Abstract
Self-passivating, so-called smart alloys are under development for a future fusion power plant. These alloys containing tungsten, chromium and yttrium must possess an acceptable plasma performance during a regular plasma operation of a power plant and demonstrate the suppression of non-desirable oxidation of tungsten in case of an accident. The up-scaling of the bulk smart alloys to the reactor-relevant sizes has begun and the first samples with a diameter of 50 mm and thickness of 5 mm became available. The samples feature high relative density of above 99% and good homogeneity. With production of bulk samples, the research program on joining the smart alloy to the structural material was initiated. In a present study, the novel titanium–zirconium–beryllium braze was applied successfully to join the smart alloy to the Rusfer-reduced-activation steel. The braze has survived at least a hundred of cyclic thermal excursions in the range of 300–600 °C without mechanical destruction.
1 Introduction and motivation
The design of the future fusion power plant is presently under intensive study worldwide. A fusion power plant needs to comply with the highest operational and safety standards [1]. Specifically, safety requirements will have a strong effect on the design and on the choice of components and materials. Plasma-facing materials (PFMs) are crucially important for a robust plasma operation of the power plant. Due to advantages such as a high threshold energy for sputtering, low tritium retention, high thermal conductivity, high melting point and moderate activation, tungsten (W) is presently chosen as a prime candidate PFM for the European DEMOnstration fusion power plant, DEMO [2].
However, the predictive modeling [3] performed for various accidental scenarios on DEMO has revealed a decisive drawback of pure tungsten. In case of the so-called loss-of-coolant accident (LOCA) with an air ingress the temperature of the tungsten cladding reaches 1000 °C and remains at such a high level for several weeks. At such a high temperature, tungsten oxidizes and radioactive neutron-activated tungsten oxide sublimates into the atmosphere. Recent studies predict the sublimation rates from 10 up to 150 kg per hour from the first wall of a future fusion power plant [4].
Self-passivating tungsten alloys were introduced as a concept by Koch and Bolt [5]. During regular plasma operation, the surface of tungsten alloys is bombarded by plasma particles. Plasma bombardment leads to preferential sputtering of the light alloying elements leaving an almost pure tungsten surface facing the plasma. In a case of an accident, the remaining alloying elements in the bulk of the alloy will react with air and create their own dense oxides protecting tungsten from oxidation and from subsequent sublimation. Modern, self-passivating, the so-called smart alloys (SA) [6, 7], contain chromium (Cr) as oxidizing alloying element and yttrium (Y) as an active element stabilizing and regulating the chromium transport in the alloy system. The most efficient alloy composition was found to be 88 wt.% of W, 11.4 wt.% of Cr and 0.6 wt.% of Y [4].
Sound progress was made in development of smart alloys recently: bulk smart alloy samples became available via mechanical alloying (MA) followed by a fast compacting using field-assisted sintering technology (FAST), also known as spark plasma sintering (SPS) [8]. The availability of bulk SA samples allowed performing the extensive qualification of smart alloys. The essential elements of this qualification are an acceptable plasma performance of smart alloys and a suppression of oxidation of the new alloy systems. The bulk W–Cr–Y systems have demonstrated an impressive resistance to sputtering by deuterium plasmas on the timescale of three weeks of continuous DEMO operation [9]. At the same time, bulk smart alloy samples have attained an outstanding resistance to oxidation. The oxidation rate of smart alloys is at least a factor of 105 lower than that of pure tungsten. The resulting sublimation was also exceptionally reduced: at least a 40-fold decrease of sublimation was observed on W–Cr–Y smart alloy as compared with that of pure tungsten [10].
This qualification of smart alloys is a further step towards realization of the prototype first wall component of the fusion power plant. On the way to such a prototype among others, there are two major challenges, which have to be addressed:
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(a)
A feasibility of an up-scaling of bulk samples smart alloy systems to the reactor-relevant sizes of several square centimeters.
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(b)
A possibility of joining of plasma-facing and a structural material. Smart alloy is a PFM, whereas the reduced-activation steels, Eurofer, Rusfer or Clam, as a structural material for a fusion power plant are currently under development in the Europe, Russia and China, respectively.
The results of joint pilot studies undertaken at Forschungszentrum Jülich GmbH (FZJ, Jülich, Germany), National Nuclear Research University MEPhI (Moscow, Russia) and at Hefei University of Technology (HFUT, Hefei, China) on the way of upscale of smart alloys for DEMO are described and analyzed in the manuscript.
2 Up-scaling production of smart alloy
2.1 Experimental
Up-scaling of smart alloys is an important activity on the way to industrial production. Since the data on the particular geometry of the first wall of DEMO remains scarce, we are aiming at reaching the dimensions planned for International Thermonuclear Experimental Reactor (ITER). There, the first wall will be castellated. The characteristic linear dimension of the beryllium first wall monoblock varies from about 20 mm [11] to 50 mm [12]. The rationale and the size of castellation originates from the evaluation of thermal loads and their inhomogeneity. Given the prospected heat loads in DEMO, it is expected that the geometry considerations will likely remain. However, the dimension of the currently produced SA bulk samples is Ø20 mm diameter with the thickness of up to 5 mm, which cannot address fully the large-scale application in a future fusion power plant such as DEMO. Therefore, it is necessary to produce the large-size SA bulk samples.
Currently, the production of SA bulk samples for experiments is realized via MA followed by either hot isostatic pressing [13] or, since recently, by the field-assisted sintering technology (FAST) [10]. Based on the previous work [8] and on the current understanding, SA bulk samples with high density, fine grains and homogeneous structures have an excellent oxidation resistance. Aiming at this target, several challenges exist for up-scaling production of SA bulk samples using the current facilities. Hot isostatic pressing (HIP) was performed below solution temperature of SA, which could achieve a fine grain microstructure but is accompanied with a lot of Cr-rich phases [13]. For FAST, a pulsed direct current-activated and pressure-assisted sintering technique, the sintering process is determined by multi densification mechanisms of localized heating, Joule heating and surface cleaning [14, 15]. Furthermore, many parameters such as the heating rate, sintering temperature, pressure, holding time, vacuum influence the FAST densification process of SA. When changing the sample size, the current density, pressure, and atmosphere applied on the sample will change even without changing the principle FAST parameters. Therefore, the attainment of a high density, fine grains, homogeneous microstructure, and anti-oxidation properties of the large-scale bulk smart alloy similar to those of small SA sample cannot be made by the simple scaling of the FAST parameters to a new sample size. In this work, small-size (Ø13 mm and Ø20 mm) SA bulk samples with high density, submicron-grain, and homogeneous structures were produced. After analyzing their densification process, a large-size SA bulk sample with 50 mm diameter was Zohm H, Angioni C, Fable E, Federici G, Gantenbein produced.
The homogenous SA powder was prepared by MA technique as reported in Ref. [16]. Then, the alloyed powder was packaged into a graphite die and consolidated by FAST using a manual sintering mode. To prevent the carbon reaction with SA during the FAST densification process, a molybdenum foil was placed in the inner surface of the graphite die. Before sintering, the chamber of the FAST facility was pumped to the pressure below 10 Pa and kept under continuous pumping for the entire sintering cycle. To achieve a similar density and microstructure of the SA samples with different sizes, the FAST densification parameters must be different. The small-size SA samples (Ø13 mm and Ø20 mm) were performed in the Labox-350 FAST system manufactured by NJS Co., Ltd. The SA samples were heated at a rate of ~ 120 °C·min−1 up to 1150 °C. The temperature was controlled by adjusting the current at a loading rate of 75 A·min−1. To remove the residual gas, the temperature at 600 °C was kept for 2–3 min during the heating stage. Meanwhile, the pressure was increased from 10 to 90 MPa. Then, the SA samples are cooled down without any holding time at the maximum temperature, similarly as described in Ref. [16]. In case of the large-size (Ø50 mm) SA sample, the sintering was performed in the Labox-6020 FAST system manufactured by NJS Co., Ltd. It could provide a higher current, larger applied load, and higher pumping rate than those of the Labox-350 system. Nevertheless, the maximum pressure applied cannot exceed 50 MPa due to safety considerations. The pressure was increased from the initial 20–50 MPa at the temperature reaching 800 °C. Due to the lower pressure attainable of 50 MPa, the sintering peak-temperature was increased from 1150 to 1300 °C to achieve densification. The Labox-6020 FAST system can provide large enough current to support the heating rate of ~ 120 °C·min−1. During the heating process of the large-size SA sample pumping mitigated the build-up of the in-chamber pressure due to the gas release from the sample. The temperature change during the FAST densification process was monitored using an optical pyrometer operated in the range from 570 to 2000 °C. Notably, the temperature changes were reflected by the measurement of the outer surface temperature of these graphite dies. Therefore, graphite die with the different thickness would result in a different temperature difference between the displayed and actual temperature. The wall thickness of Ø13 mm, Ø20 mm and Ø50 mm graphite dies are 18 mm, 20 mm and 25 mm, respectively. In addition, the following parameters (displacement, current, temperature) evolution curves were also monitored during the FAST densification process. After that, the density of the SA bulk samples was measured following the Archimedes technique. The fracture morphology of SA bulk samples was characterized by scanning electron microscopy (SEM).
2.2 Results and discussion
After FAST densification, the microstructure information of SA samples with diameter of Ø13 mm and Ø20 mm was obtained from their fracture morphologies as shown in Fig. 1. The corresponding photographs are inserted in the SEM images. A very fine and high density microstructure can be observed in these two SA bulk samples. Based on the fracture morphology of Fig. 1, the grain sizes of Ø13 mm and Ø20 mm SA samples were measured by intercept method and were approximately 100 nm. The density of SA samples was measured by Archimedes’ principle. After calculation, the relative density of these two SA samples was approximately 98.5%. Notably, there are some dark gray discontinuous grains observed from these fracture morphologies, which are attributed to the Cr-rich phase. From the previous work [17], the SA powder was completely alloyed and with homogeneous microstructure after milling 60 h. Therefore, the Cr-rich phase could be possibly formed during the FAST densification process. The sintering peak-temperature of SA sample (1150 °C) is below its solution temperature (~ 1556 °C for W-11.4wt.%Cr) [18]. For a solid-solution alloy, precipitation must have occurred while sintering is below its solution temperature. Therefore, Cr-rich phases should be inevitable in case of the current FAST densification of SA samples.
Figure 1 shows that the bulk SA samples with a Ø13 mm and Ø20 mm, which were compacted using the same sintering parameters, have a similar microstructure and density. It means that Ø13 and Ø20 mm SA samples have experienced a similar densification process. Therefore, it is meaningful to study their densification processes for production of the larger-size SA bulk samples. Figure 2 shows evolution of the basic FAST parameters such as displacement, temperature and current density. From Fig. 2a and b, it can be seen that the SA samples with different diameters of Ø13 mm and Ø20 mm have similar change trend on displacement before cooling. The densification change curves reflect the expansion of graphite punch and the shrinkage and/or expansion of the SA powder bed during FAST process. In the vicinity of the cooling stage, there exists an inflection point in the displacement curves as marked with dotted line, which outlines the change in the densification process from shrinkage to expansion. It indicates that the SA bulk samples cannot be densified further. The slight increase in displacement curve is mainly due to the expansion of the graphite punch [17]. The corresponding temperature at the inflection point was called the densification temperature (marked with a red dot), which is the displayed temperature. From Fig. 2a and b, the displayed densification temperature of the Ø13 mm and Ø20 mm SA samples are ~ 1100 °C and ~ 1080 °C, respectively. As mentioned previously, these two SA samples have similar density and microstructure, so their actual densification temperature should also be similar. Therefore, the difference in their displayed densification temperature is owing to the different wall thickness of the graphite die. The thicker graphite wall implies the farther distance from temperature detection position to the actual temperature measurement position and hence, the larger uncertainty.
Figure 2c and d show the temperature and current evolution curves of the SA samples with different diameters of Ø13 mm and Ø20 mm as a function of the sintering time, respectively. The current loaded on SA samples increases stepwise with the temperature change. Notably, the current loading has a slight difference: ~ 105 °C·min−1 for Ø13 mm and ~ 130 °C·min−1 for Ø20 mm at the detected temperature range from 700 °C to the sintering peak-temperature. This is owing to a different current density loaded on the SA samples with different diameters under the same current loading manner. Further, the different heating rates for the SA samples were also the reason that results in the different sintering time. In addition, the maximum current density at 1150 °C for the SA sample with a diameter of Ø13 mm is higher than that for the SA sample with a diameter of Ø20 mm. The small graphite die (Ø13 mm) with a thin wall means a high heat dissipation compared with that of the large graphite die (Ø20 mm). Therefore, it requires a higher density current for supporting its heat dissipation during FAST process. In the FAST system, the current flows though the graphite punch and conductive SA material and generates heat (Joule heating effect), which heats the sample. Actually, the resistance of graphite is higher than that of the SA bulk samples [16]. Higher resistance means higher current-induced Joule heat. Therefore, the heat used for the consolidation of the SA samples was mainly derived from the thermal conduction of graphite punches. Simultaneously, there is also a heat dissipation by thermal irradiation during the FAST densification process. Different dimensions of graphite die/punch mean a different condition of heat dissipation. Naturally, it is also the reason for the different required time to heat the SA system up to the detected temperature of 570 °C. In addition, the Ø20 mm SA sample with more powder mass than that of Ø13 mm SA sample would contain a larger amount of residual adsorbed gas, and therefore the temperature at 600 °C was kept for a longer time (3 min) to remove the residual gas during the heating stage.
Based on the above cases, when increasing the SA sample diameter, the changes in the current density, heating rate, display densification temperature, and heat dissipation condition, should be considered to obtain SA bulk samples with a similar density and microstructure. Based on the current understanding of the above factors and on the pressure limitation of the Labox-6020 FAST system, densification of the SA sample with a diameter of Ø50 mm was achieved by changing the sintering peak-temperature and the pressure.
The loading current evolution as a function of the sintering time is shown in Fig. 3a. It demonstrates that the heating rate is approximately 120 °C·min−1 at the temperature ranges of 570 ~ 1300 °C. Compared with the current density required for the densification of small-size SA samples (Ø13 mm and Ø20 mm), the required current density of SA sample with a diameter of Ø50 mm obviously decreases. Figure 3b shows the corresponding displacement and pressure evolution curves as function of the sintering temperature. It is shown that in the displacement change curve, the SA powder bed has an obvious shrinkage when the pressure was evenly loaded from 20 to 50 MPa. After the pressure loading, the displacement continues to decline, which is derived from the densification of the SA sample. Notably, there exists a displacement plateau when the temperature ranges from ~ 1200 to ~ 1230 °C. The displacement plateau indicates that the Ø50 mm SA sample almost reached the highest possible density at the mentioned FAST conditions. Actually, the temperature of ~ 1230 °C is still below the expected densification temperature of the Ø50 mm SA sample. Considering these two factors, the temperature required for sintering densification and preventing grain growth, the Ø50 mm SA sample was continuously heated to 1300 °C but under a lower pressure of 20 MPa. According to Ref. [18], sintering at a high temperature but under a low pressure could avoid grain growth. The displacement increases rapidly as the temperature reaches the temperature of above 1230 °C. The pressure then was quickly decreased from 50 to 20 MPa. Furthermore, compared with the small-size SA samples (Ø13 mm and Ø20 mm), the Ø50 mm SA sample possess a high densification temperature (> 1230 °C). The main reason would be that the Ø50 mm SA sample was merely loaded with a low pressure of 50 MPa.
Figure 4 shows the fracture morphology of the large-size SA sample (Ø50 mm) and its photograph after FAST densification. No noticeable cavities and/or pores can be observed and the relative density reached up to approximately 98.5%. Compared with Fig. 1, there are no dark gray discontinuous grains, as shown in Fig. 4. This result indicates that a large-sized SA sample with high density and homogenous microstructure was obtained under the current FAST sintering parameters. Notably, the homogenous microstructure was attained for the large-size SA sample, but not for the small-size ones (Ø13 mm and Ø20 mm). This should be due to the fact that the actual sintering temperature reaches up to or even exceeds its solution temperature, so the actual sintering peak-temperature of the large sample is higher than that of small-size SA sample. The actual sintering peak-temperature must be higher than the measured sintering peak-temperature because there exists a distance between the sample position and the temperature detection position. Due to the higher temperature, Cr precipitation during the FAST densification of the Ø50 mm SA sample was avoided.
The grain size of the SA sample was measured to be approximately 300 nm, as shown in Fig. 4b. The grain size is larger than that of small-size SA samples sintered at 1150 °C (~ 100 nm). The grain growth is induced by the thermal activation energy at the high temperature [19], but the grain size is still within the acceptable submicron range.
The obtained positive results on up-scaling of the SA samples to the DEMO-relevant sizes allow the next step in realizing the mockup of the first wall—the joining of the smart alloy to the structural material. The results of the pilot joining tests are reported in the next section.
3 Pilot studies on joining of smart alloys with structural materials
3.1 Experimental
The common way to join complex elemental systems is brazing—the widespread technology used in nuclear [20, 21], aerospace [22] and automotive [23, 24] industry. This technology is also used in the manufacturing process of ITER components [25, 26]. Brazing has several beneficial aspects: it does not require high pressure and is cheaper than that in i.e. hot isostatic pressing (HIP). Moreover, as the number of armoring tiles in plasma-facing components is rather high, replacement of defective tiles after manufacturing are needed. Brazing is beneficial from this point of view [27] since it allows for a local replacement of a particular damaged component. For this purpose, filler alloys in a form of foils are convenient, but the composition of such alloys should consist of reduced-activation elements only because of the requirement for the DEMO materials. Presently, there is no filler alloy consisting of low-activation elements only. Nickel [28] or copper [29]-based alloys are frequently used. In this study, we have applied a brazing alloy with an appropriate composition even without Cu.
The rapidly-solidified into foil Titanium-Zirconium-Beryllium brazing alloy with the following composition was used: 48Ti–48Zr–4Be wt.%. The foil possesses always high quality, because after rapid solidification, due to high glass forming ability [30], the alloy is amorphous with a small amount of crystalline phase [31]. The chemical elements are considered as reduced-activation [32]. The thickness of the brazing alloy was 70 μm (Tsolidus ≈ 850 °C). SA samples with dimensions of 5 × 5 × 4 mm3 were supplied by Forschungszentrum Jülich GmbH. The bulk SA samples were produced via MA and compacted using FAST. The manufacturing details can be found in e.g. Ref. [8]. For structural material the reduced-activation ferritic-martensitic (RAFM) RUSFER steel [33] in the initial ferritic state was used (iron (Fe)–12 chromium (Cr)–2 tungsten (W)—vanadium (V)—tantalum (Ta)—boron (B), wt %). Samples had dimensions of 7 × 7 × 4 mm3. The scheme of a typical specimen for brazing is presented in Fig. 5. It is known that a direct joint between tungsten and steel is impossible due to the different coefficients of thermal expansion (CTE) which causes damage to the joint even after the manufacturing process [34, 35]. To decrease thermal stresses responsible for a damage, the usage of interlayers is preferable. Ta and V efficiently reduce stresses to be occurred in tungsten [35]. In this work, pure Ta with the thickness of 200 µm and dimensions of 7 × 7 × 0.2 mm3 was chosen because it doesnot form brittle eutectic with components of the filler alloy, apart from V forming the brittle eutectic with Zr [36, 37].
The brazing process should not worsen the properties of the materials to be joined. Since that two brazing modes were used, where Tb is brazing temperature, t is dwell time at Tb, Vh is heating rate, and Vc is cooling rate:
Mode 1: Tb = 950 °C, t = 30 min, Vh = 40 °C·min−1, Vc = 20 °C·min−1. This mode was chosen to be sure that properties of the SA will remain the same after brazing. It was previously shown that the oxidation resistance of the alloy degrade at a temperature higher than 1000 °C [4], where microstructural changes could have been the reason.
Mode 2: The first step is heating up to Tb = 1100 °C with dwell time t = 60 min, Vh = 40 °C·min−1, Vc = 20 °C·min−1. The second step is aging at T = 720 °C, t = 180 min, Vh = 20 °C·min−1, Vc = 10 °C·min−1. This mode was chosen to make a thermal treatment of the steel, and this mode is called “to traditional heat treatment” (THT) of RUSFER in the sense of Ref. [38].
The mode 2 was applied to study a possibility of simultaneous brazing and heat treatment of RAFM steel and SA. It should be noted that the application of any manufacturing process to make a joint should take into account the final microstructural state of the base materials, since it should not alter the principal properties of the materials to be joined. However, this fact is often not taken into consideration [39].
After a brazing cycle, microstructural investigations of the brazed joints were carried out using ZEISS EVO 50 XVP scanning electron microscope equipped with energy dispersive spectroscopy (EDS) INCA X-ACT and wavelength-dispersive spectroscopy (WDS) INCA Wave 500. WDS was used to measure yttria concentration. Neither EDS nor WDS could identify Be, because its concentration was very low. Other elements were measured by EDS, as well as concentration profiles.
A thermocycling test (TC) was applied to analyze the reliability of the joint. The thermocycling comprised heating to 600 °C and cooling to 300 °C according to the water-cooled lithium–lead (WCLL) blanket concept. The DEMO reactor operation implies pulse and dwell periods. It is known that the operation temperature of the RAFM steel is limited by 550 °C because of the drop in properties [40,41,42]. Hence the temperature during the pulse period will not exceed 550 °C on a steel surface [43]. However, the temperature expected in a brazed joint can be even higher. Therefore, 600 °C has been chosen as upper temperature of the TC. The lower temperature of 300 °C was chosen because during the dwell period, the temperature of a brazed joint should be close to the coolant and during the dwell period the coolant will continue to flow [44]. Every 20 cycles, an appearance of the specimen was examined by macro examination at sevenfold magnification with binocular microscope. Only the specimen obtained using the brazing mode 1 was used in the experiment because the structure of the SA was preserved in its initial state. The details will be reported later in this paper. The specimen was placed into quartz ampoule connected to a vacuum pump obtaining p = 1 Pa. The specimen in the ampoule was heated up to 600 °C without dwelling, and then the ampoule was taken out of the furnace and the specimens were cooled down to 300 °C. The temperature of the specimen was controlled by Cr-Al thermocouple, which was inserted into the ampoule. This thermocycle corresponds to Vh = 4 °C·s−1 and Vc = 2 °C·s−1. In total, a hundred thermocycles were applied.
3.2 Results
3.2.1 Microstructure studies
The microstructure of the SA far from a seam was investigated before and after brazing. The initial state of SA is presented in Fig. 6a, after brazing mode 1 in Fig. 6b, and after brazing mode 2 in Fig. 6c. The initial microstructure consists of tungsten (W)—based solid solution with chromium (αW, Cr), chromium (Cr)—based solid solution with W (αCr,W), yttria—(Y–O). The microstructure is similar to those observed in Ref. [45]. No evident microstructure changes occurred after mode 1. After mode 2 decay in Cr-based phase occurred into (αW,Cr) and (αCr, W), according to a phase diagram [46]. It is known that fine distribution of Y–O precipitates along nanograin’s boundaries occur in the SA [8], and we also identifies larger ones in Fig. 6. We see that after mode 2 (Fig. 6c) the density of the large Y–O precipitates increased, which can be related to coarsening of the smaller precipitates.
Figure 7 shows the microstructure of the joints at interface to SA. A thick diffusion layer was formed; however, the thickness after different brazing modes is different. The seams are divided into two areas: A—interface, B—diffusion layer.
SEM images of the Ta/SA seams: Sample produced using the mode 1: a full view with concentration profiles and marked areas: A—interface; B1, B2—diffusion layer; c magnified view of the area A with marked layers, magnified images of the green and blue areas is shown in Fig. 8; Sample produced using the mode 2: b full view with concentration profiles and marked areas: A—interface; B1, B2—diffusion layer; d magnified view of the area A with marked layers
According to the concentration profiles (plotted on the micrograph, Fig. 7a) measured by EDS at 20 keV for the sample produced using the mode 1, the concentration of chromium does not decrease significantly towards the interface. Ti and Zr follow the common law of diffusion—descending concentration from the seam to the bulk of the SA. The peaks of Zr and Ti within layers III and IV show that not all the brazing alloys melt when they interact with these base materials. Ta does not diffuse into SA. No diffusion of any component into pure Ta occurred.
Concentration profiles for the sample produced using the mode 2 (plotted on the micrograph, Fig. 7b) are quite different. The amount of W and Ta decreases gradually from one base material to another. Whereas Ta diffuses noticeably into W, W does not do the same. Zr and Ti profiles are different from those in the sample produced using the mode 1: the concentration of Ti has a drop within layers II and III, but descends gradually beyond these layers; Zr profile has a significant drop within layers III and IV (Fig. 7b, d). This can be related to different coefficients of diffusion of Zr in W and Cr; however, there is no valid data on diffusion coefficients that are available. This is also a result of the full interaction between the brazing alloy melt and the base materials.
The detailed investigation of the area A is shown in Fig. 7c for the mode 1 and Fig. 7d for the mode 2. The microstructures are considerably different. Five layers were formed in sample produced using the mode 1 (Fig. 7c): (I) Needle-like 74Ta–16Ti–6Cr–3Zr–1W at.% phase (Magnified image of the layer is shown in Fig. 8a); (II) Mechanical mixture of 70Ta-20Ti-5W–3Zr–2Cr at.% and Ti-based phase; (III) 49Ta–26Ti–17W–7Zr–2Cr at.% phase formed within Ti-based phase; (IV) 67Ti–19Zr–6Ta–5,5Cr–2,5Ta at.% phase; (V) Two Ti–W phases formed within Ti-based phase and SA, magnified image of the layer is shown in Fig. 8b.
Magnified SEM images of the layers outlined in Fig. 7c of the sample produced using the mode 1: a green rectangle outline—layer I; b blue rectangle outline—layer V
Though beryllium could not have been identified in the course of this study, we can assume that no beryllide formed as no black-contrast phases are observed. Layers I–III (Fig. 7c) represent Ta-based crystals formed within Ti-based solution, where Ti-based solution by its contrast should be like layer IV. Concentration of Ta decreases from I to III, while Ti increases.
In weight, the percentage composition of the layer IV is 48Ti–26Zr–15Ta–7W–4Cr wt.%. Compared to the initial composition of the brazing alloy (47Ti–47Zr–4Be wt.%) Zr more effectively dissolved than Ti due to deeper diffusion into SA (Fig. 7a). Also, bright-light phases within grains and on their boundaries were formed. Most of these phases fell out during grinding.
In the layer V shown in Fig. 8b, the two phase morphologies were found, which are marked as rectangular (43.3Ti–34.8W–11.5Cr–8Ta–2.4Zr–0.1Y at. %) and hexagonal (41.9Ti–36.4W–9Ta–7.6Cr–5Zr–0.3Y at.%) outlined. The former preferably grows within SA, and the latter within Ti-based phase.
Four layers were formed in the sample produced using mode 2 in the area A (Fig. 2d): (I) needle-like 52Ta–33Ti–6Cr–5Zr–4W at.% phase; (II) chromium-based 48Cr–22Ta–14Ti–8Zr–7W at.% phase; (III) corn-like 48Ta-42W–8Ti–1Cr–1Zr at.% phase; (IV) smooth layer of the following composition 37.3W–28.1Ti–24.9Ta–7.5Cr–1.2Y–1Zr at.%.
The layers are clearly divided from each other, because all of them are one-phase structured. No layers with a composition close to the initial composition of the brazing alloy formed. Layer II is enriched with Cr, while layers III and IV are chromium depleted. Between layer III and IV crumbling is observed, probably due to the formation of the beryllium phase.
Magnified microstructure of the diffusion layers, area B pointed out in Fig. 7a, b, is presented in Fig. 9. The area is divided into two zones: B1 (Fig. 9a) and B2 (Fig. 9b), where B1 is closer to SA, and B2 is closer to Ta. Area B is divided into two zones because of the different morphologies, which is described further. The thickness of the diffusion layer in the sample produced using mode 1 is 80 µm, where B1 has a thickness of 20 µm and B2 has a thickness of 60 µm. The thickness of the diffusion layer after mode 2 is 160 µm, where B1 and B2 have a thickness 80 µm. Decay into layers of W-based and Cr-based phases is observed both in B1 and B2. Though the thickness of the layers is different for the samples produced by two modes, their compositions are similar. In B1 zone, the composition of bright W-based phase is equal to the initial composition of SA—68.9W–30Cr–1.1Y at.% (or 88.4W–10.9Cr–0.7Y wt.%), whereas in B2, a W-based phase is significantly alloyed with Ti and Ta: 50W–28.9Ti–12Ta–8Cr–0.9Y at.%. Dark Cr-rich phase is mainly alloyed with Zr and W both in B1 and B2 zones as it can be seen in Fig. 9. B1 also contains additional Cr-based phase with clear outlines. In the sample produced using mode 1, additional Cr-based phase has just started to grow and has a composition close to that of Cr-rich phase. In the sample produced using mode 2, the phase takes a distinct form and has higher W concentration, because dissolution of the inner W-based phase occurred. These phases were not observed in the area B2. That is why the diffusion layer was divided into two zones.
Figure 10 shows microstructure with EDS maps of the joints at RUSFER/Ta interface: a—mode 1; b—mode 2. No pores or cracks were observed. Probably not the whole amount of the molten brazing alloy dissolved with the base material, which resulted in a solidification of residual brazing alloy. The area of the residual brazing alloy is marked with an arrow in Fig. 10. A lower amount of residual brazing alloy was left in the mode 2 sample due to higher brazing temperature, and everything else is similar. Bright needles correspond to Ta-rich phase. Since the mode 2 is equivalent to the traditional heat treatment of RUSFER, it is important to investigate the microstructure of a steel. Figure 11 shows the microstructure of the RUSFER near the brazed seam. Martensitic phase has been formed in the bulk alloy; a thin ferritic layer was formed near the brazed seam. As this work is aimed at detailed investigations of the SA, Ta/steel joint investigation will be presented elsewhere.
According to the microstructural investigations, only the sample produced using mode 1 was selected to conduct TC, because the initial microstructure of the SA was preserved and no crumbling occurred.
3.2.2 Thermal cycling
The microstructure of the specimen after TC is presented in Fig. 12. No detachment at both interfaces was observed using macro examination and SEM. The thickness of the diffusion layer at the Ta/SA interface (area B in Fig. 12a) grew from 80 µm before thermocycling to 150 µm, where B1 had a thickness of 50 µm and B2 of 100 µm. Magnified microstructure of the area A of the Ta/SA seam is presented in Fig. 12b. The thickness of the layer I increased: a new needle-like phases grew within Ta. Evidently, iron (Fe) diffusion occurred during thermocycling, as the presence of Fe in the amount of 1 at.% in the layers IV and V was observed. Diffusion could have gone through Ta interlayer or more likely through the fillet regions, as the brazing alloy wetted the whole Ta interlayer, which is shown in Fig. 12c. Ta–W-based crystals formed within hexagonal Ti–W phase layer V. These crystals have crisp boundaries. As it can be seen from the SEM image crumbling close to these crystals occurred (Fig. 12b).
3.3 Discussions
Brazing of SA with RUSFER was successfully carried out with the use of Ta interlayer and 47Ti–47Zr–4Be wt.% brazing alloy. Heating of the SA up to 950 °C does not change the microstructure; however, brazing at higher temperatures up to 1100 °C leads to decay of the W–Cr solution.
As shown in Sect. 3.2, a thick diffusion layer was formed between Ta and SA. This fact claims good inter-diffusion of the brazing alloy and the SA. Due to the full dissolution of the brazing alloy when using mode 2 a thicker diffusion layer was formed. This layer represents decay of W–Cr alloy into layer-by-layer W-based and Cr-based solid solutions. Closer to the bulk SA composition of the W-based solid solution is similar to the initial SA alloy composition. Closer to the seam brazing alloy elements dissolved in the solid solutions: Zr mainly dissolved in Cr, and Ti in W. In the mode 2 sample an additional rectangle Cr-based phase formed, whereas in the mode 1 sample this phase has just started to form (Fig. 9). Similar layer-by-layer structure was also observed in Ref. [47].
Significantly different microstructures of the Ta/SA seam using two brazing modes were detected (Fig. 7); however, the only difference in the RUSFER/Ta seam is the thickness of residual amount of the brazing alloy (Fig. 10).
Some common features were observed for samples made using the mode 1 and 2 especially at the interface from Ta to the smart alloy (Fig. 7). The morphology of the layers marked as I is similar in both specimens. The microstructure of the layer correlates with results was presented in Ref. [48]. It was shown that the morphology of Ti-Ta alloy critically depends on Ta concentration: a lamellar or needle-like martensitic structure can form depending on the amount of Ta. Thus, the thickness of the layer I grows during thermocycling due to the ongoing diffusion of Ti into Ta.
A mechanical mixture in the layer II of the sample produced using mode 1 is similar to those formed when using Ti–22.5Cr–7.5V–3Be filler metal [49]. More likely that the bright-contrast phases in the layers III and IV were formed due to decreasing of Ta solubility in Ti solid-solution [50]. The formation of the layer IV is related to crystallization of the residual brazing alloy melt, because the composition is similar to the initial one, especially for Ti. Hence 30 min are not enough to complete dissolution of the braze, and therefore we can expect achieving better results using longer brazing time.
Evidently, the phase II in the mode 2 sample (Fig. 7d) is the Laves TaCr2 phase [51, 52]. Likely, the formation of this phase occurred due to release of Cr from the SA. Layer III is a result of crystallization after dissolution in a brazing alloy melt. Probably, the initial boundary of the SA was between the layers III and IV, because Y was not found in the layers I-III.
The microstructure of RUSFER in the mode 2 specimen was investigated, which corresponds to those that should be formed after traditional heat treatment [53]. It is important to mention that compared with the joints obtained with V interlayer, no significant formation of Ferritic grains close to the seam were observed, because neither vanadium nor titanium carbides were formed. Ferritic grains are 10 times smaller than those observed in Ref. [54] under similar conditions and in Ref. [55] after brazing at 960 °C. Also, the grain size is 20 times smaller than in Ref. [56] after HIP at 1050 °C.
The investigation of the brazed joints of the SA and RUSFER steel allows us to make a conclusion on relevance of the brazing technology for a mock-up production. However, simultaneous brazing and heat treatment with the RAFM steel with temperature higher than 1000 °C is impossible due to the decay of the W–Cr solid solution. Brazing at temperatures lower than 1000 °C, even at 950 °C, preserves the microstructure of the SA. A brazed joint with Ta interlayer can withstand at least 100 cycles of 300–600 °C heating and cooling down and expectedly even more, because no macro degradation was observed.
4 Conclusion
In the course of the paper, we have reviewed the first steps made towards realizing a first wall component for a future fusion power plant. This activity was pursued via the study of joining the smart W-Cr-Y tungsten alloy foreseen for a first wall of a fusion power plant and the reduced-activation RUSFER steel. Fully reduced activated 48Ti–48Zr–4Be wt.% brazing alloy was first time used to join tungsten alloy with steel. Brazing of the SA should be carried out at a temperature not higher than 950 °C to prevent the decay of the W–Cr solid solution. RUSFER/Ta/SA brazed joint obtained by 48Ti–48Zr–4Be wt.% at 950 °C/30 min brazing mode was capable to maintain the stable joint which retained its full mechanical integrity after the thermocycling for at least 100 cycles in the temperature range 300–600 °C. This means that further investigations, such as mechanical tests and high heat flux tests, can be carried out.
At the same time, next steps for an industrial up-scaling were undertaken successfully. The bulk smart alloy sample with the size of 50 mm was realized successfully via field-assisted sintering technology. The Ø13 and Ø20 mm SA samples feature a similar density and microstructure due to the similar sintering parameters of sintering temperature and current loading manner. Changing sample size and applied pressure during the up-scaling production SA sample, the factors of current density, heating rate, densification temperature and heat dissipation condition should be considered to achieve a desired density and a microstructure. In addition, the described study of FAST parameters has allowed an effective suppression of the chromium-rich phase formation in the course of sintering.
5 Outlook
Progress attained both in the area of brazing and industrial up-scaling allows us to pursue the activities in realization of the first wall prototype of the future fusion power plant. Both aforementioned activities are now about to be merged on the way of creation of the full-scale prototype of a first wall segment. The efforts will be focused in realizing the large full-scale joint of the smart alloy on the reduced-activation steel. This will be attempted along with brazing technology described here and by means of other innovative techniques. Among them, there is a direct sintering of smart alloy and steel via FAST and HIP. A pioneering research on direct sintering the materials and the joint in one-step using FAST and HIP is underway. The comparative study of all feasible joint techniques is foreseen.
Change history
21 August 2021
A Correction to this paper has been published: https://doi.org/10.1007/s42864-021-00115-4
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Acknowledgements
A part of these studies has been carried out within the framework of the EUROfusion Consortium and has received funding from the Euratom research and training programme 2014–2018 and 2019–2020 under grant agreement No. 633053. The views and opinions expressed herein do not necessarily reflect those of the European Commission. The research benefitted from a grant of the European Commission through the Erasmus Mundus International Doctoral College in Fusion Science and Engineering (FUSION-DC). Up-scaling production part is supported by the National Natural Science Foundation of China (Grant Nos. 52020105014 and 52001104), the Fundamental Research Funds for the Central Universities (Grant Nos. JZ2019HGTA0040, JZ2019HGBZ0113, and PA2019GDZC0096), the Natural Science Foundation of Anhui Province (Grant Nos. 201904b11020034 and 1908085ME115) and the International Postdoctoral Exchange Fellowship Program of Helmholtz-OCPC (Grant No. ZD20191015). Brazing part was funded by The Council for Grants of the President of the Russian Federation
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Bachurina, D., Tan, XY., Klein, F. et al. Self-passivating smart tungsten alloys for DEMO: a progress in joining and upscale for a first wall mockup. Tungsten 3, 101–115 (2021). https://doi.org/10.1007/s42864-021-00079-5
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DOI: https://doi.org/10.1007/s42864-021-00079-5
Keywords
- Fusion power plant
- Self-passivating smart tungsten alloys
- Joining
- Up-scaling production
- Field-assisted sintering technology