A Diagnostic Method for Proto-Neutron Star Magnetic Fields by Supernova Fallback Neutrinos

arXiv:2609.28057 · astro-ph.HE · Submitted 2026-09-23 · Read on arXiv

astro-ph.HE

Submitted: 2026-09-23

Updated: 2026-09-23

Code: https://github.com/ForestRL/FOREST

Terminology

• Core — 9× in this paper · explained in 2 episodes
• Degeneracy — 7× in this paper · explained in 3 episodes
• Abundance — 2× in this paper · explained in 1 episode
• Accretion Shock — 2× in this paper · explained in 1 episode
• Equation of State (EoS) — 2× in this paper · explained in 4 episodes
• Accretion Flows — 1× in this paper · explained in 1 episode
• Accuracy — 1× in this paper · explained in 1 episode
• Deep Underground Neutrino Experiment — 1× in this paper
• Robustness — 1× in this paper · explained in 5 episodes
• SK and Jiangmen Underground Neutrino Observatory — 1× in this paper

Sources

• Gravitational Waves from Core-Collapse Supernovae
• Hyper-Kamiokande Design Report
• GRMHD Simulations of Accreting Proto-Magnetars I. Implications for Gamma-Ray Burst Jets and Energetic Explosions
• GRMHD Simulations of Accreting Proto-Magnetars II. Implications for r-process Nucleosynthesis
• Impacts of hydrogen envelope on supernova fallback and the resulting compact remnant masses

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