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No description available.

No description available.

The transport critical current density (J(_c)) of a 37 filament Bi-2223/Ag tape has been measured as a function of field and temperature from 4.2 K up to 90 K. Data have been obtained over a large current range from 10 mA up to 100 A and in fields up to 23 T with the tape in 3 orientations with respect to field. These comprehensive data have been used to test the predictions of the flux creep and weak link models used to explain J(_c) in Bi-2223 tapes. The J(_c)(B,T) dependence of optimised Bi-2223 tapes has been calculated using a curved film model. The model assumes perfect grain connectivity and that the local superconducting properties are equivalent to those in the best reported thin films. A comparison between the calculations and measured J(_c)(B,T) dependencies suggest that in high fields at 20 K, J(_c) in presently available industrially processed tapes is only a factor of 8 below the performance of ideal fully optimised tapes. Transport measurements have been made on Bi-2223 single filaments extracted from an alloy sheathed multifilamentary tape in liquid nitrogen at 77 K in fields up to 300 mT with the field aligned parallel and perpendicular to the a-b planes. Further Jc(B,T) data have been taken in a variable temperature insert at temperatures between 60 to 90 K in fields up to 15 T. In a study of the electric field-current density {E-J) characteristics of the c-axis orientated data at 77 K, negative curvature is observed in traces below 280 mT. However, the 280 mT trace exhibits both positive and negative curvature in different current regimes in contrast to the predictions of standard theory. A laboratory scale Bi-2223 superconducting magnet producing a maximum field of 1.29 T at 4.2 K has been designed and fabricated. The magnet comprises 6 resin impregnated double wound pancakes with a 40 mm bore fabricated via the react and wind route. Critical current density measurements have been made as a function of magnetic field, angle and strain at 4.2 K and 77 K on short samples of the constituent tape. The E-J characteristics of all component coils have been measured and a comparison with short sample data shows that minimal additional damage occurred beyond that produced by the bending strain on the tape and the long length variation in J(_c). Sufficient detail is provided for the non-specialist to assess the potential use of brittle superconducting tapes for magnet technology and construct a laboratory scale magnet.

Le gaz électrogénéré dans les réacteurs électrochimiques est un phénomène à la fois électrochimique et hydrodynamique. La chute ohmique dans la solution électrolyte est l'un des paramètres importants à évaluer pour l'optimisation des réacteurs électrochimiques. Elle est due à la résistance de la solution, donc, à sa conductivité électrique et la distance entre les deux électrodes. Pour réduire la consommation énergétique de la cellule de réduction électrolytique de particules d'hématite en fer métallique, on a étudié la conception des anodes, sièges de la production des bulles d'oxygène, dans deux cellules équivalentes d'électrolyse d'eau dans un milieu alcalin. Les résultats ont montré que seulement 25% de l'anode est réellement active et que le taux de rétention augmente le long de l'anode et les bulles atteignent leur vitesse terminale dès 50% de la hauteur de l'anode. Ceci nous a permis de formuler des recommandations qui permettent d'avoir les meilleures conditions de désengagement des bulles électrogénérées, pour une consommation énergétique plus faible du procédé électrochimique / Electrogenerated gas in electrochemical reactors is considered as an electrochemical and hydrodynamic phenomenon. The ohmic drop in the electrolyte solution is one of important parameter to evaluate for the optimization design of electrochemical reactors. It is due to the resistance of the solution, therefore, its electrical conductivity and of the distance between the two electrodes. To reduce the energy consumption of the electrolytic reduction cell of hematite particles to metallic iron, we studied the design of anode, the location of oxygen bubbles production, in two equivalent cells for water electrolysis in an alkali media. The results showed that the gas hold up increases along the anode and only 25% of the initial anode height is actually active. Moreover the bubbles reach their terminal velocity after 50% of the initial anode height. This allowed us to formulate recommendations that allow the best conditions of bubbles electrogenerated disengagement and low energy consumption

The gas diffusion layer (GDL) is one of the key components in a polymer electrolyte membrane (PEM) fuel cell. It performs several functions including the transport of reactant gases and product water to and from the catalyst layer, conduction of both electrons and heat produced in the catalyst layer, as well as mechanical support for the membrane. The overarching goal of this work is to thoroughly examine the GDL structure and properties for use in PEM fuel cells, and more specifically, to determine how to characterize the GDL experimentally ex-situ, to understand its performance in-situ, and to relate theory to performance through controlled experimentation. Thus, the impact of readily measured effective water vapor diffusivity on the performance of the GDL is investigated and shown to correlate to the wet limiting current density, as a surrogate of the oxygen diffusivity to which it is more directly related. The influence of microporous layer (MPL) design and construction on the fuel cell performance is studied and recommendations are made for optimal MPL designs for different operating conditions. A method for modifying the PTFE (Teflon) distribution within the GDL is proposed and the impact of distribution of PTFE in the GDL on fuel cell performance is studied. A method for characterizing the surface roughness of the GDL is developed and the impact of surface roughness on various ex-situ GDL properties is investigated. Finally, a detailed analysis of the physical structure and permeability of the GDL is provided and a theoretical model is proposed to predict both dry and wet gas flow within a GDL based on mercury intrusion porosimetry and porometry data. It is hoped that this work will contribute to an improved understanding of the functioning and structure of the GDL and hence advance PEM fuel cell technology.

Neste trabalho investigamos os efeitos do magnetismo orbital sobre o gás de elétrons tridimensional e sobre íons de camadas abertas em matrizes metálicas. Derivamos uma expressão analítica fechada para a energia de troca do gás de elétrons tridimensional na presença de fortes campos magnéticos, incluindo contribuições do segundo nível de Landau e polarização de spin arbitrária. Esse cálculo generaliza e corrige resultados anteriores disponíveis na literatura. Em seguida, realizamos um cálculo numérico da energia de troca do gás de elétrons tridimensional na presença de campos magnéticos, permitindo a ocupação de um número ilimitado de níveis de Landau, possibilitando assim a obtenção da energia de troca para quaisquer valores de campo magnético e densidade. Em uma abordagem independente, usamos as aproximações de Thomas-Fermi e Thomas-Fermi-Dirac para construir modelos simples para a função dielétrica do gás de elétrons tridimensional no regime de campos magnéticos muito fortes (apenas o primeiro nível de Landau ocupado). Finalmente, estabelecemos vínculos entre os tratamentos fenomenológicos e de primeiros princípios do magnetismo orbital em íons de camadas abertas em matrizes metálicas. Esses vínculos forneceram um embasamento teórico para o uso dos termos de polarização orbital em cálculos Kohn-Sham e levaram à obtenção de expressões aproximadas para os funcionais de troca-correlação da teoria do funcional da densidade de corrente. / In this work, we investigate the effects of orbital magnetism in the three-dimensional electron gas and in open-shell ions in a solid. We derive a closed analytical expression for the exchange energy of the three-dimensional electron gas in strong magnetic fields including the contribution of the second Landau level and arbitrary spin polarization. This calculation generalizes and corrects earlier results available in the literature. Next, we perform a numerical calculation of the exchange energy of the three-dimensional electron gas in a magnetic field, allowing several Landau levels to be occupied, to obtain the exchange energy for arbitrary values of magnetic field and density. In an independent approach, we use the Thomas-Fermi and Thomas-Fermi-Dirac approximations to construct simple model dielectric functions for the three-dimensional electron gas in the strong magnetic field regime (where only the lowest Landau level is occupied). Finally, we establish links between the phenomenological and the first-principles treatment of orbital magnetism in open-shell ions in solids. These links provide a theoretical foundation for the use of orbital polarization terms in Kohn-Sham calculations and allow to obtain approximations to the exchange-correlation functionals of current-density functional theory.

Desenvolvemos um modelo na forma de um mapeamento bidimensional simplético (conservativo) para estudar a evolução das linhas de campo magnético de um plasma confinado no interior de um tokamak. Na primeira parte, consideramos dois perfis estudados na literatura para a densidade de corrente no plasma: um monotônico e um não-monotônico, que dão origem a diferentes perfis analíticos do fator de segurança. Nas simulações, consideramos inicialmente o sistema no equilíbrio, onde observamos, nas seções de Poincaré, apenas linhas invariantes. Em seguida, adicionamos uma perturbação (corrente externa), onde observamos cadeias de ilhas e caos no sistema. Na segunda parte consideramos um perfil também não-monotônico, mas com uma região na qual a densidade de corrente no plasma torna-se negativa, estudo ainda em aberto na literatura, que causa uma divergência no perfil do fator de segurança. Mesmo considerando o sistema apenas no equilíbrio, surgiram cadeias de ilhas muito pequenas em torno de curvas sem shear e caos localizado no sistema, característica não verificada para os outros perfis estudados no equilíbrio. Variando parâmetros relacionados à expressão da densidade de corrente, conseguimos controlar o aparecimento de regiões com cadeias de ilhas em torno de curvas sem shear e regiões caóticas. Para comprovar os resultados, aplicamos o perfil considerado a um outro mapa simplético da literatura (tokamap). Na parte final, consideramos a configuração do perfil do fator de segurança na forma de um divertor. Nessa configuração também temos uma divergência na expressão do perfil do fator de segurança. Observamos características similares (cadeias de ilhas em torno de curvas sem shear e caos) quando consideramos o perfil não-monotônico com densidade de corrente reversa. / We develop a symplectic (conservative) bidimensional map to study the evolution of magnetic field lines of a confined plasma in a tokamak. First, we considered two profiles for the plasma current density, studied in the literature: monotonic and non-monotonic, which give rise to different profiles for the poloidal magnetic field and different analytical profiles for the safety factor. In our simulations, we consider the system initially at equilibrium, where we observe, in Poincaré sections, only invariant lines. Then, we add a perturbation (external current), where we observe island chains and chaos in the system. In the second part, we consider a non-monotonic profile, but with a region which the current density becomes negative, which causes a divergence in the safety factor profile. Even considering only the sistem at equilibrium, very small island chains appeared around the shearless curves, and localized chaos. This feature was not observed for the other profiles at equilibrium. We can control the appearance of the regions with island chaind around the shearless curves and chaotic regions, by variation of parameters related to the density current expression. To comprove our results, we aplly the same profile to the other symplectic map. Finally, we consider a safety factor profile in a divertor configuration. We also have a divergence on in the safety factor profile. We observe similar features (island chains around shearless curves and localized chaos) when we consider a non-monotonic safety factor profile with a reversed density current.

Neste trabalho investigamos os efeitos do magnetismo orbital sobre o gás de elétrons tridimensional e sobre íons de camadas abertas em matrizes metálicas. Derivamos uma expressão analítica fechada para a energia de troca do gás de elétrons tridimensional na presença de fortes campos magnéticos, incluindo contribuições do segundo nível de Landau e polarização de spin arbitrária. Esse cálculo generaliza e corrige resultados anteriores disponíveis na literatura. Em seguida, realizamos um cálculo numérico da energia de troca do gás de elétrons tridimensional na presença de campos magnéticos, permitindo a ocupação de um número ilimitado de níveis de Landau, possibilitando assim a obtenção da energia de troca para quaisquer valores de campo magnético e densidade. Em uma abordagem independente, usamos as aproximações de Thomas-Fermi e Thomas-Fermi-Dirac para construir modelos simples para a função dielétrica do gás de elétrons tridimensional no regime de campos magnéticos muito fortes (apenas o primeiro nível de Landau ocupado). Finalmente, estabelecemos vínculos entre os tratamentos fenomenológicos e de primeiros princípios do magnetismo orbital em íons de camadas abertas em matrizes metálicas. Esses vínculos forneceram um embasamento teórico para o uso dos termos de polarização orbital em cálculos Kohn-Sham e levaram à obtenção de expressões aproximadas para os funcionais de troca-correlação da teoria do funcional da densidade de corrente. / In this work, we investigate the effects of orbital magnetism in the three-dimensional electron gas and in open-shell ions in a solid. We derive a closed analytical expression for the exchange energy of the three-dimensional electron gas in strong magnetic fields including the contribution of the second Landau level and arbitrary spin polarization. This calculation generalizes and corrects earlier results available in the literature. Next, we perform a numerical calculation of the exchange energy of the three-dimensional electron gas in a magnetic field, allowing several Landau levels to be occupied, to obtain the exchange energy for arbitrary values of magnetic field and density. In an independent approach, we use the Thomas-Fermi and Thomas-Fermi-Dirac approximations to construct simple model dielectric functions for the three-dimensional electron gas in the strong magnetic field regime (where only the lowest Landau level is occupied). Finally, we establish links between the phenomenological and the first-principles treatment of orbital magnetism in open-shell ions in solids. These links provide a theoretical foundation for the use of orbital polarization terms in Kohn-Sham calculations and allow to obtain approximations to the exchange-correlation functionals of current-density functional theory.

This work focuses on a better understanding of the behavior of organic light emitting devices (OLEDs) under intense electrical excitation. Attaining high exciton densities in organic semiconductors by electrical excitation is of special interest for the field of organic semiconductor lasers (OSLs). In these devices, the high singlet exciton density needed in the active layer to obtain population inversion is easily created by pulsed optical pumping, but direct electrical pumping has not been achieved yet. First, the steps necessary to achieve stable high current densities in organic semiconductors are discussed. After determining the optimal excitation scheme using single p-doped transport layers, the device complexity is increased up to full p-i-n OLEDs with their power dependent emission spectra. For this purpose, two exemplary emitter systems are chosen: the fluorescent laser dye 4-dicyanomethylene-2-methyl-6-p-dimethylaminostyryl-4H-pyran (DCM) doped into Aluminum(III)bis (2-methyl-8-quinolinato)-4-phenylphenolate (Alq3) and the efficient phosphorescent emitter system N,N'-di(naphthalen-1-yl)-N,N'-diphenyl-benzidine (alpha-NPD) doped by Iridium(III) bis(2-methyl-dibenzo[f,h]quinoxaline)(acetylacetonate) (Ir(MDQ)2(acac)). For pulsed excitation using 50 ns pulses and a repetition rate of 1 kHz, single 100 nm thin p- and n-doped transport layers sustain current densities of over 6 kA/cm2. While the maximum current density decreases with increasing device thickness, the full OLEDs still sustain current densities beyond 800 A/cm2 and exhibit a continuously increasing emission intensity with increasing input power. Next, the time-resolved emission behavior of the singlet and triplet emitter device at high excitation densities is analyzed on the nanosecond scale. Here, the peak emission intensity of the phosphorescent emitter system is found to be more than eight times lower than for the singlet emitter system at comparable current densities. The triplet emitter system exhibits a slow rise of the EL after turn-on which prevents the usage of shorter pulses to enable higher current densities. The singlet emitter system, in contrast, exhibits a fast turn-on and reaches the maximum emission intensity within less than 20 ns. By several additional experiments including streak camera measurements and pump-probe experiments, the strong EL overshoot observed in the first few ns is successfully attributed to a reduced emission intensity in the steady state due to singlet-triplet annihilation. Hence, the separation of singlet emission and singlet-triplet quenching in time domain is demonstrated. At 550 A/cm2 and 10 ns pulse rise time, a peak luminance of 1.5E6 cd/m2 is recorded. Finally, the experimental results are validated by modeling the singlet and triplet population dynamics in the emission layer of the fluorescent system to explain the time-resolved emission characteristics. Using a set of rate equations for the polaron density and the singlet and triplet exciton densities, the overshoot in singlet exciton density at the device turn-on is attributed to the separation of singlet emission and triplet quenching in time domain. Furthermore, by fitting the experimental data, the triplet-triplet annihilation rate in the host guest system is shown to become exciton density dependent at sufficiently high excitation density. / Der Schwerpunkt dieser Arbeit liegt auf dem besseren Verständnis des Verhaltens von organischen Leuchtdioden (OLEDs) bei intensiver elektrischer Anregung. Das Erreichen hoher Exzitonendichten in organischen Halbleitern ist insbesondere für organische Halbleiterlaser (organic semiconductor lasers, OSLs) von Interesse. Hierbei werden die für die Inversion benötigten hohen Singulett Exzitonendichten zwar leicht mittels gepulstem optischen Anregen (Pumpen) erreicht, jedoch konnte eine elektrische Anregung bisher noch nicht realisiert werden. Der erste Abschnitt befasst sich mit dem Erreichen von hohen Stromdichten und den dazu nötigen Schritten. Nach dem Ermitteln des optimalen Anregungsschemas an p-dotierten Einzelschichten wird die Komplexität des Systems Schritt für Schritt bis zur kompletten p-i-n OLED erhöht. Hierfür wurden exemplarisch zwei verschiedene Emittersysteme ausgewählt: Aluminum(III)bis (2-methyl-8-quinolinato)-4-phenylphenolate (Alq3) dotiert mit dem fluoreszenten Laserfarbstoff 4-dicyanomethylene-2-methyl-6-p-dimethylaminostyryl-4H-pyran (DCM) und der effiziente phosphoreszente Emitter Iridium(III)bis(2-methyl-dibenzo[f,h]quinoxaline)(acetylacetonate) (Ir(MDQ)2(acac)) in einer N,N'-di(naphthalen-1-yl)-N,N'-diphenyl-benzidine (alpha-NPD) Matrix.Bei gepulster Anregung mit einer Pulsweite von 50 ns und einer Wiederholungsrate von 1 kHz sind in 100 nm dünnen p- und n-dotierten Transportschichten Stromdichten von mehr als 6 kA/cm2 möglich. Der Maximalstrom sinkt mit zunehmender Gesamtschichtdicke ab. Die kompletten p-i-n OLEDs ermöglichen eine Stromdichte von über 800 kA/cm2 und weisen eine kontinuierlich mit der Stromdichte steigende Emissionsintensität auf. Anschließend wird die zeitlich aufgelöste Elektrolumineszenz der Singulett- und Triplett-Emitter OLEDs mit Nanosekunden-Auflösung untersucht. Die phosphoreszente OLED weist hierbei, im Vergleich zur fluoreszenten OLED bei vergleichbarer Stromdichte, eine mehr als achtmal geringere Emissionsintensität auf. Des Weiteren steigt die Emissionsintensität nur langsam an, die maximale Intensität wird erst nach 120 ns erreicht. Dies steht im Widerspruch zum Erreichen höherer Stromdichten mittels kürzerer Pulse. Die fluoreszente OLED hingegen zeigt ein schnelles Ansteigen der Emissionsintensität, die maximale Intensität wird nach weniger als 20 ns erreicht. Anhand von zusätzlichen Untersuchungen kann das beobachtete starke Überschießen der Elektrolumineszenz innerhalb der ersten Nanosekunden einer durch Singulett-Triplett Annihilation reduzierten Emission im Gleichgewichtszustand zugeordnet werden. Diese Experimente dokumentieren somit die zeitliche Trennung von Fluoreszenz und Singulett-Triplett Annihilation. Bei einer Stromdichte von 550 A/cm2 und 10 ns Flankenanstiegszeit wird eine maximale Lumineszenz von 1.5E6 cd/m2 gemessen. Der letzte Abschnitt befasst sich mit der Bestätigung der experimentellen Ergebnisse durch die Simulation der Dynamik von Singulett- und Triplett-Exzitonendichte in der Emissionsschicht. Mit Hilfe eines Satzes von gekoppelten Differenzialgleichungen für die Dichte der Polaronen, Singulett Exzitonen und Triplett Exzitonen lässt sich das Überschießen der Elektrolumineszenz der fluoreszenten OLED eindeutig der zeitlichen Trennung von Singulett Emission und Singulett-Triplett Annihilation zuordnen. Außerdem kann durch das Fitten der experimentellen Daten dargestellt werden, dass die Triplett-Triplett Annihilationsrate in dem untersuchten fluoreszenten Emittersystem bei ausreichend hohen Anregungsdichten eine starke Abhängigkeit von der Dichte der Triplett Exzitonen aufweist.