3.2. Microstructure of Sintered CoCrFeNiNb and CoCrFeNiV HEAs
Figure 2a,b show the XRD patterns of sintered CoCrFeNiNb and CoCrFeNiV HEAs at different temperatures, indicating that alloying elements significantly has a substantial impact on the phase composition and stability of the HEAs. In
Figure 2a, the CoCrFeNiNb HEA exhibits a dual-phase structure, comprising a primary FCC phase and a secondary Laves phase. The addition of Nb was found to promote the formation of the Co
2Nb-type Laves phase, which has a hexagonal close-packed (HCP) crystal structure with lattice parameters of
a = 0.4835 nm and
c = 0.7860 nm [
24]. The presence of the Laves phase suggests that Nb acts as a stabilizer for the intermetallic phase, thereby enhancing the alloy’s strength [
24]. In
Figure 2b, the CoCrFeNiV HEA exhibits an FCC phase and a σ phase. The formation of the σ phase is attributed to the metallic V element, which has very negative enthalpies of mixing with Co, Ni, and Fe, promoting the formation of an FCC solid solution with these elements. However, Cr, which is not fully dissolved in the solid solution, preferentially forms the σ phase with V [
25]. It is acknowledged that both the Laves phase and the σ phase are capable of enhancing hardness but may reduce ductility. The presence of these phases indicates that Nb and V act as strong stabilizers for the intermetallic phases, contributing to the overall strengthening of the HEAs.
Figure 2c,d show the EDS elemental mapping and the corresponding SEM images of sintered CoCrFeNiNb and CoCrFeNiV HEAs at 1100 °C with a holding time of 15 min. In
Figure 2c, the CoCrFeNiNb HEA exhibits two distinct regions in the SEM image, characterized by light gray and dark gray regions, respectively. The XRD analysis confirmed the presence of FCC and Laves phases, which is consistent with the EDS results. The light gray region is enriched in Nb, indicating the formation of the Co
2Nb-type Laves phase, while the dark gray region shows higher concentrations of Cr, Fe, and Ni, corresponding to the FCC phase. The point scan analysis (bar chart) in
Figure 2c further confirms these observations. In the CoCrFeNiNb system, Nb has very negative enthalpies of mixing with other metallic elements, which promotes the formation of stable intermetallic compounds. As a result, Nb tends to form the Co(Ni, Fe, Cr)
2Nb-type Laves phase rather than an FCC solid solution. This observation is consistent with the findings of previous studies [
26]. The CoCrFeNiV HEA exhibits a similar microstructure, as evidenced by the presence of light gray and dark gray regions observed in the SEM image. EDS mapping and the point scan results indicate that the light gray region corresponds to the FCC phase, with a uniform distribution of Cr, Co, Fe, and Ni. In contrast, the dark gray region is enriched in V, indicating the formation of the σ phase, which is consistent with the XRD pattern shown in
Figure 2b. Similar to the CoCrFeNiNb HEA, the elements, V and Cr, tend to segregate and form the σ phase, while Co, Fe, and Ni remain within the FCC matrix. These observations demonstrate that the formation of intermetallic phases, including the Laves and σ phases, is driven by the segregation behavior of Nb and V, respectively.
As illustrated in
Figure 2e,f, the TEM microstructure of CoCrFeNiNb and CoCrFeNiV HEAs confirms the dual-phase structures that were previously observed in SEM and XRD analyses. In
Figure 2e, the bright-field TEM image of the CoCrFeNiNb HEA shows a conventional dual-phase structure, where the FCC matrix appears as light gray regions and the Laves phase manifests as darker grains. The selected area electron diffraction (SAED) pattern from Region A, along the [
01]
FCC zone axis, confirms the FCC structure. The SAED pattern from Region B, along the [11
6]
Laves Laves zone axis, confirms the Co
2Nb-type Laves phase. The distribution of the Laves phase within the FCC matrix provides reinforcement and contributes to a balanced combination of strength and ductility. In
Figure 2f, the TEM image of the CoCrFeNiV HEA reveals a similar dual-phase structure, comprising of the FCC matrix and the σ phase. The SAED pattern from Region A, situated along the [
10]
FCC zone axis, confirms the FCC phase, while the pattern from Region B, positioned along the [1
1]
σ zone axis, corroborates the presence of the σ phase. The σ phase is distributed along grain boundaries and within the FCC grains, which is consistent with the findings obtained by SEM. This phase distribution suggests that V and Cr tend to segregate and form the σ phase, while the remaining elements stabilize the FCC matrix.
To further investigate the phase distribution and grain size, EBSD characterization was performed on the bulk CoCrFeNiNb and CoCrFeNiV HEAs (
Figure 3). As illustrated in
Figure 3a, the phase distribution of the CoCrFeNiNb HEA is depicted, with the red areas denoting the FCC phase, the blue areas indicating the Laves phase, and the black unindexed regions corresponding to pits caused by over-etching during the sample preparation process [
27].
Figure 3b shows the grain distribution map of the CoCrFeNiNb HEA, illustrating the spatial arrangement and orientation of FCC and Laves grains within the alloy microstructure. The map is consistent with the phase distribution shown in
Figure 3a, in which the FCC phase is predominantly distributed throughout the microstructure with finer Laves grains found within it. This observation is further quantified in
Figure 3c,d, which provide the grain size statistics for the FCC and Laves phases, showing average grain sizes of 1.81 ± 1.18 µm for the FCC phase and 1.10 ± 0.93 µm for the Laves phase, respectively. The finer and more uniform distribution of Laves grains suggests its role as a strengthening phase within the FCC matrix, contributing to enhanced mechanical properties.
Figure 3e shows the phase distribution of the CoCrFeNiV HEA, where the red areas represent the FCC phase, the yellow areas indicate the σ phase, and the black unindexed regions denote areas where indexing was not possible. The dominance of the FCC phase is evident, while the σ phase manifests isolated regions distributed along grain bounda-ries and within the FCC matrix. This phase distribution aligns well with the earlier SEM and XRD analyses, thus confirming the coexistence of FCC and σ phases.
Figure 3f pre-sents the grain distribution map, revealing a more heterogeneous particle size distribu-tion for FCC and σ phases compared to the CoCrFeNiNb HEA.
Figure 3g,h provide further quantification of the grain sizes, showing an average grain size of 0.60 ± 0.32 µm for the FCC phase and 0.39 ± 0.11 µm for the σ phase. The finer grain size of the σ phase, despite its lower abundance, indicates its potential to strengthen the alloy locally. However, its uneven distribution and limited presence suggest that its impact on the overall mechanical properties might be minimal compared to the FCC phase, which dominates the microstructure and contributes significantly to ductility and toughness. Compared to the mechanically alloyed powders (
Figure 1c–f) with particle sizes of several micrometers, the SPS-processed samples retained a significantly refined grain structure (~0.39–1.81 μm), demonstrating that the rapid heating and short sintering time effectively suppress grain growth.
In comparison with CoCrFeNiNb and CoCrFeNiV HEAs prepared by using conventional melting methods, the MA and SPS approach results in more uniform grain distribution and significantly finer grain sizes. For reference, the grain sizes of similar CoCrFeNi-based HEAs prepared via arc melting typically exceed 10 μm [
28,
29], whereas the SPS-processed samples in this study exhibited average grain sizes below 2 μm. The rapid heating and short holding times of SPS effectively limit grain growth, leading to a refined microstructure. It is anticipated that this refined grain structure will enhance the mechanical properties, including strength and toughness through grain boundary strengthening. These findings are consistent with earlier SEM and TEM observations, which demonstrate that mechanical alloying and SPS are effective in tailoring the microstructure to achieve superior performance in comparison to conventional melting techniques. While SPS currently encounters challenges in scaling up to large-sized components relative to traditional methods, continued advancements in large-scale SPS systems and mold engineering are anticipated to effectively address these issues and further expand the applicability of this technique in practical manufacturing.
3.3. Mechanical Properties of CoCrFeNiNb and CoCrFeNiV HEAs
Figure 4 illustrates the variation in hardness, relative density, and compressive stress–strain curves of CoCrFeNiNb and CoCrFeNiV HEAs at different sintering temperatures. The data presented in
Figure 4a–d were derived from the detailed measurements of compressive strength and density in
Table 1 and
Table 2, which have been consolidated here for the sake of clarity.
As shown in
Figure 4a,c, the hardness and relative density exhibit a tendency to initially increase with rising temperature, reaching a maximum at 1000 °C, followed by a decline at 1100 °C. At 800 °C, the CoCrFeNiNb HEA exhibits a hardness of approximately 3.08 GPa and a relative density of 79.6%, while the CoCrFeNiV HEA achieves higher values of 3.76 GPa and 87.1%, respectively. At this temperature, the incomplete solidification of the alloy powders gives rise to the formation of alloy blocks with relatively low density and hardness. As the sintering temperature is increased to 1000 °C, the CoCrFeNiNb HEA achieves a hardness of approximately 6.89 GPa and a relative density nearing 99.0%. Similarly, the CoCrFeNiV HEA reaches a hardness of about 5.86 GPa and a relative density of 99.1%. This improvement in hardness and densification can be attributed to the accelerated solid-state diffusion and sintering kinetics at this temperature, which promote the formation of fully densified alloy blocks with minimized porosity. However, further increasing the sintering temperature to 1100 °C results in a noticeable decline in both properties for both HEAs. This decline is primarily caused by the volatilization of elements with low melting points and highly volatility, as well as the introduction of impurities during high-temperature sintering. Moreover, the process of grain coarsening, occurring as a consequence of prolonged exposure to high-temperature conditions, leads to the generation of residual porosity. This, in turn, has a detrimental effect on the density and hardness of the alloys [
30].
Figure 4b,d show the room-temperature compressive stress–strain curves of CoCrFeNiNb and CoCrFeNiV HEAs at different sintering temperatures. Both alloys exhibit brittle fracture behavior under compressive loading at all sintering temperatures. At 800 °C, the ultimate compressive strength (σ
max) of CoCrFeNiNb and CoCrFeNiV HEAs is approximately 396 MPa and 721 MPa, respectively, with corresponding fracture strains (ε
f) of about 4.8% and 9.5%, respectively. These relatively poor compressive properties are primarily due to the incomplete densification of the alloys at this temperature. This results in insufficient bonding between the alloy particles and increased porosity, which weakens the material under compressive loading. When the sintering temperature is increased to 1000 °C, both alloys demonstrate significant improvement in compressive properties. The CoCrFeNiNb HEA achieves an ultimate compressive strength (σ
max) of 2201 MPa and a fracture strain (ε
f) of 17.5%, while the CoCrFeNiV HEA exhibits a compressive strength of 1835 MPa and a fracture strain of 16.5%. These enhancements are attributed to effective densification and solidification at this temperature, which minimize residual porosity and promote microstructural homogeneity. Based on the values reported in the literature, these strength levels are significantly higher than those of typical engineering alloys such as 316L stainless steel (~940 MPa) [
31]. In addition to surpassing conventional engineering alloys, the MA + SPS-processed CoCrFeNiNb and CoCrFeNiV HEAs also exhibit superior mechanical performance compared to similar FeCoCrNi-based HEAs fabricated via arc melting. For instance, a B-free AlFeCoNi HEA synthesized via vacuum arc melting exhibited a compressive strength of ~850 MPa and a fracture strain of ~7% [
32]. These results underscore the advantages of MA + SPS in achieving both high strength and ductility through improved densification and microstructural control.
The excellent compressive strength of the FeCoCrNiNb/V high-entropy alloy prepared in this study can be attributed to multiple factors. Firstly, the mutual diffusion and solid solution of different atoms contribute to the formation of a stable solid solution phase, providing substantial solid solution strengthening. Secondly, the rapid heating and cooling rates, along with the short holding times characteristic of SPS, effectively suppress grain growth, resulting in a refined microstructure with fine grains. Thirdly, the addition of elements with large atomic radii, such as Nb and V, facilitates the formation of secondary precipitate phases, including the Laves and σ phases. These precipitates serve as effective barriers to dislocation motion, thereby enhancing the alloy’s strength through a process known as precipitation hardening. Despite these enhancements, the compressive strength of the CoCrFeNiNb HEA exceeds that of the CoCrFeNiV HEA. Evidence from EBSD observations suggests that the uniform distribution of Laves phases in CoCrFeNiNb enhances its load-bearing capacity, thereby contributing to its superior compressive strength. In contrast, the CoCrFeNiV HEA exhibits a lower abundance of σ phases, and their uneven distribution limits their overall strengthening effect.
To investigate the fracture behaviors, the compressive fracture morphologies of CoCrFeNiNb and CoCrFeNiV HEAs at different sintering temperatures were analyzed (
Figure 5). At 800 °C (
Figure 5a,e), severe cracks and numerous unsintered powder particles are observed at the fracture site, indicating incomplete densification. As the sintering temperature increases to 900 °C (
Figure 5b,f), the bonding between alloy particles is enhanced as the powders begin to solidify. However, residual porosity and incomplete densification remain evident. At 1000 °C, the alloy powders achieve a high degree of densification, as evidenced by the fracture morphologies, as shown in
Figure 5c,g. While residual pores remain visible, their distribution and size vary due to differences in magnification and material composition. The fracture surfaces predominantly exhibit brittle characteristics, with flat regions and layered structures indicative of a transgranular fracture mechanism. As the temperature is increased to 1100 °C, distinct granular precipitates (highlighted as “particles” in
Figure 5d) become prominent on the fracture surface of the CoCrFeNiNb HEA. These precipitates, exhibiting a weak bond to the matrix, detach under compressive stress, resulting in a localized stress concentration. Additionally, the presence of larger pores, caused by grain coarsening and volatilization of low-melting-point phases, exacerbates the process of crack initiation and propagation. For the CoCrFeNiV HEA at 1100 °C, the fracture surfaces also display brittle characteristics with layered features and limited plastic deformation, while granular precipitates similar to those observed in the CoCrFeNiNb HEA are not clearly visible at the current magnification. The observed residual porosity and brittle fracture features indicate that microstructural defects remain a dominant factor in the initiation and propagation of cracks.
3.4. Electrochemical Corrosion Behavior and Resistance Mechanisms of CoCrFeNiNb and CoCrFeNiV HEAs
Figure 6a shows the potentiodynamic polarization curves of CoCrFeNi, CoCrFeNiNb, and CoCrFeNiV HEAs in a 3.5 wt.% NaCl solution at 25 °C. The polarization behavior demonstrates that the anodic current density varies with the applied potential for all three alloys. It is evident that none of the alloys exhibit clear passivation during anodic polarization, suggesting the partial breakdown of passive films in the chloride-rich environment. Tafel polarization analysis (
Table 3) provides the key corrosion resistance parameters, including corrosion current density (I
corr) and corrosion potential (E
corr), which reflect the corrosion rate and the alloy’s tendency to resist corrosion, respectively [
33]. Among the three HEAs, the CoCrFeNiNb alloy exhibits the lowest corrosion current density (3.055 μmA/cm
2) and a relatively higher corrosion potential (−0.296 V), indicating its superior corrosion resistance. Conversely, the CoCrFeNi HEA demonstrates the highest corrosion current density (3.698 μmA/cm
2) and the most negative corrosion potential (−0.378 V), indicating its lower resistance to corrosion. The enhanced corrosion resistance of CoCrFeNiNb and CoCrFeNiV HEAs is primarily attributed to the addition of Nb and V. These elements contribute to the formation of protective oxide films, such as Nb
2O
5 and V
2O
3, which act as stable barriers against aggressive chloride ions. Furthermore, the presence of Laves and σ phases in the microstructure plays a critical role. These precipitated phases provide localized sites for the formation of dense oxide layers, thereby further stabilizing the passive film and enhancing the alloys’ electrochemical stability. The combined effect of these factors significantly reduces the corrosion rate, thereby enhancing the resistance of the HEAs in chloride-containing environments.
Figure 6b–d illustrates the potentiodynamic polarization curves, equivalent electrical circuit, Nyquist plots, and Bode plots for CoCrFeNi, CoCrFeNiNb, and CoCrFeNiV high-entropy alloys (HEAs) in a 3.5 wt.% NaCl solution under their respective open-circuit potential (OCP) conditions. The equivalent electrical circuit used to fit the EIS data is shown in the upper right corner of
Figure 6b. In this model, Rs represents the solution resistance, Rct denotes the charge transfer resistance, and CPE (constant phase element) accounts for the non-ideal capacitive behavior of the electrode/electrolyte interface. This circuit is generally employed to describe the electrochemical behavior of passive films on metal surfaces in chloride-containing environments. The Nyquist plots (
Figure 6b) show that CoCrFeNiNb and CoCrFeNiV HEAs exhibit larger semicircle diameters compared to CoCrFeNi, implying higher charge transfer resistance and thus improved corrosion performance. This observation is supported by quantitative fitting using the equivalent circuit model (also shown in
Figure 6b). The fitted EIS parameters are presented in
Table 4, where CoCrFeNiNb and CoCrFeNiV show significantly higher Rct values (2.09 × 10
6 Ω·cm
2 and 1.53 × 10
6 Ω·cm
2, respectively) than CoCrFeNi (6.4 × 10
5 Ω·cm
2). These values confirm the beneficial effect of Nb and V in promoting more stable passive films. In addition, the fitted CPE parameters (Y
0 and n) suggest that the oxide layers formed on Nb- and V-containing HEAs are more capacitive and uniform, further contributing to their superior electrochemical performance. The Bode plots (
Figure 6c,d) provide further support for the findings of the Nyquist plot. In the low-frequency region, CoCrFeNiNb and CoCrFeNiV HEAs exhibit higher phase angles and impedance modulus values compared to the CoCrFeNi HEA. It has been demonstrated that higher phase angles in the low-frequency region are indicative of the formation of a more stable and compact passive film, which serves as an effective barrier against chloride ion penetration [
34]. The larger impedance modulus values also indicate improved surface film stability, which enhances the corrosion resistance of the alloys. In summary, the EIS analysis demonstrates that the CoCrFeNiNb and CoCrFeNiV HEAs possess superior electrochemical stability and corrosion resistance in chloride-containing environments. Furthermore, it is evident that CoCrFeNiNb exhibits the most robust passive film formation and the highest charge transfer resistance.
Figure 7 presents the EDS elemental mapping results of CoCrFeNiNb and CoCrFeNiV HEAs after electrochemical corrosion in a 3.5 wt.% NaCl solution. The results show that both alloys exhibit localized corrosion as the dominant mechanism, with no significant pitting observed on their surfaces. In
Figure 7a, representing the CoCrFeNiNb HEA, the elements of Co, Cr, Fe, and Ni are distributed uniformly within the FCC matrix, while Nb is enriched in specific regions corresponding to the Laves phase. The FCC phase is observed to be more prone to corrosion compared to the Laves phase, which exhibits higher resistance due to the formation of a stable Nb
2O
5 oxide layer that acts as a protective barrier against chloride ions. Similarly,
Figure 7b shows the EDS mapping for the CoCrFeNiV HEA, illustrating an even distribution of Co, Cr, Fe, and Ni in the matrix with V exhibiting enrichment in regions corresponding to the σ phase. The σ phase shows greater corrosion resistance in comparison to the surrounding FCC matrix, likely due to the formation of a V
2O
3 oxide layer that mitigates chloride ion attack.
Both HEAs exhibit preferential corrosion of the FCC phase, while the precipitated phases remain relatively intact. This behavior is typical of dual-phase alloys, where differences in electrochemical stability between phases create galvanic coupling, accelerating corrosion in the more active FCC matrix. The comparison between CoCrFeNiNb and CoCrFeNiV HEAs highlights that the addition of Nb or V enhances corrosion resistance by promoting the formation of stable oxide layers on the precipitated phases. These oxide films have an impact on the reduction in ion penetration and improvement of the electrochemical stability of the alloys in chloride-containing environments.
The XPS analysis confirms that the Nb-enriched Laves phase in the CoCrFeNiNb HEA and the V-enriched σ phase in the CoCrFeNiV HEA significantly enhance the corrosion resistance of the alloys by forming stable oxide layers. As shown in
Figure 8a, the Nb 3d spectrum of the CoCrFeNiNb HEA displays binding energies of 202.4 eV for metallic Nb (Nb
0 2d
5/
2) and 207.1 eV and 209.88 eV for Nb
5+ peaks, indicating the formation of Nb
2O
5. Similarly, the V 2p spectrum of the CoCrFeNiV HEA reveals binding energies at 513.6 eV and 521.2 eV for V
3+ peaks, thereby confirming the presence of V
2O
3 (
Figure 8c). These oxides form compact and continuous passive films that act as barriers against chloride ion penetration, reducing the corrosion rate and slowing down the propagation of corrosion pits. The O 1s spectra (
Figure 8b,c) further indicate that the passive films on both alloys contain a mixture of metal oxides and hydroxides. The main peaks at binding energies of approximately 530.1 eV and 531.8 eV correspond to O
2− species in metal oxides (Nb
2O
5 and V
2O
3) and OH
− species in hydroxides, respectively. The formation of stable oxides, such as Nb
2O
5 and V
2O
3, is critical in mitigating chloride ion attack by forming dense, protective layers that enhance the electrochemical stability of the alloys. In contrast, the FCC matrix, which is composed primarily of Fe, Co, Cr, and Ni, forms fewer protective oxides under the same conditions. Oxides such as Fe
2O
3, Co
3O
4, and NiO exhibit reduced stability in chloride-rich environments, thereby increasing the susceptibility of the FCC matrix to localized corrosion. This difference in oxide stability between the FCC phase and the precipitated phases elucidates the preferential corrosion observed in the FCC matrix, as evidenced by the surface morphology and EDS mapping results (
Figure 7).
XPS analysis highlights the critical role of the precipitated phases in enhancing the corrosion resistance of CoCrFeNiNb and CoCrFeNiV HEAs. The Nb-enriched Laves phase and V-enriched σ phase facilitate the formation of durable oxide films, which provide effective protection against aggressive chloride ions in corrosive environments. The formation of these heterogeneous passive films, which is achieved through a process of selective oxidation, contribute significantly to the alloys’ electrochemical stability and maintain their overall corrosion resistance in chloride-containing environments.