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Cosmological evolution of statistical system of scalar charged particles equations of particle dynamics in a scalar field. On the basis of kinetic equations, obtained from averaging
Cold black holes and conformal continuations space-time in four dimensions. Black hole solutions are shown to exist for a phantom scalar field whose
The Scalar-photon Coupling with Mie Invariant Within the Scope of Bianchi Type-I Cosmological Model invariant is constat or time-dependent. We study the canonical scalar field and the phantom one.
Physical Characteristics of Free Oscillations of Scalar Fields with Zero Effective Energy and Euclidean Cycles in Cosmological Models in the case of isolated classical and phantom fields and in the case of an asymmetric scalar doublet
Visible, invisible and trapped ghosts as sources of wormholes and black universes.) Such objects exist in the presence of scalar fields with negative kinetic energy ("phantoms", or "ghosts
Magnetic black universes and wormholes with a phantom scalar isotropic universe. The scalar field in these solutions is phantom (i.e. its kinetic energy is negative
No realistic wormholes from ghost-free scalar-tensor phantom dark energy fields, if the nonminimal coupling function f(Φ) is positive everywhere and the scalar field Φ itself
Relativistic Kinetic Theory of Statistical Systems with Conformally Invariant Interparticle Scalar Interaction of scalar charged particles is formulated for a conformally invariant scalar field on the basis
The Scalar-photon Coupling with Mie Invariant Within the Scope of Bianchi Type-I Cosmological Model invariant is constat or time-dependent. We study the canonical scalar field and the phantom one.
On Euclidean Limit Cycles in Cosmological Models Based on Scalar Fields of the phase trajectories of cosmological models based on classical and scalar fields near surfaces of zero
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