Testing cosmological models with the Integrated Sachs-Wolfe effect

Details Testing cosmological models with the Integrated Sachs-Wolfe effect Testing cosmological models with the Integrated Sachs-Wolfe effect

Feb 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011jphcs.280a2009r&link_type=abstract

Journal of Physics: Conference Series, Volume 280, Issue 1, pp. 012009 (2011).

Physics

Scientific paper

The cross correlation between the Cosmic Microwave Background and the Large Scale Structure of the Universe is a powerful probe to test our cosmological models. This correlation can be used to detect the Integrated Sachs-Wolfe effect, and it depends on both the geometry of the Universe and the properties of the clustering and evolution of structures; for this reason it can be used to test and constrain cosmological models and parameters as well as theories of gravity. In this proceeding we briefly introduce the ISW effect and present some of the recent cosmological tests done using it.

Affiliated with

Also associated with

No associations

Rating

Testing cosmological models with the Integrated Sachs-Wolfe effect does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Testing cosmological models with the Integrated Sachs-Wolfe effect, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Testing cosmological models with the Integrated Sachs-Wolfe effect will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1122514