Dark-Energy Evolution Across the Cosmological-Constant Boundary

Details Dark-Energy Evolution Across the Cosmological-Constant Boundary Dark-Energy Evolution Across the Cosmological-Constant Boundary

2005-01-06

arxiv.org/abs/astro-ph/0501104v1

Phys.Rev.D72:043527,2005

Astronomy and Astrophysics

Astrophysics

6 pages, 2 figures

Scientific paper

10.1103/PhysRevD.72.043527

We explore the properties of dark energy models for which the equation-of-state, w, defined as the ratio of pressure to energy density, crosses the cosmological-constant boundary w = -1. We adopt an empirical approach, treating the dark energy as an uncoupled fluid or a generalized scalar field. We describe the requirements for a viable model, in terms of the equation-of-state and sound speed. A generalized scalar field cannot safely traverse w = -1, although a pair of scalars with w > -1 and w < -1 will work. A fluid description with a well-defined sound speed can also cross the boundary. Contrary to expectations, such a crossing model does not instantaneously resemble a cosmological constant at the moment w = -1 since the density and pressure perturbations do not necessarily vanish. But because a dark energy with w < -1 dominates only at very late times, and because the dark energy is not generally prone to gravitational clustering, then crossing the cosmological-constant boundary leaves no distinct imprint.

Affiliated with

Also associated with

No associations

Rating

Dark-Energy Evolution Across the Cosmological-Constant Boundary 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 Dark-Energy Evolution Across the Cosmological-Constant Boundary, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dark-Energy Evolution Across the Cosmological-Constant Boundary will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-342500