Efeitos de campos aleatórios e de anisotropias em vidros de spins

Ising and m-vector spin-glass models are studied, in the limit of infinite-range in-teractions, through the replica method. First, the m-vector spin glass, in the presence of an external uniform magnetic field, as well as of uniaxial anisotropy fields, is consi-dered. The effects of the anisotropics on the phase diagrams, and in particular, on the Gabay-Toulouse line, which signals the transverse spin-glass ordering, are investigated. The changes in the Gabay-Toulouse line, due to the presence of anisotropy fields which favor spin orientations along the Cartesian axes (m = 2: planar anisotropy; m = 3: cubic anisotropy), are also studied. The antiferromagnetic Ising spin glass, in the presence of uniform and Gaussian random magnetic fields, is investigated through a two-sublattice generalization of the Sherrington-Kirpaktrick model. The effects of the magnetic-field randomness on the phase diagrams of the model are analysed. Some confrontations of the present results with experimental observations available in the literature are discussed

Anisotropias da radiação cósmica de fundo e vínculos em modelos com decaimento do vácuo

Many astronomical observations in the last few years are strongly suggesting that the current Universe is spatially flat and dominated by an exotic form of energy. This unknown energy density accelerates the universe expansion and corresponds to around 70% of its total density being usually called Dark Energy or Quintessence. One of the candidates to dark energy is the so-called cosmological constant (Λ) which is usually interpreted as the vacuum energy density. However, in order to remove the discrepancy between the expected and observed values for the vacuum energy density some current models assume that the vacuum energy is continuously decaying due to its possible coupling with the others matter fields existing in the Cosmos. In this dissertation, starting from concepts and basis of General Relativity Theory, we study the Cosmic Microwave Background Radiation with emphasis on the anisotropies or temperature fluctuations which are one of the oldest relic of the observed Universe. The anisotropies are deduced by integrating the Boltzmann equation in order to explain qualitatively the generation and c1assification of the fluctuations. In the following we construct explicitly the angular power spectrum of anisotropies for cosmologies with cosmological constant (ΛCDM) and a decaying vacuum energy density (Λ(t)CDM). Finally, with basis on the quadrupole moment measured by the WMAP experiment, we estimate the decaying rates of the vacuum energy density in matter and in radiation for a smoothly and non-smoothly decaying vacuum

Acelaração do universo e criação gravitacional de matéria escura fria: novos modelos e testes observacionais

Recent astronomical observations (involving supernovae type Ia, cosmic background radiation anisotropy and galaxy clusters probes) have provided strong evidence that the observed universe is described by an accelerating, flat model whose space-time properties can be represented by the FriedmannRobertsonWalker (FRW) metric. However, the nature of the substance or mechanism behind the current cosmic acceleration remains unknown and its determination constitutes a challenging problem for modern cosmology. In the general relativistic description, an accelerat ing regime is usually obtained by assuming the existence of an exotic energy component endowed with negative pressure, called dark energy, which is usually represented by a cosmological constant ¤ associated to the vacuum energy density. All observational data available so far are in good agreement with the concordance cosmic ¤CDM model. Nevertheless, such models are plagued with several problems thereby inspiring many authors to propose alternative candidates in the relativistic context. In this thesis, a new kind of accelerating flat model with no dark energy and fully dominated by cold dark matter (CDM) is proposed. The number of CDM particles is not conserved and the present accelerating stage is a consequence of the negative pressure describing the irreversible process of gravitational particle creation. In order to have a transition from a decelerating to an accelerating regime at low redshifts, the matter creation rate proposed here depends on 2 parameters (y and ߯): the first one identifies a constant term of the order of H0 and the second one describes a time variation proportional to he Hubble parameter H(t). In this scenario, H0 does not need to be small in order to solve the age problem and the transition happens even if there is no matter creation during the radiation and part of the matter dominated phase (when the ß term is negligible). Like in flat ACDM scenarios, the dimming of distant type Ia supernovae can be fitted with just one free parameter, and the coincidence problem plaguing the models driven by the cosmological constant. ACDM is absent. The limits endowed with with the existence of the quasar APM 08279+5255, located at z = 3:91 and with an estimated ages between 2 and 3 Gyr are also investigated. In the simplest case (ß = 0), the model is compatible with the existence of the quasar for y > 0:56 whether the age of the quasar is 2.0 Gyr. For 3 Gyr the limit derived is y > 0:72. New limits for the formation redshift of the quasar are also established

Espectro das ondas de spin lineares e não-lineares em multicamadas magnéticas anisotrópicas

Conselho Nacional de Desenvolvimento Científico e Tecnológico

Efeito Kerr magneto-óptico; Ressonância ferromagnética; Acoplamento bilinear; Acoplamento biquadrático

In this work, we investigated the magnetic properties of a monocrystalline Fe thin film and of Fe(80 Å)/Cr(t)/Fe(80 Å) tri-layers, with the nonmagnetic metallic Cr spacer layer thickness varying between 9 Å < t < 40 Å. The samples were deposited by the DC Sputtering on Magnesium Oxide (MgO) substrates, with (100) crystal orientation. For this investigation, experimental magneto-optical Kerr effect (MOKE) magnetometry and ferromagnetic resonance (FMR) techniques were employeed. In this case, these techniques allowed us to study the static and dynamical magnetization properties of our tri-layers. The experimental results were interpreted based on the phenomenological model that takes into account the relevant energy terms to the magnetic free energy to describe the system behavior. In the case of the monocrystalline Fe film, we performed an analytical discussion on the magnetization curves and developed a numerical simulation based on the Stoner-Wohlfarth model, that enables the numerical adjustment of the experimental magnetization curves and obtainment of the anisotropy field values. On the other hand, for the tri-layers, we analyzed the existence of bilinear and biquadratic couplings between the magnetizations of adjacent ferromagnetic layers from measurements of magnetization curves. With the FMR fields and line width angular dependencies, information on the anisotropy in three layers was obtained and the effects of different magnetic relaxation mechanisms were evidenced. It was also possible to observe the dependence of the epitaxy of the multilayers with growth and sputtering parameters. Additionally it was developed the technique of AC magnetic susceptibility in order to obtain further information during the investigation of magnetic thin films

Efeito nernst anômalo em Materiais com anisotropia magnetocristalina (110)

Conselho Nacional de Desenvolvimento Científico e Tecnológico

ISW effect through dark energy quintessence and ΛCDM models

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Influência da petrografia sobre a anisotropia à tensão de compressão e dilatação térmica de rochas ornamentais

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

Paleoambiente e proveniência da formação cabeças da bacia do Parnaíba: evidências da glaciação famenniana e implicações na potencialidade do reservatório

O histórico de prospecção de hidrocarbonetos da Bacia Paleozoica do Parnaíba, situada no norte-nordeste do Brasil, sempre foi considerado desfavorável quando comparado aos super-reservatórios estimados do Pré-Sal das bacias da Margem Atlântica e até mesmo interiores, como a Bacia do Solimões. No entanto, a descoberta de gás natural em depósitos da superseqüência mesodevoniana-eocarbonífera do Grupo Canindé, que incluem as formações Pimenteiras, Cabeças e Longá, impulsionou novas pesquisas no intuito de refinar a caracterização paleoambiental, paleogeográfica, bem como, entender o sistema petrolífero, os possíveis plays e a potencialidade do reservatório Cabeças. A avaliação faciológica e estratigráfica com ênfase no registro da tectônica glacial, em combinação com a geocronologia de zircão detrítico permitiu interpretar o paleoambiente e a proveniência do reservatório Cabeças. Seis associações de fácies agrupadas em sucessões aflorantes, com espessura máxima de até 60m registram a evolução de um sistema deltaico Devoniano influenciado por processos glaciais principalmente no topo da unidade. 1) frente deltaica distal, composta por argilito maciço, conglomerado maciço, arenito com acamamento maciço, laminação plana e estratificação cruzada sigmoidal 2) frente deltaica proximal, representada pelas fácies arenito maciço, arenito com laminação plana, arenito com estratificação cruzada sigmoidal e conglomerado maciço; 3) planície deltaica, representada pelas fácies argilito laminado, arenito maciço, arenito com estratificação cruzada acanalada e conglomerado maciço; 4) shoreface glacial, composta pelas fácies arenito com marcas onduladas e arenito com estratificação cruzada hummocky; 5) depósitos subglaciais, que englobam as fácies diamictito maciço, diamictito com pods de arenito e brecha intraformacional; e 6) frente deltaica de degelo, constituída pelas fácies arenito maciço, arenito deformado, arenito com laminação plana, arenito com laminação cruzada cavalgante e arenito com estratificação cruzada sigmoidal. Durante o Fammeniano (374-359 Ma) uma frente deltaica dominada por processos fluviais progradava para NW (borda leste) e para NE (borda oeste) sobre uma plataforma influenciada por ondas de tempestade (Formação Pimenteiras). Na borda leste da bacia, o padrão de paleocorrente e o espectro de idades U-Pb em zircão detrítico indicam que o delta Cabeças foi alimentado por áreas fonte situadas a sudeste da Bacia do Parnaíba, provavelmente da Província Borborema. Grãos de zircão com idade mesoproterozóica (~ 1.039 – 1.009 Ma) e neoproterozóica (~ 654 Ma) são os mais populosos ao contrário dos grãos com idade arqueana (~ 2.508 – 2.678 Ma) e paleoproterozóica (~ 2.054 – 1.992 Ma). O grão de zircão concordante mais novo forneceu idade ²⁰⁶Pb/²³⁸U de 501,20 ± 6,35 Ma (95% concordante) indicando idades de áreas-fonte cambrianas. As principais fontes de sedimentos do delta Cabeças na borda leste são produto de rochas do Domínio Zona Transversal e de plútons Brasilianos encontrados no embasamento a sudeste da Bacia do Parnaíba, com pequena contribuição de sedimentos oriundos de rochas do Domínio Ceará Central e da porção ocidental do Domínio Rio Grande do Norte. No Famenniano, a movimentação do supercontinente Gondwana para o polo sul culminou na implantação de condições glaciais concomitantemente com o rebaixamento do nível do mar e exposição da região costeira. O avanço das geleiras sobre o embasamento e depósitos deltaicos gerou erosão, deposição de diamictons com clastos exóticos e facetados, além de estruturas glaciotectônicas tais como plano de descolamento, foliação, boudins, dobras, duplex, falhas e fraturas que refletem um cisalhamento tangencial em regime rúptil-dúctil. O substrato apresentava-se inconsolidado e saturados em água com temperatura levemente abaixo do ponto de fusão do gelo (permafrost quente). Corpos podiformes de arenito imersos em corpos lenticulares de diamicton foram formados pela ruptura de camadas pelo cisalhamento subglacial. Lentes de conglomerados esporádicas (dump structures) nos depósitos de shoreface sugere queda de detritos ligados a icebergs em fases de recuo da geleira. A elevação da temperatura no final do Famenniano reflete a rotação destral do Gondwana e migração do polo sul da porção ocidental da América do Sul e para o oeste da África. Esta nova configuração paleogeográfica posicionou a Bacia do Parnaíba em regiões subtropicais iniciando o recuo de geleiras e a influência do rebound isostático. O alívio de pressão é indicado pela geração de sills e diques clásticos, estruturas ball-and-pillow, rompimento de camadas e brechas. Falhas de cavalgamento associadas à diamictitos com foliação na borda oeste da bacia sugerem que as geleiras migravam para NNE. O contínuo aumento do nível do mar relativo propiciou a instalação de sedimentação deltaica durante o degelo e posteriormente a implantação de uma plataforma transgressiva (Formação Longá). Diamictitos interdigitados com depósitos de frente deltaica na porção superior da Formação Cabeças correspondem a intervalos com baixo volume de poros e podem representar trapas estratigráficas secundárias no reservatório. As anisotropias primárias subglaciais do topo da sucessão Cabeças, em ambas as bordas da Bacia do Parnaíba, estende a influência glacial e abre uma nova perspectiva sobre a potencialidade efetiva do reservatório Cabeças do sistema petrolífero Mesodevoniano-Eocarbonífero da referida bacia.

Efeitos da equação de estado em hidrodinâmica relativística através de alguns observáveis

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Anisotropia magnética em nanofilmes com assimetria cristalográfica

This Thesis comprises a theoretical study about the influence of the magnetocrystalline anisotropy on the static and dynamic magnetic properties of nanofilms: monolayers and trilayers coupled through the bilinear and biquadratic exchange fields, for situations in which the systems are grown in unusual [hkl] asymmetric directions. Using a theory based on a realistic phenomenological model for description of nanometric systems, we consider the total free magnetic energy including the Zeeman interaction, cubic and uniaxial anisotropies, demagnetizing and surface anysotropy energies, as well as the exchange terms. Numerical calculations are conducted by minimizing the total magnetic energy from the determination of equilibrium static configurations. We consider experimental parameters found in the literature to illustrate our results for Fe/Cr/Fe trilayer systems. In particular, a total of six different magnetic scenarios are analyzed for three regimens of exchange fields and the [211] and [321] asymmetric growth directions. After numerically minimize the total energy, we use the equilibrium configurations to calculate magnetization and magnetoresistance curves with the respective magnetic phases and corresponding critical fields. These results are also used to establish the boundary for occurrence of saturated states. Within the context of the spin waves, we solve the equation of motion for these systems in order to find the respective associated dispersion relations. The results show similar magnetization and magnetoresistance curves for both [211] and [321] growth scenarios, including an equivalent magnetic transition behavior. However, the combination of those peculiar symmetries and influence of the exchange energies results in attractive properties, including the generation of magnetic states as a function of the asymmetric degree imposed in the [hkl] growth orientations. There is also an increasing incompatibility between the values of saturation fields of magnetization and magnetoresistance for the cases in which a magnetic field acts along intermediate cubic anisotropic axes, particularly in the situations where the bilinear and biquadratic exchange fields are comparable. The dispersion relations and static results are consistent, the corresponding magnetic states are also present in both acoustic and optical modes. Furthermore, Goldstone excitations are also observed for that particular cases of a magnetic field acting in the intermediate axes, an effect related to transitions of second order and to the spontaneous symmetry breaking imposed by the combination of the biquadratic energy with the cubic and uniaxial anisotropies.