The potential of asteroseismology for probing the core chemical stratification in white dwarf stars

TL;DR

This study demonstrates that asteroseismology can effectively probe the core chemical stratification in white dwarf stars, even with limited observational data, by utilizing new modeling tools and understanding mode trapping effects.

Contribution

The paper introduces a new parameterization and modeling approach that enhances the ability to determine core chemical profiles in white dwarfs through asteroseismology.

Findings

Core chemical stratification can be precisely determined with limited modes.

Mode trapping effects significantly influence seismic sensitivity.

Success depends on the information content of the seismic data.

Abstract

Context. The details of the C/O core structure in white dwarf stars has mostly remained inaccessible to the technique of asteroseismology, despite several attempts carried out in the past. Aims. We re-assess the potential of asteroseismology for probing the chemical stratification in white dwarf cores, in light of new highly efficient tools recently developed for that purpose. Methods. Using the forward modeling approach and a new parameterization for the core chemical stratification in ZZ Ceti stars, we test several situations typical of the usually limited constraints available, such as small numbers of observed independent modes, to carry out asteroseismology of these stars. Results. We find that, even with a limited number of modes, the core chemical stratification (in particular, the location of the steep chemical transitions expected in the oxygen profile) can be determined quite precisely due to the significant sensitivity of some confined modes to partial reflexion (trapping) effects. These effects are similar to the well known trapping induced by the shallower chemical transitions at the edge of the core and at the bottom of the H-rich envelope. We also find that success to unravel the core structure depends on the information content of the available seismic data. In some cases, it may not be possible to isolate a unique, well-defined seismic solution and the problem remains degenerate. Conclusions. Our results establish that constraining the core chemical stratification in white dwarf stars based solely on asteroseismology is possible, an opportunity that we have started to exploit.