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Cited by 170

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Direct numerical simulations of the Blandford-Znajek effect

Open access
Komissarov, S. S.·2001·Monthly Notices of the Royal Astronomical Society

Abstract

The time-dependent general relativistic equations of degenerate electrodynamics are solved numerically in order to study the mechanism of the electromagnetic extraction of the rotational energy of black holes. We performed a series of 2D runs for black holes with specific angular momentum, a, from 0.1 to 0.9 and for a monopole magnetic field assuming axisymmetry. In the inner region of the wind, the solution quickly settles to a steady state with an outgoing Poynting flux. In all cases the angular velocity of the magnetic field lines is almost half the angular velocity of the black hole. Thus, at least for the configuration considered, the Blandford–Znajek mechanism operates near its maximum power output.

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Crossref · 10.1046/j.1365-8711.2001.04863.x

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Metadata

Authors
Komissarov, S. S.
Venue
Monthly Notices of the Royal Astronomical Society
Published
2001-09-21
Volume
326
Issue
3
Pages
L41-L44
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W2137746285
Cited by
170
References
1
FWCI
3.46
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Direct numerical simulations of the Blandford-Znajek effect. https://app.cochat.ai/papers/10.1046/j.1365-8711.2001.04863.x
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Komissarov, S. S. (2001). Direct numerical simulations of the Blandford-Znajek effect. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1046/j.1365-8711.2001.04863.x

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.