Energy Extraction from Spinning Black Holes via Relativistic Jets
arXiv:1303.3004 · doi:10.1007/978-3-319-06349-2_25
Abstract
It has for long been an article of faith among astrophysicists that black hole spin energy is responsible for powering the relativistic jets seen in accreting black holes. Two recent advances have strengthened the case. First, numerical general relativistic magnetohydrodynamic simulations of accreting spinning black holes show that relativistic jets form spontaneously. In at least some cases, there is unambiguous evidence that much of the jet energy comes from the black hole, not the disk. Second, spin parameters of a number of accreting stellar-mass black holes have been measured. For ballistic jets from these systems, it is found that the radio luminosity of the jet correlates with the spin of the black hole. This suggests a causal relationship between black hole spin and jet power, presumably due to a generalized Penrose process.
15 pages, 4 figures. To appear in the proceedings of the conference "Relativity and Gravitation: 100 Years after Einstein in Prague" held in Prague, June 25-29, 2012, Jiří Bičák and Tomáš Ledvinka editors, Max-Planck Research Library for the History and Development of Knowledge, Open Access Edition, Berlin (2013)
References in corpus (5)
- Stability of Relativistic Jets from Rotating, Accreting Black Holes via Fully Three-Dimensional Magnetohydrodynamic Simulations
- Black Hole Spin via Continuum Fitting and the Role of Spin in Powering Transient Jets
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- A dichotomy between the hard state spectral properties of black hole and neutron star X-ray~binaries
- Analog Kerr Black hole and Penrose effect in a Bose-Einstein Condensate
- Launching jets from accretion belts
- Dynamo generated magnetic configurations in accretion discs and the nature of quasi-periodic oscillations in accreting binary systems
- An Improved Test of the Binary Black Hole Hypothesis for Quasars with Double-peaked Broad Balmer Lines
- Magnetic Penrose process in the magnetized Kerr spacetime
- The High-energy emission of jetted AGN