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.
Horndeski,Conservation of charge and the einstein–maxwell field equations,Journal of Mathematical Physics17(1976) 1980
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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.