Modeling general-relativistic plasmas with collisionless moments and dissipative two-fluid magnetohydrodynamics

arXiv:2111.05752 · astro-ph.HE, gr-qc, nucl-th · Submitted 2021-11-10 · Read on arXiv

astro-ph.HE, gr-qc, nucl-th

Submitted: 2021-11-10

Updated: 2026-09-18

Comments: 15 pages, minor corrections to equations

DOI: 10.1093/mnras/stac1435

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

Terminology

• Boltzmann Equation — 8× in this paper · explained in 2 episodes
• Elias — 8× in this paper · explained in 2 episodes
• Trace — 3× in this paper · explained in 2 episodes
• Accretion Flows — 2× in this paper · explained in 1 episode
• Anisotropy — 2× in this paper · explained in 3 episodes
• Generalization — 2× in this paper · explained in 13 episodes
• Angular Momentum Transport — 1× in this paper · explained in 3 episodes
• Consistency — 1× in this paper · explained in 3 episodes

Sources

• Emission of magnetar bursts and precursors of neutron star mergers
• Local well-posedness in Sobolev spaces for first-order conformal causal relativistic viscous hydrodynamics
• Magnetic reconnection in the era of exascale computing and multiscale experiments
• Relativistic Fluid Dynamics In and Out of Equilibrium -- Ten Years of Progress in Theory and Numerical Simulations of Nuclear Collisions

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