Kantowski-Sachs Brane Cosmology
| dc.creator | Makarenko, A. N. | |
| dc.creator | Obukhov, V. V. | |
| dc.creator | Osetrin, K. E. | |
| dc.date | 2003-01-31 | |
| dc.date.accessioned | 2026-07-07T03:27:36Z | |
| dc.date.available | 2026-07-07T03:27:36Z | |
| dc.description | We consider brane Kantowski-Sachs Universe when bulk space is five-dimensional Anti-deSitter space. The corresponding cosmological equations with perfect fluid are written. For several specific choices of relation between energy and pressure it is found the behavior of scale factors at early time. In particulary, for $γ=3/2$ Kantowski-Sachs brane cosmology is modified to become the isotropic one, while for $γ=1$ it remains the anisotropic cosmology in the process of evolution. | |
| dc.description | 3 pages, other comments | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0301124 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0301124 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/34489 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Kantowski-Sachs Brane Cosmology | |
| dc.type | text |