Stable Inflationary Dissipative Cosmologies

Details Stable Inflationary Dissipative Cosmologies Stable Inflationary Dissipative Cosmologies

1999-11-25

arxiv.org/abs/gr-qc/9911097v1

Int.J.Mod.Phys.D9:43-55,2000

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

13 pages, LaTeX 2.09, 1 figure. To be published in International Journal of Modern Physics D

Scientific paper

10.1142/S0218271800000050

The stability of the de Sitter era of cosmic expansion in spatially curved
homogeneous isotropic universes is studied. The source of the gravitational
field is an imperfect fluid such that the parameters that characterize it may
change with time. In this way we extend our previous analysis for
spatially-flat spaces as well as the work of Barrow.

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