25,598 research outputs found

    Inertial-Hall effect: the influence of rotation on the Hall conductivity

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    Inertial effects play an important role in classical mechanics but have been largely overlooked in quantum mechanics. Nevertheless, the analogy between inertial forces on mass particles and electromagnetic forces on charged particles is not new. In this paper, we consider a rotating non-interacting planar two-dimensional electron gas with a perpendicular uniform magnetic field and investigate the effects of the rotation in the Hall conductiv

    A Bayesian estimate of the CMB-large-scale structure cross-correlation

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    Evidences for late-time acceleration of the Universe are provided by multiple probes, such as Type Ia supernovae, the cosmic microwave background (CMB) and large-scale structure (LSS). In this work, we focus on the integrated Sachs--Wolfe (ISW) effect, i.e., secondary CMB fluctuations generated by evolving gravitational potentials due to the transition between, e.g., the matter and dark energy (DE) dominated phases. Therefore, assuming a flat universe, DE properties can be inferred from ISW detections. We present a Bayesian approach to compute the CMB--LSS cross-correlation signal. The method is based on the estimate of the likelihood for measuring a combined set consisting of a CMB temperature and a galaxy contrast maps, provided that we have some information on the statistical properties of the fluctuations affecting these maps. The likelihood is estimated by a sampling algorithm, therefore avoiding the computationally demanding techniques of direct evaluation in either pixel or harmonic space. As local tracers of the matter distribution at large scales, we used the Two Micron All Sky Survey (2MASS) galaxy catalog and, for the CMB temperature fluctuations, the ninth-year data release of the Wilkinson Microwave Anisotropy Probe (WMAP9). The results show a dominance of cosmic variance over the weak recovered signal, due mainly to the shallowness of the catalog used, with systematics associated with the sampling algorithm playing a secondary role as sources of uncertainty. When combined with other complementary probes, the method presented in this paper is expected to be a useful tool to late-time acceleration studies in cosmology.Comment: 21 pages, 15 figures, 4 tables. We extended the previous analyses including WMAP9 Q, V and W channels, besides the ILC map. Updated to match accepted ApJ versio

    Parameterized Complexity of Equitable Coloring

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    A graph on nn vertices is equitably kk-colorable if it is kk-colorable and every color is used either n/k\left\lfloor n/k \right\rfloor or n/k\left\lceil n/k \right\rceil times. Such a problem appears to be considerably harder than vertex coloring, being NP-Complete\mathsf{NP\text{-}Complete} even for cographs and interval graphs. In this work, we prove that it is W[1]-Hard\mathsf{W[1]\text{-}Hard} for block graphs and for disjoint union of split graphs when parameterized by the number of colors; and W[1]-Hard\mathsf{W[1]\text{-}Hard} for K1,4K_{1,4}-free interval graphs when parameterized by treewidth, number of colors and maximum degree, generalizing a result by Fellows et al. (2014) through a much simpler reduction. Using a previous result due to Dominique de Werra (1985), we establish a dichotomy for the complexity of equitable coloring of chordal graphs based on the size of the largest induced star. Finally, we show that \textsc{equitable coloring} is FPT\mathsf{FPT} when parameterized by the treewidth of the complement graph

    Comparação dos métodos sorológico e biológico na detecção de Potato virus Y (PVY).

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    Visando comparar a sensibilidade do método sorológico DAS-ELISA (Double antibody sandwich/Enzyme-linked immunosorbent assay) com o m´todo biológico (inoculação em espécies indicadoras) na detecção do PVY, analisaram-se 47 amostras de plantas de batata, coletadas aleatoriamente, em áreas produtoras do Município de Cristalina, GO e no Gama-DF.Resumo expandido

    An accurate formula for the period of a simple pendulum oscillating beyond the small-angle regime

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    A simple approximation formula is derived here for the dependence of the period of a simple pendulum on amplitude that only requires a pocket calculator and furnishes an error of less than 0.25% with respect to the exact period. It is shown that this formula describes the increase of the pendulum period with amplitude better than other simple formulas found in literature. A good agreement with experimental data for a low air-resistance pendulum is also verified and it suggests, together with the current availability/precision of timers and detectors, that the proposed formula is useful for extending the pendulum experiment beyond the usual small-angle oscillations.Comment: 15 pages and 4 figures. to appear in American Journal of Physic

    Avaliação de híbridos completos de mangueira da variedade Tommy Atkins, em um ciclo, no Semiárido brasileiro.

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    O objetivo do presente trabalho consiste, portanto, na avaliação de híbridos completos da tradicional variedade Tommy Atkins ou, ocasionalmente, de progênies resultantes de eventuais autofecundações, em uma safra (2013-2014), no Semiárido Brasileiro, considerando-se parâmetros físicos e químicos associados aos fruto
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