Eddington-Born-Infeld gravity and the large scale structure of the Universe

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

12 pages, 8 figures, very minor corrections and reference additions, no change to the results

Scientific paper

10.1103/PhysRevD.79.063511

It has been argued that a Universe governed by Eddington-Born-Infeld gravity can be compatible with current cosmological constraints. The extra fields introduced in this theory can behave both as dark matter and dark energy, unifying the dark sector in one coherent framework. We show the various roles the extra fields can play in the expansion of the Universe and study the evolution of linear perturbations in the various regimes. We find that, as a unified theory of the dark sector, Eddington-Born-Infeld gravity will lead to excessive fluctuations in the Cosmic Microwave Background on large scales. In the presence of a cosmological constant, however, the extra fields can behave as a form of non-particulate dark matter and can lead to a cosmology which is entirely compatible with current observations of large scale structure. We discuss the interpretation of this form of dark matter and how it can differ from standard, particulate dark matter.

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

Eddington-Born-Infeld gravity and the large scale structure of the Universe 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 Eddington-Born-Infeld gravity and the large scale structure of the Universe, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Eddington-Born-Infeld gravity and the large scale structure of the Universe will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-245717

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