J.
de Boor‡
*a,
S.
Gupta‡
a,
H.
Kolb
a,
T.
Dasgupta
b and
E.
Müller
ac
aInstitute of Materials Research, German Aerospace Center, Linder Höhe, 51147 Köln, Germany. E-mail: Johannes.deboor@dlr.de
bDepartment of Metallurgical Engineering and Materials Science, Indian Institute of Technology Bombay, Mumbai 400076, India
cInstitute for Inorganic and Analytical Chemistry, Justus-Liebig-Universität Gießen, Heinrich-Buff-Ring 58, 35392 Gießen, Germany
First published on 9th July 2015
Solid solutions of magnesium silicide and magnesium stannide exhibit excellent thermoelectric properties due to favorable electronic band structures and reduced thermal conductivity compared to the binary compounds. We have optimized the composition Mg2Si0.8Sn0.2 by Sb doping and obtained a thermoelectric figure of merit close to unity. The material comprises of several phases and exhibits intrinsic nanostructuring. Nevertheless, the main features of electronic transport can be understood within the framework of a single parabolic band model. Compared to Mg2Si we observe a comparable power factor, a drastically reduced thermal conductivity and an increased effective mass.
So far, most of the research studies are dedicated either to pure Mg2Si due to its simplicity and the relatively high thermal stability or to Sn-rich compositions similar to Mg2Si0.4Sn0.6. The latter composition exhibits a crossing of the Si and Sn sub-bands, which increases the band degeneracy and therefore drastically increases the effective mass of the electrons.4,5,10 Furthermore, the thermal conductivity is reduced compared to the binary compositions due to additional alloy scattering. There are only a few reports on the Si-rich side of the Mg2(Si,Sn) family. Tani et al. optimized the carrier concentration for Mg2Si1−xSnx for x = 0.05 and 0.1, reaching a ZTmax of 0.68 at 864 K.11 Liu et al. and Samunin et al. reported some transport data for x = 0.2 and showed a maximum ZT of around 0.8, but did not present a conclusive optimization with respect to the carrier concentration.5,12
However, investigation and optimization of Si-rich Mg2(Si,Sn), in particular Mg2Si0.8Sn0.2, is very interesting both from a fundamental and an applied point of view. Mg2Si0.8Sn0.2 has a significantly lower density than Mg2Si0.4Sn0.6 (2.3 g cm−3 < 3 g cm−3), i.e. for applications where weight is a crucial factor, it might be the optimal choice, even with inferior thermoelectric performance. Moreover, as Mg2Si is thermally and chemically more stable than Mg2Sn it is plausible that Si-rich compositions are more stable than Sn-rich compositions, allowing operation at higher temperatures. Furthermore, Mg2Si0.8Sn0.2 is closer to the technologically more developed Mg2Si, where progress in contact development has been reported.13,14 On the other hand, compared to Mg2Si an improvement of the thermoelectric properties can be expected due to increased phonon alloy scattering.
Beyond this, the composition Mg2Si0.8Sn0.2 is also very interesting with respect to fundamental aspects. According to the literature reports, there is a miscibility gap between Mg2Si and Mg2Sn whose exact borders are disputed.4,15–17 According to ref. 16, Mg2Si0.8Sn0.2 is within the miscibility gap. This provides the chance for an intrinsic nanostructure within the material, decreasing the thermal conductivity and thus enhancing the thermoelectric performance. This strategy has successfully been employed, e.g. for the PbTe family and half-Heuslers.18,19 Modeling of the Mg2(Si,Sn) family is important for a thorough understanding and further optimization. This modeling is often performed using a linear interpolation between Mg2Si and Mg2Sn for parameters like band gaps or interaction potentials.4,20,21 These theoretical assumptions have to be validated by experimental results.
In this work, we have therefore studied the microstructure and the thermoelectric properties of Mg2Si0.8Sn0.2. We demonstrate charge carrier density optimization by means of Sb doping. High temperature measurements of the electrical and thermal conductivity, Seebeck coefficient as well as Hall carrier density and mobility reveal that the electronic properties can be modelled reasonably well in the framework of a single parabolic band model. The experimental and the modeling results provide fundamental transport parameters like the effective mass, carrier mobility and interaction potentials. Additionally, we compare our results with data from the binary compound Mg2Si and provide insights into the effect of Si/Sn substitution on the electronic band structure.
Nominal composition | ρ geo [g cm−3] | ρ A [g cm−3] | x from ρA | x from XRD | |
---|---|---|---|---|---|
Mg2Si0.8Sn0.2 | #1 | 2.17 | 2.21 | 0.132 | 0.128 |
Mg2Si0.795Sn0.2Sb0.005 | #2 | 2.25 | 2.24 | 0.145 | 0.140 |
Mg2Si0.79Sn0.2Sb0.01 | #3 | 2.12 | 2.21 | 0.128 | 0.117 |
Mg2Si0.785Sn0.2Sb0.015 | #4 | 2.33 | 2.31 | 0.174 | 0.170 |
Mg2Si0.78Sn0.2Sb0.02 | #5 | 2.29 | 2.31 | 0.168 | 0.170 |
Fig. 1 shows the XRD results. All major peaks can be indexed according to the reported anti-fluorite structures (space group Fmm) of Mg2Si and Mg2Sn. The minor peak at 2θ ≈ 43° corresponds to MgO, an impurity often observed in this material class.28 The zoom-in around the 220 peak in Fig. 1(b) shows that the peaks are relatively broad and show a shift towards smaller angles, i.e. larger lattice constants compared to Mg2Si.
The relationship between the lattice constant a and Sn content x is approximately given by x = (a − aMg2Si)/(0.0427 nm).20 The calculated values of x are given in Table 1 and confirm the results and trends obtained from the density data. In fact, the good agreement between the Sn content obtained from density data and the XRD peak shift indicates good compaction and a high relative density of the samples, as significant (closed) porosity leads to a reduced x from the density data but does not affect that from the XRD peak shift.
Microstructural analysis by SEM shows a multiphase sample with a matrix in grey and minor phases in light grey and dark grey, as shown in Fig. 2. The image is taken for sample #5, but the microstructure is similar in all samples, see Fig. S2–S4 (ESI†). EDX analysis of all samples reveals that the matrix and the minor phases do not have sharp compositions, but consist of domains with similar, yet distinct local compositions.
The Sn content x and the approximate phase fractions are given in Table 2. Employing the distinct grey values of the three phases, the graphical analysis software ImageJ has been used to estimate the (areal) fraction of each phase. It yields 85% main phase, 13% of the Mg2Si-like phase and about 2% for the Sn-rich phase for the two-dimensional image. To calculate the 3D values, we assumed that the main phase is the matrix and the minor phases are isotropically included within the matrix. The phase fraction for the minor phases is then given by z2D3/2, where z2D is the fraction in the two dimensional image.
Main phase (α) | Si-rich phase (β, dark) | Sn-rich phase (γ, bright) | |
---|---|---|---|
Sn content x | 0.1 < x < 0.2 | x < 0.03 | 0.4 < x < 0.6 |
Phase fraction | 0.95 | 0.05 | <0.01 |
Fig. 3 shows the element mapping of a typical Mg2Si0.8Sn0.2 sample. The Mg2Si-like and the main phase are clearly distinguishable, and it can also be seen that the matrix phase itself has a spatially varying Sn content. Another interesting feature is the observed difference in the Sb content for the main phase and the Mg2Si-like phase. Sb is significantly more dissolved in the main phase with a higher Sn content. Presumably Sb can be more easily incorporated in Sn-richer phases due to their larger lattice constant. The EDX analysis also detects some oxygen, mainly at interface regions between the matrix phase and the Mg2Si-like phase. As MgO has been identified by XRD it can be deduced that oxygen is present presumably in the form of MgO. The matrix phase and the Mg2Si like phase are also visible in the Mg mapping. As the lattice constant increases with increase in the Sn content, the Mg density is higher in the Mg2Si-like phase than in the matrix phase, which results in the observed contrast.
Transport data of Mg2Si0.8−ySn0.2Sby are shown from room temperature to 740 K in Fig. 4. Due to better visibility only the thermal conductivity data of the undoped sample (#1) are shown here; the complete data are presented in Fig. S5 of the ESI.† The electrical conductivity (a) shows the typical decrease with increase in the temperature of a highly doped semiconductor above 400 K; below 400 K a plateau can be observed for some of the samples. The electrical conductivity also exhibits the expected increase with increase in doping. The Seebeck coefficient (b) decreases with increase in doping and increases approximately linearly with increase in the temperature for all samples.
The thermal conductivity (c) decreases with temperature for all samples but shows a much higher value for the sample with the highest doping. The thermoelectric figure of merit ZT is calculated from (a) to (c) and shows an increase with temperature for all samples. Sample #4 with y = 0.015 has the highest thermoelectric figure of merit with ZT = 0.95 at 740 K. While the ZT values for the less doped samples are lower, but comparable, sample #5 has a drastically lower figure of merit. Fig. 4(e) reveals a roughly temperature independent carrier density of all samples, except for sample #5. Here the carrier concentration is roughly constant up to 650 K after which nH decreases rapidly. As the sample has been stable during the S–σ and LFA measurements beforehand, we do not know what caused the irreversible change in the sample. It can be seen that the carrier density data of the samples are consistent with the results for S and σ and that the control over the carrier concentration is not perfect as the actual Hall carrier concentration does not exactly follow the linear trend expected from the nominal doping composition. Doping is relatively effective as one would roughly expect 1.5 × 1020 cm−3 carriers for a nominal composition of Mg2Si0.79Sn0.2Sb0.01 if one carrier per Sb atom is provided. The Hall mobility (f) decreases with increase in the temperature after an initial plateau for samples #2–#4; sample #5 shows a monotonic trend with significantly lower absolute values.
We will now analyze the results in the framework of a single parabolic band model (SPB).29 This model has been employed for Mg2Si and Mg2Si1−xSnx with reasonable success beforehand.5,21,30 For T > 500 K μH ∝ T−p holds with 1 < p < 1.5, which indicates acoustic phonon (AP) scattering as the dominant scattering mechanism. At lower temperatures, there is some deviation from this behavior, presumably due to grain boundary scattering of the charge carriers at the interfaces.28 A possible influence of alloy scattering cannot be excluded, but is not expected to be dominant due to the relatively low Sn content.6 Grain boundary scattering is an extrinsic scattering mechanism so that AP scattering can assumed to be the dominant intrinsic mechanism at all temperatures. In this case, the reduced chemical potential η and the DOS effective mass m* of the electrons can be calculated using
(1) |
(2) |
Fig. 5 Results from the single parabolic band model for Mg2Si0.8−ySn0.2Sby; for comparison, the data of Mg2Si0.9875Sb0.0125 (“Mg2Si”) from ref. 28 are also presented. (a) Calculated chemical potential for all samples. For the sample with the largest carrier concentration (#5) (η + 2)kBT is plotted as well; this gives an impression up to which energy a significant number of carriers are excited. (b) All samples show an increase in the effective mass with increase in the temperature, with sample #5 having a significantly higher effective mass. (c) The Pisarenko plot shows decent agreement between experimental data and theoretical curves using the temperature dependent effective masses of (b). (d and e) Power factor σS2 and lattice thermal conductivity (overlaid by bipolar contribution). Compared to Mg2Si, the Mg2Si0.8Sn0.2 samples show a slightly reduced power factor but a drastically reduced lattice thermal conductivity. (f) A fit of the mobility parameter μ0vs. T can be used to obtain the deformation potential. Dashed lines show the results using m*(T) while the solid lines the results from an averaged effective mass. |
The effective mass increases with temperature for all samples. While the three lower doped samples increase roughly from 1m0 to 1.25m0 in the measured temperature range, the sample with the highest doping increases from 1.25m0 to 1.35m0; m0 is the free electron mass. The Pisarenko plot in Fig. 5(c) shows reasonable agreement between the experimental and the modeling data.
The lattice thermal conductivity (and the bipolar contribution) is plotted in Fig. 5(e). It is given by κlat + κbip = κ − LσT, with for the SPB model with AP scattering. The thermal conductivities of samples #1–#4 are comparable with a slight reduction for increased doping. The lattice thermal conductivity follows the power law κlat = A + B/Tp with −1 < p < −0.5. Umklapp phonon scattering predicts a κlat ∝ T−1 behavior, while κlat ∝ T−0.5 corresponds to alloy scattering as the dominant phonon scattering mechanism. The measurement results therefore indicate a mixed scattering mechanism. At high temperature, the onset of the bipolar contribution is clearly visible for the undoped sample. The sample with the highest doping has a lattice thermal conductivity, which is more than 50%, higher than the others, indicating a significantly different thermal transport in this sample.
The carrier density independent mobility μ0 is plotted in Fig. 5(f) and is related to the Hall mobility by ref. 29. It is a material parameter and is thus supposed to be independent of the carrier concentration. Indeed one notices that the mobilities for samples #2–#4 are very similar. The mobility of sample #5 is significantly lower; however, the difference is not as large as for μH. The mobility data can be used to extract a further material parameter, the deformation potential Edef which quantifies the interaction between acoustic phonons and charge carriers. It is given by ref. 31:
(3) |
The thermoelectric potential of the material can be estimated by calculating ZT(n,T). The basic equation can be rearranged as
(4) |
Fig. 6 Experimental and theoretical results for the thermoelectric figure of merit vs. the carrier concentration at different temperatures. |
The results from eqn (4) show the expected trends: an increase in ZTmax with increasing temperature and a shift of the optimal carrier concentration towards higher values for increasing temperature. Our experimental data show good agreement with the modeling results. ZTmax obtained both from the SPB model and the experimental data is ≈0.95 at 740 K. The best experimental value is at nopt = 1.2 × 1020 cm−3, while the model predicts 0.7 × 1020 cm−3; however, the maximum is relatively broad and the model does not account for differences in κlat observed between the samples.
Our SEM/EDX results confirm the XRD results where the observed broad peaks indicate stoichiometric variations. The observed minor phases can very well be hidden in the shoulders of the broad peaks. EDX mapping also shows a lower content of the dopant Sb in the Mg2Si-like phase compared to the matrix phase. As the matrix phase has a slightly larger lattice constant a better Sb solubility can be expected.
T | n opt [1019 cm−3] | ZT max | m* [m0] | κ lat [W mK−1] | E def [eV] |
---|---|---|---|---|---|
340 | 3 | 0.2 | 1 | 2.3 | 13.0 |
740 | 7 | 0.95 | 1.25 | 1.3 | 13.0 |
We found an optimum carrier concentration nopt which is lower than the value (nopt = 18 × 1019 cm−3) stated by Liu et al.;5 however the carrier concentration optimization was mainly performed in view of compositions with a higher Sn content in their work. With respect to the effective mass we found good agreement with the literature reports: Liu et al. obtained m* = 0.93m0 for Mg2Si0.8Sn0.2, while Tani et al. obtained m* = 0.9m0 for Mg2Si0.9Sn0.1 at room temperature.
However, there are also deviations from the SPB model. Firstly, we observe an apparent increase of the carrier concentration (see Fig. 4 for nH(T) or Fig. S7(b) (ESI†) for n(T)). Secondly, we found a clear increase in the effective mass with temperature and a difference between the sample with the highest doping (#5) and the other samples. Thirdly, the carrier density corrected mobility μ0 differs for sample #5 compared to samples #2–#4 (see Fig. 5(f)), although it is a material parameter and is supposed to be independent of carrier concentrations.
The increase in n and m* with T was similarly found in Mg2Si28,30 and might be due to the non-parabolicity of the bands. The observed difference in m* for #5 compared to #2–#4 could be due to either a non-parabolic band or by the influence of the second conduction band with higher m*: Mg2Si1−xSnx has two threefold degenerate conduction bands CBL and CBH with a band gap E0 that depends on x. For small x the light conduction band is at a lower energy, while for large x the heavy band is at lower energy. The cross-over is around 0.6.5,10 The band gap between the two conduction bands is less clear for arbitrary x. Zaitsev et al. used E0,x=0 = 0.4 eV (with CBL closer to the valence band) and E0,x=1 = 0.2 eV (with CBH closer to the valence band). They suggested a linear interpolation in between which results in E0,x=0.2 = 0.28 eV.4 Bahk et al. used the same assumption for a recent transport modeling.20 On the other hand, Bourgeois et al. calculated E0,x=0 = 0.19 eV and E0,x=1 = 0.28 eV which correspond to E0,x=0.2 = 0.1 eV, i.e., a much smaller band gap for the investigated composition.15 Tan et al. calculated the interband gaps using DFT for different compositions obtaining E0,x=0.25 ≈ 0.3 eV.35 The discrepancy in the literature reports shows that the interband gap is not well characterized as the band positions are temperature dependent and the calculations do not account for this.
One possible explanation for the experimentally observed increase in m* for sample #5 compared to #2–#4 is thus a contribution of the second conduction band CBH to the electronic transport. If CBH is within (η + 2)kBT some contribution can be expected. Fig. 5(a) indicates that this would be the case for E0 < 0.2 eV. On the other hand, DFT calculations have shown that the bands of Mg2(Si,Sn) are not strictly parabolic and therefore the effective mass depends on the chemical potential.35,36 In this case, however, the density-of-states effective mass, which is related to the band shape, is not identical to the momentum effective mass (which controls the transport integrals) anymore.37 Considering only the effective mass data can thus not provide clear evidence on E0 and the question whether one or two bands contribute. Further insight can be gained by a detailed analysis of the mobility data. The fits of μ0(T) to extract the electron acoustic phonon interaction parameter Edef are plotted using m*(T), as shown in Fig. 5(f) as dashed lines. The fits are performed in the temperature region where AP scattering is clearly dominant, i.e. above 500 K. The agreement between experimental data and theoretical results is not very good, in particular with respect to the temperature dependence. As the strong temperature dependence of m*(T) is unexpected and might be an artifact of the assumed parabolic band structure we have also fitted the data using the average, temperature independent m* of each sample. The results are plotted in full lines and are in almost perfect agreement with the experimental data above 450 K. This indicates that the observed apparent increase in m*(T) is indeed an artifact of the simple SPB model assumptions.
The phonon deformation potential can be extracted from the fits if the elastic constant C11 is known. As this is not the case for this particular composition we have used a linear interpolation of the experimental room temperature values from Mg2Si and Mg2Sn, yielding C11,x=0.2 ≈ 110 GPa.38,39 This is in decent agreement with preliminary data obtained from resonant ultrasonic spectroscopy giving ≈100 GPa.40 The fitting results for Edef of samples #2–#5 are 13.1 eV, 13.5 eV, 12.8 eV, 12.8 eV, respectively, giving an average value of Edef,x=0.2 = 13.0 eV. The good agreement between the results for each sample (although μ0 is different) firstly increases the credibility of the result for Edef,x=0.2 and secondly argues against a significant influence of the second band CBH on the electronic transport: as the deformation potential for the two sub-bands differs by more than 50%,6 one should see a difference in Edef between #5 and samples #2–#4. This as well as the much better fits of μ0(T) for a temperature-independent m* indicate that the observed differences in the mobility parameter μ0 between the samples and the apparent temperature dependent m* are rather the consequences of a not strictly parabolic band CBL than due to the second band contributing to the transport.
Our result for Edef is higher than the value used by Bahk et al.: Edef,x=0.2 = 8.9 eV. The difference is not due to the mobility data but rather the used elastic constant. Bakh et al. used C11,x=0.2 ≈ 40 GPa, i.e. a much lower value. If we use the same elastic constant we obtain Edef,x=0.2 ≈ 7.9 eV in good agreement with their data. This disagreement can be figured out by mapping of the elastic constants with temperature and composition. Liu et al. obtained Edef,x=0 = 17 eV and Edef,x=1 = 10 eV, which give Edef,x=0.2 = 15.4 eV in the linear interpolation; in decent agreement with our results.6
Overall, the main features of the electronic transport can be well understood in the framework of a single parabolic band, although the material is not a single phase compound and has a complex microstructure. It is plausible that the matrix phase is dominant for the carrier transport as the Sn-rich phase has only a very small volume fraction (<1%) and the Mg2Si-like phase is significantly less doped and therefore behaves more or less like insulating particles within the matrix. The dependence of m*(T,η) indicates that the bands are not strictly parabolic. Nevertheless, the agreement between experimental data and the predictions from the simple single parabolic band model is good and the material parameters like nopt, ZTmax, m*, Edef can expected to be reasonably accurate. The observed deviations from the single parabolic band model point towards a non-parabolic band, rather than a contribution from the second band. This indicates a band gap between the light and the heavy conduction band of ≥0.2 eV, supporting an earlier work by Zaitsev et al.4 and calculations by Liu et al.,5 but in contradiction to theoretical results by Bourgeois et al.15 However, the effect of the second band cannot be totally excluded from the data. We also note that a Kane type band would lead to a lower Seebeck coefficient at high doping than a parabolic band, in contrast to what is found experimentally. More sophisticated modeling is therefore required for a full assessment of the band structure.
Comparing the properties of Mg2Si0.8Sn0.2 with those of Mg2Si, we reveal a reduction of the phonon deformation potential and an increase in the effective mass, indicating a band flattening upon Sn substitution.
Footnotes |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c5tc01535a |
‡ Contributed equally. |
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