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Constraining interacting dark energy models with latest cosmological observations

The local measurement of $H_0$ is in tension with the prediction of $Λ$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.

preprint2016arXivOpen access
Dong-Mei XiaSai Wang
astro-ph.CO
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Open access2 authors1 topic
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Dong-Mei XiaSai Wang

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