13,023 research outputs found

    Clustering, Angular Size and Dark Energy

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    The influence of dark matter inhomogeneities on the angular size-redshift test is investigated for a large class of flat cosmological models driven by dark energy plus a cold dark matter component (XCDM model). The results are presented in two steps. First, the mass inhomogeneities are modeled by a generalized Zeldovich-Kantowski-Dyer-Roeder (ZKDR) distance which is characterized by a smoothness parameter α(z)\alpha(z) and a power index γ\gamma, and, second, we provide a statistical analysis to angular size data for a large sample of milliarcsecond compact radio sources. As a general result, we have found that the α\alpha parameter is totally unconstrained by this sample of angular diameter data.Comment: 9 pages, 7 figures, accepted in Physical Review

    A2(2)A_{2}^{(2)} Gaudin model and its associated Knizhnik-Zamolodchikov equation

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    The semiclassical limit of the algebraic Bethe Ansatz for the Izergin-Korepin 19-vertex model is used to solve the theory of Gaudin models associated with the twisted A2(2)A_{2}^{(2)} R-matrix. We find the spectra and eigenvectors of the N1N-1 independents Gaudin Hamiltonians. We also use the off-shell Bethe Ansatz method to show how the off-shell Gaudin equation solves the associated trigonometric system of Knizhnik-Zamolodchikov equations.Comment: 20 pages,no figure, typos corrected, LaTe

    Thermodynamics of Decaying Vacuum Cosmologies

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    The thermodynamic behavior of vacuum decaying cosmologies is investigated within a manifestly covariant formulation. Such a process corresponds to a continuous irreversible energy flow from the vacuum component to the created matter constituents. It is shown that if the specific entropy per particle remains constant during the process, the equilibrium relations are preserved. In particular, if the vacuum decays into photons, the energy density ρ\rho and average number density of photons nn scale with the temperature as ρT4\rho \sim T^{4} and nT3n \sim T^{3}. The temperature law is determined and a generalized Planckian type form of the spectrum, which is preserved in the course of the evolution, is also proposed. Some consequences of these results for decaying vacuum FRW type cosmologies as well as for models with ``adiabatic'' photon creation are discussed.Comment: 21 pages, uses LATE

    Exact Lyapunov Exponent for Infinite Products of Random Matrices

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    In this work, we give a rigorous explicit formula for the Lyapunov exponent for some binary infinite products of random 2×22\times 2 real matrices. All these products are constructed using only two types of matrices, AA and BB, which are chosen according to a stochastic process. The matrix AA is singular, namely its determinant is zero. This formula is derived by using a particular decomposition for the matrix BB, which allows us to write the Lyapunov exponent as a sum of convergent series. Finally, we show with an example that the Lyapunov exponent is a discontinuous function of the given parameter.Comment: 1 pages, CPT-93/P.2974,late

    Inflationary Models Driven by Adiabatic Matter Creation

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    The flat inflationary dust universe with matter creation proposed by Prigogine and coworkers is generalized and its dynamical properties are reexamined. It is shown that the starting point of these models depends critically on a dimensionless parameter Σ\Sigma, closely related to the matter creation rate ψ\psi. For Σ\Sigma bigger or smaller than unity flat universes can emerge, respectively, either like a Big-Bang FRW singularity or as a Minkowski space-time at t=t=-\infty. The case Σ=1\Sigma=1 corresponds to a de Sitter-type solution, a fixed point in the phase diagram of the system, supported by the matter creation process. The curvature effects have also been investigated. The inflating de Sitter is a universal attractor for all expanding solutions regardless of the initial conditions as well as of the curvature parameter.Comment: 25 pages, 2 figures(available from the authors), uses LATE
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