@Article{FillouxPachDuriArau:2011:DeRaLI,
               author = "Filloux, C. H. and Pacheco, J. A. de Freitas and Durier, F. and 
                         Araujo, Jos{\'e} Carlos Neves de",
          affiliation = "Univ Nice Sophia Antipolis, Observ Cote Azur, Lab Cassiopee and 
                         Univ Nice Sophia Antipolis, Observ Cote Azur, Lab Cassiopee and 
                         Max Planck Inst Extraterr Phys, D-85748 Garching, Germany and 
                         {Instituto Nacional de Pesquisas Espaciais (INPE)}",
                title = "Coalescence Rate of Supermassive Black Hole Binaries derived from 
                         cosmolgical simulations: Detection rates for LISA and ET",
              journal = "International Journal of Modern Physics D",
                 year = "2011",
               volume = "20",
               number = "12",
                pages = "2399--2417",
                month = "Nov",
             keywords = "Gravitational waves, supermassive black holes, cosmological 
                         simulations.",
             abstract = "The coalescence history of massive black holes has been derived 
                         from cosmological simulations, in which the evolution of those 
                         objects and that of the host galaxies are followed in a consistent 
                         way. The present study indicates that supermassive black holes 
                         having masses greater than similar to 10(9) M(circle dot) 
                         underwent up to 500 merger events along their history. The derived 
                         coalescence rate per comoving volume and per mass interval 
                         permitted to obtain an estimate of the expected detection rate 
                         distribution of gravitational wave signals ({"}ring-down{"}) along 
                         frequencies accessible by the planned interferometers either in 
                         space (LISA) or in the ground (Einstein). For LISA, in its 
                         original configuration, a total detection rate of about 15 yr(-1) 
                         is predicted for events having a signal-to-noise ratio equal to 
                         10, expected to occur mainly in the frequency range 4-9mHz. For 
                         the Einstein gravitational wave telescope, one event each 14 
                         months down to one event each four years is expected with a 
                         signal-to-noise ratio of 5, occurring mainly in the frequency 
                         interval 10-20Hz. The detection of these gravitational signals and 
                         their distribution in frequency would be in the future an 
                         important tool able to discriminate among different scenarios 
                         explaining the origin of supermassive black holes.",
                  doi = "10.1142/S0218271811020433",
                  url = "http://dx.doi.org/10.1142/S0218271811020433",
                 issn = "0218-2718",
             language = "en",
        urlaccessdate = "16 jun. 2024"
}