Scalar perturbations in deflationary cosmological models
| dc.creator | Capozziello, S. | |
| dc.creator | Lambiase, G. | |
| dc.creator | Scarpetta, G. | |
| dc.date | 1998-06-09 | |
| dc.date.accessioned | 2026-07-07T03:32:26Z | |
| dc.date.available | 2026-07-07T03:32:26Z | |
| dc.description | We consider scalar perturbations of energy--density for a class of cosmological models where an early phase of accelerated expansion evolves, without any fine--tuning for graceful exit, towards the standard Friedman eras of observed universe. The geometric procedure which generates such models agrees with results for string cosmology since it works if dynamics is dominated by a primordial fluid of extended massive objects. The main result is that characteristic scales of cosmological interest, connected with the extension of such early objects, are selected.} | |
| dc.description | 6 pages, ISMC'98 (Potsdam), Latex file, sprocl.sty | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9806042 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9806042 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/36233 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Scalar perturbations in deflationary cosmological models | |
| dc.type | text |