The impact of nuclear equations of state on the dynamics and multi-messenger emission of magnetorotational stellar explosions

arXiv:2608.06017 · astro-ph.HE, astro-ph.SR, nucl-th · Submitted 2026-08-06 · Read on arXiv

INFN Sezione di Firenze, Florence, Italy · INAF Osservatorio Astrofisico di Arcetri, Florence, Italy · INFN Sezione di Firenze, Florence, Italy · Universite Paris-Saclay, Universite Paris Cite, CEA, CNRS, AIM, Gif-sur-Yvette, France · Observatori Astronomic, Universitat de Valencia, Valencia, Spain

astro-ph.HE, astro-ph.SR, nucl-th

Submitted: 2026-08-06

Updated: 2026-08-06

Comments: Accepted for publication in Astronomy & Astrophysics. 21 pages, 17 figures

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

Terminology

• Core — 45× in this paper · explained in 2 episodes
• Equation of State (EoS) — 3× in this paper · explained in 4 episodes
• Metallicity — 3× in this paper · explained in 3 episodes
• Abundance — 2× in this paper · explained in 1 episode
• Angular Momentum Transport — 2× in this paper · explained in 3 episodes
• Accretion Flows — 1× in this paper · explained in 1 episode
• Adam — 1× in this paper · explained in 2 episodes
• Boltzmann Equation — 1× in this paper · explained in 2 episodes
• Decoupling — 1× in this paper · explained in 2 episodes
• Degeneracy — 1× in this paper · explained in 3 episodes
• Magnetohydrodynamics (MHD) — 1× in this paper · explained in 3 episodes
• Nuclear Statistical Equilibrium — 1× in this paper
• Signal-to-noise ratio (SNR) — 1× in this paper · explained in 2 episodes
• Trace — 1× in this paper · explained in 2 episodes

Sources

• The Generalization Gap in Machine Learning EoS Inference from Core-Collapse Supernova Gravitational Waves
• Impact of the nuclear equation of state on the explodability of massive stars

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