Monitoramento da Entomofauna Epígea em pomar orgânico em processo inicial de transição agroecológica.

O estudo das relações entre diversidade e funcionamento do agroecossitema é importante no solo, por ser constituído de habitats diversos podendo-se prever mudanças no seu funcionamento em decorrência de alterações na sua diversidade (TILMAN, 1996). Nesse sentido, a utilização de insetos como bioindicadores de mudanças no ambiente pode fornecer informações úteis para o manejo e recuperação de ecossistemas degradados (ROSEMBERG et al., 1986, PARR; CHOWN, 2001)

Análise faunística da entomofauna de serrapilheira de mata primária como referência de qualidade edáfica.

Perturbações antrópicas na agricultura têm causado impactos negativos no ambiente e na qualidade do solo devido ao uso intensivo. A utilização de indicadores físicos, químicos e biológicos, que refletem a condição de sustentabilidade do ecossistema e da qualidade edáfica, tem sido proposta para mensurar a qualidade ambiental

Entomofauna do solo de Mata primária Atlântica como padrão indicador de qualidade dos agroecossistemas.

O manejo intensivo do solo tem ocasionado perda de matéria orgânica, erosão e contaminação das águas subterrâneas por meio da aplicação de herbicidas e inseticidas, além de prejuízos à microbiota e aos processos bioquímicos com efeitos evidentes na qualidade do agroecossistema.bitstream/item/59295/1/documentos-204.pd

Experimental and theoretical evidences for the ice regime in planar artificial spin ices

In this work, we explore a kind of geometrical effect in the thermodynamics of artificial spin ices (ASI). In general, such artificial materials are athermal. Here, We demonstrate that geometrically driven dynamics in ASI can open up the panorama of exploring distinct ground states and thermally magnetic monopole excitations. It is shown that a particular ASI lattice will provide a richer thermodynamics with nanomagnet spins experiencing less restriction to flip precisely in a kind of rhombic lattice. This can be observed by analysis of only three types of rectangular artificial spin ices (RASI). Denoting the horizontal and vertical lattice spacings by a and b, respectively, then, a RASI material can be described by its aspect ratio $\gamma$=a/b. The rhombic lattice emerges when $\gamma$=$\sqrt{3}$. So, by comparing the impact of thermal effects on the spin flips in these three appropriate different RASI arrays, it is possible to find a system very close to the ice regime

Informações técnicas sobre o cultivo do algodoeiro na agricultura familiar de Goiás.

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Synchronization time in a hyperbolic dynamical system with long-range interactions

We show that the threshold of complete synchronization in a lattice of coupled non-smooth chaotic maps is determined by linear stability along the directions transversal to the synchronization subspace. We examine carefully the sychronization time and show that a inadequate observation of the system evolution leads to wrong results. We present both careful numerical experiments and a rigorous mathematical explanation confirming this fact, allowing for a generalization involving hyperbolic coupled map lattices.Comment: 22 pages (preprint format), 4 figures - accepted for publication in Physica A (June 28, 2010

Chemical Potential and the Nature of the Dark Energy: The case of phantom

The influence of a possible non zero chemical potential $\mu$ on the nature of dark energy is investigated by assuming that the dark energy is a relativistic perfect simple fluid obeying the equation of state (EoS), $p=\omega \rho$ ($\omega <0, constant$). The entropy condition, $S \geq 0$, implies that the possible values of $\omega$ are heavily dependent on the magnitude, as well as on the sign of the chemical potential. For $\mu >0$, the $\omega$-parameter must be greater than -1 (vacuum is forbidden) while for $\mu < 0$ not only the vacuum but even a phantomlike behavior ($\omega <-1$) is allowed. In any case, the ratio between the chemical potential and temperature remains constant, that is, $\mu/T=\mu_0/T_0$. Assuming that the dark energy constituents have either a bosonic or fermionic nature, the general form of the spectrum is also proposed. For bosons $\mu$ is always negative and the extended Wien's law allows only a dark component with $\omega < -1/2$ which includes vacuum and the phantomlike cases. The same happens in the fermionic branch for $\mu 0$ are permmited only if $-1 < \omega < -1/2$. The thermodynamics and statistical arguments constrain the EoS parameter to be $\omega < -1/2$, a result surprisingly close to the maximal value required to accelerate a FRW type universe dominated by matter and dark energy ($\omega \lesssim -10/21$).Comment: 7 pages, 5 figure