When some magnetic field lines connect a Kerr black hole with a disk rotati
ng around it, energy and angular momentum are transferred between them. If
the black hole rotates faster than the disk, ca/GM(H) > 0.36 for a thin Kep
lerian disk, then energy and angular momentum are extracted from the black
hole and transferred to the disk (M-H is the mass and aM(H), is the angular
momentum of the black hole). This way, the energy originating in the black
hole may be radiated away by the disk. The total amount of energy that can
be extracted from the black hole spun down from ca/GM(H) = 0.998 to ca/GM(
H) = 0.36 by a thin Keplerian disk is approximate to 0.15M(H)c(2). This is
larger than approximate to 0.09M(H)c(2), which can be extracted by the Blan
dford-Znajek mechanism.