Status of Cosmology
| dc.creator | Primack, Joel R. | |
| dc.date | 1999-12-06 | |
| dc.date.accessioned | 2026-07-07T02:34:47Z | |
| dc.date.available | 2026-07-07T02:34:47Z | |
| dc.description | The cosmological parameters that I will emphasize are the Hubble parameter $H_0 \equiv 100 h$ km s$^{-1}$ Mpc$^{-1}$, the age of the universe $t_0$, the average matter density $Ω_m$, the baryonic matter density $Ω_b$, the neutrino density $Ω_ν$, and the cosmological constant $Ω_Λ$. The evidence currently favors $t_0 \approx 13$ Gyr, $h \approx 0.65$, $Ω_m \approx 0.3$, $Ω_Λ\approx 0.7$. | |
| dc.description | 14 pages, uses paspconf, to appear in "Cosmic Flows: Towards an Understanding of Large-Scale Structure," eds. S. Courteau, M.A. Strauss, and J.A. Willick (ASP Conference Series) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9912089 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9912089 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/15384 | |
| dc.subject | Astrophysics | |
| dc.title | Status of Cosmology | |
| dc.type | text |