@Article{AraujoMarr:2009:GrWaBa,
               author = "Araujo, Jose 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",
              journal = "General Relativity and Gravitation",
                 year = "2009",
               volume = "41",
                pages = "1389--1406",
             keywords = "neutron stars, gravitational waves, strange matter, background.",
             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 
                         \νobs ~ 202,000 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 = "10.1007/s10714-008-0712-7",
                  url = "http://dx.doi.org/10.1007/s10714-008-0712-7",
                 issn = "0001-7701",
                label = "lattes: 6217296674061205 1 AraujoMarr:2009:GrWaBa",
             language = "en",
           targetfile = "10.1007_s10714-008-0712-7.pdf",
        urlaccessdate = "04 jun. 2024"
}