While rhenium is an ideal material for rapid thermal cycling applications under high temperatures, such as rocket engine nozzles, its high cost limits its widespread use and prompts an exploration of viable cost-effective substitutes. In prior work, we identified a promising pool of candidate substitute alloys consisting of Mo, Ru, Ta, and W. In this work we demonstrate, based on density functional theory melting temperature calculations, that one of the candidates, Mo0.292Ru0.555Ta0.031W0.122, exhibits a high melting temperature (around 2626 K), thus supporting its use in high-temperature applications.
Among refractory metals, rhenium demonstrates a unique combination of desirable thermodynamic and mechanical properties: a high melting point (3448 K), excellent high-temperature strength, a good ablation and creep resistance, and no ductile-to-brittle transition1,2. The concurrence of low-temperature ductility and high-temperature strength makes Re-based alloys competitive candidates for structural materials with applications such as rocket engine nozzles, which involve rapid thermal cycling under high temperatures. However, rhenium is a rare element and its high cost limits its widespread use3,4. This situation has prompted the exploration of practical and efficient replacement for rhenium in rocket engine nozzle applications.
Previously, we showed that a straightforward design principle that trades off average valence electron count and cost considerations is useful in recognizing a favorable group of possible substitutes, the Mo–Ru–Ta–W quaternary alloys5, based on a thermodynamic model that integrates electronic structure calculations with the Calphad framework6, as well as through experimental synthesis and structural characterization of samples chosen in a favorable composition range. The computational thermodynamic model enabled the identification of alloy compositions on a so-called Re-equivalent plane that also preserve rhenium’s hcp structure, and thus its desirable mechanical properties7. In other words, based on a rigid-band model, promising alloys have a composition on a Re-equivalent plane on which the average number of valence electrons per atom equals that of Re. The accuracy of this simple picture was assessed through high-throughput ab initio thermodynamic calculations, and with comparisons to established binary phase diagrams sections, and further corroborated by experimental synthesis and structural characterization demonstrating single-phase multiprincipal-element hcp solid-solution samples selected from a promising composition range. This region includes the Mo–Ru–Ta–W quaternary alloys having an hcp structure at compositions near Mo0.3Ru0.512Ta0.064W0.125 and near Mo0.292Ru0.555Ta0.031W0.122, which straddle the Re-equivalent plane. Although Ru is also somewhat expensive, including it allows us to add more of the inexpensive elements such as Mo and W, thus still resulting in a net cost reduction. These specific compositions were also synthesized experimentally and their mechanical properties investigated5,8. We also showed that the proposed Ru-based alloys exhibit better thermal compatibility with Ir, which serves as an oxidation-resistant coating.9. However, it remains to be demonstrated that this proposed alloy exhibits a sufficiently high melting point for its intended application. An experimental determination of the melting point is complicated by the high temperatures involved. These alloys may have the potential to replace higher cost elements, like Re, in relatively lower-temperature thruster applications where cost is a major driver but performance, such as ablation and erosion, is adequate.
In this work, we employ density functional theory (DFT)10,11,12 to calculate the melting temperature of Mo0.292Ru0.555Ta0.031W0.122. For accuracy assessment and improvement, we also compute the melting points of its constituting elements. We use an efficient small-cell coexistence method13 and its implementation in the SLUSCHI code14, based on DFT molecular dynamics (MD), as shown in Fig. 1. This highly cost-effective and robust method allows us to perform expensive melting point calculations on multiple materials directly from DFT.
As shown in Table 1, our calculations suggest the need to use accurate pseudo-potentials where semicore elections s and p states were treated as valence states. With only valence elections, the DFT melting point errors were 210, 170, 330, and 200 K for Mo, Ru, Ta, and W, respectively. When semicore p (including s for W) electrons were further relaxed, the errors were significantly reduced to 80, 60, 100, and 170 K, respectively. The high accuracy of the latter served as strong indication that our DFT melting point calculation model will also accurately generate melting properties of Mo0.292Ru0.555Ta0.031W0.122, a promising Re-substitute alloy.
The hcp solid structure of Mo0.292Ru0.555Ta0.031W0.122 was represented by a special quasi-random structure (SQS)15 of 64-atom Mo19Ru35Ta2W8. The mcsqs code16 was employed to generate the SQS. This SQS is then feed into the SLUSCHI code, which automates the melting point calculation process via the small-cell solid–liquid coexistence method. Duplicates of half-solid-half-liquid coexistence simulations were carried out at various temperatures, and solid–liquid probability distribution was analyzed to rigorously infer the final melting temperature. The calculated meting point of Mo19Ru35Ta2W8 is 2545 ± 26 K.
A recent study suggests that, due to underbinding, GGA may systematically underestimate melting point and thus GGA value may serve as a lower boundary of melting point17. We here make a melting temperature correction on Mo0.292Ru0.555Ta0.031W0.122, based on the known melting temperature errors of its alloying elements in pure form,
where xi is the composition of each alloying element, and ΔTi is the corresponding DFT melting point error. The correction is 81 K, and the melting temperature of Mo0.292Ru0.555Ta0.031W0.122 is thus estimated to be 2626 K. This is (slightly) lower than the weighted average of the elemental melting points (2850 K), thus suggesting a eutectic topology.
While this melting temperature of 2626 K is significantly lower than that of rhenium (3459 K), this is not expected to be a limiting factor in applications where rhenium is used in conjunction with an iridium coating to improve oxidation resistance. Iridium’s melting point is only 2719 K and thus becomes the more relevant limiting factor. Our proposed alloy’s melting point would thus only lower the maximum operating temperature by about 100 K. Note that a typical rhenium/iridium combustion chamber operates at temperatures from 1925 up to 2200 °C (2473 K)18, a temperature range our alloy should still be able to withstand without melting.
We should point out that the small-size coexistence method is inherently capable of finding the correct solid crystal structure, because the solid–liquid interface facilitates the nucleation of the structure with the lowest free energy even if we initially assumed the wrong solid. In other words, the method itself serves as a corroboration to verify the correct solid structure. In our simulation, we confirm that Mo0.292Ru0.555Ta0.031W0.122 remains in hcp structure, thus further corroborating our previous computational and experimental findings5.
In addition to Mo–Ru–Ta–W alloys, we also show that Ru–Re–Ta and Ru–Re–W alloys also have favorable high melting temperatures, as summarized in Table 1, while also remaining hcp structures. These results indicate that attempting to increase the alloy’s melting point by replacing the element with the lowest melting point (Mo) by Re does appear to be an effective strategy.
It should be emphasized that the melting point reported here formally corresponds to the temperature, where the liquid and solid-free energies cross at a given fixed composition. This is the case because, over the timescale of our simulations, the species do not have the time to segrate from one phase to another, which can be readily verified by inspecting the final composition profile of the runs which terminate in a fully solid state. The real system may melt incongruently (with the solid and liquid having different compositions and the melting transformation taking place over a range of temperatures.) Our reported temperature lies in between the liquidus and the solidus, by construction.
In this system, the liquidus and solidus are likely very close to each other and thus close to our reported temperature. This is supported by the facts that (i) the alloy’s main constituent (Ru) has a similar melting point (2550 K) as our composition of interest; (ii) additional calculations to estimate the melting at a composition near the middle point between Mo0.292Ru0.555Ta0.031W0.122 (m.p. 2542 K) and pure Ru suggest a melting point approximately 2500 K. Therefore, the liquidus and solidus are indeed likely to both be very flat near the composition range of interest.
To summarize, we demonstrate, based on DFT calculations, that a potentially promising rhenium substitute alloy, Mo0.292Ru0.555Ta0.031W0.122, exhibits a very high melting temperature of 2626 K, thus supporting its high-temperature applications. This prediction uses the known errors in the calculated melting temperature of the constituting elements to minimize any systematic bias. The calculations also corroborate our previous findings from both computation and experiment that Mo0.292Ru0.555Ta0.031W0.122 has an hcp structure.
Density functional theory melting point calculations
We use an efficient small-cell extension of the coexistence method13 and its implementation in the SLUSCHI code14, based on DFT MD. This highly efficient method makes it possible to perform, directly from first principles, expensive melting point calculations. The method runs solid–liquid coexisting simulations on small-size systems, and the melting temperatures are rigorously inferred based on statistical analysis of the system’s fluctuations, namely, the temperature-dependence of the probability that simulations terminate with the system in a fully liquid state. This probability can be calculated analytically as a function of unknown thermodynamic parameters (including the melting point) that can then be determined from a fit to the observed temperature-dependent probabilities13. The accuracy (typically with an error smaller than 100 K), robustness and efficiency of the method have been demonstrated in a range of materials13,14,19,20,21,22,23,24. In particular, the small-cell coexistence method13 and the SLUSCHI code14 was employed to computationally predict the material with the highest melting point, which was subsequently confirmed by independent experiments25,26,27. DFT calculations were performed by the Vienna Ab initio Simulation Package (VASP)28, with the projector-augmented-wave (PAW)29 implementation and the generalized gradient approximation (GGA) for exchange-correlation energy, in the form known as Perdew, Burke, and Ernzerhof30. Since the simulations were performed at high-temperature conditions, we used accurate pseudo-potentials where the semicore s and p states were treated as valence states.
All data generated or analyzed during this study are included in this published article.
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This research was supported by National Science Foundation under grant DMR-1835939, by Office of Naval Research under grants N00014-16-1-3124, N00014-17-1-2202, and N00014-20-1-2225, and by Brown University through the use of the facilities at its Center for Computation and Visualization. This work uses the Extreme Science and Engineering Discovery Environment (XSEDE), which is supported by National Science Foundation grant number ACI-1548562, via the resource Stampede2 at the Texas Advanced Computing Center (TACC) through allocation DMR050013N.
The authors declare no competing interests.
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Hong, QJ., Schroers, J., Hofmann, D. et al. Theoretical prediction of high melting temperature for a Mo–Ru–Ta–W HCP multiprincipal element alloy. npj Comput Mater 7, 1 (2021). https://doi.org/10.1038/s41524-020-00473-6
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