@Article{AraujoMiraAgui:2004:GrWaBa,
author = "de Araujo, Jos{\'e} C. N. and Miranda, Oswaldo D. and Aguiar,
Odylio D.",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Tecnol{\'o}gico de Aeron{\'a}utica} and {Instituto Nacional de
Pesquisas Espaciais (INPE)}",
title = "Gravitational wave background from black holes of the Springel \&
Hernquist star formation epoch",
journal = "Monthly Notices of the Royal Astronomical Society",
year = "2004",
volume = "348",
number = "4",
pages = "1373--1378",
keywords = "black hole physics, gravitation, gravitational waves, cosmology.",
abstract = "We study the generation of a stochastic gravitational wave (GW)
background produced from a population of core-collapse supernovae,
which form black holes in scenarios of structure formation. In
particular, we take into account in the present paper the history
of star formation derived by Springel \& Hernquist, who employed
hydrodynamic simulations of structure formation in a cold dark
matter (CDM) cosmology. In addition, and contrary to previous
studies, we consider the effect of taking into account different
values of the alpha parameter, the fraction of the progenitor mass
which forms the black hole. Different values of alpha imply
different frequency bands for the GWs produced. Because the
sensitivity of the GW detectors depends on the frequency of the
GWs, it is worth studying the influence of alpha on the detection
of the background considered here. We then study the detectability
of the GW background produced in scenarios such as those studied
here and discuss what astrophysical information could be obtained
from a positive or even negative detection of such a putative
background. In particular, we show that the formation of a
pre-galactic population of black holes could have generated a
stochastic GW background that should be detected in the future by
correlating signals of a pair of advanced LIGO observatories (LIGO
III) at a signal-to-noise ratio greater than unity, if alpha >
0.5.",
doi = "10.1111/j.1365-2966.2004.07459.x",
url = "http://dx.doi.org/10.1111/j.1365-2966.2004.07459.x",
issn = "1365-2966",
language = "en",
targetfile = "j.1365-2966.2004.07459.x.pdf",
urlaccessdate = "28 abr. 2024"
}