Magnetohydrodynamics of charged interstellar dust. Multifluid models and study of the linear modes

arXiv:2608.30711 · astro-ph.GA, astro-ph.SR, physics.plasm-ph · Submitted 2026-08-31 · Read on arXiv

astro-ph.GA, astro-ph.SR, physics.plasm-ph

Submitted: 2026-08-31

Updated: 2026-08-31

Comments: Accepted for publication in Astronomy & Astrophysics

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

Terminology

• Core — 15× in this paper · explained in 2 episodes
• Decoupling — 7× in this paper · explained in 2 episodes
• Abundance — 6× in this paper · explained in 1 episode
• Adaptation — 3× in this paper · explained in 1 episode
• Alignment — 3× in this paper
• Ambipolar Diffusion — 3× in this paper
• Magnetohydrodynamics (MHD) — 3× in this paper · explained in 4 episodes
• NATO Advanced Study Institute — 3× in this paper
• Streaming Instability — 2× in this paper · explained in 2 episodes
• Adam — 1× in this paper · explained in 2 episodes
• Angular Momentum Transport — 1× in this paper · explained in 3 episodes
• Momentum transfer — 1× in this paper · explained in 2 episodes
• Robustness — 1× in this paper · explained in 6 episodes

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