Cosmology 1996
arXiv:astro-ph/9704024 · doi:10.1016/S0375-9474(97)00300-X
Abstract
The current state of cosmology is easy to summarize: a very successful standard model -- the hot big-bang cosmology -- that accounts for the evolution of the Universe from 10^{-2} sec until the present; bold ideas based upon early-Universe physics -- foremost among them inflation and cold dark matter -- that can extend the standard cosmology to times as early as 10^{-32} sec and address the most pressing questions; and a flood of observations -- from determinations of the Hubble constant to measurements of CBR anisotropy -- that are testing inflation and cold dark matter.
16 pages LaTeX with 7 eps figures. To be published in Flavor Physics (Proceedings of the Fourth KEK Topical Conference, Tsukuba, Japan, October 1996)