3.1. Liquid-State Sn/n-Type Bi2(Te,Se)3 Interfacial Reactions
The composition of the commercial n-type Bi
2(Te,Se)
3 thermoelectric material was measured using EPMA to be 40.1 at.%Bi-6.0 at.%Se-53.9 at.%Te. The composition is consistent with the typical commercial n-type TE material, and can be expressed as Bi
2(Te
0.9Se
0.1)
3. It was further characterized through XRD analysis, as shown in
Figure 1a, obtained from the soldering plane. The XRD findings revealed a strong orientation of the n-type TE substrate, evidenced by a single pronounced diffraction peak at
2-theta of 41.2°, corresponding to the (110) plane of Bi
2(Te,Se)
3. This compound exhibits a typical rhombohedral layered-structure along the c-axis (JCPDS # 50-0954, space group: R-3m with lattice parameters
a = 0.4374 nm and
c = 3.0424 nm). Moreover, the bulk Bi
2(Te,Se)
3 material was grounded to powders for further analysis.
Figure 1b demonstrates that complex diffraction peaks closely match those of the JCPDS standard patterns, indicating the poly-crystalline nature of the material. Notably, the prominent peak at 27.8° corresponds to the (015) plane. According to the XRD results, the soldering plane is associated with the (110) crystalline plane, indicating alignment with the c-axis, as illustrated in
Figure 1c.
The interfacial reactions between the liquid-state Sn solder and Bi
2(Te,Se)
3 at 250 °C for various durations are displayed in
Figure 2a–c. After 1 min of reaction, as shown in
Figure 2a, two distinct reaction layers with dense structures were observed at the interface. A bright phase layer, approximately 1.2 µm thick, was located at the side of the Bi
2(Te,Se)
3 substrate, while a dark layer, around 1.1 µm thick, was formed adjacent to the solder. With an increase in reaction time to 3 min, both the reaction layers slightly thickened, although the interfacial microstructure remined similar.
Furthermore, the reaction was prolonged to 5 min, as shown in
Figure 2b. EPMA analysis revealed the composition of the dark phase as 53.1 at.%Sn-0.2 at.%Bi-3.2 at.%Se-43.5 at.%Te, which was identified as the SnTe phase. Based on the phase equilibria of the Sn-Bi-Te system and the Se-Sn-Te system [
25,
26,
27], the solubilities of Bi and Se in the SnTe phase at 250 °C is about 10 at.%Bi and 4at.%Se, respectively, consistent with the observed composition of SnTe in the interfacial reactions. The bright phase contained 4.1 at.%Sn-49.7 at.%Bi-3.8 at.%Se-42.4 at.%Te, suggesting that it was the BiTe phase with ~4 at.%Sn and ~4 at.%Se solubilities. The Sn and Se atoms could substitute the Te lattice sites in the BiTe phase. However, there is no available data in the literature regarding the composition or solubilities of Sn and Se in the BiTe phase. The solder region near the interface exhibited a solubility of 0.5 at.%Bi, 0.1 at.%Se, and 2.3 at.%Te. Notably, some tiny bright particles were dispersed in the SnTe phase.
Figure 2c shows the interfacial results after reacting for 10 min. The dark SnTe layer, measuring approximately 4.5 µm in thickness, appeared notably thicker than the bright BiTe layer, which was approximately 1.6 thick. Evidently, the SnTe phase was composed of large particulates with presence of voids. Similarly, small bright particles were observed within SnTe phase near the BiTe layer. Based on the contrast, these particles were suggested to be Bi precipitates, likely formed due to an oversaturation of Bi. Upon increasing the reaction time to 30 min (
Figure 2d), in addition to the growth of IMC layers, the interfacial microstructure remained stable with no significant evolution.
To further explore the morphology of SnTe phase, the Sn solder of the reaction couple was removed through deep etching.
Figure 3a,b display the top-view SEI micrographs showing displaying the grain morphologies of the SnTe phase after 5 min and 30 min of reaction, respectively. The SnTe phase exhibits round grains with numerous voids. In the 5-min sample, the grain size was less than 500 nm. In contrast, the grain size increased to approximately 2 µm in the 30-min sample. This indicated that the grain coarsening occurred with aging time during the soldering reaction. From a series of microstructural observations, the SnTe phase, composed of fine grains embedded with Bi-rich particles, exhibited grain coarsening and void formation. This void formation was attributed to Bi dissolution into the solder, resulting in voids within the SnTe phase.
Moreover, it was noted that the fraction of Bi-rich particles in the SnTe layer at 10 min was significantly lower than those at 1 and 5 min. As the reaction proceeded, the SnTe grains gradually coarsened and became denser, resulting in a reduction in voids. Additionally, the Bi-rich particles dissolved into the molten solder, leading to a decrease in the amounts of Bi-rich particles in the SnTe phase. Similar phenomena were also observed after a 30-min reaction. In the n-type Bi2(Te,Se)3, Se substitutes Te in the solid solution of the Bi2(Te,Se)3 lattice. Analysis of the reaction products of SnTe and BiTe revealed the Se concentrations of approximately 3~4 at.%. This observation suggests that Se could also substitute Te in the lattices of SnTe or BiTe. The low Se concentration in the solder near the interface indicated a very limited solubility of Se in liquid Sn.
Figure 4a show the average thicknesses of both the SnTe and BiTe layers plotted against aging time at 250 °C. The SnTe layer exhibited a continuous increase in thickness with aging time. In contrast, the growth of the BiTe layer gradually ceased after 5 min of reaction and maintained a thickness of ~1.6 µm. The IMC growth can be described by the following equation [
28]:
where
x represents the IMC thickness,
k is the rate constant,
t is the aging time,
n is the time exponent. In general, the IMC growth is controlled by lattice diffusion, following a parabolic relationship with aging time, where the expected value of
n is 0.5. In
Figure 4a, the SnTe phase exhibited a nearly parabolic growth. The natural logarithm plot of SnTe thickness versus aging time yielded an n value of 0.58, close to 0.5. Accordingly, the growth was assumed to be diffusion-controlled and the average thickness of SnTe plotted against the square root of reaction time, as shown in
Figure 4b. The data fitted well to a linear trend. From the slope, the diffusion-controlled growth rate constant,
kdiff, for the SnTe phase was determined to be 0.19 µm/s
0.5. The diffusion-controlled growth rate constant is crucial in interfacial reactions, as it significantly influences the reaction kinetics and resulting microstructure. Understanding this constant helps elucidate the reaction mechanism, predict IMC growth behavior, and even determine diffusion coefficients.
During the initial soldering process at the Sn/Bi2(Te,Se)3 interface, the Te component of Bi2(Te,Se)3 substrate reacted with the solder, leading to the formation of the SnTe phase. Simultaneously, a portion of Bi from the substrate dissolved into the solder. The remaining Bi and Te constituents of the Bi2(Te,Se)3 substrate subsequently transformed to the stable BiTe phase. As the reaction progressed, the primary diffusion species, Sn, continued to diffuse to reacted with the Te, which diffused across the BiTe phase from the substrate, resulting in the additional SnTe formation. The accumulated oversaturated Bi precipitated as Bi-rich particles within the SnTe phase.
In the previous study [
24] on the Sn/p-type (Bi,Sb)
2Te
3 reactions at 250 °C, the observed reaction phases consisted of three zones: the porous SnTe, the alternating-layer microstructure of SnTe and liquid solder, and the SnTe/Sn
3Sb
2 alternating layer. The reaction-limited linear growth exhibited an exceptionally rapid rate, approximately 15 μm/min. The reaction phase zone exceeded 450 μm after 30 min of reaction. However, in the present study, the reactions of Bi
2(Te,Se)
3 with Sn demonstrated that the growth of SnTe and BiTe IMCs was relatively sluggish. The overall IMC thickness reached merely ~10 μm after 30 min of aging. These finding suggested that the soldering reactions of n-type Bi
2(Te,Se)
3 were considerably slower compared to those of p-type (Bi,Sb)
2Te
3.
3.2. Solid-State Sn/n-Type Bi2(Te,Se)3 Interfacial Reactions
The initial interface of the as-soldered Sn/Bi
2(Te,Se)
3 couple is shown in
Figure 5a. The overall reaction layer was less than 1 µm, but two distinct reaction phases were clearly visible, similar to those observed in the liquid-state interfacial reactions.
Figure 5b–d present the interfacial results at 180 °C for 30 min, 6 h, and 24 h, respectively. After 30 min of aging, the overall reaction phases measured ~2 µm, with the dark reaction layer appearing relatively thicker than the bright one. As the aging time increased, the reaction phase gradually thickened. In
Figure 5c, the compositions of the dark phase showed slight variations: 51.2 at.%Sn-1.9 at.%Bi-2.9 at.%Se-44.0 at.%Te (near the solder side, point a) and 40.3 at%Sn-14.9 at.% Bi-3.7 at.%Se-41.1 at.%Te (near the Bi
2(Te,Se)
3 side, point b). Based on the correlated phase diagrams [
25,
26], these compositions are consistent with the SnTe phase, although the inner SnTe phase demonstrated a higher Bi solubility.
Additionally, the bright phase was identified as 3.7 at.%Sn-53.1 at.%Bi-3.2 at.%Se-40.0 at.%Te, corresponding to the BiTe phase with minor solubility of Sn and Se. Notably, there were numerous dispersed bright particles within the SnTe phase. The EPMA analysis revealed that they contained a very high Bi content, suggesting that they were the Bi-rich particles.
Similar interfacial microstructures were observed in the reaction after 24 h. The dark SnTe phase was ~11 µm, while the bright BiTe phase was ~2.4 µm. The presence of numerous tiny Bi-rich particles in the SnTe phase could be attributed to their precipitation due to oversaturation. The aging temperature was raised to 200 °C. The interfacial reaction behaviors showed no significant difference, but the IMC growth rate greatly accelerated. As shown in
Figure 6a, both the SnTe and BiTe layers were formed, with a combined thickness of ~3.4 µm after only 30 min of reaction. After 6 h of aging (
Figure 6b), the SnTe layer reached a thickness of ~10 µm, embedded with numerous Bi-rich particles, and exhibited a loose-structure with voids.
It is intriguing that a significant number of voids were observed in the SnTe phase during the solid-state interfacial reactions. This is likely attributed to liquation occurring during the solid-state reaction [
29]. With the eutectic temperature of Sn-Bi at only 139 °C, and the Bi saturation concentration in Sn being approximately 10 at.% at 160 °C and 4 at.% at 200 °C, the solder enters a two-phase equilibrium of Sn and liquid as Bi is oversaturated in Sn. As Bi diffuses and dissolves into the Sn solder, exceeding the saturated concentration, local liquation in the interfacial zone could occur in the solid-state reactions. Consequently, the local liquation could cause the solder to fill the voids within SnTe grains, resulting in a loosely structured SnTe. During sample etching, the solder was removed, revealing these voids.
To further investigate the IMC growth kinetics, the interfacial reactions were also conducted at 160 °C.
Figure 7a,b show the average thicknesses of the SnTe and BiTe layers, respectively, as a function of aging time at 160 °C, 180 °C, and 200 °C. In the natural logarithm plot of SnTe thickness versus aging time, the
n values were determined to be 0.49, 0.49, and 0.51 for the reactions at 160 °C, 180 °C, and 200 °C, respectively. These
n values were very close to 0.5, indicating that the SnTe growth was govern by diffusion and followed a parabolic relationship with aging time. Assuming the growth model with
n = 0.5, the plot of the average thickness of SnTe versus the square root of aging time is depicted in
Figure 7c. The data showed a good fit of linear regression, with
R2 values (the coefficient of determination) exceeding 0.99. The diffusion-controlled growth rate constants,
kdiff, can be determined from the linear-fitting slopes. The
kdiff values were 0.0614, 0.038, and 0.0246 µm/s
0.5 at 200 °C, 180 °C, and 160 °C, respectively.
The growth rate constants increased with increasing aging temperature. To analyze the temperature dependent of the growth rate constants, it can be described by the Arrhenius equation:
where
k0 is the temperature-independent pre-exponential factor,
Q is the activation energy,
R is the universal gas constant, and
T is the absolute temperature. The Arrhenius plot presented in
Figure 7d indicated that the activation energy was 38.9 kJ/mol and the pre-exponential factor,
k0, was 0.0012 m/s
0.5. These kinetics parameters can help predict the growth rate constants at different temperatures. For instance, the growth rate constant at 120 °C was estimated to be 0.0081 µm/s
0.5. In comparison, in the Sn/p-type (Bi,Sb)
2Te
3 reaction, the SnTe growth was rapid and linear with aging time, suggested that it was reaction-controlled. The activation energy was quite high, 151.6 kJ/mol. Accordingly, the n-type Bi
2(Te,Se)
3 reaction was relatively lower, indicating that the SnTe growth is less sensitive to temperature changes.
Figure 8a–c schematically illustrate the reaction process of the solid-state Sn/Bi
2(Te,Se)
3 reactions. In
Figure 8a, both the thin SnTe and BiTe layers are initially formed during the short-time soldering. The Bi from the Bi
2(Te,Se)
3 substrate is dissolved into the solder and precipitates as tiny Bi particles in the vicinity of the interface. As shown in
Figure 8b, the dominant diffusion species of Sn diffuses and reacts with the Te atoms, which diffuses across the thin BiTe layer from the Bi
2(Te,Se)
3 substrate, resulting in the formation of the SnTe phase. The BiTe layer is passively formed and hinders the Sn atoms, thus acting as a diffusion barrier for the Te atoms. Additionally, the dispersed Bi particles in the solder gradually grow in size. With the reaction progressing, the SnTe layer continued to grow, while the BiTe layer maintain a thickness of ~2.5 µm at 180 °C and 200 °C after 360 h. In certain local regions, the BiTe phase appeared to become thinner in the later stages of the reaction, suggesting the occurrence of BiTe decomposition. As illustrated in
Figure 8c, the diffusing Sn atoms could react with the BiTe phase, leading to the decomposition of the BiTe layer to form the SnTe phase and oversaturated Bi particles. Consequently, the SnTe phase exhibits two distinct microstructures, with a significant number of small Bi-rich particles embedded within the region near the BiTe layer.
In the Sn/p-type (Bi,Sb)
2Te
3 reactions, both the SnTe and SnSb phases were fast formed with linear growth rates of 15.1 μm/h and 4.3 μm/h, respectively, at 180 °C [
23]. In comparison, the growth of IMCs in the reactions involving n-type Bi
2(Te,Se)
3 was significantly suppressed. To further examine the influence of Se and Sb additives on the IMC growth, the interfacial reactions of Te with Sn, Sn-1wt.%Sb, and Sn-1wt.%Se were conducted at 180 °C for 6 h, as shown in
Figure 9a–c. The thicknesses of the formed SnTe phases were ~12 µm, ~12 µm, and ~4 µm, respectively. It is evident that the Se additive in the solder inhibits IMC growth, while the Sb additive shows no significant influence. Moreover, the reactions of Sn with Sb
2Te
3 and Te
4.7Se
0.3 were also performed for comparison, as shown in
Figure 9d,e. The overall thicknesses of SnTe and SnSb layers in the Sb
2Te
3 reaction was approximately 55 μm. In contrast, the SnTe phase formed in the Te
4.7Se
0.3 reaction was only around 2 μm. The results clearly indicated that the presence of the Se additive in the Te substrate would greatly inhibit the IMC growth, while it was notably enhanced with the Sb additive. As a result, there was a significant difference in IMC growth between reactions involving p-type (Bi,Sb)
2Te
3 and n-type Bi
2(Te,Se)
3 substrates. However, the underlying inhibiting mechanism of the Se additive remains unclear and requires further investigation.
3.3. SAC305/n-Type Bi2(Te,Se)3 Interfacial Reactions
The interfacial reactions of Bi
2(Te,Se)
3 substrate with SAC305 solder were conducted at 250 °C. In
Figure 10a, after 1 min of reaction, similar to the Sn/Bi
2(Te,Se)
3 reactions, two reaction phases layers of SnTe and BiTe were observed. The dark SnTe phase, exhibiting a scallop morphology, was predominant. As the reaction time increased to 10 min and 30 min, as displayed in
Figure 10b and
Figure 10c, respectively, not only did the IMC layers grow thicker, but also the grains of SnTe gradually coarsened. Additionally, the Bi precipitates were also observed within the SnTe phase. In fact, Bi contained in the SnTe phase would gradually dissolve to the molten solder. Consequently, the number of Bi-rich particles in the 10-min case was much higher than that of the 30-min case.
Figure 11a shows the growth of SnTe and BiTe layers over time. In the natural logarithm plot, the
n value for the SnTe growth was 0.6, indicating that it was nearly diffusion-controlled. As illustrated in
Figure 11b, the
kdiff was determined to be 0.17 μm/s
0.5. This value was slightly lower compared to the reactions with Sn.
The SAC305/Bi
2(Te,Se)
3 reactions were further conducted at 180 °C for various durations ranging from 1 h to 24 h. The interfacial microstructures resembled those observed in the Sn/Bi
2(Te,Se)
3 reactions. Besides the gradual growth of IMCs, there was no significant evolution in the interfacial morphologies.
Figure 10d illustrates the reaction at 180 °C for 6 h. Both the SnTe and BiTe phases were present at the interface. The bright BiTe phase was characterized by its composition: 1.3 at.%Sn-49.9 at.%Bi-3.5 at.%Se-44.3 at.%Te-0.4 at.%Ag-0.6 at.%Cu. The SnTe phase exhibited two distinct regions, with the one adjacent to the BiTe side containing numerous bright particles. Its composition contained 38.7 at.%Sn-15.1 at.%Bi-2.0 at.%Se-40.2 at.%Te-0.2 at.%Ag-3.8 at.%Cu, indicating that it was the SnTe phase mixed with tiny Bi-rich particles. Additionally, it was noted that the Cu content was higher than Ag, suggesting the facile diffusion and dissolution of Cu into the SnTe phase.