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Interacting spinor, vector and scalar fields in Bianchi-I space-time: the isotropization problem to create a model with isotropization at late times, whatever the function H(I), whereas an addition of a
To theory of asymptotically stable accelerating universe in Riemann-Cartan spacetime© 2014 IOP Publishing Ltd and Sissa Medialab srl. Homogeneous isotropic cosmological models built
Anisotropy screening in Horndeski cosmologies© 2020 authors. Published by the American Physical Society. We consider anisotropic cosmologies
Cosmological Model Bianchi-I with Perfect Fluid and Interacting Vector and Scalar Fields: Problems Initial Singularity and Isotropization and phantom matter. We have shown that, the perfect fluid does not affect on model's evolution on the initial
Variations of α and G from nonlinear multidimensional gravity cosmological models in both the Einstein and Jordan conformal frames. One of the models turns out to be equally
Duality between k-essence and Rastall gravity cosmological models with a perfect fluid: one (R1) in which there is no coupling between the scalar field
Cosmology in nonlinear multidimensional gravity and the Casimir effectWe study the possible cosmological models in Kaluza-Klein-type multidimensional gravity with a
Qualitative and Numerical Analysis of the Cosmological Model with a Phantom Scalar Field© 2017 Springer Science+Business Media New YorkThe cosmological model based on the model of vacuum
Collisionless self-gravitating statistical systems of scalarly interacting particles of the Vlasov equation for the isotropic homogenous model of the Universe is found. Asymptotic solutions
Phenomenological Model of Multiphase Cosmological Scenario in Theory of Induced Gravity. This is due to the fact that the fundamental constants of the theory, such as gravitational and cosmological
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