Medidas provisórias e o poder legislativo : uma análise do impacto desse instrumento na atividade legislativa do Congresso Nacional no período de 2003-2012

Analisa se, no período 2003-2012, as MPs feriram a separação dos Poderes ao congestionar a atividade do Congresso Nacional, no período 2003-2012. Foi realizada pesquisa bibliográfica e análise de dados da produção legislativa e do trancamento das sessões do CN. Entre outros aspectos, a proporção de MPs em relação às proposições aprovadas pelo CN no período foi de uma em cinco. Concluiu-se que as MPs têm gerado significativo impacto no CN, mas ainda não arrisca a separação dos Poderes

Produção Legislativa nas democracias consolidadas e a eficácia da atividade propositiva

Objetiva iluminar a questão da eficácia no processo legislativo, mediante a comparação da experiência de produção legislativa de democracias consolidadas selecionadas

Gratificação de atividade agropecuária e de abastecimento

Estudo solicitado pela Comissão de Agricultura, Pecuária, Abastecimento e Desenvolvimento Rural da Câmara dos Deputados sobre a possibilidade de apresentação de emenda ao Projeto de Lei Orçamentária Anual - PLOA ou ao Projeto de Lei de Diretrizes Orçamentárias - PLDO, a fim de permitir que o Ministério da Agricultura, Pecuária e Abastecimento – MAPA e/ou o Ministério do Planejamento, Orçamento e Gestão – MPOG “crie Gratificação de Atividade Agropecuária e de Abastecimento para beneficiar servidores administrativos, técnicos e auxiliares do MAPA”.

MEMS basados en aleaciones con memoria de forma magnética

Estudio del comportamiento frente a campos magnéticos y cambios de temperatura de unas aleaciones de NiMnGa depositadas en forma de película delgada sobre voladizos esculpidos en Silicio

Optimization of solution-processed oligothiophene:fullerene based organic solar cells by using solvent additives

The optimization of solution-processed organic bulk-heterojunction solar cells with the acceptor-substituted quinquethiophene DCV5T-Bu-4 as donor in conjunction with PC61BM as acceptor is described. Power conversion efficiencies up to 3.0% and external quantum efficiencies up to 40% were obtained through the use of 1-chloronaphthalene as solvent additive in the fabrication of the photovoltaic devices. Furthermore, atomic force microscopy investigations of the photoactive layer gave insight into the distribution of donor and acceptor within the blend. The unique combination of solubility and thermal stability of DCV5T-Bu-4 also allows for fabrication of organic solar cells by vacuum deposition. Thus, we were able to perform a rare comparison of the device characteristics of the solution-processed DCV5T-Bu-4:PC61BM solar cell with its vacuum-processed DCV5T-Bu-4:C-60 counterpart. Interestingly in this case, the efficiencies of the small-molecule organic solar cells prepared by using solution techniques are approaching those fabricated by using vacuum technology. This result is significant as vacuum-processed devices typically display much better performances in photovoltaic cells. Keywords

Caracterización estructural y magnética de aleaciones intermetálicas Fe-Al-Si mediante espectroscopia Mössbauer

253 p.

Quantum Efficiency And Temperature Coefficients Of Gainp/Gaas Dual-Junction Solar Cell

GaInP/GaAs dual-junction solar cell with a conversion efficiency of 25.2% has been fabricated using metalorganic chemical vapor deposition (MOCVD) technique. Quantum efficiencies of the solar cell were measured within a temperature range from 25 to 160A degrees C. The results indicate that the quantum efficiencies of the subcells increase slightly with the increasing temperature. And red-shift phenomena of absorption limit for all subcells are observed by increasing the cell's work temperature, which are consistent with the viewpoint of energy gap narrowing effect. The short-circuit current density temperature coefficients dJ (sc)/dT of GaInP subcell and GaAs subcell are determined to be 8.9 and 7.4 mu A/cm(2)/A degrees C from the quantum efficiency data, respectively. And the open-circuit cell voltage temperature coefficients dV (oc)/dT calculated based on a theoretical equation are -2.4 mV/A degrees C and -2.1 mV/A degrees C for GaInP subcell and GaAs subcell.

Validación de la cuantificación de la concentración hepática de hierro mediante resonancia magnética nuclear de 1-Tesla

Introducción: La medición de la concentración de hierro hepática (CHH) por RM es una técnica no invasiva de gran utilidad en el diagnóstico de los pacientes con sospecha de sobrecarga férrica en hígado. Objetivo:Validar la eficacia de la RM 1 Tesla en la determinación de la (CHH) en pacientes con sospecha de sobrecarga férrica. Validar su capacidad para diagnosticar o descartar la presencia de una CHH sugestiva de hemocromatosis. Pacientes y métodos:Estudio observacional, transversal, con inclusión prospectiva de pacientes consecutivos. De 2002 a 2010 hemos obtenido la CHH estimada mediante RM 1 Tesla (método Gandon) y de RM 1,5 Tesla (método Alústiza), y mediante BH, en 56 pacientes consecutivos (58RM:35/23). Resultados:Grupo RM 1 Tesla: de acuerdo con CHH en BH, 15 pacientes clasificados como normales (<36µmol/g)-la RM valoró correctamente 7; sobreestimó 8-; 15 grupo hemosiderosis (36-80 µmol/g)-RM valoró correctamente 5, sobreestimó 10-; 5 grupo hemocromatosis (>80 µmol/g)-valoró correctamente las 5-. Existió una correlación entre la determinación de la CHH por BH y RM 1 Tesla con r=0.619. Existieron diferencias estadísticamente significativas (p<0.05) entre CHH media por biopsia (53.43/DE45.67/IC95%37.74 a 69.12) y por RM 1 Tesla (76.14/DE47.31/IC95% 60.46 a 92.97), con sobrevaloración por parte de la RM. Grupo RM 1,5 Tesla: de acuerdo con CHH en BH, normal en 14, hemosiderosis en 6 y hemocromatosis en 3. La RM valoró correctamente 6 y sobreestimó 8 en grupo normal; grupo hemosiderosis, 3 correctamente, 3 sobrevalorados; grupo hemocromatosis, valoró correctamente los 3. La correlación entre CHH por BH y RM 1,5 Tesla fue de r=0.815. La CHH media obtenida por BH (69,34/DE152.1/IC95% 3.57 a 135.1 ) y RM 1,5 Tesla (70.43/DE 57.63/IC95% 45.51 a 95.36) no demostraron diferencias significativas (p>0.05). Conclusiones: La determinación de CHH por RM 1 Tesla (método Gandon) es útil para diagnosticar o descartar hemocromatosis y para diagnosticar CHH normal. Existe una importante tendencia a la sobreestimación en pacientes sin y con sobrecarga férrica en la CHH obtenida por RM 1 Tesla. La determinación de CHH por RM 1,5 Tesla (método Alústiza) es superior a la de RM 1 Tesla, aunque también existe una tendencia a sobreestimar. La CHH media obtenida por BH o RM 1,5 Tesla no tuvieron diferencias significativas. En cambio si existieron entre BH y RM 1 Tesla.

Black holes in the early universe, in compact binaries, and as energy sources inside solar-type stars

This thesis consists of three separate studies of roles that black holes might play in our universe.

In the first part we formulate a statistical method for inferring the cosmological parameters of our universe from LIGO/VIRGO measurements of the gravitational waves produced by coalescing black-hole/neutron-star binaries. This method is based on the cosmological distance-redshift relation, with "luminosity distances" determined directly, and redshifts indirectly, from the gravitational waveforms. Using the current estimates of binary coalescence rates and projected "advanced" LIGO noise spectra, we conclude that by our method the Hubble constant should be measurable to within an error of a few percent. The errors for the mean density of the universe and the cosmological constant will depend strongly on the size of the universe, varying from about 10% for a "small" universe up to and beyond 100% for a "large" universe. We further study the effects of random gravitational lensing and find that it may strongly impair the determination of the cosmological constant.

In the second part of this thesis we disprove a conjecture that black holes cannot form in an early, inflationary era of our universe, because of a quantum-field-theory induced instability of the black-hole horizon. This instability was supposed to arise from the difference in temperatures of any black-hole horizon and the inflationary cosmological horizon; it was thought that this temperature difference would make every quantum state that is regular at the cosmological horizon be singular at the black-hole horizon. We disprove this conjecture by explicitly constructing a quantum vacuum state that is everywhere regular for a massless scalar field. We further show that this quantum state has all the nice thermal properties that one has come to expect of "good" vacuum states, both at the black-hole horizon and at the cosmological horizon.

In the third part of the thesis we study the evolution and implications of a hypothetical primordial black hole that might have found its way into the center of the Sun or any other solar-type star. As a foundation for our analysis, we generalize the mixing-length theory of convection to an optically thick, spherically symmetric accretion flow (and find in passing that the radial stretching of the inflowing fluid elements leads to a modification of the standard Schwarzschild criterion for convection). When the accretion is that of solar matter onto the primordial hole, the rotation of the Sun causes centrifugal hangup of the inflow near the hole, resulting in an "accretion torus" which produces an enhanced outflow of heat. We find, however, that the turbulent viscosity, which accompanies the convective transport of this heat, extracts angular momentum from the inflowing gas, thereby buffering the torus into a lower luminosity than one might have expected. As a result, the solar surface will not be influenced noticeably by the torus's luminosity until at most three days before the Sun is finally devoured by the black hole. As a simple consequence, accretion onto a black hole inside the Sun cannot be an answer to the solar neutrino puzzle.

Cu2O substrates and epitaxial Cu2O/ZnO thin film hetero-structures for solar energy conversion

Future fossil fuel scarcity and environmental degradation have demonstrated the need for renewable, low-carbon sources of energy to power an increasingly industrialized world. Solar energy with its infinite supply makes it an extraordinary resource that should not go unused. However with current materials, adoption is limited by cost and so a paradigm shift must occur to get everyone on the same page embracing solar technology. Cuprous Oxide (Cu2O) is a promising earth abundant material that can be a great alternative to traditional thin-film photovoltaic materials like CIGS, CdTe, etc. We have prepared Cu2O bulk substrates by the thermal oxidation of copper foils as well Cu2O thin films deposited via plasma-assisted Molecular Beam Epitaxy. From preliminary Hall measurements it was determined that Cu2O would need to be doped extrinsically. This was further confirmed by simulations of ZnO/Cu2O heterojunctions. A cyclic interdependence between, defect concentration, minority carrier lifetime, film thickness, and carrier concentration manifests itself a primary reason for why efficiencies greater than 4% has yet to be realized. Our growth methodology for our thin-film heterostructures allow precise control of the number of defects that incorporate into our film during both equilibrium and nonequilibrium growth. We also report process flow/device design/fabrication techniques in order to create a device. A typical device without any optimizations exhibited open-circuit voltages Voc, values in excess 500mV; nearly 18% greater than previous solid state devices.

Earth-abundant materials for solar hydrogen generation

A critical challenge for the 21st century is shifting from the predominant use of fossil fuels to renewables for energy. Among many options, sunlight is the only single renewable resource with sufficient abundance to replace most or all of our current fossil energy use. However, existing photovoltaic and solar thermal technologies cannot be scaled infinitely due to the temporal and geographic intermittency of sunlight. Therefore efficient and inexpensive methods for storage of solar energy in a dense medium are needed in order to greatly increase utilization of the sun as a primary resource. For this purpose we have proposed an artificial photosynthetic system consisting of semiconductors, electrocatalysts, and polymer membranes to carry out photoelectrochemical water splitting as a method for solar fuel generation.

This dissertation describes efforts over the last five years to develop critical semiconductor and catalyst components for efficient and scalable photoelectrochemical hydrogen evolution, one of the half reactions for water splitting. We identified and developed Ni–Mo alloy and Ni₂P nanoparticles as promising earth-abundant electrocatalysts for hydrogen evolution. We thoroughly characterized Ni–Mo alloys alongside Ni and Pt catalysts deposited onto planar and structured Si light absorbers for solar hydrogen generation. We sought to address several key challenges that emerged in the use of non-noble catalysts for solar fuels generation, resulting in the synthesis and characterization of Ni–Mo nanopowder for use in a new photocathode device architecture. To address the mismatch in stability between non-noble metal alloys and Si absorbers, we also synthesized and characterized p-type WSe₂ as a candidate light absorber alternative to Si that is stable under acidic and alkaline conditions.

Nanostructured tungsten trioxide photoanodes for solar energy conversion

Nanostructured tungsten trioxide (WO₃) photoelectrodes are potential candidates for the anodic portion of an integrated solar water-splitting device that generates hydrogen fuel and oxygen from water. These nanostructured materials can potentially offer improved performance in photooxidation reactions compared to unstructured materials because of enhancements in light scattering, increases in surface area, and their decoupling of the directions of light absorption and carrier collection. To evaluate the presence of these effects and their contributions toward energy conversion efficiency, a variety of nanostructured WO₃ photoanodes were synthesized by electrodeposition within nanoporous templates and by anodization of tungsten foils. A robust fabrication process was developed for the creation of oriented WO₃ nanorod arrays, which allows for control nanorod diameter and length. Films of nanostructured WO₃ platelets were grown via anodization, the morphology of the films was controlled by the anodization conditions, and the current-voltage performance and spectral response properties of these films were studied. The observed photocurrents were consistent with the apparent morphologies of the nanostructured arrays. Measurements of electrochemically active surface area and other physical characteristics were correlated with observed differences in absorbance, external quantum yield, and photocurrent density for the anodized arrays. The capability to quantify these characteristics and relate them to photoanode performance metrics can allow for selection of appropriate structural parameters when designing photoanodes for solar energy conversion.