Oscillations and instabilities of fast rotating neutron stars

Details Oscillations and instabilities of fast rotating neutron stars Oscillations and instabilities of fast rotating neutron stars

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009jphcs.189a2016g&link_type=abstract

Journal of Physics: Conference Series, Volume 189, Issue 1, pp. 012016 (2009).

Physics

Scientific paper

We present our results of our study of the oscillations and instabilities of rapidly rotating relativistic stars in the Cowling approximation. This is the first study of its kind and provides information on the effect of fast rotation on the oscillation spectra while it offers the possibility in studying the complete problem by including spacetime perturbations. Our study includes both axisymmetric and non-axisymmetric perturbations and provides limits for the onset of the secular bar mode rotational instability. We also present approximate formulae for the dependence of the oscillation spectrum from rotation. The results suggest that it is possible to extract the relativistic star's parameters from the observed gravitational wave spectrum.

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