Comparing pseudo-complex General relativity with EHT observations

The motivation for the pseudo-complex General Relativity (pc-GR) and its structure are explained. Simulations for a thin accretion disk around a black hole are presented. While in pc-GR the disk presents a dark ring followed by a bright one, after taking into account the low resolution of the EHT, the structural appearance remains the same. A possible procedure to find a difference will be discussed.