We reformulate the dynamics of homogeneous cosmologies with a scalar field matter source with an arbitrary self- interaction potential in the language of jet bundles and extensions of vector fields. In this framework, the Bianchi— scalar field equations become subsets of the second Bianchi jet bundle, J2 , and every Bianchi cosmology is naturally extended to live on a variety of J2 . We are interested in the existence and behaviour of extensions of arbitrary Bianchi-Lie and variational vector fields acting on the Bianchi variety and accordingly we classify all such vector fields corresponding to both Bianchi classes A and B. We give examples of functions defined on Bianchi jet bundles which are constant along some Bianchi models (first inte...
We discuss the field equations of Brans-Dicke theory for a spatially homogeneous and anisotropic Bia...
Methods and properties regarding the linear perturbations are discussed for some spatially closed (v...
Summary: "Evolution of a homogeneous and anisotropic cosmological model with interacting scalar, vec...
none1noThe Bianchi classification of the three-dimensional Lie algebras and of the spatially homogen...
In this paper we examine in detail the implementation, with its associated difficulties, of the Kill...
Lie symmetries are discussed for the Wheeler-De Witt equation in Bianchi Class A cosmologies. In par...
We investigate the consequences of (a) the source-free Maxwell equations and (b) the equations of ma...
An answer to the question: Can, in general, the adoption of a given symmetry induce a further symmet...
Abstract. Homogeneous, nearly-isotropic Bianchi cosmological models are consid-ered. Their time evol...
To analyze linear field equations on a locally homogeneous spacetime by means of separation of varia...
We determine the most general form of the antisymmetric H-field tensor derived from a purely time-de...
El títol de la versió pre-print de l'article és: Analytic integrability of the Bianchi Class B cosmo...
In this paper we use Noether symmetries of the geodesic Lagrangian in Bianchi V spacetimes to study ...
International audienceStarting from an anisotropic flat cosmological model (Bianchi type I), we show...
We use our Noetherr Symmetry Approach to study the Einstein equations minimally coupled with a scala...
We discuss the field equations of Brans-Dicke theory for a spatially homogeneous and anisotropic Bia...
Methods and properties regarding the linear perturbations are discussed for some spatially closed (v...
Summary: "Evolution of a homogeneous and anisotropic cosmological model with interacting scalar, vec...
none1noThe Bianchi classification of the three-dimensional Lie algebras and of the spatially homogen...
In this paper we examine in detail the implementation, with its associated difficulties, of the Kill...
Lie symmetries are discussed for the Wheeler-De Witt equation in Bianchi Class A cosmologies. In par...
We investigate the consequences of (a) the source-free Maxwell equations and (b) the equations of ma...
An answer to the question: Can, in general, the adoption of a given symmetry induce a further symmet...
Abstract. Homogeneous, nearly-isotropic Bianchi cosmological models are consid-ered. Their time evol...
To analyze linear field equations on a locally homogeneous spacetime by means of separation of varia...
We determine the most general form of the antisymmetric H-field tensor derived from a purely time-de...
El títol de la versió pre-print de l'article és: Analytic integrability of the Bianchi Class B cosmo...
In this paper we use Noether symmetries of the geodesic Lagrangian in Bianchi V spacetimes to study ...
International audienceStarting from an anisotropic flat cosmological model (Bianchi type I), we show...
We use our Noetherr Symmetry Approach to study the Einstein equations minimally coupled with a scala...
We discuss the field equations of Brans-Dicke theory for a spatially homogeneous and anisotropic Bia...
Methods and properties regarding the linear perturbations are discussed for some spatially closed (v...
Summary: "Evolution of a homogeneous and anisotropic cosmological model with interacting scalar, vec...