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Qualitative and Numerical Analysis of the Cosmological Model with a Phantom Scalar Field with a phantom scalar field is qualitatively analyzed.
Qualitative and Numerical Analysis of the Cosmological Model with a Phantom Scalar Field with a phantom scalar field is qualitatively analyzed.
Dynamics of Cosmological Models with Nonlinear Classical and Phantom Scalar Fields. II. Qualitative Analysis and Numerical Modeling and phantom scalar fields with self-action are performed. Complete phase portraits of the corresponding
Dynamics of Cosmological Models with Nonlinear Classical Phantom Scalar Fields. I. Formulation of the Mathematical Model describing the cosmological evolution of classical and phantom scalar fields with self-action are formulated
Qualitative and Numerical Analysis of a Cosmological Model Based on an Asymmetric Scalar Doublet with Minimal Connections. III. Multiply-Connected Factor and Character of the Singular Points, minimally interacting scalar fields, both classical and phantom, the behavior of the model near zero energy
Qualitative and numerical analysis of a cosmological model based on a phantom scalar field with self-interaction based on a phantom scalar field by qualitative analysis of the set of differential equations. We show
Scalar multi-wormholes-Weyl approach to non-vacuum configurations with massless scalar fields. Considering a phantom scalar field
Compact and extended objects from self-interacting phantom fields-interacting phantom fields. The phantom fields come from two scalar fields with a "wrong-sign" (negative) kinetic
Qualitative and numerical analysis of a cosmological model based on a phantom scalar field with self-interaction based on a phantom scalar field by qualitative analysis of the set of differential equations. We show
Scalar multi-wormholes-Weyl approach to non-vacuum configurations with massless scalar fields. Considering a phantom scalar field
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