Thesis (Ph.D.)--Boston University / Lutetium oxide doped with europium oxide (Lu20 3:Eu3+) has been established to be a bright, dense scintillator materi al with vast potential in both medical and high resolution X-ray imaging applications. Unfortunately its commercial viability has been restricted due to the manufacturing and post treatment costs associated with device fabrication. This research was aimed at the development of two vapor deposition techniques; chemical and physical vapor deposition (CVD and PVD), to produce coatings of Lu203:Eu3+ for various X-ray imaging applications. A customized CVD process to codeposit Lu20 3 and Eu20 3 was developed using lutetium and europium chloride (LuCb and EuCI3) precursors and reacting with carbon dioxide (C02) and hydrogen (H2) . An in depth study was performed by systematically varying the process parameters to explore the deposition kinetics and identify the rate limiting steps and their effects on the growth morphology using both cold and hot wall CVD reactors. The activation energy for the kinetically limited deposition of Lu20 3 from the LuCI3 - Ar - C02 - H2 system was identified to be approximately 170 kJ/mol , which is significantly lower than expected. The predominant growth orientations were identified to be { 111} and { 100} , depending on the deposition conditions. As the temperature is increased, the growth orientation preference decreases to produce a randomly oriented growth at 1150°C. The scintillation and X-ray imaging characteristics of a co-deposited Lu203:Eu3+ thin film with a {100} orientation were measured, confirming the feasibility and applicability of the CVD system to produce thick scintillator x-ray imaging devices. A fundamental study of the PVD process was performed by sputtering of Lu203:Eu3+ using a single target magnetron sputtering gun. Systematic vatiations of the deposition parameters were used to understand the effect of the ejected flux kinetic energies and deposition rate on the deposit density, stress, optical and scintillation properties. The deposition system was subsequently optimized for rapid, dense growth of a 10 um thick Lu203:Eu3+ coating at elevated temperatures. The X-ray imaging properties were measured and the results yielded an X-ray imaging resolution slightly better than 1 um with the potential for 0.5 um with further optimization, a level never before attained.

Lutetium oxide doped with europium (Lu2O3:Eu3+) has been established as a promising scintillator material with properties that are advantageous when compared to other scintillators such as cesium iodide doped with thallium (CsI:Tl). Due to high X-ray attenuation characteristics, Lu2O3:Eu3+ is an attractive material for use in high resolution digital X-ray imaging systems. However, challenges still remain especially in the area of light output for Lu2O3:Eu3+. Processing by physical vapor deposition (PVD) and manipulation of oxygen defect structure was explored in order to better understand the effect on the scintillation phenomena. PVD results were obtained using high temperature radio frequency sputtering (RF) and pulsed laser deposition (PLD) systems. Characterization of light output by radial noise power spectrum density measurements revealed that high temperature RF films were superior to those obtained using PLD. Optimization of sputtered films based on light output over a range of process parameters, namely temperature, power, pressure, and substrate orientation was investigated. Parameterization of deposition conditions revealed that: 75 watts, 10.00 mtorr, and 800°C were optimum conditions for Lu2O3:Eu3+ films. Manipulation of anionic defect structure in similar material systems has been shown to improve scintillation response. Similar methods for Lu2O3:Eu3+ were explored for hot pressed samples of Lu2O3:Eu3+; via controlled atmosphere annealing, and use of extrinsic co-doping with calcium. The controlled atmosphere experiments established the importance of oxygen defect structure within Lu2O3:Eu3+ and showed that fully oxidized samples were preferred for light output. The second method utilized co-doping by the addition of calcium which induced oxygen vacancies and by Frenkel equilibrium changed the oxygen interstitial population within the Lu2O3:Eu3+ structure. The addition of calcium was investigated and revealed that scintillation was improved with a maximum response occurring at 340ppm of calcium. PVD optimization and co-doping experimental results provided a template for the use of calcium co-doped Lu2O3:Eu3+ targets for deposition of films. Preliminary deposition results were promising and revealed that small additions (around 550 ppm) of calcium resulted in better activator efficiency. Calcium co-doped films have a predicted increase in the light yield greater than 14% when compared to analogous un-doped Lu2O3:Eu3+ films at 60keV.

A luminescência persistente é um fenômeno em que o material emite radiação de segundos a várias horas após cessada a irradiação (luz, radiação UV, feixe de elétrons, etc.). No entanto, os mecanismos que geram o fenômeno da luminescência persistente ainda não são totalmente estabelecidos. Neste trabalho os materiais Lu2O3:TR3+,M (TR,M: Pr,HfIV; Eu, Ca2+ ou Tb,Ca2+) foram preparados pelo método de estado-sólido assistido por micro-ondas (MASS) e comparados com aqueles sintetizados pelo método cerâmico. As vantagens do método MASS incluem curto tempo de processamento, aquecimento dielétrico seletivo, baixo consumo de energia e uso de equipamentos de baixo custo (forno micro-ondas doméstico), muitas vezes produzindo produtos de alta pureza e alto rendimento. Os materiais foram caracterizados pelas técnicas de espectroscopia de absorção na região do infravermelho (IR), espectroscopia Raman, difração de raios X método do pó (DRX), microscopia eletrônica de varredura (MEV), X-ray absorption near edge structure (XANES), Extended X-ray absorption fine structure (EXAFS), X-ray Excited Optical Luminescence (XEOL), espectroscopia de fotoluminescência na região do UV-Visível, espectroscopia de fotoluminescência na região do UV-UV vácuo e termoluminescência (TL). Os fósforos Lu2O3:TR3+,M (TR,M: Pr,HfIV; Eu, Ca2+ ou Tb,Ca2+) foram preparados em um curto período de tempo (22-26 min) pelo método MASS utilizando forno micro-ondas doméstico, carvão ativado como susceptor, fluxos (H3BO3 ou Na2CO3) e sem a aplicação de gases. Todos materiais preparados com fluxo de H3BO3 exibem impurezas de LuBO3 que foram quantificadas por refinamento Rietveld. Os fluxos e os dopantes não alteraram consideravelmente a estrutura cristalina da matriz C-Lu2O3. As micrografias MEV sugerem que o fluxo de Na2CO3 e os precursores nitratos geram partículas de Lu2O3 com tamanho menor devido a evolução de gases provenientes da decomposição destes compostos. Por outro lado, quando é usado óxidos como precursores os materiais apresentam maiores tamanhos de partícula e na presença de H3BO3 leva a maior agregação. Os dados de XANES indicam que houve completa redução do íon TbIV &#8594 Tb3+ e parcial do PrIV &#8594 Pr3+, devido ao uso de carvão ativado que gera CO(g) durante o tratamento térmico. Os espectros da luminescência persistente indicam emissões nas regiões do vermelho/NIR, vermelho alaranjado e verde atribuídas as transições 4fN &#8594 4fN características dos íons Pr3+, Eu3+ e Tb3+, respectivamente. As diferenças entre os espectros registrados sob excitação UV e após cessada a irradiação podem ser explicadas pela emissão da luminescência persistente predominante dos íons TR3+ no sítio S6 do que no C2. Além disso, a co-dopagem aliovalente com os íons HfIV e Ca2+ aumentam a intensidade e duração da luminescência persistente. Isto ocorre através da geração de armadilhas provenientes dos dois co-dopantes nos sítios de Lu3+ e por defeitos produzidos na compensação de carga. Os materiais fotônicos preparados pelo método MASS com fluxo de H3BO3 apresentam maior intensidade e duração da luminescência persistente comparados aos preparados pelo método cerâmico ou sem a presença de H3BO3. Os mecanismos da luminescência persistente foram desenvolvidos através de princípios similares baseados nos dados experimentais da energia do band gap, posição dos níveis de energia dos íons TR3+/2+ na matriz e energia das armadilhas. Isto confirma a solidez da interpretação dos dados experimentais dos materiais Lu2O3:TR3+,M exibindo luminescência persistentes e encoraja a expansão de modelos similares para outros materiais apresentando esse fenômeno. Os fósforos Lu2O3:Pr3+,HfIV,Lu2O3:Eu3+(,Ca2+) e Lu2O3:Tb3+,Ca2+) apresentaram sintonização de cores de emissão tanto para o fenômeno da fotoluminescência como da luminescência persistente, podendo atuar como bons candidatos nas aplicações de bioimageamento ou sensibilizadores de células solares. / Persistent luminescence is a phenomenon where the material emits radiation from seconds to several hours after cessation of irradiation (light, UV radiation, electron beam, etc.). The persistent luminescence mechanisms are not entirely established, however. In this work, the materials Lu2O3:TR3+,M (TR,M: PrHfIV; Eu, Ca2+ or Tb,Ca2+) were prepared by MASS method as well as compared to these materials synthetized by ceramic method. The advantages of MASS method include short processing time, selective dielectric heating, low energy consumption and use of inexpensive equipment (domestic microwave oven), often affording high-purity and high-yield products. The materials were characterized by Infrared absorption spectroscopy (IR), Raman spectroscopy, X-ray powder diffraction (XPD), Scanning electron microscopy (SEM), X-ray absorption near edge structure (XANES), Extended X-ray absorption fine structure (EXAFS), X-ray excited optical luminescence (XEOL), photoluminescence spectroscopy in the UV-Visible range, photoluminescence spectroscopy in the UV-UV vacuum region and thermoluminescence (TL). The phosphorsLu2O3:TR3+,M (TR,M: Pr,HfIV; Eu, Ca2+ or Tb,Ca2+) were rapidly (22-26 min) and successfully prepared by MASS method using a domestic microwave oven, carbon as susceptor, fluxes (H3BO3 or Na2CO3) and without special gases application. All materials prepared with H3BO3 flux exhibit LuBO3 impurities that were quantified by Rietveld refinement. The flux and dopants does not considerably affect the crystalline structure of the C-Lu2O3 host matrix. Scanning electron micrographs suggest that Na2CO3 flux and nitrates precursors produce Lu2O3 particles of small size due to the gases evolution from the decomposition of these compounds. On the other hand, the materials prepared from oxides precursors have particles of large size and H3BO3 flux induces particle xi aggregation. The carbon used as the susceptor generates CO gas, leading to complete reduction of TbIV to Tb3+ and partial conversion of PrIV to Pr3+ present in the Tb4O7 and Pr6O11 precursors, as indicated by XANES. Persistent luminescence spectra of the materials show emission in the red/NIR, reddish orange and green ranges assigned to the 4fN &#8594 4fN transitions characteristics of Pr3+, Eu3+ and Tb3+ ions, respectively. Differences between the spectra recorded under UV excitation and after ceased the irradiation can be explained by the predominant persistent luminescence emission of TR3+ ion in the S6 site rather than TR3+ in the C2 site. In addition, inclusion of HfIV and Ca2+ codopants in the Lu2O3 host increases the emission intensity and duration of persistent luminescence due to generation of traps caused by charge compensation in the lattice as well as these metal ions in the Lu3+ sites. The photonic materials prepared by MASS method with H3BO3 flux show higher persistent luminescence performance than those prepared by the ceramic method or MASS without flux. The persistent luminescence mechanisms were developed through similar principles based on experimental data of band gap energy, energy level positions of TR3+/2+ ions in the host and traps energy. This similarity confirms the consistency of the interpretation of experimental data for the Lu2O3:TR3+,M materials and encourages the expansion of similar models for other persistent luminescence materials. Color tuning of persistent luminescence in Lu2O3:TR3+,M (TR,M: Pr,HfIV; Eu,Ca2+ or Tb,Ca2+) provides potential applications in bioimaging as well as in solar cell sensitizers.

A luminescência persistente é um fenômeno em que o material emite radiação de segundos a várias horas após cessada a irradiação (luz, radiação UV, feixe de elétrons, etc.). No entanto, os mecanismos que geram o fenômeno da luminescência persistente ainda não são totalmente estabelecidos. Neste trabalho os materiais Lu2O3:TR3+,M (TR,M: Pr,HfIV; Eu, Ca2+ ou Tb,Ca2+) foram preparados pelo método de estado-sólido assistido por micro-ondas (MASS) e comparados com aqueles sintetizados pelo método cerâmico. As vantagens do método MASS incluem curto tempo de processamento, aquecimento dielétrico seletivo, baixo consumo de energia e uso de equipamentos de baixo custo (forno micro-ondas doméstico), muitas vezes produzindo produtos de alta pureza e alto rendimento. Os materiais foram caracterizados pelas técnicas de espectroscopia de absorção na região do infravermelho (IR), espectroscopia Raman, difração de raios X método do pó (DRX), microscopia eletrônica de varredura (MEV), X-ray absorption near edge structure (XANES), Extended X-ray absorption fine structure (EXAFS), X-ray Excited Optical Luminescence (XEOL), espectroscopia de fotoluminescência na região do UV-Visível, espectroscopia de fotoluminescência na região do UV-UV vácuo e termoluminescência (TL). Os fósforos Lu2O3:TR3+,M (TR,M: Pr,HfIV; Eu, Ca2+ ou Tb,Ca2+) foram preparados em um curto período de tempo (22-26 min) pelo método MASS utilizando forno micro-ondas doméstico, carvão ativado como susceptor, fluxos (H3BO3 ou Na2CO3) e sem a aplicação de gases. Todos materiais preparados com fluxo de H3BO3 exibem impurezas de LuBO3 que foram quantificadas por refinamento Rietveld. Os fluxos e os dopantes não alteraram consideravelmente a estrutura cristalina da matriz C-Lu2O3. As micrografias MEV sugerem que o fluxo de Na2CO3 e os precursores nitratos geram partículas de Lu2O3 com tamanho menor devido a evolução de gases provenientes da decomposição destes compostos. Por outro lado, quando é usado óxidos como precursores os materiais apresentam maiores tamanhos de partícula e na presença de H3BO3 leva a maior agregação. Os dados de XANES indicam que houve completa redução do íon TbIV &#8594 Tb3+ e parcial do PrIV &#8594 Pr3+, devido ao uso de carvão ativado que gera CO(g) durante o tratamento térmico. Os espectros da luminescência persistente indicam emissões nas regiões do vermelho/NIR, vermelho alaranjado e verde atribuídas as transições 4fN &#8594 4fN características dos íons Pr3+, Eu3+ e Tb3+, respectivamente. As diferenças entre os espectros registrados sob excitação UV e após cessada a irradiação podem ser explicadas pela emissão da luminescência persistente predominante dos íons TR3+ no sítio S6 do que no C2. Além disso, a co-dopagem aliovalente com os íons HfIV e Ca2+ aumentam a intensidade e duração da luminescência persistente. Isto ocorre através da geração de armadilhas provenientes dos dois co-dopantes nos sítios de Lu3+ e por defeitos produzidos na compensação de carga. Os materiais fotônicos preparados pelo método MASS com fluxo de H3BO3 apresentam maior intensidade e duração da luminescência persistente comparados aos preparados pelo método cerâmico ou sem a presença de H3BO3. Os mecanismos da luminescência persistente foram desenvolvidos através de princípios similares baseados nos dados experimentais da energia do band gap, posição dos níveis de energia dos íons TR3+/2+ na matriz e energia das armadilhas. Isto confirma a solidez da interpretação dos dados experimentais dos materiais Lu2O3:TR3+,M exibindo luminescência persistentes e encoraja a expansão de modelos similares para outros materiais apresentando esse fenômeno. Os fósforos Lu2O3:Pr3+,HfIV,Lu2O3:Eu3+(,Ca2+) e Lu2O3:Tb3+,Ca2+) apresentaram sintonização de cores de emissão tanto para o fenômeno da fotoluminescência como da luminescência persistente, podendo atuar como bons candidatos nas aplicações de bioimageamento ou sensibilizadores de células solares. / Persistent luminescence is a phenomenon where the material emits radiation from seconds to several hours after cessation of irradiation (light, UV radiation, electron beam, etc.). The persistent luminescence mechanisms are not entirely established, however. In this work, the materials Lu2O3:TR3+,M (TR,M: PrHfIV; Eu, Ca2+ or Tb,Ca2+) were prepared by MASS method as well as compared to these materials synthetized by ceramic method. The advantages of MASS method include short processing time, selective dielectric heating, low energy consumption and use of inexpensive equipment (domestic microwave oven), often affording high-purity and high-yield products. The materials were characterized by Infrared absorption spectroscopy (IR), Raman spectroscopy, X-ray powder diffraction (XPD), Scanning electron microscopy (SEM), X-ray absorption near edge structure (XANES), Extended X-ray absorption fine structure (EXAFS), X-ray excited optical luminescence (XEOL), photoluminescence spectroscopy in the UV-Visible range, photoluminescence spectroscopy in the UV-UV vacuum region and thermoluminescence (TL). The phosphorsLu2O3:TR3+,M (TR,M: Pr,HfIV; Eu, Ca2+ or Tb,Ca2+) were rapidly (22-26 min) and successfully prepared by MASS method using a domestic microwave oven, carbon as susceptor, fluxes (H3BO3 or Na2CO3) and without special gases application. All materials prepared with H3BO3 flux exhibit LuBO3 impurities that were quantified by Rietveld refinement. The flux and dopants does not considerably affect the crystalline structure of the C-Lu2O3 host matrix. Scanning electron micrographs suggest that Na2CO3 flux and nitrates precursors produce Lu2O3 particles of small size due to the gases evolution from the decomposition of these compounds. On the other hand, the materials prepared from oxides precursors have particles of large size and H3BO3 flux induces particle xi aggregation. The carbon used as the susceptor generates CO gas, leading to complete reduction of TbIV to Tb3+ and partial conversion of PrIV to Pr3+ present in the Tb4O7 and Pr6O11 precursors, as indicated by XANES. Persistent luminescence spectra of the materials show emission in the red/NIR, reddish orange and green ranges assigned to the 4fN &#8594 4fN transitions characteristics of Pr3+, Eu3+ and Tb3+ ions, respectively. Differences between the spectra recorded under UV excitation and after ceased the irradiation can be explained by the predominant persistent luminescence emission of TR3+ ion in the S6 site rather than TR3+ in the C2 site. In addition, inclusion of HfIV and Ca2+ codopants in the Lu2O3 host increases the emission intensity and duration of persistent luminescence due to generation of traps caused by charge compensation in the lattice as well as these metal ions in the Lu3+ sites. The photonic materials prepared by MASS method with H3BO3 flux show higher persistent luminescence performance than those prepared by the ceramic method or MASS without flux. The persistent luminescence mechanisms were developed through similar principles based on experimental data of band gap energy, energy level positions of TR3+/2+ ions in the host and traps energy. This similarity confirms the consistency of the interpretation of experimental data for the Lu2O3:TR3+,M materials and encourages the expansion of similar models for other persistent luminescence materials. Color tuning of persistent luminescence in Lu2O3:TR3+,M (TR,M: Pr,HfIV; Eu,Ca2+ or Tb,Ca2+) provides potential applications in bioimaging as well as in solar cell sensitizers.

Les détecteurs de rayon-X utilisés pour l'imagerie à haute résolution (micromètrique ou submicronique) utilisés aux synchrotrons sont pour la plupart basés sur un système de détection indirecte. Les rayons X ne sont pas directement convertis en signal électrique. Ils sont absorbés par un scintillateur qui est un matériau émettant de la lumière à la suite de l'absorption d'un rayonnement ionisant. L'image émise sous forme de lumière visible est ensuite projetée par des optiques de microscopie sur une camera 2D de type CCD ou CMOS. De nos jours, il existe différents types des scintillateurs. On distingue entre autres des scintillateurs en poudre compactée, micro structurés, céramique poly-cristalline et monocristalline. L’obtention d’une image de très bonne qualité avec une résolution spatiale au-dessous du micromètre requiert le choix d’une couche mince (1-20 µm) monocristalline. Ces types des scintillateurs peuvent être déposes sur un substrat par épitaxie en phase liquide. La très faible efficacité d’absorption dans une couche mince en fait sa faiblesse, surtout pour des énergies au-dessus de 20 keV. A l’ESRF (le synchrotron européen) des énergies jusqu'à 120 keV peuvent être exploitées pour l’imagerie. Des nouveaux scintillateurs sont donc toujours recherchés pour pouvoir améliorer le compromis entre l’efficacité d’absorption et la résolution spatiale. Dans la première partie de cet travail, un model qui décrit les détecteurs indirects pour la haute résolution, est présenté. Cet model permet de calculer la MTF (fonction de transfert de modulation) du système et peut être utilisé pour trouver la combinaison optimal de scintillateur et d’optique selon l’énergie des rayons X. Les simulations ont guidées le choix des scintillateurs à développer par épitaxie.Dans la deuxième partie, deux nouveaux types de scintillateurs développés et caractérisés dans le cadre de ce projet de thèse sont introduits : les couches minces basées sur des monocristaux de gadolinium lutétium aluminium pérovskite (GdLuAP:Eu) et d’oxyde de lutétium (Lu2O3:Eu) / X-ray detectors for high spatial resolution imaging are mainly based on indirect detection. The detector consists of a converter screen (scintillator), light microscopy optics and a CCD or CMOS camera. The screen converts part of the absorbed X-rays into visible light image, which is projected onto the camera by means of the optics. The detective quantum efficiency of the detector is strongly influenced by the properties of the converter screen (X-ray absorption, spread of energy deposition, light yield and emission wavelength). To obtain detectors with micrometer and sub-micrometer spatial resolution, thin (1-20 µm) single crystal film scintillators are required. These scintillators are grown on a substrate by liquid phase epitaxy. The critical point for these layers is their weak absorption, especially at energies exceeding 20 keV. At the European Synchrotron radiation Facility (ESRF), X-ray imaging applications can exploit energies up to 120 keV. Therefore, the development of new scintillating materials is currently investigated. The aim is to improve the contradictory compromise between absorption and spatial resolution, to increase the detection efficiency while keeping a good image contrast even at high energies.The first part of this work presents a model describing high-resolution detectors which was developed to calculate the modulation transfer function (MTF) of the system as a function of the X-ray energy. The model can be used to find the optimal combination of scintillator and visible light optics for different energy ranges, and it guided the choice of the materials to be developed as SCF scintillators. In the second part, two new kinds of scintillators for high-resolution are presented: the gadolinium-lutetium aluminum perovskite (Gd0.5Lu0.5AlO3:Eu) and the lutetium oxide (Lu2O3:Eu) SCFs