@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 = "03 jun. 2024"
}