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Radiation properties of the accretion disk around a quantum-corrected black hole

Mirjavoxir Mirkhaydarov, National University of Uzbekistan, Tashkent 100174, Uzbekistan, Tashkent, 100174, UZBEKISTANMirzabek Alloqulov, Institute of Fundamental and Applied Research, National Research University TIIAME, Kori Niyoziy 39, Tashkent 100000, Uzbekistan, Tashkent , UZBEKISTANSanjar ShaymatovZhejiang University of Technology, Institute for Theoretical Physics and Cosmology, Zheijiang University of Technology, Hangzhou 310023, China, Hangzhou, Zhejiang, 310014, CHINA
Chinese Physics Cjournal2025en
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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 .

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