Continuation of Force-Free Electrodynamics upon the loss of magnetic dominance
Morifumi Mizuno
astro-ph.HE, gr-qc, hep-th
Submitted: 2026-06-26
Comments: 31 pages, 5 figures, a supplemental movie for Fig. 3 is available (see ancillary file or https://youtu.be/W8cHlx0qxf0)
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- On the Properties of Time-Dependent, Force-Free, Degenerate Electrodynamics
- Effective Field Theory of Force-Free Electrodynamics
- Robustness of the Blandford-Znajek mechanism
- Hyperbolicity of Force-Free Electrodynamics
- Breakdown of force-free electrodynamics in electric zones
- Simulations of Axisymmetric Magnetospheres of Neutron Stars
- General Relativistic Force-Free Electrodynamics: A New Code and Applications to Black Hole Magnetospheres
- Three-dimensional numerical simulations of the pulsar magentoshere: Preliminary results
- Toward a Realistic Pulsar Magnetosphere
- Accurate Simulations of Binary Black-Hole Mergers in Force-Free Electrodynamics
- Force-free Electrodynamics in Arbitrary Geometries
- A Semilinear Wave Sector in Force-Free Electrodynamics
- Aristotelian Electrodynamics solves the Pulsar: Lower Efficiency of Strong Pulsars
- Structure of Aristotelian Electrodynamics
- Bosonization of Strong-Field Pair Plasma
- Further Results on Null and Force-free Electromagnetic Fields
- Exact Solutions to Force-Free Electrodynamics in Black Hole Backgrounds
- Relativistic Magnetic Reconnection in Astrophysical Plasmas: A Powerful Mechanism of Nonthermal Emission
- Stability in Force-Free Electrodynamics
- Generalized Rainich conditions, generalized stress-energy conditions, and the Hawking-Ellis classification
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