@article{Chou_Huang_2022, title={A novel singularity-free black hole with nonlinear magnetic monopole: Hawking radiation and quantum correction}, volume={14}, url={https://www.papersinphysics.org/papersinphysics/article/view/774}, DOI={10.4279/pip.140006}, abstractNote={<p><span dir="ltr" style="left: 194.498px; top: 507.091px; font-size: 14.944px; font-family: sans-serif; transform: scaleX(0.884183);" role="presentation">This paper introduces a nonlinear, magnetically charged, singularity-free black hole model. </span><span dir="ltr" style="left: 194.498px; top: 525.356px; font-size: 14.944px; font-family: sans-serif; transform: scaleX(0.908614);" role="presentation">The Ricci scalar, Kretschmann scalar, horizon, energy conditions, and Hawking radiation</span> <span dir="ltr" style="left: 195.05px; top: 543.621px; font-size: 14.944px; font-family: sans-serif; transform: scaleX(0.864875);" role="presentation">corresponding to the singularity-free metric are presented, and the asymptotic behavior and</span> <span dir="ltr" style="left: 195.05px; top: 561.886px; font-size: 14.944px; font-family: sans-serif; transform: scaleX(0.906331);" role="presentation">quantum correction of the model are examined. The model was constructed by coupling</span> <span dir="ltr" style="left: 195.05px; top: 580.151px; font-size: 14.944px; font-family: sans-serif; transform: scaleX(0.911941);" role="presentation">a mass function with the regular black hole solution under nonlinear electrodynamics in </span><span dir="ltr" style="left: 195.05px; top: 598.416px; font-size: 14.944px; font-family: sans-serif; transform: scaleX(0.900174);" role="presentation">general relativity. Aside from resolving the problem of singularities in Einstein’s theory of </span><span dir="ltr" style="left: 195.05px; top: 616.681px; font-size: 14.944px; font-family: sans-serif; transform: scaleX(0.855582);" role="presentation">general relativity, the model asymptotically meets the quantum correction under an effective</span> <span dir="ltr" style="left: 195.05px; top: 634.946px; font-size: 14.944px; font-family: sans-serif; transform: scaleX(0.939504);" role="presentation">field theory. This obviates the need for additional correction terms; in this regard, the</span> <span dir="ltr" style="left: 195.05px; top: 653.211px; font-size: 14.944px; font-family: sans-serif; transform: scaleX(0.888519);" role="presentation">model outperforms the black hole models developed by Bardeen and Hayward. Regarding </span><span dir="ltr" style="left: 195.05px; top: 671.476px; font-size: 14.944px; font-family: sans-serif; transform: scaleX(0.914069);" role="presentation">the nonlinear magnetic monopole source of the gravitational field of the black hole, the </span><span dir="ltr" style="left: 195.05px; top: 689.74px; font-size: 14.944px; font-family: sans-serif; transform: scaleX(0.897902);" role="presentation">energy–momentum tensors fulfill weak energy conditions. The model constitutes a novel,</span> <span dir="ltr" style="left: 195.05px; top: 708.005px; font-size: 14.944px; font-family: sans-serif; transform: scaleX(0.893816);" role="presentation">spherically symmetric solution to regular black holes.</span></p>}, journal={Papers in Physics}, author={Chou, Yu-Ching and Huang, Weihan}, year={2022}, month={Apr.}, pages={140006} }