23 Other Constraints The Cosmic Microwave Background


     Related Videos
6 Microlensing Astrometry and Other Methods
6 Microlensing Astrometry and Other Methods
The Wild West of Resveratrol and Other Polyphenol Supplements - Jeff Boost PAC
Lec 3 MIT 24 209 Philosophy In Film and Other Media
Lec 1 MIT 24 209 Philosophy In Film and Other Media

     More from this user

     Related Groups


     More on Sciencestage.com


 
  • Video url:                           Embed code: 

  • YaleCourses  status
    (0) (0 Votes)
    Views: (412)   Date: (19-03-10)   Time: (00:47:08)
  • Description: Frontiers/Controversies in Astrophysics (ASTR 160) Reasons for the expansion of the universe are addressed at the start of this lecture, focusing especially on the acceleration of dark energy. Supernovae were the first evidence for the existence of dark energy. Two other proofs are presented. The first is the Cosmic Microwave Background, which is a form of electromagnetic radiation that is perfectly smooth and equal in all directions. It firmly supports the Big Bang theory. Projects attempting to measure it, such as COBE and WMAP, are discussed. Secondly, Large-Scale Clustering is introduced: by measuring the degree of clustering, astronomers hope to advance their understanding of dark energy and dark matter. Computer simulations of the evolution of the universe are shown. Complete course materials are available at the Open Yale Courses website: open.yale.edu This course was recorded in Spring 2007.

Write a Comment
     Related Documents

     Related Wikipedia Results

     Related Pubmed Results

     Related Nature.com Results

     Related Answers.com Results




























 

Powered free by PHPmotion