Abstract

A thermodynamic model for nanocrystalline interstitial alloys is presented. The equilibrium solid solubility of carbon in 𝛼-iron is calculated for given grain size. Inside the strained nanograins local variation of the carbon content is predicted. Due to the nonlinear relation between strain and solubility, the averaged solubility in the grain interior increases with decreasing grain size. The majority of the global solubility enhancement is due to grain boundary enrichment however. Therefore the size effect on carbon solubility in nanocrystalline 𝛼-iron scales with the inverse grain size.

1. Introduction

An enhancement of solid solubility has been found in many bulk nanocrystalline materials, for instance [1, 2]. Often the bigger part of the effect can be attributed to nonequilibrium processing such as mechanical alloying [3]. However quantifying the impact of grain refinement on equilibrium solid solubility is important for understanding the behavior of nanocrystalline alloys upon thermal activation. In this context equilibrium shall be constrained by the assumption of a stable grain size.

The scope of this work is to develop a thermodynamic model of nanocrystalline alloys. It has to comprise both the nanoscale grains and the grain boundary regions, since the fraction of atoms located in those cannot be neglected. The description is based upon the previously published thermodynamic treatment of alloy grain boundaries [4]. There the grain boundaries are approximated by a uniformly dilated lattice retaining the symmetry of the bulk material [5, 6] and are characterized by their volumetric strain Δ𝑉/𝑉0.

The interstitial solution of carbon in 𝛼-iron is chosen as an alloy of practical relevance and experimental accessibility. In pure iron the nanocrystalline state is retained even after prolonged annealing at 650 K [7]. At this temperature and a time of 3600 s, the diffusion length of carbon in bulk iron exceeds 50 μm [8]. Since the carbon diffusivity will be larger in nanocrystalline iron, this enables chemical equilibration without strong grain growth.

2. Thermodynamic Model of Nanocrystalline Fe-C

The thermodynamic description of a binary Fe-C alloy under volumetric strain is based upon Kaufman and Schlosser's expression [9] for the Helmholtz free energy 𝐹. The free energy of the strained solid consists of 𝐹∘ at zero pressure and a second term that accounts for the elastic energy depending on the parameter πœ’=(𝑉/𝑉0)1/3 using the Vinet et al. universal equation of state [10]. The isothermal bulk modulus 𝐡0, the molar volume 𝑉0, and the anharmonicity parameter πœ‚0 are given at zero pressure: 𝐹=𝐹∘+9𝐡0𝑉0πœ‚20πœ‚ξ€Ίξ€½0𝑒(1βˆ’πœ’)βˆ’1πœ‚0(1βˆ’πœ’)ξ€».+1(1) A two-sublattice model Fe(Va,C)3 is used to describe the interstitial solution of carbon in 𝛼-iron. In the second sublattice carbon substitutes normally vacant octahedral sites. Here 𝑦C marks the molar fraction of carbon in the sublattice. Its relation to the carbon content given as the molar fraction π‘₯C is 𝑦C=π‘₯C/(3(1βˆ’π‘₯C)). Conveniently choosing pure 𝛼-iron and graphite as the reference state, the molar free energy 𝐹∘ of the unstrained alloy is stated by [11] in units of Joule where 𝑇 is the temperature in Kelvin: 𝐹∘=(322050+75.667𝑇)𝑦C𝑦+3𝑅𝑇Cln𝑦C+ξ€·1βˆ’π‘¦Cξ€Έξ€·ln1βˆ’π‘¦Cξ€·ξ€Έξ€Έβˆ’190𝑇1βˆ’π‘¦C𝑦C.(2) Assuming a dilute alloy, 𝐡0 and πœ‚0 of pure 𝛼-iron are used in (1). Values of 𝐡0=178.6GPa, 𝑉0=7.09β‹…10βˆ’6m3/mol [12], and πœ‚0=5.16 [13] at 𝑇=298K are employed. Their temperature dependence is calculated according to Vinet and coworkers [10] using the coefficient of volumetric thermal expansion 𝛼0=36.9β‹…10βˆ’6Kβˆ’1 [12]. At low solute concentration the molar volume 𝑉0 of the alloy varies linearly with π‘₯C, and πœ’=3ξƒŽ1+Δ𝑉/𝑉01+π‘₯CΞ©CFe,bcc(3) is obtained. The volume size factor of carbon in 𝛼-iron Ξ©CFe,bcc=0.825 is averaged from two publications [14, 15]. The equilibrium between carbon in strained 𝛼-iron and the reference state graphite is given by 𝐹+(1βˆ’π‘₯C)β‹…(πœ•πΉ/πœ•π‘₯C)=0.

The strain of the crystallite interior is calculated using WeissmΓΌller's model [16]. Accordingly local strain in bulk nanocrystalline materials is caused by the fact that the cavities defined by the adjacent grains need to accommodate a finite number of lattice planes. The maximum linear strain πœ€max is given by the interatomic distance π‘ŸNN (for iron π‘ŸNN=0.252nm [12]) and the grain size 𝐷: ||πœ€max||=14ξ‚™32π‘ŸNN𝐷.(4) The predicted root mean square strain is in good agreement with strain measured in nc-Fe by X-ray diffraction [17, 18]. Here the mean strain βŸ¨πœ€βŸ©π‘‰=βˆ’2βŸ¨π‘“βŸ©π΄/(3𝐡0𝐷) is neglected, because with a grain-boundary stress βŸ¨π‘“βŸ©π΄ of 1.1 N/m [19] it is more than a magnitude of order smaller than |πœ€max|. The volumetric strain is given by the superposition of the linear strain in three dimensions Δ𝑉/𝑉0β‰…πœ€π‘₯+πœ€π‘¦+πœ€π‘§.

Furthermore a thickness 𝑀 of 0.7 nm representing 3-4 monolayers and a value of Δ𝑉/𝑉0=0.12 is used to describe average grain boundaries. This choice of parameters yields a good agreement with an experimental value of the interface free energy of 468mJ/m2 at 1723 K [20].

Finally the resulting global solubility π‘₯Cglobal is calculated from the grain boundary and interior compositions with their respective molar fractions as weighting factors: π‘₯Cglobal=𝑓π‘₯CGB+(1βˆ’π‘“)π‘₯Cinterior,(5)𝑓=(𝐷+𝑀)3βˆ’π·3(𝐷+𝑀)3+𝐷3Δ𝑉/𝑉0ξ€Έ.(6) The molar fraction of the atoms located in grain boundaries 𝑓 is corrected for the different atomic densities and converges for Δ𝑉/𝑉0=0 and large grain sizes toward 3𝑀/𝐷.

3. Results and Discussion

Recently ab initio methods based on density-functional theory (DFT) allow for highly accurate simulation of carbon solution in 𝛼-iron. The excess enthalpy of carbon in iron as defined by [21] depending on volumetric strain was calculated at 𝑇=0𝐾 and infinite carbon dilution. The result is presented in Figure 1. Good agreement with the strain dependence of excess enthalpies computed by DFT and a modified embedded-atom method (MEAM) is observed. The calculated derivative of the excess enthalpy with respect to the atomic volume at Ξ”V/𝑉0=0 is βˆ’0.95eV/Γ…3 as compared to βˆ’1.08eV/Γ…3 (DFT) and βˆ’0.84eV/Γ…3(MEAM).

The maximum linear strain of the grain interior given by (4) can be used to calculate the local volumetric strain assuming three independent axes. For a grain size of 20 nm the linear strain varies locally between βˆ’3.8β‹…10βˆ’3 and +3.8β‹…10βˆ’3 and the volumetric strain between βˆ’0.011 and +0.011 with the frequency distribution shown in Figure 2. Close to Δ𝑉/𝑉0=0 the calculated carbon concentration in equilibrium with graphite at 673 K coincides with the linear theory of thermochemical equilibrium of solids under stress [22]. For large strains nonlinear behavior is observed. At lower values of Δ𝑉/𝑉0 indicating strong compression, the carbon concentration converges towards zero, which is the physically reasonable behavior.

The expected variation in composition between individual nanograins can be deduced from the range of values calculated for π‘₯Cinterior. For a grain size of 20 nm the ratio between the maximum (9.8β‹…10βˆ’4at.%) and the minimum carbon concentration (1.7β‹…10βˆ’5at.%) is 59. This ratio will be even larger for smaller grain sizes. Another notable consequence of the nonlinear trend of π‘₯Cinterior is that weighted averaging yields a deviation from bulk solubility despite the strain distribution symmetry. Figure 3 shows the average carbon solubility in the grain interior as a function of inverse grain size. It increases with decreasing grain size slightly. π‘₯Cinterior is doubled with respect to the bulk solubility for 11 nm grains.

The carbon concentration in grain boundaries was calculated in equilibrium with graphite assuming it to be independent of curvature and grain size. At a temperature of 673 K the computed value of π‘₯CGB is 3.9at.%. This means that carbon is enriched by a factor of 3β‹…104 in the grain boundaries with respect to the bulk. Atom probe microscopy measurements confirm the presence of a minimum of 2 at.% carbon in 𝛼-iron grain boundaries [23]. Other experiments at 873 K [24, 25] yielded higher values, expressed as excess densities of carbon at the interface of Ξ“CGBβ‰ˆ20 μmol/m2. The corresponding theoretical prediction is lower at Ξ“CGB=5 μmol/m2. The difference may be explained by the strong variation between individual grain boundaries and the information depth of the analytical methods employed. In the case of autoradiography it exceeds the grain boundary thickness of approximately 1 nm by far. The detected amount is likely to include carbon enriched at stress fields around grain boundaries as well. Then the concentration in the grain boundary core is lower than Ξ“CGB suggests.

Calculating the global solubility according to (5) yields an almost linear relation with the inverse grain size as Figure 3 illustrates. The reason is that the contribution of enriched grain boundaries dominates the size effect. Figure 4 shows the calculated solubility of carbon in nanocrystalline 𝛼-iron of various grain sizes. Thereafter a pronounced increase in equilibrium carbon solubility is to be expected in nanocrystalline iron in comparison to bulk iron.

4. Conclusions

A thermodynamic model for nanocrystalline 𝛼-phase Fe-C alloys has been presented. Considering the strained grain interior in equilibrium with graphite local variation of the carbon concentration but only a weak size effect on the average carbon solubility is found. While the extent of enrichment at grain boundaries is not precisely established, grain boundary segregation dominates the solubility increase in the nanocrystalline state. It is concluded that the excess carbon solubility in nanocrystalline iron over bulk iron is proportional to the inverse grain size. At a given temperature the overall solubility follows π‘₯Cglobalβ‰ˆπ‘₯Cbulk+const𝐷.(7)

Acknowledgments

The research of A. Kirchner was supported by Deutsche Forschungsgemeinschaft via the Emmy Noether Programme.