Understanding hydrodynamical wave-driven shear mixing in stellar radiation zones. Looking in the mirror of the dyapicnal oceanic mixing

arXiv:2605.26085 · astro-ph.SR, astro-ph.EP, physics.ao-ph, physics.flu-dyn · Submitted 2026-05-25 · Read on arXiv

Stéphane Mathis

astro-ph.SR, astro-ph.EP, physics.ao-ph, physics.flu-dyn

Submitted: 2026-05-25

Comments: 5 pages, 1 figure, Accepted for publication as a Letter in Astronomy \& Astrophysics

Journal ref: A&A 710, L19 (2026)

DOI: 10.1051/0004-6361/202660495

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Abundance — 1× in this paper · explained in 1 episode
• Core — 1× in this paper · explained in 2 episodes

Sources

• Complex dynamical regimes of the Tayler-Spruit dynamo
• Chemical transport by weakly nonlinear internal gravity waves in stars

Related papers

• HXI-DLA2: A Physics-Constrained Deep Learning Algorithm for the ASO-S Hard X-ray Imager
• Effect of Neutron Star Jets on Common Envelope Evolution
• Constraining the origin of magnetic white dwarfs
• JW-FD: A 15-Year Multimodal Dataset for Solar Flare Forecasting
• Phlegethon: a fully compressible magnetohydrodynamic code for simulations in stellar astrophysics
• Can MHD Oscillations Modulate Quasi-Periodic Plasma Release from Coronal Streamers?