices - ε< 0, H

mix

< 0

- between dissimilar atoms than between similar atoms

- Large electrochemical factor:

tendency for the solute atoms to avoid each other and to associate with the solvent atoms

- Size factor just within the favorable limit:

lead to atomic rearrangement

so as to relieve the lattice distortion imposed by the solute atoms

(39)

Five common ordered lattices

(a)L2

0

:

CuZn/FeCo/NiAl/CoAl/

FeAl/AgMg/AuCd/NiZn

(b) L1

2

:

Cu

3

Au/Ni

3

Mn/Ni

3

Fe/Ni

3

Al/

Pt

3

Fe/Au

3

Cd/Co

3

V/TiZn

3

(c) L1

0

:

CuAu/CoPt/FePt

(d) D0

3

:

Fe

3

Al/Cu

3

Sb/Mg

3

Li/Fe

3

Al/

Fe

3

Si/Fe

3

Be/Cu

3

Al

(e) D0

19

:

Mg

3

Cd/Cd

3

Mg/Ti

3

Al/Ni

3

Sn/Ag

3

In/

Co

3

Mo/Co

3

W/Fe

3

Sn/Ni

3

In/Ti

3

Sn 1.3 Binary Solutions

39

(40)

The entropy of mixing of structure with LRO is extremely small and the degree of order decrease with increasing temperature until above some critical

temperature there is no LRO at all.

This temperature is a maximum when the composition is the ideal required for the superlattice.

• The critical temperature for loss of LRO increases with increasing Ω or ΔHmix,

Ordered phase  < 0, H

mix

< 0

∆G

mix

= H

mix

- T S

mix

S

mix

~small

At high Temp.,

∆G

mix

~ large (-)

Vacancy/another atoms

(41)

< 0, H

mix

< 0 / H

mix

~ -20 kJ/mol

(fcc) (fcc)

(tetragonal) (cubic)

(cubic)

(complete solid solution)

Ordered Phase

41

(42)

Q9‐b : Order‐disorder transition

(43)

- Not classical phase change=~not depend on diffusion process - change of temperature allowed a continuous re-arrangement of

atoms without changing the phase = “2

nd

order transition”

- boundary: ordered lattice & disordered lattice/phase rule could not applied

there are cases in which an ordered phase of one composition exists in equilibrium with a disordered phase of a different composition.

- Simple composition of the type AB or AB

3

can the transformation

(i.e. at the temperature maximum) be considered diffusionless.

Order-disorder phase transformation

43

(44)

 < 0, H

mix

< 0 / H

mix

~ -21 kJ/mol

(fcc) (hcp)

Intermediate Phase

β

β’

Order-disorder transformation:

Low temp. – ordered structure High temp. – disordered structure

(45)

Q9‐c :

Intermediate phase vs Intermetallic compound

45

(46)

* Many intermetallic compounds have stoichiometric composition A

m

B

n

and a characteristic free energy curve as shown in Fig (a).

* In other structure, fluctuations in composition can be tolerated by some atoms occupying ‘wrong’ position or by atom sites being left vacant, and in these cases the curvature of the G curve is much less, Fig (b).

Intermediate Phase

(47)

H

mix

~(-)41 kJ/mol

 < 0, H

mix

< 0

(fcc) (bcc)

(fcc) (triclinic)

(cubic)

47

Intermediate Phase

(orthorhombic)

(48)

(hcp) (fcc) (FCC)

m Fd

3

(Orthorhombic)

Intermediate Phase

 < 0, H

mix

< 0 / H

mix

~ -38 kJ/mol

(49)

49

 << 0, H

mix

<< 0 / H

mix

~ -142 kJ/mol

Intermediate Phase

(50)

1) Relative atomic size

- Laves phase (size difference:

1.1~1.6 ex: MgCu2

) fill space most efficiently ~ stable

- Interstitial compound: MX, M

2

X, MX

2

, M

6

X

2) Relative valency electron

- electron phases ex_α & β brass

# of valency electrons per unit cell

→ depending on compositional change

3) Electronegativity

- very different electronegativites → ionic bond_normal valency compounds

Intermediate Phase

_”different crystal structure as either of the pure component”

MgCu

2

(A Laves phase)

3 main factors

determining the structure of Intermediate phase ?

1.3 Binary Solutions

M= Cubic or HCP ex: Zr, Ti, V, Cr, etc, X= H, B, C, and N

(51)

Metastable vs Stable miscibility gap

51

Q10: “Clustering”? → Phase separation

(52)

* The degree of ordering or clustering will decrease as temp.

increases due to the increasing importance of entropy .

∆G

mix

= ∆H

mix

- T∆S

mix

High temp. Entropy effect Solution stability

(53)

53

> 0, H

mix

> 0 /H

mix

~ +26 kJ/mol

53

(54)

Dendrite / interdendrite formation

0 10 20 30 40 50 60 70 80 90 100 400

600 800 1000 1200 1400 1600 1800

FCC1 + FCC2 FCC

Temperature (

o

C)

Cu

Dendrite Interdendrite

Cooling process in the miscibility gap

(55)

ROI 1, 2 : 1.4 nm x 2 nm x 2 nm ROI 3 : 1.2 nm x 2 nm x 23 nm

(1D concentration profile)

1 at%

Co 26.19 Cr 24.15 Fe 24.59 Ni 19.59 Cu 4.74

Compositional analysis of as-cast CoCrFeNi/Cu HEA (dendrite)

1

2 3

z y

x

2 at%

Co 0.33 Cr 0.46 Fe 0.39 Ni 5.00 Cu 93.56

0 4 8 12 16 20 24

0 20 40 60 80 100

Concentration (at%)

Distance (nm)

Co Cr Fe Ni Cu

Dendrite region: matrix (4.74 at%Cu) + 2nd phase (93.56 at%Cu)

No segregation at the interface between Matrix and 2nd phase

3-1’ at%

Co 25.29 Cr 25.63 Fe 23.63 Ni 20.66 Cu 4.42

3-2’ at%

Co 2.01 Cr 3.35 Fe 2.56 Ni 6.90 Cu 84.92

(56)

 > 0, H

mix

> 0 / H

mix

~ +17 kJ/mol

(57)

57

> 0, H

mix

> 0 / H

mix

~ +5 kJ/mol

57

(58)

>> 0, H

mix

>> 0 /H

mix

~ +60 kJ/mol

(59)

59

L1 + L2 βTi + L

L + αY

>> 0, H

mix

>> 0 /H

mix

~ +58 kJ/mol

59

(60)

Alloy design considering heat of mixing relation among constituent elements

Equilibrium condition μA,aA,d, μB,aB,d

A B

A B

Atomic fraction B

Atomic fraction B

ΔG

T T2 Tc Tl

T = Tl T = T2 a

a b

b c

c d

μA,a d

A,d

μB,a

B,d

2ΔG/∂x2=0

spinodal binodal Two liquids

(or SCLs) One liquid

(or SCL)

C2

C1 C3

ΔHmix ≫0 between A & B

creates (meta)stable miscibility gap in limited composition range

Phase separation to A-rich & B-rich phase

Different two-phase structure

by initial composition before phase separation

Positive heat of mixing relation among constituent elements

(61)

* Ti‐Y‐Al‐Co system

100nm

(Y56Al24Co20)65(Ti56Al24Co20)35

100nm

100nm

(Y56Al24Co20)25(Ti56Al24Co20)75 (Y56Al24Co20)50(Ti56Al24Co20)50

Droplet structure Interconnected structure Droplet structure

0 10 20 30 40 50 60 70 80 90 100

400 600 800 1000 1200 1400 1600

Y56Al24Co20 Ti56Al24Co20

T (K)

Ti

‐38

‐22 +15

‐30

‐28 ‐19

Y Al

Co

(62)

* La‐Zr‐Al‐Cu‐Ni system

(63)

Phase separation in metallic glasses

63

(64)

Interstitial solution

- Binary System

Ideal solution Regular solution

mixture/ solution / compound (∆H

mix

=0)

mix

AB

    

AB

1   

AA BB

H P where ( )

2   0

Real solution

H

mix

> 0 or H

mix

< 0

Random distribution

Ordered structure

 > 0, H

mix

> 0

 < 0, H

mix

< 0

Ordered alloys Clustering P

AB

Internal E P

AA

, P

BB

strain effect

(65)

65

: Solid solution → ordered phase : Compound : AB, A

2

B…

 0

H

mixS

H

mixS

 0

 0

H

mixS

> : Solid solution → solid state H

mixS

>>  0 0 phase separation (

two solid solutions

)

: liquid state phase separation (

up to two liquid solutions

)

metastable miscibility gap

stable miscibility gap

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