11,537 research outputs found

    Drastic annealing effects in transport properties of single crystals of the YbNi2B2C heavy fermion system

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    We report temperature dependent resistivity, specific heat, magnetic susceptibility and thermoelectric power measurements made on the heavy fermion system YbNi2B2C, for both as grown and annealed single crystals. Our results demonstrate a significant variation in the temperature dependent electrical resistivity and thermoelectric power between as grown crystals and crystals that have undergone optimal (150 hour, 950 C) annealing, whereas the thermodynamic properties: (c_p(T) and chi(T)) remain almost unchanged. We interpret these results in terms of redistributions of local Kondo temperatures associated with ligandal disorder for a small (~ 1%) fraction of the Yb sites.Comment: 5 pages, 4 figures, submitted to PR

    Direct observation of Fe spin reorientation in single crystalline YbFe6Ge6

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    We have grown single crystals of YbFe6Ge6 and LuFe6Ge6 and characterized their anisotropic behaviour through low field magnetic susceptibility, field-dependent magnetization, resistivity and heat capacity measurements. The Yb+3 valency is confirmed by LIII XANES measurements. YbFe6Ge6 crystals exhibit a field-dependent, sudden reorientation of the Fe spins at about 63 K, a unique effect in the RFe6Ge6 family (R = rare earths) where the Fe ions order anti-ferromagnetically with Neel temperatures above 450 K and the R ions' magnetism appears to behave independently. The possible origins of this unusual behaviour of the ordered Fe moments in this compound are discussed.Comment: 12 pages, 8 figures, accepted in J. Phys.: Cond. Matte

    A New Shear Estimator for Weak Lensing Observations

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    We present a new shear estimator for weak lensing observations which properly accounts for the effects of a realistic point spread function (PSF). Images of faint galaxies are subject to gravitational shearing followed by smearing with the instrumental and/or atmospheric PSF. We construct a `finite resolution shear operator' which when applied to an observed image has the same effect as a gravitational shear applied prior to smearing. This operator allows one to calibrate essentially any shear estimator. We then specialize to the case of weighted second moment shear estimators. We compute the shear polarizability which gives the response of an individual galaxy's polarization to a gravitational shear. We then compute the response of the population of galaxies, and thereby construct an optimal weighting scheme for combining shear estimates from galaxies of various shapes, luminosities and sizes. We define a figure of merit --- an inverse shear variance per unit solid angle --- which characterizes the quality of image data for shear measurement. The new method is tested with simulated image data. We discuss the correction for anisotropy of the PSF and propose a new technique involving measuring shapes from images which have been convolved with a re-circularizing PSF. We draw attention to a hitherto ignored noise related bias and show how this can be analyzed and corrected for. The analysis here draws heavily on the properties of real PSF's and we include as an appendix a brief review, highlighting those aspects which are relevant for weak lensing.Comment: 39 pages, 9 figure

    Collapse of the Gd3+Gd^{3+} ESR fine structure throughout the coherent temperature of the Gd-doped Kondo Semiconductor CeFe4P12CeFe_{4}P_{12}

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    Experiments on the Gd3+Gd^{3+} Electron Spin Resonance (ESR) in the filled skutterudite Ce1xGdxFe4P12Ce_{1-x}Gd_{x}Fe_{4}P_{12} (x0.001x \approx 0.001), at temperatures where the host resistivity manifests a smooth insulator-metal crossover, provides evidence of the underlying Kondo physics associated with this system. At low temperatures (below TKT \approx K), Ce1xGdxFe4P12Ce_{1-x}Gd_{x}Fe_{4}P_{12} behaves as a Kondo-insulator with a relatively large hybridization gap, and the Gd3+Gd^{3+} ESR spectra displays a fine structure with lorentzian line shape, typical of insulating media. The electronic gap is attributed to the large hybridization present in the coherent regime of a Kondo lattice, when Ce 4f-electrons cooperate with band properties at half-filling. Mean-field calculations suggest that the electron-phonon interaction is fundamental at explaining the strong 4f-electron hybridization in this filled skutterudite. The resulting electronic structure is strongly temperature dependent, and at about T160KT^{*} \approx 160 K the system undergoes an insulator-to-metal transition induced by the withdrawal of 4f-electrons from the Fermi volume, the system becoming metallic and non-magnetic. The Gd3+Gd^{3+} ESR fine structure coalesces into a single dysonian resonance, as in metals. Still, our simulations suggest that exchange-narrowing via the usual Korringa mechanism, alone, is not capable of describing the thermal behavior of the ESR spectra in the entire temperature region (4.24.2 - 300300 K). We propose that temperature activated fluctuating-valence of the Ce ions is the missing ingredient that, added to the usual exchange-narrowing mechanism, fully describes this unique temperature dependence of the Gd3+Gd^{3+} ESR fine structure observed in Ce1xGdxFe4P12Ce_{1-x}Gd_{x}Fe_{4}P_{12}.Comment: 19 pages, 6 figure

    Turbulent dissipation in the ISM: the coexistence of forced and decaying regimes and implications for galaxy formation and evolution

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    We discuss the dissipation of turbulent kinetic energy Ek in the global ISM by means of 2-D, MHD, non-isothermal simulations in the presence of model radiative heating and cooling. We argue that dissipation in 2D is representative of that in three dimensions as long as it is dominated by shocks rather than by a turbulent cascade. Energy is injected at a few isolated sites in space, over relatively small scales, and over short time periods. This leads to the coexistence of forced and decaying regimes in the same flow. We find that the ISM-like flow dissipates its turbulent energy rapidly. In simulations with forcing, the input parameters are the radius l_f of the forcing region, the total kinetic energy e_k each source deposits into the flow, and the rate of formation of those regions, sfr_OB. The global dissipation time t_d depends mainly on l_f. In terms of measurable properties of the ISM, t_d >= Sigma_g u_rms^2/(e_k sfr_OB), where Sigma_g is the average gas surface density and u_rms is the rms velocity dispersion. For the solar neighborhood, t_d >= 1.5x10^7 yr. The global dissipation time is consistently smaller than the crossing time of the largest energy-containing scales. In decaying simulations, Ek decreases with time as t^-n, where n~0.8-0.9. This suggests a decay with distance d as Ek\propto d^{-2n/(2-n)} in the mixed forced+decaying case. If applicable to the vertical direction, our results support models of galaxy evolution in which stellar energy injection provides significant support for the gas disk thickness, but not models of galaxy formation in which this energy injection is supposed to reheat an intra-halo medium at distances of up to 10-20 times the optical galaxy size, as the dissipation occurs on distances comparable to the disk height.Comment: 23 pages, including figures. To appear in ApJ. Abstract abridge

    Avaliação da resistência à penetração em diferentes sistemas em lote de reforma agrária no município de Itapeva, SP.

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    O sistema vivo, complexo e dinâmico do solo tem sido, no ultimo século, considerado apenas um suporte inerte para a obtenção de lucro pela agricultura convencional e os passivos de degradação de sua estrutura física, química e biológica já são entraves à melhoria de qualidade de vida dos agricultores, dentro da realidade de escassez de recursos e assistência técnica dos assentamentos rurais do estado de São Paulo (PRIMAVESI, 2002; GLIESSMAN, 2009). Um dos legados do manejo inadequado com maquinaria pesada e cultivo intensivo, deixado nos solos da maioria das áreas destinadas à assentamentos rurais, é a compactação ou o chamado "pé-de-grande" (RAMOS FILHO e PELLEGRINI, 2006). A destruição da bioestrutura do solo compromete a estabilidade, resistência às intempéries, fornecimento de água e oxigênio para os cultivos e, portanto, constitui-se na principal causa dos problemas de produtividade na agricultura tropical (PRIMAVESI, 2002). Dentro deste contexto têm surgido nos últimos anos diversas iniciativas de alternativas de manejo agroecológico do solo na forma de sistemas agroflorestais (SAFs). Pelo fato de aliar no mesmo espaço e/ou tempo o cultivo de grande diversidade de espécies agrícolas anuais, florestais perenes, herbáceas, arbustivas e arbóreas, os SAFs imitam e se fundamentam na estrutura multiestratificada complexa e na dinâmica dos processos ecológicos de ecossistemas florestais naturais (PENEIREIRO et al., 2002). A camada de estratos acima do solo e a "capa" de folhas o protege dos impactos do sol, chuva e vento, evitando a destruição de sua estrutura, a sua erosão e compactação. A incorporação frequente de matéria orgânica reconstrói o solo e a camada ampla e complexa de raízes abaixo da superfície promove a descompactação, aeração e aumento da infiltração de água. Experiências de SAF com objetivo de aliar conservação do solo com produção agrícola vêm sendo construídas no assentamento Pirituba II, localizado no município de Itapeva, SP, cujo histórico anterior é de produção convencional de grãos com uso intensivo de maquinaria pesada em extensas áreas de monocultivo. O presente estudo foi realizado no lote dos agricultores João Pereira da Silva e Eva Conceição da Silva que tem trabalhado com agrofloresta desde 2006. Dentro deste contexto, o monitoramento do sistema por indicadores de sustentabilidade se constitui em uma ferramenta essencial de qualificação da experiência e de base para melhorias de práticas de manejo, indicando modificações em atributos-chave na dinâmica do agroecossistema (DEPONTI et al., 2002). Neste sentido o objetivo principal deste trabalho foi analisar os efeitos do uso e manejo agroecológico do solo na forma de SAF, através de medições com equipamento de medição de compactação, o penetrômetro
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