Scalar fluctuations in dilatonic brane-worlds
| dc.creator | Bozza, V. | |
| dc.creator | Gasperini, M. | |
| dc.creator | Veneziano, G. | |
| dc.date | 2001-11-29 | |
| dc.date.accessioned | 2026-07-07T04:12:46Z | |
| dc.date.available | 2026-07-07T04:12:46Z | |
| dc.description | We derive and solve the full set of scalar perturbation equations for a class of five-dimensional brane--world solutions, with a dilaton scalar field coupled to the bulk cosmological constant and to a 3-brane. The spectrum contains one localized massless scalar mode, to be interpreted as an effective dilaton on the brane, inducing long--range scalar interactions. Two massive scalar modes yield corrections to Newton's law at short distances, which persist even in the limit of vanishing dilaton (namely, in the standard Randall--Sundrum configuration). | |
| dc.description | 10 pages. Talk presented by V. Bozza at COSMO-01 conference, Rovaniemi, 2001 | |
| dc.identifier | https://arxiv.org/abs/hep-th/0111268 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0111268 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/51020 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Scalar fluctuations in dilatonic brane-worlds | |
| dc.type | text |