Daniela GrandónCárdenas, VíctorVíctorCárdenas2025-12-062025-12-062019-03-0110.1007/s10714-019-2526-12-s2.0-85063111083https://cris-uv-2.scimago.es/handle/123456789/6974WOS:000461155900002In this work we use the latest observations on SNIa, H(z), BAO, f gas 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.enacceso abiertoAstronomy And AstrophysicsPhysics, MultidisciplinaryPhysics, Particles And FieldsPhysics And Astronomyarticle