Oscillations and instabilities in neutron stars with poloidal magnetic fields

TL;DR

This paper investigates the stability and oscillation modes of rotating, magnetized neutron stars with poloidal magnetic fields, revealing a poloidal-field instability and identifying Alfvén modes related to observed magnetar QPOs.

Contribution

It presents a self-consistent model of neutron star perturbations with multipolar poloidal fields, discovering a generic instability and hybrid oscillation modes.

Findings

Axial-led perturbations exhibit a poloidal-field instability near the neutral line.

Rotation mitigates the poloidal-field instability.

Identifies global Alfvén modes and hybrid modes in rotating magnetized stars.

Abstract

We study the time evolution of non-axisymmetric linear perturbations of a rotating magnetised neutron star, whose magnetic field is multipolar and purely poloidal. The background stellar configurations are generated self-consistently, allowing for distortions to the density distribution from rotational and magnetic forces. We find that the behaviour of axial-led perturbations is dominated by an instability generic to poloidal fields, which is localised around the `neutral line' where the background field vanishes. Rotation acts to reduce the effect of this instability. Polar-led perturbations do not appear to be unstable and in this case we find global Alfv\'en modes, whose restoring force is the magnetic field. In a rotating magnetised star there are no pure Alfv\'en modes or pure inertial modes, but hybrids of these. We discuss the nature of magnetic instabilities and oscillations in magnetars and pulsars, finding the dominant Alfv\'en mode has a frequency comparable with observed magnetar QPOs.