Linear and non-linear perturbations in dark energy models

Details Linear and non-linear perturbations in dark energy models Linear and non-linear perturbations in dark energy models

2003-11-07

arxiv.org/abs/astro-ph/0311175v2

Phys.Rev. D69 (2004) 103524

Astronomy and Astrophysics

Astrophysics

12 pages, submitted to Phys. Rev; v2: added a ref. and corrected a typo

Scientific paper

10.1103/PhysRevD.69.103524

I review the linear and second-order perturbation theory in dark energy models with explicit interaction to matter in view of applications to N-body simulations and non-linear phenomena. Several new or generalized results are obtained: the general equations for the linear perturbation growth; an analytical expression for the bias induced by a species-dependent interaction; the Yukawa correction to the gravitational potential due to dark energy interaction; the second-order perturbation equations in coupled dark energy and their Newtonian limit. I also show that a density-dependent effective dark energy mass arises if the dark energy coupling is varying.

Affiliated with

Also associated with

No associations

Rating

Linear and non-linear perturbations in dark energy models 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 Linear and non-linear perturbations in dark energy models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Linear and non-linear perturbations in dark energy models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-342183