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Magnetized black holes: The role of rotation, boost, and accretion in twisting the field lines and accelerating particles

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F23%3A00604648" target="_blank" >RIV/67985815:_____/23:00604648 - isvavai.cz</a>

  • Result on the web

    <a href="https://www.worldscientific.com/doi/epdf/10.1142/9789811269776_0333" target="_blank" >https://www.worldscientific.com/doi/epdf/10.1142/9789811269776_0333</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1142/9789811269776_0333" target="_blank" >10.1142/9789811269776_0333</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Magnetized black holes: The role of rotation, boost, and accretion in twisting the field lines and accelerating particles

  • Original language description

    Combined influence of rotation of a black hole and ambient magnetic fields creates con-ditions for powerful astrophysical processes of accretion and outflow of matter which areobserved in many systems across the range of masses, from stellar-mass black holes in bi-nary systems to supermassive black holes in active galactic nuclei. We study a simplifiedmodel of outflow of electrically charged particles from the inner region of an accretiondisk around a spinning (Kerr) black hole immersed in a large-scale magnetic field. Inparticular, we consider a non-axisymmetric magnetosphere where the field is misalignedwith the rotation axis. In this contribution we extend our previous analysis of acceler-ation of jet-like trajectories of particles escaping from bound circular orbits around ablack hole. While we have previously assumed the initial setup of prograde (co-rotating)orbits, here we relax this assumption and we also consider retrograde (counter-rotating)motion. We show that the effect of counter-rotation may considerably increase the prob-ability of escape from the system, and it allows more efficient acceleration of escapingparticles to slightly higher energies compared to the co-rotating disk

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/8JCH1080" target="_blank" >8JCH1080: Czech-Chinese collaboration for the new X-ray mission eXTP: Spectral modelling and data analysis</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2023

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Article name in the collection

    The Sixteenth Marcel Grossmann Meeting: On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics, and Relativistic Field Theories

  • ISBN

    978-981-12-6976-9

  • ISSN

  • e-ISSN

  • Number of pages

    11

  • Pages from-to

    3999-4009

  • Publisher name

    World Scientific

  • Place of publication

    Singapur - SG

  • Event location

    online

  • Event date

    Jul 5, 2021

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article

    001229112700329