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metals Article Crystallization Process and Microstructural Evolution of Melt Spun Al-RE-Ni-(Cu) Ribbons Francisco G. Cuevas 1,* , Sergio Lozano-Perez 2, Rosa María Aranda 1and Raquel Astacio 3 1Department of Chemical Engineering, Physical Chemistry and Materials Science, Higher Technical School of Engineering, University of Huelva, Campus El Carmen, Avda. Tres de marzo s/n, 21071 Huelva, Spain; r[email protected] 2Department of Materials, University de Oxford, 16 Parks Road, Oxford OX1 3PH, UK; sergio.lozano-per[email protected] 3Department of Materials Science and Engineering, Higher Technical School of Engineering, University of Sevilla, Avda. de los Descubrimientos s/n, 41092 Sevilla, Spain; [email protected] *Correspondence: [email protected]; Tel.: +34-959217448 Received: 7 March 2020; Accepted: 26 March 2020; Published: 27 March 2020 Abstract: The crystallization process, both at the initial and subsequent stages, of amorphous Al 88 -RE 4 -Ni 8 alloys (RE =Y, Sm and Ce) has been studied. Additionally, the consequences of adding 1 at.% Cu replacing Ni or Al were studied. The stability of the amorphous structure in melt spun ribbons was thermally studied by differential scanning calorimetry, with Ce alloys being the most stable. The effect of Cu to reduce the nanocrystal size during primary crystallization was analyzed by transmission electron microscopy. This latter technique and x-ray diffraction showed the formation of intermetallic phases at higher temperatures. A clear difference was observed for the Ce alloy, with a simpler sequence involving the presence of Al 3 Ni and Al 11 Ce 3 . However, for the Y and Sm alloys, a more complex evolution involving metastable ternary phases before Al 19 RE 5 Ni 3 appears, takes place. The shape of the intermetallics changes from equiaxial in the Ce alloys to elongate for Y and Sm, with longer particles for Sm and, in general, when Cu is added to the alloy. Keywords: amorphous materials; melt spinning; Al-RE-Ni alloys; crystallization 1. Introduction The disordered or amorphous structure typical of the liquid state can be maintained in solid metals by heating above their melting temperature and very quick cooling to room temperature [ 1 , 2 ]. Only particular compositions are appropriate to form metallic glasses, and depending on the composition, the necessary cooling rate varies. The importance of this process resides in the outstanding attained properties of different character such as mechanical, electrical, magnetic, or chemical, all of them of great engineering importance [3,4]. Regarding compositions, aluminum mixtures with at least other two chemical elements (although it is also possible with only one, i.e., [ 5 , 6 ]) can reach the amorphous state by quick cooling, attaining high strengths with respect to conventional aluminum alloys [ 7 ]. Properties such as elastic strain [ 8 ], or the possibility of superplastic forming in a supercooled liquid region [9] are remarkable. Initially, Al amorphous alloys with a composition Al-Fe-Si [ 10 , 11 ] showed brittleness problems that were subsequently solved by changing for instance to Al-Ni-Zr compositions [ 12 ]. Later, the development of compositions Al-RE (rare earth: La, Y, Ce)-TM (transition metal: Fe, Co, Ni) [ 6 , 13 – 16 ] allowed very high strengths (up to 1100 MPa) to be reached. This strength can be increased for some alloys by allowing the formation of up to a 50 vol.% of α -Al nanocrystals [ 17 , 18 ] at the expense of the amorphous phase. For nanocrystallized Al-RE-Ni alloys, ultimate tensile strengths Metals 2020,10, 443; doi:10.3390/met10040443 www.mdpi.com/journal/metals
Metals 2020,10, 443 2 of 18 can increase up to 1560 MPa [ 19 , 20 ], three times the value of crystalline alloys, even showing improved ductility and toughness [ 21 ]. The nanocrystal size, number, and spatial distribution are key parameters in the obtained properties. These parameters are better controlled by annealing from an amorphous structure obtained after quenching [17]. Intermetallics appearing after heating are unfavorable for the properties of the alloys [ 22 ]. Understanding this process, which should be initially avoided to preserve the best properties, is of great importance. One of the important aims of working with amorphous alloys is to obtain thick parts [ 2 ], and the formation of intermetallics is a concern in this process. Many bulk metallic glasses (BMG) have been prepared, with lots of them still to be discovered [ 23 ]. The formation of BMG can be theoretically predicted according to the physical properties of the amorphous and crystalline phases, or on known rules such as the confusion principle. However, for Al-based alloys, the glass forming ability (GFA) does not adequately follow the expected criteria, and the production of Al-based BMG is relatively difficult and limited to low Al contents [ 24 ]. Under these circumstances, Al-based alloys are bad candidates for BMG processing; and the amorphous ribbons require further processing by powder metallurgy methods. For instance, spark plasma sintering, one of the multiple electric field assisted sintering techniques, has been used to consolidate Al-Y-Ni amorphous powders [25,26]. Al-RE-Ni alloys were studied in this work. The study of the crystallization kinetics and competition of the crystalline phases [ 27 – 30 ], the expected GFA [ 31 – 33 ], and the theoretical modeling of the adequate solute range for amorphous forming [ 34 – 36 ] shows that ternary alloys with a solute content around 10–15 at.% are good candidates to attain amorphous structures. Thus, the compositions Al 88 -RE 4 -Ni 8 were selected (with RE =Y, Sm, and Ce, three well-known candidates to reach the amorphous state). The influence of small amounts of alloying elements in the primary crystallization of Al-RE-Ni systems has been previously studied [ 37 – 44 ]. In this work, it will be extended to include the subsequent appearance of intermetallic phases, which are of great importance during the consolidation process of amorphous ribbons. 2. Materials and Methods The alloys Al 88 -RE 4 -Ni 8 (RE =Y, Sm, and Ce) were selected in this work. Moreover, Al or Ni was replaced by just 1 at.% Cu, resulting in the alloys Al 87 -RE 4 -Ni 8 -Cu 1 or Al 88 -RE 4 -Ni 7 -Cu 1 . Pure metals (Al 99.9%, Ni 99.95%, Y 95%, Sm 99.9%, Ce 99.9%, and Cu 99.9%) were arc melted in vacuum to prepare the master alloys Al 90 -Cu 10 and Al 25 -RE 75 . Pure metals and master alloys in the adequate proportion were repeatedly remelted to obtain the final alloys with an adequate homogeneity. The final materials were obtained in the form of ribbons after heating the alloy at 1000 ◦ C in a melt spinning chamber filled at a 200 mbar He atmosphere. The liquid was ejected through a round nozzle 0.85 mm in diameter on a Cu wheel rotating to reach 40 m/s on its surface. A distance nozzle-wheel of 1.5 mm resulted in ribbons with a thickness of 25–30 µm and width of 1–2 mm. The amorphous character of the melt-spun ribbons was examined by x-ray diffraction (XRD, model PW 1729, Philips, Amsterdam, Netherlands, with Cu-K α radiation for 2 θ =20–80 ◦ ). Transmission electron microscopy (TEM, model CM20, Philips, Amsterdam, Netherlands, working at 200 KV) was used to characterize heat treated ribbons, after electropolishing at − 30 ◦ C in 10% perchloric acid, 90% ethanol solution. In general, the Al nanocrystals were especially attacked with this technique, being necessary to ion mill the heat treated ribbons after cooling at −30 ◦C. The thermal stability of the ribbons was studied by differential scanning calorimetry (DSC, model 2010, TA Instruments, New Castle, DE, USA) heating at 20 ◦ C/min, on times combined with final isothermal treatments, under an Ar atmosphere. Cooling was always carried out by switching offthe equipment, without particular control of the cooling rate.
Metals 2020,10, 443 3 of 18 3. Results and Discussion 3.1. Melt-Spun Ribbons XRD patterns of as-spun materials are shown in Figure 1. A broad peak at 2 θ ~38 ◦ can be observed, being representative of having reached an amorphous structure in Al alloys. Regarding the Y alloy, a small shoulder appeared for 2θ~44◦, because of the presence of some local order [41,45,46], corresponding to the initial stages of disappearance of the amorphous structure, while still being maintained. According to the confusion principle [ 47 ], the low atomic radius difference between Al and Y when compared to Al-Sm or Al-Ce [ 48 ] reduces the GFA. Al-RE-Ni alloys showed a strong linear dependence for the GFA on the size of RE elements, with bigger atoms facilitating the glass formation [ 49 ]. Nevertheless, the obtained structures can be considered amorphous from the XRD analysis. Figure 1. X-ray diffraction (XRD) patterns of Al-RE-Ni-(Cu) melt-spun ribbons. XRD also showed that, in general terms, patterns corresponding to Al 87 -RE 4 -Ni 8 -Cu 1 seemed to be flatter, and those of Al 88 -RE 4 -Ni 7 -Cu 1 tended to contain sharper peaks. On the other hand, the diffuse peak position shifted to lower angles for the Ce alloys. According to the Ehrenfest relation [ 50 ], this position was lower for a higher value of near-neighbor distance, occurring on the Ce-containing alloy, with a higher atomic radius than Y and Sm. 3.2. Crystallization Process DSC results for the as-spun ribbons are shown in Figure 2. The general behavior is a crystallization process occurring in three stages, although a small fourth stage can also appear at temperatures higher than 400 ◦ C, as shown for the Cu-free Sm-containing alloy. Crystallization can therefore be quite dependent on composition. Even the composition [ 51 ] and DSC heating rate [ 5 , 42 , 45 , 52 – 54 ] can determine the transformation temperatures, and limit the capacity to detect them when taking place very close. Thus, Y-containing alloys with a similar range of compositions as those studied in this work are usually found to crystallize from the amorphous structure in three stages [ 34 , 41 , 45 , 55 – 59 ], but four stages have also been reported [ 27 , 48 , 58 , 60 ]. Likewise, synchrotron XRD revealed the presence of two stages in Al 87 -Y 4 -Ni 9 and Al 86 -Y 4 -Ni 10 , but three stages for Al 83 -Y 4 -Ni 13 [ 29 ]. For Sm-containing
Metals 2020,10, 443 4 of 18 alloys, the first three DSC reactions have been reported [ 51 , 54 , 61 – 64 ], but a fourth reaction has also been found for similar alloys [ 53 , 61 , 65 – 68 ], and up to five reactions have been identified [ 69 ]. Regarding Ce-containing alloys, the general behavior depends on the composition, but three reactions have generally been reported for similar compositions to the one now studied [49]. Figure 2. Differential scanning calorimetry (DSC) traces at a heating rate of 20 ◦ C/min of Al-RE-Ni-(Cu) melt-spun ribbons. Comparing the three RE elements, the first reaction was quite similar for the three RE-containing alloys, only at some higher temperatures for Ce, and some starting earlier for the Y-containing alloys. Regarding the second and third reactions, the Y and Sm-containing alloys showed a very similar behavior, although the third reaction seemed to be of greater importance in Y alloys. Ce-containing alloys, however, showed a second reaction much smaller with regard to the third one, and even nearer to each other when compared with the two other cases. These different crystallization stages will be analyzed next. 3.3. Primary Crystallization The crystallization process starts for all of the alloys with a broad exothermic reaction. The onset temperatures were 150 ◦ C, 165 ◦ C, and 180 ◦ C for the Cu-free Y, Sm, and Ce-containing alloys, respectively. According to Figure 1, the Y alloys seemed to reach a less amorphous state, and Ce patterns appeared flatter and therefore more amorphous, which is now reflected in the ease in which to start crystallization. DSC showed that increasing the total amount of solute when 1 at.% Cu replaces Al resulted in slightly more stable alloys. In contrast, when Ni was replaced, therefore maintaining the total amount of solute, and with the atomic radius of Cu being more similar to the Al than to the Ni one, a reduction of the amorphous structure stability was found. XRD and TEM results from ribbons heated to the end of the first reaction at 250 ◦ C showed the formation of α -Al nanocrystals. Figure 3shows the results for the Sm-containing alloys, with similar results for the Y and Ce alloys.
Metals 2020,10, 443 5 of 18 Figure 3. Study of the first DSC reaction of Sm alloys after heating at 20 ◦ C/min to 250 ◦ C and immediate cooling: ( a ) XRD patterns of ribbons, with peaks corresponding to α -Al nanocrystals, and (b) transmission electron microscopy (TEM) dark field images and diffraction patterns (DP). Nanocrystal size measurements of the ribbons heated beyond the first DSC reaction (i.e., at 250 ◦ C) were carried out on TEM micrographs. The similar area under DSC curves ensured a similar amount of nanocrystals formed. Results obtained by line intercept showed that the presence of Cu acts to diminish the nanocrystal size. The crystals’ size mean value was thus reduced to about 9 nm when Cu was present in Sm-containing alloys, with 10.7 nm for the Cu-free alloy, and in a similar way for the Y and Ce alloys. One of the possible reasons for this is the reduction of the nucleation barrier, as reported for Al-Y-Ni-Cu [ 38 ] and Al-Ce-Ni-Cu alloys [ 70 ]. Nevertheless, for these alloys, Cu has also been found to be uniformly distributed [ 61 , 71 ], besides causing composition variations [ 70 , 72 ]. In Al-Sm-Ni alloys, heterogeneities that can act as nucleation sites have been reported after the addition of Cu [ 73 , 74 ]. In summary, there is not a clear consensus for the actual reasons for this reduction. 3.4. High Temperature Crystallization Stages The second DSC crystallization reaction for the Y and Sm-containing alloys appeared with an onset at approximately 315 ◦ C and at 335 ◦ C for the Ce alloy (see Figure 2). This reaction ends only about 35 ◦ C later for the Y and Sm alloys, and 20 ◦ C for the Ce-containing alloy, and before it has totally finished, the third reaction starts (this being more pronounced for the Ce alloy). A higher separation between the second and third reactions, allowing a better study of the processes taking place, can be attained by heating the ribbons up to 5 ◦ C before the onset of the second DSC reaction, then maintaining the temperature in an isothermal heat treatment. Figure 4shows the DSC traces thus obtained.
Metals 2020,10, 443 6 of 18 Figure 4. DSC traces (heating rate of 20 ◦ C/min up to 5 ◦ C before the onset of the second reaction and then maintaining the temperature) of the Al-RE-Ni-(Cu) alloys (vertical lines mark the heating regime change.). DSC traces at 20 ◦ C/min in Figure 2showed an asymmetry at the beginning of the second reaction for the Y and Sm alloys, not being so clear for the Ce-containing alloy. This peculiarity of the second reaction is separated in different reactions (we will call them subreactions 1 and 2) when holding the temperature in Figure 4, always more clearly for the Cu-free alloys. This different behavior for the Ce-containing alloys could be caused by a different crystallization process, which is discussed next. The third reaction remains during isothermal heating as only one, starting up to 10 min after the end of the second one. The start of this third reaction is quicker for a lower separation with respect to the second one in continuous heating, something taking place very clearly for the Ce alloys, and in general for the Cu-free alloys. The second reaction is usually a source of discrepancies in previous studies, mainly for the Y and Sm alloys. The reason is that even after heating the ribbons to make this reaction take place, identifying the phases present in the alloys is challenging. XRD patterns of ribbons isothermally treated to the end of the two subreactions of the second crystallization stage (Figure 5shows the results for the Y alloys, being similar for Sm and Ce alloys) seem to show that in both cases, only α -Al
Metals 2020,10, 443 7 of 18 nanocrystals were found. Likewise, TEM diffraction showed no spots from new phases once the second DSC reaction finished. Figure 5. XRD patterns of heat treated ribbons up to the end of the two subreactions of the second DSC reaction, and the TEM DP of the Y-containing alloys at the end of the second DSC reaction. Undoubtedly, something is happening in the second crystallization stage. The only difference with previous XRD patterns (i.e., after the primary crystallization) was an asymmetry at the left of the main Al peak, which could be related to the formation of new phases probably just nucleating, but their identification is not possible. A rough estimation can be done after (i) taking into account that the intermetallic formation requires an activation energy 25% higher than α -Al nanocrystals [ 48 ], (ii) that the amount of intermetallics and primary nanocrystals are similar, and (iii) considering the areas of the reactions under the DSC curves. Thinking of an α -Al nuclei about 10 nm in diameter, the equivalent nucleation and growth for the intermetallics would lead during the first and second subreactions of this second stage to particles of about 6 nm and 5 nm respectively, in the case of an homogeneous process. However, this same volume of new particles led to layers of 0.4 nm and 0.25 nm forming around the existing α -Al nanocrystals (values in the same order of magnitude result by computing the areas in the DSC curves of the Sm alloys). These very thin and not easily detectable layers could be the explanation for the almost similar results, therefore a heterogeneous nucleation surrounding previous α-Al nanocrystals can be proposed. As mentioned before, no clear results have been reported regarding the second and subsequent crystallization stages of these alloys. For Y alloys, Al 3 Ni, Al 16 YNi 3 , and unidentified phases have been indicated to appear [ 43 , 45 , 55 – 57 , 75 , 76 ]. The Al 16 YNi 3 phase is, in more recent years, not referred, and Al 19 Y 3 Ni 5 and Al 23 Y 4 Ni 6 have been proposed [ 27 , 29 , 77 – 79 ], the former on times considered a metastable phase, and both of them with a very similar structure to the well-known Al 4 YNi phase [ 80 , 81 ]. This metastable character is not discarded according to the Al-Y-Ni intermetallic enthalpies of formation [ 31 , 78 , 82 ], lower for Al 19 Y 3 Ni 5 than for Al 23 Y 4 Ni 6 . However, Al 19 Y 3 Ni 5 [ 29 ] and also the Al9YNi3[27,29] have been proposed as stable phases of this system.
Metals 2020,10, 443 8 of 18 Regarding Sm alloys, the second stage is related to the crystallization of Al 3 Sm (cubic + hexagonal) [ 51 , 53 ], Al 11 Sm 3 [ 65 ], or Al 3 Ni and Al 3 Sm [ 69 ]. Unknown metastable intermetallics have also been suggested [ 51 , 53 , 54 , 64 , 68 ]. After the third reaction, unknown and Al 11 Sm 3 phases [ 51 , 53 ], only binary phases such as Al 3 Sm and Al 3 Ni [ 67 ] (together to Al 4 Sm and Al 11 Sm 3 [ 69 ]), or binary and ternary phases together such as Al 11 Sm 3 and Al 7 SmNi 2 [ 54 , 62 , 64 ] are reported. Additionally, the continuity of orthorhombic Al 11 Sm 3 and the appearance of tetragonal Al 11 Sm 3 and Al 23 Sm 4 Ni 6 , which then transform from orthorhombic Al 11 Sm 3 to orthorhombic Al 4 Sm, has been proposed [65]. Ce alloys have been reported to lead to unknown metastable phases and (AlNi) 11 La 3 -like phases [ 48 ], or Al 3 Ni, Al 4 Ce, and unidentified phases [ 83 ] as well as to Al 3 Ni, Al 3 Ce, Al 11 Ce 3 , AlCeNi, and unidentified phases [84]. According to these studies, it can be concluded that both Al 3 Ni and a certain ternary phase are causing the two subreactions in the second DSC reaction of the Y and Sm-containing alloys. On the other hand, for Ce-containing alloys, Al3Ni and probably a binary Al-Ce phase should appear. Back to the present study, further heating the second DSC reaction, intermetallics clearly appeared for all the alloys. Figure 6shows the XRD patterns after heating at 20 ◦ C/min to the peak of the third DSC reaction (at about 355–365 ◦ C), to 375 ◦ C (end of the reaction) held for 30 min, to 450 ◦ C and to 600 ◦C. Metals 2020, 10, 443 8 of 19 Regarding Sm alloys, the second stage is related to the crystallization of Al3Sm (cubic + hexagonal) [51,53], Al11Sm3 [65], or Al3Ni and Al3Sm [69]. Unknown metastable intermetallics have also been suggested [51,53,54,64,68]. After the third reaction, unknown and Al11Sm3 phases [51,53], only binary phases such as Al3Sm and Al3Ni [67] (together to Al4Sm and Al11Sm3 [69]), or binary and ternary phases together such as Al11Sm3 and Al7SmNi2 [54,62,64] are reported. Additionally, the continuity of orthorhombic Al11Sm3 and the appearance of tetragonal Al11Sm3 and Al23Sm4Ni6, which then transform from orthorhombic Al11Sm3 to orthorhombic Al4Sm, has been proposed [65]. Ce alloys have been reported to lead to unknown metastable phases and (AlNi)11La3-like phases [48], or Al3Ni, Al4Ce, and unidentified phases [83] as well as to Al3Ni, Al3Ce, Al11Ce3, AlCeNi, and unidentified phases [84]. According to these studies, it can be concluded that both Al3Ni and a certain ternary phase are causing the two subreactions in the second DSC reaction of the Y and Sm-containing alloys. On the other hand, for Ce-containing alloys, Al3Ni and probably a binary Al-Ce phase should appear. Back to the present study, further heating the second DSC reaction, intermetallics clearly appeared for all the alloys. Figure 6 shows the XRD patterns after heating at 20 °C/min to the peak of the third DSC reaction (at about 355–365 °C), to 375 °C (end of the reaction) held for 30 min, to 450 °C and to 600 °C. Figure 6. Cont.
Metals 2020,10, 443 9 of 18 Figure 6. XRD patterns of ( a ) Y, ( b ) Sm, and ( c ) Ce-containing alloys after heat treating to the peak of the third DSC reaction (355–365 ◦ C) to 375 ◦ C (end of the reaction) held for 30 min, to 450 ◦ C and to 600 ◦C. Although some differences were previously observed in the DSC traces for the Ce alloys, the first big difference between the different RE elements studied was now found. The final microstructure, according to the XRD results, was quite similar for the Y and Sm-containing alloys, but different for the Ce alloys. Focusing first on the Y and Sm alloys, the Cu-free Y alloy showed the same pattern for the different heat treatments, with peaks identified as Al, Al 3 Ni, and Al 19 Y 3 Ni 5 . Nevertheless, the quite small amount of Al 3 Ni, and the coincidence of the XRD peaks with those of the other phases, makes its identification difficult. When Cu is added to the Y alloy, the high-temperature microstructure is the same, but it seems to be attained through the evolution of a metastable phase, which tends to transform to the Al 19 Y 3 Ni 5 phase. It is only possible to detect the metastable phase when the third DSC reaction is not completed (i.e., for the treatment to the peak temperature of the third reaction). According to this, the metastable phase tends to grow, and then transforms to the stable phase during the third DSC reaction, probably after appearing during the second DSC reaction. Whether the metastable phase also appears in the Cu-free alloy cannot confirmed from the XRD results because the proximity of the second and third DSC reactions does not make it possible to detect it before the Al 19 Y 3 Ni 5 phase has been totally formed, even when heating to the peak temperature of the third reaction. A similar evolution was found for the Sm-containing alloys. The existence of the Al 19 Sm 3 Ni 5 phase has not been established in previous studies, but according to the peaks’ positions, and through a comparison with the Y alloys, this can be proposed as the stable phase appearing in the Sm alloys. Based on the similarity of the Al 23 Sm 4 Ni 6 and Al 23 Y 4 Ni 6 lattice parameters (1.5939 nm, 0.40967 nm, 1.8320 nm, and 113.09 ◦ for the former [ 85 ], and 1.5836 nm, 0.4068 nm, 1.8311 nm, and 112.97 ◦ for the latter [ 77 ]), this could be an acceptable assumption. Conversely, the metastable phase prevails in the Sm alloys for tougher treatments (with a similar evolution in the Cu-free alloy to that of the Cu-containing
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