@Article{BachegaCostAbdaForn:2020:FoInDa,
               author = "Bachega, Riis R. A. and Costa, Andr{\'e} A. and Abdalla, E. and 
                         Fornazier, Karin Silva Franzoni",
          affiliation = "{Universidade de S{\~a}o Paulo (USP)} and {Yangzhou University} 
                         and {Universidade de S{\~a}o Paulo (USP)} and {Instituto Nacional 
                         de Pesquisas Espaciais (INPE)}",
                title = "Forecasting the interaction in dark matter-dark energy models with 
                         standard sirens from the Einstein telescope",
              journal = "Journal of Cosmology and Astroparticle Physics",
                 year = "2020",
               volume = "5",
                pages = "e021",
                month = "May",
             keywords = "dark energy theory, gravitational wave detectors, gravitational 
                         waves / sources, gravitational waves / theory.",
             abstract = "Gravitational Waves (GW's) can determine the luminosity distance 
                         of the progenitor directly from the amplitude of the wave, without 
                         assuming any specific cosmological model. Thus, it can be 
                         considered as a standard siren. The coalescence of binary neutron 
                         stars (BNS) or neutron star-black hole pair (NSBH) can generate 
                         GW's as well as the electromagnetic counterpart, which can be 
                         detected in a form of Gamma-Ray Bursts (GRB) and can be used to 
                         determine the redshift of the source. Consequently, such a 
                         standard siren can be a very useful probe to constrain the 
                         cosmological parameters. In this work, we consider an interacting 
                         Dark Matter-Dark Energy (DM-DE) model. Assuming some fiducial 
                         values for the parameters of our model, we simulate the luminosity 
                         distance for a {"}realistic{"} and {"}optimistic{"} GW+GRB events 
                         , which can be detected by the third-generation GW detector 
                         Einstein Telescope (ET). Using these simulated events, we perform 
                         a Monte Carlo Markov Chain (MCMC) to constrain the DM-DE coupling 
                         constant and other model parameters in 1 sigma and 2 sigma 
                         confidence levels. We also investigate how GW's can improve the 
                         constraints obtained by current cosmological probes.",
                  doi = "10.1088/1475-7516/2020/05/021",
                  url = "http://dx.doi.org/10.1088/1475-7516/2020/05/021",
                 issn = "1475-7516",
             language = "en",
           targetfile = "bachega_forecasting.pdf",
        urlaccessdate = "27 abr. 2024"
}