Holographic approach for dark energy - dark matter interaction in curved FLRW spacetime.
In this work we explore under the holographic approach the dark energy - dark matter interaction in a non-flat Friedmann-Lemaitre-Robertson-Walker spacetime, with a cut-off for the dark energy component given in terms of the Hubble scale. By considering a positive $Q$-term interaction and a specific parametrization for the coincidence parameter was found that the model admits a Type III future singularity therefore the crossing of the phantom divide is possible.
Publisher URL: http://arxiv.org/abs/1802.00097
DOI: arXiv:1802.00097v1
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