Asteroseismology of red giant stars: the potential of dipole modes

TL;DR

This paper discusses how dipole mixed modes in red giant stars, observed through space telescopes, can reveal details about their internal structure, core mixing, and angular momentum transport.

Contribution

It highlights the potential of dipole mixed modes in red giants to probe internal processes, advancing asteroseismic diagnostics.

Findings

Detection of non-radial oscillation modes in red giants.

Identification of mixed modes in G-K red giants.

Potential to study core mixing and angular momentum transport.

Abstract

Since the detection of non-radial solar-like oscillation modes in red giants with the CoRoT satellite, the interest in the asteroseismic properties of red giants and the link with their global properties and internal structure is increasing. Moreover, more and more precise data are being collected with the space-based telescopes CoRoT and {\it Kepler}. Particularly relevant has been the detection of mixed modes in a large number of G-K red giants. In this contribution we discuss the potential of these dipole mixed modes to provide information on core extra-mixing and transport of angular momentum.