Cluster number counts dependence on dark energy inhomogeneities and coupling to dark matter

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

9 pages, 8 figures. Further extensions on section on discriminating models with future surveys. Accepted for publication in Mo

Scientific paper

10.1111/j.1365-2966.2006.10774.x

Cluster number counts can be used to test dark energy models. We investigate dark energy candidates which are coupled to dark matter. We analyze the cluster number counts dependence on the amount of dark matter coupled to dark energy. Further more, we study how dark energy inhomogeneities affect cluster abundances. It is shown that increasing the coupling reduces significantly the cluster number counts, and that dark energy inhomogeneities increases cluster abundances. Wiggles in cluster number counts are shown to be a specific signature of coupled dark energy models. Future observations will possibly detect such oscillations and discriminate among the different dark energy models.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Cluster number counts dependence on dark energy inhomogeneities and coupling to dark matter 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 Cluster number counts dependence on dark energy inhomogeneities and coupling to dark matter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cluster number counts dependence on dark energy inhomogeneities and coupling to dark matter will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-716626

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.