4,980 research outputs found

    Parametric Competition in non-autonomous Hamiltonian Systems

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    In this work we use the formalism of chord functions (\emph{i.e.} characteristic functions) to analytically solve quadratic non-autonomous Hamiltonians coupled to a reservoir composed by an infinity set of oscillators, with Gaussian initial state. We analytically obtain a solution for the characteristic function under dissipation, and therefore for the determinant of the covariance matrix and the von Neumann entropy, where the latter is the physical quantity of interest. We study in details two examples that are known to show dynamical squeezing and instability effects: the inverted harmonic oscillator and an oscillator with time dependent frequency. We show that it will appear in both cases a clear competition between instability and dissipation. If the dissipation is small when compared to the instability, the squeezing generation is dominant and one can see an increasing in the von Neumann entropy. When the dissipation is large enough, the dynamical squeezing generation in one of the quadratures is retained, thence the growth in the von Neumann entropy is contained

    Avaliação das silagens do sorgo BRS-610 em sete estádios de maturação pela técnica in vitro semiautomática de produção de gases.

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    Avaliou-se a qualidade da silagem do sorgo BRS-610 produzida em sete estádios de maturação dos grãos, pela técnica in vitro semi automática de produção de gases. O delineamento foi inteiramente ao acaso, com quatro repetições por tratamento, e as médias foram comparadas pelo teste Scott-knott. Os parâmetros potencial máximo de produção de gases, tempo de colonização, taxa de produção de gases e degradabilidade efetiva da matéria seca para as taxas de passagem de 2, 5 e 8%/h foram obtidos pelo modelo de France et al. O potencial máximo de produção de gases não diferiu entre as silagens e indicou média de 170,5mLmg de matéria seca. Entre leitoso/pastoso e pastoso houve menor tempo de colonização. As maiores taxas de fermentação foram observadas nas silagens produzida entre os estádios pastoso/farináceo a seco. As degradabilidades efetivas foram semelhantes entres as silagens, com média de 46,2%. O sorgo BRS-610 produziu silagem de qualidade satisfatória, com destaque para a silagem produzida com a planta no estádio pastoso/farináceo, por associar melhor taxa de fermentação e menor tempo de colonização

    Abundance trend with condensation temperature for stars with different Galactic birth places

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    During the past decade, several studies reported a correlation between chemical abundances of stars and condensation temperature (also known as Tc trend). However, the real astrophysical nature of this correlation is still debated. The main goal of this work is to explore the possible dependence of the Tc trend on stellar Galactocentric distances, Rmean. We used high-quality spectra of about 40 stars observed with the HARPS and UVES spectrographs to derive precise stellar parameters, chemical abundances, and stellar ages. A differential line-by-line analysis was applied to achieve the highest possible precision in the chemical abundances. We confirm previous results that [X/Fe] abundance ratios depend on stellar age and that for a given age, some elements also show a dependence on Rmean. When using the whole sample of stars, we observe a weak hint that the Tc trend depends on Rmean. The observed dependence is very complex and disappears when only stars with similar ages are considered. To conclude on the possible dependence of the Tc trend on the formation place of stars, a larger sample of stars with very similar atmospheric parameters and stellar ages observed at different Galactocentric distances is neededComment: Accepted by A&
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