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Profiled spectral lines generated by Keplerian discs orbiting in the Bardeen and Ayòn-Beato-Garcìa spacetimes

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19240%2F16%3AN0000021" target="_blank" >RIV/47813059:19240/16:N0000021 - isvavai.cz</a>

  • Result on the web

    <a href="http://iopscience.iop.org/article/10.1088/0264-9381/33/8/085004/meta" target="_blank" >http://iopscience.iop.org/article/10.1088/0264-9381/33/8/085004/meta</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1088/0264-9381/33/8/085004" target="_blank" >10.1088/0264-9381/33/8/085004</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Profiled spectral lines generated by Keplerian discs orbiting in the Bardeen and Ayòn-Beato-Garcìa spacetimes

  • Original language description

    Shape and frequency-shift maps of direct and indirect images of Keplerian discs orbiting in Bardeen and Ayon-Beato-Garcia (ABG) black hole and no-horizon spacetimes are determined. Then profiles of spectral lines generated in the innermost parts of the Keplerian discs in the Bardeen and ABG spacetimes are constructed. The frequency-shift maps and profiled spectral lines are compared to those generated in the field of Schwarzschild black holes and possible observationally relevant signatures of the regular black hole and no-horizon spacetimes are discussed. We demonstrate that differences relative to the Schwarzschild spacetimes are for the no-horizon spacetimes much more profound in comparison to the regular black hole spacetimes and increase with increasing charge parameter of the spacetime. The differences are greater. for small and large inclination angles than for intermediate ones. For the no-horizon spacetimes, the differences enable us. to distinguish the Bardeen and ABG spacetime, if inclination angle to the distant observer is known. We also show that contribution of the so-called ghost images to the profiled lines increases with increasing charge parameter of the spacetimes.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    <a href="/en/project/GB14-37086G" target="_blank" >GB14-37086G: Albert Einstein Center for Gravitation and Astrophysics</a><br>

  • Continuities

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

Others

  • Publication year

    2016

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Classical and Quantum Gravity

  • ISSN

    0264-9381

  • e-ISSN

  • Volume of the periodical

    33

  • Issue of the periodical within the volume

    8

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    33

  • Pages from-to

    '085004-1'-'085004-33'

  • UT code for WoS article

    000374832400004

  • EID of the result in the Scopus database

    2-s2.0-84963975899