Gravito-thermo-electrodynamic extraction of energy from Kerr black holes
The ``force-free" magnetosphere of a Kerr black-hole in the axisymmetric steady-state possesses two integral functions of the stream-function $\Psi$; the field-line angular-velocity (FLAV) $\Omega_{\rm F} (\Psi)$, and the current-function $I(\Psi)$.
Okamoto, Isao, Song, Yoogeun
core
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