The Tayler instability at low magnetic Prandtl numbers: Chiral symmetry breaking and synchronizable helicity oscillations

TL;DR

This paper investigates the Tayler instability at low magnetic Prandtl numbers, revealing chiral symmetry breaking and oscillations in the alpha effect that could influence stellar magnetic field generation and liquid metal battery stability.

Contribution

It introduces the concept of intrinsic oscillations of the alpha effect in the Tayler instability at low magnetic Prandtl numbers, linking these oscillations to dynamo models and planetary tidal influences.

Findings

Intrinsic alpha oscillations at low magnetic Prandtl numbers.

Synchronized dynamo model based on alpha oscillations.

Potential link between planetary tides and stellar dynamo cycles.

Abstract

The current-driven, kink-type Tayler instability (TI) is a key ingredient of the Tayler-Spruit dynamo model for the generation of stellar magnetic fields, but is also discussed as a mechanism that might hamper the up-scaling of liquid metal batteries. Under some circumstances, the TI involves a helical flow pattern which goes along with some alpha effect. Here we focus on the chiral symmetry breaking and the related impact on the alpha effect that would be needed to close the dynamo loop in the Tayler-Spruit model. For low magnetic Prandtl numbers, we observe intrinsic oscillations of the alpha effect. These oscillations serve then as the basis for a synchronized Tayler-Spruit dynamo model, which could possibly link the periodic tidal forces of planets with the oscillation periods of stellar dynamos.