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.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
