Fast Rotating Relativistic Stars: Spectra and Stability without Approximation
Author:
Funder
Deutsche Forschungsgemeinschaft
National Science Foundation
Publisher
American Physical Society (APS)
Subject
General Physics and Astronomy
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevLett.125.111106/fulltext
Reference50 articles.
1. Non-Radial Pulsation of General-Relativistic Stellar Models. I. Analytic Analysis for L ≥ 2
2. Nonradial Pulsation of General-Relativistic Stellar Models. III. Analytic and Numerical Results for Neutron Stars
3. Solutions of Two Problems in the Theory of Gravitational Radiation
4. Gravitational radiation instability in rotating stars
5. Secular instability of rotating Newtonian stars
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