Quasi-toroidal oscillations in rotating relativistic stars

TL;DR

This paper investigates quasi-toroidal oscillations in slowly rotating relativistic stars, revealing that their frequencies form a continuous spectrum influenced by relativistic effects, differing from Newtonian predictions.

Contribution

It provides a first-order relativistic analysis of r-mode oscillations, showing the spectrum's continuous nature and the impact of relativistic dragging on resonance conditions.

Findings

Oscillation frequencies form a continuous spectrum.

Relativistic dragging affects resonance conditions.

Frequencies differ from Newtonian predictions.

Abstract

Quasi-toroidal oscillations in slowly rotating stars are examined in the framework of general relativity. The oscillation frequency to first order of the rotation rate is not a single value even for uniform rotation unlike the Newtonian case. All the oscillation frequencies of the r-modes are purely neutral and form a continuous spectrum limited to a certain range. The allowed frequencies are determined by the resonance condition between the perturbation and background mean flow. The resonant frequency varies with the radius according to general relativistic dragging effect.