Nonradial linear stability of liquid Lane-Emden stars
King Ming Lam

TL;DR
This paper analyzes the linear stability of liquid Lane-Emden stars under non-radial perturbations, showing stability in irrotational cases when radial modes are stable, but with limitations on controlling certain perturbation norms.
Contribution
It extends stability analysis of Lane-Emden stars to non-radial perturbations for liquid models, revealing conditions for stability and limitations on perturbation control.
Findings
Linear operator is non-negative for non-negative radial modes.
Infinite-dimensional kernel corresponds to linearly growing solutions.
Stability against non-radial irrotational perturbations when radial stability holds.
Abstract
The classical model of a star is the Lane-Emden star with dynamics governed by the Euler-Poisson equations. We consider the case of a liquid star with a "stiffened gas" equation of state . We derive the full 3D linearised Euler-Poisson system around liquid Lane-Emden stars with no symmetry assumptions on the perturbations and show that the associated linear operator is non-negative whenever the radial mode is non-negative. We show that has an infinite-dimensional kernel each element of which corresponds to a linearly growing solution to the linearised system. When restricted to irrotational perturbations and modding out the three kernel elements corresponding to momentum conservation, however, we prove that is strictly positive with coercivity bound $\langle\mathbf…
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Taxonomy
TopicsAdvanced Differential Geometry Research · Ocean Waves and Remote Sensing · Cosmology and Gravitation Theories
