Greybody factors of black holes in dRGT massive gravity coupled with nonlinear electrodynamics

TL;DR

This paper introduces new black hole solutions in dRGT massive gravity coupled with nonlinear electrodynamics, analyzes their thermodynamics, and computes bounds on their greybody factors, revealing faster evaporation compared to linear electrodynamics cases.

Contribution

The study provides novel dRGT black hole solutions with nonlinear electrodynamics and analyzes their greybody factors and thermodynamics, which was not previously explored.

Findings

Charged dRGT black holes with nonlinear electrodynamics evaporate faster.

Greybody factor bounds depend on physical parameters.

Graphical analysis illustrates parameter effects on greybody factors.

Abstract

In the context of the dRGT massive gravity coupled with nonlinear electrodynamics, we present new dRGT black hole solutions. Together with the thermodynamical properties of the solutions, we study the greybody factor of the corresponding black hole solution. To this end, we compute the rigorous bound on the greybody factor for the obtained dRGT black holes. The obtained results are graphically represented for different values of the theory's physical parameters. Our analysis shows that the charged dRGT black holes of nonlinear electrodynamics evaporate quicker than the charged dRGT black holes originated from linear electrodynamics.