Microstructure and texture assessment of Al-Mn-Fe-Si (3003) aluminum alloy produced by continuous and semicontinuous casting processes

Aluminum sheets are currently produced by the direct-chill process (DC). The need for low-cost aluminum sheets is a challenge for the development of new materials produced by the twin roll caster (TRC) process. It is expected that sheets produced from these different casting procedures will differ in their microstructure. These differences in microstructure and in the crystallographic texture have great impact on sheet mechanical properties and formability. The present study investigated microstructure and evaluated texture of two strips of Al-Mn-Fe-Si (3003) aluminum alloy produced by TRC and by hot-rolling processes. It was possible to notice that the microstructure, morphology, and grain size of the TRC sample were more homogenous than those found in hot-rolled samples. Both strips, obtained by the two processes, showed strong texture gradient across the thickness.

Aging behavior in Cu-Al-Be shape memory alloy

This article reports positron annihilation spectroscopy and calorimetric measurements of the aging behavior in a Cu¿Al¿Be shape memory alloy. An excess of single vacancies is retained in the alloy as a result of a quench. All vacancies in excess disappear after long aging time, and a migration energy EM = 1.0±0.1 eV for this process has been found to be larger than in other Cu-based shape memory alloys. The good correlation found for the concentration of vacancies and the shift in the martensitic transition temperature demonstrates that, in Cu¿Al¿Be, changes in the transition after a quench are deeply related to the excess of vacancies.

Reverse martensitic transformation in the Cu-10 wt% Al-6 wt%Ag alloy

The reverse martensitic transformation in the Cu-10 wt%Al-6 wt%Ag alloy was studied by classical differential thermal analysis (IDTA), scanning electron microscopy (SEM), energy dispersive X-ray analysis (EDX) and X-ray diffractometry (XRD). The results indicated that the presence of Ag in the Cu-10%Al alloy is responsible for the separation of the competitive reactions that occur during the reverse martensitic transformation and is also associated to an increase in the disordering degree at high temperatures, when compared with alloys without Ag addition. (c) 2005 Springer Science + Business Media, Inc.

Ageing behavior in the Cu-10 wt.%Al and Cu-10 wt.%Al-4 wt.%Ag alloys

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Thermal behavior of the Cu-10 mass%Al and Cu-10 mass%Al-4 mass%Ag alloys

The thermal behavior of the Cu-10 mass%Al and Cu-10 mass% Al-4 mass%Ag alloys was studied using classical differential thermal analysis (DTA), optical microscopy (OM) and X-ray diffractometry (XRD). The DTA curves were obtained for annealed and quenched samples. The results indicated that the presence of silver introduces new thermal events, associated to the formation of a silver-rich phase, to the shift of the equilibrium concentration to higher A1 contents and to the decomposition of the silver-rich phase in the same temperature range of the beta(1) phase decomposition.

Effect of Ag concentration on the thermal behavior of the Cu-10 mass% Al and Cu-11 mass% Al alloys

In this work the effect of Ag concentration on the thermal behavior of the Cu-10 mass% Al and Cu-11 mass% Al alloys with additions of 4, 6, 8 and 10 mass% Ag was studied using differential scanning calorimetry (DSC), in situ X-ray diffractometry (XRD) and scanning electron microscopy (SEM). The results showed that for the Cu-10 mass% Al alloy Ag addition induce the beta'(1) phase formation and for the Cu-11 mass% Al alloy these additions increase the amount of martensite formed on quenching and decrease the stability range of this phase on heating.

Reaproveitamento de lama vermelha na obtenção de compostos do tipo hidrotalcita do sistema (Zn-Ni-Cu/Fe-Al)-SO4

Compostos do tipo hidrotalcita, também conhecidos como hidróxidos duplos lamelares (HDLs), do sistema (Zn-Ni-Cu/Fe-Al)-SO₄ foram obtidos por meio de co-precipitação a pH variável (crescente) utilizando lama vermelha (LV) como material de partida devido a sua elevada porcentagem de Fe³⁺ e Al³⁺. Para tal estudo, a LV, previamente caracterizada por FRX e DRX, foi submetida à abertura ácida com HCl_conc. e H₂SO₄ 2N. Para os HDLs obtidos, foram avaliados a influência do tipo de cátion bivalente, da variação do pH de síntese (pH 5, 7, 8, 9, 10 e 12) e da variação de razão molar teórica r = M^II/M^III (2, 3 e 4) na sua estrutura cristalina mediante as seguintes técnicas de caracterização: DRX, FT-IR, MEV/EDS, TG/ATD. Os resultados FRX revelaram que a LV é composta principalmente por Fe₂O₃ (32,80%), Al₂O₃ (19,83%), SiO₂ (18,14%) e Na₂O (11,55%). DRX corrobora os resultados da análise química, visto que foram identificados os minerais: hematita, goethita, gibbsita, sodalita, calcita, anatásio e quartzo. Zn-HDLs mostraram que a o aumento de pH de síntese colabora para um melhor ordenamento cristalino do material, uma vez que os picos se tornam melhor definidos, culminando com a melhor condição experimental em pH 9 e r = 3, cujo HDL foi identificado como o mineral natroglaucocerinita (d~11 Ǻ). Nesses valores de pH, a incorporação de SO₄^2- no espaçamento interlamelar foi favorecida apesar da competição com o CO₂ presente no ar atmosférico no momento da síntese. FT-IR também indica a presença do sulfato. As análises por MEV revelam a presença de cristais muito finos e pequenos, > 2μm, de forma hexagonal que pela análise via EDS indicaram, em sua composição, os elementos Na, Zn, Fe, Al, S, C e O. TG/ATD evidenciaram quatro etapas de perda de massa: desidratação, desidroxilação, desoxidenação e dessulfatação, para os HDLs com melhor ordenamento cristalino. Para os materiais menos cristalinos, as duas primeiras etapas ocorrem simultaneamente. Ni-HDLs apresentaram três picos com posições próximas às do mineral carrboydita a partir de pH igual a 7. No entanto, a partir de pH 9, surge hematita como uma fase acessória. Também há disputa entre os ânions SO₄^2- e CO₃^2- no espaço interlamelar, visto que os valores de espaçamento basal d diminuem (de aproximadamente 9,5 até 7,8 Ǻ). Tal fato também foi observado pelo FT-IR. As análises por MEV mostraram aglomerados de minerais anédricos menores que 2μm que, via EDS indicaram composição Ni, Fe, Al, S, C e O. As análises de TG/ATD apresentaram o mesmo comportamento do sistema anterior, evidenciaram as etapas de desidratação, desidroxilação, desoxigenação e dessulfatação e, para os materiais menos cristalinos, as duas primeiras etapas também ocorrem simultaneamente. Cu-HDLs, em valores de pH entre 7 e 10, não cristalizaram a fase HDL tal qual verificada para os sistemas contendo zinco ou níquel. O cobre distorce a estrutura do octaedro causando o chamado Efeito Jahn-Teller: distorção tetraédrica no ambiente octaédrico. As análises por FT-IR apresentaram o mesmo comportamento dos sistemas anteriores, apesar de o material se apresentar amorfo via DRX. O MEV também revela aglomerados amorfos que, de acordo com o EDS, indicaram em sua composição os elementos Cu, Fe, Al, S, C e O. As análises de TG/ATD apresentaram o mesmo comportamento que os materiais menos cristalinos dos dois sistemas anteriores, para os quais as etapas de desidratação e desidroxilação ocorreram simultaneamente. Mt-HDLs (mistura de Zn²⁺, Ni²⁺, Cu²⁺), apresentaram comportamento semelhante aos HDLs de níquel, com quatro picos em posições próximas aos da carrboydita a partir de pH igual a 7. A disputa entre sulfato e carbonato também se repete, visto que os valores de espaçamento basal d diminuem (de aproximadamente 9,5 até 7,9 Ǻ), o que também pode ser notado nos espectros de FT-IR. O MEV dessas amostras também apresentaram aglomerados com tamanhos menores que 2μm e, via EDS, indicaram em sua composição os elementos Zn, Cu, Ni, Fe, Al, S, C e O. Aqui também o comportamento das curvas TG/ATD foi semelhante aos materiais pouco cristalinos obtidos anteriormente.

The effect of iron on liquid film migration and sintering of an Al-Cu-Mg alloy

Analytical transmission electron microscopy indicates that liquid film migration occurs during sintering of an Al-Cu-Mg alloy, that intragranular liquid pools develop from migrating films and that iron segregates to these pools. It is suggested that a high localised iron concentration retards the liquid film migration rate by reducing the coherency strain in the retreating grain, causing a region of the film to detach from the boundary, thus forming an intragranular pool in the advancing grain. Alloys with low iron levels develop few intragranular pools and have high sintered densities. (C) 2003 Acta Materialia Inc. Published by Elsevier Science Ltd. All rights reserved.

Aluminium phosphide as a eutectic grain nucleus in hypoeutectic Al-Si alloys

Aluminium phosphide (AlP) particles arc often suggested to be the nucleation site for eutectic silicon in Al-Si alloys, since both the crystal structure and lattice parameter of AlP (crystal structure: cubic K(4) over bar m; lattice parameter: 5.421 Angstrom) are close to that of silicon (cubic Fd3m, 5.431 Angstrom), and the melting point is higher than the Al-Si eutectic temperature. However, the crystallographic relationships between AlP particles and the surrounding eutectic silicon are seldom reported due to the difficulty in analysing the AlP particles, which react with water during sample preparation for polishing. in this study, the orientation relationships between AlP and Si are analysed by transmission electron microscopy using focused ion-beam milling for sample preparation to investigate the nucleation mechanism of eutectic silicon on AlP. The results show a clear and direct lattice relationship between centrally located AlP particles and the surrounding silicon in the hypoeutectic Al-Si alloy.

Influence of calcium on the microstructure and properties of an Al-7Si-0.3Mg-xFe alloy

The effect of Ca addition on the microstructure, physical characteristics (density/porosity), and mechanical properties (tensile and impact strength) has been investigated in an Al-7Si-0.3Mg-xFe (x = 0.2, 0.4, and 0.7) alloy. The size of Al-Fe intermetallic platelets (beta-Al5FeSi) increased with increasing Fe content. The addition of Ca modified the eutectic microstructure and also reduced the size of intermetallic Fe-platelets, causing improved elongation and impact strengths. A low level of Ca addition (39 ppm) reduced the porosity of the alloys. The tensile strength was decreased marginally with Ca addition. However, Ca addition improved the ductility of the alloy by 18.3, 16.7, and 44 pet and the impact strength by 44, 48, and 15.8 pct for Fe contents of 0.2, 0.4, and 0.7 pct, respectively.

Determination of strontium segregation in modified hypoeutectic Al-Si alloy by micro X-ray fluorescence analysis

Analysis of intra- and inter-phase distribution of modifying elements in aluminium-silicon alloys is difficult due to the low concentrations used. This research utilises a mu-XRF (X-ray fluorescence) technique at the SPring-8 synchrotron radiation facility X-ray source and reveals that the modifying element strontium segregates exclusively to the eutectic silicon phase and the distribution of strontium within this phase is relatively homogeneous. This has important implications for the fundamental mechanisms of eutectic modification in hypoeutectic aluminium-silicon alloys. (c) 2006 Acta Materialia Inc. Published by Elsevier Ltd. All rights reserved.

Chemical similarities between Galactic bulge and local thick disk red giants: O, Na, Mg, Al, Si, Ca, and Ti

Context. The formation and evolution of the Galactic bulge and its relationship with the other Galactic populations is still poorly understood. Aims. To establish the chemical differences and similarities between the bulge and other stellar populations, we performed an elemental abundance analysis of alpha- (O, Mg, Si, Ca, and Ti) and Z-odd (Na and Al) elements of red giant stars in the bulge as well as of local thin disk, thick disk and halo giants. Methods. We use high-resolution optical spectra of 25 bulge giants in Baade's window and 55 comparison giants (4 halo, 29 thin disk and 22 thick disk giants) in the solar neighborhood. All stars have similar stellar parameters but cover a broad range in metallicity (-1.5 < [Fe/H] < +0.5). A standard 1D local thermodynamic equilibrium analysis using both Kurucz and MARCS models yielded the abundances of O, Na, Mg, Al, Si, Ca, Ti and Fe. Our homogeneous and differential analysis of the Galactic stellar populations ensured that systematic errors were minimized. Results. We confirm the well-established differences for [alpha/Fe] at a given metallicity between the local thin and thick disks. For all the elements investigated, we find no chemical distinction between the bulge and the local thick disk, in agreement with our previous study of C, N and O but in contrast to other groups relying on literature values for nearby disk dwarf stars. For -1.5 < [Fe/H] < -0.3 exactly the same trend is followed by both the bulge and thick disk stars, with a star-to-star scatter of only 0.03 dex. Furthermore, both populations share the location of the knee in the [alpha/Fe] vs. [Fe/H] diagram. It still remains to be confirmed that the local thick disk extends to super-solar metallicities as is the case for the bulge. These are the most stringent constraints to date on the chemical similarity of these stellar populations. Conclusions. Our findings suggest that the bulge and local thick disk stars experienced similar formation timescales, star formation rates and initial mass functions, confirming thus the main outcomes of our previous homogeneous analysis of [O/Fe] from infrared spectra for nearly the same sample. The identical a-enhancements of thick disk and bulge stars may reflect a rapid chemical evolution taking place before the bulge and thick disk structures we see today were formed, or it may reflect Galactic orbital migration of inner disk/bulge stars resulting in stars in the solar neighborhood with thick-disk kinematics.