Inclusive Constraints on Unified Dark Matter Models from Future Large-Scale Surveys

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

22 pages, 4 figures, 2 tables

Scientific paper

10.1088/1475-7516/2012/03/039

In the very last years, cosmological models where the properties of the dark components of the Universe - dark matter and dark energy - are accounted for by a single "dark fluid" have drawn increasing attention and interest. Amongst many proposals, Unified Dark Matter (UDM) cosmologies are promising candidates as effective theories. In these models, a scalar field with a non-canonical kinetic term in its Lagrangian mimics both the accelerated expansion of the Universe at late times and the clustering properties of the large-scale structure of the cosmos. However, UDM models also present peculiar behaviours, the most interesting one being the fact that the perturbations in the dark-matter component of the scalar field do have a non-negligible speed of sound. This gives rise to an effective Jeans scale for the Newtonian potential, below which the dark fluid does not cluster any more. This implies a growth of structures fairly different from that of the concordance LCDM model. In this paper, we demonstrate that forthcoming large-scale surveys will be able to discriminate between viable UDM models and LCDM to a good degree of accuracy. To this purpose, the planned Euclid satellite will be a powerful tool, since it will provide very accurate data on galaxy clustering and the weak lensing effect of cosmic shear. Finally, we also exploit the constraining power of the ongoing CMB Planck experiment. Although our approach is the most conservative, with the inclusion of only well-understood, linear dynamics, in the end we also show what could be done if some amount of non-linear information were included.

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

Inclusive Constraints on Unified Dark Matter Models from Future Large-Scale Surveys 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 Inclusive Constraints on Unified Dark Matter Models from Future Large-Scale Surveys, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Inclusive Constraints on Unified Dark Matter Models from Future Large-Scale Surveys will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-186861

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