Asymmetries of frequency splittings of dipolar mixed modes: a window on the topology of deep magnetic fields

TL;DR

This paper explores how asymmetries in frequency splittings of dipolar mixed modes in stars can reveal the geometry of deep magnetic fields, combining analytical methods with potential observational constraints.

Contribution

It provides analytical expressions linking mode asymmetries to magnetic field topologies, offering a new diagnostic tool for probing stellar core magnetism.

Findings

Asymmetry depends on the angle between magnetic and rotation axes.

Asymmetry cannot distinguish the relative strength of multiple magnetic components.

Negative asymmetry indicates non-axisymmetric magnetic topologies.

Abstract

Space asteroseismology is revolutionizing our knowledge of the internal structure and dynamics of stars. A breakthrough is ongoing with the recent discoveries of signatures of strong magnetic fields in the core of red giant stars. The key signature for such a detection is the asymmetry these fields induce in the frequency splittings of observed dipolar mixed gravito-acoustic modes. We investigate the ability of the observed asymmetries of the frequency splittings of dipolar mixed modes to constrain the geometrical properties of deep magnetic fields. We use the powerful analytical Racah-Wigner algebra used in Quantum Mechanics to characterize the geometrical couplings of dipolar mixed oscillation modes with various possible realistic fossil magnetic fields' topologies and compute the induced perturbation of their frequencies. First, in the case of an oblique magnetic dipole, we provide the exact analytical expression of the asymmetry as a function of the angle between the rotation and magnetic axes. Its value provides a direct measure of this angle. Second, considering a combination of axisymmetric dipolar and quadrupolar fields, we show how the asymmetry is blind to unravel the relative strength and sign of each component. Finally, in the case of a given multipole, we show that a negative asymmetry is a signature of non-axisymmetric topologies. Therefore, asymmetries of dipolar mixed modes provide key but only partial information on the geometrical topology of deep fossil magnetic fields. Asteroseismic constraints should therefore be combined with spectropolarimetric observations and numerical simulations, which aim to predict the more probable stable large-scale geometries.