44,584 research outputs found
Effects of the Shear Viscosity on the Character of Cosmological Evolution
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
. 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 is an integer. In particular, it is proved that there is no
Einstein initial singularity in the models of . 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
We study transformations of finite modules over Noetherian local rings that
attach to a module a graded module defined via partial systems of parameters of . Despite
the generality of the process, which are called -transforms, in
numerous cases they have interesting cohomological properties. We focus on
deriving the Hilbert functions of -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
Our purpose is to study the cohomological properties of the Rees algebras of
a class of ideals generated by quadrics. For all such ideals we give the precise value of depth and decide whether the
corresponding rational maps are birational. In the case of dimension , when , we give structure theorems for all ideals of
codimension minimally generated by quadrics. For
arbitrary fields , we prove a polarized version
- âŠ