Future complete Einsteinian space times with U(1) symmetry, the unpolarized case
Yvonne Choquet-Bruhat
Abstract
I prove the existence of vacuum S1 symmetric Einsteinian, unpolarized, space times which are complete in the direction of the expansion, for small initial data, without supposing that the S1 orbits are orthogonal to the 3-manifolds, as was done in previous work in collaboration with V. Moncrief.
Create a lesson
Related papers
Exact algebraic separation of the gravitoelectromagnetic perturbations of Kerr-Newman-(anti-)de Sitter black holes
Jun-Kun Zhao
Breakdown of hydrodynamic universality in causal first-order viscous neutron star oscillations
Lennox S. Keeble, Alejandro Cárdenas-Avendaño
From Accelerating Rotating Black Holes to a Swirling Universe
José Barrientos, Adolfo Cisterna
Photon-Return and Polar-Focusing Crossovers near Extremal Kerr
Valentina Gonzalez-Moya, Ali Ovgun, Joel Saavedra
Thermodynamics of rotating black holes with constrained primary hair
Wentao Liu, Di Wu, Shao-Wen Wei et al.
An exact Simpson-Visser family in bumblebee gravity
A. A. Araújo Filho