Bianchi VIII vacuum solutions to Einstein's equations are causally geodesically complete to the future, given an appropriate time orientation, and the objective of this article is to analyze the asymptotic behaviour of solutions in this time direction. For the Bianchi class A spacetimes, there is a formulation of the field equations that was presented in an article by Wainwright and Hsu, and we analyze the asymptotic behaviour of solutions in these variables. We also try to give the analytic results a geometric interpretation by analyzing how a normalized version of the Riemannian metric on the spatial hypersurfaces of homogeneity evolves
We consider the asymptotic behaviour of spatially homogeneous spacetimes of Bianchi type IX close to...
The dynamics of solutions of the Einstein–Vlasov system with Bianchi I symmetry is discussed in the ...
Methods and properties regarding the linear perturbations are discussed for some spatially closed (v...
Bianchi VIII vacuum solutions to Einstein's equations are causally geodesically complete to the futu...
Bianchi VIII vacuum solutions to Einstein's equations are causally geodesically complete to the futu...
Bianchi VIII vacuum solutions to Einstein’s equations are causally geodesically complete to the futu...
Bianchi VIII vacuum solutions to Einstein’s equations are causally geodesically complete to the futu...
Bianchi VIII vacuum solutions to Einstein’s equations are causally geodesically complete to the futu...
We consider the asymptotic behaviour of spatially homogeneous spacetimes of Bianchi type IX close to...
The maximal globally hyperbolic development of non-Taub-NUT Bianchi IX vacuum initial data and of no...
Using a qualitative analysis based on the Hamiltonian formalism and the orthonormal frame representa...
Methods and properties regarding the linear perturbations are discussed for some spatially closed (v...
The asymptotic behaviour of vacuum Bianchi models of class A near the initial singularity is studied...
Assuming that the space-time is close to special solutions which will play the role of the ω-limit a...
We consider the asymptotic behaviour of spatially homogeneous spacetimes of Bianchi type IX close to...
We consider the asymptotic behaviour of spatially homogeneous spacetimes of Bianchi type IX close to...
The dynamics of solutions of the Einstein–Vlasov system with Bianchi I symmetry is discussed in the ...
Methods and properties regarding the linear perturbations are discussed for some spatially closed (v...
Bianchi VIII vacuum solutions to Einstein's equations are causally geodesically complete to the futu...
Bianchi VIII vacuum solutions to Einstein's equations are causally geodesically complete to the futu...
Bianchi VIII vacuum solutions to Einstein’s equations are causally geodesically complete to the futu...
Bianchi VIII vacuum solutions to Einstein’s equations are causally geodesically complete to the futu...
Bianchi VIII vacuum solutions to Einstein’s equations are causally geodesically complete to the futu...
We consider the asymptotic behaviour of spatially homogeneous spacetimes of Bianchi type IX close to...
The maximal globally hyperbolic development of non-Taub-NUT Bianchi IX vacuum initial data and of no...
Using a qualitative analysis based on the Hamiltonian formalism and the orthonormal frame representa...
Methods and properties regarding the linear perturbations are discussed for some spatially closed (v...
The asymptotic behaviour of vacuum Bianchi models of class A near the initial singularity is studied...
Assuming that the space-time is close to special solutions which will play the role of the ω-limit a...
We consider the asymptotic behaviour of spatially homogeneous spacetimes of Bianchi type IX close to...
We consider the asymptotic behaviour of spatially homogeneous spacetimes of Bianchi type IX close to...
The dynamics of solutions of the Einstein–Vlasov system with Bianchi I symmetry is discussed in the ...
Methods and properties regarding the linear perturbations are discussed for some spatially closed (v...