Bardeen regular black hole as a quantum-corrected Schwarzschild black hole
arXiv:1801.08872 · doi:10.1142/S0218271819500482
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 .
5 pages. V2 with minor changes. This article is a consequence of arXiv:1801.02661. Published in International Journal of Modern Physics D
References in corpus (5)
- Universality of Quantum Gravity Corrections
- Quantum-corrected black hole thermodynamics to all orders in the Planck length
- Thermodynamics of a class of regular black holes with a generalized uncertainty principle
- Entropy of the Schwarzschild black hole to all orders in the Planck length
- Entropy of Reissner-Nordstrom Black Holes with Minimal Length Revisited
Cited by in corpus (22)
- Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A
- 30 years in: Quo vadis generalized uncertainty principle?
- Quasinormal modes-shadow correspondence for rotating regular black holes
- Upper bound on the GUP parameter using the black hole shadow
- Primordial regular black holes as all the dark matter. I. Time-radial-symmetric metrics
- Infinite tower of higher-curvature corrections: Quasinormal modes and late-time behavior of D-dimensional regular black holes
- Analysis of a regular black hole in Verlinde's gravity
- Trinity of black hole correspondences: Shadows, quasinormal modes, graybody factors, and cautionary remarks
- Implications of a Simpson-Visser solution in Verlinde's framework
- Exploring Nonlinear Electrodynamics Theories: Shadows of Regular Black Holes and Horizonless Ultra-Compact Objects
- Importance of being nonminimally coupled: Scalar Hawking radiation from regular black holes
- A new class of regular black hole solutions with quasi-localized sources of matter in dimensions
- Accretion of perfect fluids onto a class of regular black holes
- Charged AdS black holes with finite electrodynamics in 4D Einstein-Gauss-Bonnet gravity
- Five-dimensional regular black holes in a brane world
- Linearized Stability of Bardeen de-Sitter Thin-Shell Wormholes
- Remarks on the effects of the quintessence on regular black holes
- Perturbative deflection angles of timelike rays
- Testing black hole metrics with binary black hole inspirals
- Black holes and wormholes in Deser-Woodard gravity
- Einstein-Yang-Mills Regular Black Holes in Rainbow Gravity
- Black bounces as magnetically charged phantom regular black holes in Einstein-nonlinear electrodynamics gravity coupled to a self-interacting scalar field