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On the r-mode spectrum of relativistic stars
Authors:Horst R Beyer  Kostas D Kokkotas
Institution:Universität Stuttgart, Institut A für Mechanik, Pfaffenwaldring 9, D-70550 Stuttgart, Germany; Department of Physics, Aristotle University of Thessaloniki, Thessaloniki 54006, Greece; Max Planck Institute for Gravitational Physics, The Albert Einstein Institute, D-14473 Potsdam, Germany
Abstract:We present a mathematically rigorous proof that the r-mode spectrum of relativistic stars to the rotational lowest order has a continuous part. A rigorous definition of this spectrum is given in terms of the spectrum of a continuous linear operator. This study verifies earlier results by Kojima concerning the nature of the r-mode spectrum.
Keywords:stars: neutron  stars: oscillations  stars: rotation
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