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Astrophysics > Cosmology and Nongalactic Astrophysics

arXiv:1608.04545 (astro-ph)
[Submitted on 16 Aug 2016 ]

Title: Constraining interacting dark energy models with latest cosmological observations

Title: 用最新宇宙学观测约束相互作用暗能量模型

Authors:Dong-Mei Xia, Sai Wang
Abstract: The local measurement of $H_0$ is in tension with the prediction of $\Lambda$CDM model based on the Planck data. This tension may imply that dark energy is strengthened in the late-time Universe. We employ the latest cosmological observations on CMB, BAO, LSS, SNe, $H(z)$ and $H_0$ to constrain several interacting dark energy models. Our results show no significant indications for the interaction between dark energy and dark matter. The $H_0$ tension can be moderately alleviated, but not totally released.
Abstract: 局部测量的$H_0$与基于普朗克数据的$\Lambda$冷暗物质模型的预测存在矛盾。 这种矛盾可能意味着在宇宙晚期,暗能量得到了加强。 我们利用最新的宇宙学观测数据,包括宇宙微波背景辐射(CMB)、重子声学振荡(BAO)、大尺度结构(LSS)、超新星(SNe)、$H(z)$和$H_0$来约束几种相互作用的暗能量模型。 我们的结果表明,暗能量与暗物质之间没有显著的相互作用迹象。 $H_0$的矛盾可以得到一定程度的缓解,但不会完全消除。
Comments: 6 pages, 4 tables, 2 figures. Version to appear at MNRAS
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
Cite as: arXiv:1608.04545 [astro-ph.CO]
  (or arXiv:1608.04545v1 [astro-ph.CO] for this version)
  https://doi.org/10.48550/arXiv.1608.04545
arXiv-issued DOI via DataCite
Journal reference: Mon.Not.Roy.Astron.Soc. 463 (2016) no.1, 952-956
Related DOI: https://doi.org/10.1093/mnras/stw2073
DOI(s) linking to related resources

Submission history

From: Sai Wang [view email]
[v1] Tue, 16 Aug 2016 10:34:31 UTC (96 KB)
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