958 resultados para FERROMAGNETIC SPIN CHAINS
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Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)
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Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)
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Pós-graduação em Física - FEG
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Pós-graduação em Química - IQ
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Motivados por estudos experimentais acerca de monocamadas de metais de transição 3d sobre superfícies de Pd, nesta dissertação investigamos o complexo magnetismo de nanoestruturas, embebidas ou adsorvidas, em superfícies metálicas através de cálculos de primeiros princípios. Utilizamos o método RS-LMTO-ASA (Real Space - Linear MuffinTin Orbital - Atomic Sphere Approximation), o qual é baseado na teoria do funcional da densidade (DFT - Density Functional Theory) e implementado para o cálculo de estruturas magnéticas não colineares. Com este propósito, investigamos nanoestruturas embebidas e ligas (2 x 2) de metais 3d (Cr, Mn, Fe, Co e Ni) na superfície Pd (110), além de nanoestruturas de Cr adsorvidas sobre a superfície de Pd (111). Primeiro, para as nanoestruturas embebidas na superfície Pd (110), analisamos a variação do momento magnético de spin orbital com relação ao número de vizinhos e de valência dos metais 3d. Também mostramos que estas estruturas têm ordenamento magnético colinear, exceto as de Cr e Mn, que apresentam magnetismo não colinear associado à frustração geométrica. Para o caso de nanofios de Cr adsorvidos sobre a superfície de Pd (111), verificamos uma configuração colinear antiferromagnética para cadeias com até 9 átomos. Para o nanofio com 10 átomos obtivemos uma configuração tipo antiferromagnética inclinada (canted). No caso de nanoestruturas de Cr bidimensionais, verificamos complexas configurações magnéticas não colineares com diferentes quiralidades.
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Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
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Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
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The aim of this paper is to present an analytical solution for the spin motion equations of spin-stabilized satellite considering only the influence of solar radiation torque. The theory uses a cylindrical satellite on a circular orbit and considers that the satellite is always illuminated. The average components of this torque were determined over an orbital period. These components are substituted in the spin motion equations in order to get an analytical solution for the right ascension and declination of the satellite spin axis. The time evolution for the pointing deviation of the spin axis was also analyzed. These solutions were numerically implemented and compared with real data of the Brazilian Satellite of Data Collection - SCD1 an SCD2. The results show that the theory has consistency and can be applied to predict the spin motion of spin-stabilized artificial satellites.
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The spin injector part of spintronic FET and diodes suffers from fatigue due to rising heat on the depletion layer. In this study the stiffness of Ga1-xMnxAs spin injector in terms of storage modulus with respect to a varying temperature, 45 degrees C <= T <= 70 degrees C was determined. It was observed that the storage modulus for MDLs (Manganese Doping Levels) of 0%, 1% and 10% decreased with increase in temperature while that with MDLs of 20% and 50% increase with increase in temperature. MDLs of 20% and 50% appear not to allow for damping but MDLs <= 20% allow damping at temperature range of 45 degrees C <= T <= 70 degrees C. The magnitude of storage moduli of GaAs is smaller than that for ferromagnetic Ga1-xMnxAs systems. The loss moduli for GaAs were found to reduce with increase in temperature. Its magnitude of reducing gradient is smaller than Ga1-xMnxAs systems. The two temperature extremes show a general reduction in loss moduli for different MDLs at the study temperature range. From damping factor analysis, damping factors for ferromagnetic Ga1-xMnxAs was found to increase with decrease in MDLs contrary to GaAs which recorded the largest damping factor at 45 degrees C <= T <= 70 degrees C Hence, MDL of 20% shows little damping followed by 50% while MDL of 0% has the most damping in an increasing trend with temperature. (C) 2013 Elsevier Ltd. All rights reserved.
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Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
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Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
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We discuss the relation between correlation functions of twist-two large spin operators and expectation values of Wilson loops along light-like trajectories. After presenting some heuristic field theoretical arguments suggesting this relation, we compute the divergent part of the correlator in the limit of large 't Hooft coupling and large spins, using a semi-classical world-sheet which asymptotically looks like a GKP rotating string. We show this diverges as expected from the expectation value of a null Wilson loop, namely, as (ln mu(-2))(2). mu being a cut-off of the theory. (C) 2012 Elsevier B.V. All rights reserved.
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Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
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Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)
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Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)