Physics of Pair-producing Gaps in Black Hole Magnetospheres: Two-dimensional General Relativistic Particle-in-cell Simulations

Black holes can launch powerful jets through the Blandford–Znajek process. This relies on enough plasma in the jet funnel to conduct the necessary current. However, in some low-luminosity active galactic nuclei, the plasma supply near the jet base may be an issue. It has been proposed that spark gap...

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Main Authors: Yajie Yuan, Alexander Y. Chen, Martin Luepker
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/adce79
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author Yajie Yuan
Alexander Y. Chen
Martin Luepker
author_facet Yajie Yuan
Alexander Y. Chen
Martin Luepker
author_sort Yajie Yuan
collection DOAJ
description Black holes can launch powerful jets through the Blandford–Znajek process. This relies on enough plasma in the jet funnel to conduct the necessary current. However, in some low-luminosity active galactic nuclei, the plasma supply near the jet base may be an issue. It has been proposed that spark gaps—local regions with unscreened electric field—can form in the magnetosphere, accelerating particles to initiate pair cascades, thus filling the jet funnel with plasma. In this paper, we carry out 2D general relativistic particle-in-cell (GRPIC) simulations of the gap, including self-consistent treatment of inverse Compton scattering and pair production. We observe gap dynamics that is fully consistent with our earlier 1D GRPIC simulations. We find strong dependence of the gap power on the soft photon spectrum and energy density, as well as the strength of the horizon magnetic field. We derive physically motivated scaling relations, and applying to M87, we find that the gap may be energetically viable for the observed TeV flares. For Sgr A*, the energy dissipated in the gap may also be sufficient to power the X-ray flares.
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spelling doaj-art-be2a51cd673f4f96b5282ae19e1a54aa2025-08-20T01:52:38ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-01985215910.3847/1538-4357/adce79Physics of Pair-producing Gaps in Black Hole Magnetospheres: Two-dimensional General Relativistic Particle-in-cell SimulationsYajie Yuan0https://orcid.org/0000-0002-0108-4774Alexander Y. Chen1https://orcid.org/0000-0002-4738-1168Martin Luepker2https://orcid.org/0009-0004-3333-7897Physics Department and McDonnell Center for the Space Sciences, Washington University in St. Louis , St. Louis, MO 63130, USA ; yajiey@wustl.eduPhysics Department and McDonnell Center for the Space Sciences, Washington University in St. Louis , St. Louis, MO 63130, USA ; yajiey@wustl.eduPhysics Department and McDonnell Center for the Space Sciences, Washington University in St. Louis , St. Louis, MO 63130, USA ; yajiey@wustl.eduBlack holes can launch powerful jets through the Blandford–Znajek process. This relies on enough plasma in the jet funnel to conduct the necessary current. However, in some low-luminosity active galactic nuclei, the plasma supply near the jet base may be an issue. It has been proposed that spark gaps—local regions with unscreened electric field—can form in the magnetosphere, accelerating particles to initiate pair cascades, thus filling the jet funnel with plasma. In this paper, we carry out 2D general relativistic particle-in-cell (GRPIC) simulations of the gap, including self-consistent treatment of inverse Compton scattering and pair production. We observe gap dynamics that is fully consistent with our earlier 1D GRPIC simulations. We find strong dependence of the gap power on the soft photon spectrum and energy density, as well as the strength of the horizon magnetic field. We derive physically motivated scaling relations, and applying to M87, we find that the gap may be energetically viable for the observed TeV flares. For Sgr A*, the energy dissipated in the gap may also be sufficient to power the X-ray flares.https://doi.org/10.3847/1538-4357/adce79Black hole physicsHigh energy astrophysicsPlasma astrophysicsNon-thermal radiation sources
spellingShingle Yajie Yuan
Alexander Y. Chen
Martin Luepker
Physics of Pair-producing Gaps in Black Hole Magnetospheres: Two-dimensional General Relativistic Particle-in-cell Simulations
The Astrophysical Journal
Black hole physics
High energy astrophysics
Plasma astrophysics
Non-thermal radiation sources
title Physics of Pair-producing Gaps in Black Hole Magnetospheres: Two-dimensional General Relativistic Particle-in-cell Simulations
title_full Physics of Pair-producing Gaps in Black Hole Magnetospheres: Two-dimensional General Relativistic Particle-in-cell Simulations
title_fullStr Physics of Pair-producing Gaps in Black Hole Magnetospheres: Two-dimensional General Relativistic Particle-in-cell Simulations
title_full_unstemmed Physics of Pair-producing Gaps in Black Hole Magnetospheres: Two-dimensional General Relativistic Particle-in-cell Simulations
title_short Physics of Pair-producing Gaps in Black Hole Magnetospheres: Two-dimensional General Relativistic Particle-in-cell Simulations
title_sort physics of pair producing gaps in black hole magnetospheres two dimensional general relativistic particle in cell simulations
topic Black hole physics
High energy astrophysics
Plasma astrophysics
Non-thermal radiation sources
url https://doi.org/10.3847/1538-4357/adce79
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