{ "id": "astro-ph/9904051", "version": "v1", "published": "1999-04-03T21:44:37.000Z", "updated": "1999-04-03T21:44:37.000Z", "title": "Cosmological Parameters", "authors": [ "Michael S. Turner" ], "comment": "27 pages LaTeX with 8 eps figures. To be published in The Proceedings of Particle Physics and the Universe (Cosmo-98), edited by David O. Caldwell (AIP, Woodbury, NY)", "doi": "10.1063/1.59381", "categories": [ "astro-ph", "hep-ph" ], "abstract": "The discussion of cosmological parameters used to be a source of embarrassment to cosmologists. Today, measurements of the cosmological parameters are leading the way into the era of precision cosmology. The CMB temperature is measured to four significant figures, T_0=2.7277+/-0.002 K; the Hubble constant is now determined with a reliable error estimate, H_0=(65+/-5) km sec^-1 Mpc^-1; the mass density of baryons is precisely determined by big-bang nucleosynthesis Omega_B = (0.019+/-0.001) h^-2; and the age of the Universe inferred from the ages of the oldest stars is 14+/-1.5 Gyr, which is consistent the expansion age. Further, we have the first full accounting of matter and energy in the Universe, complete with a self consistency check. Expressed as a fraction of the critical density it goes like this: neutrinos, between 0.3% and 15%; stars, between 0.3% and 0.6%; baryons (total), 5+/-0.5%; matter (total),40% +/- 10%; smooth, dark energy, 80% +/- 20%; totaling to the critical density (within the errors).", "revisions": [ { "version": "v1", "updated": "1999-04-03T21:44:37.000Z" } ], "analyses": { "subjects": [ "98.80.Es" ], "keywords": [ "cosmological parameters", "critical density", "self consistency check", "first full", "expansion age" ], "tags": [ "journal article" ], "note": { "typesetting": "LaTeX", "pages": 27, "language": "en", "license": "arXiv", "status": "editable", "inspire": 483703, "adsabs": "1999AIPC..478..113T" } } }