Blandford–Znajek process

The Blandford–Znajek process is a mechanism for the extraction of energy from a rotating black hole,[1][2] introduced by Roger Blandford and Roman Znajek in 1977.[3] This mechanism correctly describes how astrophysical jets are formed around spinning supermassive black holes. This is one of the mechanisms that power quasars, or rapidly accreting supermassive black holes.[4] Generally speaking, it was demonstrated that the power output of the accretion disk is significantly larger than the power output extracted directly from the hole, through its ergosphere.[5][6] Hence, the presence (or not) of a poloidal magnetic field around the black hole is not determinant in its overall power output. It was also suggested that the mechanism plays a crucial role as a central engine for a gamma-ray burst.[7]
Physics of the mechanism

As in the Penrose process, the ergosphere plays an important role in the Blandford–Znajek process. In order to extract energy and angular momentum from the black hole, the electromagnetic field around the hole must be modified by magnetospheric currents. In order to drive such currents, the electric field needs to not be screened, and consequently the vacuum field created within the ergosphere by distant sources must have an unscreened component. The most favored way to provide this is an e± pair cascade in a strong electric and radiation field.[8] As the ergosphere causes the magnetosphere inside it to rotate, the outgoing flux of angular momentum results in extraction of energy from the black hole.

The Blandford–Znajek process requires an accretion disc with a strong poloidal magnetic field around a spinning black hole. The magnetic field extracts spin energy, and the power can be estimated as the energy density at the speed of light cylinder times area:

\( {\displaystyle P=B^{2}\left({\frac {r}{r_{c}}}\right)^{4}r_{c}c={\frac {B^{2}r^{4}\omega ^{2}}{c}},} \)

where B is the magnetic field strength, \( r_{c} \) is the Schwarzschild radius, and ω is the angular velocity.[4]
See also

Penrose process, another mechanism to extract energy from a black hole
Hawking radiation, another mechanism to extract mass, hence energy from a black hole
Astrophysical jets, large structures seen around some quasars and created by the Blandford–Znajek process

References

Frolov, Valeri P.; Zelnikov, Andrei (2011), Introduction to Black Hole Physics, Oxford: Oxford University Press, ISBN 978-0-19-969229-3, Zbl 1234.83001, (Chapter 8.9: Black Holes in External Magnetic Field).
Lea, Robert (2019-01-31). "How black holes power relativistic jets". Medium. Retrieved 2020-09-10.
R. D. Blandford and R. L. Znajek, "Electromagnetic extraction of energy from Kerr black holes", Mon. Not. R. Astr. Soc. 179:433-456 (1977).
Frank, Juhan; King, Andrew; Raine, Derek J. (February 2002). Accretion Power in Astrophysics (Third ed.). Cambridge, UK: Cambridge University Press. Bibcode:2002apa..book.....F. ISBN 0521620538.
Livio, M.; Ogilvie, G. I.; Pringle, J. E. (1999-02-01). "Extracting Energy from Black Holes: The Relative Importance of the Blandford-Znajek Mechanism". The Astrophysical Journal. 512 (1): 100–104. arXiv:astro-ph/9809093. Bibcode:1999ApJ...512..100L. doi:10.1086/306777.
McKinney, Jonathan C. (2005-09-01). "Total and Jet Blandford-Znajek Power in the Presence of an Accretion Disk". The Astrophysical Journal Letters. 630 (1): L5–L8. arXiv:astro-ph/0506367. Bibcode:2005ApJ...630L...5M. doi:10.1086/468184. S2CID 18743811.
Lee, H. K.; Wijers, R. A. M. J.; Brown, G. E. (2000). "The Blandford-Znajek process as a central engine for a gamma-ray burst". Physics Reports. 325 (3): 83–114. arXiv:astro-ph/9906213. Bibcode:2000PhR...325...83L. doi:10.1016/S0370-1573(99)00084-8. ISSN 0370-1573. S2CID 7936182.

Camenzind, M.: "Compact objects in Astrophysics" (Springer 2007, ISBN 978-3-540-25770-7), p. 500, 505.

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Black holes
Types

Schwarzschild Rotating Charged Virtual Kugelblitz Primordial Planck particle

Size

Micro
Extremal Electron Stellar
Microquasar Intermediate-mass Supermassive
Active galactic nucleus Quasar Blazar

Formation

Stellar evolution Gravitational collapse Neutron star
Related links Tolman–Oppenheimer–Volkoff limit White dwarf
Related links Supernova
Related links Hypernova Gamma-ray burst Binary black hole

Properties

Gravitational singularity
Ring singularity Theorems Event horizon Photon sphere Innermost stable circular orbit Ergosphere
Penrose process Blandford–Znajek process Accretion disk Hawking radiation Gravitational lens Bondi accretion M–sigma relation Quasi-periodic oscillation Thermodynamics
Immirzi parameter Schwarzschild radius Spaghettification