A Numerical Study of Normal Modes of Rotating Neutron Star Models by the Cowling Approximation
arXiv:astro-ph/9807254 · doi:10.1086/307012
Abstract
A numerical method of mode analysis of rapidly rotating relativistic stellar models by the Cowling approximation is applied to rotating neutron stars with realistic equations of state. For selected equations of state, eigenvalues and eigenfunctions of f-modes are numerically solved for stellar models from non-rotating to maximally rotating states. Neutral points of the lower order f-modes are determined as a function of the stellar rotational frequency. As in the polytropic case, we find that the bar mode can have neutral points for models with relatively strong gravity. The rotational frequency at the neutral point increases as the gravitational mass of the model becomes larger. As astrophysical applications of our analysis, we discuss the time scales of gravitational radiation induced instability and the possibility of the resonant excitation of f-modes during inspiraling motion of compact binary systems.
13 pages, 19 figures; 5 new figures are supplemented and some are re-drawn. Accepted for publication in ApJ
References in corpus (7)
- A new class of unstable modes of rotating relativistic stars
- Gravitational Radiation Instability in Hot Young Neutron Stars
- Gravitational radiation limit on the spin of young neutron stars
- Construction of Highly Accurate Models of Rotating Neutron Stars - Comparison of Three Different Numerical Schemes
- Nonaxisymmetric Neutral Modes in Rotating Relativistic Stars
- Quasi-normal modes of rotating relativistic stars - neutral modes for realistic equations of state
- Neutral Points of Oscillation Modes along Equilibrium Sequences of Rapidly Rotating Polytropes in General Relativity --- Application of The Cowling Approximation ---
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- Dynamical Bar Instability in Rotating Stars: Effect of General Relativity
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- General-relativistic treatment of tidal -mode resonances in coalescing binaries of neutron stars. I. Theoretical framework and crust breaking
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- Dynamics of Fast Rotating Neutron Stars: An Approach in the Hilbert Gauge
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