Isotropic cosmological singularities in spatially-homogeneous models with a cosmological constant
| dc.creator | Tod, Paul | |
| dc.date | 2007-04-19 | |
| dc.date.accessioned | 2026-07-07T11:20:19Z | |
| dc.date.available | 2026-07-07T11:20:19Z | |
| dc.description | We prove well-posedness of the initial value problem for the Einstein equations for spatially-homogeneous cosmologies with data at an isotropic cosmological singularity, for which the matter content is either a cosmological constant with collisionless particles of a single mass (possibly zero) or a cosmological constant with a perfect fluid having the radiation equation of state. In both cases, with a positive cosmological constant, these solutions, except possibly for Bianchi-type-IX, will expand forever, and be geodesically-complete into the future. | |
| dc.description | 22 pages; | |
| dc.identifier | https://arxiv.org/abs/0704.2506 | |
| dc.identifier | http://arxiv.org/abs/0704.2506 | |
| dc.identifier | Class.Quant.Grav.24:2415-2432,2007 | |
| dc.identifier | doi:10.1088/0264-9381/24/9/017 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/193924 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Isotropic cosmological singularities in spatially-homogeneous models with a cosmological constant | |
| dc.type | text |