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The aberrated radiation pressure at the inner edge of the accretion disk around an astrophysical black hole imparts a relative azimuthal velocity on the electrons with respect to the ions which gives rise to a ring electric current that…

高能天体物理现象 · 物理学 2015-06-03 Ioannis Contopoulos , Antonios Nathanail , Matthaios Katsanikas

Astrophysical accretion flows are associated with energetic emission of radiation and outflows (winds and jets). Extensive observations of these two processes in X-ray binary outbursts are available. A convincing understanding of their…

高能天体物理现象 · 物理学 2019-01-11 Ioannis Contopoulos

We implement the KORAL code to perform two sets of very long general relativistic radiation magnetohydrodynamic simulations of an axisymmetric optically thin magnetized flow around a non-rotating black hole: one with a new term in the…

高能天体物理现象 · 物理学 2017-11-01 Ioannis Contopoulos , Antonios Nathanail , Alexander Sadowski , Demosthenes Kazanas , Ramesh Narayan

The Poynting-Robertson Cosmic Battery proposes that the innermost part of the accretion disk around a black hole is threaded by a large scale dipolar magnetic field generated in situ, and that the return part of the field diffuses outward…

高能天体物理现象 · 物理学 2015-06-05 Ioannis Contopoulos , Demetrios B. Papadopoulos

We reinvestigate the generation and accumulation of magnetic flux in optically thin accretion flows around active gravitating objects. The source of the magnetic field is the azimuthal electric current associated with the Poynting-Robertson…

We show that the Poynting-Robertson drag effect in an optically thin advection-dominated accretion flow around active gravitating objects generates strong azimuthal electric currents which give rise to astrophysically significant magnetic…

天体物理学 · 物理学 2009-10-30 Ioannis Contopoulos , Demosthenes Kazanas

We investigate the dynamics of radiation in an astrophysical accretion disk around a Kerr black hole. The source of the radiation is the accretion disk itself, and not a central object as in previous studies of the Poynting-Robertson…

高能天体物理现象 · 物理学 2015-06-19 Leela E. Koutsantoniou , Ioannis Contopoulos

Combined influence of rotation of a black hole and ambient magnetic fields creates conditions for powerful astrophysical processes of accretion and outflow of matter which are observed in many systems across the range of masses; from…

高能天体物理现象 · 物理学 2023-07-26 Ondrej Kopacek , Vladimir Karas

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…

高能天体物理现象 · 物理学 2020-07-21 Gustavo E. Romero , Eduardo M. Gutiérrez

We revisit the problem of magnetic field generation in accretion flows onto black holes owing to the excess radiation force on electrons. This excess force may arise from the Poynting-Robertson effect. Instead of a recent claim of the…

天体物理学 · 物理学 2009-11-07 G. S. Bisnovatyi-Kogan , R. V. E. Lovelace , V. A. Belinski

The structure and magnitude of the electromagnetic field produced by a rotating accretion disk around a black hole were determined. The disk matter is assumed to be a magnetized plasma with a frozenin poloidal magnetic field. The vacuum…

天体物理学 · 物理学 2009-11-07 A. A. Shatskiy

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…

高能天体物理现象 · 物理学 2019-01-17 Roger Blandford

Accreting black hole sources show variable outflows at different mass scales. For instance, in the case of galactic nuclei, our own galactic center Sgr A* exhibits flares and outbursts in the X-ray and infrared bands. Recent studies suggest…

高能天体物理现象 · 物理学 2024-07-17 Bestin James , Agnieszka Janiuk , Vladimir Karas

The electromagnetic field near a rotating black hole is being explored in educational style here. By employing analytic solutions for electrovacuum fields, we plot the surfaces of constant flux and we show how the field is dragged around…

天体物理学 · 物理学 2007-05-23 Z. Budinova , M. Dovciak , V. Karas , A. Lanza

Black holes attract gaseous material from the surrounding environment. Cosmic plasma is largely ionized and magnetized because of electric currents flowing in the highly conductive environment near black holes; the process of accretion then…

高能天体物理现象 · 物理学 2021-01-01 Vladimir Karas , Kostas Sapountzis , Agnieszka Janiuk

The centre of our Milky Way harbours the closest candidate for a supermassive black hole. The source is thought to be powered by radiatively inefficient accretion of gas from its environment. This form of accretion is a standard mode of…

Active galaxies and quasers are believed to harbour Black Holes at their centers and at the same time produce cosmic radio jets through which immense amount of matter and energy are ejected out of the core of the galaxy. In our work we…

天体物理学 · 物理学 2007-05-23 Tapas K. Das

The generation of magnetic fields by a battery, operating in an ion-electron plasma around a Kerr black hole, is studied in the 3+1 split of the Kerr metric. It is found that the gravitomagnetic contributions to the electron partial…

天体物理学 · 物理学 2015-06-24 Ramon Khanna

Recent studies have focused on how spinning black holes (BHs) within a binary system containing a strongly magnetized neutron star, then immersed in external magnetic fields, can acquire charge through mechanisms like the Wald process and…

高能天体物理现象 · 物理学 2025-02-04 Audrey Trova , Eva Hackmann

The mechanism by which outflows and plausible jets are driven from black hole systems, still remains observationally elusive. Notwithstanding, several observational evidences and deeper theoretical insights reveal that accretion and…

高能天体物理现象 · 物理学 2014-11-20 Debbijoy Bhattacharya , Shubhrangshu Ghosh , Banibrata Mukhopadhyay
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