| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1850721 | Physics Letters B | 2015 | 7 Pages |
Abstract
Considering a quadratic parameterization of the dark energy density, we explore signatures of evolution using data from gas mass fraction in clusters, type Ia supernova, BAO and CMB. We find – excluding CMB data – a preference for an evolution of ρde(z)ρde(z) towards smaller values as the redshift increases, a result consistent with a recent study using the BAO DR11 data by Delubac et al. (2015).
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
Víctor H. Cárdenas,