XPS Study of Chemical Changes on the La/Ce Treated Surface of A361 Aluminium Alloy Exposed to Air at Temperatures up to
The chemical changes that take place on the rare earth treated surface of the A361 aluminium alloy exposed to air at temperatures between 100 and have been examined using X-ray photoelectron spectroscopy (XPS). The most notable features discussed in this work are the disappearance of Mg and Si signals at the tested temperatures and disappearance of the Ce signal at temperatures of 400–. The biphasic microstructure of the A361 alloy, constituted by close to 12 wt% Si and the Al matrix, plays an important role in many of the results obtained. The notable growth of aluminium oxide across the conversion coating in the case of the Ce-treated surface is related to the structural transformation experienced by the cerium oxide coating at 400–.
The literature contains many studies on the behaviour of “refractory” alloys in exposure to temperatures of around 900–1000°C and the changes that rare earths produce on oxidation kinetics and the properties of the oxide films formed [1–9]. In this respect there has been shown to be a connection between these properties and oxide film growth mechanisms, and in particular the diffusion processes of reacting species [4, 6, 10–12]. In contrast, much less information is available on the oxidation behaviour of aluminium alloys exposed to relatively high temperatures, namely, 400–500°C, close to the material’s melting point.
The present work aims to contribute to knowledge on the processes that take place on the surface of the aforementioned aluminium alloy, treated with La or Ce salts, when exposed to the oxidising action of the environmental atmosphere at temperatures up to 500°C. Specifically the authors have studied changes in the chemical composition of the surface layer formed on the biphasic alloy A361, trying to relate these changes with changes in the growth mechanisms. The effect of rare earth conversion coatings applied on the A361 aluminium alloy has been studied by Pardo and their coworkers [13–15]. Following on with this issue, we examine now in greater depth some of the results reported hitherto.
The tested material was A361 aluminium cast alloy (10.5 Si, 0.53 Fe, 0.1 Cu, 0.12 Mn, 0.36 Mg, 0.11 Zn, balance Al). Prior to lanthanide treatments samples were wet ground through successive grades of silicon carbide abrasive papers from P120 to P1200, followed by diamond finishing to 0.1 m, rinsed in acetone, and dried. Oxidation was carried out in an airflow laboratory atmosphere.
The optimal conditions for electrodeposition of Ce-based coatings on composite rectangular specimens (dimensions: 30 mm 20 mm 3 mm) were achieved as follows: (a) degreasing with isopropyl alcohol in an ultrasonic bath for 5 minutes at 25°C; (b) immersion in 75% ethylene glycol monobutyl ether solution with 2000 ppm Ce (CeCl37H2O) and 1.5 wt.% NaCl followed by application of a cathodic potential of 3 V for 10 minutes at 25°C; (c) rinsing with water and drying at 105°C. The optimal conditions for electrodeposition of La-based coatings were similar, replacing 2000 ppm Ce (CeCl37H2O) with 2000 ppm La (LaCl37H2O) in the ethylene glycol mono-butyl ether solution .
Photoelectron spectra were recorded using a Fisons MT500 spectrometer (XPS) equipped with a hemispherical electron analyser (CLAM 2) and an Mg K X-ray source operated at 300 W. The samples were mechanically fixed on small flat discs supported on an XYZ manipulator placed in the analysis chamber. The residual pressure in this ion-pumped analysis chamber was maintained below 10−8 Torr during data acquisition. The spectra were collected for 20–90 minutes, depending on the peak intensities at a pass energy of 20 eV, which is typical of high-resolution conditions. The intensities were estimated by calculating the area under each peak after smoothing and subtraction of the S-shaped background and fitting the experimental curve to a mix of Lorentzian and Gaussian lines of variable proportion. Although sample charging was observed, accurate binding energies (BEs) could be determined by referencing to the adventitious C 1s peak at 285.0 eV. Atomic ratios were computed from peak intensity ratios and reported atomic sensitivity factors . The XPS analyses were normally repeated two or three times to ensure their reasonable reproducibility. The results are average compositions. The sampled areas were mm2.
The thickness of the aluminium oxide layer on the surface of the specimens was determined using the expression given by Strohmeier :
where is the thickness of the aluminium oxide layer (in nm); is the photoelectron output angle; and are the intensity of the aluminium components in metallic state and as oxide on the Al2p peak; and are the mean free path of photoelectrons in the substrate and the oxide layer; and and are the volume densities of aluminium atoms in metal and oxide . The and are 2.2 and 2.4 nm, respectively, and an ratio of 1.5 was used .
3. Results and Discussion
3.1. General Tendencies and Effect of the Microstructure
Besides the notable presence of Al and O signals at all the oxidation temperatures (Figure 1), XPS analysis of the surface of the untreated A361 alloy has revealed the presence of Si and Mg alloying elements. The intensity of the Si signal shows a clear tendency to decrease with the temperature below 300°C, while the Mg signal only appears above around 400°C, becoming especially relevant at 500°C (Figures 1 and 2).
Like the untreated surface, the surface of the A361 alloy treated with La or Ce solutions shows both O and Al signals but accompanied in this case by the La signal at all temperatures (Figure 3), or by the Ce signal at all temperatures except 500°C (Figures 4 and 5). On the other hand, conversion treatment leads to the complete disappearance of the Si signal at all the tested temperatures, which is explained by the fact that the conversion coating is built on the Si phase of this biphasic alloy [13–16]. The Mg signal is also seen to be totally absent, even at 400–500°C, temperatures at which the signal of this element had appeared on the untreated surface.
According to the above results, the following features are worthy of discussion: (i) the appearance of the Mg signal on the untreated A361 alloy at 400–500°C; (ii) the disappearance of the Mg and Si signals at all the temperatures on the treated A361 alloy; (iii) the disappearance of the Ce signal and weakening of the La signal on the treated A361 alloy at temperatures of 400–500°C.
Among the factors that probably influence the results it is necessary to consider the microstructure of the A361 alloy, with close to 12% of its surface constituted by practically pure Si (proeutectic and eutectic) and the rest by an also practically pure Al matrix . These two phases behave in different ways, both during the process of formation of the conversion coating on the metal surface and during subsequent oxidation of the A361 alloy at high temperature. As has been shown in the previous work [13–15], the deposition of rare earth elements on the A361 alloy tends to take place on surface areas corresponding to the Al-Si eutectic and primary Si precipitates, which leads to an unequal response of different points of the surface to the oxidising action of the atmosphere. Images of the heterogeneous nature of the deposits of cerium and lanthanum oxides on the surface of A361 and other Al-Si materials can be seen in earlier papers by Pardo et al. [20–22]. The Al2O3 film will therefore preferentially grow on the -Al phase areas which are apparently not protected by the conversion coating; as will be seen below, a certain degree of aluminium oxidation below the conversion coating cannot be ruled out as the coating is not completely impermeable to oxygen.
3.2. Bare Surface
Considerable Mg enrichment of the outermost surface of the untreated A361 alloy has been found at 400–500°C (Figure 6), as shown, for instance, by the Mg/Al atomic ratio value of 0.4 on the A361 surface at 500°C compared to the value of for the bulk alloy composition.
The major driving force for Mg segregation seems to be the formation of magnesium oxide by reaction with the air [12, 23, 24]. The effect is related with the different heats of formation of aluminium and magnesium oxides, with the latter being favoured. The activation energy for diffusion is also lower for Mg than for Al [12, 23–25]. As a result, the oxide film formed at high temperature on the surface of Mg-containing aluminium alloys soon becomes Mg enriched. In contrast, at room temperature an amorphous Al2O3 film is formed on the alloy surface and acts as a barrier, preventing the diffusion of a large amount of Mg through it [3, 12, 23–26]. When this film is heated above 350–400°C, the Al2O3 attains partial crystallisation , which allows Mg to diffuse through the film towards the oxide/gas interface, and therefore its oxidation in the outer part of the film . Crystallised alumina grain boundaries, or interphase boundaries between the crystalline and amorphous Al2O3, may act as diffusion short-circuits [2, 26, 27]. The presence of MgAl2O4 in the oxide film has also been related with much faster diffusion of Mg ions through the Al2O3 compared to Al and Si ions .
As illustrated in Figure 6, a value of 0.35 has been found for the Si/Al atomic ratio on the surface of the A361 alloy heated in the air at temperatures between 100 and 300°C. This ratio decreases at higher temperatures until becoming practically equal at 500°C (bulk atomic ratio0.1). Therefore, the degree of Si enrichment of the A361 alloy surface is very moderate throughout the studied temperature range. The weakening of the Si signal in the 400–500°C range may be due to lateral extension (beyond the boundary with the Si phase) of the Al2O3 film which grows from the -Al matrix, a phenomenon that will become more evident as the temperature rises. Mg diffusion via the boundaries between the Si and -Al phases  may also contribute to the concealment of the Si signal.
3.3. La and Ce Treated Surfaces
Treatment of the A361 alloy with La or Ce salt solutions leads to the formation of a nonhomogeneous surface consisting of large patches or islands of rare earth oxide together with portions of apparently clean metal. The rare earth islands are about 300 nm thick and are mainly located over the Si phase and the Al-Si eutectic colonies . According to XPS measurements the proportion of the surface occupied by rare earth atoms is of the order of 40–60%. The rest of the surface (-Al phase) is covered by a Al2O3 film of just a few nanometres in thickness, for example around 4–8 nm, depending on the oxidation temperature .
Besides being the basic component of the conversion coating islands that spread across the A361 alloy surface, the La and Ce ions must also be present in a small proportion on the remaining -Al phase areas apparently unaffected by the conversion coating, in this case as an impurity (or dopant) in the thin aluminium oxide film that grows on the -Al phase. In research on oxide formation on aluminium alloys in boiling CeCl3 solution, Gorman et al.  reported some incorporation of Ce ions into the Al2O3 of the order of 1 at% Ce.
XPS data for the rare earth treated A361 surfaces (Figures 3 and 4) shows the complete disappearance of the Si signal, despite the fact that this alloying element constitutes 12 at% of the bulk alloy. This is explained by considering that the conversion coating is built on the Si rich areas, which it thereby isolates, and so this element goes unnoticed.
The presence of Mg is also not to be expected on the surface areas protected by the thick islands of rare earth precipitates. However, Mg should at least be detected (as in the aforementioned case of the bare surface) at 400–500°C on the portions of the surface that the conversion coating leaves unprotected. For this reason the complete absence of any Mg signal at these temperatures suggests a radical change in the way the Al2O3 film thickens. One hypothesis is that the presence of small amounts of rare earth ions dissolved in the Al2O3 film lattice prevents diffusion of Mg ions from the inner oxide interface to the outer oxide-air interface by blocking the short-circuit diffusion paths in the Al2O3 oxide [3, 4, 12, 23–26, 29].
3.4. Weakening of the La Signal and Disappearance of the Ce Signal
XPS analysis of the treated A361 surface oxidised at 400–500°C shows a weakening of the La signal on the La treated surface (Figure 3) and the complete disappearance of the Ce signal on the Ce treated surface (Figures 4 and 5). This phenomenon is explained by the growth of aluminium oxide across the rare earth conversion coating.
The presence of Al2O3 on the outermost surface of the conversion coating strongly suggests that the oxidation process on the coated A361 alloy takes place mostly due to outward Al diffusion from the alloy-oxide interface and not to the inward diffusion of oxygen from the oxide-air interface. Figure 7 shows schematically how the diffusion of aluminium cations and the migration of electrons explains the appearance of Al2O3 on the outermost surface of the rare earth coating, which is in contact with the air; line and planar defects in the oxide form channels or conduits through which species diffuse rapidly (short circuit diffusion). The Al3+ ions can move along the interfaces present in the La or Ce oxide layers which run from the alloy film interface to the outer film surface.
The importance of the process of aluminium growth and extension on the rare earth treated surfaces has been quantified in the 100–500°C temperature range by means of the RE/Al XPS atomic ratio between the surface concentration of rare earths (REs) and aluminium. Figure 8 shows that the RE/Al ratio tends to decrease as the temperature rises, above all in the case of the Ce conversion coatings, where at 500°C the ratio is practically zero. Thus the permeation of the conversion coating by Al3+ ions from oxidation of the substrate, and the growth from them of the Al2O3 film on the outer surface of the coating, seems to take place much more quickly in on the Ce treated surface than on the La treated surface of the A361 alloy.
The aforementioned difference in behaviour between the two rare earths is most likely due to the structural transformation experienced by the cerium oxide at 400–500°C since the valence of cerium changes at this temperature from trivalent to tetravalent, a change that does not take place in the case of La, which remains trivalent throughout the tested temperature range. It may be imagined that the change of valence transforms the oxide into a more defective and open structure, causing greater diffusion of Al3+ ions via microcapillaries in the oxide .
4. Conclusions(1)XPS analysis of the A361 alloy surface oxidised in air at several temperatures shows important changes in the chemical composition of the surfaces treated with lanthanum or cerium salts, depending on the oxidation temperature and the nature of the conversion coating applied.(2)Notable features include the disappearance of the Mg signal on the La or Ce treated surfaces and its presence on the untreated surface oxidised at 400–500°C. It is also notable that the Si signal disappears at all the tested temperatures, and that the La signal is weakened and the Ce signal completely disappears at 400–500°C.(3)The changes in the surface chemistry have been related with changes in the Al2O3 film growth mechanism, which can proceed unevenly on the different microstructural areas of the alloy.(4)The behaviour of the cerium treated surface at 400–500°C stands out due to the transformation experienced by cerium oxide at these temperatures, as the valence of cerium changes from trivalent to tetravalent.
The authors are grateful to the MCYT (Project MAT 2009-13530).
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