Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations

arXiv:2607.29141 · astro-ph.EP, astro-ph.SR, physics.flu-dyn · Submitted 2026-07-31 · Read on arXiv

Shijun Chu, Zhao Guo, Aurélie Astoul, Adrian J. Barker, Rainer Hollerbach

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

Submitted: 2026-07-31

Comments: Accepted for publication in MNRAS on 30th July 2026 (19 pages, 15 figures, 1 table)

Project page: https://magic-sph.github.io/numerics.html

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

Terminology

• Core — 11× in this paper · explained in 2 episodes
• Frequency Dependence — 3× in this paper · explained in 2 episodes
• Chebyshev Polynomials — 2× in this paper · explained in 2 episodes
• Consistency — 1× in this paper · explained in 3 episodes

Sources

• The EBLM Project XVIII. 3D Obliquities of Five Low-Mass Eclipsing Binaries

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