6,137 research outputs found

    Ocorrência e controle da lesma Omalonyx sp. (Gastropoda: Succineidae), praga de capim-elefante (Pennisetum purpureum) em Manaus, Amazonas.

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    Neste trabalho descreveu-se a ocorrência atípica de Omalonyx sp. como praga em capim-elefante (Pennisetum purpureum), em habitat de terra firme, em Manaus-AM e sugere-se uma alternativa para o seu controle

    Effects of Velocity Correlation on Early Stage of Free Cooling Process of Inelastic Hard Sphere System

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    The free cooling process in the inelastic hard sphere system is studied by analysing the data from large scale molecular dynamics simulations on a three dimensional system. The initial energy decay, the velocity distribution function, and the velocity correlation functions are calculated to be compared with theoretical predictions. The energy decay rate in the homogeneous cooling state is slightly but distinctively smaller than that expected from the independent collision assumption. The form of the one particle velocity distribution is found not to be stationary. These contradict to the predictions of the kinetic theory based on the Enskog-Boltzmann equation and suggest that the velocity correlation is already important in the early stage of homogeneous cooling state. The energy decay rate is analysed in terms of the velocity correlation.Comment: 9 pages (figures included). To be published in J. Phys. Soc. Jpn. Vol. 73 No. 1 (2004) Added two references and removed one. Changed the name of T_{L}. Added unit constants in Sec. 5 and

    Morphological transition between diffusion-limited and ballistic aggregation growth patterns

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    In this work, the transition between diffusion-limited and ballistic aggregation models was revisited using a model in which biased random walks simulate the particle trajectories. The bias is controlled by a parameter λ\lambda, which assumes the value λ=0\lambda=0 (1) for ballistic (diffusion-limited) aggregation model. Patterns growing from a single seed were considered. In order to simulate large clusters, a new efficient algorithm was developed. For λ0\lambda \ne 0, the patterns are fractal on the small length scales, but homogeneous on the large ones. We evaluated the mean density of particles ρˉ\bar{\rho} in the region defined by a circle of radius rr centered at the initial seed. As a function of rr, ρˉ\bar{\rho} reaches the asymptotic value ρ0(λ)\rho_0(\lambda) following a power law ρˉ=ρ0+Arγ\bar{\rho}=\rho_0+Ar^{-\gamma} with a universal exponent γ=0.46(2)\gamma=0.46(2), independent of λ\lambda. The asymptotic value has the behavior ρ01λβ\rho_0\sim|1-\lambda|^\beta, where β=0.26(1)\beta= 0.26(1). The characteristic crossover length that determines the transition from DLA- to BA-like scaling regimes is given by ξ1λν\xi\sim|1-\lambda|^{-\nu}, where ν=0.61(1)\nu=0.61(1), while the cluster mass at the crossover follows a power law Mξ1λαM_\xi\sim|1 -\lambda|^{-\alpha}, where α=0.97(2)\alpha=0.97(2). We deduce the scaling relations \beta=\n u\gamma and β=2να\beta=2\nu-\alpha between these exponents.Comment: 7 pages, 8 figure

    Radiocarbon and blue optically stimulated luminescence chronologies of the Oitavos consolidated dune (Western Portugal)

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    The dune of Oitavos, the underlying paleosol, and Helix sp. gastropod shells found within the paleosol were dated using a combination of radiocarbon and blue optically stimulated luminescence (OSL). The organic component of the paleosol produced a significantly older age (~20,000 cal BP) than the OSL age measurement (~15,000 yr), while 14C age measurements on the inorganic component and the gastropods produced ages of ~35,000 yr and ~34,000 yr, respectively. Rare-earth element analyses provide evidence that the gastropods incorporate geological carbonate, making them an unreliable indicator of the age of the paleosol. We propose that the 14C age of the small organic component of the paleosol is also likely to be unreliable due to incorporation of residual material. The OSL age measurement of the upper paleosol (~15,000 yr) is consistent with the age for the base of the dune (~14,500 yr). The younger OSL age for the top of the dune (~12,000 yr) suggests that it was built up by at least 2 sand pulses or that there was a remobilization of material at the top during its evolution, prior to consolidation

    The Solar Twin Planet Search II. A Jupiter twin around a solar twin

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    Through our HARPS radial velocity survey for planets around solar twin stars, we have identified a promising Jupiter twin candidate around the star HIP11915. We characterize this Keplerian signal and investigate its potential origins in stellar activity. Our analysis indicates that HIP11915 hosts a Jupiter-mass planet with a 3800-day orbital period and low eccentricity. Although we cannot definitively rule out an activity cycle interpretation, we find that a planet interpretation is more likely based on a joint analysis of RV and activity index data. The challenges of long-period radial velocity signals addressed in this paper are critical for the ongoing discovery of Jupiter-like exoplanets. If planetary in nature, the signal investigated here represents a very close analog to the solar system in terms of both Sun-like host star and Jupiter-like planet.Comment: 8 pages, 5 figures; A&A accepted; typos corrected in this versio

    Heterogeneous Dynamics, Marginal Stability and Soft Modes in Hard Sphere Glasses

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    In a recent publication we established an analogy between the free energy of a hard sphere system and the energy of an elastic network [1]. This result enables one to study the free energy landscape of hard spheres, in particular to define normal modes. In this Letter we use these tools to analyze the activated transitions between meta-bassins, both in the aging regime deep in the glass phase and near the glass transition. We observe numerically that structural relaxation occurs mostly along a very small number of nearly-unstable extended modes. This number decays for denser packing and is significantly lowered as the system undergoes the glass transition. This observation supports that structural relaxation and marginal modes share common properties. In particular theoretical results [2, 3] show that these modes extend at least on some length scale l(ϕcϕ)1/2l^*\sim (\phi_c-\phi)^{-1/2} where ϕc\phi_c corresponds to the maximum packing fraction, i.e. the jamming transition. This prediction is consistent with very recent numerical observations of sheared systems near the jamming threshold [4], where a similar exponent is found, and with the commonly observed growth of the rearranging regions with compression near the glass transition.Comment: 6 pages, improved versio

    Granular cooling of hard needles

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    We have developed a kinetic theory of hard needles undergoing binary collisions with loss of energy due to normal and tangential restitution. In addition, we have simulated many particle systems of granular hard needles. The theory, based on the assumption of a homogeneous cooling state, predicts that granular cooling of the needles proceeds in two stages: An exponential decay of the initial configuration to a state where translational and rotational energies take on a time independent ratio (not necessarily unity), followed by an algebraic decay of the total kinetic energy t2\sim t^{-2}. The simulations support the theory very well for low and moderate densities. For higher densities, we have observed the onset of the formation of clusters and shear bands.Comment: 7 pages, 8 figures; major changes, extended versio

    Irrigação de salvação em culturas de subsistência.

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    Descrição da tecnologia; Área de captação; Tanque de armazenamento; Área de Plantio; Estudo de caso; Manejo de água de irrigação de salvação

    Patterns and Long Range Correlations in Idealized Granular Flows

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    An initially homogeneous freely evolving fluid of inelastic hard spheres develops inhomogeneities in the flow field (vortices) and in the density field (clusters), driven by unstable fluctuations. Their spatial correlations, as measured in molecular dynamics simulations, exhibit long range correlations; the mean vortex diameter grows as the square root of time; there occur transitions to macroscopic shearing states, etc. The Cahn--Hilliard theory of spinodal decomposition offers a qualitative understanding and quantitative estimates of the observed phenomena. When intrinsic length scales are of the order of the system size, effects of physical boundaries and periodic boundaries (finite size effects in simulations) are important.Comment: 13 pages with 7 postscript figures, LaTeX (uses psfig). Submitted to International Journal of Modern Physics
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