An outline of radiatively-driven cosmology
| dc.creator | Kurucz, Robert L. | |
| dc.date | 2000-03-24 | |
| dc.date | 2000-03-31 | |
| dc.date.accessioned | 2026-07-07T01:52:53Z | |
| dc.date.available | 2026-07-07T01:52:53Z | |
| dc.description | A Big Bang universe consisting, before recombination, of H, D, 3He, 4He, 6Li, and 7Li ions, electrons, photons, and massless neutrinos, at closure density, with a galaxy-size perturbation spectrum but no large-scale structure, will evolve into the universe as we now observe it. Evolution during the first billion years is controlled by radiation. Globular clusters are formed by radiatively-driven implosions, galaxies are formed by radiatively triggered gravitational collapse of systems of globular clusters, and voids are formed by radiatively-driven expansion. After this period the strong radiation sources are exhausted and the universe has expanded to the point where further evolution is determined by gravity and universal expansion. | |
| dc.description | 14 pages, 15 color figures in one file rad; revision added refs for figure 1 revision, symbols replace "sun" in figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0003381 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0003381 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/777 | |
| dc.subject | Astrophysics | |
| dc.title | An outline of radiatively-driven cosmology | |
| dc.type | text |