Silent universes with a cosmological constant
| dc.creator | Bergh, Norbert Van den | |
| dc.creator | Wylleman, Lode | |
| dc.date | 2004-02-27 | |
| dc.date | 2004-08-12 | |
| dc.date.accessioned | 2026-07-07T11:42:56Z | |
| dc.date.available | 2026-07-07T11:42:56Z | |
| dc.description | We study non-degenerate (Petrov type I) silent universes in the presence of a non-vanishing cosmological constant L. In contrast to the L=0 case, for which the orthogonally spatially homogeneous Bianchi type I metrics most likely are the only admissible metrics, solutions are shown to exist when L is positive. The general solution is presented for the case where one of the eigenvalues of the expansion tensor is 0. | |
| dc.description | 11 pages; several typos corrected which were still present in CGQ version; minor changes | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0402125 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0402125 | |
| dc.identifier | Class.Quant.Grav.21:2291-2299,2004 | |
| dc.identifier | doi:10.1088/0264-9381/21/9/006 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/201063 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Silent universes with a cosmological constant | |
| dc.type | text |