Qualitative and numerical analysis of the cosmological model based on the phantom scalar field with self-interaction. II. Comparative analysis of models of classical and phantom fields

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Based on qualitative analysis and numerical simulations of cosmological models with classical and phantom scalar fields with self-interaction are identified and clarified their characteristics, and their potential use as base models in cosmology.

Cosmological models, classical and phantom scalar fields, quality analysis, asymptotic behavior, numerical simulation, numerical gravitation

Короткий адрес: https://sciup.org/14266188

IDR: 14266188

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