Detectability of f-mode Unstable Neutron Stars by the Schenberg Spherical Antenna

J. C. N. de Araujo, O. D. Miranda, O. D. Aguiar

The Brazilian spherical antenna (Schenberg) is planned to detect high frequency gravitational waves (GWs) ranging from 3.0 kHz to 3.4 kHz. There is a host of astrophysical sources…