Energy self-extraction of a Kerr black hole through its frame-dragged force-free magnetosphere
Abstract
It is shown that when only the condition 0< F< H is satisfied, the Kerr black hole frame-drags its surrounding force-free magnetosphere with the field-line-angular-velocity (FLAV) F, where H is the horizon angular-velocity. Then, the zero-angular-momentum-observers (ZAMOs) circulating with the frame-dragging-angular-velocity ω will see that the `null surface' S N where ω N= F always exists. They will see that the outer domain D (out) outside S N is prograde-rotating with F ω>0, whereas the inner domain D (in) inside is retrograde-rotating with F ω<0, where F ω= F - ω denotes the ZAMO-FLAV. `This surface' S N must be the magneto-centrifugal divider of the force-free magnetosphere, with a kind of plasma-shed on it. Subsequently, the force-free and freezing-in conditions break down on S N, thereby allowing the particle-current sources to be set up on S N. `This surface' also is the ZAM-surface S ZAMD, on which no flow of angular momentum nor electric current can cross. Because the electric field E p reverses sign on S N, the Poynting flux reverses direction from outward to inward on S N. An electromagnetic self-extraction of energy will be possible only through the frame-dragged magnetosphere, with the inner domain D (in) nested between the horizon and `this surface' S N, in order to comply with the first and second laws of thermodynamics.
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