The r-mode spectrum of relativistic neutron stars

Details The r-mode spectrum of relativistic neutron stars The r-mode spectrum of relativistic neutron stars

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001hell.confe.130r&link_type=abstract

"5th Hellenic Astronomical Conference, held 20-22 September, 2001 in Crete, Greece. Online at http://www.astro.auth.gr/elaset/he

Astronomy and Astrophysics

Astronomy

Scientific paper

I will present recent results on both time evolutions and mode calculations of perturbations of slowly rotating relativistic stars. I will mainly focus on the axial r-modes, where I show that at least to linear order in the rotation rate, r-modes do not exist for certain stellar models, quite in contrast to Newtonian predictions. In those cases where the r-modes exist, the growth times predicted by fully relativistic calculations agree very well with the Newtonian estimates.

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