Magnetic Field Configurations in Binary Neutron Star Mergers I: Post-merger Remnant and Disk

arXiv:2506.18995 · astro-ph.HE, gr-qc · Submitted 2025-06-23 · Read on arXiv

astro-ph.HE, gr-qc

Submitted: 2025-06-23

Updated: 2026-09-24

Terminology

• Core — 9× in this paper · explained in 2 episodes
• Adam — 4× in this paper · explained in 2 episodes
• Elias — 3× in this paper · explained in 2 episodes
• Initial Data — 3× in this paper · explained in 2 episodes
• Calibration — 1× in this paper · explained in 7 episodes
• Consistency — 1× in this paper · explained in 3 episodes
• Gravitational Wave Emission — 1× in this paper · explained in 2 episodes
• Robustness — 1× in this paper · explained in 5 episodes

Sources

• Robustness of Magnetic Field Amplification in Neutron Star Mergers
• Impact of magnetic field gradients on the development of the MRI: Applications to binary neutron star mergers and proto-planetary disks
• Magnetic Flux Emergence in Binary Neutron Star Remnants
• General relativistic magnetohydrodynamics simulations for binary neutron star mergers
• Turbulence in Magnetised Neutron Stars
• Numerical relativity simulations of compact binaries: comparison of cell- and vertex-centered adaptive meshes

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