| Texto completo | |
| Autor(es): |
de Araujo, J. C. N.
;
Miranda, O. D.
;
Aguiar, O. D.
;
Mio, N
Número total de Autores: 4
|
| Tipo de documento: | Artigo Científico |
| Fonte: | WAKE CONFERENCE 2021; v. 32, p. 5-pg., 2006-01-01. |
| Resumo | |
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. (AU) | |
| Processo FAPESP: | 98/13468-9 - O detector Schenberg: proposta para o projeto, construção e operação de um detector de ondas gravitacionais esferoidal de 0.6 metros de diâmetro |
| Beneficiário: | Odylio Denys de Aguiar |
| Modalidade de apoio: | Auxílio à Pesquisa - Regular |