Bardeen regular black hole as a quantum-corrected Schwarzschild black hole

TL;DR

This paper interprets the Bardeen regular black hole as a quantum-corrected Schwarzschild black hole using a generalized uncertainty principle, providing insights into quantum gravity parameters and the cosmological constant problem.

Contribution

It offers a novel interpretation of the Bardeen black hole as a quantum-corrected Schwarzschild black hole via GUP, linking quantum gravity parameters to cosmological observations.

Findings

Bardeen black hole can be viewed as a quantum-corrected Schwarzschild black hole.

Quantum gravity parameter estimates show a large discrepancy with the cosmological constant.

The approach provides a method to evaluate quantum gravity effects using regular black holes.

Abstract

Bardeen regular black hole is commonly considered as a solution of general relativity coupled to a nonlinear electrodynamics. In this paper, it is shown that the Bardeen solution may be interpreted as a quantum-corrected Schwarzschild black hole. This new interpretation is obtained by means of a generalized uncertainty principle applied to the Hawking temperature. Moreover, using the regular black hole of Bardeen, it is possible to evaluate the quantum gravity parameter of the generalized uncertainty principle or, assuming the recent upper bounds for such a parameter, to verify an enormous discrepancy between a cosmological constant and that measured by recent cosmological observations $(\sim 10^{120})$.