An Introduction of Multiple Scales in a Dynamical Cosmology
| dc.creator | Lindesay, James | |
| dc.date | 2006-05-01 | |
| dc.date | 2006-05-09 | |
| dc.date.accessioned | 2026-07-07T07:09:40Z | |
| dc.date.available | 2026-07-07T07:09:40Z | |
| dc.description | The discovery of scale acceleration evidenced from supernovae luminosities and spatial flatness of feature evolution in the cosmic microwave background presents a challenge to the understanding of the evolution of cosmological vacuum energy. Although some scenarios prefer a fixed cosmological constant with dynamics governed in a Friedman-Robertson-Walker (FRW) geometry, an early inflationary epoch remains a popular model for cosmology. It is therefore advantageous to develop a metric framework that allows a transition from an early inflationary period to a late stage dominated by dark energy. Such a metric is here developed, and some properties of this metric are explored. | |
| dc.description | 8 pages, minor typo correction | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0605007 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0605007 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/111159 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | An Introduction of Multiple Scales in a Dynamical Cosmology | |
| dc.type | text |