%0 Journal Article
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%3 Excitation of neutron star f mode in low.pdf
%@dissemination WEBSCI; PORTALCAPES; COMPENDEX.
%2 sid.inpe.br/mtc-m16@80/2006/08.01.19.03.35
%4 sid.inpe.br/mtc-m16@80/2006/08.01.19.03
%X Neutron Stars (NSs) present a host of pulsation modes. Only a few of them, however, is of relevance from the gravitational wave (GW) point of view. Among the various possible modes the pulsation energy is mostly stored in the f-mode in which the fluid parameters undergo the largest changes. An important question is how the pulsation modes are excited in NSs. Here we consider the excitation of the f-mode in the accreting NSs belonging to Low Mass X-ray Binaries (LMXBs), which may well be a recurrent source of GWs, since the NSs are continuously receiving matter from their companion stars. We also discuss the detectability of the GWs for the scenario considered here.
%T Excitation of Neutron Star f-mode in Low Mass X-ray Binaries
%@secondarytype PRE PI
%@group DAS-INPE-MCT-BR
%@group DAS-INPE-MCT-BR
%@group DAS-INPE-MCT-BR
%@copyholder SID/SCD
%@secondarykey INPE-13924--PRE/9104
%@issn 1742-6588
%@affiliation Instituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica (INPE.DAS),
%@affiliation Instituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica (INPE.DAS),
%@affiliation Instituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica (INPE.DAS),
%B Journal of Physics: Conference Series
%P 1-5
%D 2006
%V 32
%A Araújo, José Carlos Neves de,
%A Miranda, Oswaldo Duarte,
%A Aguiar, Odylio Denys,
%@area CEA