Linear Stability Analysis of Differentially Rotating Polytropes -- New results for the m = 2 f-mode dynamical instability --
arXiv:astro-ph/0304299 · doi:10.1086/375768
Abstract
We have studied the -mode oscillations of differentially rotating polytropes by making use of the linear stability analysis. We found that the critical values of where the dynamical instability against the -mode oscillations sets in decrease down to as the degree of differential rotation becomes higher. Here is an azimuthal mode number and and are the rotational energy and the gravitational potential energy, respectively. This tendency is almost independent of the compressibility of the polytropes. These are the {\it first exact results} of the linear stability analysis for the occurrence of the dynamical instability against the -modes.
8 pages, 8 figures, accepted to ApJ
References in corpus (11)
- Simulation of merging binary neutron stars in full general relativity: case
- Relativistic simulations of rotational core collapse. II. Collapse dynamics and gravitational radiation
- Collapse of a Molecular Cloud Core to Stellar Densities: The First Three-Dimensional Calculations
- The bar-mode instability in differentially rotating neutron stars: Simulations in full general relativity
- Dynamical instability of differentially rotating stars
- Dynamical Rotational Instability at Low
- Models of Rapidly Rotating Neutron Stars: Remnants of Accretion Induced Collapse
- Dynamical instability of new-born neutron stars as sources of gravitational radiation
- R-mode oscillations of differentially and rapidly rotating Newtonian polytropic stars
- Gravitational Waves from the Dynamical Bar Instability in a Rapidly Rotating Star
- R-mode oscillations of rapidly rotating Newtonian stars - A new numerical scheme and its application to the spin evolution of neutron stars
Cited by in corpus (19)
- Accurate simulations of the dynamical bar-mode instability in full General Relativity
- The nature of low T/|W| dynamical instabilities in differentially rotating stars
- The rotational modes of relativistic stars: Numerical results
- Dynamical non-axisymmetric instabilities in rotating relativistic stars
- Axisymmetric collapse simulations of rotating massive stellar cores in full general relativity: Numerical study for prompt black hole formation
- Insights into non-axisymmetric instabilities in three-dimensional rotating supernova models with neutrino and gravitational-wave signatures
- Nonlinear Development of the Secular Bar-mode Instability in Rotating Neutron Stars
- Numerical evolution of secular bar-mode instability induced by the gravitational radiation reaction in rapidly rotating neutron stars
- Magnetic Braking in Differentially Rotating, Relativistic Stars
- Stiffness effects on the dynamics of the bar-mode instability of Neutron Stars in full General Relativity
- Neutron Star instabilities in full General Relativity using a ideal fluid
- On a role of corotation radius in the low dynamical instability of differentially rotating stars
- Unstable normal modes of low T/W dynamical instabilities in differentially rotating stars
- Magnetized stars with differential rotation and a differential toroidal field
- The Kinematic Richness of Star Clusters - II. Stability of Spherical Anisotropic Models with Rotation
- Gravitational wave content and stability of uniformly, rotating, triaxial neutron stars in general relativity
- Impacts of zonal winds on planetary oscillations and Saturn ring seismology
- Determining the stiffness of the equation of state using low T/W dynamical instabilities in differentially rotating stars
- Pseudo-Newtonian Models for the Equilibrium Structures of Rotating Relativistic Stars