On singular solutions in multidimensional gravity
| dc.creator | Ivashchuk, V. D. | |
| dc.creator | Melnikov, V. N. | |
| dc.date | 1995-07-28 | |
| dc.date.accessioned | 2026-07-07T03:30:46Z | |
| dc.date.available | 2026-07-07T03:30:46Z | |
| dc.description | It is proved that the Riemann tensor squared is divergent as $τ\ra 0$ for a wide class of cosmological metrics with non-exceptional Kasner-like behaviour of scale factors as $τ\ra 0$, where $τ$ is synchronous time. Using this result it is shown that any non-trivial generalization of the spherically-symmetric Tangherlini solution to the case of $n$ Ricci-flat internal spaces \cite{FIM} has a divergent Riemann tensor squared as $R \ra R_0$, where $R_0$ is parameter of length of the solution. Multitemporal naked singularities are also considered. | |
| dc.description | 16 pages, LaTex. Submitted to Gravitation and Cosmology (new Russian journal) | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9507056 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9507056 | |
| dc.identifier | Grav.Cosmol. 1 (1995) 204-210 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/35635 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | On singular solutions in multidimensional gravity | |
| dc.type | text |