Structure Formation in Non-singular Higher Curvature Cosmology
| dc.creator | Kawai, Shinsuke | |
| dc.creator | Soda, Jiro | |
| dc.date | 1999-06-15 | |
| dc.date | 1999-10-17 | |
| dc.date.accessioned | 2026-07-07T03:33:16Z | |
| dc.date.available | 2026-07-07T03:33:16Z | |
| dc.description | We propose novel structure formation scenarios based on a non-singular higher curvature cosmological model. The model is motivated by the $R^2$ coupling of a scalar field appearing in the string theory, and in our scenarios the universe has no beginning and no end. We give two examples with explicit parameter values which are consistent with present observations of the cosmological structure. In the first example, the origin of structures are generated as the adiabatic perturbation during the chaotic inflation, while in the second the isocurvature non-Gaussian perturbation from the superinflating era is responsible for the structure. In the second case it is possible to generate primordial supermassive blackholes whose scale is comparable to what is expected in the galactic nuclei. | |
| dc.description | 8 pages, 5 figures. Sections, figures, references added | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9906046 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9906046 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/36550 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Structure Formation in Non-singular Higher Curvature Cosmology | |
| dc.type | text |