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Emergence of magnetic null points in electro-vacuum magnetospheres of compact objects: The case of a plunging neutron star

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F20%3A10424887" target="_blank" >RIV/00216208:11320/20:10424887 - isvavai.cz</a>

  • Result on the web

    <a href="http://proceedings.physics.cz/index.php/ragtime-book/proceedings-of-ragtime-20-22a" target="_blank" >http://proceedings.physics.cz/index.php/ragtime-book/proceedings-of-ragtime-20-22a</a>

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

    Emergence of magnetic null points in electro-vacuum magnetospheres of compact objects: The case of a plunging neutron star

  • Original language description

    Relativistic effects of compact objects onto electromagnetic fields in their vicinity are investigated using the test-field approximation. In particular, we study the possible emergence of magnetic null points which are astrophysically relevant for the processes of magnetic reconnection. While the magnetic reconnection occurs in the presence of plasma and may lead to violent mass ejection, we show here that strong gravitation of the supermassive black hole may actively support the process by suitably entangling the field lines even in the electro-vacuum description. In this contribution we further discuss the case of a dipole-type magnetic field of the neutron star on the plunging trajectory to the supermassive black hole. While we have previously shown that given model in principle admits the formation of magnetic null points, here we explore whether and where the null points appear for the astrophysically relevant values of the parameters.

  • 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/GA17-13525S" target="_blank" >GA17-13525S: Sources of strong gravity and their astrophysical meaning</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2020

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    Proceedings of RAGtime 20-22: Workshops on black holes and neutron stars

  • ISBN

    978-80-7510-432-8

  • ISSN

  • e-ISSN

  • Number of pages

    10

  • Pages from-to

    165-174

  • Publisher name

    Silesian University in Opava

  • Place of publication

    Opava

  • Event location

    Opava

  • Event date

    Oct 15, 2018

  • Type of event by nationality

    EUR - Evropská akce

  • UT code for WoS article