Non-Riemannian cosmic walls from gravitational collapse
| dc.creator | de Andrade, L. C. Garcia | |
| dc.date | 1999-08-18 | |
| dc.date.accessioned | 2026-07-07T03:33:30Z | |
| dc.date.available | 2026-07-07T03:33:30Z | |
| dc.description | Two classes of metrics obtained from non-Riemannian gravitational collapse are presented.The first is the Taub planar symmetric exact solutions of Einstein-Cartan field equations of gravity describing torsion walls which are obtained from gravitational collapse of time dependent perturbation of Riemannian Taub symmetric solutions of General Relativity.The second is a modification of the Vilenkin Riemannian planar wall which is obtained from a non-Riemannian planar distribution of spinning matter. | |
| dc.description | Latex | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9908050 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9908050 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/36593 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Non-Riemannian cosmic walls from gravitational collapse | |
| dc.type | text |