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Dislocation pile-up and cleavage: Effects of strain gradient plasticity on micro-crack initiation in ferritic steel 1 Introduction 3

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Page 1: Dislocation pile-up and cleavage: Effects of strain ...Therefore, the implementation of this model in nite element analysis is quite di cult. oT overcome this di cult,y Peerlings [20]

Article published in International Journal of Fracture. The �nal publication is available atdoi:10.1007/s10704-018-0313-8

Dislocation pile-up and cleavage: Effects of straingradient plasticity on micro-crack initiation in ferritic

steel

N. A. Giang, A. Seupel, M. Kuna, G. Hütter

September 24, 2018

Abstract

Micro-cracks in ferritic steel often originate from broken or debonded carbide particles,or from cleavage of the ferrite matrix. Experiments in literature show that dislocation pile-ups at grain boundaries or particles predominantly induce micro-cracks in ferritic steel.On the other hand, the ferrite can also arrest nucleated micro-cracks owing to local plasticdeformations which reduce the stresses at the crack tip. In the present study, the compe-tition between these mechanisms is investigated by cell model simulations using e�ectivegradient plasticity (scalar gradient plasticity) for the ferrite. This theory allows to modelthe dislocation pile-up by suitable interface conditions. Potential cleavage of the ferrite orfailure of the carbide is modelled by a cohesive zone. Parameter studies are performed withrespect to the size of the particle and the strengths of ferrite and carbide.Keywords: Ferritic steel, Gradient plasticity, Unit cell model, Ductile-brittle transition

1 Introduction

Ferritic steels exhibit a ductile to brittle transition at low temperatures and/or high rates ofdeformation. The associated loss of toughness is critical in many engineering applications. Thebrittle behavior is related to transgranular cleavage of the ferrite [1]. It is well-known thatmicrostructural features of ferritic steel have a strong in�uence on fracture toughness. Thereare two main types of particles in ferritic steel at microscopic scale: non-metallic inclusions(manganese sul�des and oxides, which often have large sizes) and carbide particles (so-calledcarbides) [2]. In particular, the cementite particles (Fe3C) are a major factor for fracture of fer-ritic steel in the ductile-to-brittle transition regime. This applies especially to modern pressurevessel steels containing a reduced amount of sulfur so that the e�ect of MnS inclusions as failuresite (origin) is reduced [3]. Kroon, Faleskog and coauthors [4�6] proposed a micromechanics ap-proach in which an elastic-plastic constitutive law is used for the deformation of ferrite togetherwith a cohesive zone model for three failure mechanisms, namely cracking and debonding ofcarbide as well as for potential cleavage of the ferrite. A unit cell model with pre-cracked carbideembedded in the ferrite was employed. The major objective of their research was to investigatethe �bre-loading mechanism and the in�uence of stress triaxiality as well as plastic strain rate(i. e., indirectly related to the change of temperature) on micro-crack initiation. However, their

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model could not account for the local stress ampli�cations at grain boundaries due to a pile-upof dislocations, although it is known that this so-called strengthening mechanism is importantto initiate micro-cracks in ferritic steel [7]. The pile-up of dislocations can be described on thecontinuum mechanics level only with gradient plasticity theories. In the present study, the unitcell concept is adopted together with an e�ective gradient plasticity approach to investigate theinteraction between pile-ups of dislocations, at carbide-ferrite interface and grain boundaries,and the nucleation of cleavage micro-cracks.

2 Effective gradient plasticity

2.1 Formulation

Numerous gradient plasticity theories have been proposed in literature. Higher order theoriesfollow Mindlin's strain gradient theory in which higher order stresses are de�ned as the workconjugate of strain gradients in the energy potential [8�11]. For a review, refer to [12]. Higherorder theories are formulated within a thermodynamic framework and require additional bound-ary conditions. On the other hand, low order theories introduce gradient dependencies directlyinto the yield condition [13�16]. Consequently, low order theories do not require additionalboundary conditions. For that reason, they reduce the complexity compared to higher ordertheories. Low order strain gradient theories can be implemented in �nite element analysis withthe conventional framework of J2 plasticity.The e�ective plastic strain gradient was �rstly proposed by Aifantis [17]. In this model, the

second gradient of equivalent plastic strain εp was incorporated in the yield function. Thismodel is considered a special case of Fleck and Hutchinson's model [18], which is referred toas `explicit' gradient enhancement. In order to solve this problem in �nite element analysis,it requires C1 continuity [19]. Therefore, the implementation of this model in �nite elementanalysis is quite di�cult. To overcome this di�culty, Peerlings [20] proposed an `implicit'gradient formulation. It involves a non-local counterpart εp to the equivalent plastic strainεp together with the spatial gradient ∇εp. This model only requires C0 continuity. With itssingle additional nodal degree of freedom, it is attractive for the implementation into the �niteelement framework. The model involves a Mises-type yield function

f = σe − σf (1)

with a �ow stress σf = σy (εp) +3

2h (εp − εp)

and σe =

√3

2σ′ijσ

′ij , εp =

√2

3εpij ε

pij

together with the micro-force balance

εp − εp = `2∇2εp . (2)

Therein, σe is the von Mises equivalent stress and σy (εp) refers to the yield curve under homo-geneous deformations. As non-classical contribution, ` appears as an intrinsic material lengthscale in front of the Laplace operator ∇2. Furthermore, an additional parameter h is requiredwhich penalizes the di�erence between εp and εp. Equation (2) needs to be accompanied bysuitable boundary conditions. This can be a micro-hard boundary εp = 0 or a micro-free

boundary ~n · ∇εp = 0.

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2.2 Relation to dislocation densities

It is commonly assumed the �ow stress σf correlates to the densities of statistically storeddislocations (SSDs) and geometrically necessary dislocations (GNDs). SSDs are created in thelattice by trapping each other in random ways while the structure is imposed to homogeneousplastic deformation. The random patterns of SSDs are relevant under homogeneous plasticdeformations, whereas GNDs ensure compatibility under non-uniform plastic deformation, e. g.at grain boundaries. Both types of dislocations contribute to the strain hardening.Within the e�ective plastic strain gradient model under consideration, the densities ρS and

ρG of SSDs and GNDs are related to the equivalent plastic strain εp and its gradient ∇εp [21],respectively. The total density of dislocation amounts to ρT = ρS + ρG. Di�erent approacheshave been proposed for the individual contributions of ρG and ρS to the hardening. In thepresent study, the model by Abu Al-Rub and coauthors [22�25] is employed for the interpreta-tion of the �nite-element results with respect to dislocation densities in a post-processing step.The model is based on the critical �ow stress concept introduced by Columbus and Grujicic[26]:

σf =[σβS + σβG

]1/β. (3)

Therein, β is an interaction coe�cient. Furthermore, σG and σS are the �ow stresses associatedwith the densities ρG and ρS, respectively, which can be expressed through Taylor hardeninglaw as

σG = mαGb√ρG, σS = mαGb

√ρS (4)

wherein m is the Taylor factor, G is the shear modulus, b is the magnitude of the Burgersvector and α refers to an empirical coe�cient (α = 0.1 . . . 0.5) [25, 27, 28].Consequently, the �ow stress as a functions of the dislocation densities reads

σf = mαGb[ρβ/2S + ρ

β/2G

]1/β. (5)

This equation shows the contributions of the densities of SSDs and GNDs on the strain hard-ening. For β = 1, Eq. (5) has the same structure as Eq. (1)2 of the present gradient model,i. e. the �ow stress comprises two additive terms, associated with homogeneous (SSD) and in-homogeneous (GND) contributions. If both equations are evaluated �rstly for a uniform stateof deformation, i. e. ∇2εp = 0 (corresponding to εp = εp), and secondly for an non-uniformdeformation, the densities of both types of dislocations can be identi�ed as

ρS =

(σy(εp)

mαGb

)2

, ρG =

(h

G

`2∇2εp

mαb

)2

=

(h

G

εp − εp

mαb

)2

. (6)

Regarding the present model of gradient plasticity, the application of Eq. (6) is a post-processingstep whereby the product mαb acts as a scaling factor.

2.3 Numerical implementation

In the context of gradient-enriched damage models, Seupel et al. [29] pointed out that themicro-force balance (2) has the same structure as a stationary heat equation c∇2T + r = 0.

3

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𝜀𝜀pl = 0

H/2

H

Periodic constraints RF, U1

U1 = U2 = 0

Temp u1 = U

u1 = u2 = 0

H/2 y

x

a) b)

𝜀𝜀pl = 0

Figure 1: Simple shear of the in�nite layer with boundary conditions

Consequently, the implementation e�ort can be reduced drastically by using built-in thermo-mechanical elements in a thermomechanically coupled analysis of the commercial FEM codeAbaqus/Standard [30] if the temperature is identi�ed as T = εp. The heat capacity needs tobe chosen as c = `2. The heat source is set to r = εp − εp by means of the HETVAL usersubroutine. Finally, the e�ective yield stress σf in the yield condition, Eq. (1), needs to be setto σf = σy (εp) + 3

2 · h · (εp − εp) by means of the UHARD user subroutine which has access to

the temperature �eld T = εp. This user subroutine is provided as supplementary material.In the envisaged application, the crack propagation may become unstable which requires a

dynamic analysis. Unfortunately, Abaqus/Standard does not support inertia e�ects in ther-momechanically coupled analyses. In the modi�ed Newmark method, the inertia terms giverise to additional nodal forces (similar to d'Alembert forces). These dynamic nodal forces canbe added to a thermomechanically coupled analysis in Abaqus/standard as described in theAppendix.

2.4 Verification

In order to verify the implementation, the problem of simple shearing of a strip of height His used as a benchmark. The strip is assumed to have an in�nite length in x direction. Theboundary conditions are sketched in Figure 1. Note that micro-hard boundary conditions εp = 0are prescribed at the bottom and the top surface. Since the strip has in�nite length, both sidesof the �nite width layer W in the FE model are periodically constrained. In the veri�cationstep, the material of the layer is simply assumed to exhibit linear isotropic strain hardening

σy(εp) = σ0 + h εp (7)

wherein σ0 is the initial yield stress and h refers to the hardening modulus.Material properties are chosen as in [31]: σ0 = G/100, h = 20σ0, h = 2G/3. The ratio H/l

between height and intrinsic length is varied.Under simple shear loading, the solution of the boundary-value problem for the in�nite strip

can be found analytically by solving the ODE

d2εp

dy2− λ2 · εp +

√3σ12 − σ0

β= 0 with λ2 =

h

`2(h+ 3

2 h) (8)

for the non-local equivalent plastic strain. For micro-hard boundary conditions, the solution

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Γ εp/εy

y/H

b)

σ 12/τ 0

(a)

a) Γ εp/εy

y/H

σ 12/τ 0

(b)

Figure 2: Comparison of analytical solution and FEM solution: a) relation between stress andmean strain, b) distribution of equivalent plastic strain across the strip (normalizedto εy = σ0/E) at Γ = 0.0125

reads

εp =

√3σ12 − σ0

h

[1− cosh(yλ)

cosh(λH2 )

]. (9)

Consequently, the relation between shear stress σ12 (which is constant in the layer) and meanshearing Γ = U/H is obtained as

σ12 = G

(Γ +

√3σ0

h

[1.−

32 h

h+ 32 h

tanh(λH2 )λH2

])/

(1 +

3G

h

[1.−

32 h

h+ 32 h

tanh(λH2 )λH2

]). (10)

The analytical solution and FEM simulation of the shear stress σ12 (normalized with initialshear stress τ0 = σ0/

√3) and mean shear strain Γ are given in Figure 2a for di�erent ratios

of height to internal length scale H/`. The distribution of equivalent plastic strain acrossthe height of the layer is plotted in Figure 2b). In both �gures, the FEM solution coincidesobviously with the analytical solution so that the presented FEM implementation is veri�ed.

3 Micromechanical Model

3.1 Cell model

An axi-symmetric unit cell model under uni-axial macroscopic loading is adopted to investigatethe interaction between pile-ups of dislocations with the initiation of cleavage micro-cracks asshown schematically in Figure 3. The cell encompasses a spherical carbide particle embeddedinto two grains of ferrite. Potential fracture of the ferrite by cleavage or of the carbide and theinterface between both is modeled by cohesive zones. Cleavage of ferrite or of the carbide isassumed to appear only along the plane of symmetry z = 0. Therefore, only a quarter of thecell needs to be incorporated in the �nite element analysis. The dimensions of the cell modelare chosen as H0 = R0 = 7.45R (corresponding to a volume fraction of carbide Vp = 0.16%).A uniform vertical displacement Uz is applied at the top surface z = H0. The outer surfacer = R0 is assumed to remain cylindrical but without resulting radial loading, compare e. g.

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Cohesive zone model

Grain-1

z

RP

r

Uz

2R

Uz

Grain-2

2H0

2R0

Uz

Rg1

Carbide particle

Grain-1 Grain-2

Symmetric crack plane

Figure 3: Axi-symmetric unit cell model under uniaxial loading

[32]. Regarding the plasticity model, micro-free boundary conditions are applied at the outersurface of the unit cell. The in�uence of the respective jump conditions at the interfaces isinvestigated below in section 4.1.The load is applied quasi-statically, i. e., slow enough that inertia e�ects are negligible when

the cracks propagate stably. This means that the load is applied within a time τL which ismuch longer than the time τwave = R0/cR that the elastic waves need to pass the characteristicdistance R of the problem (cR is the velocity of the slower Rayleigh waves). In particular,τwave/τL = 0.001 is chosen in the simulations, using the same values of mass density for ferriteand carbide [4].Quadrilateral elements with bi-linear shape functions and reduced integration (CAX8RT in

the library of Abaqus) are used for the FEM simulations. The element size Le amounts toLe = 0.02R in the regions of the cohesive zones. For the employed parameter sets, this choiceensures that the element size remains comparable to the intrinsic length δ0 of the cohesive zoneLe ≤ 1.25δ0. The mesh is coarsened towards the upper parts of the cell model as shown inFigure 3.

3.2 Cohesive zone model

The cohesive zone model developed by Roth [33] is used for three types of potential failure(carbide cracking, debonding of carbide-ferrite interface and cleavage in the ferrite). Undermonotonous loading, the traction-separation relation follows an exponential curve

t = σcδ

δ0exp

(1− δ

δ0

). (11)

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t

σc

δ0

Γ0

δ

Dissipated energy

Exponential law

Figure 4: Traction-separation law of cohesive zone model

However, beyond the maximum transmittable stress at δ = δ0, called the cohesive strengthσc, the unloading path towards the origin deviates from Eq. (11). This behavior representsdissipation of energy during the separation process as illustrated in Figure 4. For the FEManalyses, the cohesive zone is implemented in Abaqus/Standard as a user-de�ned element viathe UEL subroutine [33].The two parameters of the cohesive law, i. e. the cohesive work of separation Γ0 and the

cohesive strength σc, are named corresponding to three types of modes of failure: Γ0M,Γ0P

and Γ0PM are the cohesive work of separation of ferritic matrix, carbide particle and for thedebonding of carbide-ferrite interface, respectively. Analogously, σcM, σcP and σcPM are thecohesive strengths of the ferritic matrix, carbide and carbide-ferrite interface, respectively.Actually, it is quite di�cult to de�ne exact values of these parameters. That is why the valuesΓ0PM= Γ0M and Γ0P = 0.5Γ0M from literature [4�6, 34, 35] are adopted here. The cohesivestrengths are chosen as σcP = σcPM ≤ σcM [35].Regarding the temperature dependence of the ferritic steel mentioned in [4, 5], it is well-

known that σc is hardly dependent on temperature. In contrast, the yield stress σ0 of theferrite increases with decreasing temperature [36]. Consequently, the ratio σc/σ0 increases withincreasing temperature and σc/σ0 decreases with decreasing temperature [37]. A parameterstudy is performed with respect to the ratio σc/σ0, which also implies indirectly the in�uenceof temperature on the fracture mechanism in the considered microstructure.

3.3 Material parameters

The isotropic hardening curve σy(εp) of the ferrite is given implicitly by

σy

σ0=

(σy

σ0+E

σ0εp

)N. (12)

Therein, E is Young's modulus and N is the hardening exponent. Such a relation gives rise toa power-law with respect to the total strain under uni-axial loading, compare e. g. [37].The penalty parameter of the e�ective plastic strain gradient is adopted from [19] as h = 10h0,

wherein h0 = NE1−N is the initial modulus of the power law hardening. The intrinsic material

length scale ` can be determined from indentation tests [7, 38]. The value of this quantity isassumed to lie in the µm range [39], i. e. of similar magnitude as the size of the carbide particles

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Table 1: Material properties for the cell model [4, 36, 40]

Material E/σ0 ν N `/R σc/σ0 Γ0/(σ0R)Ferrite (the matrix) 333 0.3 0.1 0. . . 0.8 1. . . 12 1.05

Carbide 666 0.3 - - 0.1. . . 12 0.525

Carbide-ferrite interface - - - - 0.1. . . 12 1.05

uz -0.75

Ez

Σ z/σ

0

σI/σ0

Grain 1

Grain 2 Grain 2

1

2

3

8.50

1.00

1.70

2.10 2.90

10.0

4

5

6.50

4.70

2.80

0.92

-0.98

1 2 3

5 4

Grain 1 Grain 2 Grain 2 Grain 1

0.20

Ez = 0.05

Ez = 0.05

(a)

u 0.75

E

/ /

Grain 1

Grain 2

Grain 2

1

2

3

8.50

.00

.70

.10 .90

10.0

4

5

6.50

4.70

2.80

0.92

-0.98

1 2 3

5 4

Grain 1 Grain 2 Grain 2 Grain 1

0.20

E = 0.05

E = 0.05

(b)

Figure 5: In�uence of micro-hard boundary condition on a) stress-strain curve and b) micro-scopic maximum principal stress before load drop at Ez = 0.05 (σcPM/σ0 = σcM/σ0 =4.0)

R. For dimensional reasons, the ratio `/R of both quantities is relevant for the plasticity-relatedsize-e�ect of the present model. The particular in�uence of the ratio `/R will be investigatedwithin a parameter study.The material properties used for the cell model are given in Tab. 1. Therein, the values of the

work of separation of a carbide particle, the interface and matrix, respectively, are normalizedto the carbide size R and the initial yield strength (i. e. Γ/(σ0R)).

4 Results and discussion

4.1 Influence of micro-hard boundary conditions, internal length scale and grain size

Firstly, the e�ect of the non-classical boundary and jump conditions of the scalar gradientplasticity theory shall be investigated. For this purpose, micro-hard conditions (εp|interface =0) are applied to the grain boundary (GB) or along the circumference of the particle (PB),respectively. Figure 5a shows the e�ective, macroscopic stress strain curves Σz−Ez of the unitcell simulations. Typical failure mechanisms and the distribution of the maximum principalstress σI are illustrated in Figure 5b. It can be seen that when micro-hard conditions are appliedneither at the particle circumference nor at the grain boundary (case 2©) or only at the particlecircumference (case 3©), the computed stress-strain curve does not exhibit signi�cant di�erencescompared to the simulations with classical plasticity (case 1©). Obviously, the dislocation pile-up at the particle is hardly relevant to the macroscopic strain hardening. However, if themicro-hard condition is applied only at the grain boundary (case 4©), strain hardening increases

8

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uz

-0.75

Ez

Σ z/σ

0

σI/σ0

Grain 1

Grain 2

Grain 2

1 2 3

0.45

1.00 1.70

2.10 2.90 11.0

4 5

1

2

3

2

4

5

6

1

3 4

5 6

11.0 9.60 7.90 6.20 4.50 2.80 -0.20

(a)

u

0.75

E

/

/

Grain 1

Grain 2

Grain 2

1 2 3

0.45

1.00

.70

.10

.90 11.0

4 5

1

2

3

2

4

5

6

1

3 4

5 6

11.0

9.60

7.90

6.20

4.50

2.80

-0.20

(b)

Figure 6: In�uence of plasticity model and internal length scale ` relative to particle radius R

signi�cantly until a micro-crack initiates at the grain boundary. When the micro-crack reachesthe particle-matrix interface, it triggers debonding of the particle from the matrix. In the lastcase (case 5©), micro-hard conditions are applied to both the grain boundary and to the particleinterface. In this case, the particle breaks after the initial micro-crack arrives at the particle-matrix interface. The stress-strain curves are similar for both cases (case 4© and case 5©), butthe micro-crack mechanisms in the cell model are signi�cantly di�erent. In following sections,micro-hard conditions are applied on both, the grain boundary and the particle circumference,for all simulations.The intrinsic length scale parameter ` can be considered as a bridge between plasticity at

micro-scale and plasticity at macro-scale. The gradient e�ects vanish and the conventionalplasticity theory is recovered if the characteristic length is set equal to zero ` = 0. Figure 6illustrates the e�ect of the gradient plasticity compared with the conventional plasticity theory.It shows that the incorporation of gradient e�ects, i. e. non-vanishing values of `/R, inducesa higher initial hardening which leads to initiation of cleavage at lower levels of macroscopicstrain Ez. For large values `/R ≥ 0.6, i. e., for small carbides R or a low density of dislocations,the initiation of cleavage leads immediately to a complete failure and the macroscopic stressΣz drops to zero. However, for lower values of `/R, the cleavage microcrack can be arrested.For a smaller value `/R = 0.2, even three distinct stages are observed: Firstly, maximumprincipal stress concentrates at the grain boundary due to dislocation pile-up (stage 1©). Whenthe principal stress exceeds cohesive strength σcM of the matrix, a micro-crack initiates at thegrain boundary (stage 2©). Subsequently, the crack grows into both grains. The dissipation dueto the plastic deformations at the tips of the growing microcrack leads to a limited macroscopichardening (stage 3©). When the microcrack arrives at the carbide, the latter debonds and themacroscopic stress drops again (stage 4©). Further loading is necessary to drive the right tip ofthe microcrack through the elastic-plastic second grain (stage 5©). Finally, the crack propagatesdynamically through the ligament of the second, carbide-free grain until complete separationof the material occurs (stage 6©).A real material contains a population of carbides of di�erent size. The intrinsic length ` is a

characteristic of micro-plastic deformation, i. e. dislocation processes in the ferritic matrix, andtherefore considered a constant property. Then, Figure 6 indicates that cleavage will initiatenear the largest carbides, since initiation there requires the lowest level of the macroscopic

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uz

cracks arrested

Ez

Σ z/σ

0

Grain 2

Grain 2

Grain 1 Grain 2 σI/σ0

9.80 8.92

-1.52 0.39 1.34

7.03

1

3

5.13 3.30 4

1 2

2

3 4

(a)

u

cracks arrested

E

/

Grain 2

Grain 2

Grain 1 Grain 2

/ 9.80 8.92

-1.52

0.39

1.34

7.03

1

3

5.13

3.30 4

1 2

2

3 4

(b)

Figure 7: In�uence of the distance of the carbide to the grain boundary

stress Σz. Furthermore, it shows that the cleavage micro-crack initiated thereby can arrest.This prediction is in agreement with experiments [1, 3, 41].For a given total volume fraction of carbides, the microstructure can di�er with respect to

the distanceRg1 − R of the carbide to the next grain boundary, compare Figure 3. In orderto investigate this in�uence, the ratio Rg1/R is varied. In this context it has to be remarkedthat the ratio Rg1/R determines also the volume fraction of the carbide within the respectivegrain and that distance of the carbide to the grain boundary and its volume fraction in thegrain cannot be varied independently in the present axi-symmetric model. The simulationresults in Figure 7 show that the macroscopic strength, the hardening behavior as well as thecrack arrest capability depend strongly on Rg1/R, i. e., on the distance of the carbide to thegrain boundary. In particular, a lower ratio Rg1/R leads to a lower strength, but requires alarger amount of dissipation for driving the micro-crack. Furthermore, the microscopic failuremechanism depends on Rg1/R: if the carbide is located close to the grain boundary Rg1/R =2.5, the particle breaks before cleavage initiates in the matrix. This prediction complies withthe experimental �nding that carbides close to or at a grain boundary are prone to initiatecleavage. The transition point with respect to Rg1/R between micro-crack initiation in thecarbide and in the matrix depends on the strength of particle and matrix (not shown here).In following sections, the internal length and the the size of the grain with carbide are chosen

at intermediate levels `/R = 0.4 and Rg1/R = 3.75, respectively.

4.2 Influence of cohesive strength on micro-crack mechanisms

The in�uences of the strengths of the particle-matrix interface σcPM and of the matrix σcM

shall be investigated by means of sensitivity studies. The (normalized) strength of the particle-matrix interface σcPM/σ0 is varied in the range of 0.1 . . . 12 and that of ferrite σcM/σ0 in therange of 1 . . . 12, respectively. It is recalled that σcM/σ0 varies with temperature as discussedin Section 3.2, whereas the direct experimental determination of σcPM is rather di�cult.Firstly, the strength of the matrix is maintained constant at σcM/σ0 = 4.0 and the strength of

the particle-matrix interface σcPM/σ0 is varied. Corresponding macroscopic stress-strain curvesare plotted in Figure 8. Again, three stages are observed: 1© a micro-crack originates at thegrain boundary due to high stress concentration induced by dislocation pile-up; 2© the micro-

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uz

cracks arrested

Ez

Σ z/σ

0

Grain 1

1.06

Grain 2

Grain 2 1

2

3

Grain 1 Grain 2

σI/σ0 8.50

-0.45

2.60

5.60

4.06

7.05

1

3

2

2 1 3

σcPM/σ0=2.0

σcPM/σ0=6.0

σcPM/σ0=8.0

3 3

3

(a)

u

cracks arrested

E

/

Grain 1

1.06

Grain 2

Grain 2 1

2

3

Grain 1 Grain 2

/ 8.50

-0.45

2.60

5.60

4.06

7.05

1

3

2

2 1 3

/ 2.0

/ 6.0

/ 8.0

3 3

3

(b)

Figure 8: In�uence of interfacial strength: a) macroscopic stress-strain curve and b) microscopicmaximum principal stress at stage 3© (Ez = 0.06)

uz

cracks arrested

Ez

Σ z/σ

0

Grain 1

1.05

Grain 2

Grain 2 1

2

3

Grain 1 Grain 2

σI/σ0 14.3

-0.75

2.00

3.80

2.90

4.70 1

3

2

2

3

3

σcM/σ0=2.0

σcM/σ0=4.0

σcM/σ0=8.0

0.15

3

3

(a)

u

cracks arrested

E

/

Grain 1

1.05

Grain 2

Grain 2 1

2

3

Grain 1 Grain 2

/ 14.3

-0.75

2.00

3.80

2.90

4.70 1

3

2

2

3

3

/ 2.0

/ 4.0

/ 8.0

0.15

3

3

(b)

Figure 9: In�uence of the strength of the ferritic matrix: a) macroscopic stress-strain curve andb) microscopic maximum principal stress at Ez = 0.06 (σcPM/σ0 = 4.0)

crack grows and arrives at the particle-matrix interface. Subsequently, the carbide-particle isbroken or debonded, which leads to softening of the cell structure and �nally 3© the micro-crackcompletely propagates through the second grain.For a low strength of the interface σcPM/σ0 ≤ 6.0, the particle debonds once the microcrack

reaches the interface. In contrast, for a high interface strength σcPM/σ0 > 6.0, the microcrackpropagates straight through the particle. However, the diagram at the left-hand side of Figure 8shows that this switch in the mechanism has no signi�cant in�uence on the macroscopic stress-strain curve.In contrast, Figure 9 shows that the strength σcM (relative to the yield stress σ0) of the

ferritic matrix has a very strong in�uence on the macroscopic stress-strain behaviour. Highvalues of σcM/σ0, i. e., a higher temperature, lead to a later initiation of cleavage and thus to amore ductile behaviour. In contrast, less energy can be dissipated for low values σcM/σ0, i. e.at low temperatures. For σcM/σ0 = 1.0, even no crack arrest stage can be identi�ed anymore.Similar tendencies are observed for weak particle interfaces σcPM/σ0 = 0.1 for which the

11

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uz

class. plasticity

Ez

Σ z/σ

0

Grain 1 22.0

Grain 2

Grain 2 1

2

3

3

Grain 1 Grain 2

σI/σ0 14.0 12.0

-0.58

0.5

3.0

10.0

2 1

1

1

2

8.0

5.0 3 4

5

3 4

5

(a)

u

class. plasticity

E

/

Grain 1 22.0

Grain 2

Grain 2 1

2

3

3

Grain 1 Grain 2

/

14.0 12.0

-0.58

0.5

3.0

10.0

2 1

1

1

2

8.0

5.0 3 4

5

3 4

5

(b)

Figure 10: In�uence of strength of matrix for weak particles σcPM/σ0 = 0.1

uz

cracks arrested

Ez

Σ z/σ

0

Grain 1 22.0

Grain 2

Grain 2 1

2

3

3

Grain 1 Grain 2

σI/σ0 24.0 10.0

-1.0

0.5

2.5

8.0

1

1

2

6.0

4.5

3 4

5

1 2

31 32

4 5

(a)

u

cracks arrested

E

/

Grain 1

22.0

Grain 2

Grain 2 1

2

3

3

Grain 1 Grain 2

/

24.0

10.0

-1.0

0.5

2.5

8.0

1

1

2

6.0

4.5

3 4

5

1 2

31 32

4 5

(b)

Figure 11: In�uence of strength of matrix for strong particles σcPM/σ0 = 12.0

particles debond, see Figure 10. This �gures contains also the case of classical plasticity forwhich no initiation of cleavage is obtained at all in the considered range of uni-axial loading,even at a relatively low cleavage strength of the matrix σcM/σ0 = 2.0.Finally, Figure 11 illustrates the e�ect of the strength of the matrix for a very strong particle-

matrix interface σcPM/σ0 = 12.0. Microscopically, the high strength of the interface leads to achange of the mechanism from debonding to breakage of the particle. However, a comparisonof the macroscopic stress-strain curves to those with an intermediate strength of the interfacein Figure 9 does not indicate a signi�cant di�erence.Independent of the particular choice of the strength σcPM of the interface, it can be concluded

that much higher values of the strength σcM of the ferritic matrix can be used with the gradienttheory than with conventional theory. Such higher values are more realistic since they lie closerto the theoretical strength σth

cM ≈ E/10 of the material. The remaining di�erence between σcM

and σthcM might be attributed to the fact that anisotropy, both of elasticity and plasticity, are

not taken into account in the present model.

12

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4.3 Distribution of dislocation densities

The relationship between dislocation densities and e�ective plastic strain and its gradient isgiven in Eq. (6). The material parameters for the ferritic matrix are chosen as in [15, 27, 28, 42�44]: Taylor's factor m is taken as m = 2.75 (corresponding to BCC polycrystalline metals),Burgers vector is chosen as b = 0.248 nm and the empirical coe�cient amounts to α = 0.3.Figure 12 shows the evolution of the densities of SSDs and GNDs for the case of intermedi-

ate strengths σcPM/σ0 = 4.0 and σcM/σ0 = 4.0 with material length scale `/R = 0.2, whosestress-strain curve with respective markings 1©� 6© was shown in Figure 6. During the propa-gation of the micro-crack, the macroscopic stress recovers two times (stage 3© and stage 5©).This behaviour is explained by the evolution of SSDs in the cell model. The SSD density in-creases with increasing e�ective plastic strain at the crack tips, which leads to enhanced strainhardening. For a weak interface, the SSD density around the crack tip is smaller compared tothat of a strong interface. Therefore, the strain hardening increases gradually, in contrast to astrong interface. Vice versa, the maximum principal stress reaches the strength of the ferrite(the matrix) slower than with the strong interface. Consequently, the micro-crack mechanismis quasi-brittle for the model with the strong interface.According to [28, 45], the GND density ρG at grain boundaries in metallic alloys lies in

the range of 1015 . . . 1018 m−2. Furthermore, ρG often exceeds the SSD density ρS by oneor two orders of magnitude. Both aspects are reproduced realistically by the simulations,see Figure 12b. At elevate position on the strain hardening curve (stage 1©), high values ofGND density are concentrated at the grain boundary indicating a dislocation pile-up. Theassociated high local stresses reach the strength σcM of the ferritic matrix thus triggering theinitiation of a micro-crack. The crack grows dynamically but arrests (stage 2©). Notice thatGND density still accumulates with ongoing loading. Therefore, when the crack arrives at theparticle-matrix interface, both GNDs and SSDs at the crack tip contribute to the recoveryof strain hardening (stage 3©). Subsequently, the microcrack from the particle coalesces withthe cleavage microcrack of the matrix (stage 4©). The propagation of the micro-crack and theassociated local stress relief cause a redistribution of GNDs at the �anks of the micro-crack. Thedensity of SSDs at the crack tip in the second grain increases since further plastic deformationsare necessary to drive the crack stably through the outer grain 2 until it cleaves completely.This event �nally induces the drop in the stress-strain curve (stage 5©).

5 Summary and conclusions

In the present study, an axi-symmetric cell model was employed to study qualitatively theinteraction of dislocation pile-up with cleavage initiation at carbide particles and at grainboundaries in ferritic steels. The plastic behaviour of the ferritic matrix was described bya higher-order theory of plasticity which incorporates the gradient of the equivalent plasticstrain. Despite its isotropic behaviour, such a theory can describe the dislocation pile-up atlarge-angle grain boundaries if micro-hard jump conditions are utilized there. The performedsimulations show that this dislocation pile-up leads to considerably increased local stresseswhich trigger initiation of cleavage of the ferrite. Both, potential cleavage as well as breakageor debonding of carbide particles were modelled by a cohesive zone.Systematic parameter studies were performed with respect to the in�uence of the strengths

of ferrite, carbide and their interface as well as with respect to the size of the carbide relative tothe intrinsic length ` of the gradient model. The parameter studies showed that the strength of

13

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uz -0.75 Ez

Σ z/σ

0

Grain 1

Grain 2

Grain 2

1 2 3

0.45

1.00 1.70

2.10 2.90 11.0

4 5

1 3 2

4 5

6

2.70

2.50

2.33

2.15 1.97

1.80 1.60

ρS[m−2]x1014 1 2 3

4 5 6

(a)

uz -0.75 Ez Σ z/σ

0

Grain 2 1 2 3

0.45

1.00 1.70

2.10 2.90 11.0

4 5

1 3 2 4

5

6

4.58

3.78

2.98

2.18 1.38

0.58 0.0

ρG[m−2]x1016

Grain 1 Grain 2

1 2 3

4 5 6

(b)

Figure 12: Evolution of dislocation densities: (a) SSDs, (b) GNDs

14

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the carbide has an in�uence on the microscopic path of crack propagation, which is, however,hardly correlated to the macroscopic stress-strain behaviour. In contrast, the ratio σcM/σ0 ofcleavage strength of ferrite to its yield stress has a strong in�uence on the macroscopic duc-tility. This ratio is directly correlated to the temperature. Considerably higher values of thecleavage strength σcM > 10σ0 could be realized in the gradient-enriched model than in modelswith conventional plasticity leading to more realistic micro-structural failure mechanisms. Theintrinsic length of the gradient theory is related to the mean free path of dislocations. Theratio of intrinsic length to the carbide size, as well as the size of the grain the carbide is em-bedded in, were found to have a strong e�ect on the macroscopic strain hardening behaviourand on potential arrest of microcracks which were nucleated at grain boundaries. These mech-anisms cannot be simulated within the conventional theory of plasticity. Thus, the gradientenhancement and the formulation of suitable jump conditions at grain boundaries are essentialto micro-mechanical modelling of the ductile-brittle transition of ferritic steels.Future quantitative studies must determine the intrinsic length `, and the penalty parameter

h, from suitable experiments like indentation tests for a particular steel. Furthermore, theemployed axi-symmetric cell model required that the carbide be located within the ferrite grain.Future 3D simulations are needed to address carbide particles located at grain boundaries.

Acknowledgements

The �nancial support by the Deutsche Forschungsgemeinschaft (German Research Foundation)under contract HU 2279-1 is gratefully acknowledged. The authors thank Stephan Roth forproviding the implementation of the cohesive element for Abaqus.

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Supplementary material

Source code of implementation of gradient plasticity in Abaqus.

Appendix: Implementation of the modified Newmark method

In the modi�ed Newmark method, the vectors of nodal accelerations and velocity, a and v,respectively, are integrated within one time increment ∆t = tm+1 − tm as

vm+1 = vm + ∆t[(1− γ)am + γam+1

], (13)

um+1 = um + ∆tvm +(∆t)2

2

[(1− 2β)am + 2βam+1

], (14)

cf. e. g. [46]. These equations can be solved for the updated accelerations

am+1 =1

β(∆t)2(um+1 − um)− 1

β∆tvm − 1− 2β

2βam . (15)

The acceleration vector can be inserted to the discretised equations of motion 0 = M · am+1 +

Fm+1int − Fm+1

ext yielding 0 = Fm+1int − Fm+1

ext with an equivalent vector of internal nodal forces

Fm+1int = Fm+1

int + M ·[

1

β(∆t)2(um+1 − um)− 1

β∆tvm − 1− 2β

2βam]. (16)

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In order to extend a static FEM program towards dynamic problems, thus, the following stepsare necessary:

1. The nodal values vm and am of velocity and acceleration, respectively, from the last timeincrement need to be stored.

2. The mass matrix M needs to be computed.

3. The additional contribution of the inertia terms to the nodal forces in Eq. (16) needsto be incorporated as well as the corresponding term 1

β(∆t)2M to the sti�ness matrix

∂Fm+1int /∂um+1.

These steps can �rst be performed individually for each element without changes to the globalFEM program and secondly without knowledge of the internal nodal forces Fm+1

int .We implemented the procedure in Abaqus/Standard as user-de�ned elements via the UEL

interface. Such a user-de�ned element needs to be super-imposed to each thermomechanicalbuilt-in element of Abaqus. The user-de�ned element needs to reserve space for the nodalquantities vm and am, respectively, in form of �solution-dependent variables� (SDVs). Secondly,it computes the updated accelerations and velocities by Eqs. (13) and (15) based on the currentestimate um+1 for the nodal displacement. Subsequently, the element mass matrix is computedwhich is required for the user-de�ned element to compute the inertia terms, i. e. the secondterm on the right-hand side of Eq. (16). Finally, the user-de�ned element returns this elementcontribution to the nodal forces and the respective contribution to the sti�ness matrix to theglobal program.This methodology can be used with any built-in element of Abaqus. It is only required

that the same element topology and shape functions are used in the superimposed user-de�nedelements. For the present study, values β = 1/2 and γ = 1 are used for the Newmark parameterscorresponding to an Euler-backward scheme.

19