A general Grad-Shafranov equation is obtained via differential forms, together with a scalar-field Lagrangian that yields the equation on-shell.
Particle Acceleration in Collisionless Magnetically Arrested Disks,
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Flux eruptions in MADs enhance non-axisymmetry near the black hole via m=1 and m=2 modes driven by vertical magnetic flux bundles formed through reconnection and expelled by buoyancy.
In a Kerr-Sen-like spacetime from Bumblebee gravity, increasing the Lorentz symmetry breaking rate and Bumblebee charge enlarges the allowed region for energy extraction via magnetic reconnection and moves it closer to the horizon, with peak efficiency when cosmic censorship is marginally violated.
citing papers explorer
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General Grad-Shafranov Equation
A general Grad-Shafranov equation is obtained via differential forms, together with a scalar-field Lagrangian that yields the equation on-shell.
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The azimuthal structure of magnetically arrested disks during flux eruption events
Flux eruptions in MADs enhance non-axisymmetry near the black hole via m=1 and m=2 modes driven by vertical magnetic flux bundles formed through reconnection and expelled by buoyancy.
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Energy extraction from a rotating black hole via magnetic reconnection: Bumblebee gravity
In a Kerr-Sen-like spacetime from Bumblebee gravity, increasing the Lorentz symmetry breaking rate and Bumblebee charge enlarges the allowed region for energy extraction via magnetic reconnection and moves it closer to the horizon, with peak efficiency when cosmic censorship is marginally violated.