Shadow of the Kerr-like black hole

Abstract The detailed study of horizon structure and the shadow cast by a Kerr-like black hole (BH) is performed. The trajectory of light rays forming the shadow of BH is found using the solutions of geodesic equation for the motion and effective potential of a photon around Kerr-like BH for differe...

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Main Authors: Furkat Sarikulov, Farruh Atamurotov, Ahmadjon Abdujabbarov, Bobomurat Ahmedov
Format: Article
Language:English
Published: SpringerOpen 2022-09-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-022-10711-4
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author Furkat Sarikulov
Farruh Atamurotov
Ahmadjon Abdujabbarov
Bobomurat Ahmedov
author_facet Furkat Sarikulov
Farruh Atamurotov
Ahmadjon Abdujabbarov
Bobomurat Ahmedov
author_sort Furkat Sarikulov
collection DOAJ
description Abstract The detailed study of horizon structure and the shadow cast by a Kerr-like black hole (BH) is performed. The trajectory of light rays forming the shadow of BH is found using the solutions of geodesic equation for the motion and effective potential of a photon around Kerr-like BH for different values of deviation parameter l in Kerr-like spcetime metric. It is observed that with an increase in the parameter l the size of the shadow of the BH is decreased. Additional, we have consider effect of plasma on BH shadow and the plasma influence on the shadow of Kerr-like BH, the size of observable radius of BH shadow and oblateness are explored with more details.
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spelling doaj.art-57f79611ff6843aeba87fee36961e7da2022-12-22T04:05:05ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522022-09-0182911210.1140/epjc/s10052-022-10711-4Shadow of the Kerr-like black holeFurkat Sarikulov0Farruh Atamurotov1Ahmadjon Abdujabbarov2Bobomurat Ahmedov3Ulugh Beg Astronomical InstituteInha University in TashkentUlugh Beg Astronomical InstituteUlugh Beg Astronomical InstituteAbstract The detailed study of horizon structure and the shadow cast by a Kerr-like black hole (BH) is performed. The trajectory of light rays forming the shadow of BH is found using the solutions of geodesic equation for the motion and effective potential of a photon around Kerr-like BH for different values of deviation parameter l in Kerr-like spcetime metric. It is observed that with an increase in the parameter l the size of the shadow of the BH is decreased. Additional, we have consider effect of plasma on BH shadow and the plasma influence on the shadow of Kerr-like BH, the size of observable radius of BH shadow and oblateness are explored with more details.https://doi.org/10.1140/epjc/s10052-022-10711-4
spellingShingle Furkat Sarikulov
Farruh Atamurotov
Ahmadjon Abdujabbarov
Bobomurat Ahmedov
Shadow of the Kerr-like black hole
European Physical Journal C: Particles and Fields
title Shadow of the Kerr-like black hole
title_full Shadow of the Kerr-like black hole
title_fullStr Shadow of the Kerr-like black hole
title_full_unstemmed Shadow of the Kerr-like black hole
title_short Shadow of the Kerr-like black hole
title_sort shadow of the kerr like black hole
url https://doi.org/10.1140/epjc/s10052-022-10711-4
work_keys_str_mv AT furkatsarikulov shadowofthekerrlikeblackhole
AT farruhatamurotov shadowofthekerrlikeblackhole
AT ahmadjonabdujabbarov shadowofthekerrlikeblackhole
AT bobomuratahmedov shadowofthekerrlikeblackhole