@AudiovisualMaterial{EvangelistaAraś:2010:StBaGr,
abstract = "Binary Systems are the the most studied sources of gravitational
radiation, both theoretically and observationally. Theoretically,
the mechanisms of emission and the behaviuor of the orbital
parameters are well known and can be written in analytic form in
several cases, which is a great advantage in terms of
computational work; observationally, even though gravitational
waves have not been detected yet, the strongest indication of the
its existence have arisen from the observation of binary systems,
more specifically the Hulse-Taylor binary pulsar. When one begins
to detect gravitational radiation, one of the observed pattern of
the signals will probably be of stochastic background nature
because there will be a superposition of the signals emited by a
plenty of sources around the Universe. So, our task here is to
develop a method for summing the gravitational waves emited by
cosmological binary compact systems in order to find out the shape
of the spectra, that is, we will develop a method for obtaining
the stochastic background generated by these systems. We use here
an analogy with a problem of statistical mechanics in order to
perform this sum, besides taking into account the temporal
variation of the orbital parameters of the systems..",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)}",
author = "Evangelista, Edgard de Freitas Diniz and Ara{\'u}jo, Jos{\'e}
Carlos Neves de",
city = "Sao Jos{\'e} dos Campos",
conferencename = "Workshop da P{\'o}s-Gradua{\c{c}}{\~a}o, (DAS/INPE).",
date = "17 - 18 Nov. 2010",
language = "pt",
publisher = "Instituto Nacional de Pesquisas Espaciais",
publisheraddress = "S{\~a}o Jos{\'e} dos Campos",
ibi = "8JMKD3MGP7W/3958U4B",
url = "http://urlib.net/rep/8JMKD3MGP7W/3958U4B",
title = "Stochastic background of gravitational waves generated by compact
binary systems",
year = "2010",
urlaccessdate = "22 jan. 2021"
}