A generalized Compton wavelength deformation of Schwarzschild spacetime yields EHT and solar system bounds on the deformation parameter epsilon, currently consistent with general relativity.
Shadows near supermassive black holes: from a theoretical concept to GR test
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abstract
General relativity (GR) passed many astronomical tests but in majority of them GR predictions have been tested in a weak gravitational field approximation. Around 50 years ago a shadow has been introduced by J. Bardeen as a purely theoretical concept but due to an enormous progress in observational and computational facilities this theoretical prediction has been confirmed and the most solid argument for an existence of supermassive black holes in Sgr A* and M87* has been obtained.
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Phenomenology of Schwarzschild-like Black Holes with a Generalized Compton Wavelength
A generalized Compton wavelength deformation of Schwarzschild spacetime yields EHT and solar system bounds on the deformation parameter epsilon, currently consistent with general relativity.