Inflationary Cosmology
| dc.creator | Turner, Michael S. | |
| dc.date | 1997-04-03 | |
| dc.date.accessioned | 2026-07-07T02:23:08Z | |
| dc.date.available | 2026-07-07T02:23:08Z | |
| dc.description | Inflation is a bold and expansive extension of the Standard Cosmology. It holds the promise to extend our understanding of the Universe to within 10^{-32}sec of the big bang and answer most of the pressing questions in cosmology. Its boldest assertion is that all the structure observed in the Universe today arose from quantum-mechanical fluctuations on subatomic scales. A flood of cosmological observations and laboratory experiments are testing inflation and within five years we should know whether inflation is to become part of a new standard cosmology. | |
| dc.description | 25 pages LaTeX (cupconf.sty) with eps figures. To be published in Relativistic Astrophysics: A Conference in Honour of Igor Novikov's 60th Birthday (Cambridge University Press, Cambridge, 1997) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9704040 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9704040 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/11135 | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Inflationary Cosmology | |
| dc.type | text |