@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 = "23 abr. 2024"
}