Os efeitos da atmosfera de sinterização e do tamanho inicial das partículas na sinterização da céria contendo 10% em mol de gadolínia (GdO1,5) foram sistematicamente estudados neste trabalho. Materiais de partida com três valores para a área de superfície específica foram utilizados, 210 m2/g, 36,2 m2/g e 7,4 m2/g. Diferentes cinéticas de sinterização foram verificadas. Quanto menor o tamanho inicial das partículas, menor é a temperatura para o início da sinterização e mais acelerada a densificação do material. Curvas mestres de sinterização foram construídas para cada um dos materiais analisados. Um programa computacional foi especialmente desenvolvido para este propósito. Diferenças significativas entre as energias de ativação para densificação foram verificadas. Para este trabalho foi determinado que, quanto menor o tamanho inicial de partícula, menores as energias de ativação. A evolução das distribuições de tamanhos de cristalitos foi investigada para os materiais de maior área superficial específica. Foi determinado que a eliminação e migração de poros (pore drag) é o mecanismo predominante para o crescimento de grãos durante o início da sinterização da céria gadolínia. Os efeitos da atmosfera de sinterização no desvio de estequiometria, na densificação, na evolução microestrutural e na condutividade elétrica da céria-gadolínia foram analisados. Atmosferas redutoras, oxidantes e inertes foram usadas para este propósito. Desvios na estequiometria da céria foram verificados no volume do material, sendo este dependente da área de superfície específica e da atmosfera utilizada. Quanto maior o potencial de redução da atmosfera utilizada, maior a concentração de Ce3+ no material. Com o aumento da concentração de Ce3+ um aumento no tamanho médio de grãos foi verificado. Uma diminuição na condutividade elétrica total, intra e intergranular foram determinadas para as amostras sinterizadas em atmosferas redutoras. / The effects of the sintering atmosphere and initial particle size on the sintering of ceria containing 10 mol% gadolinia (GdO1.5) were systematically investigated. The main physical parameter was the specific surface area of the initial powders. Nanometric powders with three different specific surface areas were utilized, 210 m2/g, 36,2 m2/g e 7,4 m2/g. The influence on the densification, and micro structural evolution were evaluated. The starting sintering temperature was verified to decrease with increasing on the specific surface area of raw powders. The densification was accelerated for the materials with smaller particle size. Sintering paths for crystallite growth were obtained. Master sintering curves for gadolinium-doped ceria were constructed for all initial powders. A computational program was developed for this purpose. The results for apparent activation energy showed noticeable dependence with specific surface area. In this work, the apparent activation energy for densification increased with the initial particle size of powders. The evolution of the particle size distributions on non isothermal sintering was investigated by WPPM method. It was verified that the grain growth controlling mechanism on gadoliniadoped ceria is the pore drag for initial stage and beginning of intermediate stage. The effects of the sintering atmosphere on the stoichiometry deviation of ceria, densification, microstructure evolution, and electrical conductivity were analyzed. Inert, oxidizing, and reducing atmospheres were utilized on this work. Deviations on ceria stoichiometry were verified on the bulk materials. The deviation verified was dependent of the specific surface area and sintering atmosphere. Higher reduction potential atmospheres increase Ce3+ bulk concentration after sintering. Accelerated grain growth and lower electrical conductivities were verified when reduction reactions are significantly present on sintering.

Os efeitos da atmosfera de sinterização e do tamanho inicial das partículas na sinterização da céria contendo 10% em mol de gadolínia (GdO1,5) foram sistematicamente estudados neste trabalho. Materiais de partida com três valores para a área de superfície específica foram utilizados, 210 m2/g, 36,2 m2/g e 7,4 m2/g. Diferentes cinéticas de sinterização foram verificadas. Quanto menor o tamanho inicial das partículas, menor é a temperatura para o início da sinterização e mais acelerada a densificação do material. Curvas mestres de sinterização foram construídas para cada um dos materiais analisados. Um programa computacional foi especialmente desenvolvido para este propósito. Diferenças significativas entre as energias de ativação para densificação foram verificadas. Para este trabalho foi determinado que, quanto menor o tamanho inicial de partícula, menores as energias de ativação. A evolução das distribuições de tamanhos de cristalitos foi investigada para os materiais de maior área superficial específica. Foi determinado que a eliminação e migração de poros (pore drag) é o mecanismo predominante para o crescimento de grãos durante o início da sinterização da céria gadolínia. Os efeitos da atmosfera de sinterização no desvio de estequiometria, na densificação, na evolução microestrutural e na condutividade elétrica da céria-gadolínia foram analisados. Atmosferas redutoras, oxidantes e inertes foram usadas para este propósito. Desvios na estequiometria da céria foram verificados no volume do material, sendo este dependente da área de superfície específica e da atmosfera utilizada. Quanto maior o potencial de redução da atmosfera utilizada, maior a concentração de Ce3+ no material. Com o aumento da concentração de Ce3+ um aumento no tamanho médio de grãos foi verificado. Uma diminuição na condutividade elétrica total, intra e intergranular foram determinadas para as amostras sinterizadas em atmosferas redutoras. / The effects of the sintering atmosphere and initial particle size on the sintering of ceria containing 10 mol% gadolinia (GdO1.5) were systematically investigated. The main physical parameter was the specific surface area of the initial powders. Nanometric powders with three different specific surface areas were utilized, 210 m2/g, 36,2 m2/g e 7,4 m2/g. The influence on the densification, and micro structural evolution were evaluated. The starting sintering temperature was verified to decrease with increasing on the specific surface area of raw powders. The densification was accelerated for the materials with smaller particle size. Sintering paths for crystallite growth were obtained. Master sintering curves for gadolinium-doped ceria were constructed for all initial powders. A computational program was developed for this purpose. The results for apparent activation energy showed noticeable dependence with specific surface area. In this work, the apparent activation energy for densification increased with the initial particle size of powders. The evolution of the particle size distributions on non isothermal sintering was investigated by WPPM method. It was verified that the grain growth controlling mechanism on gadoliniadoped ceria is the pore drag for initial stage and beginning of intermediate stage. The effects of the sintering atmosphere on the stoichiometry deviation of ceria, densification, microstructure evolution, and electrical conductivity were analyzed. Inert, oxidizing, and reducing atmospheres were utilized on this work. Deviations on ceria stoichiometry were verified on the bulk materials. The deviation verified was dependent of the specific surface area and sintering atmosphere. Higher reduction potential atmospheres increase Ce3+ bulk concentration after sintering. Accelerated grain growth and lower electrical conductivities were verified when reduction reactions are significantly present on sintering.

Solid Oxide Fuel Cells (SOFCs) are devices that directly convert chemical energy into electrical energy, without proceeding through a Carnot combustion cycle. These devices are based on the usage of solid oxide electrolytes operating at relatively elevated temperatures. Two major hurdles must be overcome in order to decrease the operating temperatures of practical SOFCs. The first relates to reducing ohmic losses within solid electrolytes. The second relates to the need for developing high performance electrodes since electrolyte reaction rates at both anode and cathode are affected detrimentally as operating temperatures fall. This PhD project has focussed on addressing the first hurdle in two innovative ways: 1. the implementation of solid electrolytes with higher ionic conductivity than zirconia, 2. the development of very thin film electrolytes as thick as 5ƒÝm. Several thin films with novel electrode-electrolyte structures were fabricated and evaluated in order to demonstrate the viability of low temperature SOFC operations. Development of such thin films was innovative and challenging to achieve. The approach taken in this work involved fabricating a dense and thin gadolinia doped ceria (10GDC - Gd 10wt%, Ce 90wt%) oxide electrolyte. 10GDC is an electrolyte exhibiting higher conductivities than conventional materials during low temperature operations. A research contribution of this PhD was the demonstration of the deposition of 10GDC thin films using RF magnetron sputtering for the first time. 10GDC thin film electrolytes with thickness in a range between 0.1 to 5ƒÝm were fabricated on 10 yttrium stabilised zirconium (10YSZ) substrates by using a RF magnetron sputterer. The primary parameters controlling 10GDC thin film deposition using this method were explored in order to identify optimal conditions. The fabricated films were subsequently analysed for their morphology, composition and stoichiometry using a variety of methods, including Scanning Electron Microscopy (SEM) with Energy Dispersive X-ray Spectrometry (EDS), optical microscopy, X-ray Photoelectron Spectroscopy (XPS), and X-ray Diffraction (XRD). A preliminary test was conducted in order to examine the function of 10GDC thin film electrolytes together with the cathode and anode substrates at intermediate temperatures (700oC). A complete planar single cell was designed and assembled for this purpose. However, when fully assembled and tested, the cell failed to generate any voltage or current. Consequently, the remainder of the PhD work was focused on systematically exploring the factors contributing to the assembled fuel cell failure. As fabrication failure analysis is seldom reported in the scientific literature, this analysis represents a significant scientific contribution. This analysis proceeded in a series of steps that involved several different methods, including SEM, red dye analysis, surface morphology and cross section analysis of the cell. It was found that pinholes and cracks were present during the fuel cell operating test. Cathode delamination was also found to have occurred during the test operation. This was determined to be due to thermal expansion mismatch between the cathode substrate and the 10GDC electrolyte thin film. A series of suggestions for future research are presented in the conclusion of this work.

Made available in DSpace on 2014-12-17T14:06:52Z (GMT). No. of bitstreams: 1 BeatrizC.pdf: 4078508 bytes, checksum: 01a5dec5db97a60acc69b635fdbd40bc (MD5) Previous issue date: 2009-01-04 / The direct use of natural gas makes the Solid Oxide Fuel Cell (SOFC) potentially more competitive with the current energy conversions technologies. The Intermediate Temperature SOFC (IT-SOFC) offer several advantages over the High Temperature SOFC (HT-SOFC), which includes better thermal compatibility among components, fast start with lower energy consumption, manufacture and operation cost reduction. The CeO2 based materials are alternatives to the Yttria Stabilized Zirconia (YSZ) to application in SOFC, as they have higher ionic conductivity and less ohmic losses comparing to YSZ, and they can operate at lower temperatures (500-800?C). Ceria has been doped with a variety of cations, although, the Gd3+ has the ionic radius closest to the ideal one to form solid solution. These electrolytes based in ceria require special electrodes with a higher performance and chemical and termomechanical compatibility. In this work compounds of gadolinia-doped ceria, Ce1-xGdxO2-δ (x = 0,1; 0,2 and 0,3), used as electrolytes, were synthesized by polymeric precursors method, Pechini, as well as the composite material NiO - Ce0,9Gd0,1O1,95, used as anode, also attained by oxide mixture method, mixturing the powders of the both phases calcinated already. The materials were characterized by X ray diffraction, dilatometry and scanning electronic microscopy. The refinement of the diffraction data indicated that all the Ce1-xGdxO2-δ powders were crystallized in a unique cubic phase with fluorite structure, and the composite synthesized by Pechini method produced smaller crystallite size in comparison with the same material attained by oxide mixture method. All the produced powders had nanometric characteristics. The composite produced by Pechini method has microstructural characteristics that can increase the triple phase boundaries (TPB) in the anode, improving the cell efficiency, as well as reducing the mass transport mechanism effect that provokes anode degradation / A utiliza??o direta do g?s natural torna a c?lula a combust?vel de ?xido s?lido (SOFC) potencialmente mais competitiva com as atuais tecnologias para convers?o de energia. A SOFC de temperatura intermedi?ria (IT-SOFC) oferece muitas vantagens sobre a SOFC de alta temperatura (HT-SOFC), que incluem melhor compatibilidade t?rmica entre os componentes, partida r?pida com menos consumo energ?tico, redu??o de custos de obten??o e opera??o. Os materiais baseados em CeO2 s?o alternativas aos eletr?litos de zirc?nia estabilizada com ?tria (YSZ) para aplica??es em SOFC, pois t?m condutividade i?nica maior e menores perdas ?hmicas em compara??o a YSZ, e podem operar a temperaturas mais baixas (500-800?C). C?ria tem sido dopada com uma variedade de c?tions, entretanto, o Gd3+ possui o raio i?nico mais pr?ximo do ideal para forma??o da solu??o s?lida. Esses eletr?litos baseados em c?rio requerem eletrodos especiais com um alto desempenho e compatibilidade termomec?nica e qu?mica. Neste trabalho compostos c?ria dopada com gadol?nia, Ce1-xGdxO2-δ (x = 0,1; 0,2 e 0,3), utilizadas como eletr?litos, foram sintetizados a partir do m?todo dos precursores polim?ricos, Pechini, assim como o material comp?sito NiO - Ce0,9Gd0,1O1,95, usado para anodo, obtido tamb?m pelo m?todo de mistura dos ?xidos, p?s das duas fases j? calcinadas. Os materiais foram caracterizados atrav?s das t?cnicas de difra??o de raios X, dilatometria e microscopia eletr?nica de varredura. O refinamento dos dados obtidos pela difra??o de raios X indicou que todos os p?s de Ce1-xGdxO2-δ cristalizaram em uma ?nica fase c?bica com estrutura fluorita, e que o comp?sito obtido por Pechini produziu menores tamanhos de cristalitos das fases em compara??o com o p? sintetizado por mistura de ?xidos em uma mesma temperatura de calcina??o. Todos os p?s obtidos t?m caracter?sticas nanom?tricas. O comp?sito obtido por Pechini possui caracter?sticas microestruturais que podem aumentar a fronteira de fase tripla (TPB) dentro do anodo, melhorando a efici?ncia da c?lula, assim como reduzir o efeito do mecanismo de transporte de massa que provoca degrada??o do anodo

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