Radiation properties of the accretion disk around a quantum-corrected black hole
Abstract In this work, we study the radiation properties of the quantum-corrected black hole (BH). For simplicity, we consider test particles around the quantum-corrected BH. With this aim, we define the important quantities of test particles around the quantum-corrected BH: the effective potential, energy, angular momentum, and innermost stable circular orbit (ISCO). In addition, we explore the radiation properties of the accretion disk around the quantum-corrected BH considering the Novikov-Thorne model. We find that the values of the flux of the electromagnetic radiation and the temperature of the disk increase slightly with the increase of the quantum correction parameter α . To obtain more information, we plot the temperature profile using a color map. Finally, we consider the spectral luminosity of the accretion disk under the influence of the quantum correction parameter α .
Authors
- Mirzabek Alloqulov (ORCID: https://orcid.org/0000-0001-5337-7117)
- Sanjar Shaymatov (ORCID: https://orcid.org/0000-0002-5229-7657)
- Mirjavohir Mirxaydarov
Institutions
- Tashkent Institute of Irrigation and Agricultural Mechanization Engineers (UZ)
- National University of Uzbekistan (UZ)
- Zhejiang University of Technology (CN)
Publication Details
- Journal
- Chinese Physics C
- Published
- 2025-08-12
- DOI
- https://doi.org/10.1088/1674-1137/adfa83
- Primary Topic
- Astrophysical Phenomena and Observations
- Type
- article
- Field-Weighted Citation Impact
- 0.00