@Article{ChirentiSilvAgui:2012:NoOsNe,
               author = "Chirenti, Cecilia and Silveira, Patrick R. and Aguiar, Odylio D.",
          affiliation = "Center for Mathematics, Computation and Cognition Federal 
                         University of ABC and {Instituto Nacional de Pesquisas Espaciais 
                         (INPE)} and {Instituto Nacional de Pesquisas Espaciais (INPE)}",
                title = "Non-Radial Oscillations of Neutron Stars and the Detection of 
                         Gravitational Waves",
              journal = "International Journal of Modern Physics: Conference Series",
                 year = "2012",
               volume = "18",
               number = "1",
                pages = "48--52",
             keywords = "neutron stars, oscillations, gravitational waves.",
             abstract = "We study the non-radial oscillations of relativistic neutron 
                         stars, in particular the (fundamental) f-modes, which are believed 
                         to be the most relevant for the gravitational wave emission of 
                         perturbed isolated stars. The expected frequencies of the f-modes 
                         are compared to the sensitivity range of Mario Schenberg, the 
                         Brazilian gravitational wave spherical detector.",
                  doi = "10.1142/S2010194512008185",
                  url = "http://dx.doi.org/10.1142/S2010194512008185",
                 issn = "2010-1945",
        urlaccessdate = "12 maio 2024"
}