English

Non-adiabatic Effect on Convective Mode

Solar and Stellar Astrophysics 2026-03-12 v2

Abstract

The systematic analysis of non-adiabatic effect on convective mode has been conducted using wave energy relation. In the adiabatic analysis, the "propagation diagram" for convective mode is proposed as a useful tool to see its behavior. In the non-adiabatic analysis, it is found that for strongly non-adiabatic case, a monotonically growing convective mode becomes oscillatory. In this phase, the radial displacement and the distribution of wave energy show only one bump, in which the distribution of entropy energy eS almost overlaps with the distribution of gravity energy eg. Entropy energy eS seems to act as potential energy of oscillatory convection. In addition to this, this change occurs not gradually, but abruptly with change of non-adiabatic indicator.

Keywords

Cite

@article{arxiv.2601.12756,
  title  = {Non-adiabatic Effect on Convective Mode},
  author = {Hiroyasu Ando},
  journal= {arXiv preprint arXiv:2601.12756},
  year   = {2026}
}

Comments

8 pages, 7 figures, accepted for publication in PASJ

R2 v1 2026-07-01T09:10:06.080Z