Production and detection of relic dilatons in string cosmology
| dc.creator | Gasperini, M. | |
| dc.date | 2000-09-28 | |
| dc.date.accessioned | 2026-07-07T03:25:17Z | |
| dc.date.available | 2026-07-07T03:25:17Z | |
| dc.description | This paper summarizes the contribution presented at the {\sl IX Marcel Grossmann Meeting} (Rome, July 2000). It is stressed, in particular, that a non-relativistic background of ultra-light dilatons, produced in the context of string cosmology, could represent today a significant fraction of cold dark matter. If the dilaton mass lies within the resonant band of present gravitational antennas, a stochastic dilaton background with a nearly critical density could be visible, in principle, already at the level of sensitivity of the detectors in operation and presently under construction. | |
| dc.description | 2 pages, Latex, summary of the contribution presented at the IX Marcel Grossmann Meeting (Rome, July 2000). To appear in the proceedings (World Scientific, Singapore) | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0009098 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0009098 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/33648 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Production and detection of relic dilatons in string cosmology | |
| dc.type | text |