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The generation of relativistic jets in active sources such as blazars is a complex problem with many aspects, most of them still not fully understood. Relativistic jets are likely produced by the accretion of matter and magnetic fields onto…

High Energy Astrophysical Phenomena · Physics 2020-07-21 Gustavo E. Romero , Eduardo M. Gutiérrez

The current understanding of the formation of powerful bi-directional jets in systems such as radio galaxies and quasars is that the process involves a supermassive black hole that is being fed with magnetized gas through an orbiting…

High Energy Astrophysical Phenomena · Physics 2009-03-25 C Sivaram , Kenath Arun

The origin of jets emitted from black holes is not well understood, however there are two possible energy sources, the accretion disk or the rotating black hole. Magnetohydrodynamic simulations show a well-defined jet that extracts energy…

Astrophysics · Physics 2009-11-10 Vladimir Semenov , Sergey Dyadechkin , Brian Punsly

An introduction is given to a meeting on the role of massive and stellar black holes in powering non-thermal activity in a rich variety of cosmic sources. Relevant properties of magnetized, spinning black holes are summarized and their…

High Energy Astrophysical Phenomena · Physics 2019-01-17 Roger Blandford

One of the most interesting high-energy, astrophysical phenomena are relativistic jets emitted from highly localized sky location. Such jets are common in Nature, observed to high redshift and in a range of wavelengths. Their precise…

High Energy Astrophysical Phenomena · Physics 2010-09-02 Nicolas Yunes

A brief summary is given of an alternative interpretation of the Event Horizon Telescope observations of the massive black hole in the nucleus of the nearby galaxy M87. It is proposed that the flow is primarily powered by the black hole…

High Energy Astrophysical Phenomena · Physics 2022-07-14 Roger Blandford , Noemie Globus

Recently, microquasar jets have aroused the interest of many researchers focusing on the astrophysical plasma outflows and various jet ejections. In this work, we concentrate on the investigation of electromagnetic radiation and particle…

High Energy Physics - Phenomenology · Physics 2021-11-02 Th. V. Papavasileiou , O. T. Kosmas , J. Sinatkas

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 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

Short gamma ray bursts are presumably results of binary neutron star mergers, which lead to the formation of a stellar mass black hole, surrounded by a remnant matter. The strong magnetic fields help collimate jets of plasma, launched along…

High Energy Astrophysical Phenomena · Physics 2019-03-06 K. Sapountzis , A. Janiuk

Accreting black holes are responsible for producing the fastest, most powerful outflows of matter in the Universe. The formation process of powerful jets close to black holes is poorly understood, and the conditions leading to jet formation…

Electron-positron pairs may be produced near accreting black holes by a variety of physical processes, and the resulting pair plasma may be accelerated and collimated into a relativistic jet. Here we use a self-consistent dynamical and…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Monika Moscibrodzka , Charles F. Gammie , Joshua C. Dolence , Hotaka Shiokawa

Supermassive black holes are found at the centers of most galaxies and their inspiral is a natural outcome when galaxies merge. The inspiral of these systems is of utmost astrophysical importance as prodigious producers of gravitational…

High Energy Astrophysical Phenomena · Physics 2015-05-18 Carlos Palenzuela , Luis Lehner , Steven L. Liebling

Recently, microquasar jets have aroused the interest of many researchers focusing on the astrophysical plasma outflows and various jet ejections. In this work, we concentrate on the investigation of electromagnetic radiation and particle…

High Energy Astrophysical Phenomena · Physics 2022-03-02 Theodora Papavasileiou , Odysseas Kosmas , Ioannis Sinatkas

Jets are endemic to both Galactic solar mass and extragalactic supermassive black holes. A recent 86 GHz image of M\,87 shows a jet emerging from the accretion ring around a black hole, providing the first direct observational constraint on…

High Energy Astrophysical Phenomena · Physics 2024-04-22 Brian Punsly

Recent observations suggest that in black hole X-ray binaries jet/outflow formation is related to the hot plasma in the vicinity of the black hole, either in the form of an advection-dominated accretion flow at low accretion rates or in a…

High Energy Astrophysical Phenomena · Physics 2015-06-15 Qingwen Wu , Xinwu Cao , Luis C. Ho , Ding-Xiong Wang

Radio galaxies are a subclass of active galactic nuclei that drive relativistic jets from their center and are observed in radio to very-high-energy gamma rays. The emission mechanisms and regions are still unknown. High-energy gamma rays…

High Energy Astrophysical Phenomena · Physics 2024-11-15 Riku Kuze , Shigeo S. Kimura , Kenji Toma

Rotating black holes are known to launch relativistic jets and accelerate particles provided they accrete a magnetized plasma. However, it remains unclear how the global magnetic field orientation affects the jet powering efficiency. Here,…

High Energy Astrophysical Phenomena · Physics 2025-08-27 Enzo Figueiredo , Benoît Cerutti , Kyle Parfrey

The formation of jets in black hole accretion systems is a long-standing problem. It has been proposed that a jet can be formed by extracting the rotation energy of the black hole ("BZ-jet") or the accretion flow ("disk-jet"). While both…

High Energy Astrophysical Phenomena · Physics 2024-02-13 Hai Yang , Feng Yuan , Hui Li , Yosuke Mizuno , Fan Guo , Rusen Lu , Luis C. Ho , Jieshuang Wang

The formation of jets in black hole accretion systems is a long-standing problem. It has been proposed that a jet can be formed by extracting the rotation energy of the black hole ("BZ-jet") or the accretion flow ("disk-jet"). While both…

High Energy Astrophysical Phenomena · Physics 2024-03-26 Hai Yang , Feng Yuan , Hui Li , Yosuke Mizuno , Fan Guo , Rusen Lu , Luis C. Ho , Xi Lin , Andrzej A. Zdziarski , Jieshuang Wang
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