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

In this work, we study the radiation properties of the quantum-corrected black hole (BH). For simplicity, we consider test particles around quantum-corrected BH. With this aim, we define the important quantities of test particles around 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 get 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.