A solution to the problem posed by Byland and Scialom
| dc.creator | Zotov, M. Yu. | |
| dc.date | 1999-08-19 | |
| dc.date | 2000-09-15 | |
| dc.date.accessioned | 2026-07-07T03:33:30Z | |
| dc.date.available | 2026-07-07T03:33:30Z | |
| dc.description | Recently, Byland and Scialom studied the evolution of the Bianchi I, the Bianchi III and the Kantowski-Sachs universe on the basis of dynamical systems methods (Phys. Rev. D57, 6065 (1998), gr-qc/9802043). In particular, they have pointed out a problem to determine the stability properties of one of the degenerate critical points of the corresponding dynamical system. Here we give a solution, showing that this point is unstable both to the past and to the future. We also discuss the asymptotic behavior of the trajectories in the vicinity of another critical point. | |
| dc.description | REVTeX, 2 pages; v2: the title changed to avoid ambiguity -- thanks to Brad Woodworth | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9908052 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9908052 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/36594 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | A solution to the problem posed by Byland and Scialom | |
| dc.type | text |