2018/04/30 by Daniela Grandon, Victor H. Cardenas · 1 citation
Physics and Astronomy · #astro-ph.CO #gr-qc
paper · pdf · doi:10.1007/s10714-019-2526-1
16 pages, 3 figures. arXiv admin note: text overlap with arXiv:0803.0982 by other authors
arxiv created 2018/10/19 · arxiv updated 2019/03/20
In this work we use the latest observations on SNIa, H(z), BAO, fgas in clusters and CMBR, to constrain three models showing an explicit interaction between dark matter and dark energy. In particular, we use the BOSS BAO measurements at z ≃ 0.32, 0.57 and 2.34, using the full 2-dimensional constraints on the angular and line of sight BAO scale. We find that using all five observational probes together, two of the interaction models show positive evidence at more than 3 σ. Although significant, further study is needed to establish this statement firmly.