@Article{EvangelistaArau:2013:NeMeCa,
author = "Evangelista, Edgard F. D. and Araujo, Jose Carlos Neves de",
affiliation = "{} and {Instituto Nacional de Pesquisas Espaciais (INPE)}",
title = "A new method to calculate the stochastic background of
gravitational waves generated by compact binaries",
journal = "Modern Physics Letters A",
year = "2013",
volume = "28",
number = "38",
pages = "1350174",
note = "{Setores de Atividade: Pesquisa e desenvolvimento
cient{\'{\i}}fico.}",
keywords = "Ondas Gravitacionais, Estrelas de Neutrons, Fundos
Cosmol{\'o}gicos de Ondas Gravitacionais, Gravitational waves,
stochastic background, double neutron stars.",
abstract = "In the study of gravitational waves (GWs), the stochastic
background generated by compact binary systems are among the most
important kinds of signals. The reason for such an importance has
to do with their probable detection by the interferometric
detectors [such as the Advanced LIGO (ALIGO) and Einstein
Telescope (ET)] in the near future. In this paper we are concerned
with, in particular, the stochastic background of GWs generated by
double neutron star (DNS) systems in circular orbits during their
periodic and quasi-periodic phases. Our aim here is to describe a
new method to calculate such spectra, which is based on an analogy
with a problem of Statistical Mechanics. Besides, an important
characteristic of our method is to consider the time evolution of
the orbital parameters.",
doi = "10.1142/S0217732313501745",
url = "http://dx.doi.org/10.1142/S0217732313501745",
issn = "0217-7323",
label = "lattes: 6217296674061205 2 EvangelistaArau:2013:NEMECA",
language = "en",
urlaccessdate = "27 abr. 2024"
}