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@InProceedings{MarranghelloAraś:2006:DeNeSt,
               author = "Marranghello, Guilherme F. and Ara{\'u}jo, Jos{\'e} Carlos 
                         Neves",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)}",
                title = "Determining the neutron star equation of state from gravitational 
                         wave detections",
            booktitle = "Anais...",
                 year = "2006",
         organization = "Reuni{\~a}o Anual da Sociedade Astron{\^o}mica Brasileira, 32.",
             abstract = "We briefly review the properties of quasi-normal modes of neutron 
                         stars and black holes. Specially addressing our study to the 
                         Brazilian spherical antenna, on which a possible detection would 
                         occur at 3.0-3.4 kHz, we analyze the consequences of a possible 
                         detection of such quasi-normal modes. Since the source can be 
                         identified, by its characteristic damping time, we are able to 
                         extract information about the neutron star or black hole. These 
                         informations lead to a strong constraint in the nuclear matter 
                         equation of state, namely, the compression modulus should be 
                         K»220MeV.",
  conference-location = "Atibaia, SP",
      conference-year = "30 jul - 03 ago",
                label = "self-archiving-INPE-MCTIC-GOV-BR",
             language = "pt",
         organisation = "Sociedade Astron{\^o}mica Brasileira",
           targetfile = "marranghello_determining.pdf",
        urlaccessdate = "24 jan. 2021"
}


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