Usual and phantom scalar fields in five dimensions: compactification and flat thick brane solutions
| dc.creator | Dzhunushaliev, V. | |
| dc.creator | Folomeev, V. | |
| dc.creator | Myrzakul, S. | |
| dc.creator | Myrzakulov, R. | |
| dc.date | 2008-01-25 | |
| dc.date | 2008-10-08 | |
| dc.date.accessioned | 2026-07-07T10:07:55Z | |
| dc.date.available | 2026-07-07T10:07:55Z | |
| dc.description | In the model of a gravitating system with two scalar fields (one of which is phantom), two new types of regular solutions are found: mechanism for compactification of an extra dimension and a flat thick brane solution. It is shown that the first model has solutions oscillating over the extra coordinate and giving a finite radius of compactification of the fifth dimension and the second model is a flat thick brane embedded in the 5D Minkowski spacetime. Geometry of both models corresponds to a five-dimensional Minkowski space-time. Consideration of linear perturbations shows stability of the obtained solutions. | |
| dc.description | title is changed, new results are added | |
| dc.identifier | https://arxiv.org/abs/0801.3874 | |
| dc.identifier | http://arxiv.org/abs/0801.3874 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/170817 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Usual and phantom scalar fields in five dimensions: compactification and flat thick brane solutions | |
| dc.type | text |