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The detection of rapidly variable gamma-ray emission in active galactic nuclei has generated renewed interest in magnetospheric particle acceleration and emission scenarios. In order to explore its potential, we study the possibility of…

High Energy Astrophysical Phenomena · Physics 2020-06-04 Grigorios Katsoulakos , Frank M. Rieger

Spark gaps are likely the source of plasma in active black hole (BH) magnetospheres. In this paper, we present results of 1D general-relativistic particle-in-cell simulations of a starved BH magnetosphere with a realistic treatment of…

High Energy Astrophysical Phenomena · Physics 2020-10-21 Shota Kisaka , Amir Levinson , Kenji Toma

We study the response of a starved Kerr black hole magnetosphere to abrupt changes in the intensity of disk emission and in the global magnetospheric current, by means of 1D general relativistic particle-in-cell simulations. Such changes…

High Energy Astrophysical Phenomena · Physics 2022-01-19 Shota Kisaka , Amir Levinson , Kenji Toma , Idan Niv

In some low-luminosity accreting supermassive black hole systems, the supply of plasma in the funnel region can be a problem. It is believed that a local region with unscreened electric field can exist in the black hole magnetosphere,…

High Energy Astrophysical Phenomena · Physics 2018-08-29 Alexander Y. Chen , Yajie Yuan , Huan Yang

We investigate the dynamics and emission of a starved magnetospheric region (gap) formed in the vicinity of a Kerr black hole horizon, using a new, fully general relativistic particle-in-cell code that implements Monte Carlo methods to…

High Energy Astrophysical Phenomena · Physics 2018-09-12 Amir Levinson , Benoît Cerutti

This is the second paper in a series where we examine the physics of pair producing gaps in low-luminosity accreting supermassive black hole systems. In this paper, we carry out time-dependent self-consistent fully general relativistic 1D…

High Energy Astrophysical Phenomena · Physics 2020-06-10 Alexander Y. Chen , Yajie Yuan

(Abridged) An issue of considerable interest in the theory of jet formation by the Blandford-Znajek mechanism, is how plasma is being continuously supplied to the magnetosphere to maintain it in a force-free state. Injection of…

High Energy Astrophysical Phenomena · Physics 2024-07-19 Idan Niv , Omer Bromberg , Amir Levinson , Benoit Cerutti , Benjamin Crinquand

Black holes are known to launch powerful relativistic jets and emit highly variable gamma radiation. How these jets are loaded with plasma remains poorly understood. Spark gaps are thought to drive particle acceleration and pair creation in…

High Energy Astrophysical Phenomena · Physics 2020-04-22 Benjamin Crinquand , Benoît Cerutti , Alexander Philippov , Kyle Parfrey , Guillaume Dubus

In the absence of a sufficient amount of plasma injection into the black hole (BH) magnetosphere, the force-free state of the magnetosphere cannot be maintained, leading to the emergence of strong, time-dependent, longitudinal electric…

High Energy Astrophysical Phenomena · Physics 2024-01-22 Koki Kin , Shota Kisaka , Kenji Toma , Shigeo S. Kimura , Amir Levinson

Non-thermal magnetospheric processes in the vicinity of supermassive black holes have attracted particular attention in recent times. Gap-type particle acceleration accompanied by curvature and Inverse Compton radiation could in principle…

High Energy Astrophysical Phenomena · Physics 2017-12-18 Frank M. Rieger , Grigorios Katsoulakos

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…

High Energy Astrophysical Phenomena · Physics 2025-05-30 Yajie Yuan , Alexander Y. Chen , Martin Luepker

This work studies jet-like electromagnetic configurations surrounding a slowly-spinning black-hole immersed in a uniformly magnetized force-free plasma. In the first part of this work, we present a family of stationary solutions that are…

High Energy Astrophysical Phenomena · Physics 2015-06-24 Huan Yang , Fan Zhang , Luis Lehner

Recent observations of Sgr A$^*$ by Fermi and HESS have detected steady gamma-ray emission in the GeV and TeV bands. We present a new model to explain the GeV gamma-ray emission by inverse Compton scattering by nonthermal electrons supplied…

High Energy Astrophysical Phenomena · Physics 2015-06-03 Masaaki Kusunose , Fumio Takahara

The origin of pulsar radio emission is one of the old puzzles in theoretical astrophysics. In this Letter we present a global kinetic plasma simulation which shows from first-principles how and where radio emission can be produced in pulsar…

High Energy Astrophysical Phenomena · Physics 2023-12-12 Ashley Bransgrove , Andrei M. Beloborodov , Yuri Levin

In the inner regions of an accretion disk around a black hole, relativistic protons can interact with ambient matter to produce electrons, positrons and $\gamma$-rays. The resultant steady state electron and positron particle distributions…

Astrophysics · Physics 2009-11-11 S. Bhattacharyya , N. Bhatt , R. Misra

Black hole solutions in general relativity come with pathologies such as singularity and mass inflation instability, which are believed to be cured by a yet-to-be-found quantum theory of gravity. Without such consistent description, one may…

General Relativity and Quantum Cosmology · Physics 2023-02-14 Rajes Ghosh , Mostafizur Rahman , Akash K Mishra

Context: The origin of ultra-rapid flares of very high-energy radiation from active galactic nuclei remains elusive. Magnetospheric processes, occurring in the close vicinity of the central black hole, could account for these flares. Aims:…

High Energy Astrophysical Phenomena · Physics 2021-06-30 Benjamin Crinquand , Benoît Cerutti , Guillaume Dubus , Kyle Parfrey , Alexander Philippov

Some active galactic nuclei, microquasars, and gamma ray bursts may be powered by the electromagnetic braking of a rapidly rotating black hole. We investigate this possibility via axisymmetric numerical simulations of a black hole…

Astrophysics · Physics 2008-11-26 Jonathan C. McKinney , Charles F. Gammie

Pulsed emission from gamma-ray pulsars originates inside the magnetosphere, from radiation by charged particles accelerated near the magnetic poles or in the outer gaps. In polar cap models, the high energy spectrum is cut off by magnetic…

Astrophysics · Physics 2009-10-31 Alice K. Harding

The black hole shadow, a direct probe of the event horizon's gravitational influence, has been observationally confirmed by the Event Horizon Telescope (EHT). While theoretical models of shadows in vacuum are mature, real astrophysical…

High Energy Astrophysical Phenomena · Physics 2025-11-20 Sai Karan Mukthapuram , Sandeep Kumar Kataria
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