@Article{GariazzoDiVaMenaNune:2022:LaInCo,
               author = "Gariazzo, Stefano and Di Valentino, Eleonora and Mena, Olga and 
                         Nunes, Rafael da Costa",
          affiliation = "{Istituto Nazionale di Fisica Nucleare (INFN)} and {University of 
                         Sheffield} and {Universidad de Valencia-CSIC} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)}",
                title = "Late-time interacting cosmologies and the Hubble constant 
                         tension",
              journal = "Physical Review D",
                 year = "2022",
               volume = "106",
               number = "2",
                pages = "e023530",
                month = "July",
             abstract = "In this manuscript we reassess the potential of interacting dark 
                         matter-dark energy models in solving the Hubble constant tension. 
                         These models have been proposed but also questioned as possible 
                         solutions to the H0 problem. Here we examine several interacting 
                         scenarios against cosmological observations, focusing on the 
                         important role played by the calibration of supernovae data. In 
                         order to reassess the ability of interacting dark matter-dark 
                         energy scenarios in easing the Hubble constant tension, we 
                         systematically confront their theoretical predictions using a 
                         prior on the supernovae Ia absolute magnitude MB, which has been 
                         argued to be more robust and certainly less controversial than 
                         using a prior on the Hubble constant H0. While some data 
                         combinations do not show any preference for interacting dark 
                         sectors and in some of these scenarios the clustering \σ8 
                         tension worsens, interacting cosmologies with a dark energy 
                         equation of state w<-1 are preferred over the canonical 
                         \ΛCDM picture even with cosmic microwave background data 
                         alone and also provide values of \σ8 in perfect agreement 
                         with those from weak lensing surveys. Future cosmological surveys 
                         will test these exotic dark energy cosmologies by accurately 
                         measuring the dark energy equation of state and its putative 
                         redshift evolution.",
                  doi = "10.1103/PhysRevD.106.023530",
                  url = "http://dx.doi.org/10.1103/PhysRevD.106.023530",
                 issn = "1550-2368 and 1550-7998",
             language = "en",
           targetfile = "PhysRevD.106.023530.pdf",
        urlaccessdate = "20 maio 2024"
}