Volume 366, Number 2, February I 2001
|Page(s)||395 - 406|
|Published online||15 February 2001|
Classification of multifluid CP world models
Astronomisches Institut der Ruhr-Universität, 44780 Bochum, Germany e-mail: jthomas, firstname.lastname@example.org
Accepted: 14 November 2000
Various classification schemes exist for homogeneous and isotropic (CP) world models, which include pressureless matter (so-called dust) and Einstein's cosmological constant Λ. We here classify the solutions of more general world models consisting of up to four non-interacting fluids, each with pressure , energy density and an equation of state with . In addition to repulsive fluids with negative pressure and positive energy density, which generalize the classical repulsive (positive) Λ component, we consider fluids with negative energy density as well. The latter generalize a negative Λ component. This renders possible new types of models that do not occur among the classical classifications of world models. Singularity-free periodic solutions as well as further "hill-type", "hollow-type"and "shifting-type"models are feasible. However, if one only allows for three components (dust, radiation and one repulsive component) in a spatially flat universe the repulsive classical Λ fluid (with ) tends to yield the smoothest fits of the Supernova Ia data from Perlmutter et al. (1999). Adopting the SN Ia constraints, exotic negative energy density components can be fittingly included only if the universe consists of four or more fluids.
Key words: Cosmology: miscellaneous / Cosmology: theory
© ESO, 2001
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