@Article{NunesDiVa:2021:DaSeIn,
               author = "Nunes, Rafael da Costa and Di Valentino, Eleonora",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Durham 
                         University}",
                title = "Dark sector interaction and the supernova absolute magnitude 
                         tension",
              journal = "Physical Review D",
                 year = "2021",
               volume = "104",
               number = "6",
                pages = "e063529",
                month = "Sept.",
             abstract = "It has been intensively discussed if modifications in the dynamics 
                         of the Universe at late times are able or not able to solve the H0 
                         tension. On the other hand, it has also been argued that the H0 
                         tension is actually a tension on the supernova absolute magnitude 
                         MB. In this work, we robustly constrain MB using Pantheon 
                         supernovae Ia sample, baryon acoustic oscillations, and big bang 
                         nucleosynthesis data, and assess the MB tension by comparing three 
                         theoretical models, namely the standard \ΛCDM, the wCDM, and 
                         a nongravitational interaction between dark energy (IDE) and dark 
                         matter. We find that the IDE model can solve the MB tension with a 
                         coupling different from zero at 95% CL, confirming the results 
                         obtained using a H0 prior.",
                  doi = "10.1103/PhysRevD.104.063529",
                  url = "http://dx.doi.org/10.1103/PhysRevD.104.063529",
                 issn = "1550-2368 and 1550-7998",
             language = "en",
           targetfile = "nunes_dark.pdf",
        urlaccessdate = "12 jun. 2024"
}