3.1. Sn/FeCoNiCr Reactions
Figure 1a–f present the BEI micrographs illustrating the interfacial microstructural evolution in the Sn/FeCoNiCr reactions at 250 °C over aging durations ranging from 10 min to 24 h. After 10 min of reaction, as shown in
Figure 1a, a reaction layer approximately 1.8 ± 0.4 µm thick forms at the interface, exhibiting a loose and porous microstructure. Notably, in the BEI imaging mode, the boundary between the reaction layer and the FeCoNiCr substrate appears blurry and irregular, rather than forming a well-defined, planar interface. This phenomenon is attributed to the non-uniform dissolution rates of the constituent elements in the FeCoNiCr MEA substrate. During the initial stage, the dissolution of the substrate into the molten solder is relatively more pronounced.
Figure 1b shows that after 30 min of aging, the reaction phase grew significantly thicker while retaining a porous and non-dense microstructure. This suggests that the reaction phase consisted of numerous grains, with the pore regions filled with solder. Notably, some larger grains were observed in the reaction phase near the solder. A similar phenomenon was observed in the 2 h sample, as shown in
Figure 1c, where the reaction phase particulates, approximately 10 µm in size, appeared to detach from the interface and disperse into the solder. EPMA analysis revealed that the reaction phase (point a) had a composition of 16.5 at.%Fe-9.2 at.%Cr-6.3 at.%Co-1.1 at.%Ni-66.9 at.%Sn. This composition corresponds to the FeSn
2 phase with high Cr and Co solubilities, and it was labeled as the (Fe,Cr,Co)Sn
2 phase in this study. The corresponding analysis results are presented in
Table S1. The composition of the reaction phase layer (point b) near the FeCoNiCr substrate was 12.7 at.%Fe-13.5 at.%Cr-5.6 at.%Co-1.0 at.%Ni-67.2 at.%Sn, which also corresponds to the (Fe,Cr,Co)Sn
2 phase.
As the reaction time was extended to 6 h, as shown in
Figure 1d, the interfacial (Fe,Cr,Co)Sn
2 layer with a porous structure exhibited no significant growth, while the severe dispersion of large and dense (Fe,Cr,Co)Sn
2 particulates was observed. This suggests that the interfacial (Fe,Cr,Co)Sn
2 layer underwent dissolution, leading to the grain growth of (Fe,Cr,Co)Sn
2 particulates in the solder. Further prolonging the reaction time to 12 h, as depicted in
Figure 1e, revealed more pronounced IMC spalling. Notably, the dispersion phases had two distinct contrasts. The dark phase had a round particulate structure, approximately 10 µm in size, whereas the bright phase had an unusually large plate-like structure, exceeding 100 µm in length. EPMA analysis identified the dark phase as (Fe,Cr,Co)Sn
2, while the bright phase was confirmed to be (Co,Ni)Sn
3.
The Sn/FeCoNiCr reaction at 250 °C after 24 h exhibited a similar interfacial microstructure. The (Fe,Cr,Co)Sn
2 phase layer, with a thickness of 6.5 ± 0.4 µm, was present at the interface. Additionally, (Fe,Cr,Co)Sn
2 particulates and chunky (Co,Ni)Sn
3 phases were dispersed in the solder matrix near the interface. The series of microstructural features observed at each time point were highly consistent across multiple independent specimens, demonstrating the high reproducibility of the interfacial reaction behavior. Furthermore, the reaction couple was deep-etched to completely remove the solder, exposing the IMC.
Figure 2a,b show the morphologies of FeSn
2 and CoSn
3, respectively. The (Fe,Cr,Co)Sn
2 grains displayed a well-faceted polyhedral shape with a diameter of approximately 10 µm, while the (Co,Ni)Sn
3 appeared as rectangular plate-like structures with sizes on the order of several hundred micrometers.
The XRD analysis presented in
Figure 2c shows that most of the distinct diffraction peaks correspond well to FeSn
2, confirming the presence of the (Fe,Cr,Co)Sn
2 phase. FeSn
2 has a body-centered orthorhombic structure (JCPDS #73-2030, S.G.
I4/mcm,
a = 0.6520 nm,
c = 0.5312 nm). The α-CoSn
3 has an end-centered orthorhombic structure (JCPDS #48-1813, S.G.
Cmca,
a = 1.686 nm,
b = 0.6268 nm,
c = 0.6270 nm). The XRD spectra of the (Co,Ni)Sn
3 phase revealed a strong peak at (12, 0, 0), indicating that the normal direction of the plate surface is aligned with the a-axis. These XRD spectra are consistent with the IMC phases observed at the interface.
The observed results indicate significant IMC spalling in the liquid-state Sn/FeCoNiCr interfacial reactions, suggesting unstable interfacial behavior. In contrast, a prior study [
30] on the Sn/FeCoNiCrMn reaction demonstrated the excellent interfacial stability, as no IMC spalling occurred even after prolonged reaction times. To further investigate and clarify the differences in interfacial behavior, the Sn/FeCoNiCrMn reactions were conducted at 250 °C.
Figure 3a–c show the interfacial microstructure of the Sn/FeCoNiCrMn reactions at 250 °C after 2 h, 12 h, and 24 h, respectively. As reported in the prior study [
30], the dense (Fe,Cr,Co)Sn
2 reaction phase exhibited no significant growth over the aging period. Notably, the (Fe,Cr,Co)Sn
2 phase layer remained highly stable without any IMC spalling. These observed interfacial results clearly demonstrate that CoNiCrMn possesses superior interfacial stability compared to FeCoNiCr.
Figure 3d shows the morphology of (Fe,Cr,Co)Sn
2 in the sample after 24 h of aging. In addition to the faceted columnar morphology exhibited by the (Fe,Cr,Co)Sn
2 grains, several large (Co,Ni)Sn
3 grains with plate-like morphologies were also observed. However, the formation of (Co,Ni)Sn
3 grains was sparse and relatively rare across the entire substrate. The initial formation of (Fe,Cr,Co)Sn
2, as presented in
Figure 3f, also exhibited a faceted pillar-like morphology, with grain diameters of approximately 0.5 µm. Additionally, several thin, plate-like grains were observed, suggested to be (Co,Ni)Sn
3, with sizes around 3.5 µm. By comparing
Figure 2a and
Figure 3d, it was found that the grain sizes of (Fe,Cr,Co)Sn
2 were similar in both systems, suggesting that the presence of Mn in the FeCoNiCrMn alloy did not significantly affect the nucleation and growth behavior of the (Fe,Cr,Co)Sn
2 phase, compared to the FeCoNiCr reaction.
EPMA analysis indicates that the (Fe,Cr,Co)Sn
2 phase contained high levels of Cr, moderate amounts of Co, and trace amounts of Ni and Mn. It suggests that most of the Ni and Mn from the substrate, along with a portion of the Co, preferentially dissolved into the solder, whereas Cr remained largely incorporated within the (Fe,Cr,Co)Sn
2 phase. The differing dissolution behaviors of these transition metals in molten Sn can be reasonably explained by their limiting partial molar enthalpies. The reported values for Fe, Cr, Co, Ni, and Mn in Sn are +34, +32, +1, −13, and −22 (kJ/mol), respectively [
32]. The positive values for Fe and Cr indicate repulsive interactions with molten Sn, which is consistent with the Sn–Fe and Sn–Cr phase diagrams, both exhibiting monotectic reactions and limited mutual solubility [
33,
34]. In contrast, the negative enthalpies for Ni and Mn suggest attractive interactions with Sn, promoting their dissolution. This behavior is also supported by the Sn–Ni and Sn–Mn phase diagrams [
35,
36]. Co, with an enthalpy value near zero, exhibits an intermediate dissolution behavior in Sn.
In both the FeCoNiCr and FeCoNiCrMn reactions, the dissolution of Co and Ni into molten Sn resulted in supersaturation, which subsequently led to the formation of (Co,Ni)Sn3. Interestingly, the dissolved Co and Ni atoms primarily contributed to the growth of a limited number of large, plate-like (Co,Ni)Sn3 grains. This observation suggests that the nucleation of (Co,Ni)Sn3 is kinetically hindered, likely due to a high nucleation barrier, leading to preferential growth on pre-existing sites rather than the widespread formation of fine grains. Furthermore, the amount of (Co,Ni)Sn3 formed in the FeCoNiCr system was significantly greater than that in the FeCoNiCrMn reaction. This difference can be attributed to the higher total concentration of Co and Ni (25 at.%) in FeCoNiCr compared to 20 at.% in FeCoNiCrMn, resulting in a greater availability of these elements for dissolution into Sn and subsequently enhancing the formation of (Co,Ni)Sn3.
3.2. Sn/FeCoNiMn Reactions
Figure 4a–f present the interfacial microstructures of the Sn/FeCoNiMn reactions aged at 250 °C for various durations. After 10 min of aging, as shown in
Figure 4a, a thin interfacial reaction layer with a thickness of 1.9 ± 0.2 µm was formed. Similar to the FeCoNiCr system, the interface between IMC and the FeCoNiMn MEA appeared blurry and irregular, which can be attributed to the non-uniform dissolution of the multiple constituent elements in the MEA. Upon extending the aging time to 2 h (
Figure 4b), significant interfacial evolution was observed. The reaction layer developed a porous structure, and numerous fine IMC particulates were dispersed within the solder region adjacent to the interface. At 6 h (
Figure 4c), in addition to the porous interfacial IMC layer and fine dispersed phases, a large bright phase emerged in the solder matrix. EPMA analysis revealed that the porous interfacial phase contained 8.7 at.% Co and 5.3 at.% Mn in the FeSn
2 structure, and it was thus designated as the (Fe,Co,Mn)Sn
2 phase. The bright chunky phase was identified as (Co,Ni)Sn
3. The corresponding EPMA data are summarized in
Table S2.
Figure 4d,e display the interfacial microstructures of the Sn/FeCoNiMn reaction after 12 h of aging. Several stripe-shaped (Co,Ni)Sn
3 phases, approximately 200 µm in length, were observed in the solder matrix, along with numerous fine (Fe,Co,Mn)Sn
2 particles dispersed near the interface. These fine IMC particulates are presumed to have spalled from the porous (Fe,Co,Mn)Sn
2 interfacial layer. After 24 h of reaction, a similar interfacial microstructure was maintained, as shown in
Figure 4f. The observed microstructural evolutions were highly consistent across all specimens, indicating excellent reproducibility. The consistent features observed across all specimens highlight the excellent reproducibility of the interfacial reaction behavior.
Figure 5a,b further present the grain morphologies of the (Fe,Co,Mn)Sn
2 and (Co,Ni)Sn
3, respectively. Remarkably, the (Fe,Co,Mn)Sn
2 grains exhibited a fine faceted pillar-like morphology with diameters below 1 µm, while the (Co,Ni)Sn
3 phase showed large, plate-like structures. Additionally, the XRD analysis shown in
Figure 5c confirms the formation of both Fe (Fe,Co,Mn)Sn
2 and (Co,Ni)Sn
3 phases on the FeCoNiMn substrate, consistent with the microstructural observations.
In comparison to the reactions involving the three substrates, i.e., FeCoNiCr, FeCoNiMn, and FeCoNiCrMn, the dispersed FeSn
2 phases exhibited distinct morphologies and behaviors, as illustrated in
Figure 6a–c. In the Sn/FeCoNiCrMn system (
Figure 6c), the interface remained stable, and no dispersed (Fe,Cr,Co)Sn
2 particles observed in the solder. In contrast, the Sn/FeCoNiCr system showed the significant dispersion of large (Fe,Co,Cr)Sn
2; particulates into the solder, while the Sn/FeCoNiMn reaction resulted in only fine, uniformly distributed (Fe,Co,Mn)Sn
2 particles. In the Sn/FeCoNiCr system, the interfacial (Fe,Cr,Co)Sn
2 phase layer likely underwent partial dissolution, followed by grain regrowth. Due to the strong repulsive interaction between Cr and molten Sn, the reprecipitated (Fe,Cr,Co)Sn
2 tends to form larger grains to minimize surface energy. As the reaction progressed, these destabilized IMCs detached from the interface and dispersed into the solder matrix, reflecting the interfacial instability driven by compositional and thermodynamic factors.
In contrast, as shown in
Figure 6b, numerous fine (Fe,Co,Mn)Sn
2 particles were observed dispersed within the solder in the Sn/FeCoNiMn system. This behavior is likely attributed to the attractive interaction between Mn and molten Sn, which facilitates Mn dissolution and may assist in the nucleation and stabilization of FeSn
2. Consequently, grain growth is suppressed, favoring the formation of finer (Fe,Co,Mn)Sn
2 particles. The finer morphology also results in a higher surface area-to-volume ratio, which further enhances the thermodynamic favorability of Mn–Sn interactions. On the other hand, the Sn/FeCoNiCrMn reaction exhibited a highly stable interfacial microstructure, with no (Fe,Cr,Co)Sn
2 particles dispersed in the solder. This suggests a synergistic effect between Cr and Mn on interfacial stability. While Mn promotes elemental dissolution into molten Sn, Cr exhibits a strong repulsive interaction with Sn, thereby suppressing dissolution. As a result, Fe and Cr atoms are predominantly retained in the interfacial IMC layer, effectively preventing spallation and the dispersion of the (Fe,Cr,Co)Sn
2 phase into the solder. Overall, the distinct interfacial behaviors among the three systems are governed by the dissolution tendencies of the HEA constituent elements and their thermodynamic affinities with Sn. The competitive effects of Cr and Mn play a pivotal role in determining the morphology, distribution, and stability of the interfacial IMCs.
3.3. SAC305/FeCoNiCr Reactions
The FeCoNiCr MEA substrate was also reacted with SAC305 solder at 250 °C. As displayed in
Figure 7a, an irregular IMC phase began to spall into the solder matrix after 2 h of aging. The EPMA analysis results, summarized in
Table S3, indicate that the composition of the interfacial region (point a) was 17.4 at.%Fe-10.2 at.%Cr-3.2 at.%Co-66.0 at.%Sn, along with trace amounts of 1.7 at.%Cu and 1.6 at.%Ni, corresponding to the (Fe,Cr,Co)Sn
2 phase. In contrast, a nearby small dispersed particle (point b) exhibited a composition of 18.2 at.%Fe-7.3 at%Co-4.2 at.%Cu-1.9 at.%Cr-1.8 at.%Ni-66.5 at.%Sn. This IMC was identified as an FeSn
2-type compound enriched in Co and Cu, with only minor Cr and Ni content, and is thus designated as (Fe,Co,Cu)Sn
2. Although both IMCs were classified as FeSn
2-type phases, they exhibited distinctly different chemical compositions. The dispersed IMC phase contained significantly higher Co and Cu contents and much lower Cr content, compared to the interfacial phase. When the reaction time was extended to 6 h (
Figure 7b), a slight thickening of the interfacial (Fe,Cr,Co)Sn
2 was observed, accompanied by a more pronounced spallation of (Fe,Co,Cu)Sn
2 into the solder matrix.
After 12 h of reaction, as shown in
Figure 7c, a similar interfacial microstructure was observed. According to the EPMA results (
Table S3), the dispersed IMC phase of (Fe,Co,Cu)Sn
2 contained lower Cr content but higher Co and Cu contents, compared to the interfacial (Fe,Cr,Co)Sn
2 layer. The Cu present in the dispersed (Fe,Co,Cu)Sn
2 phase originated from the SAC305 solder, indicating that Cu atoms substituted into Fe lattice sites within the FeSn
2 structure. This substitution likely enhanced the phase stability of the IMC. Compared to the large dispersed (Fe,Cr,Co)Sn
2 phase observed in the Sn/FeCoNiCr reaction (
Figure 1d), the dispersed (Fe,Co,Cu)Sn
2 phase formed in SAC305 exhibited a markedly finer microstructure. This observation suggests that the Cu addition promotes the nucleation of finer IMC particles, possibly by lowering the interfacial energy and stabilizing smaller grains. In contrast, Cr addition appears to favor the formation of larger IMC particulates, likely due to its repulsive interaction with molten Sn. Such repulsion suppresses the formation of smaller grains and facilitates the coarsening or growth of larger ones.
For comparison,
Figure 8a,b show the interfacial microstructures in SAC305/FeCoNiCrMn reaction at 250 °C after aging for 2 h and 24 h, respectively. As reported in the prior study [
30], the interface remained highly stable, with no significant microstructural evolution, and only a few (Fe,Cr,Co)Sn
2 grains were observed dispersed in the solder near the interface. Similar to the reactions with Sn, the FeCoNiCrMn HEA exhibited superior interfacial stability compared to the FeCoNiCr MEA. Furthermore, the morphology of the (Fe,Cr,Co)Sn
2 grains is shown in
Figure 8c, consisting of a mixture of large faceted grains and small ones. In comparison to the Sn/FeCoNiCrMn system, the reduced grain size of (Fe,Cr,Co)Sn
2 in the SAC305 solder is likely attributed to the presence of Cu, which may promote IMC nucleation and inhibit grain coarsening.
3.5. Contact Angle Analysis of SAC305 Solder on MEA/HEA Substrates
The wettability between SAC305 solder and MEA/HEA substrates was evaluated through contact angle measurements, as shown in
Figure 10a–c. Among the three substrates, the FeCoNiMn substrate exhibited the lowest contact angle (27 ± 1°), indicating superior wettability, while FeCoNiCr showed the highest (40 ± 1°). The contact angle for FeCoNiCrMn (38 ± 1°) was slightly lower than that of FeCoNiCr, which may be attributed to the reduced Cr content or the beneficial influence of Mn addition on interfacial wettability. This difference in wettability can be explained by Young’s equation:
Here,
,
, and
refer to the solid–vapor, solid–liquid, and liquid–vapor surface energies, respectively, and
θ is the contact angle, as illustrated in
Figure 10b. Since the liquid–vapor surface energy (
) of SAC305 is constant in all cases, variations in contact angle primarily reflect changes in solid–liquid interfacial energy (
). A lower contact angle corresponds to a lower solid–liquid interfacial energy, indicating stronger interfacial affinity interactions and improved adhesion between the solder and substrate.
Figure 10.
Cross-sectional images showing the contact angles of SAC305 solder on different MEA/HEA substrates after reflow at 250 °C for 20 s in an argon atmosphere: (a) FeCoNiMn, (b) FeCoNiCr, and (c) FeCoNiCrMn. Figure (b) also illustrates the corresponding surface energy relationships derived from Young’s equation.
Figure 10.
Cross-sectional images showing the contact angles of SAC305 solder on different MEA/HEA substrates after reflow at 250 °C for 20 s in an argon atmosphere: (a) FeCoNiMn, (b) FeCoNiCr, and (c) FeCoNiCrMn. Figure (b) also illustrates the corresponding surface energy relationships derived from Young’s equation.
The better wettability observed for FeCoNiMn is consistent with thermodynamic data. Mn exhibits a higher affinity toward Sn, which reduces the solid–liquid interfacial energy (), enhances adhesion between the solder and substrate, and promotes the dissolution of the FeCoNiMn substrate into the solder. Conversely, Cr tends to form more stable native oxides and shows weaker affinity with Sn, leading to higher interfacial energy and poorer wettability, as evidenced by the higher contact angle on the FeCoNiCr substrate. These findings suggest that Mn addition improves interfacial adhesion and promotes more thermodynamically favorable solder spreading behavior, which may contribute to enhanced solder joint integrity.