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    Fundamentals of Weld SolidificationJohn N. DuPont, Lehigh University

    MICROSTRUCTURAL EVOLUTION dur-ing solidification of the fusion zone representsone of the most important considerations forcontrolling the properties of welds. A widerange of microstructural features can form inthe fusion zone, depending on the alloy compo-sition, welding parameters, and resultant solidi-fication conditions. The primary objective ofthis article is to review and apply fundamentalsolidification concepts for understanding micro-structural evolution in fusion welds.

    Microstructural Features in FusionWelds

    Figures 1 through 3 schematically demon-strate the important microstructural featuresthat must be considered during solidificationin fusion welds (Ref 1, 2). On a macroscopicscale, fusion welds can adopt a range of grainmorphologies similar to castings (Fig. 1), inwhich columnar and equiaxed grains can poten-

    tially form during solidification. The final grainstructure depends primarily on alloy composi-tion and the heat-source travel speed. Althoughsome of the concepts applicable to grain struc-ture formation in castings apply to welds, thereare also some unique differences. While thecolumnar and equiaxed zones can form inwelds, the fine-grained chill zone at the moldwall represented by the fusion line is rarelyobserved in welds. Fundamental concepts asso-ciated with nucleation are needed to understandthese differences. In addition, the solid/liquidinterface in welds is typically curved and itsrate of movement is controlled by the heat-source travel speed, which leads to differencesin formation of the columnar zone within

    welds. These differences can be understoodthough application of competitive grain growthprocesses that occur during solidification.

    On a microscopic scale, there can also be awide range of substructural morphologieswithin the grains (Fig. 2), including planar(i.e., no substructure), cellular, columnar den-dritic, and equiaxed dendritic. The type and rel-ative extent of each substructural region isgoverned by the process of constitutionalsupercooling in which the liquid becomes

    cooled below its liquidus temperature due tocompositional gradients in the liquid. Theextent of constitutional supercooling in theweld is determined by the alloy composition,welding parameters, and resultant solidificationparameters. Lastly, the distribution of alloyingelements and relative phase fractions withinthe substructure (Fig. 3) are also importantmicrostructural features that strongly affectweld-metal properties. The particular exampleshown in Fig. 3 represents a case in whichextensive residual microsegregation of alloyingelements exists across a cellular substructureafter nonequilibrium solidification. This micro-segregation, in turn, produces a relatively highfraction of intercellular eutectic and associatedsecondary phase. The microsegregation behav-ior and concomitant amount of secondary phasethat forms can each be understood with soluteredistribution concepts. Lastly, dendrite tipundercooling can become important athigh solidification rates associated with high-energy-density welding processes. Tip under-

    cooling can lead to significant changes in theprimary solidification mode, distribution of sol-ute within the solid, and final phase fractionbalance. Rapid solidification concepts areneeded to understand these phenomena. Allof these fundamental solidification concepts(nucleation, competitive grain growth, constitu-tional supercooling, solute redistribution, and

    Fig. 1 Types of grain morphologies that can form infusion welds

    Fig. 2 Types of substructure morphologies that can form within the grains of fusion welds

    ASM Handbook, Volume 6A, Welding Fundamentals and Processes

    T. Lienert, T. Siewert, S. Babu, and V. Acoff, editors

    Copyright# 2011 ASM InternationalW

    All rights reserved

    www.asminternational.org

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    rapid solidification) depend on the solidificationparameters during welding. Thus, the importantsolidification parameters are briefly described,followed by detailed discussions and applica-tion of fundamental solidification concepts forunderstanding microstructural evolution.

    Solidification Parameters

    The temperature gradient (G), solid/liquidinterface growth rate (R), and cooling rate (e)are the important solidification parameters.These three parameters are related by:

    e GR (Eq 1)

    This simple relation is not always intuitive andcan be understood more clearly with the helpof Fig. 4. This figure shows a fixed temperaturegradient moving from right to left at a rate R sothat t1 > t2. At a fixed position x*, the temper-ature is reduced from T1 to T2 within the timet1 t2. In other words, the time it takes for a

    temperature reduction (i.e., the cooling rate) isgoverned by the rate of movement (R) of thetemperature gradient (G) through space.

    The solidification parameters are not con-trolled directly in fusion welding but are gov-erned by the welding parameters. As explainedin more detail subsequently, the growth rate isdetermined largely by the speed of the heatsource and shape of the weld pool. The coolingrate and temperature gradient are controlled pri-marily by the heat input (HI), which is defined as:

    HIZP

    S(Eq 2)

    where Z is the heat-source transfer efficiency, Pis the heat-source power, and S is the heat-source travel speed. The heat input representsthe amount of energy delivered per unit lengthof weld. It should be noted that e, G, and R can-not be represented by single values duringsolidification. Due to the complex nature ofheat flow in the weld pool, the spatial distribu-

    tion of temperature is not linear. Similarly, thevalue of R typically varies throughout the weldpool due to the change in growth directionsbetween the solid/liquid interface and heatsource. As a result, the values of e, G, and Rare functions of position and time. In general,the temperature gradient and cooling rate eachdecrease with increasing heat input. Detailedheat-flow equations can be used to quantifythe influence of welding parameters on solidifi-cation parameters. Heat flow in welding is dis-cussed in more detail in other articles in thisVolume (see, for example, the article FactorsInfluencing Heat Flow in Fusion Welding).

    Nucleation Considerations in FusionWelding

    Although the microstructures of castings andwelds share some similarities, there are alsosome significant differences. For example, asshown schematically in Fig. 5 (Ref 3), castingstypically exhibit a chill zone that consists offine equiaxed grains which form near the moldwall. This zone forms as a result of nucleationat the mold/casting interface. This region is typ-ically followed by a columnar zone and anotherequiaxed zone near the center of the casting.The columnar grain region and the centralequiaxed grain zones can also form in fusion

    welds. However, the equiaxed grains associatedwith the chill zone generally do not form infusion welds. The differences in these featurescan be understood with the application of

    nucleation theory, which is covered in thissection.

    Nucleation Theory

    Figure 6 compares examples of homoge-neous nucleation in a liquid (Fig. 6a, b) and het-erogeneous nucleation on a preexisting moldwall (Fig. 6c, d). The change in free energyassociated with homogeneous nucleation(Ghom) is given by (Ref 4):

    Ghom VsGv ASLgSL (Eq 3)

    where Vs is the volume of the nuclei, Gv is thevolume free-energy change associated withnucleation, ASL is the solid/liquid interfacialarea, and gSL is the solid/liquid interfacialenergy. The volume free energy is the drivingforce for solidification and is shown schemati-cally in Fig. 7(a), which shows the variationin volume free energy for the solid and liquidas a function of temperature. Note that Gv =0 at the melting point, so there is no drivingforce for solidification at T = Tm. Thus, under-cooling is generally required to drive the nucle-ation process. The interfacial energy is apositive contribution to the overall free-energychange and therefore works to oppose forma-tion of the nucleus. The change in volume freeenergy with undercooling (T) is given by:

    Gv LT

    Tm(Eq 4)

    where L is the latent heat of fusion. A sphericalnucleus is favored over other shapes becauseit provides the minimum surface area/volume ratio, thus providing the largest pos-sible reduction in Ghom by maximizingthe negative VsGv term and minimizingthe positive ASLgSL term. For a spherical

    Fig. 3 Potential distribution of alloying elements andphase fractions that can form in fusion welds.

    Example shown is for a simple eutectic system that formsprimary a phase and intercellular a/b eutectic underconditions of nonequilibrium solidification. Location ofcomposition trace is across primary and eutectic aphase, as shown by horizontal dotted line.

    Fig. 4 Schematic illustration showing relation betweentemperature gradient (G), growth rate (R), and

    cooling rate. The cooling rate is controlled by the rate ofmovement of the temperature gradient.

    Fig. 5 Schematic illustration of grain structures thatcan form in castings, showing the chill zone

    near the mold wall, the columnar zone, and theequiaxed zone in the center of the casting. Source: Ref 3

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    nucleus of radius r, the free-energy change forhomogeneous nucleation is given by:

    Ghom 4

    3pr3Gv 4pr

    2gSL (Eq 5)

    Equation 5 is plotted in Fig. 7(b), whichshows the individual contributions to Ghom

    and the overall change in Ghom. The overallchange in Ghom goes through a maximum,which describes the critical radius (r*) atwhich point the reduction in Ghom due to4/3pr3Gv begins to become larger than theincrease in Ghom associated with the 4pr

    2gSLterm. A nucleus that forms with a radius smal-ler than r* is unstable, because any furtherincrease in the nuclei radius will produce anincrease in Ghom. Conversely, any nuclei thatforms with a radius larger than r* is stable,because further growth in the nuclei leads toan overall reduction in Ghom. The maximumin Ghom is denoted as G* and representsthe activation energy associated with homoge-neous nucleation. This condition is given by:

    dGhom

    dr 4pr2Gv 8prgSL 0 at r

    (Eq 6)

    From which the following expressions can bederived for r* and G*:

    r 2gSLGv

    (Eq 7a)

    G 16pg3SL

    3 Gv 2

    (Eq 7b)

    Equations 7 and 4 can be combined toreveal the influence of undercooling on r* andG*:

    r 2gSL

    L

    Tm

    T(Eq 8a)

    G 16pg3SL

    3L2

    Tm

    T

    2

    (Eq 8b)

    Note that, according to Eq 8(a) and (b), r* andG* are infinite when T = 0, indicating thatnucleation cannot occur without some under-cooling. The undercooling is needed so thatthe reduction in Ghom due to the volumefree-energy change (by way of Eq 4) is largerthan that due to the increase in Ghom asso-ciated with the interfacial energy term. Thus,r* and G* each decrease with increasedundercooling.

    For heterogeneous nucleation on an existingmold wall, the overall free-energy change isgiven by (Ref 4):

    Ghet VsGv ASLgSL ASMgSM gLM(Eq 9)

    The first two terms are identical to those forhomogeneous nucleation. The third term(ASMgSM) represents the increase in overall freeenergy from formation of the solid/mold inter-face, while the fourth term (ASMgLM) representsthe reduction in overall free energy associated

    with elimination of some of the liquid/moldinterface due to formation of the nucleus. Notethat the interfacial energy between two solids istypically less than that between a solid and aliquid. Thus, the ASM(gSM gLM) term is typi-cally negative so the Ghet < Ghom. Thevalues of Vs, ASL, and ASM will depend on theshape of the nucleus as determined by the wet-

    ting angle, y (Fig. 6d). The value ofy, in turn,is governed by the relative values of surfaceenergies and is given by a force balance in thehorizontal direction as:

    gLM gSM gSL cosy (Eq 10a)

    y cos1gLM gSM

    gSL

    (Eq 10b)

    Assuming the nucleus forms as a sphericalcap, the values of ASL, ASM, and Vs are givenby:

    ASL 2pr21 cosy (Eq 11a)

    ASM pr2sin2 y (Eq 11b)

    VS pr32 cos y

    1 cosy 2

    3(Eq 11c)

    Equations 9 to 11 can be combined for anexpression forGhet:

    Ghet 4

    3pr3Gv 4pr

    2gSL

    S y (Eq 12)

    where:

    S y 2 cosy 1 cos y 2

    4(Eq 13)

    Note that 0 y 180 and 0 S(y) 1.Thus, it is apparent that Ghet Ghom. Thisis shown schematically in Fig. 8. Low valuesofy are an indication that the solid/mold inter-facial energy is low so that the solid easily wetsthe mold wall. This leads to low values of S(y)and reduced values ofGhet; that is, nucleationis made easier for reduced values ofgSM.

    Application to Fusion Welding

    Fusion welding represents a unique case

    that can be most easily understood bystarting with Eq 10(b) and noting that themold wall and the solid are identical, becausethe base metal acts as the mold in fusion weld-ing. Thus, it can immediately be noted thatfusion welding leads to the followingconditions:

    gSM 0 (Eq 14a)

    gLM gSL (Eq 14b)

    Fig. 6 Schematic illustrations of homogeneous (a andb) and heterogeneous (c and d) nucleation.

    Figures on the left are for a temperature above themelting point. Figures on the right are for a temperaturebelow the melting point. The wetting angle, y, is shownin (d).

    Fig. 7 (a) Variation in volume free-energy withtemperature for the solid and liquid. (b)

    Variation in surface energy term, volume free-energyterm, and DG

    homwith nucleus radius for homogeneous

    nucleation

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    y cos1gSLgSL

    0 (Eq 14c)

    Sy 0 0 (Eq 14d)

    Thus, from Eq 12, theactivation energy in fusionwelding (Gfw) for nucleation is givensimply by

    Gfw = 0. This is compared toGhom andGhetin Fig. 8. This can be interpreted by noting thatthe base-metal mold presents a perfect crystallo-graphic match forgrowthof thesolid fusion zone.Thus, there is no solid/mold interface in fusionwelding due to this perfect crystallographicmatching. An example of this in a fusion weldmade with the electron beam process is shownin Fig. 9 (Ref 5). Note that there are no fineequiaxed grains at the fusion line, as oftenobserved in the chill zone of castings. Instead,the weld-metal grains grow directly fromthe pre-existing base-metal grains. As a result, there is nobarrier to formation of thesolid. This conditionisreferred to as epitaxial growth, because growthoccurs directly fromthe preexisting solidwithoutthe need for nucleation. Therefore, there is noundercooling required to initiate solidificationat the fusion line, and solidification commencesat the liquidus temperature of the alloy. It shouldbe noted thatundercoolingcan stilloccur neartheweld centerline due to the process of constitu-tional supercooling, as explained in more detaillater.This canlead to theformation of thecentralequiaxed zone often observed in fusion welds.Undercooling can also be required for nucleationof new phases during solidification.

    Grain Structure of Fusion Welds

    As described previously, the weld-metalgrains will grow epitaxially from the preexist-ing base-metal grains. However, not all of thesegrains will be favorably oriented for continuedgrowth. Two primary factors control thecontinued competitive growth of weld-metalgrains:

    The grains tend to grow in a direction anti-parallel to the maximum direction for heatextraction.

    The solid will grow in the easy-growthcrystallographic directions.

    The first criterion results from the need totransport the latent heat of solidification down

    the temperature gradient into the cooler basemetal. Because the temperature gradient ishighest in a direction perpendicular to thesolid/liquid interface, the resultant heat-flowrate is also highest in this direction. Thus, thegrains tend to grow in a direction perpendicularto the solid/liquid interface. The second crite-rion results from the preferred crystallographicgrowth direction, which, for cubic metals, isalong the [100] directions. By combining thesetwo criteria, it can be seen that grains that havetheir easy-growth direction most closelyaligned to the solid/liquid interface normal willbe most favorably oriented to grow, thuscrowding out less-favorably-oriented grains.This phenomenon accounts for the columnargrain zone that is often observed in castings,shown schematically in Fig. 5. In this case,the grains that nucleated near the mold walland have their easy-growth direction alignednormal to the mold/casting interface outgrowthe less-favorably-oriented grains, leading tothe columnar region.

    The situation is slightly more complex infusion welding, because the pool shape pro-duces a curved solid/liquid interface that is con-stantly in motion as it follows the heat source.This is shown schematically in Fig. 10 (Ref6). Grains at the fusion line may initially be ori-ented in a favorable direction for growth, buttheir direction may become unfavorable as the

    curved solid/liquid interface changes its posi-tion. These grains may then eventually beovergrown by other grains that exhibit morefavorable orientation for growth as the solid/liq-uid interface sweeps through the weld. Anexample of this is shown on a weld in nearlypure (99.96%) aluminum in Fig. 11(a) (Ref 7).

    As may be expected, the pool shape can havea strong influence on competitive grain growthand the resultant grain structure of the weld.In turn, the pool shape can be influenced bythe welding parameters. At low-to-moderateheat-source travel speeds, the pool shape is gen-erally elliptical and typically produces the grainstructure pattern shown in Fig. 11(a). However,

    at higher travel speeds, the pool shape becomeselongated into a teardrop shape in which thesolid/liquid interface is straight. This elongatedshape is attributed to the low thermal gradientand high growth rate that exist at the weld cen-terline. The release of latent heat is proportionalto the growth rate. Because the growth rate ishighest at the weld centerline, the release rateof latent heat is also highest at the weld center-line. However, the temperature gradient is at a

    Fig. 9 Example of epitaxial growth from the fusion linein an electron beam weld of alloy C103.

    Original magnification: 400. Source: Ref 5

    Fig. 10 Schematic illustrations of competitive graingrowth in welds. (a) Early growth of grains

    near the fusion line. (b) Continued growth of favorably-orientated grains at a later time. Source: Ref 6

    Fig. 8 Comparison of free-energy changes associatedwith homogeneous nucleation, heterogeneous

    nucleation, and fusion welding

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    minimum at the weld centerline, so it is difficultto transport the latent heat away from the poolto permit solidification. This causes elongationof the pool near the weld centerline and leadsto the teardrop shape. In this case, the directionof grain growth does not change (because thesolid/liquid interface is no longer curved), andthe grains grow straight toward the weld center-

    line until grains growing from each side of theweld intersect. This process typically leads toa centerline grain boundary, as shown inFig. 11(b) (Ref 7).

    Axial grains that grow along the direction ofheat-source travel can also occasionally beobserved in fusion welds. The various types ofgrain morphologies are summarized in Fig. 12(Ref 6). Examples of grain structures producedwith elliptical and teardrop-shaped weld poolswere shown in Fig. 11. Figures 12(c) and (d) rep-resent conditions in which an axial grain growsalong the direction of the heat-source travel.These grains form in the region where the solid/liquid interface is generally perpendicular to thedirectionof heat-sourcetravel, so that it becomesfavorable for one or more grains to grow in thisdirection. The width of this zone can depend onthe pool shape. The region of the interface thatis perpendicular to the heat-source direction isrelatively small in an elongated weld pool, sothe width of axial grains will also be small. Bycomparison, this perpendicular region is rela-tively larger for an elliptical pool, so the axialgrain region can also be larger.

    The large columnar grains and the potentialpresence of centerline grain boundaries are gen-erally undesirable from a weldability andmechanical property point of view. Centerlinegrain boundaries can often lead to solidificationcracking associated with solidification shrinkage

    andlow-melting-point filmsthat become concen-trated at the centerline. Fine, equiaxed grains aredesired overcoarse columnargrains forimprove-ments in bothcracking resistance andmechanicalproperties (at low temperature). One effectivemeans for minimizing or eliminating the coarsecolumnar grains is through manipulation of thepool shape. Figure 13 shows an example of aweld in which the arc was oscillated at a fre-quency of 1 Hz in a direction normal to theheat-sourcetravel (Ref8). In thiscase, the contin-uously changing direction of the solid/liquidinterface makes it difficult for the columnargrains to extend over large distances, thusproviding a degree of grain refinement. Grainsize reduction can also be achieved through the

    use of inoculants. This process takes advantageof heterogeneous nucleation (discussed previ-ously) and liquid undercooling that occur due toconstitutional supercooling. This topic isdescribed in more detail in the next section.

    Substructure Formation in FusionWelds

    As shown previously in Fig. 2, grains inwelds typically exhibit various substructural

    morphologies within the grains that can be cel-lular, columnar dendritic, or equiaxed dendritic.Cellular and columnar dendritic morphologiesdevelop due to breakdown of the initially planarsolid/liquid interface that forms at the fusionline, while equiaxed dendrites form by nucle-ation of solid in undercooled liquid, typically

    near the weld centerline. Formation of thesefeatures can be understood with the concept ofconstitutional supercooling. The basics of thistopic are described first, followed by applica-tion of the theory to understanding the substruc-ture formation in fusion welds.

    Constitutional SupercoolingAs shown by the phase diagram in Fig. 14(a),

    formation of a solid leads to rejection of soluteinto the liquid. The extent of solute enrichmentin the liquid progresses as solidification pro-ceeds and the liquid composition follows theliquidus line. The solute rejected by the solidat the solid/liquid interface must be transportedaway from the interface by diffusion and/orconvection in the liquid. If the solid/liquidinterface growth rate is relatively high (whichleads to a high rate of solute rejection) and/orthe transport of solute into the liquid by diffu-sion or convection is low, then a solute bound-ary layer can develop in the liquid near the

    solid/liquid interface. Because solute enrich-ment leads to a reduction in the liquidus tem-perature (for an element that partitions to theliquid), it follows that the presence of a solute

    Fig. 12 Summary of various grain morphologies that can form from weld pools of different shapes. Source: Ref 6

    Fig. 13 Grain structure in a fusion weld of alloy 2014made with transverse arc oscillation. Source:

    Ref 8

    Fig. 11 Examples of (a) competitive grain growth and(b) a centerline grain boundary forming on a

    weld in 99.96 % Al. The weld in (a) was made at awelding speed of 250 mm/min (10 in./min). The weld in(b) was made at a welding speed of 1000 mm/min (40in./min). Source: Ref 7

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    boundary layer leads to a gradient in the liqui-dus temperature near the solid/liquid interface.This is shown schematically in Fig. 14(b) and(c), where the liquidus temperature is relativelylow at the solid/liquid interface due to the largeamount of solute in the liquid at that point. Theliquidus temperature gradually increases awayfrom the interface as the solute concentrationdecreases. The liquidus temperature does notchange outside the solute boundary layer.

    Next, consider how the relative magnitudesof the liquidus temperature (TL) gradientdescribed previously (dTL/dx) and the actualtemperature (Ta) gradient (dTa/dx) in the liquidaffect the stability of a planar solid/liquid inter-face that forms as the alloy initially starts tosolidify. Figure 15(a) shows the condition fora relatively steep temperature gradient such that

    dTa/dx > dTL/dx in the liquid. The planar inter-face is moving to the right and develops protru-sions during growth. Such protrusions canoccur in practical situations due to interfacepinning effects from inclusions in the liquidand/or differences in the rate of growth betweenneighboring grains that exhibit different crystal-lographic orientations relative to the solid/liq-uid interface (as described previously in thesection about competitive grain growth). Forthis case in which dTa/dx > dTL/dx, the tip ofthe protrusion encounters liquid that is at a

    temperature above the liquidus temperature ofthe alloy. Thus, the solid protrusion is not stableand melts back so that the planar interfaceremains stable. Under this condition, no sub-structure forms.

    Figure 15(b) shows the case for a relativelylow-temperature gradient in which dTa/dx 0:617100No1=3

    1 TN

    3

    Tc3

    " #Tc (Eq 23)

    where G is the temperature gradient in the liq-uid, No is the total number of heterogeneoussites available for nucleation per unit volume,TN is the associated undercooling required

    for nucleation, and

    Tc is the undercooling atthe solid/liquid interface, which depends onthe temperature gradient and growth rate. Thevalue ofTc can be calculated using dendritegrowth undercooling models (Ref 20, 21). Thepractical difficulty in the application of Eq 23lies in the ability to determine appropriatevalues ofTN and No. Nevertheless, the modelis useful because it was shown to correctly cap-ture the observed effects of various factors onthe CET, such as growth rate, temperature gra-dient, and alloy composition.

    More recently, Gauman et al. (Ref 22)extended the analysis proposed by Hunt. Thecomposition profile in the liquid was calculateddirectly using the appropriate solution of the

    diffusion equations for an isolated dendrite witha parabolic tip geometry. This was then used todetermine the liquidus temperature profile (Tz).The actual local temperature profile in the liq-uid (Tq,z) was considered to be controlled byheat extraction through the solid and was deter-mined through knowledge of the temperaturegradient and dendrite tip temperature as deter-mined by the Kurz, Giovanola, Trivedi (KGT)model (Ref 21). The actual undercooling(Tz) at any location within the liquid is thengiven by:

    Fig. 18 Example of equiaxed zone in the centerline ofa weld made with the gas tungsten arc

    welding process on 6061 aluminum. Source: Ref 2

    Table 1 Constitutional supercooling

    calculations for the aluminum-coppersystem showing the critical growth ratesrequired for breakdown of the solid/liquidinterface for various values ofGand Co thatmay be encountered in casting, arc welding,and laser welding

    Co,wt% Cu

    G = 20 C/mm (casting)

    G = 200 C/mm(arc welding)

    G = 2000 C/mm(laser welding)

    0.5 0.0024 0.024 0.242 0.0006 0.006 0.064 0.0003 0.003 0.03

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    Tz Tz Tq;z (Eq 24)

    Equiaxed grains will nucleate anywherein this undercooled region where the actualundercooling is more than that required fornucleation, Tz > TN. The critical volumefraction required for a fully equiaxed structureoriginally proposed by Hunt was used as the

    critical CET value.Figure 19 shows an example of a microstruc-

    ture selection map that was generated for thenickel-base single-crystal CMSX-4 using theapproach described previously (Ref 12). Thesolid continuous line in the plot represents thetransition between values of the solid/liquidinterface growth rate and temperature gradientin the liquid that lead to the CET. A G-R com-bination below this line will result in columnarsingle-crystal growth, while combinationsabove this line lead to equiaxed growth and lossof the single-crystal structure. Material para-meters required for calculation of the map weredetermined using a multicomponent thermody-namic database. The values of No and TNwere assumed to be No = 2 1015/m3 andTN = 2.5

    C. An increase in the value of Noor a decrease in the value of TN will widenthe range where equiaxed growth occurs. Thismap is useful in a practical sense because itidentifies combinations of G and R that permitretention of the single-crystal structure duringweld repair. The use of heat-flow equationscan then be used to link R and G to the weldprocessing parameters, such as heat-sourcepower, travel speed, and preheat temperature,in order to develop process-microstructuremaps for successful weld repair.

    Gauman et al. (Ref 12, 15) developed a sim-plified relationship between the temperature

    gradient, growth velocity, volume fraction ofequiaxed grains (j), and nuclei density (No) as:

    Gn

    R a

    ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi4pNo

    3 ln1 j3

    s

    1

    n 1

    " #n(Eq 25)

    where a and n are material constants that aredetermined by fitting calculations of the consti-tutional tip undercooling from the KGT model

    to an equation of the form T = (aR)1/n. ForCMSX-4, these values are a = 1.25 106

    K3.4/ms and n = 3.4 This relation is valid underhigh-temperature gradient conditions in whichthe value of No is most important forcontrolling nucleation and the value of TNcan be ignored. Welds can be prepared undervarious values of G and R, and the resultant

    volume fraction of equiaxed grains (j) can bedirectly measured on the weld cross sections.In this case, No is the only unknown in Eq 25and can thus be determined experimentally byfitting Eq 25 to the measured values ofj. ForCMSX-4, this results in No = 2 10

    15/m3.When the original condition for a fully colum-nar microstructure proposed by Hunt is invoked(j = 0.0066), all values on the right side of Eq25 are known and lead to the following condi-tion for avoiding the CET:

    Gn

    R> K (Eq 26)

    where K is a material constant that depends onNo, j, a, and n. For CMSX-4, K = 2.7 1024

    K3.4m4.4s. This approximate condition isshown as the dotted line in Fig. 19, and it canbe seen that this approximation is more restric-tive than the results obtained by the detailedcalculations. However, Eq 25 is useful becauseit permits straightforward coupling of R and Gto the weld processing parameters.

    Figure 20 shows an example of a microstruc-ture selection map for three different welds onalloy CMSX-4 (labeled A, B, and C)prepared under different processing conditions.This plot shows the variation in the Gn/R ratioas a function of depth in the weld pool. Asexpected, the Gn/R ratio is highest at the fusion

    line (bottom of the weld) and decreases as thetop of the weld is approached. The criticalvalue for the CET of CMSX-4 is superimposedon the plot. Welds prepared under conditions inwhich the critical value of Gn/R remains belowthis critical value everywhere in the weld areexpected to retain the single-crystal structure(e.g., weld A), while welds prepared withregions less than this value (e.g., welds B andC) will undergo the CET and lose the single-

    crystal structure. Experimental identification ofstray grains showed good agreement with thepredictions of Fig. 20.

    Figure 21 shows a process-microstructuremap that was proposed to reveal semiquantita-tive relations between the important processingparameters of heat-source travel speed (Vb),power (P), and preheat temperature (T0). This

    map was calculated using a single, integratedaverage of the Gn/R ratio to represent the varia-tion in G and R that occurs with position in themelt pool. The region of high Vb and low Prepresents very low heat-input conditions thatare insufficient to cause melting. At any travelspeed, a reduction in power is beneficial, andthis can be attributed to an increase in the tem-perature gradient. The results suggest that theeffect of heat-source travel speed depends onthe level of heat-source power. At low powers(i.e.,

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    within the range of parameters investigated.The processing window for the GTA welds isslightly smaller than the laser welds. This isprobably associated with the higher-intensityheat source of the laser that produces a highertemperature gradient.

    Vitek (Ref 24) improved upon the modeldeveloped by Gauman et al. (Ref 12) that per-

    mitted a more in-depth analysis of the effectof travel speed. In the early model, the Gn/Rratio was used as an indicator of stray grain for-mation, and a simple Gn/R value was calculatedat the centerline of the weld and averagedthrough the thickness. This neglects orientationeffects of the solidification front and does notprovide an accurate representation of straygrain tendency, because the fraction of straygrains does not vary linearly with Gn/R. Withthe newer approach, the fraction of stray grainswas determined directly at discrete positions inthe weld pool and used to determine an area-weighted average of stray grains as an indicatorof stray grain tendency. This improves theaccuracy by accounting for the pool shape andvariations in G and R around the pool.

    Figure 23 shows the calculated variation inthe weighted area fraction of stray grains inthe weld fc as a function of welding speedfor different weld powers. The tendency forstray grain formation decreases fc decreases)with a decrease in power and an increase inwelding speed. Increasing travel speed is partic-ularly advantageous. The only minor exceptionto this trend is observed at the lowest powerand travel speed, where an increase in travelspeed causes a small increase in fc initiallybefore fc then decreases with increasing travelspeed. These results indicate that, within thisregime, the potential beneficial effect of the

    increase in temperature gradient produced byincreasing travel speed is outweighed by thedetrimental effect of an increase in growthrate that occurs with increasing travel speed.This can be understood by noting that theformation of stray grains depends on theGn/R ratio (where n = 3.4 for CMSX-4, for

    example). Thus, stray grain formation is moresensitive to G than R. The anomalous effect oftravel speed at low power has been attributed tochanges in weld pool shape. At low powers andtravelspeeds,the weld pool shape is one in whichthe area susceptible to stray grain formation is arelatively large fraction of the total weld poolarea. However, this trend is quickly diminished

    with further increases in travel speed.Factors Affecting Substructural Scale.

    Dendrite spacing (l) can have an importantinfluence on the mechanical properties andtime required for postweld homogenizationtreatments and therefore deserves some con-sideration. Kurz and Fisher (Ref 25) have pro-posed a geometrical model for primarydendrite spacing that leads to a relationship ofthe form:

    / G0:5R0:25 (Eq 27)

    which suggests that R and G have differentfunctional relationships on l. Recall that Gand R are related to the cooling rate through

    Eq 1. In most cases, dendrite spacing is relatedsemiempirically to the cooling rate through anequation of the form:

    Aen (Eq 28)

    where A and n are material constants and typi-cally 0.3 n 0.5. Thus, dendrite spacingdecreases with increasing cooling rate. Thisconcept can be added to the G-R diagramshown previously in Fig. 16. Note that theratio of G/R controls the type of substructure,while the quantity GR (= e) controlsthe substruc-tural scale. As discussed previously, the coolingrate is inversely proportional to the heat input.Thus, high heat inputs lead to low cooling rates

    and large dendrite spacings in the weld; this hasbeen observed experimentally in a number ofalloysystems (Ref2628). It should alsobe notedthat the cooling rate will vary throughout theweld due to changes in G andR, so that variationsin l within the fusion zone due to these changesare also expected.

    Solute Redistribution duringSolidification

    Binary Models. Solute redistribution is animportant topic because it controls both the dis-tribution of alloying elements across the cellu-lar/dendritic substructure and the type/amountof phases that form in the fusion zone during

    solidification. For many applications, soluteredistribution can be effectively assessed withthe aid of several simple models developed forbinary alloys. These are reviewed first, followedby models developed for ternary alloys. Exampleapplication of the models to multicomponentalloys is also described, followed by a discussionon the application of thermodynamic modelsdeveloped for multicomponent alloys.

    There are various solute redistribution mod-els available for binary alloys that account forsuch factors as solute diffusivity in the liquidand solid, dendrite tip undercooling, and coars-ening. A good review on the subject is availablein Ref 29. For many fusion welding applica-tions, a large extent of solute redistributionbehavior can be understood with the fairly sim-ple equilibrium and nonequilibrium (Scheil)(Ref 30) models that account for the extremecases of solute redistribution:

    Equilibrium lever law :

    Cs kCo

    1 kfL k(Eq 29a)

    CL Co

    1 kfL k(Eq 29b)

    Nonequilibrium :

    Cs kCo1 fsk1 (Eq 30a)

    CL CofLk1

    (Eq 30b)

    2500

    2000

    1500

    1000Laserpower,W

    500 Not meltedNot melted

    103

    102

    10

    Laser scanning speed, mm/s

    1

    Single-crystallized withdirectional dendrite

    Single-crystallized withdisoriented dendrite

    Polycrystallized withstray crystal

    Single-crystallized withdirectional dendrite

    Single-crystallized withdisoriented dendrite

    Polycrystallized withstray crystal

    101

    102

    0

    (a)

    1500

    1000

    Weldingh

    eatinput,W

    500

    102

    10

    Welding speed, mm/s

    1 101

    0

    (b)

    Fig. 22 Influence of heat-source power and travel speed on stray grain formation for alloy CMSX-4 for (a) laser weldsand (b) gas tungsten arc welds. Source: Ref 23

    Fig. 23 Calculated variation in the weighted areafraction of stray grains in the weld as a

    function of welding speed for three different weldpowers. Source: Ref 24

    Fundamentals of Weld Solidification / 105

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    where Cs and CL are the solid and liquid com-positions at the solid/liquid interface, Co is thenominal alloy composition, fs and fL are thefraction solid and fraction liquid, and k is theequilibrium distribution coefficient, which isgiven by k = Cs/CL. These expressions assumelinear solidus and liquidus lines so that kis con-stant throughout solidification. The value of kis

    an important parameter because it describes theextent to which a particular element partitionsbetween the solid and liquid. For k < 1, the sol-ute partitions to the liquid, and the smallerthe value of k, the more aggressive the parti-tioning to the liquid. For elements in whichk > 1, the solute partitions to the solid duringsolidification.

    The equilibrium lever law assumes completediffusion in the liquid and solid during solidifi-cation, equilibrium at the solid/liquid interface,and no undercooling during growth. The non-equilibrium lever law (often referred to as theScheil equation) carries similar conditions,except that diffusion in the solid is assumed tobe negligible. These two cases represent theextreme conditions of residual microsegrega-tion after solidification. The equilibrium leverlaw represents the case where there are no con-centration gradients in the liquid or solid duringsolidification, and there is no residual microse-gregation in the solid after solidification. Incontrast, nonequilibrium conditions representthe most severe case of residual microsegrega-tion in the solid after solidification becausesolid diffusivity is negligible.

    As an example, consider a binary eutectic A-B system, shown in Fig. 24(a), that exhibits lin-ear solidus and liquidus lines, a value of k =0.02 (for solute element B), a eutectic composi-tion of 20 wt% B, and a maximum solubility

    limit of 4 wt% B. Figures 24(b) and (c) showthe variation in liquid composition during solid-ification under equilibrium and nonequilibriumconditions for two alloys: one below the maxi-mum solid solubility with Co = 2 wt% B andone above the maximum solid solubility withCo = 5 wt% B. For the 2 wt% B alloy, the solid-ification conditions under each extreme arequite different. Under equilibrium conditions,the liquid composition never becomes enrichedto the eutectic composition because solute inthe solid is uniformly distributed and thereforecapable of dissolving all the solute before theeutectic point is reached in the liquid. Notefrom Eq 29(b) that the maximum solute enrich-ment in the liquid for the equilibrium condition

    is given as Co/k, which occurs when fL = 0. Inthis case, Co/k < Ce (the eutectic composition).The resultant microstructure directly after solid-ification would simply consist of primary awith a uniform distribution of B. For the non-equilibrium case, the liquid composition willalways become enriched to the eutectic point.Thus, directly below the eutectic temperature,the 2 wt% B alloy exhibits primary a with aconcentration gradient and 0.06 weight fractionof the a/b eutectic when solidified under non-equilibrium conditions.

    The two extreme solute redistribution beha-viors for the 5 wt% B alloy are compared inFig. 24(c). For the equilibrium case, the liquidcomposition will become enriched to the eutec-tic point because the nominal composition isabove the maximum solid solubility. In otherwords, Co/k> Ce. This eutectic reaction occurswhen there is 0.06 weight fraction remaining

    liquid. Thus, the solidification microstructuredirectly after equilibrium solidification consistsof primary a with a uniform distribution of Bat the maximum solid solubility of 4 wt% and0.06 weight fraction of the a/b eutectic. Forthe nonequilibrium case, the liquid compositionis always higher at any stage during solidifica-tion (i.e., any particular value of fL), becausethe solid does not dissolve as much solute. Asa result, more liquid remains when the eutecticcomposition is reached (0.18 weight fraction),and more of the eutectic constituent forms inthe solidification microstructure. The final alloyhere exhibits primary a with a concentrationgradient and 0.18 weight fraction of the a/beutectic (three times the weight fraction ofeutectic that formed for the equilibrium case).Figure 24(d) shows the corresponding soluteprofiles in the a solid phase after solidificationfor the 2 wt% B alloy. Under equilibrium con-ditions, there is simply primary a with auniform distribution of 2 wt% B. For nonequi-librium conditions, the primary a phase exhibitsa concentration gradient with a minimum ofkCo = 0.4 wt% B and a maximum at the solubil-ity limit of 4 wt% B. The portion of solid thatexhibits a uniform composition of 4 wt% Brepresents the eutectic a (the composition ofthe eutectic b is not shown).

    Equations 30(a) and (b) have the interestingproperty that CL! 1 as fL! 0 and Cs! 1

    as fs! 1 (for k < 1), which indicates that thesolid will always be enriched to the maximumsolid solubility, while the liquid will alwaysbe enriched to the eutectic composition undernonequilibrium conditions. This can be attribu-ted to the lack of diffusion in the primary aphase, which leads to the inability of all the sol-ute to be incorporated into the primary phase.This can be understood by direct inspectionof Fig. 24(d) and noting that the dissolved sol-ute in the solid is given by the area under theCs fs curve. For the equilibrium case, the totaldissolved solute is obviously 2 wt% B, which isthe nominal value. However, the dissolved sol-ute for the nonequilibrium case is always lessthan this due to the regions in the solid where

    Cs < Co. In this case, the excess solute mustbe accommodated by formation of the eutecticconstituent that contains the B-rich b phase.

    Strictly speaking, it is important to note thatthe solute redistribution equations described inthis section do not account for undercoolingeffects that can occur at the cell/dendrite tipduring nonplanar solidification. Under high-energy-density welding processes that are oper-ated at high travel speeds, this undercoolingeffect may become significant. This subject isdiscussed in more detail in the section Rapid

    Solidification Considerations in this article.However, this effect is typically not significantunder many moderate cooling-rate conditionstypical of arc welding and high-energy-densityprocesses operating at low heat-source travelspeeds. In these cases, the models describedfor planar solidification can be applied on alocal scale within a small volume element that

    encompasses a planar interface. An example

    1200

    (a)

    (b)

    (c)

    (d)

    Temperature,

    K

    1000

    800Liquid

    0

    25

    20 Nonequilibrium

    CO

    = 2 wt% B

    Equilibrium

    Fraction liquid

    15

    10

    Liquidcomposition,wt%B

    5

    00 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1

    5 10 15 20

    Composition, wt% B

    25 30 35 40 45 50

    600

    400

    200 +

    0

    25

    20 Nonequilibrium

    Nonequilibrium

    CO

    = 2 wt% B

    Equilibrium

    Equilibrium

    Fraction liquid

    15

    10

    Liquidcomposition,wt

    %B

    5

    00 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1

    Fraction Solid, fs

    Solidc

    omposition,C

    s

    00

    1

    2

    3

    4

    5

    0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1

    Fig. 24 Example of solute redistribution calculationsfor equilibrium and nonequilibrium

    conditions. (a) Hypothetical phase diagram. (b) Variationin liquid composition for Co = 2 wt%. (c) Variation inliquid composition for Co = 5 wt%. (d) Variation in solidcomposition for Co = 2 wt%

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    of this is shown in Fig. 25 for cellular solidifi-cation. Here, the solidification process can berepresented by the enclosed region shown andnoting that solidification starts at the cell core(where fs = 0) and finishes at the cell boundarywhen two cells meet (fs = 1). The soluteredistribution then occurs locally within thegiven volume element that exhibits an essen-

    tially planar interface between the liquid andsolid.

    The only difference that separates thesetwo extreme cases of solute redistribution dur-ing solidification is the solute diffusivity inthe solid. Thus, it is useful to consider theextent of solute diffusivity expected for a givenset of parameters and resultant cooling rate.The Brody-Flemings model was the firstattempt at taking back-diffusion into the solidinto account during solidification and is givenas (Ref 31):

    Cs kCo 1 fs

    1 ak

    k1(Eq 31a)

    CL Co 1 1 fL1 ak

    k1(Eq 31b)

    a Dstf

    L2(Eq 31c)

    The a parameter in Eq 31(c) is a dimension-less diffusion parameter, while Ds is the diffu-sivity of solute in the solid, tf is thesolidification time (cooling time between theliquidus and terminal solidus), and L is halfthe dendrite arm spacing. The Dstf term in thenumerator of Eq 31(c) essentially representsthe distance that solute can diffuse in the solid

    during solidification, while the half dendritearm spacing, L, represents the length of the con-centration gradient. Thus, when Dstf

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    elements. For example, calculation of the aparameter for carbon in nickel will yield valuesthat are significantly greater than unity. This isto be expected, because carbon diffuses by aninterstitial mechanism and therefore exhibitsdiffusion rates that are orders of magnitudehigher than the substitutional alloying elements.Evidence for this is reflected in the activation

    energy term (Q) for diffusion of carbon innickel shown in Table 2. Note that Q for thesubstitutional alloying elements varies over afairly narrow range of 255 to 299 kJ/mol, whilethe value for carbon is approximately half thisat 135 kJ/mol.

    Figure 27(a) shows calculated results for sol-ute redistribution of carbon in nickel (Ref 39).In this figure, the solute redistribution behaviorwas calculated with Eq 31 and 32 using thetemperature-dependent diffusion rate of carbonin nickel. Comparison is made between thenonequilibrium Scheil equation and the leverlaw. Note that the detailed results from theClyne-Kurz model are essentially identical tothat of the lever law, indicating that completesolid-state diffusion of carbon is expected innickel-base alloys during solidification. A simi-lar effect can be expected for nitrogen in nickel.This calculation was conducted for a coolingrate of 650 C/s (1170 F/s) through the solidi-fication temperature range. Higher cooling ratestypical of high-energy-density welding mayalter this result and begin to limit carbon

    diffusion in the solid. Aside from this possibil-ity, these results demonstrate that carbon (andnitrogen) can be expected to exhibit completediffusion in the solid during most welding con-ditions. Figure 27(b) shows a similar calcula-tion for substitutional diffusion of titanium ina body-centered cubic Fe-10Al-5Cr alloy thatwas calculated using the detailed model pro-

    posed by Kobayashi (Ref 33, 41). These resultsare somewhat similar to those for carbon innickel in that solid-state diffusion is essentiallycomplete at moderate cooling rates. However,diffusion may become insignificant at very highcooling rates typical of high-energy-densityprocesses. These results are meant to serve asexample calculations that can be applied tounderstanding solute redistribution behavior infusion welds of any alloy system when the per-tinent alloy parameters are known.

    For conditions in which solid-state diffusionis negligible, microsegregation will persist inthe as-solidified weld (except for the case inwhich k = 1). An example of this is shown inFig. 28 for fusion welds in a niobium-bearingsuperalloy (Ref 36, 42). The final degree ofmicrosegregation can be assessed by directdetermination of the k value for the element ofinterest, where the degree of microsegregationwill increase with decreasing k value (for kvalues < 1). For example, the lowest concentra-tion will occur at the dendrite core where solid-ification initiates. Direct inspection of Eq 30

    indicates that, at the start of solidification whenfs = 0, the dendrite core composition (which isthe first solid to form) is given by kCo.

    Although the models described earlier werestrictly developed for binary alloys, they canbe used in a quantitative manner for multicom-ponent engineering alloys when the alloy prop-erly mimics the solidification behavior of a

    binary system. An example is provided hereby application of the simple binary Scheil equa-tion to Ni-Cr-Mo-Gd alloys. A typical as-solidi-fied microstructure of an alloy is shown inFig. 29(a). These alloys exhibit g dendritesand an interdendritic g/Ni5Gd eutectic-typeconstituent. Research (Ref 43, 44) has shownthat gadolinium controls the solidificationbehavior of these alloys. In particular, thesolidification temperature range and amountof terminal eutectic-type constituent thatforms at the end of solidification are essentiallydominated by the gadolinium concentration.Solidification of these alloys initiates at theliquidus temperature by the formation of pri-mary g-austenite. As solidification proceeds,the liquid becomes increasingly enrichedin gadolinium until the liquid ! g + Ni5Gdeutectic-type reaction is reached, at which pointsolidification is terminated.

    This reaction sequence and temperaturerange is similar to that expected in the binarynickel-gadolinium system. Simple binary

    Fig. 26 Dimensionless a parameter as a function of cooling rate for a wide range of alloying elements in nickel

    0.200

    (a)

    (b)

    0.150

    0.100

    Clyne-Kurz model

    Scheil equation

    Lever law

    Fraction solid, fs

    0.050

    0.0000.0

    3.0

    2.0

    1.0

    Ticon

    centrationinsolid,wt%

    0.00.0 0.2 0.4

    Fraction solid, fs

    0.6 0.8 1.0

    0.2

    30,000 C/s

    Scheil

    Lever law

    30 C/s

    0.1 C/s

    Solidcomposition,wt%C

    0.4 0.6 0.8 1.0

    Fig. 27 Comparison of solute redistribution behavior.(a) Carbon in a nickel-base superalloy

    calculated using the lever law, Scheil equation, andClyne-Kurz model. (b) Titanium in an Fe-10Al-5Cr-1.5Ti-0.4C alloy with varying cooling rates (calculated usingthe Kobayashi model) compared to the lever law andScheil cases. Source: Ref 39

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    nickel-gadolinium alloys with less than approx-imately 13 wt% Gd exhibit a similar two-stepsolidification sequence consisting of primaryaustenite formation followed by a terminaleutectic reaction involving the Ni17Gd2 inter-metallic at 1275 C (2327 F). By comparison,the multicomponent Ni-Cr-Mo-Gd alloys com-plete solidification at $1258 C ($2295 F)by a terminal eutectic-type reaction involvingthe Ni5Gd intermetallic. Thus, although the sec-

    ondary phase within the terminal eutectic con-stituent is different in each case, the terminalreaction temperatures are very similar. Asshown in Fig. 29(b), a pseudo-binary solidifica-tion diagram can be developed for this systemthat is similar to the phase diagram of a binaryeutectic alloy. In this case, the solvent is repre-sented by the Ni-Cr-Mo solid-solution g-austen-ite phase, and gadolinium is treated as thesolute element. The similarity of this g-gadolin-ium binary system to a binary eutectic system isreadily evident in several ways:

    The as-solidified microstructure consists ofprimary g dendrites surrounded by an inter-dendritic eutectic-type constituent in whichthe secondary phase in the eutectic is soluterich.

    The amount of eutectic-type constituentincreases with increasing solute content.

    The proportional amount of each phasewithin the eutectic constituent is relativelyinsensitive to nominal solute content.

    It was also observed that the eutectic tempera-ture is not strongly dependent on the nominalgadolinium concentration. Key points of the dia-gram shown in Fig. 29(b) were determined witha combination of thermal analysis and quantita-tive microstructural characterization techniques.Figure 29(c) shows a comparison of themeasured and calculated g/Ni5Gd fractioneutectic from fusion welds made on alloys withvarious gadolinium concentrations. In this plot,a comparison is made with the calculated

    eutectic fraction using the simple Scheil equa-tion. The Scheil equation can be used for eutec-tic fraction calculations by noting that, whenCL = Ce (the eutectic composition), the remain-ing fraction liquid (fL) transforms to fractioneutectic (fe), so that:

    fe

    Ce

    Co 1=k1

    (Eq 35)

    Good agreement is observed betweenthe measured and calculated values. This sup-ports the use of a pseudo-binary analog formodeling the solidification behavior of thesealloys.

    Ternary Models. The expressions derivedearlier for binary alloys can be used quantita-tively in multicomponent alloys when thealloy behaves like a binary system. However,many engineering alloys exhibit multiple reac-tions during solidification that occur over arange of temperatures and exhibit more thanone eutectic constituent. Thus, they typically

    cannot be treated in a quantitative fashionwith the simpler models described earlier.In this case, models for ternary alloys can beuseful, and relatively simple solidificationpath equations can be derived for limiting casesof solute redistribution in ternary alloys. Twosets of solute redistribution equations areneeded to fully describe the solidification pathsof ternary alloys. The first set describes the var-iation in liquid composition and fractionliquid during the primary stage of solidification.These expressions can be used to identifyif the liquid composition is enriched to a mono-variant eutectic-type reaction and, if so,what type of reaction will occur and the frac-tion of total eutectic constituent that will

    form in the microstructure. The second set ofexpressions describes the variation in liquidcomposition and fraction liquid during themonovariant eutectic reaction. These expres-sions can be used to determine if the liquidcomposition is enriched to the ternary eutecticreaction and the fractions of both the monovar-iant and ternary eutectic constituents. Only theprimary solidification path expressions are dis-cussed here. More detailed information on thefull ternary model can be found elsewhere(Ref 45).

    For ternary solidification, three limiting casescan be identified based on the diffusivity of sol-ute in the solid phases:

    Negligible diffusion of each solute in thesolid phases, referred to as nonequilibriumsolidification

    Negligible diffusion of one solute in thesolid phases and infinitely fast diffusion ofthe other solute in the solid phases, referredto here as intermediate equilibrium.

    Infinite diffusion of each solute in the solidphases (equilibrium)

    Expressions for the primary solidification pathsfor these three conditions are given by:

    20

    (a)

    (b)

    15

    10

    5

    0 10 20

    Distance, m

    Dendrite

    core

    Interdendritic

    region

    Nb

    Si

    30 40 50

    Composition,wt%

    0

    Fig. 28 Example of microsegregation in a weld of aniobium-bearing nickel-base superalloy. (a)

    Micrograph showing position of composition trace. (b)

    Corresponding electron probe microanalysis resultsshowing niobium microsegregation. Source: Ref 36, 42

    Fig. 29 (a) Microstructure of fusion weld on a Ni-Cr-Mo-Gd alloy. (b) Pseudo-binary phase

    diagram for the g-gadolinium system. (c) Comparison of

    the measured and calculated g/Ni5Gd fraction eutecticfrom fusion welds made on alloys with variousgadolinium concentrations. Source: Ref 44

    Fundamentals of Weld Solidification / 109

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    Equilibrium:

    CLA CoA

    1kaA1kaB

    CoBkaB CLB

    CLB

    kaA

    (Eq 36a)

    Intermediate equilibrium:

    CLA CoACoB kaBCLB1 kaBCLB

    kaA1(Eq 36b)

    Nonequilibrium: CLA CoACLB

    CoB

    kaA 1kaB 1

    (Eq 36c)

    where fL is the fraction liquid, Coj is the nomi-nal concentration of element j, CLj is the con-centration of element j in the liquid, and kij isthe equilibrium distribution coefficient for ele-ment j in phase i. When the liquid compositiongiven by Eq 36 intersects a monovariant eutec-tic line, the remaining fraction liquid transformsto a binary-type eutectic and possibly the ter-

    nary eutectic. Thus, the value of fL at the inter-section point of the primary solidification pathand monovariant eutectic line defines the totalamount of eutectic in the microstructure.Details on the calculation procedure for deter-mining this value are provided elsewhere (Ref45). The difference among the three cases con-sidered here is governed by the diffusivity ofsolutes in the solid phases. Thus, the conditionthat most closely describes the solidificationbehavior for an actual application can be deter-mined by calculation of the a parameter foreach of the solute elements of importance.

    Figure 30 shows an example of primarysolidification path calculations made for fusionwelds on multicomponent superalloys that formthe g/NbC and g/Laves eutectic-type constitu-ents at the end of solidification (Ref 46).Although these alloys contain multiple ele-ments, they can be treated as a pseudo-ternaryg-Nb-C system. Niobium and carbon are treatedas the important solute elements here becauseeach element partitions aggressively to the liq-uid during solidification and leads to the forma-tion of the niobium- and carbon-rich NbC phaseand the niobium-rich Laves phase. For this sys-tem, niobium exhibits negligible diffusion,while carbon diffuses infinitely fast. Thus,Eq 36(b) was used for these calculations. Cal-culations are shown for alloys with similar nio-bium concentrations and various amounts of

    carbon. Note that the addition of carbon pushesthe primary solidification path up into the car-bon-rich side of the liquidus projection. The liq-uid composition must then travel a longdistance down the g/NbC eutectic line as theg/NbC constituent forms. This accounts for theobserved influence of carbon that leads to largeamounts of the g/NbC constituent in thesealloys. It was also observed that carbon addi-tions increase the start temperature of the L !g + NbC reaction. This effect is not intuitive,because solute additions in which k < 1 (such

    as carbon) typically lower reaction tempera-tures. The calculations demonstrate the reasonfor this effect. The dotted arrow near the g/NbC eutectic line represents the direction ofdecreasing temperature (as determined throughthermal analysis). Note that carbon additionsdrive the solidification path to the carbon-richregion of the diagram where the L ! g +

    NbC reaction is relatively high, thus accountingfor the observed effect. Reasonable agreementwas obtained between the measured and calcu-lated volume fractions using these expressions(Ref 46).

    Modeling of Multicomponent Alloys. Therelatively simple models described previouslyare useful for assessing the solidifcation behav-ior of alloys that behave in a manner analogousto binary or ternary alloys. However, suchapproaches may be limited in some engineeringalloys. Multicomponent thermodynamic andkinetic software is now available that can alsobe used for understanding solidifcation behav-ior in such systems, and a simple example isprovided here. Figure 31(a) shows a light opti-cal micrograph of a weld between a superauste-nitic stainless steel (CN3MN) with $6 wt% Moand a nickel-base filler metal (IN686) with $14wt% Mo (Ref 47). This weld was prepared atthe 21% dilution level. Welds in these alloyssolidify with a primary L ! g solidifcationmode and then terminate solidifcation by a L! g + s reaction. Thus, the final weld micro-structure consists of primary g dendrites andinterdendrtic g/s eutectic. The s phase is amolybdenum-rich phase. Welds made at lowdilution levels (i.e., high molybdenum levels)would be expected to form relatively large frac-tions of the s phase. However, as shown inFig. 31(b), the s-phase content does not change

    significantly with weld dilution level and asso-ciated nominal molybdenum concentration ofthe alloy. This immediately suggests that otherfactors besides the nominal concentration ofmolybdenum are also affecting the s-phasecontent.

    The s-phase content is controlled by theamount of eutectic constituent that forms dur-ing the end of solidification. The fraction ofeutectic is, in turn, controlled by the nominalalloy composition (Co), eutectic composition(Ce), and distribution coefficient (k) for molyb-denum (Eq 35). Note that the nickel and ironcontents in the weld change appreciably with

    changes in dilution, and these changes in nickeland iron may affect the values of k and Ce.Figure 32(a) shows the variation in liquid com-position during solidification using a multicom-ponent Scheil simulation with Thermocalc (Ref48). The Scheil simulation is justified herebecause, as shown in Fig. 26, all the substitu-tional elements of interest are known to exhibitinsignificant diffusion rates during solidificationin austenite. Results are shown for welds at var-ious dilution levels. Solidification starts at thenominal composition (Co), which is controlledby the dilution level. The eutectic composition(Ce) is given by the inflection point where theeutectic reaction L ! g + s begins. It is appar-ent that the eutectic composition decreasesappreciably with increasing dilution. Figure 32(b) shows the variation in the molybdenum par-tition coefficient (k) for the same dilution levelsof interest. The partition coefficient for a givendilution does not vary significantly duringsolidification, but it increases slightly (from

    Fig. 30 Example of primary solidification pathcalculations made for fusion welds

    on multicomponent superalloys that form the g/NbC andg/Laves eutectic-type constituents at the end ofsolidification. Source: Ref 46

    Dendrite CoreInterdendritic Region

    20 m

    5

    (a)

    (b)

    4.5

    4

    3.5

    3

    2.5

    21.5

    1

    0.5

    00 20 40 60

    Dilution, %

    Volumefractionofsigmaphase,

    %

    80 10

    Fig. 31 (a) Light optical micrograph showing primaryaustenite and interdendritic s phase that forms

    in a dissimilar weld between a superaustenitic stainlesssteel base metal and nickel-base filler metal. (b) Variation ins-phase content withdilution. Source: Ref 47

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    $0.67 to 0.84) with decreasing dilution.Figure 32(c) summarizes the variations in Co,Ce, and k as a function of dilution. An increasein Co and a decrease in Ce and k will increasethe fraction eutectic and resultant amount ofsecondary phase. These results demonstratethere are offsetting effects in these parametersthat keep the s-phase content relatively inde-

    pendent of the weld-metal composition. Inother words, Ce and k each decrease withincreasing dilution, which would, in itself, leadto an increase in fraction eutectic and amountofs phase. However, these changes are offsetby the decrease in nominal molybdenum con-centration that occurs with increasing dilution.This accounts for the relatively constant s-phase content observed in these welds.

    The final s-phase content will also dependon the maximum solid solubility of molybde-num in the austenite and s phases. All ofthese factors can be accounted for with a com-plete multicomponent Scheil simulation. Table 3shows the amount ofs phase calculated for allthe dilution levels of interest. There is reason-able agreement between the measured and cal-culated amounts of s phase. These resultsalso carry important practical implications,because IN686 filler metal can be used at vari-ous dilution levels with minimal changes tothe s-phase content in the weld, which is bene-ficial from a solidification cracking and tough-ness standpoint.

    Rapid Solidification Considerations

    The conditions described previously ignorethe effects of the nonplanar interface and solutebuildup in the liquid on dendrite tip undercool-

    ing. Such factors can become important at highsolidification rates associated with high-energy-density welding processes. These undercoolingeffects are shown schematically in Fig. 33.The liquidus and solidus lines for a planar inter-face (tip radius, r = 1) are shown by the solidlines. Solute enrichment in the liquid at thesolid/liquid interface results from solute rejec-tion directly from the tip and diffusion downthe solute gradient that exists between the cells.This local enrichment produces a reduction inthe tip temperature, TC, as shown in Fig. 33.Undercooling is also produced by the surfaceenergy effects due to the tip with a finite radius.In this case, the solidus and liquidus linesare depressed relative to those for an infinite

    30

    (a)

    Liquidcomposition

    ,wt%Mo

    25

    20

    1.0 0.9 0.8

    Fe, Ni, Cr, Mo, C, Mn, P, Si, Cu, N

    100% Dilution

    83% Dilution

    0% Dilution

    21% Dilution

    37% Dilution52% Dilution

    0.7 0.6

    Fraction liquid

    0.5 0.4 0.3 0.2 0.1 0.0

    15

    10

    5

    0

    1.00

    (b)

    kvalue

    0.90

    0.80

    0.00 0.10 0.20

    Fe, Ni, Cr, Mo, C, Mn, P, Si, Cu, N

    0.30 0.40

    Fraction solid

    0.50 0.60 0.70 0.80 0.90 1.00

    0.70

    0.60

    0.50

    0.40

    0.30

    0.20

    0.10

    0.00

    0% Dilution21% Dilution

    100% Dilution

    83% Dilution

    52% Dilution37% Dilution

    1.0

    (c)

    Partitioncoe

    fficient,kMo

    Composition,wt%

    0.8

    0 20 40

    Dilution, %

    60 80 100

    0.6

    0.4

    0.2

    0.0

    30

    20

    kMo

    CoMo

    CeMo

    10

    0

    Fig. 32 Multicomponent Scheil calculations for fusion welds made between a superaustenitic stainless steel alloyand a nickel-base filler metal showing (a) variation in liquid composition with fraction liquid, (b) variation

    in kMo with fraction solid, and (c) variation in Co, Ce, and kMo with dilution

    Table 3 Comparison of the percent svalues calculated using ThermoCalc andmeasured experimentally

    Dilution, % Calculated s phase, % Measured s phase, %

    100 1.9 1.4 0.2

    83 2.4 1.7

    0.352 2.3 1.6

    0.2

    37 1.9 2.0

    0.421 1.4 2.1

    0.4

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    radius, as shown by the dotted lines. Thecorresponding undercooling associated with afinite tip radius is given by the Tr term inFig. 33. As a result of these two effects, the liq-uid temperature and composition can bechanged significantly from (To, Co) to (Tt, Ct),as shown in the figure. Also note that this pro-duces an increase in the dendrite core composi-

    tion from kCo to kCt. This change in theoperating point of the dendrite tip can have asignificant effect on the stability of the primarysolidification phase, the final distribution of sol-ute in the solid, and the final phase distribution.

    Different approaches have been used to solvethe dendrite undercooling problem in order todetermine the local tip temperature and compo-sition. For example, Burden and Hunt (Ref 49)assumed that the dendrite tips grow with aradius that minimizes undercooling. Thisassumption was used to solve directly for thetip radius, which then provided a direct solutionfor the undercooling and resultant tip composi-tion. However, this assumption does not capturethe observed behavior in which a dendriticinterface eventually reverts to a cellular andthen planar interface at high solidification velo-cities. Note also that this reversion to a planarinterface is not captured within the classicalconstitutional supercooling criteria (describedpreviously), because the model neglects surfacetension effects. At high solidification velocities,the cell spacing is decreased, which leads to anincrease in the solid/liquid interfacial area.The increase in surface area helps accommo-date the rapid rate of solute rejection requiredat high solidification velocities but also leadsto increased surface energy. At very high velo-cities, the cellular interface is no longer ener-getically favorable, and a planar interface

    reappears.The dendrite tip radius and solute redistribu-tion around the tip are actually coupled, so thatthe assumption of a cell tip growing to mini-mize undercooling is not completely accurate.This condition has been considered in greaterdetail by Kurz et al. (Ref 21). In the KGTmodel, the tip radius is related to the tempera-ture gradient and growth rate through the Pecletnumber (Pe) by:

    R2p2

    Pe2D2l

    R

    mlCo1 k

    Dl 1 1 kIPe

    G 0 (Eq 37)

    where G is the Gibbs-Thomson parameter (ratioof specific solid/liquid interfacial energy to

    melting entropy), Pe is the Peclet number givenby Pe = Rr/2Dl, and I(Pe) is given by I(Pe) =Peexp(Pe)E1(Pe), where E1 is the exponentialintegral function.

    Direct solution of Eq 37 for the dendrite tipradius is not possible because Pe is defined interms of both R and r. Thus, the expressionmust be solved numerically in which a widerange of Pe values are selected to determine

    I(Pe), and then the quadratic Eq 37 is solvedfor R numerically. Once R is known, the den-drite radius is given by r = 2PeDl/R. The

    resultant tip temperature and composition arethen given by:

    Cl Co

    1 1 kIPe(Eq 38)

    Tt To mlCl

    2

    r(Eq 39)

    As shown schematically in Fig. 33, this newoperating point of the dendrite tip (i.e., thechange in tip composition and temperature from(To, Co) to (Tt, Ct)) also affects the subsequentsolute redistribution because the new core com-position is changed from kCo to kCt. Sarreal etal. (Ref 50) addressed this problem by assumingthat undercooling at the dendrite tip is dissipatedby forming a certain fraction of primary solidphase, fos , that is given by the lever law at theundercooled temperature:

    fos Co C

    l

    Cl k 1(Eq 40)

    Under conditions in which solute diffusion inthe solid is negligible (which is often the casefor substitutional alloying elements at highsolidification velocities), the final fraction ofeutectic that forms is then given by the modi-fied form of the Scheil equation:

    fe 1 fo

    s Ce

    Cl

    1k1

    (Eq 41)

    Various levels of complexity can beaccounted for with the KGT model. For exam-ple, Dl and ml can each vary with temperature,while k can vary with both temperature and

    solidification velocity. At high solidificationvelocities, the value of k ! 1 due to solutetrapping in the solid. This velocity dependencecan be accounted for with the model proposedby Aziz (Ref 51) in which the effective distri-bution coefficient, k0, is given by:

    k0 k aiR

    D

    1 aiRD

    (Eq 42)

    where ai is related to the interatomic distanceand is typically between 0.5 and 5 nm. Equation42 has the form in which k0= k at low values of

    R and k0 = 1 at high R values.Figure 34 shows example calculations of

    the KGT model for an Ag-5wt%Cu alloy.The results demonstrate how the tip radius(denoted as R in Fig. 34a), temperature, andcore composition (Cs* in Fig. 34c) change withincreasing solidification velocity. The curves inFig. 34(a) and (c) demonstrate how variousassumptions about Dl, ml, and k affect theresults. Note that the dendrite radius initiallydecreases with increasing velocity but then rap-idly increases and becomes infinite at highgrowth velocities. This is the condition inwhich a planar interface is restabilized. The

    Composition

    T

    emperature

    Solidus for r= rt

    Solidus for r=

    Liquidus for r=

    Liquidus for r= r

    kCo kCt Ct

    Tc

    Tt

    To

    Tr

    Co

    Fig. 33 Schematic illustration showing dendrite tipundercooling

    103

    102

    (a)

    104

    105

    106

    107

    102 101 1 10

    V, cm/s

    Ag 5 wt% Cu

    G= 105 K/cm

    D,ko,m

    =const.

    D(T)

    ko,m

    =const.

    D(T),k

    (V)

    ko,m

    =c

    onst.

    D(T)

    ,k(V

    ,T),

    m(T

    )

    D(T),k(

    V)an

    dko,

    m=cons

    t. D(T

    )an

    dko

    ,m=con

    st.

    D,k

    o,m

    =con

    st.

    R,cm

    102 103

    1200

    (b)

    1180

    1160

    1140

    1120

    102 101 1 10

    V, cm/s

    Ag 5 wt% Cu

    G= 105 K/cm

    Tt,K

    Tt

    Tt

    Tt Tt

    102 103

    5

    (c)

    4

    3

    2

    1

    102 101 1 10

    V, cm/s

    Ag 5 wt% Cu

    G= 105 K/cm

    C

    *s,wt%

    102 103

    Fig. 34 Results from Kurz, Giovanola, Trivedi (KGT)model calculations showing variation in (a)

    dendrite radius, (b) dendrite tip temperature, and (c) cellcore composition as a function of growth rate. Source:Ref 21

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    extent of undercooling at high velocities can bequite significant and can lead to subsequentenrichment in the cell core composition relativeto that under ideal Scheil conditions (Fig. 34c).This effect provides one mechanism for reduc-ing the extent of residual microsegregation thatoccurs in many alloys that exhibit low solutediffusivity in the solid.

    Stainless steels represent an importantgroup of engineering alloys in which dendritetip undercooling can have a significant in-fluence on the primary phase that forms. Thecomposition of many commercial stainlesssteels is adjusted to induce primary delta-ferrite(d) solidification. The delta-ferrite phase isdesirable as the first solidification phasebecause it exhibits a higher solubility for trampelements, such as phosphorus and sulfur. Thus,with primary ferrite solidification, more of thephosphorus and sulfur are kept in solution andavoid the low-melting-point phosphorus- andsulfur-rich phases that are known to aggravatesolidification cracking. In contrast, the solubil-ity for these tramp elements is relatively lowin austenite (g), and stainless steels that solidifyas primary austenite are well known to be rela-tively sensitive to this form of cracking.Although some stainless steels have a nominalalloy composition that is designed to solidifyas ferrite (under low solidification velocities),the nominal composition can lie close to thetransition in primary solidification mode so thatdendrite tip undercooling can cause a shift inthe primary solidification mode at higher cool-ing rates.

    Fukumoto and Kurz (Ref 52) used a multi-component form of the KGT model to predicthow solidification velocity and resultant tipundercooling affects primary phase stability instainless steels. In this work, interface responsefunctions were developed by calculating the tiptemperature of the d and g phases as a functionof solidification velocity. An example calcula-

    tion for an Fe-18Cr-11.3Ni (wt%) alloy solidi-fied with a temperature gradient of 400 K/mmis shown in Fig. 35. The primary solidificationphase is identified by noting that the phase withthe highest tip temperature is the one that willsolidify first. Note that, for this alloy and tem-perature gradient, a shift in the primary solidifi-cation mode is expected at a solidification rateof 3.2 10-2 m/s, and such shifts have beenobserved experimentally.

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    Fig. 35 Phase stability calculations for an Fe-18Cr-11.3Ni alloy solidified with a temperature gradient of 400 K/mm(290 F/in.). The primary solidification phase is identified by noting that the phase with the highest tip

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