Exploring perfect fluid accretion onto quantum-corrected Reissner–Nordstrom black hole

Abstract

The current study examines astrophysical accretion near a static and spherically symmetric, quantum-corrected charged black hole. Furthermore, the analysis focuses on fluid dynamics in the vicinity of gravitationally quantum-corrected Reissner–Nordstrom Anti-de Sitter black hole for the polytropic and isothermal forms, categorized by their equation of state. We utilized the Hamiltonian dynamical procedure to explore the behavior of the specified fluids. As part of the investigation, the sonic or critical points are identified, revealing key transitions in fluid flow. Also, we have presented the fluid behavior in a closed form through a graphical representation. The results of this research help us to analyze the accretion phenomenon within the effects of quantum gravity.