Issue |
A&A
Volume 659, March 2022
|
|
---|---|---|
Article Number | A53 | |
Number of page(s) | 6 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361/202142666 | |
Published online | 04 March 2022 |
Local heating due to convective overshooting and the solar modelling problem
1
University of Exeter, Physics and Astronomy, EX4 4QL Exeter, UK
e-mail: i.baraffe@ex.ac.uk
2
École Normale Supérieure, Lyon, CRAL (UMR CNRS 5574), Université de Lyon, France
3
Department of Physics and Astronomy, Georgia State University, Atlanta, GA 30303, USA
4
Centre for Fusion, Space and Astrophysics, Department of Physics, University of Warwick, Coventry CV4 7AL, UK
Received:
15
November
2021
Accepted:
22
December
2021
Recent hydrodynamical simulations of convection in a solar-like model suggest that penetrative convective flows at the boundary of the convective envelope modify the thermal background in the overshooting layer. Based on these results, we implement in one-dimensional stellar evolution codes a simple prescription to modify the temperature gradient below the convective boundary of a solar model. This simple prescription qualitatively reproduces the behaviour found in the hydrodynamical simulations, namely a local heating and smoothing of the temperature gradient below the convective boundary. We show that introducing local heating in the overshooting layer can reduce the sound-speed discrepancy usually reported between solar models and the structure of the Sun inferred from helioseismology. It also affects key quantities in the convective envelope, such as the density, the entropy, and the speed of sound. These effects could help reduce the discrepancies between solar models and observed constraints based on seismic inversions of the Ledoux discriminant. Since mixing due to overshooting and local heating are the result of the same convective penetration process, the goal of this work is to invite solar modellers to consider both processes for a more consistent approach.
Key words: stars: evolution / stars: interiors / Sun: helioseismology / Sun: interior / convection
© ESO 2022
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.