43,112 research outputs found

    Effects of the Shear Viscosity on the Character of Cosmological Evolution

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    Bianchi type I cosmological models are studied that contain a stiff fluid with a shear viscosity that is a power function of the energy density, such as ζ=αϔn\zeta = \alpha \epsilon^n. These models are analyzed by describing the cosmological evolutions as the trajectories in the phase plane of Hubble functions. The simple and exact equations that determine these flows are obtained when nn is an integer. In particular, it is proved that there is no Einstein initial singularity in the models of 0≀n<10\leq n < 1. Cosmologies are found to begin with zero energy density and in the course of evolution the gravitational field will create matter. At the final stage, cosmologies are driven to the isotropic Fnedmann universe. It is also pointed out that although the anisotropy will always be smoothed out asymptotically, there are solutions that simultaneously possess non-positive and non-negative Hubble functions for all time. This means that the cosmological dimensional reduction can work even if the matter fluid having shear viscosity. These characteristics can also be found in any-dimensional models

    Hilbert polynomials of j-transforms

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    We study transformations of finite modules over Noetherian local rings that attach to a module MM a graded module Hm0(grI(M))H^{0}_{\mathfrak{m}}( \mathrm{gr}_{I}(M)) defined via partial systems of parameters of MM. Despite the generality of the process, which are called j\mathbf{j}-transforms, in numerous cases they have interesting cohomological properties. We focus on deriving the Hilbert functions of j\mathbf{j}-transforms and studying the significance of the vanishing of some of its coefficients.Comment: This manuscript has been submitted to a journa

    Ideals generated by quadrics

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    Our purpose is to study the cohomological properties of the Rees algebras of a class of ideals generated by quadrics. For all such ideals I⊂R=K[x,y,z]I\subset R = K[x,y,z] we give the precise value of depth R[It]R[It] and decide whether the corresponding rational maps are birational. In the case of dimension d≄3d \geq 3, when K=RK=\mathbb{R}, we give structure theorems for all ideals of codimension dd minimally generated by (d+12)−1{{d+1}\choose{2}}-1 quadrics. For arbitrary fields KK, we prove a polarized version
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