Mesoscale Turbulence in Type Ia Supernova Deflagrations II. Evidence for Fuel Preheat Due to Flame Thermal Expansion from Lagrangian Analysis

arXiv:2610.02677 · astro-ph.SR, astro-ph.HE, physics.data-an, physics.flu-dyn, physics.plasm-ph · Submitted 2026-10-02 · Read on arXiv

astro-ph.SR, astro-ph.HE, physics.data-an, physics.flu-dyn, physics.plasm-ph

Submitted: 2026-10-02

Updated: 2026-10-02

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