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Cosmological models with homogeneous and isotropic spatial sections is the basis for the majority of modern cosmological models. We give an example of a metric all of whose
Nonminimal isotropic cosmological model with yang-mills and higgs fieldsWe establish a nonminimal Einstein-Yang-Mills-Higgs model, which contains six coupling parameters
Cosmological models with homogeneous and isotropic spatial sections is the basis for the majority of modern cosmological models. We give an example of a metric all of whose
Nonminimal isotropic cosmological model with yang-mills and higgs fieldsWe establish a nonminimal Einstein-Yang-Mills-Higgs model, which contains six coupling parameters
Scalar Field in Cosmology: Potential for Isotropization and Inflation that the scalar field possesses zero spin, it was basically considered in isotropic cosmological models
Non-minimally coupled nonlinear spinor field in FRW cosmologyWithin the scope of a FRW cosmological model we have studied the role of spinor field
Examples of Exact Exponential Cosmological Solutions with Three Isotropic Subspaces in Einstein–Gauss–Bonnet Gravity presented.). In this case, the multidimensional cosmological model deals with four factor spaces
Kinetics of small disturbances in an isotropic universe I. Derivation of the equations for the disturbancesGravitational disturbances in an isotropic cosmological model are considered within the bounds
Spinor field in Bianchi type-IX space-timeWithin the scope of Bianchi type-IX cosmological model we have studied the role of spinor field
SPINOR FIELD IN BIANCHI TYPE-II UNIVERSEWithin the scope of Bianchi type-II cosmological model we have studied the role of spinor field
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