Weyl corrections to Einstein-Maxwell black holes alter thermodynamic stability, topological classification, photon shadows, and accretion disk luminosity, enabling constraints on the correction parameter from astrophysical observations.
Churilova,Analytical quasinormal modes of spherically symmetric black holes in the eikonal regime,The European Physical Journal C79(2019) 629
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Astrophysical Signature and Optical Appearance of Weyl--Corrected Einstein--Maxwell Black Holes
Weyl corrections to Einstein-Maxwell black holes alter thermodynamic stability, topological classification, photon shadows, and accretion disk luminosity, enabling constraints on the correction parameter from astrophysical observations.