Extracting energy from a black hole through its disk

Authors
Citation
Lx. Li, Extracting energy from a black hole through its disk, ASTROPHYS J, 533(2), 2000, pp. L115-L118
Citations number
16
Categorie Soggetti
Space Sciences
Journal title
ASTROPHYSICAL JOURNAL
ISSN journal
0004637X → ACNP
Volume
533
Issue
2
Year of publication
2000
Part
2
Pages
L115 - L118
Database
ISI
SICI code
0004-637X(20000420)533:2<L115:EEFABH>2.0.ZU;2-N
Abstract
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.