22,035 research outputs found

    On the relation between mass of pion, fundamental physical constants and cosmological parameters

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    In this article we reconsider the old mysterious relation, advocated by Dirac and Weinberg, between the mass of the pion, the fundamental physical constants, and the Hubble parameter. By introducing the cosmological density parameters, we show how the corresponding equation may be written in a form that is invariant with respect to the expansion of the Universe and without invoking a varying gravitational "constant", as was originaly proposed by Dirac. It is suggest that, through this relation, Nature gives a hint that virtual pions dominante the "content" of the quantum vacuum

    Aggregation in a mixture of Brownian and ballistic wandering particles

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    In this paper, we analyze the scaling properties of a model that has as limiting cases the diffusion-limited aggregation (DLA) and the ballistic aggregation (BA) models. This model allows us to control the radial and angular scaling of the patterns, as well as, their gap distributions. The particles added to the cluster can follow either ballistic trajectories, with probability PbaP_{ba}, or random ones, with probability Prw=1PbaP_{rw}=1-P_{ba}. The patterns were characterized through several quantities, including those related to the radial and angular scaling. The fractal dimension as a function of PbaP_{ba} continuously increases from df1.72d_f\approx 1.72 (DLA dimensionality) for Pba=0P_{ba}=0 to df2d_f\approx 2 (BA dimensionality) for Pba=1P_{ba}=1. However, the lacunarity and the active zone width exhibt a distinct behavior: they are convex functions of PbaP_{ba} with a maximum at Pba1/2P_{ba}\approx1/2. Through the analysis of the angular correlation function, we found that the difference between the radial and angular exponents decreases continuously with increasing PbaP_{ba} and rapidly vanishes for Pba>1/2P_{ba}>1/2, in agreement with recent results concerning the asymptotic scaling of DLA clusters.Comment: 7 pages, 6 figures. accepted for publication on PR

    Cosmological constant constraints from observation-derived energy condition bounds and their application to bimetric massive gravity

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    Among the various possibilities to probe the theory behind the recent accelerated expansion of the universe, the energy conditions (ECs) are of particular interest, since it is possible to confront and constrain the many models, including different theories of gravity, with observational data. In this context, we use the ECs to probe any alternative theory whose extra term acts as a cosmological constant. For this purpose, we apply a model-independent approach to reconstruct the recent expansion of the universe. Using Type Ia supernova, baryon acoustic oscillations and cosmic-chronometer data, we perform a Markov Chain Monte Carlo analysis to put constraints on the effective cosmological constant Ωeff0\Omega^0_{\rm eff}. By imposing that the cosmological constant is the only component that possibly violates the ECs, we derive lower and upper bounds for its value. For instance, we obtain that 0.59<Ωeff0<0.910.59 < \Omega^0_{\rm eff} < 0.91 and 0.40<Ωeff0<0.930.40 < \Omega^0_{\rm eff} < 0.93 within, respectively, 1σ1\sigma and 3σ3\sigma confidence levels. In addition, about 30\% of the posterior distribution is incompatible with a cosmological constant, showing that this method can potentially rule it out as a mechanism for the accelerated expansion. We also study the consequence of these constraints for two particular formulations of the bimetric massive gravity. Namely, we consider the Visser's theory and the Hassan and Roses's massive gravity by choosing a background metric such that both theories mimic General Relativity with a cosmological constant. Using the Ωeff0\Omega^0_{\rm eff} observational bounds along with the upper bounds on the graviton mass we obtain constraints on the parameter spaces of both theories.Comment: 11 pages, 4 figures, 1 tabl

    Produção artesanal de pães, cucas, bolos e bolachas.

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    Cap. 1: Boas práticas no preparo de alimentos; Cap. 2: Para o seu pão "dar certo"; Cap. 3: Cálculo de custos e receitas de pães; Cap. 4: Receitas de cucas, bolos e bolachas; Cap. 5: Atitudes empreendedoras que auxiliam o agricultor familiar na agregação de valor e na diversificação da unidade produtiva.bitstream/item/120035/1/LV2012producaoartesanalGuarienti.pd
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