Constraints on dark energy evolution

TL;DR

This study constrains dark energy models with rapid equation of state transitions using combined cosmological data, finding no evidence for such transitions at high redshifts and confirming the robustness of fundamental parameters.

Contribution

It introduces a method to constrain high-redshift dark energy transitions by combining SN Ia, CMB, and galaxy power spectrum data, showing these transitions are strongly disfavored.

Findings

Transitions at high redshift are strongly rejected.

Fundamental cosmological parameters are well constrained regardless of transitions.

No current data favors the existence of a rapid dark energy transition.

Abstract

We investigate a class of dark energy models in which the equation of state undergoes a rapid transition and for which the Hubble SN Ia diagram is known to be poorly discriminant. Interestingly enough, we find that transitions at high redshift can lead to distortion in the correlation function of dark matter at lower redshift. We therefore use a combination of the SN Ia Hubble diagram, Cosmic Microwave Background data and power spectrum from the Sloan Digital Sky Survey Luminous Red Galaxies (SDSS LRG) to constrain the redshift of a possible transition. We find that the fundamental cosmological parameters are well constrained independently of the presence of a transition. Acceptable transitions from an equation of state close to $w = 0$ to a value close to -1 are strongly rejected at redshifts much higher than those for which Large Scale Structure and SN Ia data are available: the transition redshift can be rejected up to a value as high as 10. We conclude that no preference for a transition appears from present-day data.