@Article{YangVaDiNuPaMo:2019:LiSoDa,
               author = "Yang, Weiqiang and Vagnozzi, Sunny and Di Valentino, Eleonora and 
                         Nunes, Rafael da Costa and Pan, Supriya and Mota, David F.",
          affiliation = "{Liaoning Normal University} and {Stockholm University} and 
                         {University of Manchester} and {Instituto Nacional de Pesquisas 
                         Espaciais (INPE)} and {Presidency University} and {University of 
                         Oslo}",
                title = "Listening to the sound of dark sector interactions with 
                         gravitational wave standard sirens",
              journal = "Journal of Cosmology and Astroparticle Physics",
                 year = "2019",
               volume = "7",
                pages = "e037",
                month = "July",
             keywords = "cosmological simulations, dark energy theory, dark matter theory, 
                         gravitational waves / theory.",
             abstract = "We consider two stable Interacting Dark Matter-Dark Energy models 
                         and confront them against current Cosmic Microwave Background data 
                         from the Planck satellite. We then generate luminosity distance 
                         measurements from O(10(3)) mock Gravitational Wave events matching 
                         the expected sensitivity of the proposed Einstein Telescope. We 
                         use these to forecast how the addition of Gravitational Wave 
                         standard sirens data can improve current limits on the Dark 
                         Matter-Dark Energy coupling strength (xi). We find that the 
                         addition of Gravitational Waves data can reduce the current 
                         uncertainty by a factor of 5. Moreover, if the underlying 
                         cosmological model truly features Dark Matter-Dark Energy 
                         interactions with a value of xi within the currently allowed 1 
                         sigma upper limit, the addition of Gravitational Wave data would 
                         help disentangle such an interaction from the standard case of no 
                         interaction at a significance of more than 3 sigma.",
                  doi = "10.1088/1475-7516/2019/07/037",
                  url = "http://dx.doi.org/10.1088/1475-7516/2019/07/037",
                 issn = "1475-7516",
             language = "en",
           targetfile = "yang_listening.pdf",
        urlaccessdate = "27 abr. 2024"
}