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@Article{EvangelistaAraś:2014:NeMe,
               author = "Evangelista, Edgard de Freitas Diniz and Ara{\'u}jo, Jos{\'e} 
                         Carlos Neves de",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)}",
                title = "The Gravitational Wave Background from Coalescing Compact 
                         Binaries: A New Method",
              journal = "Brazilian Journal of Physics",
                 year = "2014",
               volume = "44",
                pages = "824--831",
                 note = "{Setores de Atividade: Pesquisa e desenvolvimento 
                         cient{\'{\i}}fico.}",
             keywords = "Bin{\'a}rias Compactas, Fontes Astrof{\'{\i}}sicas de Ondas 
                         Gravitacionais, Fundos Cosmol{\'o}gicos de Ondas 
                         Gravitacionais.",
             abstract = "Gravitational waves are perturbations in the space-time that 
                         propagate at the speed of light. The study of such phenomenon is 
                         interesting because many cosmological processes and astrophysical 
                         objects, such as binary systems, are potential sources of 
                         gravitational radiation and can have their emissions detected in 
                         the near future by the next generation of interferometric 
                         detectors. Concerning the astrophysical objects, an interesting 
                         case is when there are several sources emitting in such a way that 
                         there is a superposition of signals, resulting in a smooth 
                         spectrum which spans a wide range of frequencies, the so-called 
                         stochastic background. In this paper, we are concerned with the 
                         stochastic backgrounds generated by compact binaries (i.e., binary 
                         systems formed by neutron stars and black holes) in the coalescing 
                         phase. In particular, we obtain such backgrounds by employing a 
                         new method developed in our previous studies.",
                  doi = "10.1007/s13538-014-0272-0",
                  url = "http://dx.doi.org/10.1007/s13538-014-0272-0",
                 issn = "0103-9733",
                label = "lattes: 6217296674061205 2 EvangelistaArau:2014:NeMe",
             language = "en",
        urlaccessdate = "24 nov. 2020"
}


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