@Article{NunesVagKumDiVMen:2022:NeTeDa,
               author = "Nunes, Rafael da Costa and Vagnozzi, Sunny and Kumar, Suresh and 
                         Di Valentino, Eleonora and Mena, Olga",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {University 
                         of Cambridge} and {} and {University of Sheffield} and {University 
                         of Valencia}",
                title = "New tests of dark sector interactions from the full-shape galaxy 
                         power spectrum",
              journal = "Physical Review D",
                 year = "2022",
               volume = "105",
               number = "12",
                pages = "e123506",
                month = "June",
             abstract = "We explore the role of redshift-space galaxy clustering data in 
                         constraining nongravitational interactions between dark energy 
                         (DE) and dark matter (DM), for which state-of-the-art limits have 
                         so far been obtained from late-time background measurements. We 
                         use the joint likelihood for prereconstruction full-shape (FS) 
                         galaxy power spectrum and postreconstruction Baryon Acoustic 
                         Oscillation (BAO) measurements from the BOSS DR12 sample, 
                         alongside Cosmic Microwave Background (CMB) data from Planck: from 
                         this dataset combination we infer H0 1/4 68.02+0.49 and the 2?? 
                         lower limit ?? > ???0.12, among the strongest limits ever reported 
                         on the DM-DE coupling strength ?? for the particular model 
                         considered. Contrary to what has been observed for the ??CDM model 
                         and simple extensions thereof, we find that the CMB + FS 
                         combination returns tighter constraints compared to the CMB + BAO 
                         one, suggesting that there is valuable additional information 
                         contained in the broadband of the power spectrum. We test this 
                         finding by running additional CMB-free analyses and removing sound 
                         horizon information, and discuss the important role of the 
                         equality scale in setting constraints on DM-DE interactions. Our 
                         results reinforce the critical role played by redshift-space 
                         galaxy clustering measurements in the epoch of precision 
                         cosmology, particularly in relation to tests of nonminimal dark 
                         sector extensions of the ??CDM model.",
                  doi = "10.1103/PhysRevD.105.123506",
                  url = "http://dx.doi.org/10.1103/PhysRevD.105.123506",
                 issn = "1550-2368 and 1550-7998",
             language = "en",
           targetfile = "PhysRevD.105.123506.pdf",
        urlaccessdate = "25 jun. 2024"
}