Period spacings in red giants I. Disentangling rotation and revealing core structure discontinuities

TL;DR

This paper introduces a method to disentangle rotation effects from mixed-mode spacings in red giant stars, enabling automated analysis of core structures and rotational splittings from asteroseismic data.

Contribution

It develops an analytical approach and a new visualization technique using stretched periods to accurately measure period spacings and rotational splittings in complex mixed-mode patterns.

Findings

Effective separation of rotational splittings from mixed-mode spacings.

Automated measurement of asymptotic period spacing.

Enhanced detection of buoyancy glitches in stellar cores.

Abstract

Asteroseismology allows us to probe the physical conditions inside the core of red giant stars. This relies on the properties of the global oscillations with a mixed character that are highly sensitive to the physical properties of the core. However, overlapping rotational splittings and mixed-mode spacings result in complex structures in the mixed-mode pattern, which severely complicates its identification and the measurement of the asymptotic period spacing. This work aims at disentangling the rotational splittings from the mixed-mode spacings, in order to open the way to a fully automated analysis of large data sets. An analytical development of the mixed-mode asymptotic expansion is used to derive the period spacing between two consecutive mixed modes. The \'echelle diagrams constructed with the appropriately stretched periods are used to exhibit the structure of the gravity modes and of the rotational splittings. We propose a new view on the mixed-mode oscillation pattern based on corrected periods, called stretched periods, that mimic the evenly spaced gravity-mode pattern. This provides a direct understanding of all oscillation components, even in the case of rapid rotation. The measurement of the asymptotic period spacing and the signature of the structural glitches on mixed modes are then made easy. This work opens the possibility to derive all seismic global parameters in an automated way, including the identification of the different rotational multiplets and the measurement of the rotational splitting, even when this splitting is significantly larger than the period spacing. Revealing buoyancy glitches provides a detailed view on the radiative core.