摘要
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.
| 源语言 | 英语 |
|---|---|
| 页(从-至) | 7-15 |
| 页数 | 9 |
| 期刊 | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics |
| 卷 | 644 |
| 期 | 1 |
| DOI | |
| 出版状态 | 已出版 - 4 1月 2007 |
| 已对外发布 | 是 |
指纹
探究 'Observational H (z) data and cosmological models' 的科研主题。它们共同构成独一无二的指纹。引用此
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