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Gravitational wave asteroseismology | University of Tübingen
uni-tuebingen.de
May Daniela D. Doneva, Erich Gaertig, Kostas D. Kokkotas and Christian Krüger. Fast rotating neutron stars can be destabilized by the so-called Chandrasekhar-Friedman-Schutz (CFS) instability, i.e. certain nonaxisymmetric oscillation modes can become unstable due to the emission of gravitational radiation for very high rotation rates of the star.
f-mode instability | Universität Tübingenuni-tuebingen.de › ...
uni-tuebingen.de
Erich Gaertig, Kostas Glampedakis, Kostas D. Kokkotas, Burkhard Zink. A classic result in gravitational physics is that pulsation modes in rotating compact stars ...
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