@Article{PereiraMira:2010:MaBlHo,
author = "Pereira, Eduardo dos Santos and Miranda, Oswaldo Duarte",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)}",
title = "Massive black hole binary systems in hierarchial scenario of
structure formation",
journal = "International Journal of Modern Physics D",
year = "2010",
volume = "19",
pages = "1271",
month = "Sept.",
keywords = "massive black hole, structure formation, galaxies.",
abstract = "The hierarchical scenario of structure formation describes how
objects like galaxies and galaxy clusters are formed by mergers of
small objects. In this scenario, mergers of galaxies can lead to
the formation of massive black hole (MBH) binary systems. On the
other hand, the merger of two MBH could produce a gravitational
wave signal detectable, in principle, by the Laser Interferometer
Space Antenna (LISA). In the present work, we use the
Press?Schechter formalism, and its extension, to describe the
merger rate of haloes which contain massive black holes. Here, we
do not study the gravitational wave emission of these systems.
However, we present an initial study to determine the number of
systems formed via mergers that could permit, in a future
extension of this work, the calculation of the signature in
gravitational waves of these systems.",
doi = "10.1142/S0218271810017263",
url = "http://dx.doi.org/10.1142/S0218271810017263",
issn = "0218-2718",
label = "lattes: 3748594477326830 1 PereiraMira:2010:MABLHO",
language = "en",
url = "http://www.worldscinet.com/ijmpd/19/1908n10/S0218271810017263.html",
urlaccessdate = "11 maio 2024"
}