Bianchi-type string cosmology involves generalizations of the FRW backgrounds with three transitive spacelike Killing symmetries, but without any a priori assumption of isotropy in the 3D sections of homogeneity. With emphasis on those cases with diagonal metrics and vanishing cosmological constant which which have not been previously examined in the literature, the present findings allow an overview and the classification of all Bianchi-type backgrounds. These string solutions (at least to lowest order in alpha prime) offer prototypes for the study of spatial anisotropy and its impact on the dynamics of the early universe
This manuscript is devoted to the investigation of the Bianchi type I universe in the context of f (...
We investigate the spatially homogeneous Bianchi Type III cosmological models with magnetized anisot...
The Wheeler-DeWitt equation is considered in the context of generalized scalar-tensor theories of gr...
We determine the most general form of the antisymmetric $H$-field tensor that is admitted by all pos...
A classification of all possible spatially homogeneous 4D string backgrounds (HSBs) has been obtaine...
We study the low energy string effective action with an exponential type dilaton potential and vanis...
The second order Ordinary Differential Equation which describes the unknown part of the solution spa...
We study the low energy string effective action with an exponential type dilaton potential and vanis...
We investigate in detail the qualitative behaviour of the class of Bianchi type B spatially homogene...
In the Bianchi I cosmology some subclasses of the Horndeski theory allow for the non-standard anisot...
We ask whether the problem on the initial conditions in Cosmology can be solved if an efficient elim...
Here we studied Bianchi type-I cosmological models with massive strings in general relativity in fiv...
In cosmological group field theory (GFT) models for quantum gravity coupled to a massless scalar fie...
Abstract. Homogeneous, nearly-isotropic Bianchi cosmological models are consid-ered. Their time evol...
To understand the observational properties of cosmological models, in particular, the temperature of...
This manuscript is devoted to the investigation of the Bianchi type I universe in the context of f (...
We investigate the spatially homogeneous Bianchi Type III cosmological models with magnetized anisot...
The Wheeler-DeWitt equation is considered in the context of generalized scalar-tensor theories of gr...
We determine the most general form of the antisymmetric $H$-field tensor that is admitted by all pos...
A classification of all possible spatially homogeneous 4D string backgrounds (HSBs) has been obtaine...
We study the low energy string effective action with an exponential type dilaton potential and vanis...
The second order Ordinary Differential Equation which describes the unknown part of the solution spa...
We study the low energy string effective action with an exponential type dilaton potential and vanis...
We investigate in detail the qualitative behaviour of the class of Bianchi type B spatially homogene...
In the Bianchi I cosmology some subclasses of the Horndeski theory allow for the non-standard anisot...
We ask whether the problem on the initial conditions in Cosmology can be solved if an efficient elim...
Here we studied Bianchi type-I cosmological models with massive strings in general relativity in fiv...
In cosmological group field theory (GFT) models for quantum gravity coupled to a massless scalar fie...
Abstract. Homogeneous, nearly-isotropic Bianchi cosmological models are consid-ered. Their time evol...
To understand the observational properties of cosmological models, in particular, the temperature of...
This manuscript is devoted to the investigation of the Bianchi type I universe in the context of f (...
We investigate the spatially homogeneous Bianchi Type III cosmological models with magnetized anisot...
The Wheeler-DeWitt equation is considered in the context of generalized scalar-tensor theories of gr...