Radiative characteristics of accretion disks around rotating regular black holes

Authors

  • Ye. Kurmanov Al-Farabi Kazakh National University, Almaty, Kazakhstan
  • T. Konysbayev Al-Farabi Kazakh National University, Almaty, Kazakhstan
  • G. Suliyeva Al-Farabi Kazakh National University, Almaty, Kazakhstan
  • G. Ikhsan Al-Farabi Kazakh National University, Almaty, Kazakhstan
  • N. Saiyp Al-Farabi Kazakh National University, Almaty, Kazakhstan
  • G. Rabigulova Al-Farabi Kazakh National University, Almaty, Kazakhstan
  • A. Urazalina Al-Farabi Kazakh National University, Almaty, Kazakhstan

DOI:

https://doi.org/10.26577/ijmph.2024v15i1a7
        82 74

Abstract

Our research focuses on examining the characteristics of thin accretion disks encircling rotating regular black holes. In this study, we investigate the important features of accretion disks surrounding Bardeen's regular black holes, which play a crucial role in addressing the singularity issue. The horizon configuration of rotating Bardeen black holes is analyzed in details, as well as the innermost stable circular orbits related to this spacetime. The primary goal is to derive quantitively the radiative flux, differential and spectral luminosities of the accretion disk. Within the specified gravitational field, particularly, by taking the parameter r_0*>0 and fixing the j=0.2, our findings show that the corresponding accretion disk’s luminosity exceeds that one predicted by the Kerr metric at identical value of spin parameter ( j=0.2). Making the juxtaposition of Bardeen’s black hole parameter  with the spin parameter  of the Kerr black hole we reveal that the spacetime corresponding to the non-rotating Bardeen black holes, in some certain cases, can imitate the Kerr spacetime.

Keywords: rotating Bardeen spacetime, angular velocity, angular momentum, energy and radiative flux.

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Published

2024-06-20

How to Cite

Kurmanov, Y. ., Konysbayev, T. ., Suliyeva, G., Ikhsan, G., Saiyp, N. ., Rabigulova, G., & Urazalina, A. (2024). Radiative characteristics of accretion disks around rotating regular black holes. International Journal of Mathematics and Physics, 15(1), 57–67. https://doi.org/10.26577/ijmph.2024v15i1a7

Issue

Vol. 15 No. 1 (2024): International Journal of Mathematics and Physics

Section

PHYSICS

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