4,754 research outputs found

    Magnetite and its transformation to hematite in a soil derived from steatite.

    Get PDF
    O presente trabalho objetivou caracterizar o mineral magnetico e identificar suas rotas pedogeneticas de transformacao em um solo formado sobre esteatito, de Minas Gerais, Brasil. O oxido de ferro isoestrutural ao espinelio foi identificado e caracterizado por analises quimicas, difracao de raios X, espectroscopia Mossbauer e medidas de magnetizacao de saturacao. Na rocha fresca, foi encontrada magnetita estequiometrica e bem cristalizada, com parametro da rede cubica, ao = 0.8407(5) nm. Nas fracoes areia e silte, foram detectadas magnetita parcialmente alterada e hematita estequiometrica e bem cristalizada, com parametros de rede hexagonal, a = 0.5036(3) nm e c = 1.375(4)nm. A ocorrencia dessas hematitas deveu-se principalmente a oxidacao do Fe2+ a Fe3+, no sitio octaedrico de magnetita, durante a pedogenese. Esse processo foi caracterizado pelo aparecimento de pequena quantidade de Fe3+ eletronicamente desacoplada, encontrada nas magnetitas parcialmente oxidadas, cujas formulas para as diferentes estequiometrias foram propostas. Verificou-se tambem pequena quantidade de ilmenita nas amostras de rocha e de solo

    Confinement in the 3-dimensional Gross-Neveu model

    Full text link
    We consider the NN-components 3-dimensional massive Gross-Neveu model compactified in one spatial direction, the system being constrained to a slab of thickness LL. We derive a closed formula for the effective renormalized LL-dependent coupling constant in the large-N limit, using bag-model boundary conditions. For values of the fixed coupling constant in absence of boundaries λλc19.16\lambda \geq \lambda_c \simeq 19.16, we obtain ultra-violet asymptotic freedom (for L0L \to 0) and confinement for a length L(c)L^{(c)} such that 2.07m1<L(c)2.82m12.07 m^{-1} < L^{(c)} \lesssim 2.82 m^{-1}, mm being the fermionic mass. Taking for mm an average of the masses of the quarks composing the proton, we obtain a confining legth Lp(c)L^{(c)}_p which is comparable with an estimated proton diameter.Comment: Latex, 4 pages, 2 figures (one new), some changes in tex

    Structure and Dynamics of the Globular Cluster Palomar 13

    Get PDF
    We present Keck/DEIMOS spectroscopy and Canada-France-Hawaii Telescope/MegaCam photometry for the Milky Way globular cluster Palomar 13. We triple the number of spectroscopically confirmed members, including many repeat velocity measurements. Palomar 13 is the only known globular cluster with possible evidence for dark matter, based on a Keck/High Resolution Echelle Spectrometer 21 star velocity dispersion of σ = 2.2 ± 0.4 km s^(–1). We reproduce this measurement, but demonstrate that it is inflated by unresolved binary stars. For our sample of 61 stars, the velocity dispersion is σ = 0.7^(+0.6)_(–0.5) km s^(–1). Combining our DEIMOS data with literature values, our final velocity dispersion is σ = 0.4^(+0.4)_( –0.3) km s^(–1). We determine a spectroscopic metallicity of [Fe/H] = –1.6 ± 0.1 dex, placing a 1σ upper limit of σ_([Fe/H]) ~ 0.2 dex on any internal metallicity spread. We determine Palomar 13's total luminosity to be M_V = –2.8 ± 0.4, making it among the least luminous known globular clusters. The photometric isophotes are regular out to the half-light radius and mildly irregular outside this radius. The outer surface brightness profile slope is shallower than typical globular clusters (Σ α r^η, η = –2.8 ± 0.3). Thus at large radius, tidal debris is likely affecting the appearance of Palomar 13. Combining our luminosity with the intrinsic velocity dispersion, we find a dynamical mass of M_(1/2) = 1.3^(+2:7)_(–1.3) × 10^3 M_☉ and a mass-to-light ratio of M/L_V = 2.4^(+5.0)_(–2.4) M_☉/L_☉. Within our measurement errors, the mass-to-light ratio agrees with the theoretical predictions for a single stellar population. We conclude that, while there is some evidence for tidal stripping at large radius, the dynamical mass of Palomar 13 is consistent with its stellar mass and neither significant dark matter, nor extreme tidal heating, is required to explain the cluster dynamics

    Nematóides como indicadores biológicos de sustentabilidade: oportunidades em projetos.

    Get PDF
    xEdição dos Resumos do XXXIX Congresso Brasileiro de Fitopatologia, SALVADOR, BA, ago. 2006

    Atualização da rede hidrográfica do Estado do Mato Grosso do Sul.

    Get PDF
    Este trabalho, quando finalizado, dará apoio ao Sistema Interativo de Suporte ao Licenciamento Ambiental (SISLA) para a execução de atividades relacionadas à fiscalização das áreas de preservação permanente e em atividades de licenciamento ambiental no estado do Mato Grosso do Sul
    corecore