A universe of Friedmann type with pressure

Physics

Scientific paper

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Scientific paper

We propose a method of obtaining homogeneous and isotropic cosmological
models satisfying physical conditions for τ → 0 and τ
→ ∞. The model obtained in this way describes a universe
filled with matter, the equation of state of which changes in time from
the asymptotically ultrarelativistic to the asymptotically dust state.

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