@Article{AllahyariNuneMota:2022:SlGrLi,
               author = "Allahyari, Alireza and Nunes, Rafael da Costa and Mota, David F.",
          affiliation = "{Institute for Research in Fundamental Sciences (IPM)} and 
                         {Instituto Nacional de Pesquisas Espaciais (INPE)} and {University 
                         of Oslo}",
                title = "No slip gravity in light of LISA standard sirens",
              journal = "Monthly Notices of the Royal Astronomical Society",
                 year = "2022",
               volume = "514",
               number = "1",
                pages = "1274--1281",
                month = "June",
             keywords = "gravitation, gravitational waves, cosmology: observations, dark 
                         energy.",
             abstract = "Standard sirens (SS) are the gravitational wave analogue of the 
                         astronomical standard candles, and can provide powerful 
                         information about the dynamics of the Universe up to very high z 
                         values. In this work, we generate three mock SS catalogues based 
                         on the merger of massive black hole binaries which are expected to 
                         be observed in the LISA operating frequency band. Then, we perform 
                         an analysis to test modifications of general relativity (GR) 
                         inspired by the no slip gravity framework. We find that in the 
                         best scenarios, we can constrain the free parameters which 
                         quantify deviations from GR to 21 per cent accuracy, while the 
                         Hubble parameter can be simultaneously fit to 6 per cent accuracy. 
                         In combination with CMB information, we find a 15 per cent 
                         accuracy on the modified gravity free parameters and 0.7 per cent 
                         accuracy on the Hubble parameter. The SS events at very large 
                         cosmological distances to be observed in LISA band will provide a 
                         unique way to test nature of gravity, but in the context of the 
                         analysis performed here, it will not be possible to distinguish 
                         the no slip gravity from GR.",
                  doi = "10.1093/mnras/stac1445",
                  url = "http://dx.doi.org/10.1093/mnras/stac1445",
                 issn = "0035-8711 and 1365-2966",
             language = "en",
           targetfile = "stac1445.pdf",
        urlaccessdate = "14 jun. 2024"
}