materials science manual chapter 7
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Chapter 7. Non-equilibrium solid phase transformations
Chapter 7.NON-EQUILIBRIUM SOLID PHASE TRANSFORMATIONS
7.1 Introduction
The purpose for strengthening metallic materials is to extend the elastic range and raise their yield
and ultimate strength. The underlying mechanism responsible is the generation of more
dislocation while restricting their movement. However, complete pile up of dislocations must be
prevented, because it may result into brittle fracture. Six techniques are recognised to give rise to
strengthening in metallic materials.
(i) Workhardening: Strengthening due to creation of dislocations during cold working, while
distorting the lattice.
(ii) Solid solution hardening: Introduction of substitutional or interstitial solid solute atoms that
result in lattice distortion which restricts dislocation movement, thus strengthening the metal.
(iii) Grain size: Fine grain size raises the grain boundary area hence the dislocation density.
Hence fine grain size is associated with high strength and density.
(iv) Dispersion hardening: When particles of a second phase are dispersed in the matrix of a
metallic phase, they may form a coherent matrix lattice with some degree of lattice distortion.
Such a situation inhibits dislocation movement, thus strengthening the material.
(v) Transformation hardening: The transformation of the crystalline structure during heat
treatment may result into formation of a structure with fewer slip planes and distortions.
Martensitic transformation in steels is an example of such mechanism which results into
considerable hardening of steels.
(vi) Irradiation hardening: X-ray or Gamma radiations can produce vacancies or lattice
defects. However this technique is not commercially applied.
In this chapter, we cover two basic strengthening mechanisms resulting from non-equilibrium
phase transformations in metallic materials, namely precipitation hardening and martensitic
transformations.
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7.2 Dispersion (Precipitation) Hardening
PRECIPITATION is the decomposition of a solid solution into two solid phases of different
composition, the precipitate and the solid solution.
' + (7.1)
PRECIPITATION HARDENING is the process whereby hardening of an alloy is caused by the
precipitation of a constituent from a supersaturated solid solution by heating to some elevated
temperature.
AGE HARDENING is a form of precipitation hardening in which there is a spontaneous increase of
hardness at room temperature with lapse of time, on a supersaturated solid solution.
The phenomena of precipitation hardening can occur ONLY in those alloys in which there is a
decrease of solid solubility with decreasing temperature resulting in formation of a supersaturated
solid solution upon fast cooling of the alloy from above the solvus line. This phenomena occurs in
certain types of aluminium alloys (e.g. Al-Ag, Al-Mg) and in Cu-Be alloys.
The process of precipitation hardening has three important steps as illustrated in Fig. 7.1:
(a) Solution treatment: The alloy is first heated to a temperature above the solvus temperature
and held until a homogeneous solid solution is produced. This step dissolves the
precipitate and reduces any segregation present in the original alloy.
(b) Quench: The solid solution which contains the solid solution only, is then rapidly cooled or
quenched. The atoms do not have enough time to diffuse to potential nucleation sites and
allow the phase to form. After the quench, the structure contains , the supersaturated
solid solution of.
(c) Age: Finally, the supersaturated is heated to a temperature below the solvus
temperature. At this aging temperature the atoms are able to diffuse short distances.
Because the supersaturated solid is unstable, extra solute atoms diffuse to numerous
nucleation sites and a precipitate forms and grows. If we were to hold the alloy for a
sufficient time at the aging temperature, the equilibrium and structure is produced.
The first stage in the precipitation reaction is the formation of nuclei of the precipitating phase,followed by the growth of the nuclei to larger particles. This results into lattice distortion which is
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responsible for the hardening of the alloys. The actual cause of age hardening however, is the
obstruction to the motion of dislocations set up by the fine transition precipitate particles and the
strains produced by the mismatch of the transition products with the matrix.
If an alloy is held for a long period of time at the treatment temperature, coagulation of the
particles is observed and this intermediate phase becomes stable. This phenomena is called
overaging.
Other changes that are observed to accompany precipitation are:
1. Increase in electrical conductivity (except in Al-Cu alloys)
2. Increase in hardness, passing through a max. and then decreasing.
3. Increase in strength with hardness, decrease in ductility.
L
+L600
700
500
400
300
200
0 2 4 6 8
Weight percent Copper
1
2
3
5.65
548
'
''
Quench
Age
Fig 7.1: Steps in the heat treatment of an Al-Cu precipitation hardening alloy
During the aging of Al-Cu alloys, a series of precipitates form before the equilibrium is produced.
At the start of aging, the copper atoms concentrate on {100} planes in the matrix and produce
very thin clusters of copper atoms called GUINIER-PRESTON, or GP-I, zones. As aging
continues, more copper atoms diffuse to the precipitate and the GP-I zones grow into thin disks, or
GP-II zones. Later, the GP-II zones dissolve and , which is similar to the stable , forms.
Finally, dissolves and the stable phase precipitates.
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The non-equilibrium precipitates - GP-I, GP-II and the - are coherent precipitates (Fig. 7.2). The
strength of the alloy increases with aging time as these coherent phases grow in size during the
initial stages of heat treatment. When these coherent precipitates are present, the alloy is in the
aged condition.
Fig. 7.2: A coherent precipitate
Fig. 7.3: A non coherent precipitate phase
When the stable non-coherent phase precipitates, the strength of the alloy decreases. Now the
alloy is in the overaged condition, as illustrated by Fig. 7.3.
Aging at room temperature is called natural aging. Aging at higher temperatures is called artificial
aging, because the alloy is heated to produce precipitation.
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REQUIREMENTS FOR AGE HARDENING
Four conditions must be satisfied:
1 The phase diagram must display decreasing solid solubility with decreasing temperature.
2 The matrix should be relatively soft and ductile and the precipitate should be hard and
brittle.
3 The alloy must be quenchable, rapidly enough to suppress formation of the second phase.
4 The precipitate that forms must be coherent with the matrix structure in order to develop the
maximum strength and hardness.
7.3 Non-equilibrium solid phase transformations of Austenite
7.3.1 Introduction
When steel is quenched rapidly from high temperatures, there is no time for the austenite (-Fe) to
transform to the lamellar structure called pearlite.
Pearlite consists of alternate plates of a-iron (ferrite) and iron carbide (cementite, Fe3C). During
fast cooling, the separate ferrite and cementite particles cannot form.
When the - phase is quenched below a certain temperature called Ms (Martensite starts
temperature), a new phase called martensite begins to form. Martensite has a body centred
tetragonal structure. The c/a ratio is proportional to the carbon content of the steel. On the other
hand, martensite can be regarded as a BCC crystal structure which has been distorted along one
axis as a result of the presence of carbon atoms. The atoms of martensite are less densely
packed than austenite, hence an expansion occurs during the transformation giving rise to
evolution of internal stresses.
The martensitic transformation is diffusionless and usually results in the formation of platelets
which form by a shearing mechanism at velocities above one third the velocity of sound in the
material.
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Below a temperature called Mf(martensite finish temp.) no more austenite is transformed to
martensite. There is usually some retained austenite. Ms and Mfvary with carbon content in
carbon steel, as illustrated in Fig.7.4. The temperature Ms is further affected by the alloy content:
Ms = 561-474 (%C)-33(%Mn) - 17 (%Ni)-17 (%Cr)-21 (%Mo)
Mf is about 215 C below Ms
The structure martensite is very hard and strong. Dislocations move only with great difficulty.
The strength and hardness of martensite increase with carbon content, as shown in Fig. 7.5.
-200
-100
0
100
200
300
400
500
600
0 0.2 0.4 0.6 0.8 1 1.2 1.4
Carbon wt %
Temperature,C
Ms C
Mf C
Fig. 7.4. Effect of carbon content on Ms and Mf Temperatures.
0
10
20
30
40
50
60
70
1 2 3 4 5 6 7 8
Carbon, wt %
Hardness,HRC
50% Martensite
100% Martensite
Fig. 7.5. The effect of carbon content on Martensite hardness
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7.3.2. Decomposition of Austenite
In alloys, the structural changes are preferably documented in equilibrium phase diagrams.Equilibrium means that they have been established for conditions where the properties of thesystem do not change with time and infinitum. In reality, equilibrium conditions are rarelyencountered; i.e. the cooling (or heating) rates are not slow enough to allow the continual phaseadjustments (diffusion) to occur. Under these conditions, data from equilibrium diagrams are nolonger directly applicable but serve only as an estimate.
Under equilibrium conditions, austenite, a solid solution of carbon in iron, is decomposed topearlite after precipitating ferrite in hypo-eutectoid steels, or cementite in hyper-eutectoid steels, asshown in Fig. 7.6.
0.035 0.8
723 C
910 C
Carbon, wt %
Austenite
()
Pearlite + Ferrite -Fe
+
P
Pearlite + Fe 3C
+ Fe 3C
P
Fe 3C
Fig. 7.6. The steel part of the iron carbon phase diagram
Mechanism of Pearlite Formation
The pearlite transformation of supercooled austenite is a diffusion mechanism. Austenitedecomposes with the formation of ferrite (almost pure iron) and cementite containing 6.67 %
carbon. The carbide appears first as its nuclei are formed at the boundaries of the austenitegrains. (Fig. 7.7). As a result, the adjacent volumes of austenite Are depleted of carbon, becomeless stable, and undergo the allotropic transformation from austenite to ferrite. Thus small crystalsof ferrite are formed adjacent to the cementite (iron carbide). Subsequent diffusion leads toformation of more platelets of iron carbide with simultaneous formation of ferrite plates, to form amixture or colony, called pearlite. The structure of pearlite is characteristically lamellar. Thegreater the degree of supercooling, the finer the ferrite-cementite structure obtained.
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Fe 3C
Grain
Boundary
(a) (b)(c)
Fig. 7.7. Development of pearlite structure
Transient coolingThe effect of cooling rate on the decomposition of Austenite in a eutectoid steel is illustrated in Fig.7.8.
Cooling rate, v
Lower c riticalcooling rate
Upper criticacooling rate
A+T
Arz
M s
M f
F
+
Fe 3C
A r1 Beginning of decompositionA to F+Fe3C (Pearlite)
End of decomposition to P
T+M+A M+ A ret
M
Fig. 7.8. Effect of cooling rate on the transformation of austenite
As we increase the cooling rate, the temperature at which the austenite transforms to Pearlite islowered. The higher the cooling rate, the lower the decomposition temperature, the moredispersed (finer) the ferrite - cementite structure obtained. At higher cooling rates, the pearliteoccurs as a very fine structure often called Sorbite or Troostite (T) . At some high cooling rates,below the temperature Arz, a new modified structure called Bainite occurs. Bainite consists of
ferrite with finely dispersed cementite globules. When the cooling rate exceeds a critical coolingrate, at a lower temperature, Ms, martensite begins to form. This transformation continues until a
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temperature Mfis reached. Any untransformed austenite remains in the structure as retained
austenite (Aret).
7.3.3. Kinetics of Martensitic Transformation
Baines and Davenproof studied the isothermal decomposition of austenite. Small specimen wereheated above the upper critical temperature, Ac3, to form austenite. Subsequently they werequenched in a suitable bath at a certain temperature. After holding at that temperature for differentperiods of time, the specimen were withdrawn and quenched in water. By so doing, themicrostructure transformed so far is kept and the remaining austenite is converted to martensite.From the microsection, the amount of transformed austenite can be assessed. If the procedure isexecuted for different halting temperatures a series of s-shaped curves is obtained. These canthen be summarized on a Time-Temperature-Transformation (TTT) diagram.
1 2 3 4
100
80
60
40
20
0
Holding Time (s)
Thalt
time
Temp
Thalt
A31
to P at GB
2
3
4
100% Pearlite
P
Fig. 7.9. Isothermal transformation of austenite
Fig. 7.9 shows how the S-curve is produced, and Fig. 7.10 shows how the TTT diagram isproduced.
Three ranges are distinct on the TTT diagram:
(a) PEARLITIC: Down to temperatures of about 550 C, pearlite is formed. At highertemperatures the pearlite is coarse, and at lower temperatures it is fine.
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(b) BAINITE: Between 550 and 350 C, Bainite is formed. Bainite consists of cementite, finelydispersed particles in ferrite. It is hard but reasonably ductile. Upper Bainite is coarse, andits microstructure can be resolved in an optical microscope. Lower Bainite is very fine, andcan only be resolved by an electron microscope.
(c) MARTENSITE: This range exists at temperatures below Ms. The formation of martensite isdiffusionless and is therefore independent of time.
100
50
0
800
700
600
500
400
300
200
100
0
-100
Thalt(C)
650 500 350
A3
A1
Coarse
Fine
PEARLITE
Coarse
Fine
PEARLITE
M
Fig. 7.10. Development of the TTT diagram from the isothermal transformation of Austenite.
7.3.4 TTT Diagrams for Continuous Cooling
In the foregoing section, the kinetics of austenite transformation were established for the case ofisothermal cooling. A more realistic approach is achieved by studying the behaviour while coolingcontinuously.
Consider the TTT diagram shown in Fig. 7.11, showing various cooling curves super - posed onthe diagram.
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800
700
600
500
400
300
200
100 I II IIIIV
Log (time)
A3
A1
B
P
1
2
3
4
5
5
Transformations
1. Ferrite starts
2. Ferrite ends, Pearlite starts
3. Pearlite ends
4. Bainite starts5. Bainite ends
Composition of microstructure
I : Pure Martens ite
II: Fine pearlite, coarse bainite
III: Ferrite, Fine pear lite, Bainite
IV: Ferrite, Pearlite
Fig. 7.11: TTT diagram of a carbon steel for continuous cooling (CCT)
Alloying of steels alters the form and shape of the TTT diagram.
7.3.5 Hardenability Curves
CCT and TTT diagrams are not available for all steels, and it is not easy to accurately determine
the cooling rates. Instead, a JOMINY TEST is used to cmpare the hardenability of steels. A bar100 mm long and 25 mm in diameter is austenitized, placed in afixture , and sprayed at one endwith water. This procedure produces a wide range of cooling curves - very fast at the quenchedend, and almost air cooling at the opposite end. Fig. 7.12 illustrates the set up of the Jominy test.
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Support
Water
splash Hardness
50 HRC
Hardenability
index
Fig. 7.12 The Jominy Test
After the quenching, hardness measurements are made along the length of the specimen andplotted as shown to produce a hardenability curve. The distance from the quenched end whichgives a minimum hardness of 50 HRC is called the hardenability index. This represents theregion that full underwent martensitic transformation. The hardenability index therefore representsthe depth to which a particular steel can be hardened, and increases accordingly with alloyadditions. Refer to notes in the Practical handbook.
7.3.6. Tempering of Martensite
Martensite is extremely brittle, and its transformation give rise to high internal stresses which maycause cracking. A subsequent heat treatment, called tempering, may relieve the stresses and/oralter the microstructure to produce a better material. For stages of martensite tempering aredistinguished:
80-150 C The specimen contracts, C atoms can move to a certain extent and the tetragonaldistortion is reduced. Slowly the so called cubic martensite is formed. Fine
carbide precipitates are precipitated (-carbide).
150-290 C Specimen expands (0-1) % elongation, the tetragonal lattice is transformed to thecubic lattice, fine carbides are precipitated, retained austenite transformed intocubic martensite.
290-400 C Specimen contracts again, all carbon is precipitated
Above 400
Carbide coagulate, globules can be seen in an optical microscope.
TABLE 7.1 EFFECT OF TEMPERING TEMPERATURE ON THE HARDNESS OF A CARBONSTEEL, C=1.3%
Tempering Temp.(C)
20 100 200 300 400 500 600 700
HRC 63 63 59 55 48 41 34 25
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TABLE 7.2 EFFECT OF TEMPERING TEMPERATURE ON THE MECHANICAL PROPERTIESOF A CARBON STEEL, C= 0.45 %
TemperingTemp. (C)
HardnessHBN
Tensilestrength(MPa)
Yield strength(MPa)
Elongation (%) Reduction inArea(%)
300 320 1050 750 10 30400 285 1000 700 15 40
500 250 900 620 20 50
600 220 800 520 25 55
700 200 700 430 30 60
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