3.1. Phase Analysis of Grain Refiner for Al-5Ti-1B-1RE Master Alloy
The Al-5Ti-1B-1RE intermediate alloy prepared by melt-matching synthesis was analysed for physical phase by XRD diffraction technique. The phase analysis of Al-5Ti-1B-1RE master alloy synthesized by melt-matching method was carried out using XRD diffraction technology. The chemical composition analysis was carried out using German Spike SPECTRO MAXx mm06 direct reading spectrometer. The microstructure of the second phase was analyzed using scanning electron microscopy (SEM), energy dispersive spectrometer, and transmission electron microscopy (TEM). The refinement effect of industrial pure aluminum was observed and analyzed using optical microscope (OM). In the process of synthesis and preparation, when hexachloroethane was pre-pressed into a block and pressed into the aluminum liquid, the absorption rate of the reactants can be greatly increased. The main reason for this was that hexachloroethane produced a large amount of gas at high temperatures, which can play a role in rapid stirring, so that the aluminum powder, titanium powder and potassium fluoborate were fully dispersed and in contact with the melt. C
2Cl
6 is a white crystal with a density of 2.091 g/cm
3 and a sublimation temperature of 185.5℃. It produces the following reaction when pressed into an aluminum liquid [
30]:
The boiling point of the reaction product C
2Cl
4 is 121℃, and participates in refining together with AlCl
3, so that the titanium powder and potassium fluoroborate absorption will be greatly improved. The Al-5Ti-1B-1RE master alloy grain refiner synthesized at a reaction temperature of 830 ℃ was subjected to X-ray diffraction phase analysis, as shown in
Figure 2.
From
Figure 2, it can be seen that during the reaction process, in addition to the diffraction peaks of Al phase, there are also diffraction peaks of TiA1
3, TiB
2 and Ti
2A1
20RE phases. This indicated that Ti, which was supersaturated in the Al melt, should have been synthesized with Al to form the TiA1
3 phase. However, due to the introduction of RE elements, its activity in the Al melt was very high and the surface energy was also very high, in order to reduce the surface energy and its solid solubility in the aluminum melt was very low, there was a free state of the RE elements involved in the reaction of A1 and Ti to generate the Ti
2A1
20RE phase, i.e., Ti
2A1
20Ce and Ti
2A1
20La phase. Due to the fact that KBF
4 and Ti powder were added to the aluminum melt in the form of pressed blocks, the atomic density and reactivity were significantly lower than those of RE added in bulk. Therefore, they preferentially interacted with the Al melt. It mainly underwent the following reactions (6) - (9) [
31]:
As the synthesis reaction proceeded the Ti
2A1
20RE phase was increasing and the amount of TiA1
3 phase was decreasing. However, the reaction (7) proceeded sufficiently due to the excess of added Ti elements, so there was still residual TiA1
3 phase present in the Al melt after TiA1
3 was fully involved in the reaction (9). The TiB
2 phase was very stable, and it did not react with RE, and no titanium-boron rare-earth compounds were detected at the end of the reaction. So the second phase in the synthesized and prepared refiner was mainly TiA1
3, TiB
2, Ti
2A1
20RE phases, as shown in
Figure 2. The chemical composition of the synthesized and prepared Al-5Ti-1B-1RE master alloy refiner was examined as shown in
Table 1, and from the data, it can be indicated that the synthesized chemical composition achieved the chemical composition of the design goal.
The morphological characteristics and distribution of the second phase in the synthesized and prepared Al-5Ti-1B-1RE master alloy were analyzed by scanning electron microscopy (SEM) and energy spectroscopy (EDS). Synthesis reaction temperature of 830 ℃, as shown in
Figure 3, in which the size of the larger gray blocky, with obvious angular phase, as pointed out A in
Figure 3. After further analysis by energy spectroscopy, as shown in
Figure 3b, it mainly contained two elements of aluminum and titanium, with an atomic percentage content ratio of Ti:Al ≈ 1:3, which can be determined as TiA1
3. The appearance shape was similar to TiA1
3, with a larger size and a whitish surface, as indicated by B in
Figure 3. According to the energy spectrum analysis, as shown in
Figure 3 (c), it mainly contained titanium, aluminum, and rare earth elements, with an atomic percentage ratio of Ti: Al: RE ≈ 2:20:1. Based on
Figure 2, it can be determined that the Ti
2A1
20RE phase was composed of Al, A1
3Ti, and RE, and had a complex face-centered cubic structure. The small-sized black gray particles distributed in the matrix, as indicated by C in
Figure 3, were analyzed by energy spectrum. As shown in
Figure 3d, they mainly contain two elements, titanium and boron, and were distributed in the aluminum matrix. Their atomic percentage ratio was Ti: B ≈ 1:2. Combined with
Figure 2, it can be determined that they were TiB
2 phase, which had good chemical stability and did not react with RE. RE mainly acted as a surfactant, dispersant, and catalyst in aluminum melt, adsorbing and forming a liquid film at the solid-liquid interface, hindering the contact between particles, reducing the surface tension of the interface, reducing the contact and repulsive force between second phase particles, reducing agglomeration, and making TiB
2 particles more evenly distributed. It was extremely beneficial for improving the surface wettability and grain refinement of TiA1
3 and TiB
2 in aluminum melt.
From the TEM image of TiB
2 in the Al-5Ti-1B-1RE master alloy at a synthesis temperature of 830 ℃ in
Figure 4, it can be clearly observed that TiB
2 had a relatively regular hexagonal shape with a tendency to aggregate, as indicated by the red arrow in
Figure 4. TiB
2 particles aggregated together, with a cluster size of approximately 1.2μm, while the size of the individual TiB
2 particles is about 0.6 μm, as indicated by the arrows in Figure. 4. When evaluating TiB
2 contained in aluminum master alloy refiners, the standard specifies [
32]: the size of loose TiB
2 agglomerates ≤ 25μm, the presence of no dense TiB
2 agglomerates and TiB
2 particles with a size ≤ 2μm should account for more than 90% with a roughly uniform and dispersed distribution. The TiB
2 agglomerate size in the Al-5Ti-1B-1RE master alloy prepared at synthesis temperature was approximately 1.0 μm ≤ 25μm, with more than 90% of TiB
2 particles having sizes ≤ 2 μm and no dense TiB
2 agglomerates present. This indicated that the TiB
2 particle size in the grain refiner prepared by this process had reached the standard specification.
3.2. Calculation and Analysis of Thermodynamics
Computational analysis of thermodynamics, which was seriously missing from the study of key issues in the preparation process, was carried out during the synthesis of Al-5Ti-1B-1RE master alloys prepared by the melt-matching method due to the approximate Ti/B mass ratio of 5:1 exceeding the mass ratio of Ti and B in TiB
2 (2.2׃1). Therefore, the main reaction products of KBF
4 and Ti in the aluminium alloy melt at atmospheric pressure 1103.15K (temperature 830 °C) are AlB
2, TiAl
3 and TiB
2, whose thermodynamic calculations were in accordance with the conditions of the standard reaction heat effect method calculations, which were carried out by the Kirchhoff equations for the first approximation of the standard reaction heat effect [
33]:
Where: and are the heat and entropy of phase transition of a substance. If the substance undergoing phase transition is a product in the reaction, it is marked with a positive sign, and if it is a reactant, it is marked with a negative sign.
During the synthesis of the prepared Al-5Ti-1B-1RE master alloys by the melt-matching method, the main reactions occurring were as follows:
2KBF4(l)+3Al(l) =AlB2+2KAlF4(l)
=-48072+36.363×1103.15=-7928.15655
Ti(s) +3Al (l) =TiAl3(s)
=-18227+15.712×1103.15=-894.3072
AlB2(s) +TiAl3(s) =TiB2(s) +4Al (l)
=-73381+38.996×1103.15=-30362.5626
According to the thermodynamic data for the standard reaction Gibbs free energy change ∆G ≤ 0, the reaction proceeds spontaneously to the right. When the synthesis temperature was 1103.15 K (830 °C), it was calculated that (1) -48072 + 36.363 × 1103.15= -7928.15655 kJ•mol-1< 0, AlB2 can be produced in the aluminium melt. When, the temperature T1 ≥ 1322.00 K (1048.85 ℃), the reaction (11) proceed to the left and AlB2 cannot stabilise, since the refiner synthesis temperature was at atmospheric pressure 830 ℃ < 1048.85 ℃, AlB2 can stabilise at 830 ℃. When -18227+15.712 × 1103.15=-894.3072kJ• mol-1<0, reaction (12) proceeded to the right to generate TiAl3. When, the temperature T2 ≥ 1160.07K (886.92 ℃), reaction (12) proceeded to the left, and TiAl3 could not exist stably. TiAl3 decomposed and dissolved. Since the synthesis temperature of the grain refiner was at atmospheric pressure 830 ℃ < 886.92 ℃, TiAl3 could exist stably at 830 ℃.When -73381+38.996T3=-73381+38.996 × 1103.15
=-30362.5626 kJ • mol-1<0, reaction (13) proceeded to the right, producing TiB2, which had a much lower free energy ∆ G than AlB2. When , T3 ≥ 1881.76 K (1608.61℃), the reaction (13) proceedsed to the left and TiB2 cannot be stabilised. TiB2 can be stabilised in the synthesis process at atmospheric pressure of 830°C. After adding Al-5Ti-1B-RE refiner to the melt, Al3Ti was dissolved and excess Ti was released into the melt. Due to the more negative Gibbs free energy of TiB2 compared to AlB2 and Al3Ti, from a thermodynamic perspective, AlB2 was extremely unstable in high-temperature A1-Ti-B-RE melts. As the reaction time prolonged, the transformation of AlB2 to TiB2 occurred, i.e., chemical reaction Equation (8): AlB2(s) +TiAl3(s) =TiB2+4Al (l). At the same time, the melting point of AlB2 (950 ℃) was much lower than that of TiB2 phase (2980 ℃), so Ti in the melt tends to combine with B to form TiB2. According to the principle of minimum energy in the system, the system always needs to adjust itself to reach the lowest energy and be in a stable equilibrium state. Therefore, reaction Equation (8) was sufficient to fully occur, ensuring the stable existence of TiB2 particles in the aluminum melt. Under the influence of gravity, the second phases TiB2 and TiAl3 generated by the reaction enter the aluminium melt, where TiAl3 interacted with it due to the presence of rare earths in the melt:
=-227024+74.837×1103.15=-144467.56345 kJ·mol-1< 0
When the synthesis temperature was 1103.15 K (830 °C), by calculating (1) -227024 + 74.837 × 1103.15 = -144467.56345 kJ·mol-1< 0, the result was the production of Ti2A120RE. When T4 ≥ 3033.58 K (2760.43 ℃),, the reaction (14) proceeds to the left, Ti2A120RE can not be stabilised, and Ti2A120RE decomposed and dissolved, and since the refinement agent synthesis temperature was at atmospheric pressure 830℃ < 2760.43℃, Ti2A120RE can be stabilised at 830 ℃. According to the free energies, it can be determined that the synthesis temperature of the grain refiner was 830 ℃, and each reaction (11) - (14) can proceed to the right.
The Gibbs free energy was the lowest in the chemical reaction for synthesizing Ti2A120RE, indicating its best stability. According to the Gibbs free energy function of Equation (14), it can be calculated that at a temperature of T=1103.15 K, ΔG=-144467.56345 kJ • mol-1. The lowest value indicated a very good trend of spontaneous chemical reaction, which was also the fundamental reason why the melt matching reaction method can significantly reduce production costs. Therefore, the synthesis temperature not only affected the thermodynamic process of the reaction, but also caused changes in the composition and structural state of the melt by affecting the stability of the compound, and inherited this change into the solid structure. Therefore, when the synthesis temperature was higher than a certain value, the decomposition of certain phases (e.g. TiAl3, etc.) occurred, which changed the structure of the melt composition, thus affecting the kinetic process of crystallisation.
3.3. Crystallization Kinetics Analysis
The total free energy of the system decreases as the crystal size grows with the growth of the nucleus during the crystallisation process. The reaction continues in a direction that is conducive to the growth of the crystal nucleus. The growth of crystal nuclei is considered to be a process in which atoms in the liquid phase migrate to the surface of the crystal nucleus, i.e., the liquid-solid interface advances towards the liquid phase. During the solidification process, there are two types of atomic migration occurring simultaneously at the liquid-solid interface, namely, the migration of atoms from the liquid phase to the solid phase and the migration of atoms from the solid phase to the liquid phase. If
N represented the number of atoms that migrate per unit area in time t, then [
34]:
Where: RF - the solidification rate, Rm - melting rate, AF - the probabilities of liquid phase atoms reaching the solid phase, Am solid phase atoms reaching the liquid phase and being able to settle (without being bounced back due to collisions), GF - the probabilities of liquid phase atoms transitioning to solid phase, Gm -the probabilities of solid phase atoms transitioning to liquid phase, NL - the atomic migration numbers per unit area of liquid at the interface, Ns the atomic migration numbers per unit area of solid phases at the interface, νL - the vibrational frequencies of the atoms in the liquid, νs - the vibrational frequencies of the atoms in the solid phases, QF - the activation energies of the atoms for the leaps from the liquid phase to the solid phase, Qm - the activation energies of the atoms for the leaps from the solid phase to the liquid phase.
If T
i (interface temperature) = T
m (melting point temperature), then R
F = R
m, Solidification and melting were in dynamic equilibrium, i.e., the number of atoms that migrated from the liquid phase to the solid phase nucleus was equal to the number of atoms that migrated from the nucleus to the liquid phase, so the nucleus cannot grow. To promote the growth of crystal nuclei, that was, to push the solid-liquid interface into the liquid phase,
RF >
Rm was required. The interface temperature T
i that satisfied this condition must be lower than the melting point temperature T
m, that was, there must be a certain dynamic (kinetic) undercooling degree Δ
Tk (Δ
Tk = T
m – T
i) at the interface . The dynamic undercooling Δ
Tk was necessary for achieving net atomic transport from liquid to solid at the interface. And in the supercooled liquid, a large number of phase undulations of varying sizes sprang up every instant. At a certain temperature, the probability of phase fluctuations of different sizes occurring varied. The probability of phase fluctuations occurring in both large and small sizes was small, and there was a limit value r
max for the largest phase fluctuations occurring at each temperature. The size of r
max was related to temperature. The higher the temperature, the smaller the r
max size, and the lower the temperature, the larger the r
max size. The larger phase fluctuations that appeared in supercooled liquids were likely to transform into crystal nuclei during crystallization, and these phase fluctuations were the germ of the crystal nucleus, namely the crystal embryo. The effect of crystal embryo on the crystallisation kinetic process, the nucleation rate (
I) of the solid phase precipitated from the liquid phase [
35]:
Where: I - nucleation rate; k - coefficient of Boltzmann's constant with respect to atomic diffusion; - number of nuclei in the melt; ΔS - entropy of nucleation; ΔT - supercooling of nucleation.
According to Equation (17), the nucleation rate I was directly proportional to the number of embryos in the melt, and increased exponentially with the increase of nucleation undercooling ΔT. Therefore, when preparing Al-5Ti-1B-1RE master alloy by melt matching method, the solid-liquid interface advanced towards the liquid phase when the solidification rate RF >Rm melting rate. If the undercooling degree ΔT of nucleation was larger and the critical number of embryos was greater, the nucleation rate I was higher, vice versa. The higher the melt temperature, the smaller the nucleation supercooling ΔT, the stronger the diffusion of atoms, the smaller phases may merge and grow preferentially and the smaller the number of critical embryos, the lower the nucleation rate I was.
From the above, it can be seen that when the Al-5Ti-1B-1RE master alloy was prepared by the melt-matching method, the nucleation rate I of the undercooled liquid mainly depended on the thermodynamic nucleation work at higher temperatures (with lower undercooling ΔT), and the activation energy Q of dynamic atomic diffusion became a secondary factor. When the temperature was low (with a large degree of undercooling ΔT), the nucleation rate N mainly depended on the kinetic atomic diffusion activation energy Q, while the thermodynamic nucleation work became a secondary factor. When the temperature was appropriate, there was a certain degree of undercooling ΔT, and the thermodynamic nucleation rate I1 and the dynamic nucleation rate I2 had an optimal combination. At this point, the nucleation rate I reached its maximum value and a “peak” appeared on the nucleation rate curve, which was inherited into the solid structure.
Figure 5.
Relationship curve between nucleation rate I and undercooling ΔT.
Figure 5.
Relationship curve between nucleation rate I and undercooling ΔT.