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Interacting dark sector and the coincidence problem within the scope of LRS Bianchi type I model interaction between dark energy and dark matter in locally rotationally symmetric (LRS) Bianchi-I space
The anisotropic distribution of the dark energy within the scope of LRS Bianchi type I model and anisotropic dark energy. We assume that the shear scalar (σ) is proportional to expansion scalar (θ). A
Interactions in the dark sector within the scope of Bianchi type-V model) and anisotropic dark energy (DE) is considered. Assuming a law for deviation from the equation of state (Eos
The change of the Universe epochs within the scope of Bianchi type-V model-V cosmological model with dark matter and anisotropic dark energy. It is assumed that the two sources minimally
Multidimensional cosmology, constants and transition to new SI units-component anisotropic fluid is presented. The metrics of solutions are defined on a manifold that contains a product
Spinor field in Bianchi type-IX space-time of energy-momentum tensor of spinor field along the principal axis are not the same (i.e.,), even
SPINOR FIELD IN BIANCHI TYPE-II UNIVERSE in the evolution of the Universe. It is found that in this case the components of energy-momentum tensor of spinor
Anisotropic deformations of spatially open cosmology in massive gravity theory to study anisotropic deformations of the spatially open homogeneous and isotropic cosmology in the ghost
The late cosmic acceleration and the coincidence problem in Bianchi type i Universe-minimal interaction between dark energy (DE) and dark matter (DM) allows to combine the transition from matter
Dark energy fingerprints in the nonminimal Wu-Yang wormhole structure. Solutions of the first type relate to the model, in which the dark energy is anisotropic; i.e., the radial
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