Effects of adding La and Ce to hydrotalcite-type Ni/Mg/Al catalyst precursors on ethanol steam reforming reactions

Catalyst precursors composed of Ni/Mg/Al oxides with added La and Ce were tested in ethanol steam reforming (ESR) reactions. La and Ce were added by anion-exchange. The oxides were characterized by X-ray photoelectron spectroscopy (XPS) and X-ray absorption near-edge structure (XANES) analysis. The catalyst precursors consist of a mixture of oxides, with the nickel in the form of NiO strongly interacting with the support Mg/Al. The XPS analysis showed a lanthanum-support interaction, but no interaction of Ce species with the support. The reaction data obtained with the active catalysts showed that the addition of Ce and La resulted in better H(2) production at 550 degrees C. The CeNi catalyst provided the higher ethanol conversion, with lower acetaldehyde production, possibly clue to a favoring of water adsorption on the weakly interacting clusters of CeO(2) on the surface. (C) 2010 Elsevier B.V. All rights reserved.

Novel Ni-Mg-Al-Ca catalyst for enhanced hydrogen production for the pyrolysis-gasification of a biomass/plastic mixture

A Ni-Mg-Al-Ca catalyst was prepared by a co-precipitation method for hydrogen production from polymeric materials. The prepared catalyst was designed for both the steam cracking of hydrocarbons and for the in situ absorption of CO2 via enhancement of the water-gas shift reaction. The influence of Ca content in the catalyst and catalyst calcination temperature in relation to the pyrolysis-gasification of a wood sawdust/polypropylene mixture was investigated. The highest hydrogen yield of 39.6molH2/g Ni with H2/CO ratio of 1.90 was obtained in the presence of the Ca containing catalyst of molar ratio Ni:Mg:Al:Ca=1:1:1:4, calcined at 500°C. In addition, thermogravimetric and morphology analyses of the reacted catalysts revealed that Ca introduction into the Ni-Mg-Al catalyst prevented the deposition of filamentous carbon on the catalyst surface. Furthermore, all metals were well dispersed in the catalyst after the pyrolysis-gasification process with 20-30nm of NiO sized particles observed after the gasification without significant aggregation.

Síntese, caracterização e avaliação catalítica de Vo x/Mg yAlo x na reação de decomposição do isopropanol

Vanadium oxide supported on hydrotalcite-type precursors was studied in the decomposition of isopropanol. Hydrotalcite-type compounds with different y = Mg+2/Al+3 ratios were synthesized by the method of coprecipitating nitrates of Mg+2 and Al+3 cations with K2CO3 as precipitant. The X-ray diffraction patterns of Al-rich hydrotalcite precursors showed the presence of crystalline phases of brucite and gibbsite. It was shown that chemical composition, texture, acid-base properties of the active sites and also Mg/Al ratio strongly affect the formation of the products in the oxidation of isopropanol. The Al-rich catalysts were much more active than the Mg-rich ones, converting isopropanol mainly to propylene.

Influence of basic properties of Mg,Al-mixed oxides on their catalytic activity in knoevenagel condensation between benzaldehyde and phenylsulfonylacetonitrile

The catalytic performance of Mg,Al-mixed oxides (MO20, MO25 and MO33) derived from hydrotalcites was evaluated in the Knoevenagel reaction between benzaldehyde and phenylsulfonylacetonitrile at 373 and 383 K. The best results were obtained for the sample MO20 that presented the highest basic sites density and external area and the smallest crystallite sizes. The relative amount of basic sites with weak to intermediate strength also played an important role on catalytic performance. By increasing the catalyst content from 1 to 5 wt.% at 383 K, a complete conversion of the reactants is attained, producing α-phenylsulfonylcinnamonitrile with a selectivity of 100%.

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.

Co/Mg/Al hydrotalcite-type precursor, promoted with La and Ce, studied by XPS and applied to methane steam reforming reactions

Catalysts` precursor of Co/Mg/Al promoted with Ce and La were tested in the steam reforming of methane (SRM). The addition of promoters was made by anion-exchange. The oxides characterization was made by X-ray Photoelectron Spectroscopy (XPS) analysis that confirmed Co(2+) species in free form on surface and interacted with Mg and Al in the form of solid solution. In the SRM with high fed molar ratio of H(2)O:CH(4) = 4:1, the catalysts showed a great affinity with water and immediately deactivated by oxidation of the active sites. In the stoichiometric ratio of H(2)O:CH(4) = 2: 1 the catalysts were active and presented low carbon deposition during the time reaction tested. Also a test with low fed molar ratio H(2)O:CH(4) = 0.5:1 was carried out to evaluate the stability of the catalysts by CH(4) decomposition and all the catalysts were stable during 6 h of reaction. Promoted catalysts presented lower carbon deposition. (C) 2009 Elsevier B. V. All rights reserved.

Estudo do uso de hidrotalcites de Mg-Al como catalisadores heterogéneos para produção de biodiesel

A transesterificação de óleos vegetais ou gorduras animais com um álcool de baixo peso molecular é o principal processo utilizado na produção de biodiesel. Actualmente os processos industriais utilizam catalisadores homogéneos para acelerar a reacção. No entanto a utilização de catalisadores heterogéneos, no processo de transesterificação, tem sido sugerido por vários investigadores pois, são amigos do ambiente e podem ser regenerados e reutilizados portanto possibilitam a utilização de processos contínuos. Neste contexto, a utilização de hidrotalcites Mg-Al, como catalisadores heterogéneos para produção de biodiesel foi investigada neste trabalho experimental. As hidrotalcites com diferentes razões molares Mg/Al (Mg/Al=1, 2, 3 e 4) foram preparadas pelo método de co-precipitação. As diversas matrizes catalíticas obtidas, calcinadas a diferentes temperaturas, foram caracterizadas por difracção de raios X (DRX), análise térmica (TG-DSC), espectroscopia de infravermelhos (MIR), microscopia electrónica de varrimento (SEM) e isotérmicas de adsorção com azoto (BET). Estes catalisadores foram testados na metanólise de óleos vegetais para produzir biodiesel. As hidrotalcites Mg/Al=2, HT2A e HT2B (preparada com metade da quantidade de NaOH) calcinadas a 507 ºC e 700 ºC, respectivamente, foram as que apresentaram melhores resultados ao catalisar a reacção com um rendimento em éster superior a 97%, utilizando 2.5% da massa de catalisador, em relação à massa do óleo, razão molar metanol/óleo igual a 12, temperatura reaccional de 65 ºC durante 4h. Foi também investigada a reutilização do catalisador e o efeito da temperatura de calcinação. Constatou-se que o catalisador hidrotalcite HT2B apresentou melhor comportamento catalítico pois permitiu catalisar a reacção de transesterificação até três ciclos reaccionais, convertendo em ésteres 97%, 92% e 34% no primeiro, segundo e terceiro ciclos reaccionais, respectivamente. A análise de, algumas propriedades do biodiesel obtido como, o índice de acidez, a viscosidade e o índice de iodo mostraram que os resultados obtidos estão dentro dos valores limite recomendados pela norma EN 14214. Em anexo apresenta-se uma comunicação à First International Conference on Materials for Energy, Karlsruhe, 2010.

Estudo do Uso de Hidrotalcites de Mg-Al como Catalisadores Heterogéneos para Produção de Biodiesel

A transesterificação de óleos vegetais ou gorduras animais com um álcool de baixo peso molecular é o principal processo utilizado na produção de biodiesel. Actualmente os processos industriais utilizam catalisadores homogéneos para acelerar a reacção. No entanto a utilização de catalisadores heterogéneos, no processo de transesterificação, tem sido sugerido por vários investigadores pois, são amigos do ambiente e podem ser regenerados e reutilizados portanto possibilitam a utilização de processos contínuos. Neste contexto, a utilização de hidrotalcites Mg-Al, como catalisadores heterogéneos para produção de biodiesel foi investigada neste trabalho experimental. As hidrotalcites com diferentes razões molares Mg/Al (Mg/Al=1, 2, 3 e 4) foram preparadas pelo método de co-precipitação. As diversas matrizes catalíticas obtidas, calcinadas a diferentes temperaturas, foram caracterizadas por difracção de raios X (DRX), análise térmica (TG-DSC), espectroscopia de infravermelhos (MIR), microscopia electrónica de varrimento (SEM) e isotérmicas de adsorção com azoto (BET). Estes catalisadores foram testados na metanólise de óleos vegetais para produzir biodiesel. As hidrotalcites Mg/Al=2, HT2A e HT2B (preparada com metade da quantidade de NaOH) calcinadas a 507 ºC e 700 ºC, respectivamente, foram as que apresentaram melhores resultados ao catalisar a reacção com um rendimento em éster superior a 97%, utilizando 2.5% da massa de catalisador, em relação à massa do óleo, razão molar metanol/óleo igual a 12, temperatura reaccional de 65 ºC durante 4h. Foi também investigada a reutilização do catalisador e o efeito da temperatura de calcinação. Constatou-se que o catalisador hidrotalcite HT2B apresentou melhor comportamento catalítico pois permitiu catalisar a reacção de transesterificação até três ciclos reaccionais, convertendo em ésteres 97%, 92% e 34% no primeiro, segundo e terceiro ciclos reaccionais, respectivamente. A análise de, algumas propriedades do biodiesel obtido como, o índice de acidez, a viscosidade e o índice de iodo mostraram que os resultados obtidos estão dentro dos valores limite recomendados pela norma EN 14214. Em anexo apresenta-se uma comunicação à First International Conference on Materials for Energy, Karlsruhe, 2010.

Disseny i implementació d'una aplicació T.P.V. destinada al petit comerç

En el petit comerç i el seu entorn, es produeixen un seguit d'accions totes elles relacionades d'una manera o d'una altra, amb la venda d'articles als clients finals, començant per l'entrada dels articles comprats als proveïdors, passant per l'etiquetatge i acabant per la pròpia venda i el control de vendes posteriors a partir de llistats.Aquest projecte va adreçat a tot el petit negoci que necessita vendre productes d'una manera ràpida, àgil i eficient, així com portar una gestió dels aspectes més rellevants relacionats amb la venda. És en aquest escenari on sorgeix la idea de COMTPV. La finalitat de l'aplicació COMTPV serà la de cobrir les necessitats dels petits comerços per tal de poder informartitzar la venda d'articles als clients finals i les gestions relacionades.

Grain refinement studies on Mg and Mg-Al based alloys

Demand on magnesium and its alloys is increased significantly in the automotive industry because of their great potential in reducing the weight of components, thus resulting in improvement in fuel efficiency of the vehicle. To date, most of Mg products have been fabricated by casting, especially, by die-casting because of its high productivity, suitable strength, acceptable quality & dimensional accuracy and the components produced through sand, gravity and low pressure die casting are small extent. In fact, higher solidification rate is possible only in high pressure die casting, which results in finer grain size. However, achieving high cooling rate in gravity casting using sand and permanent moulds is a difficult task, which ends with a coarser grain nature and exhibit poor mechanical properties, which is an important aspect of the performance in industrial applications. Grain refinement is technologically attractive because it generally does not adversely affect ductility and toughness, contrary to most other strengthening methods. Therefore formation of fine grain structure in these castings is crucial, in order to improve the mechanical properties of these cast components. Therefore, the present investigation is “GRAIN REFINEMENT STUDIES ON Mg AND Mg-Al BASED ALLOYS”. The primary objective of this present investigation is to study the effect of various grain refining inoculants (Al-4B, Al- 5TiB2 master alloys, Al4C3, Charcoal particles) on Pure Mg and Mg-Al alloys such as AZ31, AZ91 and study their grain refining mechanisms. The second objective of this work is to study the effect of superheating process on the grain size of AZ31, AZ91 Mg alloys with and without inoculants addition. In addition, to study the effect of grain refinement on the mechanical properties of Mg and Mg-Al alloys. The thesis is well organized with seven chapters and the details of the studies are given below in detail.

Síntese, caracterização, propriedades e aplicação dos sistemas Mg- Al, Zn-Al e Mg-Fe

The Layered Double Hydroxides has become extremely promising materials due to its range of applications, easily obtained in the laboratory and reusability after calcination, so the knowledge regarding their properties is of utmost importance. In this study were synthesized layered double hydroxides of two systems, Mg-Al and Zn-Al, and such materials were analyzed with X-ray diffraction and, from these data, we determined the volume density, planar atomic density, size crystallite, lattice parameters, interplanar spacing and interlayer space available. Such materials were also subjected to thermogravimetric analysis reasons for heating 5, 10, 20 and 25 ° C / min to determine kinetic parameters for the formation of metaphases HTD and HTB based on theoretical models Ozawa, Flynn-Wall Starink and Model Free Kinetics. In addition, the layered double hydroxides synthesized in this working ratios were calcined heating 2.5 ° C / min and 20 ° C / min, and tested for adsorption of nitrate anion in aqueous solution batch system at time intervals 5 min, 15 min, 30 min, 1h, 2h and 4h. Such calcined materials were also subjected to exposure to the atmosphere and at intervals of 1 week, 2 weeks and 1 month were analyzed by infrared spectroscopy to study the kinetics of regeneration determining structural called "memory effect"

Extraktion und nanoanalytische Charakterisierung refraktärer Nanometallpartikel frühester solarer Materie und Synthese metallischer Nanopartikel aus dotierten Ca-Mg-Al-Si-Schmelzen

Primitive kohlige Chondrite sind Meteorite, die seit ihrer Entstehung im frühen Sonnensystem kaum verändert wurden und dadurch einen Einblick in Prozesse geben, die zur Bildung und Veränderung der ersten festen Materie führten. Solche Prozesse können anhand von Bruchstücken dieser Meteorite detailliert im Labor studiert werden, sodass Rückschlüsse auf die Entwicklung unseres Sonnensystems im frühen Stadium getroffen werden können. Ca-, Al-reiche Einschlüsse (CAIs) aus chondritischen Meteoriten sind die ersten Festkörper des Sonnensystems und enthalten viele refraktäre Metallnuggets (RMNs), welche hauptsächlich aus den Elementen Os, Ir, Ru, Mo und Pt bestehen. Nach weit verbreiteter Ansicht sind diese Nuggets wahrscheinlich im Gleichgewicht mit dem solaren Nebel kondensiert, bereits früher oder gleichzeitig mit Oxiden und Silikaten. Die exakten Mechanismen, die zu ihren heute beobachteten Eigenschaften führten, sind allerdings unklar. Um frühere Arbeiten fortzuführen, wurde eine hohe Anzahl RMNs in vier unterschiedlichen Typen von Meteoriten detailliert studiert, darunter solche aus dem nahezu unveränderten Acfer 094, Allende (CV3ox), Leoville (CV3red) und Murchison (CM2). Die RMNs wurden in-situ, assoziiert mit ihren Wirtsmineralen und auch in Säurerückständen gefunden, deren Präparationsprozedur in dieser Arbeit speziell für RMNs durch eine zusätzliche Dichtetrennung verbessert wurde.rnDie Ergebnisse decken eine Reihe von Ungereimtheiten zwischen den beobachteten RMN-Eigenschaften und einer Kondensationsherkunft auf, sowohl für Kondensation in solarer Umgebung, als auch für Kondensation aus Material von Supernovae oder roten Riesen, für die die Kondensationssequenzen refraktärer Metalle speziell für diesen Vergleich berechnet wurden. Stattdessen wurden in dieser Arbeit neue Einblicke in die RMN-Entstehung und die Entwicklung der ersten Festkörper (CAIs) durch eine Kombination aus experimentellen, isotopischen, strukturellen und petrologischen Studien an RMNs gewonnen. Viele der beobachteten Eigenschaften sind mit Ausfällung der RMN aus einer CAI-Schmelze vereinbar. Ein solches Szenario wird durch entsprechende Untersuchungen an synthetisch hergestellten, mit refraktären Metallen im Gleichgewicht stehenden CAI-Schmelzen bestätigt. Es folgt aus den Ergebnissen, dass die Mehrzahl der RMNs isotopisch solar ist und alle untersuchten RMNs innerhalb von CAIs bei rascher Abkühlung (um bis zu 1000 °C/40 sek.) einer CAI-Schmelze gebildet wurden. rn