Bardeen spacetime as a quantum corrected Schwarzschild black hole: Quasinormal modes and Hawking radiation

TL;DR

This paper investigates the quasinormal modes and Hawking radiation of the Bardeen black hole, a regular black hole model interpreted as a quantum-corrected Schwarzschild black hole, revealing deviations in overtones and suppressed radiation due to quantum effects.

Contribution

It provides accurate calculations of quasinormal modes and Hawking radiation for the Bardeen black hole, addressing previous inaccuracies and analyzing quantum correction effects.

Findings

Overtones deviate significantly from Schwarzschild values with quantum corrections.

Hawking radiation intensity is suppressed by up to three orders of magnitude.

Deviations are most prominent near the event horizon.

Abstract

The Bardeen black hole holds historical significance as the first model of a regular black hole. Recently, there have been proposed interpretations of the Bardeen spacetime as quantum corrections to the Schwarzschild solution. Our study focuses on investigating the quasinormal modes and Hawking radiation of the Bardeen black hole. We have observed that previous studies on the quasinormal modes for the Bardeen black hole suffer from inaccuracies that cannot be neglected. Therefore, we propose accurate calculations of the quasinormal modes for scalar, electromagnetic, and neutrino fields in the Bardeen spacetime. Additionally, we have computed the grey-body factors and analyzed the emission rates of Hawking radiation. Even when the quantum correction is small and the fundamental mode only slightly differs from its Schwarzschild value, the first several overtones deviate at an increasingly stronger rate. This deviation leads to the appearance of overtones with very small real oscillation frequencies. This outburst of overtones is closely linked to the fact that the quantum-corrected black hole differs from its classical limit primarily near the event horizon. Moreover, the intensity of the Hawking radiation is significantly suppressed (up to three orders of magnitude) by the quantum correction.