The generality of inflation in closed cosmological models with some quintessence potentials
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🌌 astro-ph
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inflationclosedenoughgeneralitymodelspotentialsquintessencewide
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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.
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Cited by 1 Pith paper
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