Kang Yina,
Xianli Su*a,
Yonggao Yana,
Ctirad Uherb and
Xinfeng Tang*a
aState Key Laboratory of Advanced Technology for Materials Synthesis and Processing, Wuhan University of Technology, Wuhan 430070, P. R. China. E-mail: suxianli@whut.edu.cn; tangxf@whut.edu.cn
bDepartment of Physics, University of Michigan, Ann Arbor, MI 48109, USA
First published on 4th February 2016
The relationship between the temperature and the composition as well as the microstructure of a Sb-doped Mg2Si0.30Sn0.70 solid solution was systematically studied according to the Mg2Si–Mg2Sn pseudo-binary phase diagram. This work shows that the composition, distribution pattern, and fraction of in situ nanostructures can be controlled by the heat treatment carried out at a specific peritectic reaction temperature. A large number of in situ nanoprecipitates were observed when the sample was quenched at 900 K or 1130 K. However, quenching at 900 K resulted in the formation of agglomerates while quenching at 1130 K yielded a more even dispersion of nanoprecipitates. Monochromatic X-ray studies, back-scattering images and HRTEM results showed that the composition of the nanoprecipitates when quenched at 900 K was the Mg2Si-rich phase, while the nanostructure was the Mg2Sn-rich phase when quenched at 1130 K. The lattice thermal conductivity decreased dramatically due to the well distributed Mg2Sn-rich nanoprecipitates, and the maximum ZT of about 1.2 was achieved at around 750 K. Moreover, the average value of the figure of merit ZTaverage reached about 0.9 in the range of 300–800 K, about a 15% higher value than in the sample composed of Mg2Si-rich nano-agglomerates. This study demonstrates that carrying out heat treatments at the phase transformation temperatures is a simple and controllable method to design and form in situ nanostructures, which is of vital importance in the fabrication of nanocomposites and optimization of the thermoelectric performance.
Mg2Si1−xSnx solid solutions are consist of earth abundant, inexpensive, and environmentally friendly raw elements and possess a relatively high volume power density. They are expected to be operated in the temperature range of 300–800 K.23 So far, the electronic properties of Mg2Si1−xSnx have been optimized by adjusting the Si/Sn ratio,24,25 by doping with Sb or Bi,26–29 and by varying the stoichiometry of Mg.30,31 And the thermal properties have been tuned by altering the Si/Sn ratio or by introducing nanoinclusions.19,32,33 However, tuning the thermal conductivity by changing the Si/Sn ratio has been hampered by the fact that there is a miscibility gap for compositions 0.4 ≤ x ≤ 0.6 (ref. 34) which precludes to use the most disordered structure with x = 0.5. Consequently, nanostructuring has been explored as an alternative strategy of reducing the thermal conductivity.35
It is important to keep in mind that grain boundaries and interfaces scatter not only phonons but also charge carriers and thus decrease the mobility.36–38 Benefits of nanostructuring are realized only if the mean-free path of phonons is reduced to a greater extent than the mean-free path of charge carriers. Consequently, it is desirable to have nanostructures that are coherent or at least semi-coherent with the matrix. Such nanostructures still scatter phonons very effectively but exert only a minor influence on the transport of charge carriers.39–41
Several studies have shown that semi-coherent and coherent interfaces can be achieved in the Mg2Si1−xSnx system via phase segregation, by making use of the miscibility gap. For instance, using the melt spinning technique, X. Zhang et al.42 synthesized Mg2Si0.4Sn0.6 solid solution decorated with 10–20 nm homogeneously distributed nanoparticles, while W. Liu et al.43 observed numerous Mg2Sn-rich nanoprecipitates in Mg2Si0.4Sn0.6, prepared by a two-step solid state reaction (SSR) method. However, different morphologies were obtained with Mg2Si0.3Sn0.7, a solid solution containing a larger fraction of Mg2Sn. In this case, a single phase structure with good homogeneity was achieved by melt spinning, while Mg2Si-rich nanoinclusions were observed when the solid solution was prepared by the two-step SSR method.44 The key point behind the inconsistent results is that the researchers have not clearly understood how the composition and the microstructure of Mg2Si1−xSnx evolve and depend on the preparation methods due to a complicated and unclear phase diagram. According to the Mg2Si–Mg2Sn pseudo-binary phase diagram,34,45,46 there are three peritectic reactions in the system taking place at 1130 K, 900 K, and 837 K, respectively (1130 K: Mg2Si0.2Sn0.8(L) + Mg2Si0.4Sn0.6(S) → Mg2Si0.3Sn0.7(S); 900 K: 7Mg2Si0.28Sn0.72(L) + 3Mg2Si0.86Sn0.14(S) → 10Mg2Si0.45Sn0.55(S) + 0.04Si(S); 837 K: Mg0.9Si0.03Sn0.07(L) + Mg2Si0.88Sn0.12(S) → Mg0.98Sn0.02(S) + Mg2Si0.43Sn0.57(S)). The composition and the phase (solid or liquid) differ from one another depending on which peritectic reaction is involved, thus the composition and the microstructure of the resulting solid solutions are very sensitive to the synthesis process and its parameters.
In this study, Sb-doped Mg2Si0.30Sn0.70 was chosen as an example with which to shed light on the inconsistency of results when guided by the existing Mg2Si–Mg2Sn pseudo-binary phase diagram and carrying out the synthesis using different peritectic reactions. The results showed that the microstructure and the composition depend strongly on the temperature at which the sample was quenched. Specifically, a single phase material was successfully obtained when quenching at 1080 K. In contrast, quenching at a lower temperature of 900 K, one obtained lots of Mg2Si-rich nanoprecipitates which tend to agglomerate, while quenching at a higher temperature of 1130 K resulted in Mg2Sn-rich nanoprecipitates which were uniformly distributed. This high-temperature quenched solid solution with Mg2Sn-rich nanoprecipitates has an outstanding TE performance with the average value of the figure of merit ZTaverage ∼ 0.9 in the temperature range of 300–800 K and the peak value ZTmax of ∼1.2 near 750 K. Moreover, this particular nanostructured solid solution showed an excellent thermal stability. After extended annealing at 773 K for no less than 15 days, the TE properties were essentially unchanged which is of critical importance for power generation applications. All in all, a high TE performance Mg2Si0.30Sn0.70 solid solution was obtained by carefully designing the composition and the distribution pattern of in situ nanoinclusions according to the phase diagram.
| Sample | 1st SSR | 2nd SSR | Actual composition |
|---|---|---|---|
| 1 | 837 K-6 h | — | Mg2.158(Si0.281Sn0.719)0.978Sb0.022 |
| 2 | 837 K-6 h | 900 K-4 h | Mg2.148(Si0.289Sn0.711)0.979Sb0.021 |
| 3 | 837 K-6 h | 1080 K-4 h | Mg2.139(Si0.306Sn0.694)0.982Sb0.018 |
| 4 | 837 K-6 h | 1130 K-4 h | Mg2.082(Si0.346Sn0.654)0.981Sb0.019 |
The phase composition of the solid solution at different steps of processing was characterized using a PANalytical X'Pert Empyrean type X-ray diffractometer with Cu Kα and Kα1 radiations, and the lattice parameters were calculated by the Rietveld method. For the regular X-ray diffraction, the ratio of Kα2/Kα1 was 0.5, with the generator voltage and the tube current to be 40 kV and 40 mA, respectively, and the scan range was 10–80 degrees with a scan step size of 0.02 degree and the divergence slit of 0.38 mm. Except the scan step size of 0.005 degree as well as the divergence slit of 0.5 mm, all parameters were the same as aforementioned for the monochromatic X-ray diffraction. The actual chemical composition and back-scattering images of the polished ingots were analyzed by electron probe microanalysis (EPMA) with the aid of JEOL JXA-8230 system. The microstructure of the fractured surface was characterized by field-emission scanning electron microscopy (FESEM) using a Hitachi SU8020 apparatus. And high resolution transmission electron microscopy (HRTEM) was carried out with a JEOL JEM-2100F equipment.
The electrical conductivity and the Seebeck coefficient in the range of 300–800 K were acquired on a commercial ZEM-3 system (Ulvac Sinku-Riko) in helium by a standard four-probe DC configuration. The Hall coefficient at 300 K was measured by the five probe method using a physical property measurement system (PPMS, Quantum Design). The carrier concentration and the carrier mobility were then calculated from the equation nH = 1/eRH and μH = σRH, respectively. The thermal conductivity was determined by κ = λCpρ, where λ is the thermal diffusivity acquired by the laser flash method (Netzsch LFA 457), Cp is the specific heat measured by a differential scanning calorimeter (TA DSC Q20) in argon, and ρ is the density determined by the Archimedes method in alcohol.
To explore the thermal stability of in situ formed nanostructures (solid solution quenched at 1130 K), the sintered ingot was coated with BN spray and annealed in air at 773 K for 15 days.47 The microstructure and the transport properties of thus annealed sample were then characterized in detail.
m group, and the reference pattern of Mg2Si0.30Sn0.70 is derived from JCPDS # 01-089-4254 by modifying the Si/Sn ratio.48 The major phase of the products after the first SSR step was Mg2Si1−xSnx (x ≥ 0.7) and the Mg2Si-rich phase together with a tiny amount of unreacted Mg and Sn. Almost the same composition (except for the absence of Sn) was obtained after the second SSR step carried out at 900 K and 1080 K. However, when the second reaction step was carried out at 1130 K, a very different outcome resulted with Mg2Si1−xSnx (x ≤ 0.7) and Mg2Sn-rich phase being detected. Though multiple phases still coexisted after the second SSR step, a single phase material was obtained upon subsequent sintering, see Fig. 1(b). This indicates that sintering is helpful in promoting the formation of single phase solid solution as it enhances the process of mass transfer.49 However, a closer look, see Fig. 1(c), reveals that the XRD peaks of the sintered ingots have shifted to higher angles and the lattice parameters (shown in Fig. SI1, ESI†) decreased as the temperature of the second SSR step increased. We suspected that the powders prepared for X-ray investigations after sintering may have still contained traces of Mg2Si-rich or Mg2Sn-rich phases,50 but these were too difficult to distinguish from the major phase due to the very similar lattice parameters and mixed wavelengths of Kα1 and Kα2 radiation. To verify this point, monochromatic X-ray diffraction was conducted on powders of the sintered ingots, Mg2Si-rich second phase was detected in the sintered ingots quenched at 837 K and 900 K, while a single phase material was obtained when quenched at 1080 K. Increasing the quenching temperature to 1130 K, Mg2Sn-rich phase was detected (presented in Fig. 1(d)). The results were also confirmed by the electron back-scattering (see Fig. 2) images, where the circled regions indicate the Mg2Si-rich phase (it was the second phase in Fig. 2(a) and (b), while the major phase in Fig. 2(d)). Moreover, EPMA data (shown in Table 1) also confirm the difference in the phase composition of this solid solution subjected to different heat treatment conditions. To get a clear picture regarding the phase composition of the solid solution, an inquiry into the formation mechanism and microstructure during different peritectic reactions was made according to the Mg2Si–Mg2Sn pseudo-binary phase diagram.
Though researchers argued about the actual region of the miscibility gap, they agreed on the peritectic temperature, as E. N. Nikitin et al.34 conducted the experiment with a longer annealing time and slower crystallization than that of Sh. F. Muntyanu et al.51 we take the diagram plotted by E. N. Nikitin et al. as a reference. Taking the Mg2Si0.30Sn0.70 solid solution as an example (see Fig. SI2, ESI†), and starting with a liquid at high temperature, the liquidus will be reached upon cooling the melt at about 1200 K (the process 1 → 2). A solid phase with the composition of approximately Mg2Si0.75Sn0.25 will appear together with the liquid phase of Mg2Si0.3Sn0.7 expressed schematically as:
| L → SA(Mg2Si0.75Sn0.25) + LB(Mg2Si0.3Sn0.7) |
As the temperature decreases (the process 2 → 3), the composition of the solid changes along the AC line while that of the liquid changes along the BE line. At 1130 K, by a lever rule, the composition should be SC(Mg2Si0.6Sn0.4)
:
LE(Mg2Si0.2Sn0.8) = 1
:
3. However, the composition varies as there follows a peritectic reaction (the process 3 → 3′):
| Mg2Si0.2Sn0.8(L) + Mg2Si0.6Sn0.4(S) → 2Mg2Si0.4Sn0.6(S) |
The resulting products are SD(Mg2Si0.4Sn0.6)
:
LE(Mg2Si0.2Sn0.8) = 1
:
1, and they will change along the DH line and EI line, respectively if keep cooling (the process 3′ → 4). Due to the heat loss by radiation, the actual temperature of the sample when quenched was a bit lower than 1130 K (in reality it was ∼1120 K when cooling down in the oversaturated salt water, measured by a chromel–constantan thermocouple), so the composition after quenching should have been SF(Mg2Si0.35Sn0.65)
:
LG(Mg2Si0.18Sn0.82) = 12
:
5. This was confirmed by the XRD, the back-scattering images and the EPMA results which indicate the Mg2Si-rich matrix together with the Mg2Sn-rich second phase.
Single phase was obtained when quenched at 1080 K, and this is due to the critical temperature at which liquid and solid phases coexist (the process 3′ → 4). The liquid phase speeds up the mass transfer which is helpful for forming a homogeneous solid solution. When the temperature drops a bit below 1080 K, the liquid phase disappears and Mg2Si0.30Sn0.70 solid forms.
About 40 years later after the reports by E. N. Nikitin et al.34 and Sh. F. Muntyanu et al.51 researchers found another two peritectic reactions happen at 900 K and 837 K, by calculations and experiments.45,46 The phase transformation process at 900 K is almost the same as at 1130 K, as shown in Fig. SI3(a), ESI.† Liquid appears when the temperature goes to 900 K:
| Mg2Si0.3Sn0.7(S) → 0.97Mg2Si0.28Sn0.72(L) + 0.03Mg2Si0.86Sn0.14(S) |
This is followed by the peritectic reaction:
| 7Mg2Si0.28Sn0.72(L) + 3Mg2Si0.86Sn0.14(S) → 10Mg2Si0.45Sn0.55(S) + 0.04Si(S) |
The products would have been Mg2Si0.28Sn0.72(L)
:
Mg2Si0.45Sn0.55(S)
:
Si(S) = 9
:
1
:
4 × 10−3. As the content of Si was rather small compared with others, only the Mg2Sn-rich matrix and the Mg2Si-rich second phase were observed.
A similar situation happens at 837 K, where the peritectic reaction (shown in Fig. SI3(b), ESI†) is:45,46
| Mg0.9Si0.03Sn0.07(L) + Mg2Si0.88Sn0.12(S) → Mg0.98Sn0.02(S) + Mg2Si0.43Sn0.57(S) |
The actual composition after quenching would have been Mg2Si0.27Sn0.73
:
Mg2Si0.43Sn0.57 = 13
:
3, consistent with the data mentioned above. A minor Mg phase was observed, likely the result of intentionally added Mg to compensate for the evaporative loss.
Because liquid has appeared during the peritectic reaction, quenching at the phase transformation temperatures may result in the formation of unique nanostructures due to the non-equilibrium solidification.52,53 Consequently, the microstructure of samples prepared using different heat treatments was characterized in detail. Since the phase composition and the state of the second phase before quenching (both were solids) were similar when heat treated at 837 K and 900 K, while very different when heat treated at 1130 K, the samples quenched at 900 K and 1130 K were selected as representatives to explore the size and distribution of different nanostructures (shown in Fig. 3). Thermal stability of the nanostructures was also characterized by annealing at 773 K for 15 days. Fig. 3(a) and (b) are the FESEM images of powders after the second SSR step, while Fig. 3(c) and (d) are those of the sintered ingots, and Fig. 3(e)–(h) provide the size distribution of nanoparticles appearing in Fig. 3(a)–(d), respectively. The microstructure and the nanoparticle size distribution of the annealed bulk structures (773 K for 15 days) are shown in Fig. SI4, ESI.† Nanoprecipitates with the size around 25 nm were observed after heat treatment at 900 K as well as at 1130 K, and they grew up to about 45 nm after sintering. Moreover, the most striking difference concerns the distribution pattern. When quenched at 900 K, the nanoprecipitates tend to agglomerate while they were well-dispersed when quenched at 1130 K. The morphological difference is induced primarily by the state of the second phase during different peritectic reactions. The second phase, composed of Mg2Si0.45Sn0.55, was a solid before quenching at 900 K (similarly when quenched at 837 K). In contrast, the second phase comprising Mg2Si0.18Sn0.82 was a liquid before quenching at 1130 K, and the Mg2Sn-rich nanoprecipitates were evenly dispersed without any tendency to agglomerate due to the much faster mass transfer in the liquid phase. After annealing at 773 K over an extended period of time for no less than 15 days, the size of the nanoprecipitates was essentially unchanged, boding well for high temperature applications of Mg2Si1−xSnx solid solutions containing in situ grown nanoinclusions. HRTEM analysis, shown in Fig. 4, was conducted to reveal the composition and microstructure of nanoprecipitates, beyond the information gained from monochromatic X-ray diffraction data mentioned above. Fig. 4(a) and (b) are low magnification images of the sintered ingots with the second SSR step quenched at 900 K and 1130 K, respectively, while Fig. 4(c) and (d) are the same images at higher magnification. As clearly shown in Fig. 4(a), the nanoprecipitates agglomerated when the second reaction step was quenched at 900 K, while well-dispersed nanoparticles were observed when quenching is done at 1130 K, the results were consistent with the FESEM data. Such finely dispersed Mg2Sn-rich nanoprecipitates facilitate a suppression of the lattice thermal conductivity, as we shall see later. Moreover, at least semi-coherent interfaces are observed between the matrix and the nanoprecipitates which is favorable for electronic transport properties. It is follows that the composition and the distribution pattern of in situ formed nanoprecipitates can be designed and tuned through a carefully selected and applied heat treatment at a specific temperature where the phase transformation takes place, and the fraction of nanoprecipitates can be properly adjusted according to a lever rule of the relevant phase diagram.
![]() | ||
| Fig. 5 (a) The carrier concentration and the carrier mobility at 300 K; (b) the electrical conductivity; (c) the Seebeck coefficient; (d) the power factor; (e) the Pisarenko plot (S–nH) at 300 K; (f) the μH–nH plot at 300 K, of samples with different heat treatments. The reference data of W. Liu et al.54 are noted in (e) and (f). | ||
The temperature dependent thermal conductivity κTotal, the sum of the lattice thermal conductivity κLattice combined with the bipolar contribution κBipolar, and the ZT value are shown in Fig. 6. The value of κLattice + κBipolar was calculated by subtracting the electronic part κelectron = LσT from the total thermal conductivity κTotal. The Lorenz number L was calculated based on the SPB model under the relaxation time approximation, and is shown in Fig. SI5, ESI.†,54,56 As there was little difference between κelectron of samples quenched at different temperatures, the different values of κTotal were caused mainly by variations in the lattice thermal conductivity which behaved as κLattice ∝ T−0.7, indicating the mixed dominance of Umklapp scattering and alloy scattering.57,58 The lattice thermal conductivity of the sample quenched at 1130 K is much lower than the value of other samples likely due to the presence of well distributed Mg2Sn-rich nanoprecipitates.59 However, the bipolar effect started to be important at a somewhat lower temperature (∼600 K) as a consequence of the lower carrier concentration. The theoretical minimum value of the lattice thermal conductivity of ∼0.7 W m−1 K−1 above 500 K was estimated using the Cahill model by taking the Debye temperature of θD = 247 K and the average phonon velocity of νaverage = 2375 m s−1.43,60 Comparing this value with the experimental data, it shows that there is still some room to reduce the lattice thermal conductivity further.
Since the value of κLattice + κBipolar of the sample quenched at 1130 K is notably smaller than that of other samples, simple calculations were made to give an insight into the effect of semi-coherent and coherent nanoprecipitates. The Hashin–Shtrikman (H–S) model describing the lattice thermal conductivity of a binary composite was applied to explain the changing trend before the bipolar effect becomes important at high temperature:61,62
:
Mg2Si0.18Sn0.82 = 12
:
5 (mole fraction), with the second SSR step quenched at 1130 K, according to the phase analysis mentioned above. In terms of the volume fraction, it should be Mg2Si0.35Sn0.65
:
Mg2Si0.18Sn0.82 = 2.85
:
1, i.e., x1 = 74% and x2 = 26%. The lattice thermal conductivity of the composite under the H–S model was obtained by interpolation according to the inequations mentioned above. Judging from Fig. 6(c), the actual value of the lattice thermal conductivity of this sample was significantly lower than what calculations predict, suggesting that the decrease of the lattice thermal conductivity cannot be explained simply by the formation of binary composite, nanoprecipitates and newly grown grain boundaries/interfaces should also be taken into consideration. Thus, the calculation was revised33,63 by assuming that all Mg2Si0.18Sn0.82 nanoprecipitates are of the 45 nm size and dispersed homogeneously, as observed in the FESEM image. The resulting value (solid curve in Fig. 6(c)) is much closer to the actual experimental value than that predicted by the H–S model, even though the temperature dependence is not perfect.
Due to its lower lattice thermal conductivity, the value of ZTaverage observed on the sample quenched at 1130 K reached ∼0.9 over the temperature interval 330–800 K. This is about 15% higher than that of the sample quenched at 837 K. The maximum figure of merit of the sample quenched at 1130 K reached ∼1.2 near 750 K. Annealing this sample at 773 K for 15 days had essentially no effect on the transport properties, demonstrating a bright prospect for the TE power generation.
Footnote |
| † Electronic supplementary information (ESI) available. See DOI: 10.1039/c5ra27171a |
| This journal is © The Royal Society of Chemistry 2016 |