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Simplest cosmological model with the scalar field II. Influence of cosmological constant

A. Yu. Kamenshchik·I. M. Khalatnikov·A. V. Toporensky
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Abstract

Continuing the investigation of the simplest cosmological model with the massive real scalar non-interacting inflaton field minimally coupled to gravity we study an influence of the cosmological constant on the behaviour of trajectories in closed minisuperspace Friedmann-Robertson-Walker model. The transition from chaotic to regular behaviour for large values of cosmological constant is discussed. Combining numerical calculations with qualitative analysis both in configuration and phase space we present a convenient classification of trajectories.

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A. Yu. Kamenshchik, I. M. Khalatnikov, A. V. Toporensky. 1998-01-23. Simplest cosmological model with the scalar field II. Influence of cosmological constant. https://doi.org/10.1142/s0218271898000127

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