Abstract
In this work, we confront ten cosmological models with observational H (z) data. The possible interaction between dark energy and dust matter is allowed in some of these models. Also, we consider the possibility of (effective) equation-of-state parameter (EoS) crossing -1. We find that the best models have an oscillating feature for both H (z) and EoS, with the EoS crossing -1 around redshift z ∼ 1.5.
| Original language | English |
|---|---|
| Pages (from-to) | 7-15 |
| Number of pages | 9 |
| Journal | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics |
| Volume | 644 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - 4 Jan 2007 |
| Externally published | Yes |