@Article{EvangelistaArau:2014:StBaGr,
               author = "Evangelista, Edgard de Freitas Diniz and Araujo, Jose Carlos Neves 
                         de",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)}",
                title = "Stochastic Background of Gravitational Waves Generated by Compact 
                         Binary Systems",
              journal = "Brazilian Journal of Physics",
                 year = "2014",
               volume = "44",
               number = "2-3",
                pages = "260--270",
                month = "June",
                 note = "{Setores de Atividade: Pesquisa e desenvolvimento 
                         cient{\'{\i}}fico.}",
             keywords = "Bin{\'a}rias Compactas, Fontes Astrof{\'{\i}}sicas de Ondas 
                         Gravitacionais, Ondas Gravitacionais.",
             abstract = "Binary systems are the most studied sources of gravitational 
                         waves. The mechanisms of emission and the behavior of the orbital 
                         parameters are well known and can be written in analytic form in 
                         several cases. Besides, the strongest indication of the existence 
                         of gravitational waves has arisen from the observation of binary 
                         systems. On the other hand, when the detection of gravitational 
                         radiation becomes a reality, one of the observed pattern of the 
                         signals will be probably of stochastic background nature, which 
                         are characterized by a superposition of signals emitted by many 
                         sources around the universe. Our aim here is to develop an 
                         alternative method of calculating such backgrounds emitted by 
                         cosmological compact binary systems during their periodic or 
                         quasiperiodic phases. We use an analogy with a problem of 
                         statistical mechanics in order to perform this sum as well as 
                         taking into account the temporal variation of the orbital 
                         parameters of the systems. Such a kind of background is of 
                         particular importance since it could well form an important 
                         foreground for the planned gravitational wave interferometers 
                         DECI-Hertz Interferometer Gravitational wave Observatory (DECIGO), 
                         Big Bang Observer (BBO), Laser Interferometer Space Antenna (LISA) 
                         or Evolved LISA (eLISA), Advanced Laser Interferometer 
                         Gravitational-Wave Observatory (ALIGO), and Einstein Telescope 
                         (ET).",
                  doi = "10.1007/s13538-014-0178-x",
                  url = "http://dx.doi.org/10.1007/s13538-014-0178-x",
                 issn = "0103-9733",
                label = "lattes: 6217296674061205 2 EvangelistaArau:2014:StBaGr",
             language = "en",
        urlaccessdate = "25 abr. 2024"
}