The frequencies and damping times of neutron star (and quark star) oscillations have been computed using the most recent equations of state available in the literature. We find that some of the empirical relations that connect the frequencies and damping times of the modes to the mass and radius of the star, and that were previously derived in the literature, need to be modified. © 2005 American Institute of Physics.
Gravitational waves from neutron stars described by modern EOS / Benhar, O; Ferrari, Valeria; Gualtieri, Leonardo. - 751:(2005), pp. 211-213. (Intervento presentato al convegno 16th SIGRAV Conference on General Relativity and Gravitational Physics tenutosi a Vietri sul Mare; Italy nel 13-16 September 2004) [10.1063/1.1891555].
Gravitational waves from neutron stars described by modern EOS
FERRARI, Valeria;GUALTIERI, Leonardo
2005
Abstract
The frequencies and damping times of neutron star (and quark star) oscillations have been computed using the most recent equations of state available in the literature. We find that some of the empirical relations that connect the frequencies and damping times of the modes to the mass and radius of the star, and that were previously derived in the literature, need to be modified. © 2005 American Institute of Physics.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
