Skip to content
lectern.tv
1/4

Omega and the End of the Universe

Professor

49:10·2008·introductory level

This session explores the role of gravity in cosmic expansion, explaining why the expansion rate cannot be constant. It details methods for calculating the universe's actual density and proposes hypotheses for dark matter, including WIMPs and MACHOs.

Frontiers/Controversies in Astrophysics (ASTR 160)

Source: YaleCourses via YouTubeWatch on YouTube

Comments

Add a comment...Sign in