The generality of inflation in closed cosmological models with some quintessence potentials

Abstract

We have investigated the generality of inflation (the probability of inflation in other words) in closed FRW models for a wide class of quintessence potentials. It is shown that inflation is not suppressed for most of them and for a wide enough range of their parameters. It allows us to decide inflation is common enough even in the case of closed Universe.

7 pages, 6 eps figures, to appear in PRD

References in corpus (2)

• The Cosmological Constant and Dark Energy
• Cosmological constraints from Archeops

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