Kiselev Black holes in quantum fluctuation modified gravity

TL;DR

This paper derives new black hole solutions in quantum fluctuation modified gravity, analyzing their thermodynamics and energy conditions, and exploring the effects of metric fluctuations on black hole properties.

Contribution

It introduces a general solution framework for black holes in quantum fluctuation modified gravity, including thermodynamic and energy condition analyses.

Findings

New black hole solutions in quantum fluctuation modified gravity.

Analysis of Hawking temperature and horizon properties.

Constraints on metric fluctuation parameters.

Abstract

We obtain a new general solution for the gravitational field equations in quantum fluctuation modified gravity, which reduces to different classes of black holes surrounded by fluids, by taking some specific values of the parameter of the equation of state. We discuss the strong energy condition in a general way and also for some special cases of different fluids. In addition, the Hawking temperature associated to the horizons of solutions and constraints on the parameter characterizing the fluctuation of metric are taken into account in our analysis.