We study the general chaotic features of dynamics of the phantom field modelled in terms of a single scalar field coupled conformally to gravity. We demonstrate that the dynamics of the FRW model with dark energy in the form of phantom field can be regarded as a scattering process of two types: multiple chaotic and classical non-chaotic. It depends whether the spontaneously symmetry breaking takes place. In the first class of models with the spontaneously symmetry breaking the dynamics is similar to the Yang-Mills theory. We find the evidence of a fractal structure in the phase space of initial conditions. We observe similarities to the phenomenon of a multiple scattering process around the origin. In turn the class of models without the sp...
We investigate the cosmological dynamics of a nonminimally coupled scalar field system described by ...
AbstractWe find the group of symmetry transformations generated by interacting fluids in spatially f...
We argue that the wave function describing a FRW universe with a massive scalar field must reflect t...
We study the general features of a dynamics of a phantom field in the cosmological context. In the c...
The results on chaos in FRW cosmology with a massive scalar field are extended to another scalar fie...
We investigate the cosmological evolution of an interacting phantom energy model in which the phanto...
We find that the expansion of the universe is accelerating by analyzing the recent observation data ...
Phantom energy can be visualized as a scalar field with a (non-canonical) negative kinetic energy te...
AbstractWe construct phantom energy models with the equation of state parameter w which is less than...
The latest cosmological observations by the Planck collaboration (and combined with others) are com...
A class of braneworld models can lead to phantom-like acceleration of the late universe, but without...
The cosmological model with two phantom scalar fields with the special choice of field's potential i...
In this paper, we introduce a non-minimally conformally coupled scalar field and dark matter in F(T)...
The SNe type Ia data admit that the Universe today may be dominated by some exotic matter with negat...
It is shown that phantom scalar models can be mapped into a mathematically equivalent, modified $F(R...
We investigate the cosmological dynamics of a nonminimally coupled scalar field system described by ...
AbstractWe find the group of symmetry transformations generated by interacting fluids in spatially f...
We argue that the wave function describing a FRW universe with a massive scalar field must reflect t...
We study the general features of a dynamics of a phantom field in the cosmological context. In the c...
The results on chaos in FRW cosmology with a massive scalar field are extended to another scalar fie...
We investigate the cosmological evolution of an interacting phantom energy model in which the phanto...
We find that the expansion of the universe is accelerating by analyzing the recent observation data ...
Phantom energy can be visualized as a scalar field with a (non-canonical) negative kinetic energy te...
AbstractWe construct phantom energy models with the equation of state parameter w which is less than...
The latest cosmological observations by the Planck collaboration (and combined with others) are com...
A class of braneworld models can lead to phantom-like acceleration of the late universe, but without...
The cosmological model with two phantom scalar fields with the special choice of field's potential i...
In this paper, we introduce a non-minimally conformally coupled scalar field and dark matter in F(T)...
The SNe type Ia data admit that the Universe today may be dominated by some exotic matter with negat...
It is shown that phantom scalar models can be mapped into a mathematically equivalent, modified $F(R...
We investigate the cosmological dynamics of a nonminimally coupled scalar field system described by ...
AbstractWe find the group of symmetry transformations generated by interacting fluids in spatially f...
We argue that the wave function describing a FRW universe with a massive scalar field must reflect t...