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Quasinormal modes and shadow of a Schwarzschild black hole with GUP

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arxiv 2108.04998 v2 pith:FMALPHWD submitted 2021-08-11 gr-qc hep-th

M. A. Anacleto , J. A. V. Campos , F. A. Brito , E. Passos This is my paper · ORCID
classification gr-qchep-th
keywords blackholequasinormalschwarzschildshadowlimitmodesanalysis
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We consider quantum corrections for the Schwarzschild black hole metric by using the generalized uncertainty principle (GUP) to investigate quasinormal modes, shadow and their relationship in the eikonal limit. We calculate the quasinormal frequencies of the quantum-corrected Schwarzschild black hole by using the sixth-order Wentzel-Kramers-Brillouin (WKB) approximation, and also perform a numerical analysis that confirms the results obtained from this approach. We also find that the shadow radius is nonzero even at very small mass limit for finite GUP parameter.

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Cited by 5 Pith papers

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