@Article{AraujoMarr:2008:GrWaBa,
author = "Araujo, Jos{\'e} Carlos Neves de and Marranghello, Guilherme F.",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and
{Universidade Federal do Pampa}",
title = "Gravitational wave background from neutron star phase transition
for a new class of equation of state",
journal = "Journal of Physics: Conference Series",
year = "2008",
volume = "122",
pages = "012041",
note = "{7th Edoardo Amaldi Conference on Gravitational Waves (Amaldi7)}",
keywords = "gravitational radiation detectors, mass spectrometers, neutron
star.",
abstract = "We study the generation of a stochastic gravitational wave (GW)
background produced by a population of neutron stars (NSs) which
go over a hadron-quark phase transition in its inner shells. We
obtain, for example, that the NS phase transition, in cold dark
matter scenarios, could generate a stochastic GW background with a
maximum amplitude of hBG ~ 10^-24, in the frequency band ~ 20 -
2000 Hz for stars forming at redshifts of up to z ~ 20: We study
the possibility of detection of this isotropic GW background by
correlating signals of a pair of 'advanced' LIGO observatories.",
doi = "10.1088/1742-6596/122/1/012041",
url = "http://dx.doi.org/10.1088/1742-6596/122/1/012041",
issn = "1742-6588",
label = "lattes: 6217296674061205 1 AraujoMarr:2008:GrWaBa",
language = "pt",
targetfile = "1742-6596_122_1_012041.pdf",
url = "http://iopscience.iop.org/1742-6596/122/1/012041",
urlaccessdate = "01 maio 2024"
}